Daniel and Kelly’s Extraordinary Universe - Can we put black holes to work for us?

Episode Date: March 10, 2022

Daniel and Jorge discuss how the twisted spacetime around a spinning black hole can be used to pull energy from a black hole. Learn more about your ad-choices at https://www.iheartpodcastnetwork.comS...ee omnystudio.com/listener for privacy information.

Transcript
Discussion (0)
Starting point is 00:00:00 This is an I-Heart podcast. December 29th, 1975, LaGuardia Airport. The holiday rush, parents hauling luggage, kids gripping their new Christmas toys. Then, everything changed. There's been a bombing at the TWA terminal. Just a chaotic, chaotic scene. In its wake, a new kind of enemy emerged, terrorism. Listen to the new season of Law and Order Criminal Justice System
Starting point is 00:00:33 On the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. My boyfriend's professor is way too friendly, and now I'm seriously suspicious. Wait a minute, Sam. Maybe her boyfriend's just looking for extra credit. Well, Dakota, luckily, it's back to school week on the OK Storytime podcast, so we'll find out soon. This person writes, my boyfriend's been hanging out with his young professor a lot. He doesn't think it's a problem, but I don't trust her. Now he's insisting we get to know each other, but I just want or gone.
Starting point is 00:01:01 Hold up. Isn't that against school policy? That seems inappropriate. Maybe find out how it ends by listening to the OK Storytime podcast on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. Every case that is a cold case that has DNA. Right now in a backlog will be identified in our lifetime. On the new podcast, America's Crime Lab, every case has a story to tell. And the DNA holds the truth. He never thought he was going to get caught. And I just looked at my computer screen.
Starting point is 00:01:31 I was just like, ah, got you. This technology's already solving so many cases. Listen to America's Crime Lab on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. Hi, it's Honey German, and I'm back with season two of my podcast. Grasias, come again. We got you when it comes to the latest in music and entertainment with interviews with some of your favorite Latin artists and celebrities. You didn't have to audition? No, I didn't audition.
Starting point is 00:01:56 I haven't auditioned in like over 25 years. Oh, wow. That's a real G-talk right there. Oh, yeah. We'll talk about all that's viral and trending with a little bit of cheesement and a whole lot of laughs. And of course, the great bevras you've come to expect. Listen to the new season of Dacus Come Again
Starting point is 00:02:13 on the IHeartRadio app, Apple Podcast, or wherever you get your podcast. Hey, Daniel, when is all this physics research going to pay off? Pay off? What do you mean? Did you invest in some exoplanet startup? Kind of like with my taxes, right? Isn't all of physics research funded by the public? I guess that's true, but isn't the sheer pleasure of learning about the universe enough for you? Like, you want some cash out also? It's not enough for my bank account, that's for sure. But, you know, I'd be nice to get at least some nice inventions out of it.
Starting point is 00:02:53 You know, I think everyone is still waiting for the teleporting machine or the backer. Or the warp drive? Hmm, well, I might be able to offer you a pasta maker. Is it a warp pasta maker? No, but it's a black hole-powered spaghettiification machine. Oh, what? What's the plan? Are we going to open an Italian restaurant next to a black hole?
Starting point is 00:03:11 Yeah, exactly. Fresh black hole pasta delivered in a thousand years. You're getting no tip for me if it takes a thousand years to get my dinner. Darker than a squid ink. Is it fusion fusili or Inguinea la physicist? It must be orzos because their length contracted. Orzo's the little grain ones. Hi, I'm Horham, a cartoonist, and the creator of PhD comics.
Starting point is 00:03:45 Hi, I'm Daniel. I'm a particle physicist and a professor at UC Irvine, and I do make homemade pasta. Oh, you do. Do you make each noodle individually, or do you have one of those, like, machines? Oh, I sculpt them by hand. Each one is a work of art. I give them a name. I mint an NFT for each one. I see. And then everyone just gets one piece of pasta for dinner.
Starting point is 00:04:07 One big pasta. Exactly. Pastone, they call it. One giant two. You just set it down in the middle of the dinner table. Say, here, eat this. That's right. Exactly.
Starting point is 00:04:17 Technically, it's pasta. No, we use a pasta machine and so we slice it up into spaghetti or linguine or one of the other inis. Yeah, we have one of those in our house and we've used it a few times but it's a lot of work it absolutely is a lot of work but there's also something fun about it you get your kitchen all flowery and your pants all covering flour and at the end you get something which tastes a little bit better than something you could buy in the store a little bit better i guess might be worth it then but welcome to our podcast daniel and horhe explained the universe a production of iHeart radio in which we turn your brain into spaghetti by exploring all of the mysteries
Starting point is 00:04:49 of the universe everything that's out there that makes sense to us and everything that's out there that doesn't yet make sense. We talk about the tiniest little particles buzzing around in your toenail all the way up to super massive black holes anchoring enormous galaxies billions of years away. We don't shy away from the biggest, deepest, darkest,
Starting point is 00:05:08 most bonkers question because we want to introduce you to the craziness that is this universe. That's right. We take all of that amazing research that physicists and scientists are doing at the edge of human knowledge. We take that and we boil it for a really long time until it's soft and soggy.
Starting point is 00:05:24 enough for people to consume. No, no, no. We stop at just the right moment so we can serve up the information Aldente. We like it with a little bit of crunch. Do your kids like it with a little bit of crunch? Mine like it super soggy.
Starting point is 00:05:35 Yeah, I know mine like it overcooked. They even call it overcooked. They're like, make sure to make it overcooked. Make sure you overcook it and then we sprinkle it with a little bit of olive oil, right? And dad jokes. Exactly.
Starting point is 00:05:45 Do you like your pasta with bananas? Well, that's how we're serving it today. Oh, man. We just invented a new recipe, Banana Marinara. That's just fun to say A and B, intriguingly tasty perhaps. Maybe, I don't know, maybe more controversial than pineapple on pizza as banana on pasta. It's a slippery slope once you start putting fruit into Italian food.
Starting point is 00:06:08 Especially if the banana peels are all over the floor, then it's definitely a slippery slope. Yeah. So we like to talk about science and all of the amazing things that people are out there discovering and all of the big mysteries, all the things we don't know about the universe, everything that physicists are in their offices and labs thinking about and pondering about that maybe one day will be something that everybody knows. That's right. And there's a variety of motivations for digging into the mysteries of the universe. Some of us just want to know are driven by an insatiable curiosity to understand the universe.
Starting point is 00:06:39 See it as a giant puzzle, a mystery posed for humanity that we need to unravel no matter how many millennia it takes to gain that understanding of the universe. But others, the more practical-minded folks among us, might be interested in figuring out how the universe works to better our lives, to figure out how to put it to work for us, to take advantage of that knowledge, to deliver inventions to humanity. Yeah, because that's what the universe is therefore, right? It's there for us. It's the whole reason it's there is just to make our life easier and more exciting. I suppose, maybe. I mean, it could be there for the aliens, right? Maybe we're just part of the aliens universe. Wait, what? We're there for the aliens? Hopefully not for
Starting point is 00:07:20 dinner. Maybe. Maybe we're just here to be a plot twist in some drama that's been going on for thousands of years over on Proxima Centauri, you know? Oh, I see. We're just like an adjacent to an event or Avengers movie or something. Exactly. You thought you were going to be part of the main cast.
