Theories of Everything with Curt Jaimungal - A New Era in Quantum Mechanics Is Finally Here... | Jacob Barandes

Episode Date: January 30, 2025

As a listener of TOE you can get a special 20% off discount to The Economist and all it has to offer! Visit https://www.economist.com/toe In this captivating of Theories of Everything, Jacob Barandes... and I delve into the intricate world of Indivisible Stochastic Processes and their profound impact on quantum mechanics. We explore how these non-Markovian systems introduce quantum phenomena like superposition and interference without the traditional wave function collapse. Join My New Substack (Personal Writings): https://curtjaimungal.substack.com Listen on Spotify: https://tinyurl.com/SpotifyTOE Timestamps: 00:00 - Episode Introduction 02:15 - Overview of Quantum Mechanics 05:30 - Introduction to Indivisible Stochastic Processes 10:45 - Understanding Symmetry Breaking 15:00 - Mirror Symmetry in Physical Systems 20:30 - Spontaneous vs. Explicit Symmetry Breaking 25:00 - Real-World Examples of Symmetry Breaking 30:15 - Connection to Cosmology and FLRW Models 35:45 - Implications for the Flow of Time 40:00 - Introduction to the Measurement Problem in Quantum Mechanics 45:30 - Comparing Indivisible Stochastic Processes to Bohmian Mechanics 50:00 - The Role of Philosophy in Physics 55:20 - Historical Interactions Between Physicists and Philosophers 01:05:30 - Deep Dive into Indivisible Stochastic Processes 01:40:06 - Markovianity in Quantum Mechanics 01:42:12 - Linearity and Unitarity in Quantum Evolution 01:43:23 - Unistochastic Processes and Quantum Channels 01:45:20 - Quantum Channels and Steinspring Dilation 01:46:18 - Hamiltonian Formulation Analogy 01:49:05 - Double-Slit Experiment with Indivisible Processes 01:52:08 - Measurement Devices and Emergibles 02:00:04 - Seminar Culture and Philosophy in Physics 02:02:38 - Coarse-Grained Double-Slit Example 02:05:03 - No Wave Function Collapse in Indivisible Processes 02:12:16 - Philosophical Insights and Importance in Physics 02:18:08 - Critique of David Griffiths' Quantum Mechanics Textbook 02:35:07 - Closing Remarks and Future Topics Links Mentioned (additional links in comments): - Jacob’s website: https://www.jacobbarandes.com/ - Jacob’s first appearance on TOE: https://www.youtube.com/watch?v=7oWip00iXbo&ab_channel=CurtJaimungal - Jacob’s talk on “A New Formulation of Quantum Theory”: https://www.youtube.com/watch?v=sshJyD0aWXg - The Stochastic-Quantum Correspondence (Jacob’s paper): https://arxiv.org/pdf/2302.10778 - McTaggart’s paper on time: https://philpapers.org/archive/MCTTUO.pdf - Putnam’s paper on time and geometry: https://www.jstor.org/stable/2024493?origin=JSTOR-pdf - Neil deGrasse Tyson on TOE: https://www.youtube.com/watch?v=HhWWlJFwTqs - Einstein-Podolsky-Rosen paper: https://cds.cern.ch/record/405662/files/PhysRev.47.777.pdf - Greta Hermann’s paper on quantum mechanics in the philosophy of nature: https://cqi.inf.usi.ch/qic/grete_en.pdf - John Bell’s paper on the Einstein Podolsky Rosen paradox: https://journals.aps.org/ppf/pdf/10.1103/PhysicsPhysiqueFizika.1.195 - Bell’s theorem without inequalities (paper): https://arxiv.org/pdf/quant-ph/0409190 - Quantum mysteries revisited (paper): https://www.physics.smu.edu/scalise/P5382fa15/Mermin1990a.pdf - Quantum Theory by David Bohm (book): https://www.amazon.com/Quantum-Theory-Dover-Books-Physics/dp/0486659690 - Bohm’s second paper on quantum theory: https://journals.aps.org/pr/abstract/10.1103/PhysRev.85.180 - Dirac’s textbook on quantum mechanics: https://www.amazon.com/Principles-Quantum-Mechanics-International-Monographs/dp/0198520115 - Wigner’s paper on the mind-body question: https://www.scribd.com/doc/240712078/Eugen-Wigner-Remarks-on-the-Mind-body-Question #science #physics #theoreticalphysics #quantumphysics Learn more about your ad choices. Visit megaphone.fm/adchoices

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Starting point is 00:01:30 are reflecting things that are really there. The people who gave us the biggest revolutions in modern physics, quantum theory and relativity, were all strongly connected to philosophy. Physicists have grappled with the seemingly outlandish implications of quantum theory that particles are purportedly in multiple places simultaneously and there's a mysterious
Starting point is 00:01:49 wave function that collapses upon measurement and a framework that requires so-called imaginary numbers, etc. I traveled to the oldest physics laboratory in the United States to meet at Harvard with theoretical physicist and philosopher Jacob Barndes, who is the co-director of the graduate studies department there, where we go into technical depth into his innovative reformulation of quantum theory for more fundamental mechanics called Indivisible Stochastic Processes. My name is Kurt Jaimungal and this was part of my three-day tour of Harvard, Tufts and MIT, where I recorded five podcasts, one of them being with Jacob Barndes that you're
Starting point is 00:02:22 seeing now, which was actually over seven hours long, so we're splitting it into two. The others are with Michael Levin, Anna Chownika, and Manolis Kellis. There's also Professor William Hahn, a computer scientist, and that was filmed live at the MIT Media Lab. Subscribe to get notified. Jacob's breakthrough theory raises new provocative questions such as what if quantum waves don't exist? Did physics lose its soul by abandoning philosophy? Does time flow differently in quantum physics? And was Einstein right all along? It's good to be here.
Starting point is 00:02:54 It's really lovely to see you again. The last time we talked, I enjoyed it tremendously. Yeah, me too. So let's talk about physical philosophy versus the philosophy of physics. People have heard about the philosophy of physics. What is physical philosophy? Yeah. So my research has sort of two sides.
Starting point is 00:03:16 There's the physical philosophy side and there's the philosophical physics side. Let me start with physical philosophy. So the way I describe physical philosophy, it's the use of results and ideas and discoveries and theories from physics to address traditional questions in philosophy, in particular in metaphysics. So the kinds of questions that we're interested in here are questions about space and time, the philosophy of time, causation. There are very interesting connections between physics and causation, some of which we'll hopefully have a chance to talk about today.
Starting point is 00:03:58 Also the philosophy of probability, which is a very subtle and very complicated area. And also the metaphysics of laws, which is a rich, very interesting area of inquiry. And so just thinking about what do our best current physical theories bring to bear on these traditional questions? How do they constrain what we can say about those sorts of things? So here's a good example, a concrete example.
Starting point is 00:04:23 Philosophers, metaphysicians have been thinking about the nature of time for a very, very long time, right? You go back to Parmenides and Heraclitus and people thinking about, you know, is time something that flows? Is time something that is just an illusion? And there's this very famous paper, which maybe you can link to because it's a beautiful paper and people should read it, by MacTaggart, a philosopher, about over 100 years ago on the nature of time. And he introduces this terminology,
Starting point is 00:04:53 the A series, the B series, the C series, these different ways of thinking about time and how much structure it has. The A series is this idea that events that take place in time can be classified as past, present, the A series is this idea that events that take place in time can be classified as past, present, and future, but that seems to like distinguish a notion of a present, and is that really a sensible notion? And there's the B series, which has less structure.
Starting point is 00:05:16 This just says that events can only be classified in terms of earlier or later, so there's like a pairwise relationship between them only, and there's no distinguished notion of a present. And the C series has even less structure. It just says that there's a sense of an ordering of events, that given any three events, we can say which takes place between the other two, but without privileging a direction in time. And he explores all of these ideas in the essay,
Starting point is 00:05:38 but right around the same time, Albert Einstein was developing special relativity, and special relativity has some pretty serious implications for how we think about the nature of time. In particular, although many people have heard of phenomena like time dilation, the idea that observers moving in different states of motion will have different senses in which time flows,
Starting point is 00:06:02 like the rate at which time flows for one observer may be different from the rate at which time flows for one observer may be different from the rate at which time flows for another. And maybe some people have heard of length contraction or Lorentz contraction that spatial distances in the direction of the change of reference frame can be distorted. Somewhat less known as the breakdown in simultaneity,
Starting point is 00:06:21 which is this idea that observers in different states of motion will assign different events to be in their present. So for an observer in one frame of motion, some collection of events may be in what an observer identifies as their present moment. But to an observer in a different frame of motion, their sense of the present is like tilted. It's like tilted a little bit so that things that the first observer would have said were
Starting point is 00:06:43 in the future are in the second observer's present, as are some things that might have been in the first observer's past. And this feature of special relativity that simultaneity is not an invariantly defined concept has profound implications for how we think about the philosophy of time. And these were explored by people like rather famously the philosopher Hilary Putnam in the 60s, who wrote a really beautiful paper, which you should also link to because it's just very beautifully argued. And he makes the case for what he calls four-dimensionalism. You might call it eternalism, the idea that because different observers will disagree on which events are in their presence, if we just take the totality of all the things that everybody thinks are in their presence,
Starting point is 00:07:27 it's basically all of space time. If you look at observers at different locations, different frames of motion, and does that mean that everything in space time is just in some sense there already? You know, the future is not a thing that has yet to happen. The future is not a thing that is unfolding, but our experience of the flow of time is merely psychological and special activity is actually telling us in some very strong sense that we're living in an eternalist so-called block universe where everything is just there.
Starting point is 00:07:51 So this is a fantastic example of where the things we're learning from contemporary successful physical theories, thoroughly empirically established like physical theories, bring to bear some very important constraints on what you might've thought were purely metaphysical questions. So I call this general subject physical philosophy. On the other hand, I also work in what I would call philosophical physics and the name is supposed to resemble
Starting point is 00:08:18 like theoretical physics, mathematical physics, computational physics. It's a methodology for doing physics, not philosophy, but rather than say mathematical physics, computational physics. It's a methodology for doing physics, not philosophy. But rather than say mathematical physics, where you're doing physics by stating axioms, improving theorems, or theoretical physics, where you're formulating models and then calculating predictions within the models
Starting point is 00:08:40 and comparing them with experiments, or computational physics, where you're simulating physical processes in a computer and making predictions that way. Philosophical physics tries to make progress on physics using some of the tools that you might traditionally have associated with philosophy. So what are those kinds of tools? Thought experiments, coming up with counter examples, sharpening definitions, sharpening questions, right? Sometimes you're dealing with a problem in science or physics more specifically,
Starting point is 00:09:13 where the questions are not yet sharply formed enough that they will, you know, you could subject them to experimental study. Sometimes you have to do some work beforehand to sharpen those questions. That's the kind of thing that philosophers like to do. Identifying implicit assumptions, hidden assumptions, and that's something we'll be talking about because some of my work is closely connected
Starting point is 00:09:39 with this idea of identifying implicit assumptions. Assumptions that may get in the way of making scientific progress, subjecting ideas to a logical analysis, and also to what I call rigorous scrutiny. Because in philosophy, we're not generally guided by empirical data or observation. You might think that there's just, well, if you don't have empirical data, what are you doing? Well, you're not without any tools at all, right? So one of the things that philosophers like to do Is just be really really careful in how they talk about things now
Starting point is 00:10:13 They define things being very careful with every step of their logic Stealing their premises as clearly as possible so that if you find fault with their arguments You can identify where the problem is. It's just sharpening everything and subjecting things to rigorous scrutiny. These are all tools and techniques that come from philosophy, and I call them philosophical physics. And this doesn't even include just taking ideas from philosophy, like actual just picking up ideas from philosophy and seeing if they have some use in physics. And I think there's a proud tradition of this kind of work.
Starting point is 00:10:42 I've talked to philosophers of science who've told me that the greatest philosopher of physics of the 20th century was Albert Einstein. And when you look at, especially Einstein's earlier work, what is he doing? He's subjecting definitions and ideas to rigorous scrutiny. I mean, how much time did he spend trying to pin down exactly what we mean by an inertial reference frame? You might think inertial reference frames are like the scenery of Newtonian physics. Like, what could you really gain by spending a lot of time really rigorously scrutinizing what is the precise definition of inertial reference frame and scrutinizing when you know that you're actually in an inertial reference frame? But think about how much mileage Einstein got out of thinking about inertial reference frames, which laws of physics should be the same in every inertial reference frame, realizing that the speed of light is one of these laws of physics that should be the same in every
Starting point is 00:11:31 inertial reference frame. And then, you know, his greatest, what he described as the greatest idea ever had, which is realizing that, you know, it's impossible to distinguish the local short duration effects of a gravitational field from being in a reference frame that is in uniform acceleration. And that realization is what, you know, eventually evolves into the equivalence principle and leads him into his theory of general relativity. He has this idea in 1907, and he described it as the happiest idea of his life. So and of course, I'll get into this more a little bit later,
Starting point is 00:12:07 but Einstein was thoroughly steeped in philosophy. We'll talk a little bit about the greats of 20th century physics and how much philosophy they did. So I think there's a really a strong tradition of philosophical physics in history. And I'm certainly not the only one who practices, I think, this discipline, but I think there's really something to say about it. I think it really does contribute something to how we can make progress in physics.
Starting point is 00:12:36 And so that's the other side, I think, of what I do. So what's the standard view of philosophy of physics or philosophy in general from people who consider themselves to be scientists or who actually are practicing scientists. So for instance, when I was speaking to Neil deGrasse Tyson, he was saying, well, philosophy, what has it done? What give me, Kurt, an example of something that philosophy has contributed to modern day physics in the past 30 years?
Starting point is 00:13:00 Sure in the past, thought experiments. That's a lovely question. I actually know Neil Tyson. We worked together when I was in high school. This is some interesting history. So I grew up in New York City, and I used to go to the Museum of Natural History all the time. It was one of my favorite places. I mean, if anyone who's like listening to this has never been to the American Museum of Natural History,
Starting point is 00:13:24 you are missing out. It is, it's like going to a magical fairyland for, you know, like science and it's amazing. And I got lucky when I was in high school to intern at the museum and there was a period of time when I was working in the astronomy department and I worked with Neil Tyson. It was amazing. I mean, he's great. So, of course, you know, I do very, very politely disagree with that sentiment. I'll give you a couple of examples. So here are some things that have come out of philosophical thinking about physics, philosophy. I mean, the lines are a little blurry here because obviously if you're doing philosophy that's very close to physics, one could accuse you of just doing physics.
Starting point is 00:14:09 But, okay, let me think of an example. This one is from the 80s. Okay, so 1982, Zurich and Wooters and then independently, an absolutely, definitely philosopher of science, Dennis Deeks, independently formulated what we now call the no-cloning theorem. So no-cloning theorem and quantum theory is a very simple, very beautiful theorem. What it says is that if you were given, as traditionally formulated, a quantum state in the form of a wave function or state vector, just some object in Hilbert space that describes in a traditional sense the state of your quantum system, and you don't do any measurements on it.
Starting point is 00:14:54 You've prepared it, but you haven't measured the position, you're leaving it pristine. Is there a way to build some kind of apparatus that can make another system be in exactly the same quantum state? That is, can you, you know, if your first system was, you know, some simple quantum system and it's in some state, can you bring in a second quantum system of the same kind
Starting point is 00:15:19 and run both systems through some kind of machine that will make the second system be in the same quantum state as the first system every time, right, every time. And the answer is you can't. If you set the machine up so that it works some of the time, then all you have to do is set up the first system in a superposition of those possibilities and that we'll find is that you cannot get the other system
Starting point is 00:15:41 to be in the right quantum state that is also the same superposition. This is called the no cloning theorem. And the cloning theorem is useful. I mean, people certainly shows up all over the place in physics. It shows up in high energy theory. It shows up in all kinds of places. I guess that's 1982.
Starting point is 00:15:57 I mean, that's a little bit outside the boundary of the 30 years. What's happened since the 90s? And we're not allowed to talk about your work yet. Ah, yeah, we can't talk about work yet. I mean, that's an interesting question. I mean, from the point of view of like... So it's a bit difficult because, like I said, the boundaries here are a little blurry. If you think about people like
Starting point is 00:16:23 Martin Lazord or Eric Uriel or JB Manchek, these are people who work in foundations of general relativity. And, you know, their work is super mathematical. I mean, if you ask them, do you consider yourself first and foremost a philosopher? Or I haven't asked Eric or I haven't asked all these people like what do you first think of yourself as? But they certainly come to philosophy seminars they give philosophy talks they certainly sound like philosophers and they're doing like work on general relativity. They're proving things about space-time that are
Starting point is 00:17:01 interesting facts. So I you know, and then of course the lines between quantum foundations and quantum information are also very blurry. So I'll tell you, here's an interesting story, okay? You've all probably heard of qubits, right? Qbit, right? So a qubit is supposed to be a quantum bit.
Starting point is 00:17:19 And usually the way that we're, the term is introduced, people will say it's a portmanteau of quantum and bit, right? You know, bit, I think the term bit goes back to Claude Shannon. That itself is a portmanteau of binary digits. You know, Claude Shannon introduced many of the ideas in information theory and communication theory in the 40s, back when he was at Bell Labs.
Starting point is 00:17:45 And then the idea is that you have classical bits and you also have these modern quantum bits or qubits. But the name qubit is a very, it's a very funny word because if you look at it, it's spelled Q-U-B-I-T. You'd be hard pressed to think of many other words in English that are a Q and a U and then there's no other vowel, just a consonant right away.
