Daniel and Kelly’s Extraordinary Universe - Could the Universe be shaped like a donut?

Episode Date: June 7, 2022

Daniel and Jorge talk about how much dark chocolate can fit in Universes of various shapes and sizes. See omnystudio.com/listener for privacy information....

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Starting point is 00:02:06 From Mary Mary to Jennifer Hudson, we get into the soul of the music and the purpose that drives it. Listen to Culture raises us on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. Hey Horne, if you were designing a universe, would you make it the shape of a snack food? Hmm. It's a very specific question, Daniel. Can I make it like a Cheeto shaped or Dorito shaped? Hey, if you're making a universe, there are no rules.
Starting point is 00:02:41 Ooh, I can go nuts or bananas? Hey, can I make the universe banana shaped? How about you? I think instead of going for fruity inspiration, I might draw my inspiration from chocolate. Hmm, what shape is chocolate? Well, you know, I like my universe. the way I like my chocolate. Flat, dark, infinite. You make it sound a little inappropriate there. Isn't the universe expanding also? Is that due to dark chocolate energy? That's also the reason
Starting point is 00:03:08 that I'm expanding. Are you going to be shaped like a banana soon? I'm going to be the size of the universe eventually. We all have a dream. Hi, I'm Jorge. I'm a cartoonist and the creator of PhD comics. Hi, I'm Daniel. I'm a particle physicist and a professor of UC Irvine. And I really do feel like I have an infinite appetite for dark chocolate. Infinite? Wow, that's a lot. You know, infinite's no joke. It means you can eat it forever all the time. Yeah, I feel like I've never reached the limit, you know.
Starting point is 00:03:49 Somebody puts a plate of chocolate there. I just keep snacking on it. And eventually they've got to take it away. So I've never reached the point where I'm like, stop. Sounds like you haven't tried hard enough, Daniel. I need to do more experiments, that's what you're saying. That's right. You need to explore the whole range of possibilities, the upper limits and the lower limits. There's got to be a boundary, and I am devoted to finding it, wherever the cost.
Starting point is 00:04:13 Even if it causes your beltline to go, to be unbounded. But anyways, welcome to our podcast, Daniel and Jorge Explain the Universe, a production of iHeard radio. In which we snack our way to an understanding of the craziest questions of the universe. We try to take bite-sized pieces out of some of the biggest questions in the universe. How big is it? What shape is it? Where does it come from? Where is it going to end?
Starting point is 00:04:37 What is it made out of? And fundamentally, how does it all work? We talk about all of these questions and we try to explain all of them to you while you sample your favorite snack food. Yes, it is a very tasty or, as Daniel says, crazy universe. crazy tasty, tasty universe for us to sample and enjoy and savor because it is out there. It's very dark and interesting and full of amazing things that we have yet to discover. Speaking of snack foods, I know that people like to munch on something while they watch TV. Do you think people munch on something while they listen to podcasts?
Starting point is 00:05:07 Wait, I thought people fell asleep while listening to our podcasts. Are they eating and sleeping at the same time? Isn't that dangerous? I don't know. Do they fall asleep with their hand in the Cheetos bowl or something? I'm sure there are people who snack while listening to us. I mean, I wash dishes while listening to podcasts. Well, I wondered if the crunching would interfere with they're listening.
Starting point is 00:05:25 Well, anyway, let us know if you have a favorite Daniel and Jorge snack food. Maybe we can get them to sponsor an episode. Yeah, it's great. I mean, you're feeding your stomach and your mind at the same time. You're expanding in all directions everywhere. That's good episodes on dark energy funded by dark chocolate makers. That's no joke, Daniel. We could do it.