Starting point is 00:07:36 Turns out you only got a few lines. You won't get your own Marvel movie for another trillion years, perhaps. They'll eventually make a Marvel movie out of every single person in the Marvel universe, right? It'll be the ultimate crossover, you know? It would just be called not the Marvel universe, just the universe. Just the universe. Well, regardless of why the universe exists, a question we may never know the answer to.
Starting point is 00:07:59 It is interesting to think about how we can put the universe to work for us. Because sometimes the knowledge that physics extracts does have practical value. Yeah, I mean, we have nuclear fission, right? Powering most of Europe, I think, in a lot of the United States and around the world. That was all physics, right? That was all physics. The good and the bad. We also have nuclear weapons pointed at civilian populations and used for political ends.
Starting point is 00:08:23 But, you know, there's two sides to every corner. Yeah, that's right. It's all your fault also. But even our everyday sort of inventions that we use every day, you know, our cell phones have, you know, there's physics stuff in it that we learn. Maybe not the cutting edge stuff now, but the stuff that was cutting edge a long time ago, you know, all those tiny little circuits and how they work down at the atomic level, we needed physics to understand how to make those things.
Starting point is 00:08:46 That's right. Essentially, the nature of your life. today, the way you live your day is the way it is because we understood quantum mechanics that led to revolutions in computing and therefore electronics and your life. And so it's true that basic research digging into the nature of space and time and forces eventually gives us the power to change our lives. You know, it's a song I've sung many times on this podcast. I don't understand why politicians don't just invest more in basic research because it pays itself back a hundredfold. Every dollar you spend today gives your children and your grandchildren
Starting point is 00:09:21 improve quality of life. I don't get it. Why don't invest in that more? Actually, that's kind of an interesting philosophical question. Like, do you think we could have invented the cell phone without knowing physics, right? Like, could we just have been tinkered and then done engineering just to get it to work and eventually got on the cell phone without understanding quantum mechanics or fusion? Absolutely. I think from a philosophical point of view, it is possible to make technological advancements without understanding what you're doing we have sort of like the invention of modern science at least in the western world only like 500 years ago this question of like trying to develop models that explain what we're seeing but we definitely had technological advancement well
Starting point is 00:10:00 before then people have been forging very impressive like samurai swords for thousands of years without understanding like what's going on with the metallurgy they were doing why are you dipping the sword in water now and then you dip it in this other thing and you wait this number of of seconds. You can sort of random walk your way into technology without understanding what's going on. Could you get all the way to the cell phone? You know, you give yourself off another thousand years or million years? Yeah, maybe. Wait, so are you saying that we don't need physics then? I think that's what you just concluded. I think technically you don't need physics, but definitely it helps. It supercharges your technological advancements because you understand what's going on, then you can come up with new
Starting point is 00:10:38 ideas for how to use them. You're like a little sprinkle of parsley at the top of the pasta. Is that what physics has been reduced to in this episode? No, I'd say you're the reason you're getting your pasta in five minutes instead of in a million years. Oh, I see, I see, I see. You're the reason it's not stale and stiff and dry it out. We're getting hot fresh pasta because of physicists. That's right. I'll take credit for that.
Starting point is 00:11:00 Hot fresh cell phones. Slurp it up. Would you like a little parsley on your cell phone? Have it some bananas. Well, at least you can look at pictures of bananas and parsley in your cell phone now instead of in a thousand years. So that's something. That's something, yeah. Exactly. I'll put that on my CV.
Starting point is 00:11:16 You can swipe left on a banana and do all kinds of things. But yeah, it is a pretty amazing universe. And sometimes we wonder if we can put more of it to work for us, especially the things out there that are amazing and seemingly super amazingly incredibly powerful. Exactly. Because we are struggling constantly as a species to extract enough energy for our survival. Yet at the same time, we are surrounded by intensely powerful astrophysical objects. The sun, of course, is a great example.
Starting point is 00:11:44 We capture a tiny little bit of its energy. And they're even more powerful, incredibly vast things out there that are like huge engines pumping out energy. Could we take advantage of some of these incredible astrophysical machines to gather some energy we need, you know, to charge our cell phones? So today on the podcast, we'll be asking the question. Can we put black holes to work for us? Whoa.
Starting point is 00:12:14 Daniel, I feel like this is going to that idea of putting an Italian restaurant next to a black hole. And maybe having the black hole wash the dishes for us. Is that what you mean? Yeah, I'm just wondering when the black holes are going to unionize, you know, when they're going to rise up against us, their oppressors, and be like, hey, these conditions are terrible. I'm stuck out here in the middle of nowhere, and we're just eating gas and dust all day.
Starting point is 00:12:33 Interesting. Then they're going to change their name to red holes. You know, in solidarity of communism. that's right black holes of the universe unite you have nothing to lose but your event horizons that is their ultimate plan isn't it all black holes they just want to unite and get and basically create one giant union or one giant black hole one socialist black hole exactly that's the future of the universe this is a question about tapping into the power of these crazy objects I mean the amount of light radiated from black holes the amount of gravitational energy stored in
Starting point is 00:13:09 black holes. We are like sitting on the edge of an incredible river of energy and we're just really bad at tapping into it. We're like burning coal that we dig up from underground to get tiny little slivers of energy out. It's ridiculous. Yeah, there's a lot of amazing things happening in the universe. But you know, I would think that black holes would be sort of like the last place you go to to get energy or to get anything useful out of it because, you know, they're kind of in the name. They're holes. It's like, why would you go to a hole to get something out of it? Maybe we could throw our trash into the black hole so we wouldn't have to think about it. But it's kind of weird, right?
Starting point is 00:13:45 Because black holes suck everything in. And once it gets sucked in, you can't get out. So it's kind of weird to think that you could use them for anything useful. That's true. But they are also really vast stores of energy. I mean, the reason that they are black holes is because they have so much mass in them. And that mass reflects internal store and energy. So you could think of a black hole like a giant cosmic battery.
Starting point is 00:14:07 So much energy has been poured into it. It's just sitting there, compressed and dense and bubbling up. So it's tempting to think, like, can we tap into that a tiny little bit? But it's weird because we know nothing can ever get out of a black hole. That's true. We can't take anything out of a black hole. But remember, the black holes have influence far beyond their event horizon. If you are anywhere near a black hole, it will tug on you the same way the sun does.
