Daniel and Kelly’s Extraordinary Universe - Could dark matter be making flashes of light?

Episode Date: October 10, 2023

Daniel and Jorge break down a new study that looks for dark matter using both gravity and light.See omnystudio.com/listener for privacy information....

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Starting point is 00:00:00 This is an I-Heart podcast. It's important that we just reassure people that they're not alone, and there is help out there. The Good Stuff podcast, Season 2, takes a deep look into One Tribe Foundation, a non-profit fighting suicide in the veteran community. September is National Suicide Prevention Month, so join host Jacob and Ashley Schick as they bring you to the front lines of One Tribe's mission. One Tribe saved my life twice. Welcome to Season 2 of The Good Stuff. Listen to the Good Stuff podcast on the iHeartRadio app, Apple Podcasts, or wherever you get your podcast. I'm Dr. Scott Barry Kaufman, host of the Psychology Podcast.
Starting point is 00:00:38 Here's a clip from an upcoming conversation about how to be a better you. When you think about emotion regulation, we'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 is easier. Complex problem solving takes effort. Listen to the psychology podcast 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. Grazias, 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?
Starting point is 00:01:17 No, I didn't audition. I haven't audition 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. achievement and a whole lot of laughs. And of course, the great bibras you've come to expect.
Starting point is 00:01:32 Listen to the new season of Dresses Come Again on the IHeartRadio app, Apple Podcasts, or wherever you get your podcast. Let's start with a quick puzzle. The answer is Ken Jennings' appearance on The Puzzler with A.J. Jacobs. The question is, what is the most entertaining listening experience in podcast land? Jeopardy Truthers believe in... I guess they would be conspiracy theorists. That's right. They gave you the answers and you still blew it.
Starting point is 00:02:04 The Puzzler. Listen on the iHeart radio app, Apple Podcasts, or wherever you get your podcasts. Hey, Daniel, I'm curious. How does a physicist make mental. images of some of the tricky things you do research on. You know, I'm not sure you really want to see inside the brain of physicists. It's a bit of a miss. Well, let's find out.
Starting point is 00:02:34 What's your mental image of dark matter? Okay, that's a really tough one because it's invisible. I guess I sort of imagine it like water, which is, you know, mostly transparent, but you can definitely tell it's there. So we're all swimming in a bath of dark matter? I hope there's some dark matter rubber duckies out there. Some dark duckies. I wonder if they have a cute song for that on.
Starting point is 00:02:55 That would make dark matter bath time lots of fun. It's a special episode on the letter D for dark matter. Hi, I'm Jorge, I'm a cartoonist and the author of Oliver's Great Big Universe. Hi, I'm Daniel. I'm a particle physicist and a professor at UC Irvine. And this episode is brought to you by the taxpayers of California. Is it? They're not paying me.
Starting point is 00:03:31 This professor is brought to you by the taxpayers of California, I should say. I thought our heart was paying you. Are you double dipping here, Daniel? Sounds like it. I am multifaceted. You're multi-paid. Is that what you're saying by multiple people? Sounds like a good setup there.
Starting point is 00:03:50 I got no complaints. But anyways, welcome to our podcast, Daniel and Jorge Explain the Universe, a production of iHeartRadio. In which we try to bring multiple streams of understanding together into your brain. There's so many ways to understand the universe, so many questions to ask about it, so many things to understand. The challenge of physics is to weave all those together
Starting point is 00:04:11 into one coherent, comprehensive story that explains the universe to us and to you and to our kids. And that is the goal of this podcast. That's right, because it is a vast universe full of all kinds of things that start with all kinds of letters, the letter A, the letter B, the letter C, all of the letters in the universe, even the ones we haven't discovered yet. Even letters in other alphabets. In particle physics, we often reach to the Greek alphabet to name our particles.
Starting point is 00:04:37 Is that why it's all Greek to me? That's exactly right. And sometimes when we run out of Greek letters, we dip into the Hebrew alphabet. I thought you were going to say you're going to dip into alien alphabets. Or one day, we might have variables that are only defined in an alien language. That sounds wonderful. I look forward to figuring out how to write alien letters in Word. You're going to need like another app like Triolingu or something.
Starting point is 00:05:03 I'm sure this is going to be a unicode symbol for alien languages. Oh, does that mean there'll be alien emojis? What if the first message we get from aliens is just in emojis? Then we need our kids to help us interpret it. Yeah, let's hope it's not like food icons. Like, hey, hey dinner. Hey, hot dog, hamburger pizza. I think the food emojis have other meanings sometimes.
Starting point is 00:05:27 You know, the eggplant, for example. I don't know what you're talking about, Daniel. What kinds of websites have you been surfing? Ask your kids about it later. I doubt it. But anyways, it is a big universe full of amazing things to study and observe. If we can actually see them. One of the challenges of understanding the universe is first figuring out what's out there.
Starting point is 00:05:51 We begin by using the natural senses we're all familiar with, our eyes, our ears, our noses, et cetera. But there's so much more out there that we can detect with more subtle methods. Yeah, because there's a lot of stuff out there that we can see, but also a lot of stuff we can't see. One of the most amazing discoveries in recent decades has been the idea that most of the universe is out there, but we can't see it or touch it or feel it.
Starting point is 00:06:15 As we progress scientifically and technologically, we build new kinds of eyeballs, new kinds of sensors, new kinds of ears that let us detect things happening in the universe that were otherwise invisible and impossible for us to notice. Sometimes that means seeing entirely new signals like photons of very high energy or low energy. Sometimes that means noticing patterns in other signals like the rotations of galaxies and gravitational hints in the motions of other objects that tell us there's so much more going on out there than we could immediately see.