Starting point is 00:05:45 Yeah, exactly. Tap into some of those Swiss chocolate funds. Yeah, tapping to that big chocolate money. But anyways, it is a pretty interesting universe out there that we can see from our little perch out here and then sitting on top of a round rock in the corner of the Milky Way galaxy in a small corner of the gigantic universe that we are surrounded by. And even though we are stuck on this rock so far, we can still ask some of the biggest, craziest questions about the whole universe, about what's going on super duper far away. Because, of course, we can look out into the universe. Sort of like we're trapped in a tiny lighthouse and we're looking out at the horizon
Starting point is 00:06:22 and wondering what's going on over there. We can't go visit it, but it's sending us messages that let us find answers to some of our biggest question. Yeah, it's pretty amazing that from our little point of view here in the little rock floating out in space, we've managed to know so much about the universe and what's out there. But you've got to kind of wonder what else is out there or what happens if you keep going out there in space?
Starting point is 00:06:43 What are you going to encounter? and what is the overall shape of the universe? I think it's a great metaphor for our curiosity. You know, we think about what's going on on on our planet, what's going on in our solar system, what's going on in the galaxy. No matter how far you explain, people will always wonder what's going on further than that, right? There's no limit to our curiosity, just like there's no limit to my capacity to eat dark chocolate.
Starting point is 00:07:09 No matter how far you explain, people will want to know what's past the edge of the universe. One of those habits seems healthier than the other, Daniel. I think they're tied together. I think dark chocolate fuels my curiosity. What does your doctor say about this type of curiosity? This is why I stock going to doctors, really. You are a doctor. So really, you don't need another doctor.
Starting point is 00:07:31 That's right. I tell myself to take off my pants because I no longer fit into them. But I think the two questions are connected, you know. Could there be an infinite amount of dark chocolate in the universe for me to eat? Only if the universe is literally infinite. I see. You're saying we're sort of like humans are kind of like eternal busy buddies. You know, we're always wondering what's going on out there beyond the horizon. Yeah, exactly. We want to know what's just beyond our ability to understand.
Starting point is 00:07:57 We'll never be satisfying when go, you know what, 100 billion light years, that's enough for me. There's always going to be somebody who wonders, but what's past that? What if you kept going? And I think the reason for that is that the universe and history of science is filled with crazy surprises. Every time we've looked further than we imagined, we found crazy stuff. Think all the way back to Edwin Hubble, discovering that there are other galaxies out there. What a mind-blowing realization to think it's not just our galaxy sitting in space, but that there are hundreds, thousands, trillions of other galaxies.
Starting point is 00:08:29 That's the kind of realization we're going for. Yeah, it's pretty mind-blowing. And so far we can see pretty far out there into the universe. We can see up to about 45, 46 billion light years. That's as far as we can see, right? That's as far as humans are able and can see, right? Because of the limitations of the speed of light. Yeah, it's a bit of a subtle question how far we can see in the universe.
Starting point is 00:08:51 You might imagine it would be the age of the universe times the speed of light, that photons would be racing through space to us, and then we couldn't see anything past 13 or 14 billion light years away. But because the universe is expanding, some of the stuff that sent us photons a long time ago is now much, much further away. And so we can see light from things that are now very, very far away, out to about 45 billion light years. And eventually, we'll even see out to about 62 billion light years. Yeah. So that's kind of as far as we can see.
Starting point is 00:09:23 Like that's the range of our vision as human beings in this universe. But I guess, like you say, there are people who wonder what's beyond that? You know, if I keep going past 65 billion light years, what am I going to find? Am I going to hit a wall? Is this the universe going to go on forever? or is it going to do something even crazier? Yeah, well, put me in that category. I'm not satisfied to only see 62 billion light years away.
Starting point is 00:09:47 I want to know all of it. I want to know what's beyond that. I want to know if it goes on forever, if it curves on back on itself, if there's some huge cosmic store of dark chocolate just past the edge of our vision. That's your carrot, Daniel. You know, the carrot that's driving you to do science.
Starting point is 00:10:03 You just want to discover dark chocolate everywhere, even among the fundamental particles. You want to know if there's a dark chocolate. Yeah, there could be a secret dark chocolate reservoir past the edge of the observable universe. You know what, in my next grant, I'm going to put funds for dark chocolate. And I'm going to argue that it's essential for doing science. At least for Daniel, for Daniel to do science. You need a little motivation in the morning.