Starting point is 00:18:05 Why that very funny spelling? And I'm not saying I'm the first to notice this funny spelling. In fact, there's a very famous physicist, David Merman, who also is interested in quantum foundations, among other things, and he doesn't like that spelling because he says it's like the spelling is really very non-standard. I think he likes to write it as Q hyphen bit and not Q-U-B-I-T. So where did that spelling come from? The term was coined by Ben Schumacher at Kenyon College and Bill Wooders, who I mentioned before, at Williams College. The story is that Bill Wooders was visiting Kenyon College, and this was in Ohio.
Starting point is 00:18:48 And they were both driving to the airport in Columbus. And they were talking about how they needed a new scheme for talking about quantum information. This was in 1992, just outside of the 30-year mark. I'm sorry. We're just a little over 30 years. And it was Bill, so I got this information from one of Ben's students, Mary Gerhardinger, she told me this story. Bill was in the car and he said, wouldn't it be funny if we called these things qubits, because there's a unit of measure in the Bible called a qubit. But in the Bible, it's spelled C-U-B-I-T.
Starting point is 00:19:27 It's a unit of measure. It's like, I don't know, distance from your elbow to the tip of your finger. And if you read Genesis, you'll hear God telling Noah to build the ark, and it's supposed to be this many qubits long and this many qubits tall, right? And they're like, but it starts with a C, because the Bible is classical. Do you get it? Like, what's more classical than the Bible? Let's just replace the C with a Q, and it will be a modern version of a cubit. That's funny.
Starting point is 00:19:54 And they both thought it was hilarious. As you know, on Theories of Everything, we delve into some of the most reality spiraling concepts from theoretical physics and consciousness to AI and emerging technologies, to stay informed in an ever-evolving landscape, I see The Economist as a wellspring of insightful analysis and in-depth reporting on the various topics we explore here and beyond. The Economist's commitment to rigorous journalism means you get a clear picture of the world's most significant development.
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Starting point is 00:21:07 Head over to their website, www.economist.com slash totoe to get started. Thanks for tuning in and now back to our explorations of the mysteries of the universe. And they both thought it was hilarious. And so the name comes from this conversation that they had. And Bill Wooders did a lot of work in quantum foundations. Ben Schumacher worked with John Wheeler, who in addition to being a very great theoretical physicist and a fantastic mentor who had many, many famous students.
Starting point is 00:21:40 Richard Feynman was one of the students. So many students. Jacob Bekenstein, many very famous students, was also very philosophically curious. Hugh Everett of the Many Worlds Interpretation, which hopefully we'll talk about, was also one of his students. And so he really enjoyed having these really deep philosophical conversations, and he created a real atmosphere of philosophical inquiry in his research group. Zurich worked with John Wheeler. So does that count as a philosophical contribution?
Starting point is 00:22:08 I mean, Schumacher and Wooters were not at R1 universities. They were not at major universities. They were both at liberal arts colleges, and they were interested in very foundational questions. I mean, does that count as philosophy? It's kind of hard to say, but... Now, I guess you can go farther. I mean, if you count as philosophy? It's kind of hard to say, but... Now, I guess you can go farther. I mean, if you're willing to go farther back and take ideas that came out of philosophical thinking,
Starting point is 00:22:31 but that are still proving themselves to be super useful, there's a lot more, right? I mean, you could... I mean, if you're just talking about quantum mechanics, not even general relativity, you know, the notion of entanglement goes back to philosophical disputes between, you know, the notion of entanglement goes back to philosophical disputes between, you know, people like Schrodinger and Einstein. The Einstein-Podolsky-Rosen
Starting point is 00:22:53 paper from 1935, maybe the most cited paper Einstein's name is on, is an extended philosophical argument. They lay out their premises. They lay out a very detailed philosophical argument, which we can talk about, and, you know, they make a metaphysical claim about quantum mechanics. A physical and a metaphysical claim about whether quantum mechanics could be considered complete, even if it's practically, perfectly useful. Um... Hmm. Killer messaged you yesterday? This is so dangerous, I gotta get out of this. Based on a true story.
Starting point is 00:23:46 New season Mondays at 9 Eastern and Pacific. Only on W. Stream on Stack TV. Their work, you know, the EPR argument, the Inus Podilska Rosen paper, inspired a lot of people. I'll get to who it inspired, but let me just say that before I get to that, there's a paper by absolutely a philosopher, Greta Hermann. So Greta Hermann was a philosopher, a student of Emmy Noether, who, mathematician, made major contributions to physics,
Starting point is 00:24:16 symmetries and conservation laws, Noether's theorem is super important, arguably the most important theorem in physics. And so her student, Greta Hermann, she's a philosopher, she's a neocontian, and she wrote a large number of papers on physics and metaphysics and on the developing quantum theory. And she wrote a paper, we read it in my philosophy of quantum mechanics class, and it's a paper in which she is studying the nature of causation in quantum mechanics. And she sets up this thought experiment. It's a beautiful thought experiment, and the paper was published in 1935, several months
Starting point is 00:24:49 before the EPR paper. It was widely read apparently. It's likely that Einstein read this paper. And the thought experiment that's used in the EPR paper bears a strong resemblance to the thought experiment that's in Greta Herman's paper. Okay, so like, you know, clear, interesting threads going on in the 1930s. Then of course, John Bell picks up the thread and publishes a paper in 1964,
Starting point is 00:25:17 his famous no-go theorem paper, the first appearance of what we now call Bell's theorem. And that paper is called On the Einstein-Podolsky-Rosen Paradox. That's what he calls the paper. He takes the EPR paper and he extends the argument into a statement about what he calls what we now call hidden variables theories. And you've got further results that build on Bell's Theorem.
Starting point is 00:25:43 You have the famous CHSH inequality, which comes in 1969. That's Clauser Horn, Shimoniholtz, which is a somewhat more general version of the Bell inequality. In the 90s, so we're in the 90s now, you've got a Greenberger, Horn, and Zeilinger, the GHD paper. There's a beautiful version of this argument by David Merman in American Journal of Physics, which I can also send you links to. These are all beautiful papers to read.
Starting point is 00:26:09 And these papers all deal with entangled systems. And in particular, Bell's paper and the GHZ paper deal with particular kinds of quantum states. The GHZ paper introduces these GHZ states. And GHZ states show up all over the place in atomic molecular optical physics today, and in quantum information. I feel like every time someone uses a GHZ state, or uses, you know, Bell violating states or things like that in order to do something in quantum cryptography or to certify the randomness of the quantum random number generator, they should have to pay royalties
Starting point is 00:26:52 to the field of philosophy of physics and quantum foundations. The No Signaling Theorem is an important result that comes out of quantum foundations. This is in the late 70s and early 80s, I think. One version of the argument is by the same people who gave us the GRW spontaneous collapse theory, right? And so, you know, and the no signaling theorem is also a theorem that shows up all over the place. But I think, you know, and I can make more examples. I mean, there's quantum teleportation.
Starting point is 00:27:28 You know, in some of David Deutsch's early papers introducing some of the basic ideas that led to quantum computing, he is very explicit in the papers about how what he's trying to do in trying to imagine building a quantum computer is confirm that many worlds is the correct interpretation of quantum mechanics, right? So he's motivated by interpretational philosophical questions to a substantial degree. But I think probably my favorite example is decoherence. So whenever you propose a new way to think about quantum mechanics, people will often say, do we really need this? Doesn't decoherence solve this problem?
Starting point is 00:28:00 There's a physics solution to this problem. We don't need philosophy, do we? But decoherence comes out of philosophy, right? So, um... How? Okay, so there are some rudiments of ideas from, you know, that we might associate with decoherence that go all the way back to like Mott in the 1920s.
Starting point is 00:28:17 But the first serious, rigorous formulation of decoherence that I've ever been able to find shows up in chapter 22. So these are the end chapters of David Bohm's textbook quantum theory. This is 1951 he publishes this textbook. It's before he introduces his pilot wave theory and You know, he's a very philosophically curious person in addition to being a physicist And in his book on quantum mechanics, he doesn't just want to teach quantum mechanics. He also wants to deal with some of these lingering questions about how the measurement process is supposed to work.
Starting point is 00:28:54 So in the later chapters of his book, he goes through the measurement process in as much detail as he is able to, based on the axioms that were available, the Dirac von Neumann axioms, the axioms associated with Paul Dirac and John von Neumann from 1930 and 1932, respectively. And, you know, he, he, he tries to formulate a measurement process, he has a system, a quantum system that is to be measured, it's in some superposition, he brings in in like a physical measuring device, he models the whole thing with a system to be measured and the measuring device, he lets them interact, he ends up with this superposition.
Starting point is 00:29:32 And then he argues that some of the probabilistic quantities one might wanna calculate, the averages one might wanna calculate, they exhibit these very strange quantum effects, these so-called interference effects. But once the measurement proceeds far enough and measuring device interacts sufficiently strongly, and I don't remember in the book
Starting point is 00:29:53 whether he includes the environment or not, I'd have to remember exactly what he does there, but basically enough degrees of freedom from outside the system get involved, you get what he calls, the phrasing he uses is the destruction of interference in the process of measurements. That's what he calls it is the destruction of interference in the process of measurement. That's what he calls it. The destruction of interference in the process of measurement, which is decoherence.
Starting point is 00:30:09 That's a more extended version of the term decoherence. And that's exactly what decoherence is. So he writes this book. He apparently has conversations with Albert Einstein about it. This is 1951, 1952. Albert Einstein is still alive at that point. And he has some conversations with Albert Einstein and Albert Einstein is dissatisfied with his approach. Says he should go work on it a little more. And he goes back and he independently rediscovers
Starting point is 00:30:37 some work that was done by de Broglie in the late 1920s. De Broglie had developed the first sort of early pilot wave theories. Bohm independently redevelops these. Eventually he and de Broglie had developed the first sort of early pilot wave theories. Bohm independently redeveloped these. Eventually he and De Broglie connect. Now we call these theories the De Broglie-Bohm theory, or sometimes just Bohmian mechanics. And in this theory, you've got not just the wave function evolving in some high dimensional space where the wave functions live,
Starting point is 00:31:00 but the wave function is also guiding around these corpuscular particle-like things, the Bohmian particles, the Bohmian projectiles, the Bohmian corpuscles. And, you know, one obvious question you could ask is, well, if you have both these projectiles and you have a pilot wave, and Bell and Bohm in these papers specifically says that the pilot wave is real,
Starting point is 00:31:27 metaphysically real to the same extent that the particle locations are. Then when you do something like the double slit experiment and you send a pilot wave through these two slits of an experiment, right, and they land on a screen, why doesn't the screen light up in all the places where the wave hits it, right? So the wave diffracts, you get these intensity peaks,
Starting point is 00:31:54 these famous interference peaks in the wave function. The projectile is guided to only one of the locations. When you actually run the experiment, you only see one landing site. But the question is, well, but what about the other empty waves, empty shells, the parts of the wave function that land on the screen and don't have a particle in them? Why don't they hit something and do something? And Bohm wrote two papers. He was a pair of papers.
Starting point is 00:32:19 In the second paper, he goes through the measurement process. He goes through this example. And he basically uses decoherence to explain why we only see one landing site. So decoherence was developed in this textbook and then put to use almost immediately in a very applied sense to get his pilot wave theory off the ground and to make it to show that it was empirically adequate, at least for non-relativistic systems of finitely many particles. The threat is then picked up again in the 70s by Dieter Ze, who did some very deep and important work on decoherence. Apparently, he had some career repercussions for working on such a philosophical foundational area. And then decades later, physicists, practical working physicists working with, you know,
Starting point is 00:33:11 AMO systems, atomic molecule optical systems, physicists trying to implement real-world quantum computers, trying to implement unitary gates and actually get simple quantum computers to work. But even physicists in all kinds of other areas, physicists trying to understand early universe cosmology, physicists trying to understand systems and condensed matter, people are now worrying about decoherence all the time. You read papers, every paper talks about what is the decoherence time scale of this or that. Decoherence is now a major component of what we do in physics today. It's happening all the time right now.
Starting point is 00:33:46 And again, I would just say that maybe we should pay some royalties to poor David Bohm, who was run out of the United States. He spent a lot of his career in Brazil and couldn't get back to the United States, and Ze, who suffered some career repercussions. And there's this attitude that, oh, thinking about foundational philosophical questions is a waste of time. How could it be a waste of time, given all of the fruit that it has produced?
Starting point is 00:34:13 So, you know, what I would say is, and this is just a general message to anyone who's thinking about how best to contribute to the development of science. The field of philosophy of physics, the field of, I would say, like, the more philosophical side of quantum foundations, because there are also parts of quantum foundations
Starting point is 00:34:34 that are much closer to, like, practical quantum information type stuff. But the sort of more, like, philosophical side of it, this is an area that has had very few people work on it, right? There are very few permanent tenure track academic positions that are devoted to this kind of work. A lot of the people who are doing this work got their academic positions to do something else and then transitioned into this work.
Starting point is 00:34:55 So there's very few people responsible for a lot of these results. There is very little research funding. And so if you were the sort of person watching this and wondering, like, where would funding make the biggest difference in physics? Should we devote more funding to already very well funded areas of physics? Would an additional million dollars make a huge difference to some of these areas? I can tell you that like philosophy of physics, the intersection of physics and philosophy, the more philosophical side of quantum foundations and
Starting point is 00:35:26 physics, the intersection of physics and philosophy, the more philosophical side of quantum foundations, and also the more philosophical side of the foundations of general relativity and the foundations of many other important areas of physics. That's where I think every dollar would go very far. So if you're in the market for endowing professorships, that is a way to make a huge impact on the field. Great. Speaking of the foundations of quantum mechanics, are they inconsistent as they stand in textbook quantum theory? So, if you take textbook quantum theory to be...
Starting point is 00:35:59 quantum theory is formulated according to the Dirac-von Neumann axioms. Again, that's Paul Dirac as he formulated them basically in 1930 in his famous book, Principles of Quantum Mechanics, and John von Neumann in 1932, Mathematical Foundations of Quantum Mechanics. People divide the axioms up in various ways. I'll give a super quick discussion. They say that to every quantum system,
Starting point is 00:36:24 we associate a kind of a vector space called a Hilbert space, a space of vectors involving complex numbers. The elements of this vector space are called state vectors. Loosely speaking, they can be also called wave functions. There's some terminological nuance around that. And these are supposed to represent in some sense, the state of a quantum system.
Starting point is 00:36:43 More generally, you have to use what's called a density operator, which is a little more complicated, but we'll put that aside. And then the next axiom is that as time evolves, these quantum states, whether state vectors or wave functions or density matrices, are supposed to evolve according to what's called a unitary time evolution.
Starting point is 00:36:59 If it's sufficiently smooth and nice, it can be written as a differential equation, an equation that tells you moment to moment, in a Markovian way, what each next state will be given the present state. We call that differential equation when it's for wave functions, we call it the Schrödinger equation. If it's density operators, we call it the von Neumann equation.
Starting point is 00:37:17 And then there's all these axioms of measurements. The observable things that you could measure about a system are represented by operators or matrices, these self-adjoint things a system are represented by operators or matrices, these self-adjoint things called self-adjoint operators, matrices. These are the observables of your theory. The possible results you can get when you measure one of them is called an eigenvalue. It's one of the eigenvalues of these operators.
Starting point is 00:37:37 The probability with which you'll get that is given by this formula that takes the state, the quantum state of the system, and takes, you know, we call it projection operator, but a piece of this operator, you put them together, it gives you the probability you'll get that result when you do the measurements. And then once you've done the measurements, this quantum state of the system is projected or collapses to reflect the result and ensure that you'll get the same result
Starting point is 00:37:57 if you measure it again right away. Those are the traditional Dirac-Vinam and axioms, and people slice them up in different ways. But I like to think of them as those five axioms, right? Hilbert spaces, unitary time evolution, observables as self-adorned operators, the Born rule for probabilities of measurement outcomes, and then collapse. There are problems with these axioms. Not when dealing with, you know, microscopic systems. Microscopic systems, things tend
Starting point is 00:38:25 to work out pretty well. And when people say quantum mechanics works just great, they mean microscopic systems. If you want to do a tabletop experiment, an atomic experiment or laser experiment, you're working with tabletop systems, microscopic systems, theory works great. Works great. If you limit yourself to these particular examples, what's the problem? If you limit yourself to these particular examples, what's the problem? If you wanna do a particle physics experiment, a high energy physics experiment, you're building a giant particle accelerator,
Starting point is 00:38:56 you're talking about the Large Hadron Collider or something like that, you have beams of subatomic particles that are flying together, and there's debris that comes out, you collect all the debris. These are all microscopic systems. Quantum mechanics makes beautiful predictions
Starting point is 00:39:10 about these results. So you're not gonna see any discrepancies for these kinds of systems, at least to the extent that the Dirac von Nomenaxiums give a self-consistent description for microscopic systems, which they appear to do. Perfectly empirically adequate description, the theory works great.
Starting point is 00:39:24 So what's the problem? Why does anyone have any issue? We talked before in our last conversation, and I talked about this thought experiment that was proposed, I think originally by Hugh Everett in his long form thesis in 1956, 57, when he was a graduate student at Princeton, working for John Wheeler.
Starting point is 00:39:47 Not the one he ultimately published. He published a shorter version. But in the longer version, he opens it up with a thought experiment that has since been usually attributed to Eugene Wigner, who was also at Princeton. And we talked about how Wigner had this paper called On the Mind-Body Question in the early 1960s. But in his thought experiment, we imagine trying to do quantum mechanics with a system that is not small.
Starting point is 00:40:08 It is not small, it is not ultra cold, it is not, you know, pristine. The quantum system is something big enough to be a measuring device itself or even an observer. So again, this thought experiment is called the Wigner's Friend Thought Experiment. Wigner is on the outside of a box. The box is perfectly sealed.