Starting point is 00:06:46 Yeah. And one of the biggest pieces of stuff out there that we can see is called, dark matter. It accounts for about 27% of the universe, right, Daniel? That's right. In any given chunk of the universe, just over a quarter of the energy is devoted to dark matter. And only 5% of it is made of the kind of stuff that you and I are made out of, baryons, corks, leptons, this kind of stuff. Which means that there's a lot more of the invisible stuff out there than the visible stuff. Yeah, which kind of makes you wonder if maybe we're the ones that are invisible. Maybe we need to learn those dark matter emojis pretty quickly. But could we see
Starting point is 00:07:20 them. Maybe you are receiving dark matter emojis. You just don't know it. I have kind of an outdated operating system. So a lot of the emojis I get are question marks anyway. Maybe those are the aliens trying to talk to me. Maybe they're actually sending you question marks. They're like, Daniel, why are you getting paid so many ways for the same thing? You know, I do get lots of questions from listeners. So maybe some of those are actually coming from the aliens. Interesting. Are you calling our listeners aliens? I'm saying we're inclusive, right? Everybody is welcome. We try to reach everybody. Not just humans. Well, there you go.
Starting point is 00:07:52 If you want to stump a physicist, just send them a question in the form of emojis. You know how they summarize movies sometimes with just emojis? I wonder if you can do that with physics theory. What? They summarize movies with just emojis? Yeah, or books or stories or news items. Oh, I feel really out of touch. Speaking of out of touch, that's what Dark Manor is.
Starting point is 00:08:12 It's stuff that's out there that you can't see and you can't even touch, right? Because it doesn't feel the electromagnetic force, so you can feel it with your fingers. That's right. It doesn't emit light, give off light, reflect light, or interact with light at all, which makes it pretty dark. And if a huge chunk of the universe is so dark but so important, then scientists really have to figure out how to study it, how to understand what it is. So we're doing our best to be creative to find new ways to look for it. So that we can study it and kind of figure out what it's made out of. And so there are maybe new ideas out there about how to do this. So today on the podcast, we'll be tackling the question.
Starting point is 00:08:57 Could Dark Matter be making flashes of light? I always figured Dark Matter was pretty flashy. Well, I don't know the name Dark Matter is more mysterious than flashy, isn't it? Well, that's just what we call it. Maybe it's something we can't see, but really inside it's fancy and flashy. Maybe when we finally meet the beings made of Dark Matter, they'll be like annoyed or offended or disappointed that we call them dark matter. Hopefully they won't flashes.
Starting point is 00:09:25 You mean like zap us with a laser beam from orbit or open the trench code? I mean like Santa's fruit emojis. So as usual, we were wondering how many people out there had thought about the idea of seeing dark matter through flashes of light. Thank you very much to our group of volunteers who answers these questions. We love hearing your thoughts on the topic of the day. If you would like to contribute, please don't be shy. is welcome whether you've been listening for years or weeks or days or this is your first episode just write to me to questions at danielanhorpe.com so think about it for a second do you think
Starting point is 00:09:59 dark matter could be making flashes of light that we could see here's what people had to say i don't know but that'd be cool the concept of dark matter making flashes of light is quite interesting since dark matter seems to make up a large port of the universe i don't see why it could be giving off light pulses, given the right circumstances. I think that only directly by baking stuff made of regular matter to behave in a certain way due to gravitational effects. Since it doesn't interact with the electro-weak force, I think not. All right.
Starting point is 00:10:35 I think that pretty much summarizes the episode here. I don't know, but that would be cool. I feel like that's almost every episode. That's the emoji version of the episode, yeah, if you had to summarize it. So that would be what shrug, question mark, check mark. Is that how you summarized in emojis? Yeah, or like a black square for dark matter, question mark, truck. And then the emoji with the sunglasses for cool.
Starting point is 00:10:58 Yeah, or sparkles. Isn't there a sparkles emoji? Well, it depends how flashy you want to get, Daniel. Let's go all out. We got multiple funding sources here. There you go. Let's go out with a flash of jail time. But anyways, let's get down to it.
Starting point is 00:11:11 Daniel. Let's recap for listeners. What is dark matter in the first place? It's important that we explain what we mean when we say dark matter because I notice there's lots of different ideas out there about what dark matter is. Online, you see a lot of people saying dark matter is just a placeholder. It's just a way to say we don't know. Other people talk about dark matter as if it was a very specific theory of a very specific particle. There's a whole bunch of people in the middle to talk about dark matter as a sort of general catalog of ideas.
Starting point is 00:11:39 But all of these things are there to explain something that we don't understand, which is that there's a lot of grass. happening in the universe that we cannot explain. Like when you look at how galaxies spin and when you look at how the universe formed and all the gravity necessary to pull the stars together into galaxies, we just cannot explain all that galaxy using the stuff that lights up, using the stuff made of quarks that either glows or reflects light or gives off light. We just cannot tell the story of the universe and have it make sense without something else out there providing a bunch of gravity. So much gravity is missing that you need five times as much of this mysterious stuff we call dark matter as there is normal matter. So very briefly, dark matter is just an idea to explain all this unexplained gravity in the universe. Yeah, and there are different ways that scientists have sort of found or think that dark matter is there. And they are, as you said, they all relate to gravity.
Starting point is 00:12:34 But I think basically the main idea is that what we see of the universe tells us that there's more matter out there than the stuff that glows or that we can see and feel, right? Exactly. And the story started with the guy. galaxy rotation curves. We looked at galaxies and measured how fast they spin and we noticed that they spin really, really fast. And if you add up all of the stars and the gas and the dust in those galaxies, they don't provide enough gravity to hold that galaxy together as it spins. So that was evidence number one. And for decades, we knew about that, but it was sort of hard to accept the idea that there could be so much more missing matter out there. It was just one piece of evidence. But slowly over the decades, we've pieced together lots of total. totally independent measurements that tell us that there is missing stuff out there, that there's matter out there providing gravity that we cannot see. Like initially, for example, it could have just been that a galaxy's out there had a lot of like dark rocks, right, or gas that you couldn't see through the telescope.