Starting point is 00:10:25 Well, you know, there is a clear correlation between chocolate consumption and Nobel Prize winning. I'm not saying it's causal, but there's a correlation. So, you know, when I do apply to the Nestle Foundation for chocolate research, then I think I'm going to put that in. There is a causation, I think. You know, I think winning Nobel Prizes makes you hungrier for chocolate, right? There's something about that, you know, northern European, you know, flare
Starting point is 00:10:46 that makes you crave the chocolate. I don't know. I think it works either way. If you win the Nobel Prize, you celebrate by eating chocolate. If you don't win the Nobel Prize, you console yourself by eating chocolate. I see. So the correlation doesn't make sense
Starting point is 00:10:58 to your physics, at least the way you do it. Not the way that I eat chocolate. But it is an interesting question. What's out there beyond the universe, beyond the 65 billion light years that we might be able to see someday? Are you going to hit a wall? Is it going to come around? What is the size and shape of the universe?
Starting point is 00:11:14 And I love thinking about this question, the shape of the universe, because it feels like something really deep and fundamental. It's something that must be like written into the real source code of the universe. It's not just like, oh, where is a planet or where are there aliens, things that are affected by randomness. There's something which is a deep truth about the universe. It's something which like reveals. its nature. Yeah, you're basically asking the biggest question you can ask, right? Like,
Starting point is 00:11:40 when you're asking about the size and shape of the universe, you're asking, what is this shape of the entire universe? Like, it has to encompass all of it, not just like a part of it, all of it. Yeah, I guess you can ask, what is the shape of the multiverse? That might be a bigger question. Oh, what? You just blew my mind. What is the shape of the multiverse? It's shaped like a Marvel movie. It's shaped like a dollar bill, I'm pretty sure. shaped like the money they're raking in. I hope they're spending some of that money on chocolate to celebrate. But it is the biggest question we can ask,
Starting point is 00:12:11 and it's a question we don't know the answer to, right? I mean, first of all, we can't see out to the edge of the universe, right? At least we haven't seen an edge to it. And so it's kind of a weird question to ask, what is the size and shape of the universe if we can't see all of it? It's like sitting in the middle of the United States and asking what is the shape of the United States if you've never been to or can ever get to the coast.
Starting point is 00:12:32 That's right. But although it seems impossible, science always finds a way to like take the first nibble off of the question to think, well, well, what can we do? If we can't answer the entire question directly, then, you know, can we find some way to limit the possible answers? What can we do with our limited data and our limited view of the universe? And to me, it's incredible what we have learned, what we have been able to rule out about the universe just from looking around. Wait, are you saying we can just ask the universe what its size and shape? You know, I emailed the universe and invited to be on the podcast, but it hasn't answered yet. And so I'm going to have to resort to the classic way, which is doing physics experiment,
Starting point is 00:13:11 which is basically asking the universe question. Interesting. Yeah, I guess if you ask anyone by email what their size and shape is, you probably won't get an answer. I got a cease and desist from the universe legal department. Yeah. Stay away from me. Blocked. Blocked by the universe. Wow, that's harsh. But it is an interesting question. And so today on the podcast will be asking, is the universe shaped like a donut?
Starting point is 00:13:41 And does it taste like a donut too, Daniel? This seems like a very specific question. It's a specific question, an idea motivated by some hints we've seen in some recent studies that suggested that maybe the universe is chocolate filled after all. Wait, chocolate filled or shaped like a donut or like a donut with chocolate in it. Exactly. The universe might be a chocolate filled donut in the end. I don't think I've ever heard of a chocolate-filled donut.
Starting point is 00:14:05 Usually chocolate is on top. You've never heard of a chocolate-filled donut. Are you serious? Well, if it has something in the inside, then it's not a donut, is it? Oh, man. What's a jelly-filled donut then? Is it a jelly-filled-not-donut? It's a jelly-filled cake.