Starting point is 00:14:30 And so the mass of the black hole, even though it's contained within the event horizon, can influence things outside the event horizon. and you can use that gravity to maybe charge your cell phone. I see. You just want to mooch off of their influence, all of their hard-earn, you know, connections and information. That's right. You go to the Black Hole's Instagram page and you leave a comment
Starting point is 00:14:51 and maybe you'll get a few followers. That's the plan. I see. There you go. First to pose. But yeah, and this has something to do with the concept called the Ergosphere, which is sort of a weird, weird thing, right? Yeah, people are used to thinking about Black Hole's as just having an event
Starting point is 00:15:07 horizon. But black holes turn out to be much more complicated than that. They have various regions within and outside of the event horizon that might let you tap into it to use its energy. And so that's a central part of this concept invented by Roger Penrose to tap into the energy of a black hole. Through its ergosphere, right? So that's kind of a strange word. So as usual, we were wondering how many people out there had heard of this concept of the ergosphere or know that it's related to black holes. So Daniel went out there into the internet to ask people the question, what do you think is an ergosphere? And thanks very much to our volunteers. If you'd like to participate, please just email me. It's very easy. You can record your
Starting point is 00:15:47 answers at home in the leisure of your bathrobe or whatever you like. Please just email us to questions at danielandhorpe. Right, but you don't have to wear a bathrobe to answer to you. Or is that a weird little request just from you? You don't have to wear anything. You don't have to tell me what you're wearing. It's totally up to you. No dress code for these questions. Well, I feel like the more we talk about this, the creepier it gets. Yes, agree. Anyways, here's what people have to say. People had some pretty interesting answers.
Starting point is 00:16:15 Ergo, the following. Well, that makes me think of two things. The exosphere, which is the sort of furthest limitations, I think, of our planet. The exosphere is like the furthest layer out maybe before the magnetosphere. You think of like Atmo, Troposphere. So maybe Ergosphere has something to do with that. layering system of different tiered spheres around the earth but it also makes me think of ergonomics so maybe it has something to do with the most ergonomic the
Starting point is 00:16:50 most efficient way to have a spear or some sort of three-dimensional object I happen to know that ergo means work and sphere is around object if I had to guess I would say it's some kind of moving or working round object or surrounds something that's round, that's moving. That's the best guess I got, though. Well, Ergosphere obviously makes me think of the term atmosphere, but it's nothing I ever heard in relation to Earth. So I would think maybe it has to do with the atmosphere of other planets, maybe even the atmosphere around stars. Well, it sounds like ergonomics, but I'm guessing it doesn't have anything to do with that. So maybe some sort of atmosphere. All right. People had some pretty good answers here. I mean, people sort of
Starting point is 00:17:46 related it to ergonomics, which is maybe sort of related, right? Because as someone, as someone pointed out, the word ergo means work. Yeah, I like that when people have no idea what I'm talking about, they try to break down the linguistics and understand the origins of the word, because that assumes that somebody out there in the astronomy community has made a sensible choice of names for this thing. Ha, ha, ha, the fools. Little did they know, you just pick names out of a hat. That's right.
Starting point is 00:18:11 It is a bit of a leap of faith, so I appreciate that. Thank you. That's a vote of confidence right there for astronomical naming. But sort of, is that true? Does ergo really mean work? Like, that's where ergonomics come from? I just kind of got my mind blown a little bit. Yeah, ergonomics is like, how do you sit comfortably while you do work.
Starting point is 00:18:28 I see. It's not the economics of work. I know it's the nomics of the ergo. But yeah, so it has something to do with black holes and also work, which is kind of what we're talking about, right? Getting black holes to work for us. Exactly. So the ergosphere plays an important role in trying to extract work from a black hole
Starting point is 00:18:49 to get it to give you energy. Yeah, and also to do it in a comfortable posture so that it doesn't get lower back pain. All right, well, Daniel, maybe let's start at the beginning here and maybe step us through what? exactly is a black hole for thus of us who had not heard about it before or heard our podcast. So black hole is the most dramatic feature of Einstein's general relativity. This concept that gravity is not just a force, it's not just the way two things tug at each other, but it's not really a force. It just comes out of the fact that space itself is curved. So when you have a really
Starting point is 00:19:23 massive object, it curves space time, meaning that it changes the relationship between points and makes some of them closer and some of them further. So that light, for example, appears to travel in a curve. It's very naturally moving through curved space. So matter bends space. It tells space how to curve. And then space tells matter how to move. And if you have enough matter somewhere,
Starting point is 00:19:48 if you have enough density of stuff in a small enough area, then you curve space so much that it's distorted that every path now leads towards the center. And that's what a black hole is. It's a region of space where every path now leads towards the center of the black hole, making it impossible to exit. Some people think it's because gravity is so strong. It's like tugging on those photons and making it impossible for them to leave. That's sort of a Newtonian view of a black hole.
Starting point is 00:20:15 A better way to think about it is that space is so distorted that every future you have ends in the singularity. Every path you could take always ends at the center of the black hole if you're inside the event horizon. Right, because like even the Earth does that, right? Like the Earth technically sort of bent space time around it so that it, to us, you know, it kind of down is the only way to go, right? I mean, the gravity we feel now sitting here, like the reason I'm sitting in my ergonomic chair is that space time around me is bent in such a way that it makes my body go towards the center of the Earth.
Starting point is 00:20:48 Yeah, precisely. Every mass bin space, not just black holes, not just the sun, not just the Earth, but you and a banana you ate this morning also bends space. It's just that the amount of bending depends on the amount of mass. And so the more mass you have in a small amount of space, the more bending you get. Right.
Starting point is 00:21:06 And so a black hole is sort of like the earth, but just super duper dense, right? Like a lot more denser and a lot more massive. Yeah. And you can make a black hole out of almost any mass. If you took the earth, for example, and compactified it down to the size of a peanut, all that same matter,
Starting point is 00:21:22 everything that's in and on the earth. squeeze down to less than a centimeter, you would get a black hole. And it would have the same gravitational strength as the Earth does now, but you could get much closer to most of that mass. So if you got really close to that peanut, it would have a very, very strong pull on you. Right. In fact, it's kind of mind-blowing to think about it.
Starting point is 00:21:41 Like, if you took the Earth and you, like, only left like a mile of Earth at the surface, right? Like if you hollered it out, kind of like an egg shell, and you took everything that was in the middle, the yolk, and you squeezed it down to the size of a peanut, then like we wouldn't tell the difference, right? Like life would just go on exactly the same way. You know, like at the center of the return to a black hole and we wouldn't maybe feel it. Well, you wouldn't feel it gravitationally, that's for sure.
Starting point is 00:22:07 You would have the same gravitational force on yourself. That's true. Of course, it would change, you know, tectonics and lava flow and all sorts of other stuff. And I don't think that a shell of the earth that's a mile thick could hold itself up. But from a gravitational point of view, absolutely, you'd feel the same force. because for gravity, you can always replace an object with a point particle at its center of mass with that same mass and you'll feel the same gravity. You're not sensitive to the details of how the object is put together.