Starting point is 00:13:31 Exactly. Or it could have been that gravity worked differently over really, really long distances. Like we've measured gravity in the solar system and on Earth, but maybe over hundreds of thousands of light years, gravity operates different. than Newton and even Einstein suggested that could have been the explanation when you were just looking at one example just at galaxy rotation curves but now we have lots of other ways to probe this you know we look for example at the structure of the universe how did it come together how did you go from blobs of gas mostly dispersed through the universe clumping together
Starting point is 00:14:05 into stars and galaxies and that requires gravity and if you run the universe without any dark matter just with the kind of matter we can see, you don't get stars in galaxies after 14 billion years. There isn't enough gravity to do it. You've got to add in the dark matter, and boom, then you get a universe that looks just like ours. So it's another very convincing piece of evidence that there is matter out there.
Starting point is 00:14:27 It's not just like gravity operates differently at those distance scales. It really is missing matter. But could you ask the same question about these large scale structure theories? Could it be just that gravity works differently than we thought at different scales? and that might explain why galaxies formed the way they are?
Starting point is 00:14:42 It is possible, and people who work on these theories, they're called like Mon modified Newtonian dynamics, have tried to tweak them. I've not seen one that can successfully explain both the galaxy rotation curves and the large-scale structure of the universe. Mostly these theories are tuned to explain the galaxy rotations, and they don't even try to explain the other evidence for dark matter. What's this other evidence?
Starting point is 00:15:07 Maybe one of the most compelling and precise piece of evidence, for dark matter is seeing its effect on the very, very early universe plasma. Before stars were formed, we really had any structure in the universe at all. It was just huge blobs of hot gas everywhere in the universe. And we see the glow from that gas in the cosmic microwave background radiation. When that gas cooled enough to become transparent, when it formed neutral atoms, so photons mostly could fly through it, those photons are still around and we see them. So they're like the last glow of this plasma from the very early universe.
Starting point is 00:15:37 And we see ripples in that plasma, ripples that show us how the normal matter and the dark matter and the photons were all sloshing around. And it's a very, very precise measurement. And it tells us how much normal matter there is in the universe, how much radiation there was in the universe, how much dark matter there was in the universe back then. It's very, very precise because we've taken these very, very detailed maps of these early universe plasma. And that tells us that there is a component of that plasma that doesn't interact with photons. It's not barionic. It's not our kind of matter at all. So it's another completely independent measurement that tells us there's a dark but
Starting point is 00:16:14 gravitationally active component to the universe. Now, is that also due to gravity? Like, does that evidence also depend on our current model of gravity? It does, but those are much shorter distances. Those oscillations ended up seeding the larger scale structure of the universe, but it was before a lot of the expansion. So we're talking about things that happened over short distance scales. There were short distance, but there are large distances.
Starting point is 00:16:36 distance now. That's right. But the CMB comes from when it was short distance. Earlier you were asking if this could all just be due to like long distance gravitational effects and the CMB probes shorter distance scales gravity because the picture we have of it comes from back when things were much more cozy and compact. All right. So then the prevailing picture is that there's a lot of stuff out there, stuff that creates
Starting point is 00:16:57 gravity and feels gravity, but we just can't see it. So let's get into what it could be, how we might see it and what might be new ways. to figure out where it is and what it's doing. So we'll dig into that. But first, let's take a quick break. I had this, like, overwhelming sensation that I had to call it right then. And I just hit call.
Starting point is 00:17:21 I said, you know, hey, I'm Jacob Schick. I'm the CEO of One Tribe Foundation. And I just wanted to call on and let her know. There's a lot of people battling some of the very same things you're battling. And there is help out there. The Good Stuff Podcast, Season 2, takes a deep look into One Tribe Foundation. Foundation, a non-profit fighting suicide in the veteran community. September is National Suicide Prevention Month, so join host Jacob and Ashley Schick as they
Starting point is 00:17:44 bring you to the front lines of One Tribe's mission. I was married to a combat army veteran, and he actually took his own life to suicide. One Tribe saved my life twice. There's a lot of love that flows through this place, and it's sincere. Now it's a personal mission. Don't have to go to any more funerals, you know. I got blown up on a React mission. I ended up having amputation below the knee of my right leg and the traumatic
Starting point is 00:18:06 brain injury because I landed on my head. Welcome to Season 2 of the Good Stuff. Listen to the Good Stuff podcast on the IHeart Radio app, Apple Podcasts, or wherever you get your podcast. Hey, sis, what if I could promise you you never had to listen to a condescending finance, bro, tell you how to manage your money again. Welcome to Brown Ambition. This is the hard part when you pay down those credit cards.
Starting point is 00:18:26 If you haven't gotten to the bottom of why you were racking up credit or turning to credit cards, you may just recreate the same problem a year from now. When you do feel like you are. bleeding from these high interest rates. I would start shopping for a debt consolidation loan, starting with your local credit union, shopping around online, looking for some online lenders because they tend to have fewer fees and be more affordable. Listen, I am not here to judge. It is so expensive in these streets. I 100% can see how in just a few months you can have this much credit card debt when it weighs on you. It's really easy to just like stick your head in the sand.
Starting point is 00:19:02 It's nice and dark in the sand. Even if it's scary, it's not going to go away. Just because you're avoiding it, and in fact, it may get even worse. For more judgment-free money advice, listen to Brown Ambition 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 and about. backlog will be identified in our lifetime.
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Starting point is 00:21:05 guests for this new season of Family Secrets. Listen to Family Secrets Season 12 on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. All right, we're talking about Dark Matter. Now, Daniel, how many episodes now have we talked about Dark Matter? Oh, man, so many episodes. But it's still a thing people are most confused and most interesting. about in the emails we get from people. People are still in the dark about it.
Starting point is 00:21:39 Yeah. And it's a really active area of research, obviously, because it's one of the biggest open questions in modern physics. So people are constantly trying to come up with new theories for what dark matter might be. Is it this particle? Is it that particle? Is it not a particle at all? Is it something else entirely? And new ways to spot dark matter. If it's this kind of particle, how could we see it? Could we build a detector to observe it? So it's a huge area of active research. Yeah, I guess we can't just wait for the Sesame Street episode on it. We could just sit back and wait for the aliens to show up and tell us the answers to the
Starting point is 00:22:12 universe, but that'd be kind of embarrassing if they showed up and we had like nothing to contribute. Yeah, it'd be more embarrassing if they have to do it over dinner while they eat us. I wonder if they would feel less bad about eating us if they knew we weren't, you know, dark matter intelligent. All right, well, we just kind of define what dark matter is. It's the stuff we think that's out there to explain a lot of the gravitational effects we see in how the universe form and also in the microwave background radiation.