Starting point is 00:40:26 Vigner is one observer. Inside the box is Vigner's friend. Vigner's friend is also an observer, a big system, but perfectly sealed inside the box. And Vigner's friend does a measurement on some superposed microscopic quantum system inside the box. And now we have a problem. Because we can describe the situation in two ways. We can treat Wigner's friend, the person in the sealed box,
Starting point is 00:40:55 as a thing that is an observer, that does measurements, and then we're supposed to use the measurement axioms and the collapse axiom. Or because the person's sealed in a box and there is a second observer on the outside who has not done a measurement on the box or the contents, maybe we should treat the box and its contents as not subject to the collapse axiom. And now all of a sudden we have an ambiguity in the middle of the theory. The Dirac-Vinamon axioms are simply ambiguous in this circumstance.
Starting point is 00:41:23 They don't render a judgment of what you're supposed to do. And when we spoke last time, I laid out a whole menu of possible things you could do, and each of them leads you down a different road, right, for how you would resolve this problem. So this is just an inconsistency. And I wanna make clear here, there's a difference between a theory being unintuitive
Starting point is 00:41:40 or exotic or eccentric, and a theory being inconsistent. So let me give you an analogy, a real world analogy. You've got a friend and your friend is lovable and trustworthy and nice and always there for you. But your friend is eccentric, okay? What do you do? What you do is you love your friend because we all love eccentric people.
Starting point is 00:42:03 Like we're all eccentric to some degree. I'm eccentric, we're all eccentric. We like eccentric people. Eccentric people are interesting. They're interesting because they're often surprising and they're creative and you never know what you're gonna get and it's always very interesting. Even if it's sometimes like confusing what they do.
Starting point is 00:42:18 But it's okay, right? They're just eccentric. We like eccentric people. And we've got eccentric physical theories. Newtonian physics, you know, despite its reputation of being, oh, it's Newtonian, it's classical, it's when everything made sense. There's a lot of stuff about Newtonian physics that doesn't make a lot of intuitive sense, right? You know, Newtonian physics says that a system, a body in motion will just stay in motion unless it's acted upon by something.
Starting point is 00:42:44 It doesn't come to rest. That's very unintuitive. We intuitively feel like things should come to rest. Aristotle believed that the natural state of all objects was at rest. And in Newtonian physics, it's just not. You need an explanation for why a thing would come to rest. But there are a lot of other examples like this
Starting point is 00:43:01 in Newtonian physics. We have all this intuition about how circular motion should work. We have this intuition that when you're, you know, moving water around in a bucket that there's a centrifugal force pulling it in. That's intuitive, but that's like not how it really works. Gyroscopes are where all intuition breaks down, right? That's all Newtonian physics. Newtonian physics is filled with things that are a little bit unintuitive.
Starting point is 00:43:27 And things only get worse from there. I mean, special relativity is super unintuitive. We talked about time dilation, the idea that the time progresses differently for observers in different frames of motion, that what we call all the events that are simultaneous, like they're all happening now, our notion of now is relative and the different people will disagree on which events are now and
Starting point is 00:43:47 which events are in the future and the past. That's very unintuitive. And don't even get me started about gender relativity. So I love gender relativity. I have taught gender relativity here. So we have a graduate level course in gender relativity, physics 210. It's like one of my favorite courses to teach. I've been teaching for over 10 years.
Starting point is 00:44:05 I learn something new about general relativity every time. I'm always surprised. General relativity, that class is like an eccentric friend. Every time I teach it, it's like you learn something totally new and surprising. And you're like, really, it really works this way. It really does. So, general relativity is another example of a theory
Starting point is 00:44:23 that is just really, really deeply unintuitive. I mean, we always set aside like a half hour every time I teach the class just to talk about the weirdness of black holes. And this is just not even like when you start worrying about quantum effects, just like regular treating black holes as classical objects. Black holes are really unintuitive in a lot of ways. And so I'll just set aside half an hour. I'll just open the floor and I'll just ask students to ask me whatever weird questions they have in the black holes. Like, student will be like, if I stick my arm in a black hole, and can I pull it out? Or, or all these weird things you could ask, like, what does it look like if I send someone to a black hole? Can they ever come? All these like weird questions you could ask. So, general relativity is super, super unintuitive. Jackson, Jackson level electromagnetism. So one of the course I teach is Jackson level electromagnetism. So one of the course I teach is Jackson level electromagnetism. There are a lot of very unintuitive things that happen in electromagnetism also. So it's not that we don't have theories that are eccentric, we do.
Starting point is 00:45:17 I should say that all of these theories do have places where they break down. The breakdown in a physical theory is called, well, a singularity in the theory. Singularities aren't necessarily geometric point-like things. They're just places where your equations stop working. Electromagnetism has this famous divergence of the self-energy of point particles. General relativity famously has singularities. Everyone's heard of the singularities of the Big Bang
Starting point is 00:45:39 and black holes and various other places where general relativity breaks down. Newtonian mechanics has weird singular behavior in certain kinds of systems. Yeah, yep. There's a famous paper by Shia in the 1990s on a five body system that exhibits singular behavior. And it was originally predicted that this could exist
Starting point is 00:45:57 by Poincare, I think a century earlier. So, you know, all these theories of places they break down and what do we do as philosophers, as scientists, as physicists, whatever, we look at these theories and we go, okay, the theories work in these regimes. Sometimes they make very unintuitive claims or predictions, and we're okay with that. We like weird, cool physics, as long as it's self-consistent. And there are certain places in which the theory breaks down, and we'll need to either replace the theory with something else if we're lucky.
Starting point is 00:46:21 If we're unlucky, maybe we won't find a better theory that will replace it, whatever. Quantum mechanics is kind of like that, right? There are regimes in which you're working with microscopic systems and quantum mechanics is nice and self-consistent. We don't run into these ambiguities or inconsistencies. It's a little unintuitive in some of these situations, sure. But when you confront something like the Vigner's Friend thought experiment and other thought experiments people have proposed over the years, now you're talking not about things being unintuitive. You're talking about a singularity in the
Starting point is 00:46:53 theory. You're talking about an inconsistency. You're talking about something where the theory is just broken. No one would say, well, you know, the self-energy of a point particle like magnetism is just unintuitive. People would say, this is clearly something wrong that we need to fix. And all I'm saying is the same thing is true of quantum mechanics. There are regimes in which it works well, and there are other situations that we can extrapolate it to where things seem to break down. These situations do entail an extrapolation of the theory from microscopic physics to
Starting point is 00:47:25 macroscopic physics. I mean, we're assuming you can go from, you know, the level of an angstrom, 10 to the negative 10 meters, that's 10 billionths of a meter, all the way up to a one meter scale, the size of a human. You know, to get the Wigner's Thenthor experiment, you have to have an extrapolation of the theory to that size. Either you can do that extrapolation and you run into the Wigner's Synthartic experiment, you have to have an extrapolation of the theory to that size. Either you can do that extrapolation and you run into the Wigner's friend problem, or you can't, but if you can't,
Starting point is 00:47:51 well then there must be some other place where the theory breaks down. In any event, something goes wrong. And we just have to deal with that. We have to confront that problem and manage it. But I would go a step farther than that. It's not just that the theory seems to have places where it's ambiguous about what it's predicting or where it's inconsistent.
Starting point is 00:48:14 The theory also only makes a very narrow kind of prediction, according to the Dirac, Von Neumann axioms. So the Dirac, Von Neumann axioms, and again, these are the axioms you'll read if you pick up Griffith's textbook on quantum mechanics or Shankar's textbook on quantum mechanics or Sakharaj's, you know, all the standard textbooks, Townsend's book on quantum mechanics, Gottfried's book on quantum mechanics, Leibov.
Starting point is 00:48:40 The theory predicts measurement outcomes. It predicts what you'll see on the readings, on the dials, on the gauges, on the displays of measuring devices. And it predicts the probability with which you will see those readings on measuring devices. You can compute averages in these theories. They're called expectation values, but those averages are definitionally, axiomatically, statistically weighted averages
Starting point is 00:49:12 of numerical measurement results, weighted by measurement outcome probabilities. We're talking about a very narrow kind of phenomenon, right? A very narrow category of phenomena. The Dirac-von-Neumann formulation of quantum mechanics predicts measurements, what happens with measurements. It's a very narrow slice, a very narrow category of phenomena.
Starting point is 00:49:38 When we spoke last time, we talked about how there are all other kinds of phenomena that seem to be happening around us. In the deep past, you know, primordial gases mixing in the early universe. Today, birds foraging, people falling in love, all that stuff. There's like lots of phenomena that seem to be taking place that all lie, strictly speaking, outside the axiomatic ambit of the Dirac-von Neumann axioms.
Starting point is 00:50:00 So what are we to do with this? We either say that Dirac- Neumann quantum mechanics simply is not giving a complete description of nature Which is kind of sad and if it's not where is the outer boundary? Now, there are some philosophers who defend this point of view Nancy Cartwright is a famous philosopher who has argued that maybe we just have different theories in different domains, the universe is many dappled. They're just like different theories for different things. But it would certainly be an interesting intellectual exercise and it would certainly be nice if we could extend quantum theory to describe more of the world.
Starting point is 00:50:34 If we do that, now we have a job to do. We either have to explain why all these other phenomena are in fact measurements, despite the lack of measuring devices or whatever, we have to somehow show that all of these things are in fact measurements, despite the lack of measuring devices or whatever. We have to somehow show that all these things are in fact measurements, and therefore in fact lie within the axiomatic ambit of theory. Some people propose that. But the onus is on them to show that it really works. And it's not clear that it does. Or we need to somehow extend the theory,
Starting point is 00:51:00 change the axioms in order to encompass more of the world. And that's part of what I'm interested in doing. Now, there are people who will say, wait a second, decoherence. What about decoherence, right? I mean, sure, okay, fine. The philosophers, or at least physicists who cared a lot about philosophy,
Starting point is 00:51:18 they gave us decoherence, but we haven't now. Doesn't decoherence solve all these problems? Well, Bohm certainly didn't think it'd solve these problems. He introduced decoherence, and it was insufficient. And ultimately, he introduced his pilot wave corpuscular theory in order to actually get a result. The reason decoherence doesn't do the job is decoherence takes a wave function or state vector, more generally what's called the density matrix,
Starting point is 00:51:44 the density operator. And it shows that under certain circumstances, when it's evolving interacting with an environment in the right way or interacting with a measuring device that's coupled to an environment the right way, the density matrix will change in a certain way. It'll become approximately what we call a diagonal matrix in a certain representation. We call this a basis. And you know, there'll be some entries on the sort of diagonal of the matrix and the other entries will be approximately zero.
Starting point is 00:52:07 At this point we're supposed to say the measurement's been done and there's an outcome. The problem is there's nothing in the dynamics, not in the Schrodinger equation, not in the generalizations of the Schrodinger equation, not in the Lindblad equation or the quantum channels that you use to describe this. There's no known dynamics within normal quantum theory that singles out one of the outcomes. You still need to apply the Born rule to get a probability out of this. And you still need to apply a projection postulate
Starting point is 00:52:38 to single out one outcome. There's nothing in the dynamics that will do that for you. And from time to time, people have proposed that maybe there's some sufficiently complicated quantum standard textbook quantum dynamics that will in fact cause the system to single out one outcome, but this is impossible because of the no communication theorem,
Starting point is 00:52:58 the no signaling theorem that I mentioned before. Collapsing down to individual states looks superficially like a non-local process, and you can't get a non-local process happening from what we call a local Hamiltonian. And this is guaranteed by the no signaling theorem. So there's definitely something that's just not working here. And pinning all this down, not just hand waving and saying, oh, decoherence, don't ask me any more questions,
Starting point is 00:53:22 pinning this down is a worthwhile exercise. Subjecting this problem to rigorous scrutiny may bear fruit. It has borne fruit already, and I would argue it will continue to bear fruit going forward. Hi, everyone. Hope you're enjoying today's episode. If you're hungry for deeper dives into physics, AI, consciousness, philosophy, along with my personal reflections, you'll find it all on my sub stack. Subscribers get first access to new episodes, new posts as well, behind the scenes insights, and the chance to be a part of a thriving community of like-minded pilgrimers. By joining, you'll directly be supporting my work and helping keep these conversations at the cutting edge. So click the link on screen here. Hit subscribe and let's keep pushing the boundaries of knowledge together.
Starting point is 00:54:11 Thank you and enjoy the show. Just so you know, if you're listening, it's C-U-R-T-J-A-I-M-U-N-G-A-L dot org. KurtJaimungal dot org. And I would argue it will continue to bear fruit going forward. Now going forward, I'd like to talk about your approach, your indivisible stochastic processes. Prior to that, okay, and just so people know, there are three sources. One is the previous interview that we've had with Jacob, and that's on screen right now. It's over two hours long and it's quite in-depth. Another source is I have a substack post where I cover my interpretation of Jacob's theory. And then the third is obviously your papers directly.
Starting point is 00:54:51 All three of these will be linked on screen and in the description. Prior to that, I want to talk about Wigner's thought experiment, his friend. How is that not just Schrodinger's cat but replacing the cat with a friend? You're completely right. I mean, if you think of the cat as an observer, and the quantum system being observed is the radioactive atomic nucleus that is momentarily in a superposition of decayed and not decayed, it is Wigner's Friend's thought experiment. When, I mean, the origins of the Schrodinger's cat thought experiment go back to discussions
Starting point is 00:55:29 between Einstein and Schrodinger. Einstein had a somewhat less playful example involving gunpowder that could either go off or not go off. And Schrodinger in this 1935 paper replaces this with this famous cat. But Schrodinger doesn't describe the cat as an observer. I think the real innovation is just rethinking the experiments. You could, I think, absolutely think of the cat as Wigner's friend. If you think that cats count as observers, which I do,
Starting point is 00:55:58 and friends, cats are friends and observers, absolutely, then it really, it's more a question of perspective, right? If you don't think of the cat as a candidate observer, then you're not doing the Vigners Friend Thought experiment. If you think of the cat as just as legitimate observer as a person, despite not having a PhD, there's always obligatory jokes that go with the Vigners Friend Thought experiment. You're always supposed to say something like, but don't call the humane society. I mean, I don't know why people always do that.
Starting point is 00:56:24 Scott Aronson has like some joke about why is it people always make jokes about this. But yes, if you think of the cat as an observer, then it is just the Wigner's Friend Thought Experiment. I think part of the reason why people like to separate these two is in some versions of the Wigner's Friend Thought Experiment, you're supposed to be able to ask a question to Wignerers Friend, like slide a little note in and ask questions. And if you ask the wrong kind of question, you'll cause a collapse. And if you ask the right kind of a question, you don't get a collapse.
Starting point is 00:56:55 And you can't do that with a cat. Cats don't talk. At least all the cats I've ever met don't talk. So there are some situations in which actually we do like it to be a sentient and sapient observer who can communicate. But broadly speaking, they are very similar thought experiments. Okay. Now, just before we move on, and we're going to get to some of the audience questions that people have asked both in the comments and then also on Twitter threads and so on about the previous podcast.
Starting point is 00:57:27 Okay. You mentioned Putnam earlier and then it's this eternalism because you can slice up any moment of now. So if there are multiple moments of now, then is it just that every single moment of now exists? Okay. What are the counter arguments to that? It's tough.
Starting point is 00:57:48 The Putnam argument for four-dimensionalism or eternalism is, it's a tough argument to refute, but there have been attempts. And I would recommend that people watching this read some of these papers because, you know, they're beautifully written by very smart, amazing people. So again, just to rehearse this argument, if you think of space for all purposes just as like a horizontal line and time as a vertical line, you can visualize all of space-time as like a, like think of graph paper with like the horizontal axis is space,
Starting point is 00:58:29 all three dimensions of space somehow like projected down into one dimension and then a vertical dimension, right? The idea is that what an observer calls now might be a horizontal line in this picture. All the moments at all points in space that are all happening at the same vertical time coordinate all the same time coordinates now and What special activity suggests is that if you're in a state of motion? Then that slice is tilted a little bit It's like not quite horizontal anymore relative to the first slice and so things that are further in the future compared with one observer are
Starting point is 00:59:04 In the present of the second observer and so forth. One way I like to think about this is the pancake model of space-time. So imagine a stack of pancakes. Each pancake is supposed to be all of space, the whole spatial universe at one moment in time. And think of this in the pre-relativistic idea, like the Newtonian conception that there's just a well-defined notion of what is all of space at every moment in time, you've got a stack of pancakes, and let's say one of the pancakes is the hot pancake.
Starting point is 00:59:30 The hot pancake is the now pancake. It's the pancake that is what's happening right now. And somehow the hot pancake is somehow incrementing, right? And this is the passage of time. Now you run into some very deep questions like how quickly are the pancakes moving? They're moving at one second per second. Does one second per second make sense?
Starting point is 00:59:48 If you divide a second by a second, isn't that just unitless? Like, what are we talking about? How does, okay, but let's put all that aside for a second. Just imagine that there is some notion of a moving now, this sort of metaphysically presentist idea that the present exists, it's a well-defined thing, and it is somehow incrementing forward.
Starting point is 01:00:03 What special TV seems to suggest is that observers in different states of motion will slice the stack of pancakes slightly diagonally. And so an observer who is moving at some, you know, it doesn't even have to be super fast, because if you talk about the whole universe, even slow motion will actually, you know, ultimately produce a clear discrepancy. But, you know, the slices are now tilted. And if you're cutting the stack of pancakes at a slight tilt, how can there be a hot pancake anymore?
Starting point is 01:00:33 The two observers don't even agree on whether the slices are horizontal slices or diagonal slices. How could there be a metaphysically invariant notion that one of them in one particular slicing is in fact the hot pancake. So you can see why this is like a very difficult argument to refute. But there have been attempts. So Brad Scout, MIT has a book with a particular perspective on this.
Starting point is 01:00:58 I encourage people to take a look at this approach. Another approach is Jean Annis-Mail, who is at Johns Hopkins University, philosopher of physics, philosopher of science. She has a book called How Physics Makes Us Free. And she has a very interesting argument about how you might get around this problem. I'm not going to be able to do justice to the argument here, but I would recommend people read the book, because she's a fantastic writer, and I think people will find it very interesting to read this book. There's a paper from not long ago by David Wheelys at Princeton.