Starting point is 00:22:34 Right. And in fact, it would still kind of keep on spinning, right? Because black holes can spin. That's right. Black holes can spin. And if you make a black hole out of something that is spinning, then that black hole has to spin because spin is something that's conserved in this universe. something that's spinning can't stop spinning
Starting point is 00:22:51 unless you have some external torque on it. So in an isolated system, like a star out in space, if it's spinning and then collapses into a black hole, that black hole has to have the same amount of spin as the original star. One thing that's interesting about black holes is that, you know, like if you made a black hole out of the earth, you would sort of know what was inside of that black hole, right?
Starting point is 00:23:10 It would be the earth, just really squished together. But maybe not, right? Like maybe when things get squished down that much, things maybe change. And we have no idea what's going on when you squeeze it that small. We definitely have no idea what's going on inside the black hole. Like general relativity tells us, you don't have matter in the same way that we do, that it's all squeezed down into a singularity, a point of zero volume, but non-zero mass. And that's the sort of classical picture. That's what Einstein's prediction tells us. But we also know that that's wrong. That can't possibly be what
Starting point is 00:23:42 actually inside a black hole for a couple of reasons. One is that there's an infinity. There's an infinite density. So it's not as much a prediction of general relativity as a breakdown of general relativity. Like, this is where general relativity doesn't work anymore. And the other is that we know it violates quantum mechanics. You can't have a point of zero size and know exactly where it is and have it have zero velocity. It's just too much information. That amount of information doesn't exist in the universe. So we don't know what's going on with the matter that's inside a black hole, but we know it's definitely not a singularity. It's probably some other crazy frothing quantum stuff. And the closest analog we have are neutron stars, which are very, very dense remnants from stars that are not dense enough to become a black hole, but close.
Starting point is 00:24:28 And inside the heart of a neutron star, there are crazy things going on with very high temperatures and pressures and weird forms of matter that we've never seen before. All new kinds of pasta inside. Maybe it turns into kuskos, right? Like a little tiny ball, a fuzzy infinite singularity. Cosmic kuscus. That sounds like a nice name for a dish. All right, well, Black holes also have something pretty interesting called an ergosphere that may be able to do work for us and solve all of our energy needs. So let's get into what an ergosphere is.
Starting point is 00:24:56 But first, let's take a quick break. December 29th, 1975, LaGuardia Airport. The holiday rush, parents hauling luggage, kids gripping their new Christmas toy. Then, at 6.33 p.m., everything changed. There's been a bombing at the TWA terminal. Apparently, the explosion actually impelled metal glass. The injured were being loaded into ambulances. Just a chaotic, chaotic scene.
Starting point is 00:25:36 In its wake, a new kind of enemy emerged, and it was here to stay. Terrorism. Law and order, criminal justice system is. is back. In season two, we're turning our focus to a threat that hides in plain sight. That's harder to predict and even harder to stop. Listen to the new season of Law and Order Criminal Justice System on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. My boyfriend's professor is way too friendly, and now I'm seriously suspicious. Wait a minute, Sam. Maybe her boyfriend's just looking for extra credit. Well, Dakota, it's
Starting point is 00:26:16 Back to School Week on the OK Storytime podcast, so we'll find out soon. This person writes, my boyfriend has been hanging out with his young professor a lot. He doesn't think it's a problem, but I don't trust her. Now, he's insisting we get to know each other, but I just want her gone. Now, hold up. Isn't that against school policy? That sounds totally inappropriate. Well, according to this person, this is her boyfriend's former professor, and they're the same age.
Starting point is 00:26:38 And it's even more likely that they're cheating. He insists there's nothing between them. I mean, do you believe him? Well, he's certainly trying to get this person to believe him because he now wants. wants them both to meet. So, do we find out if this person's boyfriend really cheated with his professor or not? To hear the explosive finale, listen to the OK Storytime podcast on the Iheart Radio app, Apple Podcasts, or wherever you get your podcast. A foot washed up a shoe with some bones in it.
Starting point is 00:27:01 They had no idea who it was. Most everything was burned up pretty good from the fire that not a whole lot was salvageable. These are the coldest of cold cases, but everything is about to change. Every case that is a cold case that has DNA right now in a backlog will be identified in our lifetime. A small lab in Texas is cracking the code on DNA. Using new scientific tools, they're finding clues in evidence so tiny you might just miss it.
Starting point is 00:27:30 He never thought he was going to get caught. And I just looked at my computer screen. I was just like, ah, gotcha. On America's Crime Lab, we'll learn about victims and survivors, and you'll meet the team behind the scenes at Othrum. the Houston lab that takes on the most hopeless cases to finally solve the unsolvable. Listen to America's Crime Lab on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. I'm Dr. Scott Barry Kaufman, host of the Psychology Podcast.
Starting point is 00:28:02 Here's a clip from an upcoming conversation about exploring human potential. I was going to schools to try to teach kids these skills, and I get eye rolling from teachers or I get students who would be a little. like, it's easier to punch someone in the face. When you think about emotion regulation, like, you're not going to choose an adaptive strategy, which is more effortful to use, unless you think there's a good outcome as a result
Starting point is 00:28:25 of it, if it's going to be beneficial to you. Because it's easy to say, like, go you, go blank yourself, right? It's easy. It's easy to just drink the extra beer. It's easy to ignore, to suppress, seeing a colleague who's bothering you and just, like, walk the other way. Avoidance is easier. Ignoring is easier. Denials is easier.
Starting point is 00:28:41 drinking is easier yelling screaming is easy complex problem solving meditating you know takes effort listen to the psychology podcast on the iHeart radio app apple podcasts or wherever you get your podcasts all right we're talking about black holes and their ergosphere that's apparently a feature of holes that we may be able to tap into for energy. I guess the idea would be to go to a black hole, Daniel, and set up like an ergosphere energy sucking station next to them. Yeah, precisely. And ergospheres are really cool because they're a feature of a more complicated black hole.
Starting point is 00:29:30 Like, typical black hole you imagine is what you just described, take the earth, compactify it down to a peanut, you get a black hole. But most actual black holes out there in the universe have more than just mass. they also have spin, like we talked about. And the reason is that basically everything out there in the universe that could make a black hole is spinning. It's very rare to find something out there in the universe that's not spinning in some way. The sun is spinning. The earth is spinning.
Starting point is 00:29:54 The solar system is spinning. The galaxy is spinning. Everything is spinning. So if you're going to make a black hole, then it's going to end up spinning. And spinning black holes are more complicated than your normal like vanilla short side black hole. And they have more than just an event horizon. They have several regions both with. within and outside the event horizon with really fascinating different effects on the space time.
Starting point is 00:30:17 Whoa. And I guess, you know, it's kind of weird to think of a hole spinning, right? Like a hole is the lack of something, you know? It's like if I dig a hole on the ground, that hole is not, it's weird to think that the hole will spin. It is weird to think about that. And there's sort of two things to grapple with there. One is what's spinning on the inside of the hole and the other is what's spinning on the outside. On the inside, it's hard to think about things spinning because we imagine a singularity at the heart of the black hole, at least in classical general relativity.