Starting point is 00:22:39 Now, there are candidates where what we think this stuff might be, right, Daniel? There are lots of ideas for what dark matter might be. And people initially thought, well, maybe dark matter isn't some new weird kind of stuff. It's just more of the kind of stuff we already know about. But, you know, it was just hiding or something. People thought maybe dark matter is like neutrinos because neutrinos are tiny little particles that don't interact with photons. They don't give off light.
Starting point is 00:23:03 They don't reflect light. They pass right through a lot of stuff. So they seemed initially like a really good candidate maybe for dark matter. Maybe the universe is just filled with uncountable numbers of neutrinos. That would have been amazing. But neutrinos don't have a lot of mass. They're very, very low mass particles, which means they almost always move nearly the speed of light. And one thing we do know about dark matter is that it's kind of slow moving.
Starting point is 00:23:29 It's not a fast particle. Well, I guess that those are two questions. First of all, why can neutrinos go slow, even if they're light? Can you still stop them from moving? You can stop a neutrino because they have very low mass, but their mass is so low. It's like thousands of times lower than even an electron that essentially any energy in neutrino has means it's moving at almost the speed of light.
Starting point is 00:23:49 So it's almost impossible to have a natural process that produces a huge number of neutrinos and have them be slow moving. And you also said dark matter is cold. How do we know it is cold if we can't feel it? Yeah, we know that dark matter can be moving very fast because of the way it's influenced the structure of the universe. Like, dark matter is mostly responsible for what we see out there. The reason you have a galaxy here or a galaxy there
Starting point is 00:24:11 is because there's a huge blob of dark matter that created gravitational attraction that pulled all that gas in to form the stars and the galaxy. Now, if dark matter was moving really, really fast, if it was hot, then it wouldn't clump the same way. It would spread itself out much more. So we know that dark matter has to be below a certain speed, basically, or it wouldn't have clumped into these blobs,
Starting point is 00:24:32 which then form the structure of the universe. Like, if you run simulations where dark matter is a fast-moving particle, you don't get the same kind of structure that we see in our universe. That means dark matters to be slow-moving or cold, as physicists say. And that means that it can't be neutrinos. Couldn't it be like super massive, but hot too? Well, hot essentially refers to its velocity. Regardless of its mass, the issue is the velocity.
Starting point is 00:24:55 And the problem is neutrinos basically can't have low velocity. We know that dark matter can't be moving very fast. Otherwise, it would spread itself out and wash out the structure of the universe. All right. Well, then how is it that we can see it? How can we hope to see it and study it then? Yeah, it's tricky. You know, the one thing that we do know is that dark matter feels gravity.
Starting point is 00:25:13 So gravitational studies are a surefire way to detect dark matter. The problem is that gravity is super duper weak. It's like the weakest of the fundamental forces. If it even is a fundamental force, it's weaker than the weak force by like 10 to the 30, which means that it's basically impossible to use gravity to detect tiny bits of dark matter. Like we can see like solar system size chunks of dark matter maybe, but anything smaller than that, the gravity from it is too weak for us to even detect it. And that means that you couldn't really use gravity to detect the particle nature of dark matter.
Starting point is 00:25:47 Like one of the deepest questions is what is dark matter made out of? Is it this kind of particle? Is that kind of particle? But gravity is really too weak to tell us anything about the particle nature of dark matter. dark matter. And we don't even know if it is a particle, right? It could be that dark matter is something that doesn't form into particles. Is that possible? It's totally possible. It's not a mainstream idea. Like most of modern physics right now is focused on the idea of particle dark matter because the kind of matter that we know is all made of particles. And so we extrapolate and we say,
Starting point is 00:26:16 well, probably this other kind of matter is made out of particles. And you might think that sounds reasonable. It's a pretty basic assumption. But it's also extrapolating from 5% of the universe to like 25% of the universe. It's entirely possible that the physics of this other huge section of the universe is very different from anything we've imagined. We've talked in the podcast before about unparticles or other weird kind of theories that describe it as not made of particles. So like as you zoom in, it doesn't ever change. It's not like there's a basic unit of it. You can just keep zooming in forever and it always looks the same. That would be really weird, but super awesome. But the mainstream theories are mostly particle dark matter because that's what we know,
Starting point is 00:26:56 to think about because that's kind of the only way you know how to think about things right well you know there are people trying to think outside the box that requires a lot more creativity and flashes of insight but there definitely are people out there working on sort of crazier theories of what dark matter is but I think most people are working on particle dark matter because yeah that's what we're good at thinking about I mean you talk to a particle physicist you're going to get a particle explanation for everything I guess I mean like we haven't seen anything that isn't explained by particle theory, right? And we wouldn't even know what that math would look like. Yes and no. We've never seen anything that we've been able to explain with a non-particle-based
Starting point is 00:27:35 theory. But remember, there's 95% of the universe, dark matter and dark energy, that we still can't really explain. So particle-based theories are the only ones that have ever been successful, but they've only been successful in 5% of the universe. So yes and no. I guess there's a lot out there that we can't still explain. So maybe our current theory only covers 5% of the universe. Yeah, that's exactly right. So we should definitely keep an open mind to other crazy theories of what dark matter might be. But currently we're mostly working on is dark matter a particle? Is it a new kind of particle? What does it do? How could we possibly spot it if it is a particle? All right. So if it is a particle, how do we see it? How do we study it? We know that it feels gravity. What else does it feel or not feel? So the short answer is we have no idea. Like it could be that dark matter feels some new kind of force with itself. It could be that dark matter feels no form. forces other than gravity and like that could totally be our universe in which case it's almost
Starting point is 00:28:30 impossible to ever discover the particle nature of dark matter it could just be a mystery forever because gravity is just so weak there's another possibility that dark matter is kind of misnamed that dark matter does actually interact with our kind of matter through some mechanism we haven't discovered yet that is not really truly a hundred percent dark but i guess you mean using electromagnetic forces or other kinds of forces? Like dark in terms of light or dark in terms of all the forces in nature? We're imagining maybe there's a new force out there also. So we're suggesting maybe dark matter some new kind of particle, right? And in addition, maybe there's a new force out there, a force that helps dark matter particles interact with our kind of particles.