Starting point is 01:01:28 He's a metaphysician who does some work in philosophy of science also at Princeton. And he has an argument that, you know, putting aside the special at this argument, he's like, you know, maybe we can't, maybe it's a difficult argument to deal with, but at least rather than try to refute that negative argument, an argument against presentism, maybe there are good arguments for presentism. We should focus on those. And his argument in that paper is that many of our fundamental laws of physics appear to be Markovian. And Markovian laws are by definition laws that take a notion of a present state and tell you the later states without really worrying about anything in the past. And he's like, you know, why should the laws be Markovian if we're living in an eternalist
Starting point is 01:02:08 universe, if we live in an eternalist four dimensional universe where the whole block is just like there? Why would our laws only care about the present state? There'd be no explanation for this. But if only the present really exists and the past doesn't exist, that would give an explanation for why our laws only care about the present. Unfortunately, as I'm sure you and people who are watching will surmise, I have some issues with this argument
Starting point is 01:02:32 because the whole point of the formulation of quantum mechanics we're gonna talk about is that actually the laws may not fundamentally be Markovian at all. And if they're not Markovian, then all of a sudden that argument doesn't maybe work so well. Yeah. It's my understanding, we're going to get to it, that your evolution laws depend on the past, and it's not as if they depend on the future.
Starting point is 01:02:53 Right. So in the eternalist state, when they're saying that why would we privilege the present, and then you're saying, well, in yours, you're not, but you're also not privileging the future. You actually are privileging the past. So you still don't take an eternalist's block. So this is a subtlety, right? The fundamental laws of physics that we know about today, to a very good approximation, have a feature called time-aversal invariance or time symmetry.
Starting point is 01:03:27 Newtonian mechanics, famously if you run a system in one particular, you know, in some particular process and then someone plays a reverse version of the, you watch a video of it and someone's rewinding and they're rewinding at normal speed and you watch the whole thing happen in reverse. Although they look weird or unlikely, there doesn't appear to be any violation of Antony physics in what you're seeing.
Starting point is 01:03:48 So famous example, a teacup falls off of the table, shatters, you could also have all the pieces have just the right initial conditions so that they have some initial velocity that's just right to bounce them together and they just land perfectly together and they reseal together and form a teacup and the teacup has just the right kinetic energy that it bounces off the lines on the table like it's unlikely but doesn't actually
Starting point is 01:04:13 violate any of the laws in 20 physics and this this this works out pretty well until you get to the standard model there are some systems involving K-ons and standard model that exhibit a slight violation of time reversal invariance. Technically it's CP invariance, but the symmetry in which you replace particles and antiparticles is called C symmetry. The symmetry in which you do a parity or spatial reflection and everything is called parity symmetry
Starting point is 01:04:40 and then there's time reversal. And the standard model, our best theory of fundamental particle physics that's based on quantum field theory, has this feature that is exactly CPT invariant. If you take any process in the standard model and do a combined particle goes to anti-particle, vice versa and parity and time reversal transformation,
Starting point is 01:04:57 everything stays the same. And there are some systems that violate CP symmetry. And then by the CPT invariance, that means they violate T or time-reversal symmetry. But there are rare processes. It's not clear that they have anything to do with the macroscopic distinction of future and past that we tend to see.
Starting point is 01:05:16 There are some conjectures about this, but no one has a firm argument that these two things are closely related. So the idea of a physical theory like we're talking about that somehow privileges the past but not the future in an eternalist universe seems a little bit odd. I should say right off the bat that the indivisible stochastic formulation does not fundamentally privilege the past or the future. You could just as well formulate a quantum system that's going the other way. The theory doesn't specifically,
Starting point is 01:05:48 it's just that when you actually consider a particular system, it'll be a system in which the past plays a different role from the future, but you could also consider a system in which the future plays a different role from the past. We call it not a fundamental breaking of time reversal and variance, but a spontaneous breaking of time reversal and variance.
Starting point is 01:06:04 Not a breaking in the sense that fundamentally, like nature's somewhat picking out future versus past, but just that in a given instantiation, in a given situation, nature has to pick one particular direction in each instantiation and depicts one over the other. Like the laws of Newtonian mechanics fundamentally are rotation invariant,
Starting point is 01:06:22 but you are not rotation invariant. Your atoms formed in a particular shape, and whatever shape they formed, and toning mechanics fundamentally are rotation invariant, but you are not rotation invariant. Your atoms formed in a particular shape and whatever shape they formed, picked out a direction in space. So you spontaneously break rotation invariance, even though fundamentally like the laws in toning physics are rotation invariant.
Starting point is 01:06:36 The laws of quantum physics, according to this indivisible stochastic approach, are fundamentally time reversal invariant, but in a forgiven model, they will typically favor one direction of time over the other. I should have said there is one other way to save At least I can think of one other way to save the idea of a flow of time a directness to time and This is to say well, okay special relativity is a very good theory, but we're living in
Starting point is 01:07:02 is a very good theory, but we're living in an expanding universe. We're living in a space time that appears to go back to some kind of big bang hypersurface, some initial big bang everywhere. And, you know, distances between objects are growing with time in some particular way. It turns out that in these kinds of, we call them cosmologies.
Starting point is 01:07:26 So cosmology is the subject of the study of the universe, but a particular like space-time model that solves Einstein's field equations at the level of the whole universe is called a cosmology. And in the cosmology, we seem to be living in approximately what's called Einstein-Dissider cosmology, described by the FLRW model. In this model, there is in fact a preferred slicing of space, right? You just take every point in the universe and ask like how long ago was the Big Bang from that point?
Starting point is 01:07:59 And take all the points that are all 13.78 billion years since the Big Bang and they form a hypersurface. And if you just do that, you'll actually get kind of like a preferred slicing of the universe. And you might go, that seems to contradict special relativity, well, but general relativity is not special relativity.
Starting point is 01:08:16 General relativity is a different theory. And in general relativity, different space times can globally, like at the scale of the whole space time, spontaneously break the symmetry of the slicings, the so-called Lorentz symmetry. Because there's a preferred Big Bang hypersurface, there's a preferred foliation or slicing of space time into slices of now.
Starting point is 01:08:40 And so just the history of the universe, the way that it happened to be instantiated for the Bing appears to have picked out a preferred way to slice the universe. And then you could say, okay, well, then that really is the fundamental notion of time. Time is really flowing from one such surface to the next. And sure, if you zoom in really close to like a planet
Starting point is 01:09:03 or a star or some very localized thing, things look like special relativity. You don't notice the whole shape of the cosmology and all the different reference frames look the same and all the slicing's look like they're in the same footing. But on a global cosmological scale, there in fact is a preferred way to slice things and time really flows from one slice to the other
Starting point is 01:09:20 in some fundamental sense in that picture. But this leads to some other really deep questions. Is the geometry of our cosmology a fundamental fact? Or is it merely a contingency? Could the universe have formed in lots of other ways? And it just happened that it formed in this particular way with this preferred slicing. And if it was contingent, if the universe could have formed
Starting point is 01:09:43 in lots of ways or could have been eternal, but happened to form in this particular way, can you metaphysically say that time flows in some fundamental sense based on what was a contingent fact about the universe, right? Like, if you think the flow of time is some fundamental feature of reality, should it depend on accidents of history? No pun intended, but you get my point, right? So, just to close the circle, that's like one other way people have thought about maybe restoring a notion of the flow of time.
Starting point is 01:10:10 Okay. Sorry, that was a lot, but yeah. Okay, briefly, before we close that circle, you mentioned that in GR you can spontaneously break Lorentz symmetry. What's the difference between breaking a symmetry and spontaneously breaking a symmetry? Okay, so... Um... If you take a theory, and the basic, like, equations that formulate laws of that theory, simply fail to have a certain symmetry.
Starting point is 01:10:40 And by a symmetry here, I mean a transformation that would, maybe for certain kinds of theories, certain kind of laws, leave the laws unchanged. For this particular theory, they do not leave the laws unchanged. So let me give an example. Let's suppose that the universe is described by the Newtonian physics near Earth's surface, and that is the whole universe. There is in fact no Earth. The universe is infinitely big, and it is like Earth's surface forever, right? Earth's surface just goes on in every direction forever.
Starting point is 01:11:13 There is the ground, and it never ends. You can go as far as you want, and it doesn't wrap around. It just goes on forever, right? There's no planets or anything like that. The whole universe is just life near an infinitely big surface. That's all that there ever is. And that's fundamentally all that there is. It's not an accident of history.
Starting point is 01:11:32 That's just how the universe is. It was fundamentally like its existence is just this infinite ground that goes forever. And gravity points down. And that's a law of nature, a completely fundamental law of nature that gravity points down. This is a theory that fundamentally breaks three-dimensional rotation invariance. The basic laws of this theory include that there is a force called gravity that points in a particular direction and if you take any system in this universe and rotate it in a way that is not parallel to the ground,
Starting point is 01:12:06 universe and rotate it in a way that is not parallel to the ground, the laws look different now. Right? Things fall sideways now. Like the theory, the laws are not invariant under this transformation. We would call that an explicit breaking of rotation symmetry. I see. Okay. So I guess terminologically, I'm confused because breaking to me seems like it was there before and then now it's broken. So breaking in this instance just means it fails to have it to begin with. That's right. Fails to have it to begin with, that's the better way to say it. I guess the terminology is because these are often symmetries that were there in earlier theories and then maybe in a deeper theory the symmetry is gone.
Starting point is 01:12:38 So we say that like, that kaons violate time reversal symmetry, right? We call it a violation or breaking because before we discovered these particles, we thought it was a symmetry and it's broken by canes, right? So I think maybe that's one way to think about it. Or maybe it's that we have a lot of theories in which certain symmetries are approximately true, but they're like not exactly true. And then we can think of certain particular things
Starting point is 01:13:00 in the theory that violate it. Whereas broadly speaking, it's not violated. That's entirely fair. But the example of Spineisbrigg would be like the actual earth, right? The actual earth is not an infinite surface. It's a sphere in space. And when you're on the earth,
Starting point is 01:13:14 you do feel like gravity is pointing in a particular direction, but this is just an accident of earth being there. If you could delete the earth and we're just floating in space, then suddenly you would have full access to the right. There'd be no notion of up or down or left. Like the left or right is actually subtle because it's parity invariance, which is a different thing.
Starting point is 01:13:32 But I mean, there's no preferred like direction in space if Earth isn't there. Earth's presence by an accident of just, that's the way this particular corner of the universe was instantiated, not at the level of fundamentally changing laws of physics, but Earth being there and us living on the Earth makes us think that a symmetry that is fundamentally there, rotation variance, full three-dimensional rotation variance, is in fact not there.
Starting point is 01:13:52 It's hidden from us. Some people say spontaneous symmetry hiding is a better term than spontaneous symmetry breaking. But yeah, so this just points to this distinction between, am I really saying a certain symmetry is not there in the fundamental statement of the theory, or is it just hidden or missing because of the way that a particular system has instantiated the theory? Okay, so I didn't know that, for instance, when you were talking about molecules that form you
Starting point is 01:14:16 and the molecules have some rotational invariance, but you don't, thankfully, have that rotational invariance. I have a rotational invariance. As far as we can tell. But that forming of you was not spontaneous. So the person who's watching or listening is thinking, well, it took quite some time to form Jacob. Jacob didn't- The word spontaneous is a turvart, yeah.
Starting point is 01:14:33 Okay. Because I thought spontaneous symmetry breaking had to do with you have a potential well and then you get to the minimum of it and you produce some ghost-tone bosons. And I thought it was just for that case. I didn't realize it was any time that a symmetry was broken, you call it spontaneously broken. When it's broken by the way a particular system happens to form or a particular solution to the theory.
Starting point is 01:14:54 So another way to, here's another way to think about spontaneous symmetry breaking. There is a puzzle called Shape by Shape. It's this little, it's a square, it's this delightful little puzzle. You've got these yellow shapes and these orange shapes, and you have a picture you're supposed to create. And you take all the shapes
Starting point is 01:15:14 and you put them into the square and you try to fit them all in the square. And they have to fit exactly in the square with no gaps. And they have to replicate the picture you see. It's like a yellow background with an orange shape in the middle, and you have to replicate that. And the setup of this game is mirror symmetric.
Starting point is 01:15:31 It's a square, the playing field is a square, which is perfectly mirror symmetric. And although some of the pieces are what we call chiral, chiral means that they're handed. There's like, the pieces look like a left-handed piece or right-handed piece. It turns out they're not really chiral because you can just flip them over. You can flip them over and then you discover the fact that, yeah.
Starting point is 01:15:50 But in any particular way that they're flipped, they pick out what seems like one direction. So, you know, and there's like an equal number of pieces. Everything about the setup of this game is mirror symmetric. You can lay out the board, lay out all the pieces, lay them out in a way that, you know, you look at it in a picture and you just flip the thing over and it looks exactly the same. And you could even have a picture you're trying to make. And this picture you're trying to make
Starting point is 01:16:11 is also mirror symmetric, right? You look at the picture, it's some totally symmetric looking figure. And so you're like, okay, I should be able to take my symmetric puzzle pieces and create a symmetric picture. And I should be able to do it by putting the pieces into a configuration that is mirror symmetric. And it turns out some cases you can't.
Starting point is 01:16:29 In some cases, all the solutions to this problem, despite the fact that the problem, the laws of this system are mirror symmetric, none of its solutions are mirror symmetric. Once you've solved it, you discover that the solutions are always lopsided. There's like different pieces on one side versus the other, and there's no solution that is balanced and symmetric. We would say this is a system that entails spontaneous symmetry breaking. The equations, the fundamental laws are symmetric, but all
Starting point is 01:17:02 the possible ways to solve it are not. Now, you could also have systems, maybe there's a puzzle in which it can be solved in a symmetric way and it can also be solved in a non-symmetric way. We would still call the solutions that are not symmetric, but still solve the puzzle, we'd still call them spontaneous breaking solutions. So, this is a phenomenon that happens all over the place. There's another example that we've, you know, one of my colleagues here, Kamran Vafa, a professor of high energy theoretical physics, works in string theory. He has a lovely book called Puzzles to Solve the Universe, I think.
Starting point is 01:17:37 It's connected to a seminar course he teaches here. And he has this puzzle he really likes. It's this puzzle where you've got four cities that are on the corners of a square. And the question is, how can you connect them with roads? So you can get from any one city to any other city, driving on roads, using the minimum amount of road length or pavement possible. This problem is completely rotation symmetric.
Starting point is 01:18:03 It's a square, right? It was stated in a way that didn't privilege any direction, and you can always rotate the square any way you want. It looks the same. So you might think that the solution is going to be, I don't know, an X, but, you know, an X doesn't... An X works because you can make an X, and then you could go to the middle of the X, and you could get any city. It turns out that Xs use too much pavement.
Starting point is 01:18:21 The solutions that minimize the amount of pavement used are these kind of like double Y solutions. And there's one that goes horizontally and one that goes vertically. And these minimize the amount of pavement and they both violate the symmetry of the problem. So this is spontaneous image breaking and we see it all over the place.
Starting point is 01:18:38 If you've ever wondered, how can the universe look so asymmetric given that the fundamental laws of physics appear to have so many symmetries? Fundamental laws of physics don't seem to privilege direction to a very good approximation. They don't seem to privilege handedness, left versus right handedness.
Starting point is 01:18:57 They don't seem to privilege like the direction of time. And yet the universe looks so asymmetric. This is basically all just a huge set of examples of spontaneous visual breaking. You can have a fundamental system where the laws or the equations are fundamentally invariant under a bunch of symmetries, but when you actually write down the solutions to them,
Starting point is 01:19:17 every molecular configuration is a solution to the standard model. Many of them simply fail to have all the symmetries of the underlying theory. Okay, so we've made the audience sit elated too long now. So tell the audience and myself again a recapitulation of last podcast about what indivisible stochastic processes are. And if you feel like relating it to Bohmian mechanics, because people already know what Bohmian mechanics are, you've covered it, then feel free to do so as a bridge.
Starting point is 01:19:47 Sounds great, yeah. So the top line version of this is, you know, there's this joke about the television show Seinfeld being a show about nothing. This is a theory about something. It's a theory about phenomena happening. So again, we had this problem in the Dirac-Van Noyman formulation of quantum mechanics, the textbook formulation, that the only category of phenomena we're talking about is this narrow category of measurement outcomes, whereas we have this much bigger category of phenomena that's going to be happening all over the place. I call this the category problem. It's distinct from the famous measurement problem of quantum mechanics. So it'd be nice to have a theory in which stuff is just happening. Now, this is not the only approach that does this, and later on I'll talk about
Starting point is 01:20:28 pilot wave theory, Bohmian mechanics, the Everettian or many worlds approach, spontaneous collapse approaches. There are other reformulations of quantum mechanics in which phenomena are happening, and they all, in various ways, address this category problem that is not adequately addressed by standard theory. So one way to think about this is this is yet one more way to actually have phenomena happening in a broad sense beyond merely the narrow category of measurement outcomes.
Starting point is 01:20:57 Another way to think about this is it's a way to make the world safe for good old-fashioned probability theory. So when we do quantum mechanics according to the Hilbert space Dirac-von Neumann formulation, we have these very exotic mathematical entities, these vectors or density operators and Hilbert spaces and the Born rule, and it feels very different from ordinary probability theory. Probabilities do show up, but there are many things that you just can't do using probability theory. You have to use this much more ornate, esoteric apparatus, this formal apparatus in this sort of Hilbert space language. In this approach, we restore our ability to do
Starting point is 01:21:41 quantum mechanics using good old-fashioned probability theory. That's one other way to think about what we're trying to accomplish with all of this. But let me actually go one step deeper before I lay out how it works. Another way to think about this is there are two long-running prevailing assumptions about what physical theories are supposed to be like. One assumption is that laws of a theory should be Markovian. Laws of a theory should take some notion of a present physical state and then tell you what happens next.