Starting point is 00:30:48 And a singularity has no size, a zero volume. So it's sort of like when we talk about a quantum particle, an electron, that has spin, but we don't say it physically spins. It can't spin because there's no extent to it. It doesn't change by spinning. So black holes that spin don't have singularities in them. They have something else. they have a ring inside. It's like a ringularity instead of a singularity.
Starting point is 00:31:14 That's a nice pun. But I guess maybe one way to picture it is that if you like imagine a black hole forming, right? It's not every, the stuff that makes, that goes into the black hole is not going to go straight in and compact itself. It's usually like stuff that's swirling. And because of gravity, it's swirling towards the middle. And then at some point it gets squished so much that it enters the event horizon. But maybe like the idea is that maybe as it goes in, it preserves some of that spin so that. maybe inside of the black hole, things are still spinning.
Starting point is 00:31:41 Like the center, maybe we don't know what's going on, but the stuff right outside the center, up until the event horizon, maybe that stuff is still going around in circles. Definitely it is. And we see that, right? That's what the accretion disk is. It's stuff that has so much spin that it hasn't yet fallen into the black hole. Like you might wonder, how does anything avoid falling into a black hole?
Starting point is 00:32:01 Well, the same way that the Earth avoids falling into the sun because we are spinning around that we have orbital velocity. And we can't just, like, lose that. can't just go away. Earth can't just stop spinning around the sun and fall into the sun. In the same way, the stuff that's on deck to go into the black hole but is spinning around it, you can't just like give up that spin and fall in. The way things fall into the black holes that they bump into each other and that slows them down or knocks one of them into the black hole knocks one of them out. So you're right. Things that are about to go into a black hole mostly spin around
Starting point is 00:32:34 it and then fall in. And if you think about it, if you're just like a random particle, headed towards a black hole, unless you're headed exactly at the center of it, then you have some spin relative to the center of the black hole. Imagine just a spinning disk, for example. If you're a particle and you hit a spinning disc, unless you hit it at the very center, then you're going to make that disc spin faster or slower. Right. But I guess I mean like as I have this sort of spin relative to the black hole,
Starting point is 00:33:00 and then as I enter the event horizon, and before I fall to the very core of the black hole, maybe I'm still going around in circles. or in a spiral you are yeah you still have that spin exactly and so things are spinning on the outside of the black hole and things are spinning on the inside of the black hole and that's just because of conservation of angular momentum right it can't go away and so if the black hole sort of isolated in space then the stuff that started forming the black hole has to keep spinning and what's fascinating is that you know maybe the insangularity it's like a circle of zero
Starting point is 00:33:35 volume that's spinning so you can have angular momentum But even more interesting is what's going on outside the event horizon. Because outside the event horizon of a spinning black hole is not like a hole that you just sort of like slide into. It's more like a whirlpool, which I think you were like describing. As you fall in, you're spinning around it. And it's so strong that it's spinning space itself. It's like dragging space around with it as it spins. Well, what do you mean?
Starting point is 00:34:00 Like it's swirling space time itself? Yeah, remember we had an episode about frame dragging this incredible experiment, gravity probe B that has the smoothest balls known to man spinning in these gyroscopes out in a satellite in space. And these gyroscopes can detect how the earth spinning is dragging space with it, which makes those gyroscopes twist a tiny bit. So this has the effect of spinning things, not just pulling on them. So because the earth is spinning, it doesn't just tug on satellites out in space. It also gently spins them a little bit. That's because it's dragging space with it. Sort of like imagine putting a fork into a big sheet of pasta and spinning it,
Starting point is 00:34:43 the whole sheet of pasta then gets like twirled up around the fork. Whoa. And that's just sort of a consequence of the speed limit of the universe, kind of? Like, why does that dragging occur? Why do things get spun around if they're not touching actually the center? It's just an extension of the question, you know, why does space get bent around masses? We don't know. It's just something we've observed. And the effect of space, getting bent is the force of gravity. Now, the effect of space dragging around a spinning object is that it causes a spin on things. So remember, the curvature of space creates this fictitious force of gravity. The gravity is not just like pulling you towards the densest spot. It's also
Starting point is 00:35:23 spinning you a little bit. So you're saying kind of like the earth spinning right now is imparting a little bit of spin on the moon, for example. Yes. And it's a very, very subtle effect compared to its tug, which is why I took a very sensitive experiment. We have a whole episode on Gravity Probe B and what is frame dragging. People should dig into if they're interested in that. The effect of space being spun around on the outside, past the event horizon, of a spinning black hole creates this new region we call the ergosphere. Wait, let me go back a little bit.
Starting point is 00:35:55 In the example of the Earth and the Moon, like the Earth spinning is imparting some spin on the Moon, but in the sense that it's making the Moon spin faster. in place, or it's making it spin faster sort of around the Earth? Spin faster in place. Like if you put an object in orbit around the Earth that wasn't spinning, the Earth but very gently started to spin around its own axis. Interesting. And is that because of sort of like the difference in the distance from the end of the
Starting point is 00:36:21 moon that's furthest from the Earth and the difference to that from the point that's closer to the Earth? You know, do you know what I mean? Like, could that be a way to explain why this spinning happens? Yeah, like imagine what would happen if you put a ball into a whirlpool. It wouldn't just fall in towards the center. It would start to spin because the current on the inner side of it wouldn't be the same strength as the current on the outer side of it.
Starting point is 00:36:43 And that would be an effective rotation on the Earth. I see. Like the side of the moon closer to the Earth is getting maybe pushed along a little bit faster, which is then making the moon kind of spin in place. Yeah, it's sort of like tidal forces where the Earth is pulling harder on the near side of the moon, for example, than the far side, because of the difference in their distance from the center of the Earth, and that effectively elongates the moon.
Starting point is 00:37:08 In this case, it's the swirling of space time, which is faster, closer to the spinning object, the Earth of the black hole, just like the near side of the moon is being dragged faster than the far side. So it effectively spins the moon as well as carrying it along in this swirling space time. Wow. All right, so then you're saying that this is kind of what happens outside of a black hole.
Starting point is 00:37:31 like if I'm outside of a black hole, I'm going to get spun in place because the part of me that's closer to the black hole sort of wants to spin faster around the black hole and the part of me that's furthest away from the black hole. And so now imagine a photon moving around a black hole. We're still outside the event horizon, right? All the same rules apply to a spinning black hole
Starting point is 00:37:51 that you can't escape the event horizon. But now there's this funny region outside the event horizon. Think about a photon moving around a black hole. A photon moving around a black hole is now moving through space itself that's being dragged. And so there's this region outside the event horizon where a photon moving as fast as it can at the speed of light through that space
Starting point is 00:38:13 would appear to be stationary to you. It's sort of like swimming upstream. So say you're, for example, far away from the black hole and you're watching this spinning black hole and you see a photon enter this region outside the event horizon and move against the current of the black hole. So the black hole spinning one way and the photon is going the other direction.