Starting point is 00:29:15 So call this a new dark force or a portal to the dark sector or whatever. If there is this new kind of force, then maybe it helps dark matter particles bump into our kind of particles or turn into our kind of particles or somehow interact with our kind of particles, which would make them effectively visible. But would you need to come up with a new kind of force? Couldn't it interact with us through the weak force or the strong force somehow? It's totally possible that dark matter could have interacted with us via one of the forces we know already, but we basically ruled that out with our experiments.
Starting point is 00:29:48 Have we really? Is that official? If dark matter interacted with the strong force, it would be a very powerful interaction because the strong force is super duper strong. And that would actually be pretty easy to find. We look for dark matter giving off photons. We've never seen that. So we don't think that dark matter actually directly interacts with photons.
Starting point is 00:30:06 We've also looked for dark matter interacting via the weak force. And this is probably the biggest area of experimental dark matter particle physics right now with these huge tanks underground, very quiet liquid like xenon. and we wait for dark matter to pass through the earth and interact with one of these xenon molecules and give it a little kick. So these huge tanks of underground liquid xenon are just waiting for a dark matter particle to bump into it via the weak force. And if it does interact via the weak force, we can calculate how often that should happen. And we've been running these experiments for years and years and years and we've never seen a blip that looks like dark matter
Starting point is 00:30:43 kicking one of these xenon molecules via the weak force. So now we can pretty definitely rule it out. I see. We've been putting stuff out there to hopefully interact with Dark Matter through the weak force, but so far nothing has been bumped that way. So now you're saying the Dark Matter probably doesn't interact with the weak force. As time goes on and we don't see any of those interactions, we will more confidently say that they never happen. If you only listen for a day, it might be that they only happen once a year and you just haven't seen one yet. But after you've listened for five years, 10 years, 20 years, either you're getting very, very unlucky or it just doesn't happen. And so now we've had big enough detectors running for enough years that we're
Starting point is 00:31:21 pretty confident ruling that out. But it doesn't mean that there isn't a new kind of force, like an even weaker force that would allow dark matter to interact with our detectors. So that's what they're looking for now. Like they call it the feeble force. It's weaker than weak. That's the idea. Exactly. Weaker than weak. We don't we have seen it already with our detectors with the tanks of xenon there sitting there waiting? Depends on how weak it is. If it's super duper extra week, if it's the feeblest force you can imagine, it might take a very, very long time. It might be so unlikely that you have to run for 10 years or 100 years in order to see it. And that's why we're also at the same time using other methods to try to look for these kinds
Starting point is 00:32:01 of interactions. Like we're hoping to use this new feeble force to create dark matter at particle colliders. What do you mean? Like when you collide protons or quarks like that, it might make dark matter? Yeah. If this feeble force exists that allows dark matter. matter to bump into protons and neutrons inside a xenon atom, then in principle, you can reverse that. You can say, well, what if we smash protons together? Maybe sometimes they can
Starting point is 00:32:27 use the feeble force to create dark matter because that's what we do with the particle collider. We annihilate protons together and create new kinds of stuff. And the cool thing about a collider is that anything that's out there, you can make it as long as your protons can interact with it. So anything that protons interact with, we produce at the collider eventually. Things that interact with protons a lot, we produce them all the time. Things that don't interact with protons very often, we produce them more rarely. So Higgs bosons are pretty rare, for example. But we combed through all of those collisions looking for evidence of the production of dark matter. Wouldn't we have seen evidence of that already? I mean, you've been running the LHC for a long time and particle
Starting point is 00:33:03 colliderous for decades. You know, if there was some sort of unaccounted for force, wouldn't we have seen it by now? We haven't seen anything. You're right. And again, it's a question of the strength of that force. If that force was as strong as the weak force, yeah, we probably would have seen it. And the longer we run our colliders and don't see it, the weaker that force has to be to still be consistent with our data, to still be hiding from all of these experiments. But we don't know how weak that force is. Maybe it's really ridiculously weak, so weak that we haven't seen it underground and we haven't seen it in our colliders. So we actually turn to another mechanism to try to see this super duper weak force in action, which is to look at the center of the galaxy
Starting point is 00:33:42 to see if dark matter is smashing into itself. I see. Use the center of the galaxy as a particle collider. Exactly. Because one problem with the particle collider is that it's not very dense, right? We have protons smashing into protons, but it's like very few protons.
Starting point is 00:33:58 And we try to run it as often as we can, and it adds up to zillions of collisions, but it just might not be enough. But we think that the center of the galaxy is very, very dense with dark matter. We can map out where the dark matter is in the galaxy, by looking at how things rotate and how fast things are moving. And we suspect that the center of the galaxy is very dense with dark matter.
Starting point is 00:34:19 And so if dark matter has this feeble force, this super weak force, then occasionally two dark matter particles should bump into each other and produce normal matter particles, like the opposite of what we think might happen in the collider, or two protons smashed together to make dark matter, run that backwards in time. We hope that's the operation happening in the center of the galaxy. So we turn these special telescopes to the words of the center of the galaxy and look for these characteristic flashes of light that might come from those collisions. Interesting. That sounds a little cheaper than building a $30 billion collider here on Earth.
Starting point is 00:34:53 Well, it was only $10 billion, right? So we can save you $20 billion off the top right there. And it wasn't that cheap because you're building a particle detector and launching it into space, which is never simple. All right. Well, let's get into the details of how we're using the center of the galaxy as a collider to look for dark matter. Let's dig into that. But first, let's take another quick break. Your entire identity has been fabricated. Your beloved brother goes missing without a trace. You discover the depths of your mother's illness, the way it has echoed and reverberated throughout your life, impacting your very legacy.