Starting point is 01:22:20 If your theory is time-reversible, the laws are time-reversible, then it should also be able to tell you what would happen previously, at least in principle. Another of the two assumptions is that there's an all-or-nothing deal when it comes to observables. The things we can observe about a theory are either all there, they're all, when we measure some observable, we are passively revealing some existing feature or property of our system, in which case we should be able to describe these things with any kind of probability
Starting point is 01:22:54 distribution we want, including joint probabilities, where we can say, what's the probability that this observable has this pre-existing value and that observable has that pre-existing value and that observable, and we can put a probability distribution on all of these things in some simple way. And if we can't, then we just give up. If we can't, then it's all out the window. Can't do it.
Starting point is 01:23:13 There are good reasons to think that we can't do this in quantum mechanics. There's a famous no-go theorem, originally proved by Bell, but because of the way that it was published, the first version that came into print, I think, was by Kochen and Specker in the 1960s. It's called the Kochen-Specker-Nogo theorem. And the Kochen-Specker theorem basically says that there are some quantum systems in which this is impossible. There are some systems in which you cannot assume all observable things
Starting point is 01:23:40 have prior values that you are merely passively revealing. And there's a beautiful way to explain it. A very simple version, much simpler than the original version, it's due to Asher Perez in the 1990s. Imagine you're playing a weird version of Tic-Tac-Toe. This is a very strange version of Tic-Tac-Toe. Here's how it's going to work. You know Tic-Tac-Toe?
Starting point is 01:24:02 This we call it in America. I know it's not called, it's called crosses and O's or whatever in different places. But Tic-Tac-Toe, you've got a grid, it's got nine empty squares. We're not gonna play it the normal way. We're gonna play it the following way. I am going to close my eyes and I'm going to imagine
Starting point is 01:24:17 an arrangement of O's and X's on this board. I'm gonna close my eyes and I'm gonna tell you, I promise you, I can visualize, I see it, I see a bunch of O's and X's. It's in my head. Believe me, I really know what it is. And what you're gonna do is you're gonna call out a single row or a single column.
Starting point is 01:24:36 That's it. And if your row or column that you call out has an odd number of X's, you win. If it has an even number of Xs, you win. If it has an even number of Xs, you lose. And you only get one try. If you guess and you fail, then we're done. You lose that round. We can play again, but then I have to come up
Starting point is 01:24:55 with a new board, okay? So super simple game. So the way that the game would work, and when I teach my philosophy quantum mechanics class, we do this, we do this example. I say, I've got the board, okay, and I'm gonna go to, first person, you pick a row or column, the person says,
Starting point is 01:25:08 second row, and I write X, O, X. Sorry, even number of X's, you lose. We erase it, I say, I'm coming up with a new board, and the second person says, I'm gonna pick the second row again, and this time the second row is O, O, O. Sorry, even number of X's, zero in this case, you lose. And then I erase it, I come up with a new board,
Starting point is 01:25:22 the next person goes, and they keep trying different rows and columns. What they discover is that every time they pick a row, they always get an even number of Xs. First row, it's always an even number of Xs. Second row, third row, always an even number of Xs. When they pick columns, the first column always an even number of Xs,
Starting point is 01:25:40 the second column always an even number of Xs. But the third always has an odd number of Xs every time. And so they learn this, they'll just keep picking the last column always an even number of X's, but the third always has an odd number of X's every time. And so they learn this, so just keep picking the last column and they always win. Just keep picking the last column and they always win. But then they go, well, wait a second, this doesn't make sense. If you've really thought of this board in your head, then you're saying that you've thought of a board in your head where every row has an even number of X's.
Starting point is 01:26:02 The first two columns also have an even number of X's, but the third column has an odd number of Xs. This is impossible. It can't be because even plus even plus even is even if all the rows secretly in my head have an even number of Xs. Like it can't be just an image in your head that's static. Right, there can't be a static image in my head in which all the rows have an even number of Xs.
Starting point is 01:26:21 And the first two columns have an even number, the third has an odd number because row plus row plus row, but even column plus column plus column would be odd. That's clearly incompatible. You must be creating the results only when we ask about them. You can't already have a preexisting board in your mind and I go, you win.
Starting point is 01:26:37 You're right. But there are quantum systems with this feature with nine observables, nine observables with the feature that the rows all have an even number and the first two columns have an even number but the last one is an odd number. And you look at the system and you go, there's no way this system could already know beforehand what it was gonna reveal.
Starting point is 01:26:56 The measurement process must bring about, at least in some cases, the results. So the hard way to read this is to say, well, if some results are the result of the measurement process and don't merely passively reveal a pre existing situation, then then there's simply no pre existing results. It's all or nothing. They're either all there or they're not there. That is also something I would push back on. So again, Markovianity in the laws, this assumption that laws should be things like differential equations that take the present state and give you later states.
Starting point is 01:27:32 And second, there's this all or nothing relationship, either all the things you could observe are there, waiting to be seen, can be assigned joint probability distributions as needed, or they're just like not there, there's just nothing there. And these are two things that are challenged in this approach. Both of these things are dropped, the Markovianity and this assumption. In this picture, the fundamental laws of nature are not Markovian and some observable quantities are reflecting things that are really there and others are emergent effects of the interaction between
Starting point is 01:28:00 the measuring device and the system being measured. This is one way in which the theory is actually quite similar to Bohmian mechanics. People have known for a very long time that in Bohmian mechanics, some things you observe like where your particles are, are revealing preexisting facts of the matter. Bell gave a word for things that were really out there. He called them not observables, but beables.
Starting point is 01:28:21 It's the way that the system can be, like beable instead of observable. Some people read it and think it's beable, but it's but beables. It's the way that the system can be like beable instead of observable. Some people read it and think it's beable, but it's actually beable. Whereas other things you can observe are not really reflecting a thing that was there. And they're just emergent features of the of the story. I call these emergibles instead of beables. To an external measuring device, they look just as real as a beable. But really, what you're seeing in a measuring device is this sort of emergent pattern. It's not really reflecting something that's fundamentally there.
Starting point is 01:28:47 Now, Bohm mechanics does this. In Bohmian mechanics, you know, the positions of particles are beables. You measure them and you're really seeing where the particles were. But when you measure like the momentum of your particle, the momentum you actually see in your experiment is not literally the pre-existing momentum, it's this sort of immersion defect of the interaction with the system. And there's a paper, you can look up on the archive, it's called Naive Realism about Operators. It's from 1996, it was written by Dahmer, Dürr, Goldstein and Zanghi.
Starting point is 01:29:21 And it's specifically about this thing, that to think that every self-adjoint operator that in textbook quantum mechanics, direct quantum mechanics, we would associate with the observable, is revealing something that pre-exists in the system is actually, as they put it, too naive. You can really have some things that are there and some things that are not there, and it's totally fine. It's not a serious problem. And I'll come back to this point a little bit later because some of the questions that
Starting point is 01:29:43 we've gotten from people have been about like basis dependence and in this picture, can you really measure everything? And the answer is you can. It's just that some of them are going to be be-ables and some of them are going to be emerge-ables. Okay, so we drop those two things. There's an old saying, I can't quite pin down who said it. Some people attribute it to John Wheeler again, that if you could explain quantum mechanics,
Starting point is 01:30:05 you should be able to say it in one sentence. I don't know if Wheeler was the one who originally said this. People can source this. But here it is in one sentence. In the indivisible formulation of quantum mechanics, every system has an actual configuration belonging to some menu of possible configurations we call the configuration space. I do have to put an and in, and there's a comma and an and,
Starting point is 01:30:31 it's still one sentence, and the dynamics, the dynamical rules, the laws by which the configuration changes with time is characterized by a sparse set of directed conditional probabilities that generically fail to be divisible in time. That's the whole picture. And in principle, you can get everything out of that one sentence. Everything is now just mathematics.
Starting point is 01:30:58 So there's no more ands. There's no more ands. That's it. That's the picture. Let's now, let's talk about like what, so if you want to talk in terms of Occam's razor, like this is, you know, we'll come back to Occam's razor in a little bit. Please. But, but, just say like this is, this is like axiomatically pretty simple.
Starting point is 01:31:15 There's no statement about Hilbert space or whatever. Everything is phrased in terms of things we know and are familiar with, configurations that physically are. Which configurations depend on the system? If you want to model a system of particles, you use particle configurations. If you want to use fields, you use field configurations. If you want to use whatever discrete registers in a qubit memory register, you'd use those. Whatever it is you want to use, discrete, continuous, whatever you want. And then the laws themselves are phrased as probabilistic
Starting point is 01:31:42 statements, but they're classical probabilities. They're classical, ordinary probabilities, classicals may be too strong a word because maybe you might demand that classical time-evolving probabilities must be Markovian. I don't, I think it's a little bit prejudicial to say that they have to be that way. But certainly they're just normal probabilities. They're not weird Hilbert space things. They don't have complex numbers in them. They're just regular probabilities. They sum to one.
Starting point is 01:32:03 They do the things that probabilities are supposed to do. That's the picture. And then in the first of the papers, the paper called the Stochastic Quantum Correspondence, which is on the archive, it's now just a set of mathematical mappings. You take this picture and you just do these sort of mathematical transformations and you end up with the same story but formulated in this Hilbert space language with time evolution operators and state vectors
Starting point is 01:32:31 and density operators and self adjoint. This picture is just like a different mathematical phrasing of this indivisible picture. And there's a lovely analogy to be found here between these indivisible systems, these indivisible systems, these indivisible stochastic systems that have this Hilbert space formulation
Starting point is 01:32:48 that's very exotic and has complex numbers in it and it's got all these weird symmetries, it's got basis invariance, you have all these different bases you can use. There's a beautiful correspondence between that connection, that stochastic quantum correspondence and the so-called Hamiltonian formulation of classical physics.
Starting point is 01:33:06 So Newtonian systems, classical Newtonian systems, interestingly are not quite Markovian, right? Think about it, right? You can't predict how a particle will behave knowing only its position. You actually have to know its position, and you have to know its infinitesimally earlier position. You actually need to know its position and you have to know its infinitesimally earlier position. You actually need two pieces of information. Now we don't usually formulate it that way because it's a little cumbersome to talk about where it is now and where it
Starting point is 01:33:33 is infinitesimally before, like DT, you know, D like infinite calculus, infinitesimal D before. That's like kind of cumbersome to do. So instead what we do is we subtract the two and divide by DT and call that a velocity. But it's the same information. If you want to like numerically simulate a Newtonian system and you like discretize time to do it, you would specify where it is now, where it was a moment ago, and you'd plug this into a discretized version of Newton's second law of force equals mass times acceleration and you would predict the behavior of the system.
Starting point is 01:34:04 So even a 20 physics is a little bit non-Markovian. But we do tricks. We don't like having it be non-Markovian. So what we do is we replace the two positions at the two infinitesimally adjacent times with a position and a so-called instantaneous velocity, which is kind of this trick so that we can treat these two things
Starting point is 01:34:22 as both being at the same time. And now we've made the formalism look Markovian. Now we have a state at the initial time that consists of both the coordinate, so called coordinate, the position and the velocity. But we need twice the variables now. We've increased the number of variables in order to phrase this thing as a Markovian system, and this is an old thing you can do with, in stochastic processes, the theory of stochastic processes,
Starting point is 01:34:46 if you consider a system that is a little bit non-Markovian, so not extremely non-Markovian, like these indivisible processes we're talking about, but a system in which you need to know the present state and maybe just one earlier state, maybe two earlier states, to then figure out how this system will evolve. You can take these systems
Starting point is 01:35:03 and you can treat them like they're Markovian by just increasing what you mean by the state space. I see. Like you triple the state space so that now you can just treat these three things as if they're all on one slice and now you've turned it to a Markovian system. And so there's this lore that you can take
Starting point is 01:35:18 any non-Markovian system and make it Markovian just at the cost of making the state space big enough. Just like in Newtonian mechanics, we take what was just coordinates and we double it to be coordinates and velocities, and now we have what looks like a Markovian description. This doesn't work for an indivisible system. When systems are sufficiently extremely non-Markovian,
Starting point is 01:35:34 you can't do this. And I think this was a little bit of tunnel vision. People thought, well, you can always do this, so what's so interesting about very non-Markovian systems? But if the system is non-Markovian enough, this trick doesn't work, and you actually have something that's really non-Markovian systems. But if the system is non-Markovian enough, this trick doesn't work, and you actually have something that's really non-trivially different.
Starting point is 01:35:47 But then what you can do is reformulate the Syntonian system in what's called the Hamiltonian formulation. And the Hamiltonian formulation, we rephrase what we were talking about the state space, the states, the positions and velocities in terms of what are called canonical coordinates, which kind of generalize the notion of the position, and the canonical momenta,
Starting point is 01:36:08 which generalize the idea of a velocity. And then we call the state space a phase space. The terminology apparently goes back to Boltzmann, who used the idea, because he was thinking in terms of like the phase of like a pendulum or something like that, some oscillatory system, like where is it in its motion, in its cycle, what phase is it in? This idea is much more general than that.
Starting point is 01:36:27 We call this a phase space. And in a phase space, we've got these variables, the Q variables, which are like the generalization of position, and the P variables, which are like the generalizations of velocity, the so-called canonical momenta. And in terms of the Qs and P's, we can reformulate Newton's laws as first order differential equations, which basically means Markovian. You specify the Q and the P, and then you uniquely get what the next Q and P are at
Starting point is 01:36:54 all subsequent moments in time. So this makes the system look like it's beautifully Markovian. Position and momentum are now in a perfectly equal footing. The differential geometry speak for this as we're now working on what's called the cotangent bundle of the configuration manifold, but it's not necessary to conceptually understand what's going on here. But what's interesting about this Hamiltonian formulation
Starting point is 01:37:13 is it looks weird. It has all these enhanced symmetries. For example, now that we've put the coordinates, the Qs, which again, generalize the notion of position, and the Ps, which generalize momentum, we've put them on this sort of very similar footing and they enter into the theory in this very equitable way. We can now do changes of variables
Starting point is 01:37:33 where we can take Q and replace it with P and P and replace it with negative Q. And in so doing, you could take a harmonic oscillator with a mass and a spring constant and get a new harmonic oscillator where the mass of the new harmonic oscillator is the reciprocal of the spring constant of the old and the new spring constant is the reciprocal of the mass of the old. But you could also do much more bizarre transformations.
Starting point is 01:37:55 These changes of variables, which are carefully designed to keep the equations, the laws looking very similar, are called canonical transformations. And there is a beautiful connection between these, changes of variables of your phase space, and basis transformations in Hilbert spaces. There's actually a beautiful mathematical relationship between them. It helped inspire Dirac to introduce his formulation of quantum mechanics, this sort of analogy
Starting point is 01:38:23 between these two things. And the analogy can make it even stronger through a series of papers. There was a paper by Franco Strocci in the 1960s called Complex Coordinates for Quantum Mechanics, I think. And then a paper in 1985 by Andre Heslott. And that paper, I can't remember the name of the paper, but it's from 1985, where they make this analogy
Starting point is 01:38:45 much tighter. They show that any quantum system in Hilbert space language can be rewritten in a way that looks just like a classical Hamiltonian system for a system of coupled harmonic oscillators. It's this beautiful framework I call the Stroche-Heslott formulation. And I think there's like a YouTube video of a talk I gave on it. If people want to see the details, we can link to that. People can see how it works. So the connection between this freedom to do all these weird changes of variables
Starting point is 01:39:08 that mix up what you mean by the Qs and what you mean by the Ps. You could make a new Q be Q plus P and a new P be, mix them up in all these bizarre ways that make the fundamental picture very murky. Like once we've done this, it's sort of hard to remember what our original system even was. There's a close connection
Starting point is 01:39:24 between that enhanced set of symmetries and the basis rotations in quantum mechanics. You also see the emergence of complex structure, complex numbers in the Hamiltonian formulation. There's a beautiful way you can take the Qs and the Ps and write the Qs as Q plus square root of minus one, the imaginary unit times P, up to some engineering dimensions. You have to get the units right.
Starting point is 01:39:48 But basically you can define a complex variable and rewrite the whole picture in complex coordinates and it simplifies the mathematics in a very beautiful way. And this brings the analogy out with quantum mechanics even tighter. For those viewers who know about Poisson brackets, if you rephrase Poisson brackets in terms of these sort of complex representations, it makes canonical quantization look even viewers who know about Poisson brackets, if you rephrase Poisson brackets in terms of these sort of complex representations, it makes canonical quantization look even more clean. So we have this incredible similarity.
Starting point is 01:40:13 You start with a non-Marcovian system, in this case just second-order non-Marcovian, Newtonian mechanics, depends on coordinates and like the previous time coordinate. And we can reformulate it as a, uh, Markovian looking, uh, beautiful, this Hamiltonian phase space formalism with all these enhanced symmetries and even complex structures, and we can do really powerful things. I mean, these canonical transformations can be used to solve all kinds of difficult problems in ways that are difficult to do in Newtonian mechanics. They even lead to a wave-like picture called the Hamilton-Jacobi formulation,
Starting point is 01:40:47 which led to Schrodinger discovering wave mechanics. And there's this complete analogy where you could take an indivisible stochastic system, which is also a non-Markovian system, much more non-Markovian and probabilistic, the system I just described to you that I laid out, and do this change of mathematical representation, and you get a Hilbert space picture,
Starting point is 01:41:09 which also is very exotic looking, and also has a very murky sort of physical world picture, and also has all these enhanced symmetries, these basis rotations, and also sees the emergence of complex numbers. The analogy is actually very close between these two pictures. And again, that change of representation to the Hilbert space picture is called the stochastic quantum correspondence. But now we can do all kinds of things that we couldn't do before.