Starting point is 00:38:32 It's sort of like swimming upstream. So like somebody in a whirlpool trying to escape. So you're saying like the black hole is dragging space around, sort of like you said, like the fork, you know, twirling on a plate of spaghetti. And so the spaghetti is all wanting to sort of troll in one direction. You're saying, what if I shoot a photon that's going in the opposite direction? You're saying it's going to seem like it's not moving?
Starting point is 00:38:52 Exactly. The same way a photon inside the event horizon, trying to escape the black hole in your sort of normal vanilla black hole, would appear to stop, right? Because it can't escape the event horizon. For an outside observer, that photon can appear to have zero velocity as it tries to climb out of the gravitational well of the black hole's event horizon. But of course, it can't make it out. The analogous behavior for a spinning black hole in a photon in its ergosphere is that the photon is trying to go around the black hole moving opposite the direction of spin, but unable to overcome the swirling of space
Starting point is 00:39:28 itself because it's limited to moving through space at the speed of light. It's like somebody trying to swim against a whirlpool and getting swept up along with it. Now inside the ergosphere, it gets overcome by the swirling of space, so it actually moves backwards. The opposite direction you would expect. The edge of the ergosphere is defined as the points where the photon appears to be motionless, where its speed is exactly counteracted by the swirling of space. And outside the ergosphere further from the black hole, of course, photons can overcome this swirling of space because it's not as strong. Whoa. I see. So because, you know, the event horizon is where you might, in a stationary black hole, that's where a photon that's
Starting point is 00:40:09 trying to leave the black hole would seem like it's stuck in space, right? Not moving, right? But you're saying that for spinning black holes, because of this dragging effect, there's some weird stuff that happens outside of the event horizon where you can actually maybe see a photon kind of stop in space. That's right. Inside the ergosphere, which is this region outside the event horizon, in order to be like stationary relative to the black hole, you would have to be moving faster than light. And so at the ergosphere, what defines the edge of the ergosphere is where a photon,
Starting point is 00:40:39 which is moving at light speed, can be stationary relative to the black hole. And so outside the ergosphere, of course, you can be stationary relative to the black hole without going faster than the speed of light. inside the ergosphere because space is being spun so fast to be stationary with respect to the black hole you would have to go faster than the speed of light which is impossible so everything even photons are like pushed along in this whirlpool outside the event horizon inside the ergosphere wow i thought that was kind of like impossible to see a photon like stop there's a really subtle and fascinating point here that we're going to dig into in a future episode it's true that
Starting point is 00:41:16 photons are always observed to be going at the speed of light. That's like a well-known result of special relativity. But there are some qualifiers to that that are not usually explained. Those qualifiers are that the photon has to be near you, has to be a local photon, and it has to be in flat space, space without any curvature. So local observers, people always see nearby photons moving at the speed of light. But things that are far away from you, general relativity says that if space is curved, you could see photons going at faster than the speed of light or less than the speed of light or even stopping. Because in general relativity, it's very hard to even define what you mean by the velocity of objects that are far away from you in curved space.
Starting point is 00:41:56 Like you wouldn't actually maybe see this photon stopping because, you know, there's all kind of weird stuff going on. Also, it's weird stuff going on. And what you mean by velocity in that case is not even well defined. But we'll dig into that in an upcoming episode. Right. Not to mention also the question of how do you even see a photon, right? Like the only way to see a photon is if it hits your eyeball. Like if a photon at stock outside of a black hole, how do you even see it? You can't see it, right? You can't even bounce a photon off of that. If you can't get to it, then you can't interact with it and you can't observe it. All right. So then an ergosphere is sort of the region of space around a black hole, a spinning black hole where space is being
Starting point is 00:42:33 dragged so much, it like it can overpower a photon. Yeah. And there's one more really cool wrinkle about this, which is the shape of the ergosphere. You might think it would be a sphere, right? Well, wrong. It's more like a torus or a donut. It's not spherically symmetric because there's a spin axis and the effect is due to spin. So the ergosphere is like a donut around that spin axis. There's actually no ergosphere past the event horizon along the north-south spin axis because there's no spin in that direction. But on the plane where it's spinning, perpendicular to the north-south axis, the ergosphere can extend out like 50% further than the event horizon, depending, of course, on how fast the black hole is spinning. And so there's no ergosphere,
Starting point is 00:43:18 sort of like on the north pole and the south pole, it's sort of like a big fat blob around the event horizon along the equator. Oh, I see. But wait, is it a donut, like a torus? Or is it more like a, you know, one of those jelly-filled donuts, which is like just a flat block? It should have been called the ergo jelly-filled donut. You're exactly right. right? No, but seriously, like what's the shape? Is it shaped like a donut with a hole in the middle? Or is it shape more like a blobby piece of bread? It's a blobby pizza dough that's spinning, right? And so it doesn't actually have a hole in the middle. At the very core, its minimum size is the event horizon itself. And then it grows out to be to have a larger radius at the equator. So it's like a spinning piece of pizza dough. I feel like there's a mathematical name for that kind of shape, but we just don't can't come up with it right now. It's not jelly-filled donut, is it? It's the jelly donut.
Starting point is 00:44:07 It's totally the jelly-filled donut. I hear geometers talk about that all the time. All right. Well, apparently you can use this ergosphere, this jelly-filled donut area around a spinning black hole to get some work out of the black hole. So let's get into how to do that. But first, let's take a quick break.
Starting point is 00:44:36 The holiday rush, parents hauling luggage, kids gripping their new Christmas toys. Then, at 6.33 p.m., everything changed. There's been a bombing at the TWA terminal. Apparently, the explosion actually impelled metal, glass. The injured were being loaded into ambulances. Just a chaotic, chaotic scene. In its wake, a new kind of enemy emerged, and it was here to. to stay. Terrorism.
Starting point is 00:45:09 Law and order criminal justice system is back. In season two, we're turning our focus to a threat that hides in plain sight. That's harder to predict and even harder to stop. Listen to the new season of Law and Order Criminal Justice System on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. My boyfriend's professor is way too friendly. and now I'm seriously suspicious. Well, wait a minute, Sam.
Starting point is 00:45:38 Maybe her boyfriend's just looking for extra credit. Well, Dakota, it's back to school week on the OK Storytime podcast, so we'll find out soon. This person writes, my boyfriend has been hanging out with his young professor a lot. He doesn't think it's a problem, but I don't trust her. Now, he's insisting we get to know each other, but I just want her gone.
Starting point is 00:45:55 Now, hold up. Isn't that against school policy? That sounds totally inappropriate. Well, according to this person, this is her boyfriend's former professor and they're the same age. And it's even more likely that they're cheating. insists there's nothing between them. I mean, do you believe him? Well, he's certainly trying to get this person to believe him because he now wants them both to meet. So, do we find out
Starting point is 00:46:14 if this person's boyfriend really cheated with his professor or not? To hear the explosive finale, listen to the OK Storytime podcast on the IHeart Radio app, Apple Podcasts, or wherever you get your podcast. A foot washed up a shoe with some bones in it. They had no idea who it was. Most everything was burned up pretty good from the fire that not a whole lot was salvageable. These are the coldest of cold cases, but everything is about to change. Every case that is a cold case that has DNA right now in a backlog will be identified in our lifetime. A small lab in Texas is cracking the code on DNA. Using new scientific tools, they're finding clues in evidence so tiny you might just miss it.