Starting point is 00:35:32 Hi, I'm Danny Shapiro. And these are just a few of the profound and powerful stories I'll be mining on our 12th season of Family Secrets. With over 37 million downloads, we continue to be moved and inspired by our guests and their courageously told stories. I can't wait to share 10 powerful new episodes with you, stories of tangled up identities, concealed truths, and the way in which family secrets almost always need to be told. I hope you'll join me and my extraordinary guests for this new season of Family Secrets. Listen to Family Secrets. Listen to Family Secrets Season 12 on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. I had this, like, overwhelming sensation that I had to call it right then.
Starting point is 00:36:21 And I just hit call, said, you know, hey, I'm Jacob Schick. I'm the CEO of One Tribe Foundation. And I just wanted to call on and let her know there's a lot of people battling some of the very same things you're battling. And there is help out there. The Good Stuff Podcast, Season 2, takes a deep look into One Tribe Foundation, a nonprofit fighting suicide. in the veteran community. September is National Suicide Prevention Month, so join host Jacob and Ashley Schick
Starting point is 00:36:45 as they bring you to the front lines of One Tribe's mission. I was married to a combat Army veteran, and he actually took his own mark to suicide. One Tribe saved my life twice. There's a lot of love that flows through this place, and it's sincere. Now it's a personal mission. Don't have to go to any more funerals, you know.
Starting point is 00:37:01 I got blown up on a React mission. I ended up having amputation below the knee of my right leg and a traumatic brain injury because I landed on my head. Welcome to Season 2 of the Good Stuff. Listen to the Good Stuff podcast on the Iheart radio app, Apple Podcasts, or wherever you get your podcasts. Hola, it's Honey German. And my podcast, Grasias Come Again, is back.
Starting point is 00:37:22 This season, we're going even deeper into the world of music and entertainment with raw and honest conversations with some of your favorite Latin artists and celebrities. You didn't have to audition? No, I didn't audition. I haven't auditioned in like over 25 years. Oh, wow. That's a real G-talk right there. Oh, yeah.
Starting point is 00:37:38 We've got some of the biggest actors, musicians, content creators, and culture shifters sharing their real stories of failure and success. You were destined to be a start. We talk all about what's viral and trending with a little bit of chisement, a lot of laughs, and those amazing vizras you've come to expect. And of course, we'll explore deeper topics dealing with identity, struggles, and all the issues affecting our Latin community. You feel like you get a little whitewash because you have to do the,
Starting point is 00:38:08 code switching? I won't say white wash because at the end of the day you know, I'm me. But the whole pretending and you know, it takes a toll on you. Listen to the new season of Grasas Come Again
Starting point is 00:38:17 as part of my Cultura podcast network on the IHartRadio app, Apple Podcast, 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
Starting point is 00:38:32 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 00:38:57 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. All right, we're looking for dark matter. I had some right here, Daniel. You don't know where I put it? emoji-based directions to it.
Starting point is 00:39:40 Derry. I'll send you some arrows. That might not be helpful there. But yeah, there's a lot of matter missing in the universe. Whole 27% of the universe is out there, but it's invisible. We can't see it or touch it. It's called dark matter. And our only hope for ever studying its particle nature is that there's some sort of new force that we haven't discovered yet, some super weak force that you're calling the feeble force.
Starting point is 00:40:04 Although, Daniel, I'm kind of disappointed you didn't call it the dark force. Because then forever it would dominate my destiny. Exactly, right? Then you get the cool red lightsabers or the cool laser pointers when you give your lectures. Yeah, that's true. But I didn't want to have to grow those horns. Not all Sith have horns. That's a relief.
Starting point is 00:40:23 You need to brush up on your Star Wars there. Apparently, yeah. But yeah, our only hope forever studying the particle nature of dark matter is that it feels a new kind of force we haven't seen before. And we can't generate that force apparently here in our colliders. But there's hope that maybe you can use the center of the center of the. galaxy as a collider to maybe study this part of this aspect of dark matter we think we're hoping is there exactly and the idea is dark matter smashes into itself and then via this new feeble force turns into standard model particles maybe tau leptons or b quarks or something and those particles
Starting point is 00:40:59 can then give you flashes of light because those particles do interact with light so what we do is we turn this telescope to the center of the galaxy and we look for these flashes of light that we can't otherwise explain. If you see flashes of light that look like they come from dark matter turning into particles we know, then you can say, oh, there's evidence for dark matter there. Wait, the idea is that dark matter smashes into itself. Why does it have to smash into itself? It doesn't have to. It's possible for dark matter also interact with normal matter particles in the center of the galaxy, the way it might interact, for example, with our tanks of xenon underground. But the signature we're looking for would come from two dark matter particles
Starting point is 00:41:38 smashing into itself, producing like a pair of bottom quarks or a pair of tau leptons, which then give off some photons which travel to our telescope and we observe them. Wait, so two dark matter particles can interact with each other and generate regular kind of matter. Yeah, exactly. Why? Does that work the other way too? Like can regular matter interact and come up with dark matter? That's what we're trying to do with the Large Hadron Collider is smash regular matter together, protons and turn it into dark matter. We haven't seen that yet. So we're trying to do the opposite, smash dark matter together and turn it into regular matter. It's like the inverse collider. What's the inverse of a collider? An expander? A separator? It just runs it the other