Starting point is 01:41:32 Okay, so one example. Why is the dynamical equation of quantum mechanics Markovian? It's Markovian because you can just see as you do this change of representation, you can see how we took a non-Markovian thing and wrote it as a Markovian kind of evolution at the cost of introducing all of these weird new ingredients. The phases, the off-diagonal entries, the density matrices, interference effects, superposition. All of these ingredients are the cost that you incur by trying to represent what is fundamentally not a Markovian system, an extremely non-Markovian system
Starting point is 01:42:16 as a Markovian system, they're the prices you pay. We talked before about like, are these memory effects? Memory is not quite the right metaphor for indivisible stochastic processes. Traditional non-Markovian processes require that you specify sort of conditional probabilities, condition and arbitrarily many previous times. That's very complicated and has a lot of structure
Starting point is 01:42:40 and contains a lot of information. And you can legitimately ask, where is that information being stored? An indivisible process is actually much simpler. It doesn't entail the specification of all those higher order non-Markovian probabilities. It's much sparser. All you're supplied with are first order
Starting point is 01:42:54 conditional probabilities that don't concatenate, that can't be divided, that aren't Markovian. So there's actually less information and less memory, much less memory than is in a traditionally stated non-Murcovian process There's no question about where is the memory being stored? It's not that there's memory per se it's that the system's evolution doesn't depend only on the present state So memory is not quite the right word for it, but there's a kind of memory ish quite the right word for it, but there's a kind of memory-ish kind of thing.
Starting point is 01:43:26 And that's what's being encoded in all of those coherences and superposition interference, which otherwise don't have any, you know, in the traditional textbook formulation, they're just math that produce, you know, empirical implications when we do experiments. But like, we don't have like a meaning that we can attach to them. Here, we can attach a meaning. They're the artifacts of taking what is ultimately not a Markovian process and forcing it to be in a Markovian formalism. But we can go beyond that, right?
Starting point is 01:43:54 So we can explain why the equations look Markovian. We can explain what the interference terms are and the phases and the coherences and the superpositions. We can explain what those things are. We can also explain why the evolution law is linear. For a closed quantum system, a system that is not engaging in information exchange with its larger environment,
Starting point is 01:44:14 the evolution is given by a linear equation, the Schroedinger equation, if the system is sufficiently smoothly evolving in time or more generally unitary evolution. These are linear. And the question is, where does that linearity come from? It's just an axiom, according to the textbook Dirac von Neumann axioms,
Starting point is 01:44:29 but in the indivisible approach, it just comes right out of the change of representation. It comes out of the fact that ordinary probability has a linear law. If you're given initial probabilities and you wanna compute final probabilities and you're using the conditional probabilities that are given to you in laws, the relationship between the early probabilities and the later probabilities is a linear law. It's given by what's called Bayesian marginalization. I mean, there's various terms for it. Law of total probability. But it's a linear relationship and that linear relationship becomes the linearity
Starting point is 01:45:05 of time elution of quantum mechanics, so now that has an explanation too. And you might go, well, what about unitarity? I mean, I didn't start my indivisible process, how did it know to become unitary? It turns out that there's a class of indivisible processes called, they're based on what's called a unistochastic transition matrix. The term unistochastic goes back to a lecture in like the late 1980s, but the idea actually goes back, it's a much older term. So Robert Thompson introduced the term unistochastic, but the original term was orthostochastic and it was introduced by Alfred Horn, a mathematician in the 1950s.
Starting point is 01:45:45 And he wasn't studying stochastic processes. He was just studying the analytic properties, the pure math analytic properties of stochastic matrices. And he noted there was a particular kind of stochastic matrix, the kinds of matrices that show up in stochastic theories. These matrices are matrices with non-negative entries. They're square. They have non-negative entries, they're square, they have non-negative entries, and their columns all sum to one. But there's a particular subclass of them that he called orthostochastic, today we call them unistochastic, that have very beautiful, interesting analytic properties. From the standpoint of a pure mathematician, they have very neat properties.
Starting point is 01:46:19 The idea of building a physical stochastic process using these as the matrices that contain all of your conditional probabilities, that is new. I mean, that wasn't an idea that people had proposed. So you could just say the particular kind of indivisible processes I'm interested in are unistochastic processes. And these are exactly the processes
Starting point is 01:46:39 that when you run them through the stochastic quantum correspondence, on the other side, you end up with unitary evolution. Now you might go, that's a little dissatisfying because that'll explain why evolution is unitary. You had to assume a particularly special kind of stochastic process, of an indivisible process that it was unistochastic.
Starting point is 01:46:56 The technical definition is unistochastic process is a process where all the conditional probabilities are related in a very simple way to the entries of Unitary Matrix. That makes it seem a little bit too canned. But there's a theorem that's proved in the first of the papers, the Stochastic Quantum Correspondence paper, that even if you don't start with a unistochastic process,
Starting point is 01:47:18 even if you start with just a completely boring, ordinary, generic, indivisible stochastic process, you do the change of representation to the Hilbert space picture. You can always write that process as what's called a quantum channel. A quantum channel is also known as a linear completely positive trace preserving map. These are well studied in the quantum information literature. It's not obvious that you can do this, but you can. It's a simple, yeah. The mapping from the indivisible stochastic processes
Starting point is 01:47:49 to the Hilbert space picture can be represented by a quantum channel or is a quantum channel? So you start with your indivisible stochastic process, which is a probabilistic. It just says, given where the system is now, this is the probability it'll be there later. You run it through the stochastic quantum correspondence. You now have density matrices and state vectors,
Starting point is 01:48:08 all this stuff show up. And the time evolution is now carried out by what's called a time evolution operator that takes your current state and gives you your later state. In general, this time evolution operator is not unitary. Unless your original process was unistochastic. In general, if it's not originally unistochastic, then the time evolution operator will not be unistochastic. In general, if it's not originally unistochastic, then the time of the shepard will not be unistochastic.
Starting point is 01:48:28 But it turns out you can still write it as a quantum channel. This time evolution operator that shows up on the other side looks kind of weird, but it turns out it can be written as this very well studied thing called a quantum channel. And quantum channels can be turned into unitary evolution by another change of representation. Borrowing a theorem by Stein-Spring in the 50s, the Stein-Spring Dilation Theorem,
Starting point is 01:48:47 by increasing the dimension of your Hilbert space in a bounded way, for those who care, it's going from an n-dimensional Hilbert space to an n-cubed dimensional Hilbert space at the most, which corresponds to adding one or two extra degrees of freedom. You can implement the evolution as a unitary evolution anyway. And this is really cool because it means that even if you didn't start with a special kind of, you start with a totally generic indivisible stochastic process, all it's saying is, given the configuration of the system here,
Starting point is 01:49:14 here's the probability distribution of where it will be later. When you run it through this stochastic quantum correspondence, get a Hilbert space picture, you go, oh no, it's a Hilbert space picture, and I see a lot of stuff, but the evolution is not given by a unitary operator It's not given by the Schrodinger equation, you know, that's that's not great It turns out with a simple change of representation one second change of representation You can implement the evolution in a unitary way But what's called the dilation of the Hilbert space and this gives finally an explanation of where unitarity comes from
Starting point is 01:49:41 Where that axiom that the time of Luci be unitary, it emerges from this set of transformations. So it's really nice to be able to like explain where these things come from. And now I can get to a question that came up from a couple of people in the comments. It seems like we started with this indivisible stochastic process. We end up on this other side, and it kind of seems like one basis for the Hilbert space is special, right? So a Hilbert space is a vector space,
Starting point is 01:50:13 all of the objects, the state vectors are vectors, and people may know that a vector is a mathematical object. The simplest versions of vectors are arrows. Let's take an arrow, an arrow pointing in some direction in space with some direction and some length. And if you draw a coordinate system, imagine an arrow in like, on a graph paper, right? An arrow on graph paper, there's an x-axis and a y-axis, and you can ask, how far do we have to go along the x-axis,
Starting point is 01:50:41 and how far along do we have to go along the y-axis to get from the bottom of the arrow to the top of the arrow? And the distance along the x-axis and the distance along the y-axis, and how far along do we have to go along the y-axis to get from the bottom of the arrow to the top of the arrow. And the distance along the x-axis and the distance along the y-axis are called the components of the vector. It's got this x component and this y component. Those are the components of the vector. But if I change my axes, if I like turn them a little bit, without changing the arrow, the arrow is the same, but the axes have tilted, well, then I have different distances now. I have a new distance, the x' distance and the y' distance, the new distances.
Starting point is 01:51:10 So a single vector has different component representations depending which basis you use. And the Hilbert spaces of quantum mechanics have this feature. In quantum mechanics, the different bases are associated with different kinds of things you might want to measure. So, for example, if your vector is pointing exactly along a certain axis, it means that if you measure that observable, you're definitely gonna get that result and definitely no other results. But if you measure a different observable,
Starting point is 01:51:32 one whose axes are tilted, now your vector is not pointing exactly along that direction anymore. It's got some component along one axis and some component along another. And the Born rule tells you how to take those components and compute probabilities. And so we discover is that even if one observable has a definite result
Starting point is 01:51:45 because the arrow is pointing exactly along one axis, a different observable with different axes will give probabilistic results. And if you somehow change your arrow so it's pointing along one of those axes, now the first observable will not have a definite result and this is just the uncertainty principle. That for certain pairs of observables when you know one with certainty, when measurements are guaranteed to yield a definite result for one of them with certainty, measurements are not guaranteed to yield definite results for others with certainty.
Starting point is 01:52:09 This is related to the ability to change bases. You may wonder, is this basis dependence preserved? This base independence that I can take a vector and write it on any basis I want. But the answer is a lot like in Hamiltonian mechanics. We start with a physical system with an actual position and a particular momentum that has a clear meaning. It's the momentum, it's like for some systems, it's mass times velocity.
Starting point is 01:52:34 It's like a clear definition of momentum. We formulated in this Hamiltonian phase space picture. But then we can do all these weird canonical transformations where we can change variables and change what we mean by Q and change what we mean by P. And all of a sudden it's like not clear what the new Q means, what the new P means. And you might go, well, Newtonian mechanics must be wrong
Starting point is 01:52:56 because Newtonian mechanics didn't have this independence. Newtonian mechanics picked out a particular Q and P, but Hamiltonian mechanics treats them all like they're the same. There's this symmetry under changing your definition of Q and P, but Hamiltonian mechanics treats them all like they're the same. There's this symmetry under changing your definition of Q and P. This means that Newtonian mechanics is wrong because it doesn't have canonical transformation dependence. That's very analogous to what's going on here. It's true that you start with a particular system in the indivisible stochastic side of the picture.
Starting point is 01:53:21 The system has configurations. Those configurations correspond to a particular basis on the Hilbert space side. Once you're on the Hilbert space side, now you have the freedom to change your bases however you want. But because the theory is mathematic, like it's just a theorem, you can go from one picture to the other. And this Hilbert space picture is mathematically
Starting point is 01:53:35 a representation of the first picture. Just like in Hamiltonian classical mechanics, you have the freedom to do these basis transformations, they're totally available. The one lingering question you might ask now is, well, but can I measure other observable? Like the ones that were tied to the configurations are ones that will be very simple to represent
Starting point is 01:53:55 on the Hilbert space side. They correspond to what we call diagonal operators. What about all the other observables? The ones that are not diagonal, the ones that don't commute with the first set, that correspond to these other bases, right? Those can also be measured. What's going on with those? The answer is it's just like in bole mean mechanics. If you set your system up and couple it to a measuring device, and the measured device could measure one
Starting point is 01:54:17 of the beables, one of the ones that tightly corresponds to the original configurations, it will passively reveal what the system had as that feature. But if you change your measuring device, just pick up a quantum textbook, look at measurement, like how they formulate measurements in terms of unitary transformations, and just change your measuring device,
Starting point is 01:54:39 now it's gonna measure a different property, measure one of the immergibles. You run the exact same process, measuring device will stochastically end up in one of its measurement outcomes with the correct probability given by the Born Rule. It just comes out of the formalism. But the thing it's measuring is not a fundamental feature
Starting point is 01:54:56 of the system. It's measuring really like an emergent pattern of the mutual dynamics of the system itself and the measuring device measuring it. Some properties you're passively revealing what was already there, those correspond to that special basis. And properties that don't correspond to the special basis
Starting point is 01:55:13 can still be measured and they'll still produce results on measuring devices. And the measuring devices will still stochastically end up in their correct readout configurations with the correct probabilities. And as far as the measuring device is concerned, it has measured something just as real as for a beable. But what it's really measured
Starting point is 01:55:27 is one of these emergent patterns, these emergibles. And so from the point of view of like the outside world, the emergibles are on the same footing as the beables. Together the beables and the emergibles collectively form the full, we call it a non-community of algebra of observables for the quantum system. So this deals with this question of basis dependence. And this isn't new.
Starting point is 01:55:50 So another way to formulate quantum mechanics is the path integral formulation. So people may be familiar that there's this sort of Hilbert space formulation and there's this other formulation in which to predict probabilistically where the system will end up you're supposed to somehow start with initial configuration and write down every candidate trajectory the system could have. All the trajectories, ones that do not satisfy the classical laws of physics, every one you can imagine, assign each of them a special numerical factor, add all the factors together as this very tricky integration
Starting point is 01:56:22 called a functional integral, and get a complex number out that when you mod square it, do this particular operation on it, you get a probability. And you can reformulate quantum mechanics at least at the level of making its predictions in this way. This path integral formulation goes back to Paul Dirac in a 1932 paper. Oh, I didn't know that. Paul Dirac was the first to introduce it. All the way down to like you slice up the time interval into little bits and you introduce
Starting point is 01:56:47 complete sets. It's a beautiful, beautiful paper. He was trying to understand what is the role of the Lagrangian in these. So before 1932, people had formulated quantum mechanics in the language of Hamiltonians, in the language of Hamiltonian-Jacobi theory. And Dirac was just very curious. He wanted to know, does the Lagrangian formulation show up in quantum mechanics also? And he found this very beautiful way to do it
Starting point is 01:57:07 using these sort of functional integrals. But Dirac was just content to write it all out, like formally state everything and not turn it into a machine for calculating things. 10 years later, Richard Feynman picked it up while he was a PhD student. And this was like in 1942. He was a PhD student. And this was like in 1942. He was a PhD student at Princeton,
Starting point is 01:57:27 also again a student of John Wheeler. And he turned Dirac's formalism into an actual recipe for calculating things. And then a few years later, he ended up publishing a review article, talking in detail. And we can post all of these to the YouTube video if you want or people can see all these papers.
Starting point is 01:57:49 So a few years later he wrote a review article about all of this and he says at the beginning there's nothing so far that I can do with this that cannot be done with ordinary methods. You can imagine someone saying well then what good is it if it only makes the same predictions as ordinary quantum mechanics and you can't do anything with functional integrals or path integrals that you couldn't do with earlier methods, what use is it? And by the way, it also picks out a basis. Because to do the path integral formulation, you have to pick a basis. For example, when you do path integrals for particles, usually what you do is you pick positions, you pick what's called the position basis and you everything with positions. You don't usually do the path integral in other bases. You can, but any particular choice of how you formulate the path integral picks that one basis. So you could say, this is basis dependent. You could say it doesn't do anything
Starting point is 01:58:35 that we couldn't already do. It's a weird picture. And it was for a long time. And then eventually people discover there were some calculations that were just too hard to do in the traditional approach. Today, if you wanna formulate a non-abelian gauge theory, like a Yang-Mills theory, like QCD,
Starting point is 01:58:55 you're probably not gonna wanna do it using the canonical Hilbert space approach. You're probably gonna wanna do it with a functional pathological approach. Eventually, and it took many years, I mean, from 1932 until when people really needed these decades, were able to realize there were some things that now we could do much more easily
Starting point is 01:59:10 with this new formalism. So, of course, this gives me hope that formulating quantum mechanics in a new way, not the Hilbert space way, not the path integral way, a new way, even if it doesn't obviously do anything that you couldn't do otherwise, even if it doesn't obviously do anything that you couldn't do otherwise, even if there aren't any obvious immediate applications as the sort of thing that maybe 10, 15, who knows?
Starting point is 01:59:31 Feynman himself said that any good theorist should know a bunch of different ways to do the same thing because when you formulate a theory in multiple different ways, you discover different knobs you can turn, different things you could do that might have been harder to imagine doing in one formulation that are easier to imagine doing in another formulation. So that gets this sort of basis independence question. We can get to some of the other comments and questions people have had, but let me pause there and ask if you have questions before we go on. So let's see if I understand this correctly and I can simplify this.
Starting point is 02:00:02 So Markovian, let's understand what Markovian means. This means your system, you look at the present state and you can determine the next state. Okay, when we say the present state we tend to think, oh Newtonian mechanics is Markovian because you say, well let's specify the position and then maybe the mass and then the velocity as well. Now. But then you're saying, well what is the velocity? It's actually the position just an infinitesimal time ago. So you could introduce a new variable called velocity or you could just think of what the time is now and what the
Starting point is 02:00:34 time was ago, making it non-Markovian because it's now no longer the present. This is equivalent, I believe, it's equivalent to Newtonian, the Newtonian formulation, but in what we'reian, the Newtonian formulation, but in what we're taught as the Newtonian formulation you've introduced something new. So you're saying that look, in that similar manner, we can make an analogy here where there's these indivisible stochastic processes, these little guys operating around here. What exactly are they? I'm going to ask you about that afterward.
Starting point is 02:01:01 But they're operating here and they're stochastic. What about all these, you're saying they correspond to quantum mechanics, how? Quantum mechanics is linearity, unitarity, superposition, interference. Are you suggesting that when we take this non-Markovian and we make it Markovian, that just as in the Newtonian case we introduce something new, that we're introducing something new, and those correspond to linearity, superposition, interference, and so on. Yeah. Yeah. And complex structure and basis, and the ability to change bases and all this stuff, they all, it's exactly right. It's exactly right.