Starting point is 00:46:56 He never thought he was going to get caught, and I just looked at my computer screen. I was just like, ah, gotcha. On America's Crime Lab, we'll learn about victims and survivors, and you'll meet the team behind the scenes at Othrum, the Houston Lab that takes on the most hopeless cases to finally solve the unsolvable. Listen to America's Crime Lab on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. I'm Dr. Scott Barry Kaufman, host of the Psychology Podcast. Here's a clip from an upcoming conversation about exploring human potential. I was going to schools to try to teach kids these skills and I get eye rolling from teachers or I get students who would be like, it's easier to punch someone in the face. When you think about
Starting point is 00:47:42 emotion regulation, like you're not going to choose an adapted strategy which is more effortful to use unless you think there's a good outcome as a result of it if it's going to be beneficial to you. Because it's easy to say like go you go blank yourself, right? It's easy. It's easy to just drink the extra beer. It's easy to ignore to suppress seeing a colleague who's bothering you and just like walk the other way avoidance is easier ignoring is easier denials is easier drinking is easier yelling screaming is easy complex problem solving meditating you know takes effort listen to the psychology podcast on the iHeart radio app apple podcasts or wherever you get your podcasts
Starting point is 00:48:32 All right, Daniel, how do you put a giant jelly-filled donut that bends space and time to work for you instead of just adding some weight around your middle part? The idea invented by Roger Penrose is to throw something into the black hole's ergosphere and have it gravitationally slingshot out because of the swirling of space time and have it come out with more speed, more energy than it had going in. You have, for example, a rock or a spaceship or something and you let it come close to the black hole. you do not go inside the event horizon or of course it's lost forever you just go into the whirlpool near it inside the ergosphere and what happens there is you're sucked into this whirlpool you pick up a bunch of energy because the black hole is pulling on you so it's speeding you up so now you have this energy but of course you want to get out right you don't want to just spend the rest of your life swirling around a black hole eventually to fall in so what you have to do is somehow escape
Starting point is 00:49:26 the vicinity of this black hole but now you've picked up all this energy which is pulling you in towards the center. So what you have to do is sacrifice something. You like chop off a piece of your block or you use some fuel or something. You throw something into the event horizon. You sacrifice some part of your ship into the event horizon, which gives you momentum in the other direction,
Starting point is 00:49:47 kicks you out. And in the end, you come out with more energy than you came in with. Wait, what? Hmm. Okay, so I guess the idea is to throw something at a black hole, but not and have it sort of like do a swing by, of the black hole without going
Starting point is 00:50:02 into the event horizon because if it goes into the event horizon then you're toast but you just go right outside of it and somehow you're able to escape that wouldn't something escape anyways like you know we're swinging around the sun you can swing a satellite
Starting point is 00:50:15 towards the sun but it'll just come out the other way yeah it's possible to whip around the sun and come out the other side it's harder to do that with a black hole because the angles of escape start to shrink down as you get close to the black hole until you have to be going straight away perpendicular from the black hole in order to escape. We do something similar all the
Starting point is 00:50:35 time. Change the direction of your space probe and give it a little bit of a speed boost. You can swing it around Jupiter. It doesn't have to fall into Jupiter. You can just go around Jupiter and it can pick up some energy. And we talked about that once on a previous episode. And what that does is steal a little bit of the energy from Jupiter and it gives it to the probe. This is an analogy to that, but it's more powerful because the ergosphere has a lot of energy in it. So it's like a supercharged version of this gravitational slingshot. I see.
Starting point is 00:51:06 So then the idea is that I slingshot something into a black hole and somehow miraculously it comes out with more energy than it had when it went in. Yeah. And it's not a miracle. You know, it's physics. The reason it has more energy than when it came in is that it's stealing some of that energy from the black hole. The black hole is using its gravity.
Starting point is 00:51:24 It's using this spinning mass to spin space time. and you're getting carried along with it. So it's boosting up your kinetic energy. It's giving you more velocity. I see. So the idea would be like I throw a rock at the black hole. It goes through the ergosphere. It picks up some spin, like it spins and splice.
Starting point is 00:51:41 And then it shoots out the other end or maybe it comes back around towards me. And now I have the same rock that I threw in, but now it's spinning, which has some extra energy to it. Not quite. You throw a rock near a black hole into the ergosphere. It wouldn't necessarily just come out, right? Something that comes that close to a black hole is very likely eventually going to fall into the black hole. So if you throw it that close to a black hole, it's probably doomed. It's technically possible for it to escape, but it's probably doomed.
Starting point is 00:52:09 But it will pick up a bunch more energy before it falls into the black hole because space time is dragging. It is pulling on it. Now, in order to get it out of the ergosphere, you're going to have to either burn some fuel on your rocket or split that rock in half so that part of it falls into the center of the black hole. and part of it gets a push out of the ergosphere. But you're saying then what comes back is only half a rock. Yes. You get half a rock back, but it has more energy than the rock you threw in. What do you mean?
Starting point is 00:52:36 Like, it's coming at me faster than the one I, like I drop it in, but it comes at me with a whole bunch of velocity. Yeah, exactly. And so you throw the rock in and you get a smaller rock out, but it has overall more kinetic energy than the rock you threw in. Oh, I see. So it's like I'm feeding the black hole, and in exchange, I'm getting shot at by little rocks.
Starting point is 00:52:55 Yes, but it's not an even exchange, right? The black hole is getting some mass because it gets part of your rock, but it's giving you more energy than you're giving it. So you're extracting energy from the black hole. Wait, what? So the black hole loses in this little scheme of yours. The black hole slows down a tiny bit. If you do this, you're essentially stealing some of the energy from the black hole spin,
Starting point is 00:53:20 which effectively slows it down a tiny bit. The same way hawking radiation shows, shrinks the size of a black hole by stealing some of its energy, giving a little boost to a particle. This steals some of the energy of the black hole spin and slows down its spin. Whoa. So does that mean that then you're sort of killing the black hole a little bit? You're slowing down the black hole, stealing some of its energy. And so you can steal some like almost 30% of the energy of the black hole can be stored in its spin. So yeah, you can steal that much energy from a black hole using this idea.