Starting point is 00:14:18 It needs to have a hole in the middle, right, to be a donut, doesn't it? Oh, man, this is turned into a food argument podcast. I hear those are more popular than the science podcast. Let's roll with it. We've done the murder mystery podcast recently, and now we're doing the food. argument podcast. Absolutely. I think there's lots of different shapes donuts can be. I think the classic shape, you know, is basically a torus with a hole in the middle, but you could still put chocolate inside that torus, right? Oh, you mean a long, like the ring of it, you can stuff it with
Starting point is 00:14:47 chocolate. Yeah, a ring of chocolate. Why not? Sounds delicious to me. Sounds like a heart attack. Well, we'll see if the universe agrees with me or with you by the end of the episode. But anyways, apparently it's a possibility that the universe could be shaped like a donut, which sounds both bellicious and filling. And so that's the question we'll be trying to answer today. And so as usual, we were wondering how many people out there had thought about equating the universe with a treat like a donut. So thanks to our ever-rotating group of volunteers who answer these questions for us on the podcast. It's always fun to hear your answers and it gives us a sense for what people are thinking.
Starting point is 00:15:23 If you'd like to participate for a future episode, please don't be shy. I know you're out there waiting for an invitation. Just write to me to questions at Danielanhorpe.com. And Danny will send you a donut if you answer the question, right? Sure, a digital donut. A little emoji donut. Well, think about it for a second. Do you think the universe is shaped like a donut?
Starting point is 00:15:43 It was what people had to say. I think the universe could be shaped like a donut, and it could be that we just don't see all of the universe from our vantage point. But I doubt that it is because I would think we would see some kind of evidence of it in the microwave background. So from that, it really appears that the universe does not have curvature to it. I don't think the universe is shaped like a donut unless initial expansion was not uniform in every direction.
Starting point is 00:16:17 I would guess it's more likely to be a hollow sphere. Yeah, I mean, could it be? Is an interesting question. Yeah, I mean, I imagine it could be. I think I've heard about this before. I remember at some point somebody, maybe in a documentary or something, saying that if you look straight forward. If you were able to like see into infinity, you would look at the back of your head, which I guess if you were on a donut, you could probably do that if space was like
Starting point is 00:16:45 sort of bent like that. I don't think the universe is shaped like a donut. I think if it was, we would have noticed by now because there'd be a lot less photons and activity coming from the center of the donut. I think so long as information is consistently available, you know, across the entire universe, it really doesn't matter what the shape is. And as long as time and space are concentric, I think the universe can be any shape. And there are probably universes of all shapes and sizes out there. Frankly, I think that the universe could be shaped like anything, and it wouldn't surprise me. there's this idea that you know you start in one place and you go in one direction and then
Starting point is 00:17:34 eventually you're just back at that place and yeah that fits donut shape to me is me all right pretty wide range of answers some people seem skeptical some people are like sure why not the universe is is weird and surprising you could be shaped like anything exactly and some people even commenting that donuts have jam inside of them and so they're arguing i think they agree with you you know that the shape we're talking about is more like a bagel than a donut Interesting. Whoa. Should we rename the episode then? Could the universe be shaped like a bagel? Well, the question then is, can you put chocolate inside of a bagel? Obviously, yes, Daniel. You can put chocolate inside of anything.
Starting point is 00:18:09 All right, then I'm fine with it. What I call it whatever, as long as you put chocolate inside of it. Wow. Man, you're really hungry here today, Daniel. Have you had your daily dose of chocolate yet? I'll reward myself after the podcast. Assuming this podcast is not infinite, I guess. So yeah, so let's get into this idea of the shape of the universe. it's kind of weird to think about the universe having a shape, right? Because the universe could be infinite. And even if it's not infinite, are you saying like the walls of the universe are shaped like a donut? What exactly do you mean by the shape of space?
Starting point is 00:18:38 So the shape of space refers to basically how the universe is connected on the really, really big scale. You know, we are used to thinking about space as like something we are floating in. And we're also used to thinking about space as like maybe being curved. General relativity tells us that mass and energy. You know, all this kind of stuff can curve space. That's sort of a local curvature. But, you know, if you have curvature in space, if space bends in some way, then you can imagine putting it together into some big shape.