Starting point is 02:01:37 Okay. Okay. So now the question that the audience has or had is, how do you deal with interference experiments? Also, we can get to it in order, if you like, Bell. What does it say about the Bell's inequality? And what are the beables exactly in this framework, this formulation? Let me start with the interference experiment ones. Let's start there.
Starting point is 02:01:59 So the simplest answer to that question is if there's a mathematical duality or representation that takes you from an indivisible stochastic process to this Hilbert space picture, and let me just quickly say, the mapping is not one-to-one, it's many-to-many. A given indivisible stochastic process may have many Hilbert space representations, and a given Hilbert space representation can represent many different indivisible stochastic processes, but this is not new. The same relationship holds for Newtonian systems and Hamiltonian formulation. A single Newtonian system can have multiple different Hamiltonian formulations and a single Hamiltonian formulation can represent many different Newtonian systems. So this is not like a new thing.
Starting point is 02:02:37 Okay, but the point is that these indivisible systems do have this representation in this sort of Hilbert space picture. And the representation is just math. I mean, every Hilbert space picture can be regarded as an indivisible stochastic system in disguise and vice versa. So any predictions you make with a Hilbert space picture are going to be preserved. The explanation though is gonna be different. So let's take the double slit experiment. And this is actually gonna be helpful because I think one question someone had was,
Starting point is 02:03:11 can I give a hello world example? You know, computer programming, the simplest program you read is something that just prints hello world. What's the simplest example I can give? I'll give you a simple example. Let's consider a double slit experiment and we'll make it so simple.
Starting point is 02:03:23 We're gonna coarse grain it, that's the term of art. We're going to coarse grain it to simplify it. So instead of the particle being able to be just like anywhere, we're going to coarse grain the description so that we're only talking about is the particle in the upper part of the chamber or the lower part of the chamber. Just upper and lower. Basically turning the particle into a qubit, into a two quantum state system. It's a two state system.
Starting point is 02:03:44 Upper chamber, lower chamber. The particle is upper chamber, lower chamber. It then, in a, and we'll just imagine that something is like sliding it forward and just some like, just keep it super simple. We're sliding the particle forward, it encounters a wall, and the wall's got an upper hole and a lower hole, right? As walls do.
Starting point is 02:04:00 As wall, well, not all walls have upper holes and lower holes, this particular wall is an upper hole and a lower hole. And then beyond the wall there is a projection, a detection screen, a screen where the particle can land and we're going to coarse-screen that the particle can land in the upper part or the lower part of the screen. So this system is sufficiently simple that it actually encompasses many systems you might deal with in quantum information.
Starting point is 02:04:21 Mach-Zehnder interferometers, there were some questions about Mach-Zehnder interferometers and the Elitzer vitamin bomb tester example. These are all based on a very similar kind of very simplified coarse-grained version of the double slit experiment. Now I'm not going to be able to do the calculations in the air. When I teach my class on philosophy of quantum mechanics, I do go through the calculations and I've got a nice write-up and if you want I can send you a draft of it. It's not in the paper yet, but I can send through the calculations and I've got a nice write up and if you want I can send you a draft of it, it's not in paper yet,
Starting point is 02:04:45 but I can send you the draft and show you all the steps. But even this example, right, because we're filling in all the details now in the traditional textbook approach, you basically set it up and then you measure the end and you don't really talk about what's going on ontologically, physically in between. I mean, you're writing like a wave equation,
Starting point is 02:05:01 you think in terms of waves, but of course the moment you go beyond one particle to 10 or 20, something of the wave picture is now in a 20 dimensional space, it doesn't make any intuitive sense. We're doing it very differently. We're actually gonna follow the particle and write down the probabilities, write everything down.
Starting point is 02:05:16 And what you do when you do this is, every time you run the experiment, one particle going through the particle lands in the upper chamber, upper part of the detection screen or the lower part. And you do this experiment many times. Every run of the experiment, the particle lands in just upper chamber, upper part of the detection screen or the lower part. And you do this experiment many times. Every run of the experiment,
Starting point is 02:05:27 the particle lands in just one spot, either the upper part or the lower part. Over many, many, many repetitions of the experiment, you build up a histogram. You build up like a distribution of landing sites. And what you find is those landing sites look just like the distribution you would have gotten if there had been wave interference in the problem. But there's no wave in the problem. There's actually no wave in the problem. And the interference is an artifact of the indivisibility. Why? How can we so there's a limit to how much we can say about like, because indivisible processes are by their nature really unintuitive. Physical theories can be unintuitive. That's the thing about physical theories.
Starting point is 02:06:05 But in this simple case, at least, we can actually shed some light on where the interference is coming from in this very simple example. And why there isn't interference when we do this, like with a Newtonian system. In a Newtonian system where you're just like throwing rocks at the wall, one at a time,
Starting point is 02:06:24 you don't over many landing sites get this distribution, this pattern. Why? One way to understand it is that if you're throwing the rocks and they're being thrown either deterministically or if we want to even like let it be probabilistic, we do probabilistically. The way you would say it is you would say,
Starting point is 02:06:42 okay, well, I throw the rock, it gets to the wall with the holes in it. Either it goes to the upper hole, or the lower hole. Let's suppose it goes to the upper hole. Now that we know it's at the upper hole, let's start there, and then use the laws of Newtonian mechanics to figure out where it goes. If it goes to the lower hole, let's start there and use the laws of Newtonian mechanics to figure out where it goes. But notice what I did there, I divided up the evolution. I assume that Newtonian, that the laws given to you in the system are of the form that you can take the system at the intermediate location, at the holes, and Newtonian mechanics gives you the laws for what happens next.
Starting point is 02:07:21 And when you do that, you get no interference. You get the standard pattern. In the indivisible formulation, you're not given those laws. The dynamical laws that describe where this particle is going do not have the feature that when they get to the middle wall and go through, I mean, the particle at any moment is only in one place. It's either in the upper hole or the lower hole, still true. But once it's there, you can't say,
Starting point is 02:07:43 all right, let's suppose it's in the upper hole. Let's restart the evolution, and But once it's there, you can't say, all right, well, let's suppose it's in the upper hole. Let's restart the evolution. And then the theory doesn't give you a law for that. There's simply no dynamical description for starting at the holes and then saying what comes next. It's not supplied in the laws. That is the indivisible law that describes the entire experiment from beginning to end
Starting point is 02:08:02 is more general. There's simply a more general class of such indivisible laws that fail to have this divisibility property at the holes. If we demand that the laws be divisible at the holes, we're singling out a subclass of indivisible processes. Cause you could just imagine, let me not consider the most general indivisible process. Let's consider just indivisible processes
Starting point is 02:08:24 where you're given the laws from the beginning to the wall, and you also have new laws that go from the wall to the screen. If you limit yourself to just those indivisible processes, you will see almost no interference. There'll be a little bit left because there's still some indivisibility, but it will mostly be gone. But if you don't limit yourself to those special cases,
Starting point is 02:08:44 you will in general see interference. and they will mostly be gone. But if you don't limit yourself to those special cases, you will in general see interference. So the failure of Markovianity at the holes, the inability to restart the evolution and have in your hands the laws for what comes next during the holes, the failure to have that means that you can have the kinds of laws that will lead to interference. Now, there are modifications to this experiment.
Starting point is 02:09:04 For example, what if you look to see what hole the particle goes through? And we can implement this very simply by adding another two state, two configuration system near the holes. Suppose I've got a little second particle, little second device with two configurations. And all it does is it stays off
Starting point is 02:09:24 in its initial off configuration if the particle goes to the upper hole. If the particle goes to the lower hole, it switches to on. Okay? That's all it does. It just does these two things. Sure. You can model this very neatly.
Starting point is 02:09:35 You put it in. You actually want to give this thing deterministic laws. You want this to deterministically have the property that when the particle goes to the upper hole, it always stays off. I mean, it goes to the lower hole, it always changes to on. You can implement that with a pretty easy set of equations, give it that deterministic behavior. Now, when you evolve the system, the interference goes away.
Starting point is 02:09:55 You can just, I mean, you just rerun the indivisible process and you'll see that there's just no interference anymore. What's really nice, and this is actually a really nice example of this, is if you throw away the information that was in that little detector particle, the one that was detecting it, or if the detector particle communicates with the outside world and that information is now irretrievable and it's not accessible to us. And what we can do is classically marginalize. So marginalization is when you have a joint probability distribution, it's a probability for like two things, and we sum over one of the variables to drop it out of our awareness. This is a standard move in ordinary probability
Starting point is 02:10:36 theory. When you do that for the time evolving process, the time evolving process for the original particle suddenly has a division event, a division that is now available at the walls. And so what was an indivisible process is now divisible at the walls, thanks to the detector particle that we have marginalized out. And this is another way to see that divisibility is now restored at the walls and gives another way to understand why the interference effects go away. But there are a couple things to say about this. Number one, this division event is related to decoherence.
Starting point is 02:11:14 I mean, the process by which we marginalize is just in stochastic language, which in Hilbert space language we would call decoherence. If you look at density matrices, you'll see that the division event, seen at the level of the Hilbert space corresponds to off-diagelentries disappearing. That's what happens in decoherence. But the crucial thing here is there was no wave function here. The particle always had one location as it was moving through the apparatus. There was no superposition.
Starting point is 02:11:44 There's nothing to collapse. So if the question is, isn't a division event just collapse? Well, no, there was no wave function, the particle was not superposed between being in the upper and lower parts of the chamber, nothing ever had to collapse. The division event is what you would say on the stochastic side of the correspondence, what decoherence is on the other side. But because there was never a superposition, there's no need to now single out one outcome or collapse anything or project anything.
Starting point is 02:12:14 So the measurement problem, this basic fact that in the textbook formulation, you bring in a measuring device, it becomes entangled, you get a superposition, now you have all these superposed possibilities. And then somehow if somewhere in the superposition there is a measuring device, it becomes entangled, you get a superposition, now you have all these superposed possibilities, and then somehow if somewhere in the superposition there is a measuring device, we're supposed to collapse it somehow, but why and what magical property of measuring devices makes things collapse? This is the measurement problem. It just fails to happen in this picture.
Starting point is 02:12:36 There's never a need to get anything to collapse. So I would say that's the simplest hello world example and has the side effect of also explaining what's going on in the double slit experiment and what interference is happening here. So is the division event your version of what traditionally is thought of as collapse? And are division events just what occurs when you integrate out over marginal probability? That's right. So you marginalize over whatever has read out the configuration of your system and then
Starting point is 02:13:03 your system now has what looks like divisible stochastic dynamics. And this certainly plays a functional role in the theory that is analogous to what decoherence and then collapse plays in Hilbert's, in the Dirac-Feyer axioms. And certainly if you're gonna write this story in Hilbert space language, you would use decoherence and collapse to explain what's going on in Hilbert space picture.
Starting point is 02:13:29 But now we have underwritten those weird axioms that seem very ad hoc and mysterious with a very boring stochastic process where there is no wave function to collapse. And when the measurement happens, in this case just a readout from a little detector bit, there's just a classical marginalization that causes the indivisible dynamics to have an event when you can divide. It's momentarily divisible and then the inference goes away. So I want to bring up something that you just mentioned, which harkens back to earlier in the conversation. So you said in the Newtonian picture, you throw a ball and there are two slits, two holes, and then you notice that it goes over the top one, you say, okay, let's just start the
Starting point is 02:14:12 evolution from here or the bottom one you go from there. And you said, well, this doesn't apply in the quantum case or in the indivisible case because you can't divide. And what was interesting to me was you said, notice that so and so. And what you said, which is notice that you said, hey, you can look at it now. So in other words, you can divide your time. I was thinking, okay, I didn't, as I was following you along, I didn't notice that I was making that assumption.
Starting point is 02:14:36 And earlier in the conversation, you said, what philosophers are extremely trained in is noticing implicit assumptions. Yes. So this, even though, even though this is, even though it's not, well let me read about Hegel because Hegel will inform my physics, it's not that per se, even though that may be the case. I'm sure there's some inspiration that can be taken there. It's also the thinking that Hegel had or the thinking that philosophers have that you can apply. Yeah, I mean it's important to know that philosophy is a huge discipline, right?
Starting point is 02:15:07 And, you know, there's ancient Greek philosophy, there are all kinds of philosophies associated with different areas of the world historically. And in the Western tradition, so to speak, there's early modern philosophy, and then, you know, and then you develop this sort of weird divide between the continental philosophy and analytic philosophy. And then where does philosophy of science fit in? Philosophy of science is probably closer to analytic philosophy in a lot of ways. There's some dispute over exactly whether it's a part of analytic philosophy or not.
Starting point is 02:15:38 But like, a lot of the tool sets that one uses in philosophical physics do seem to come from the analytic tradition in philosophy. This is the part of philosophy associated with logic and metaphysics and philosophy of mind and to some degree, depending on how you phrase things, philosophy of science. So Hegel is sort of more associated with the continental tradition in philosophy, and there's just been, I think, less interaction between the continental tradition and physics. I think what a lot of people who maybe have had some exposure to philosophy, maybe not a lot, when they think about how useful philosophy is to physics, I think they're often thinking about the parts of philosophy
Starting point is 02:16:19 that are not super connected to math and physics. Sorry, how is fear and trembling going to have the implication about F equals MA? Right. But I think a lot of those people would say Bersh and Russell, well, of course, Bersh and Russell is a good thing to say about physics. He wrote a book on relativity and he's a mathematician, but he was an analytic philosopher. He was like one of the towering analytic philosophers, right? Quime and so, you, and the early people who developed quantum mechanics were like deeply enmeshed, you know, in Vick and Sen. I mean, there's a beautiful interview.
Starting point is 02:16:54 I would also recommend linking it. It's from the 1970s by Pete and Buckley, who were doing an interview with the CBC. It's an interview with Werner Heisenberg toward the end of his life. It's a fantastic interview. I mean, it's amazing to hear him talking and actually hear his voice and hear him describing the early days of quantum theory and all the people he met. And he spends a lot of time talking about philosophy. He talks about his friendship with Wittgenstein.
Starting point is 02:17:20 He talks about how confused he was by the Tractatus, you know, and he's not unique. I mean, he wrote a book called Physics and Philosophy. And the book is filled with Kantian metaphysics, and that's the book where he has this chapter. It's from 1958 where he introduces the Copenhagen interpretation where he like tries to formulate it. We'll talk a little bit about that. You know, and he's arguing with Schrodinger and Einstein, and they're all arguing over who's the proper, like who's more correctly representing Kantian philosophy.
Starting point is 02:17:49 And you had neo-Kantians like Greta Herman, we talked about Greta Herman, and all these people were talking with, they were all connected with, you know. So, you know, there was an incredible amount of cross-pollination between the analytic philosophers of the early 20th century and physicists. Physicists themselves were thoroughly trained in philosophy.
Starting point is 02:18:09 There's another paper you should link to. This is a paper by Don Howard. It's a paper in Physics Today from 2005. It's called Albert Einstein as a Philosopher of Science. And it's all about just how much philosophy Einstein was doing. He'd read Kant's Three Critiques by age 16. Wow. And...
Starting point is 02:18:32 That takes 16 years. I mean, he did what he did, right? He was super interested in philosophy. When he went to university, there were mandatory courses in philosophy of science, both at the university. And then after he left university, he ran a philosophy of science reading club. He was deeply immersed in Spinoza. He was very inspired by Ernst Mach. He even wrote an obituary for Ernst Mach in which he talks about the importance of epistemology. He says, the ablest students, the ones who are most independent of thought
Starting point is 02:19:09 are the ones who took epistemology the most seriously. Like this is 1916 when Mach died. And he was a huge fan of Schopenhauer also. And so I mean, and so was Schrodinger. I mean, they all, you know, Schrodinger's Schrodinger cat paper mean, they all, you know, Schrodinger's, Schrodinger's cat paper has sections with words like epistemology in them, like in a physics paper, right? You know, and Bohr was philosophic.
Starting point is 02:19:34 I mean, they were all like, so, and I find this kind of striking because there's this attitude today that like, who needs philosophy? But the people who gave us the biggest revolutions in modern physics, quantum theory and relativity, were all either deeply strongly connected to philosophers or they were interacting with philosophers or they were philosophers or they were at least very thoroughly trained in philosophy. If you were trying to create
Starting point is 02:20:01 new breakthroughs in physics, wouldn't you take that as an example? Now look, I understand that there are a lot of philosophers who are not trained in physics, and people who are not trained in physics sometimes say things that are not very helpful for physics, but the answer to this is very simple. We need people who are thoroughly trained in physics and thoroughly trained in philosophy so that they don't say nonsense things, so they actually make meaningful contributions and help bring these two disciplines together. Because I think that would fertilize the soil, so to speak.
Starting point is 02:20:32 I mean, so much of modern physics has its roots in ideas that were generated during that incredibly formative period in the early half of the 20th century, the first half of the 20th century. And we're facing a lot of very deep problems today. You know, Einstein, I think in a paper, I think it's mentioned in the Howard paper, in 1936, Einstein wrote a paper called Physics and Reality, which he talked about how we're living in a time in 1936 when there's so much we don't understand about nature and there's so many deep questions we have.
Starting point is 02:21:00 And this is exactly the time you need philosophy. You need to be steep in philosophy and think very philosophically about things, carefully and rigorously using all these tools that I called philosophical physics, you know, to avoid falling prey to slogans, to avoid falling prey to groupthink, to being able to have an independence of mind. One of the most famous things that Einstein wrote about philosophy is a letter he wrote to a philosopher of science named Robert Thornton in 1944. In which he said that when he meets many scientists of his time, he feels like he's
Starting point is 02:21:31 meeting someone who's seen many trees, but has never seen a forest. And that a thorough training in philosophy gives people the kind of independence of mind that distinguishes, you know, a mere artisan from a real pursuer of truth. I think that makes a lot of sense. And in my own experience, having taught courses here for a long time, the students who were most philosophically curious, many of whom took philosophy courses, upper level philosophy courses, often made the strongest physicists. They were very careful in how they formulated things.