Starting point is 00:53:55 Oh, I see. But you wouldn't kill the black hole because the only thing you can steal is the spin of it. You can't steal the actual black hole in the middle. Yeah, but remember that mass is just a reflection of energy that's stored inside. And so the spin of the black hole contributes to its mass, right? A black hole that's spinning is more massive than a black hole with the same stuff in it that's not spinning because the whole gravitational energy reflects all the internal energy, even spin. So you are stealing some of its mass. You're right, but I guess what I mean is that you can steal energy from it, but at some point, the black hole is going to stop spinning. It's going to be game over for your little energy
Starting point is 00:54:32 sucker. That's right. You'll suck all the rotational energy out of this giant cosmic battery. And then all you'll be left with is a short child black hole. You'll shrink the ergosphere gradually down to the event horizon and it'll disappear because short child black holes, normal ones that don't spin, don't have an ergosphere. Right. But it'll be a bigger black hole, short child black hole, you fed at all these little rocks. That's true, but you've stolen more energy than you've given. So net, it'll lose energy and therefore lose mass. I see.
Starting point is 00:55:03 But you lose a bunch of rocks, too. A bunch of rocks, yeah, exactly. And you might remember this actually is a plot point in my favorite movie, Interstellar. There's some moment when they realize they don't have enough fuel to get where they're going. And so they do a black hole gravitational slingshot where they dive into the ergosphere and take advantage of the penrose process. Wow. And then what did they sacrifice? They burned a bunch of fuel, right? And it's effectively the same thing.
Starting point is 00:55:29 If you use fuel, you're giving yourself a momentum kick and you're kicking something else out the other end. Oh, interesting. All right. So then we could potentially get energy from this ergosphere, but you got to shoot a lot of rocks. Is there a more sort of like practical scenario or some sort of like device that would do this automatically? You could do this also with photons, right? You can drop photons into the ergosphere and they would come out with more energy than they went in. They wouldn't be going faster, but it would change their frequency. And so if you built some device that, like, dropped photons into the ergosphere and they came out, you could basically be harvesting the energy of the black hole by increasing the power of your light. All right.
Starting point is 00:56:09 So then the scheme would be to gather a bunch of rocks, throw them at a black hole, and then have something that trends, when they come back faster at us, we somehow harness that energy. If you did this, for example, to the black hole at the center of our milky hole. way, Sagittarius A star, you could steal as much energy as all the stars in the Milky Way are putting out in a billion years. So we're talking about like vast cosmic amounts of energy that would just really dwarf, you know, all of human energy production. Right. Because I think what you mean is that the black hole at the center of our galaxy has all that energy stored in its spin. It has as much energy in its spin as the light that the Milky Way emits in a billion years.
Starting point is 00:56:53 Yeah, there's a huge amount of energy stored in the spin of the black hole at the center of the galaxy. So that could potentially be stolen from us by some rocky scheme. Exactly. Maybe aliens are building pasta makers right next to the center of the galaxy. Yeah, that's right. Does it work with orzo pasta too? Like if I throw a bunch of little orzo palettes, do they come out, you know, like linguine on the other side? I suppose so. You know, for me, the question is, is it theoretically possible to get. energy out of a black hole once the answer is yes the rest is up to the engineers but i guess you know to do this you would need a lot of rocks right you would need a lot of you would need to build like giant rockets or something or giant spaceships or giant like black hole the harvester devices
Starting point is 00:57:40 or vehicles that you throw in and then they know when to start coming out to on the other side and that's your job i guess i'm not sure to say thanks for telling us that but um you're not telling us how to make it work. And our time is up. Thank you very much. And good luck. I'm going to go make some homemade pasta. Exactly. Time for lunch. No, but seriously, like how practical is this idea, right? Like you would need to come up with like some kind of spaceship that you throw into the black hole that then what? Then separates and then boost its way out. And then you catch it on the other side. Yeah. So you'd need to develop some system, you know, we have like explosive elements in rocks or rocks that split in half or you know somehow devise a way to do it
Starting point is 00:58:28 with particle beams but you know in principle it is possible uh all right and so this idea is interesting because kind of where things are headed in the universe we're heading towards sort of like an all black hole universe right like eventually all of the black holes in the center of all those galaxies will eventually sort of consume all of those those galaxies and then they those clusters might It also kind of crunched down to giant black holes. So we're going through a future where everything will be black holes, right? And so it might be good to know how to get energy out of it. Suns will continue to burn in this universe.
Starting point is 00:59:02 And we do know that black holes will live on for billions and trillions of years. And so instead of just getting our energy from the nearest star, we might need to learn how to get it from the nearest black hole. Right. But even then, it's going to run out, right? Like, this is not a renewable resource, is it? Like, once you take all the spin out of a black hole, it's kind of maybe useless to us?
Starting point is 00:59:21 I suppose, but there are vast quantities of energy stored in these black holes beyond even, I think, our capacity to charge our phones. I don't know. I wouldn't put it past humans to swipe their way into oblivion in the trillions of years. All right. Well, an interesting idea and potentially maybe something that could propel humanity into the far, far future. And just kind of another lesson about where the universe likes to hide energy, how it has all these crazy processes out there that are maybe storing vast amounts of potential energy.
Starting point is 00:59:55 And we already know that the universe around us is very, very dense with energy. Every atom in your body contains an incredible amount of energy. A raisin's worth of matter has more energy than a nuclear bomb. And so it's just a question of figuring out how to harvest that and how to do it safely. Yeah, I think I'll focus on the Jorge sphere first and the ergosphere. Well, the more pasta you eat, the larger the Jorge sphere gets. then my head starts to spin and that creates a singularity or at least another jelly-filled donut. Exactly, the banana guillarity.
Starting point is 01:00:26 All right, well, we hope you enjoyed that. Thanks for joining us. See you next time. wherever you listen to your favorite shows. December 29th, 1975, LaGuardia Airport. The holiday rush, parents hauling luggage, kids gripping their new Christmas toys. Then, everything changed.
Starting point is 01:01:17 There's been a bombing. at the TWA terminal, just a chaotic, chaotic scene. In its wake, a new kind of enemy emerged, terrorism. Listen to the new season of Law and Order Criminal Justice System on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. My boyfriend's professor is way too friendly, and now I'm seriously suspicious. Wait a minute, Sam. Maybe her boyfriend's just looking for extra credit. Well, Dakota, luckily, it's back to school week on the OK Storytime podcast.
Starting point is 01:01:48 We'll find out soon. This person writes, my boyfriend's been hanging out with his young professor a lot. He doesn't think it's a problem, but I don't trust her. Now he's insisting we get to know each other, but I just want her gone.
Starting point is 01:01:59 Hold up. Isn't that against school policy? That seems inappropriate. Maybe find out how it ends by listening to the OK Storytime podcast and the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. I'm Dr. Scott Barry Kaufman,
Starting point is 01:02:13 host of the Psychology Podcast. Here's a clip from an upcoming conversation about how to be a better you when you think about emotion regulation you're not going to choose an adaptive strategy which is more effortful to use unless you think there's a good outcome avoidance is easier ignoring is easier denials easier complex problem solving takes effort listen to the psychology podcast on the iHeart radio app apple podcasts or wherever you get your podcasts this is an iHeart podcast

There aren't comments yet for this episode. Click on any sentence in the transcript to leave a comment.