Starting point is 00:42:17 direction, you know? Instead of colliding normal matter to make dark matter, we collide dark matter to make normal matter. So wait, the picture is that in the center of the galaxy, you're saying there's a high density of dark matter. And some dark matter particle just happens to smash head on with another dark matter particle. Hopefully they're going fast enough to actually sort of interact and create a lot of energy. And then out of that comes a regular matter particle from the center of the galaxy that then we see here on Earth and go, yep, that came from two dark matter particles. Yeah. And if you want the microparticle physics explanation, two dark matter particles smashed together, form some new kind of particle that mediates this feeble force, call it a dark
Starting point is 00:42:58 photon or something. And then that dark photon turns into a pair of normal particles like two bottom corks or two tau-leptons or two muons or something. And then those produce photons, which then we see here. But then how can we hope to like discern that from all the way here? The center of the galaxy is, you know, 50,000 light years away? It's very tricky. And that's exactly the difficulty of this method. Number one, it's far away. We think that these photons would be very high energy. So we think that gamma rays would survive, travel from the center of the galaxy. But the real problem is that we don't understand the center of the galaxy. So a lot of stuff going on there making flashes of light anyway that we can't really understand. And so actually we have
Starting point is 00:43:42 seen flashes of light from the center of the galaxy that we cannot explain, that no astrophysical explanation has been provided to explain these flashes of light. And so some people are actually pretty excited about that. They say, whoa, maybe this is dark matter. But, you know, the problem is we really know what's in there in the center of the galaxy. It's a very weird, dense region. We just did a whole episode about how weird it is and how little we understand about what's there. So it could just be new weird stuff made of normal matter in the center of the galaxy, flashing lights in ways we don't understand, or it could be dark matter, creating these flashes of light. Wait, wait, wait. What do these flashes look like? Like you're just looking at the
Starting point is 00:44:20 galaxy, center of the galaxy, and suddenly there's like a spike or a pulse or a train of pulses, What do these flashes look like? So these flashes come as individual photons. So this telescope, a Fermilat telescope, can see gamma ray photons, which are just photons in a certain energy range, in this case from 50 million electron volts, up to a trillion electron volts. And they see a bunch of these gamma ray photons from the center of the galaxy,
Starting point is 00:44:47 and we cannot explain them otherwise. Like one at a time? Well, the detector can only see one photon at a time, yeah. I guess I mean like you see one and then you don't see one for another year, or is it you see like a whole bunch of? of them in a cluster or something. So the higher energies, they're definitely more rare than they are at the lower energies, but there's a lot of them.
Starting point is 00:45:03 It's not just like one or two or seven photons. You know, we're talking about thousands of photons here accumulated over many, many years. And so people are trying to understand where are these photons coming from? Is there something going on with normal matter at the center of the galaxy, or is this actually dark matter? But I guess why are they unexplainable or why are they so mysterious? Isn't it just like, oh, here's a photon with a lot of energy? Well, we have an idea for what's at the center of the galaxy.
Starting point is 00:45:29 We think that there's a black hole there. We think there's a swirl of stuff around the black hole. We think there's a certain density of stars. We think there's gas and dust and all sorts of stuff. And we use that model to predict what we should see from the center of the galaxy. And we see all that stuff. Plus we see more. We see another spectrum of photons that have sort of like a different shape.
Starting point is 00:45:48 Like they emit light in different patterns. They're distributed around the center of the galaxy. And their brightness and their wavelengths can't be explained by. any of the components that we do know about in the center of the galaxy. So it's definitely something new happening in the center of the galaxy, emitting photons in a way that we can't otherwise explain. And it's consistent with some theories of dark matter. All right.
Starting point is 00:46:09 Well, let's dig into that part of it. Then what's the connection between gravity and or what might be the connection between gravity and these flashes of light? Yes, so we've been seeing these flashes for a while. And there's been theories of dark matter for decades from the center of the galaxy. but people have been unsure about what it means because we don't understand what's going on at the center of the galaxy very well. So recently people came up with a really cool, clever idea to combine gravitational information with these flashes of light. They say, look, if there is dark matter creating these flashes of light,
Starting point is 00:46:41 we should be able to zero in on where these flashes come from and see if there's dark matter there by seeing if there's a gravitational effect from that dark matter. Like if there's a blob of dark matter there that's extra dense and making these flashes, we should be able to see gravitational lensing from that dark matter blob to tell us, oh, that really is dark matter and not just some star going crazy. Couldn't it just be a star going crazy or maybe like a quasar or something like that? Doesn't that seem more likely? Or like, how do you know which is more likely?
Starting point is 00:47:09 Exactly. We don't really understand what's there. So it is tricky. But the first thing they did is they tried to map all the gravitational lensing near the center of the galaxy and measure that by seeing like how that distorts light from behind the galaxy. Like a galaxy is in the background far away. How is their light being distorted as it passes through the center of the galaxy?
Starting point is 00:47:28 So that's the gravitational lensing measurement. They use that as a way to just see like, are there pockets of extra gravity in the center of the galaxy? So they make a map of all this gravitational lensing. And then they line that up with the map of these extra flashes from the center of the galaxy. And boom, boom, boom, they do line up. They line up very nicely. So there seems to be this correlation between where the. there's extra gravitational lensing and where there's more gamma ray flashes.