Starting point is 02:22:08 They knew the difference between deductive argument and an inductive argument and one that was neither. So here's the thing that happens frequently. So on the one hand, if you've got rigorous, credible premises and you follow them in a rigorous, logical, math-a-weighted conclusion, so you've got a deductive argument, you've got a math proof. We like those. Science often doesn't take that form. Sometimes you prove theorems in science, but a lot of the time we're making inductive arguments. We start with credible premises, we call it the evidence, and then we use arguments that
Starting point is 02:22:38 are more or less rigorous. They can't be maybe perfectly rigorous, and we arrive at a conclusion that is, strictly speaking, stronger than the premises, something that is not necessarily entailed by the premises, but is strongly supported by the premises. We assign some evidentiary credence or probability. We say, I'm this certain that my conclusions are true, given the premises, which are very credible and rigorous and reliable and my reasoning.
Starting point is 02:23:01 That's an inductive argument. And in a lot of science, there's inductive arguments. And then what we do is we take the conclusions, and usually they're like a theory or prediction, and we go out and measure them, and we get confirmation, and we feel stronger that we've done a good job. But there are a lot of arguments in some areas of physics that are neither deductive or inductive,
Starting point is 02:23:17 where the premises are themselves wild speculations. And you take these wild speculations, and then you make arguments that are themselves wildly speculative, and you arrive at conclusions that are speculations. And you take these wild speculations and then you make arguments that are themselves widely speculative and you arrive at conclusions that are speculations like on top of speculations and speculations. And I just don't even know what to do with something like that. I don't know how to follow those arguments. And I really don't think that someone who's like thoroughly trained in philosophy is going to find those sorts of arguments very credible. And I think especially at a time when in certain areas of physics we are very limited in our
Starting point is 02:23:49 experimental data and we're trying very hard to be very careful in our reasoning, this is exactly the time when you want the kind of rigorous scrutinizing that you get from a training in philosophy. So again, this is like a second appeal. For anyone who wants to make a big impact on physics, I think in terms of cost-benefit ratio, you know, supporting people who do impact on physics, I think in terms of cost-benefit ratio, you know, supporting people who do this kind of work I think would be particularly important. Okay, so you said independence of thought is what philosophy trains you to have.
Starting point is 02:24:16 Also precision of thought. So Scott Aronson is someone that we brought up earlier, or that you brought up. And Will Hahn here, also you can't see him but he's behind the cameras professor at Florida Atlantic University helped put on this event called MindFest and Scott Aaronson was there and Scott Aaronson said okay well he didn't say this but the implication was that most physicists most scientists think of philosophers as just engaging in this ill-defined unfalsifiable nonsense that's incoherent. And he was saying when he was speaking, he never had to be so precise in his speech as he was around a philosopher. Yeah, philosophy seminars.
Starting point is 02:24:51 So there are many people maybe who are watching who've never been to a philosophy seminar before. Maybe many people watching haven't been to a physics seminar. That's okay. I mean, people come to this. I mean, you've got people who are brand new. Maybe they're students, maybe they're in secondary school, maybe earlier than secondary school, I don't know.
Starting point is 02:25:07 Or maybe they just got into different fields, or maybe they're not in academia, and that's all great. I mean, we're all contributing in some way to the world, hopefully. But there are many people who maybe have been to physics seminars and don't know what a philosophy seminar is like. And I'm going to tell you, when you go to a philosophy seminar, especially in philosophy of science or philosophy of physics or analytic philosophy, the level of precision in your language, I mean, you have to be...
Starting point is 02:25:29 So the way they usually work is, so I... Physics seminars usually work like this. There's a speaker who talks for 45 minutes, maybe an hour, depends on the length of the seminar. People often interrupt, like the middle of the seminar, they'll just...they make questions, they just sort of interrupt in the middle. And someone who's maybe not very practiced, who's giving the talk may get derailed,
Starting point is 02:25:49 and this can sometimes lead to problems, but hopefully everyone's respectful in the questions if there are any are kept brief. And then at the very end of the seminar, they all thank the speaker, they clap, they thank the speaker, and then they say, all right, we've got five minutes for questions, any questions?
Starting point is 02:26:02 And, you know, most people don't, I mean, they can't, I mean, there's just no time to really ask a substantive question. A lot of people feel very nervous because they're like, oh, maybe there's a more senior person here, a professor who wants to ask a question and I don't want to interfere. Or if there's only gonna be like time for one question,
Starting point is 02:26:16 I don't want to ask a question that's gonna be like a bad question. So people like often feel very nervous about asking questions and there isn't really a good substantive dialogue. In philosophy seminars, what often happens is, you have a talk, half hour, 45 minutes, sometimes they go an hour, then there's a break. People go and they take five minutes, they get refreshments, they come back, and then there's like an hour of discussion, right?
Starting point is 02:26:38 And the discussion is often the most interesting part of the seminar, right? And because there's like an hour, everybody asks questions, the students ask questions, because no one is afraid they're asking the one question. No one's afraid they're gonna look bad because there's gonna be 10 more questions after their question. And people can really have a substantive discussion and dialogue.
Starting point is 02:26:56 So that's great. And I actually really like the culture of these seminars because they're very welcoming. A lot of times they'll say that students get to go first because they really wanna prioritize students asking questions. But I will tell you, the expectation of the precision of your language is high, right? If you say something that is not very carefully stated,
Starting point is 02:27:15 people will immediately say, I'm sorry, that's too vague, and you like, precise-ify that. So I think there's this attitude, I think, among some, you know, some scientists, I wouldn't say there's a lot of scientists who are very familiar with this, but I think some who think that philosophers are just making stuff up and we're very, very vague and we're just sort of, but if you've been to a philosophy seminar, it's quite the opposite because you don't have the ability to rely on empirical data. You can't just say, well, I don't need to explain it, just look at the data.
Starting point is 02:27:37 You rely on the strength of your logical reasoning in a very significant way. And I think that could be brought to bear in how we do physics more than we currently do it. I don't know if you saw some of the lectures on Toh. I hope to bring some of that to it. So, like with Yang Hui, he was going on, and he's like, I like this because, Kurt, normally I have 45 minutes, but here I have two hours. And so you can ask me questions
Starting point is 02:28:00 and we can get to all of it plus questions. Well, I know you're sitting there waiting to catch me whenever I say something that's not sufficiently sharp and rigorous. And that's, it, so this reminds me a lot more of the philosophy seminars that I go to. And that's really nice. And look, there are many things I think that your program is doing, right? I mean, you're informing audiences of interesting ideas from all directions, you're inspiring, but I think you're also modeling a kind of dialogue that I think we need more of in academia, in science and philosophy
Starting point is 02:28:33 generally speaking. Holding people accountable, having extended discussion, really getting to the questions, really getting to the deep parts of people's ideas, not letting people get away with slogans. You know, and physics has a lot of slogans that people just, they hear someone very prominent say and then they just repeat it, right? I mean, like, really like taking this apart. And this is just not like a general public service announcement because I know there
Starting point is 02:29:01 are a lot of people who are watching who are not scientists yet or maybe ever, maybe this is just not the direction they want to pursue. And maybe this is just some advice, right? Obviously watching your podcast series is a great move, that's great. But you know, people will sometimes tell folks, well, you really can't contribute to science or philosophy or whatever until you've done the requisite training. You need to do an undergraduate program.
Starting point is 02:29:27 You need to read books. You need to take coursework. You need to get graded on them. You need to do exams. You need to actually learn all these techniques. You need to learn how to do this. In physics, it means learning Newtonian mechanics, learning electromagnetism, learning thermodynamics,
Starting point is 02:29:42 learning quantum mechanics, depending on what direction you go in. You may learn astronomy or biophysics or computational physics or high energy or whatever it is that you will learn. But like really do all of that. Do all the problem sets, learn everything, take the time. This is a years long process of rigorous training.
Starting point is 02:29:57 And if you wanna make contributions at the research level, you'll most likely have to do some kind of graduate work like a PhD program. And many people don't know that, by the way, that PhD programs, at least in the United States in the sciences, are funded. You don't pay to go to graduate school for a PhD. It's important to know that. When I was, like, learning about science,
Starting point is 02:30:13 I thought you had to pay to do a PhD program, and I thought that was important. But you actually get paid to be in a PhD program in the sciences. It's important for people to know. And a lot of people look at that, and they think it's instrumentable. They're like, but I have an idea. I have a great idea. I just want to contact a physicist and tell them my idea and have them work on it. And what you say is,
Starting point is 02:30:29 you really, really need to do the training first. Cause there's just so much you have to learn. It's like Picasso was this amazing artist, but he had to master traditional techniques before he could go and break them. And I know a lot of people will say, but if I learn all the techniques and I spent all the years learning all of this,
Starting point is 02:30:44 won't I just become like everybody else? Won't I im I learn all the techniques and I spend all the years learning all of this, won't I just become like everybody else? Won't I imbibe all the same conventional wisdom and all the slogans? That is a risk. So what I would tell people, if you want to embark on this journey, and it is an amazing journey, I mean, learning physics has been,
Starting point is 02:30:57 it's like, it's incredible. If you love physics and you spend years learning it, it's the most incredible thing you can imagine. You do have to work a little bit not to get absorbed into sort of calcified conventional wisdom. So while you're learning it, you just have to remind yourself every once in a while... Of your original ideas? Of your original ideas, sure. Sometimes you discover that the ideas will continue to work. Sometimes you discover that they don't work, that's fine.
Starting point is 02:31:23 But you also just, every time you learn to do a technique, you learn how to calculate something, you learn how to calculate the energy eigenvalues of a one-dimensional quantum mechanical system, or you learn how to calculate scattering amplitudes in a quantum field theory or whatever, you want to separate out the methodologies of learning, like how do I calculate something, how do I do something, how do I model something, from the ideology? Cause people will say, they'll say, well, you said you calculate it. And what this means is that what's going on in nature is, and that's the moment you wanna be like,
Starting point is 02:31:53 whoa, hang on a second, hang on a second. I follow the calculation, it's empiric, whatever, but you've now transcended this particular methodology and now you're making a substantive statement about metaphysics, about something that's out there. That requires some rigorous scrutiny. That's where you require a little bit of skepticism. And maintaining a foot in that sort of skeptical sphere as you go through, I think, is the best way to do it. But that's just what it is to be a good philosopher.
Starting point is 02:32:21 Like, a good philosopher will see statements, sometimes very provocative, sometimes very ambitious statements, maybe over ambitious statements from any quarter could be from a scientist and say, hang on a second, wait a second, not so fast, let's make sure that this extrapolation that you're making here is really rigorous and really makes sense. And I'll give you an example. So here's a concrete example. This is all very sort of abstract. Let me bring it down to earth.
Starting point is 02:32:54 This is a little bit of a sensitive topic, right? Okay. One of my favorite, like one of my idols in physics is David Griffiths. Many people in physics have read David Griffiths' books. David Griffiths is legendary. And I think the world of him. I learned physics from his books.
Starting point is 02:33:14 I learned particle physics the first time from his book, introduction to elementary particles, quantum mechanics learned from his quantum mechanics book, electromagnetism I learned from his electromagnetism book. He has rightly earned a status of this sort of legendary figure in physics. He's had a bigger impact on physics than almost anybody. Right. And I like his writing for the most part,
Starting point is 02:33:32 but he does have a kind of tone sometimes when he writes that's very dismissive. He'll sometimes just dismiss things. And because he's so like actually kind of honest, he'll often have a footnote where he'll say, I'm being too strong, I shouldn't dismiss this. Really, it's like this. But a lot of people don't read the footnotes
Starting point is 02:33:53 or they get confused about them. And I'll give you a very concrete example. In his quantum mechanics book, he says in the beginning, and so many students have read this, he says there are three ways to think about quantum mechanics. There's the realest way to think about quantum mechanics, which is just to say that before we do a measurement, the thing we're measuring, it just exists. Now we've already talked about how that's really not, that's like a, it's not really
Starting point is 02:34:15 a nuanced enough view. There's the realist view. The thing we're about to measure was already there. The second is the orthodox view, which is the thing we're measuring wasn't there. There was no pre-existing property. The thing we were measuring didn't exist before we measured it. Particles are nowhere until we measure them. And then the third possibility is the agnostic position.
Starting point is 02:34:38 I'm not going to try to answer. He says these are the three positions. And this really like steamrolls a lot of nuance in this discussion. And then he says, for a while, they were partisans of all three of these views. And then not long ago, but that means 1964, which is actually a long time ago, a guy named John Bell came along and proved a theorem and the theorem eliminated the agnostic position as being possible and turned it into an experimental question whether the realist position was true
Starting point is 02:35:07 or the orthodox position. Experiments have now confirmed that the orthodox position is correct. And that's it. He just says, that's it. And then you like read the footnote. In the footnote, he's like, well, that's too strong a statement.
Starting point is 02:35:20 There are actually other theories that, you know, but the words he uses is they tend to be cumbersome and implausible, but never mind. That particular phrasing is kind of funny because I worked on a project a couple of years ago on whether magnetic forces could do work on particles. It turns out they can if particles have intrinsic magnetic dipole moments. And I, and Griffiths updated the fifth edition of his book on electromagnetism and included a footnote mentioning this paper.
Starting point is 02:35:53 So I have a footnote. But he says theories like the thing I wrote down, he says they tend to be cumbersome and implausible but nevermind. He uses exactly the same language for these things as he does for all these other persons of quantum mechanics. And given that these other formulations of quantum mechanics, I think, are good, and people should work on them, they do tell us something, I think, now I feel like I'm a good company, right?
Starting point is 02:36:19 We'll come back to some of that magnetic dipole stuff maybe a little bit later. Now what's strange about this is that at the end of Griffith's book, he has a beautiful afterword. It's the final chapter, it's a chapter 12, where he goes through Bell's theorem in detail, which is not a thing you commonly find in introductory quantum mechanics books. And he has a lovingly good treatment of Bell's 1964 theorem. It's the earliest version of Bell's theorem. He does say a couple of things
Starting point is 02:36:45 that are a little bit dodgy there, but his treatment is actually really very good. And he does make mention to some of these other approaches, but it's like at the end of the book, a lot of students don't see that part of the book. And I just worry that students reading this book will take the things he says in the main text, not the footnotes, not the qualifications, not the other stuff that happened later, and they'll just repeat them. They'll just say, oh, I was wrong, realism is wrong, David Griffiths has said that the orthodox approach is the only approach and there's no point in pursuing this further. And any other attempts to pursue anything else are just pursuing theories
Starting point is 02:37:16 that are cumbersome and implausible, but never mind. That's the kind of thing that someone who's new in physics needs to be on the look at for. You see statements like that that are really now metaphysical statements, and you need to be like, well, hang on a second. That doesn't quite follow from the methodologies that we're doing. And I think it behooves someone writing a textbook, someone teaching physics, to be as clear and careful as they can be about when they've stopped presenting something that's calculational, methodological, model development, and they've now moved into
Starting point is 02:37:48 this is the way nature is as a result. We've learned that there is no fact of the matter about anything we're measuring, that particles don't have anything before they're measured, that there's no way to fix quantum mechanics, that these are statements that are not supported by what we have, and I think people who are interested in doing a serious study in physics should know at the beginning to be on the lookout for those kinds of statements. I think that would be the piece of advice I would share. Jacob, it's been a pleasure. Three hours and we're not even halfway through.
Starting point is 02:38:21 Yes, Kurt, it turns out when you want to reformulate foundational theory in physics, it takes time. It doesn't happen all at once. Well it takes chunks of time. Chunks of time and it's indivisible, but it looks like we have a good division event coming up. Okay, great. Okay, so we're going to take a division event now, which means that you'll get part two of this conversation, which is the third time that I'm speaking to Jacob in total.
Starting point is 02:38:43 The first time I've spoken to Jacob is on screen. The second time is right here. The third part will come out in a couple weeks from now. And what we'll talk about are the Bell experiments or the Bell inequalities. We're going to get to other questions people had. People had questions about entanglements. People had questions about causation in this approach. And there were also questions about what relationship this approach has to problems in statistical
Starting point is 02:39:08 mechanics and to some of the other interpretations and formulations of quantum mechanics. Right. Also wave-particle duality. What does that mean in this approach and also just traditionally? Right. Okay. See you next time. Yeah.
Starting point is 02:39:23 Definitely subscribe and ensure that you watch part two as we talk about what are the misconceptions of the wave-particle duality. Also, what are challenges of applying indivisible stochastic processes to quantum field theory? Is gravity indeed quantum? What about stochastic general relativity? What about the misinterpretations of nonlocality and Bell's theorem? Jacob also gives a new perspective on entanglement without wave function collapse and talks about the difficulty in defining causation at a fundamental level. We also talk about the philosophy of probability and what the origin of probability
Starting point is 02:39:54 is in statistical mechanics. And of course, Jacob has his critiques of the many worlds interpretation and then goes over open questions and future research in indivisible stochastic processes. You do not want to miss this. It's a banger episode. Subscribe to get notified. New update! Started a sub stack. Writings on there are currently about language and ill-defined concepts as well as some other
Starting point is 02:40:17 mathematical details. Much more being written there. This is content that isn't anywhere else. It's not on theories of everything. It's not on Patreon. Also, full transcripts will be placed there at some point in the future. Several people ask me, hey Kurt, you've spoken to so many people in the fields of theoretical physics, philosophy and consciousness. What are your thoughts? While I remain impartial in interviews, this substack is a way to peer into my present deliberations on these topics.
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