Starting point is 00:19:08 Like if space doesn't curve, if it's flat, it can make an infinite sheet. That would be the shape of space. If space does curve, you can imagine it being like a sphere or a donut or some other weird shape. So the curvature of space is connected to this other question of the shape of space. curvature is sort of local. The shape of space is sort of global. It's asking like how is all of space put together? Think in two dimensions for a moment because it's easier. Imagine you have a bunch of rings and you have to connect them together into a 2D surface. You could loop them together into a flat sheet or you could make it into a sphere or something else. These are different shapes
Starting point is 00:19:47 because they have fundamentally different properties. And mathematically speaking, two shapes are fundamentally the same if you can smoothly morph one into another. So two different shaped spheres or even a sphere and an ellipsoid are basically the same shape. But a sphere and an infinite flat sheet are not the same. One is infinite. The other is finite. There are other shapes like ones with a hole in it, like a donut that are not the same as a sphere or a flat sheet. That's the meaning of shape in a global sense, which is related to, but different from curvature in a local sense. I see. And I guess just to be clear, you actually mean space time, right?
Starting point is 00:20:31 Because when you're talking about gravity, kind of bending or giving space curvature, you're actually talking about the curvature of space time, right? You kind of have to take time into consideration as well. Well, we do think about how the shape of space evolves with time. And the shape also contributes to how the universe expands or contracts or doesn't. So yes, this is a dynamical thing, the shape of the universe, The curvature of the universe can change, although its fundamental shape cannot. Yes, it is interesting to think about it as a function of time.
Starting point is 00:20:59 Right. And it's kind of interesting that you related to this idea because I know we've talked a lot in this podcast about how gravity and energy kind of bends space time in the sense that, you know, we're not going around the sun because it's pulling on us. We're going around the sun because the space time around it is sort of shaped like a bowl. And so we're kind of stuck in this loop around it. Is that sort of what you're saying, like on a global or universal scale, does the universe have some sort of like curvature to it? It's a really fascinating idea that, you know, space is curved, that gravity is not like a force the way we think about other forces, but instead it's a fictitious force. It's a force that appears to act because we can't see that space is curved. Like if I look at a piece of space, I can't tell you, is it curved?
Starting point is 00:21:41 But I could shine a light through it. And if I see where that light goes, then I can tell you whether space is curved. So we can see the effect of curved space, even though we can't see the curvature directly. So now imagine you're building a universe and I'm giving you pieces of it, right? And each piece has curvature. So if I only give you curved pieces, what kind of big universe shape can you build? Well, you can't build like an infinitely flat space, like a huge sheet. But you could build like a sphere or a circle or a donut or something else that has a curved surface.
Starting point is 00:22:12 So the building blocks of the local curvature I'm giving you, do constrain the kind of overall. all shape that you can build for the universe. I think what you're saying is, it's kind of like, you know, if I measure the land around me and I see that the land sort of curves around me downwards or towards the center of the earth, then it kind of tells you that me the whole earth is round. Exactly. If you can measure the curvature on the surface of the earth, then you know that the earth can't go on forever or can't be flat because you see that it's curved, right?
Starting point is 00:22:40 If you imagine that the rest of the earth is curved the way the piece you're standing on is curved, then that suggests that probably it's a big sphere. Although, you know, it could also be a donut. Or I guess it could also be kind of like a dome, right? A dome goes on forever. Like if you're standing on a parabola at the bottom of a parabola, you think it's curved, but it could keep going forever, right? Mathematically, a parabola has the opposite curvature of a sphere. But yeah, parabola is an open construction. And so you can have curvature and still have an infinite shape, so that curvature is negative instead of positive. But that's a detail. Right. So you're saying that, you know, somehow we can't see the entire universe, but maybe by measuring the curvature around us, we could maybe, you know, get a sense or an idea of what the overall shape of the universe is.