Starting point is 00:47:56 That's pretty interesting. Although it could just be something else, I wonder? Like, you know, maybe where there's a lot of dark matter. There's also a lot of black holes. Exactly. And everybody's very skeptical at first, right? You don't want to just like jump up and down and claim you discover dark matter. So then they try to explain this with other sources, you know, and one idea they have in this
Starting point is 00:48:15 paper is that maybe it's blazars. Blazars are these super awesome galaxies that are generating a really powerful beam of light from the center of the galaxy. If you have a super massive black hole at the core of a galaxy, then its magnetic field can funnel radiation up and down the north and south pole of that galaxy and produce a very powerful beam of light. And if that beam of light is pointed right at the earth, the relativistic effects effectively make the earth a little shorter and pile up the light beams a little bit to make it extra bright. So these things are called blazars. And blazars could also explain these effects that we're seeing. And we're
Starting point is 00:48:52 And so in the paper, they analyze like, well, is this just more Blazars than we anticipated or is it dark matter? And they can explain part of this effect with Blazars, but there's a part of it that Blazars cannot explain, and that is very nicely explained by dark matter. And so this is the challenge with studying dark matter. It's like, is what we're seeing dark matter or is it something else we don't understand? Because dark matter is still kind of a fuzzy idea. Yeah. I mean, we don't really know or have a clear idea what it's. nature is, I feel like we're sort of like putting assumptions on top of assumptions and top of
Starting point is 00:49:26 assumptions and then checking that. That is what we're doing. We're making hypotheses and we're checking them and we're coming up with alternatives like, is this dark matter? Is this something else? What we know is that there is something new happening at the center of the galaxy. Something is generating these flashes of light that we do not understand. Maybe it's dark matter. Maybe it's some other new astrophysical source. Maybe it's some new process that's distorting light from behind the galaxy. We don't know. There's something new to be discovered there. We don't know. We don't know if that lines up with these other mysteries we're seeing, like galactic rotation curves and the structure of the galaxy. So maybe this reveals something about dark matter, but maybe
Starting point is 00:49:59 it reveals something about something else, right? We're so clueless about the nature of the universe that we're trying to put these puzzle pieces together, but maybe they don't click. Maybe they're parts of different puzzles. It's just because we're at the beginning of understanding the universe that we're so clueless about how to put this all together. Yeah, I guess it could be anything. Could be aliens sending us emojis. Maybe those high-speed photons are their version of Exactly. Maybe there are express emojis. Hopefully they're safe for work. This is a very difficult kind of science because the data is sparse. You just have like these flashes of light from the center of the galaxy and we're very far away from the center, as you
Starting point is 00:50:36 said. So I've been to like whole conferences dedicated just to this signal and understanding it and people show completely different interpretations. They say, oh, I can explain all of it using some astrophysical source. And other people say, no, that's impossible. It can't describe it. And other people say, well, you forgot to account for all these uncertainties in that. And if you let these things float and consider other possible ways that these things can interact, then maybe it explains it. So we really are at the beginning days of understanding what it is we're seeing. But it's cool to see people try to line these things up, you know, gravity and flashes
Starting point is 00:51:06 of light and other ways to try to get ideas for what dark matter might be. All right. Well, it sounds like it's still kind of an open question and a big mystery, but it is a pretty exciting idea to kind of like use one mystery to try to explain another mystery. It's like you're piling on the mysteries. We are piling on the mysteries and we're trying to line things up. You know, we're trying to come up with a coherent explanation for everything we see out there in the universe. It's not fair to have one story you tell in one case and a completely different story you tell in another case, right?
Starting point is 00:51:34 You need a single theory that explains everything we see. And that's really a challenge, especially because the data is not as good as we'd like it to be. You know, we'd like to have these sensors at the center of the galaxy, probing these things in detail with very fine spatial resolution. but instead we're limited to these like tiny cameras orbiting very far from the center of the galaxy trying to get a glimpse like imagine you were trying to understand what was happening in manhattan and all you had was like a camera in indiana it'd be pretty tricky yeah especially with all those buildings it'd be hard to kind of see what's going on in between there so it sounds like maybe we just need to send a pro to the center of the galaxy right figure out what's there you know and just
Starting point is 00:52:11 wait 50,000 years or so yeah some poor graduate student is going to wait 50,000 years to defend their thesis. I'll get paid for that. I could get paid for that while I'm doing this podcast. Sounds good. I mean, as long as we're double dipping. Are your checks going to come from the center of the galaxy because you might be waiting a while. No, no, no. They're going to come in a dollar bill emojis. They're magically transforming to cash into my Venmo or the new X app. Quantum cash entanglement. There you go. I'll be rich and not rich at the same time. I hope your finances don't collapse. All right. Well, another reminder that there are still humongous mysteries out there in the universe and that there are scientists out there actively
Starting point is 00:52:52 searching for the answers, searching for it, trying to find ways to study it, and reveal to the rest of us what its true nature is. So remember that dark matter is really a whole suite of ideas. It's not just like a blank check placeholder for things we don't understand. It's an empty chalkboard for us to fill in with details and scientists are constantly coming up with ideas for what dark matter might be and then being creative about how we might discover it. because we hope one day to fill that chalkboard in with something we really do understand. Does that mean you have to call it Dark Matters or Darks Matter? These are the types of questions that I get paid to think about from multiple people.
Starting point is 00:53:31 Sounds good. Sounds like you are qualified to answer that question. As are we all. All right. Well, we hope you enjoyed that. Thanks for joining us. See you next time. Thanks for listening and remember that Daniel and Jorge Explain the Universe is a production of IHeartRadio.
Starting point is 00:53:54 For more podcasts from IHeartRadio, visit the IHeartRadio app, Apple Podcasts, or wherever you listen to your favorite shows. us how to spend our own money. No thank you. Instead, check out Brown Ambition. Each week, I, your host, Mandy Money, gives you real talk, real advice with a heavy dose of I-feel uses, like on Fridays when I take your questions for the BAQA. Whether you're trying to invest for your future, navigate a toxic workplace, I got you. Listen to Brown Ambition on the IHeart Radio app, Apple Podcast, or wherever you get your podcast. Hi, it's Honey German, and I'm back with season two of my podcast. Grasias, come again.
Starting point is 00:54:48 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. I haven't auditioned in like over 25 years. Oh, wow. That's a real G-talk right there. Oh, yeah.
Starting point is 00:55:03 We'll talk about all that's viral and trending with a little bit of cheesemeter and a whole lot of laughs. And of course, the great bevras you've come to expect. Listen to the new season of Grasias Come Again on the IHeart Radio app, Apple Podcast, or wherever you'd be. Get Your Podcasts. It's important that we just reassure people that they're not alone, and there is help out there. The Good Stuff podcast, Season 2, takes a deep look into One Tribe Foundation, a non-profit
Starting point is 00:55:30 fighting suicide in the veteran community. September is National Suicide Prevention Month, so join host Jacob and Ashley Schick as they bring you to the front lines of One Tribe's mission. One Tribe saved my life twice. Welcome to Season 2 of The Good Stuff. Listen to the Good Stuff podcast on the IHeart Radio app, Apple Podcasts, or wherever you get your podcast. This is an IHeart podcast.

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