Starting point is 00:23:27 Exactly. And what we want is the curvature on the biggest scale. We don't really care about how much the sun is bending the shape of space in our neighborhood. That doesn't affect the overall shape of the universe. We want to know, like, how much is all the stuff in the universe bending the shape of space? What shape of space is that? consistent with. Just in the same way of like if you want to measure the surface of the earth, you could be standing locally on something flat or something pointy or, you know, in a bowl or something doesn't change the overall structure. So when we measure the curvature of the universe, we want to make measurements on as big a scale as possible to avoid like the local fluctuations and deviations. Are you saying that the universe might have a curvature to it or that space might have a curvature to it without stuff in it? You know, like or are you saying space
Starting point is 00:24:14 has a curvature to it because there's stuff in it. This is a really important point and a subtle one. The universe has some curvature and some shape, right? If the curvature is positive like a sphere or it's flat like an infinite surface or it's negative like a parabola as you described. And that just is part of the nature of the universe. And you can put stuff in the universe and that can change the amount of curvature. You can make the universe more or less curved by putting stuff into it.
Starting point is 00:24:42 But you can't change the fundamental nature of the universe. curvature or topology of the universe. You can't like make a sphere universe into a flat universe by putting stuff into it or the other way around. I see because I think, you know, there's sort of two things, right? There's stuff and energy and then there's space. Those are two kind of separate things. And so you can imagine an empty universe where it's just space or like if you took out all the stuff and energy in our universe, we would just be left with the space we have. And so you're saying like without any stuff in it, what is the shape of that space? Does that space have? curvature or is it totally like flat and even yeah although we're interested in our universe which does
Starting point is 00:25:20 have stuff in it and the stuff affects the amount of curvature you know for example one of the things in our universe is dark energy which we don't understand at all but it's expanding the universe that tends to decrease the curvature of the universe it like stretches everything out imagine you're like the little prints you're standing on a tiny little planet and then that planet expands to be huge the curvature you experience decreases the amount the planet curves away under you decreases so the stuff that's in the universe can affect the amount of curvature, but it can't affect the shape, right? Like you can't take a curved universe and put stuff into it and make it flat. You can contract it. Like you put a bunch of mass into a universe. That's a sphere. It's going to make that collapse
Starting point is 00:25:58 into a point. Interesting. So you're saying that if I take out of all the stuff and energy in the universe, I would be left with space. And that space could be in the shape of a sphere or a donut or something. And the stuff in it wouldn't be able to change that. Wouldn't be able to change that. And it's connected to this other idea that, you know, the shape of space. space, it's topology, it's global curvature, plus the amount of stuff, the matter, the density, and the dark energy, all those together determine, like, whether the universe is expanding or contracting. This is one element of that. We're talking about the shape of space, which is not something that can be changed by dark energy or dark matter or the arrangement of stuff. It's just
Starting point is 00:26:33 like it's something that's deep and true about the universe itself. It's just baked in. I mean, it's its shape, right? Like, you know, nothing but the universe can change its shape. Yeah, and shape in a very specific way, right? You know, we're not talking about size. You can have a universe that's a sphere and it can grow or it can collapse. So in that sense, the universe can change, but it can't change from like a sphere to an infinitely flat universe or to a parabolic universe. That kind of thing can't change. Right. And do you know that sort of mathematically or how do you know that it can't change? Well, I guess we know that mathematically, but you can also just think about it intuitively, like, how could you take a finite universe, which is a sphere and suddenly transform it into an infinite
Starting point is 00:27:14 a flat plane. Or you can imagine a sphere even growing, you know, arbitrarily large, but then how do you suddenly transform that smoothly into a flat universe? You know, the universe can change. It can't evolve, but it has to happen in a smooth way. You can't have like a sudden jump where the universe is all of a sudden completely different. This is like a basic element of the nature of the universe. It doesn't seem like you could change it from one moment to the next. All right. Well, let's get into what are the possible shapes and curvatures of the universe and what it all. It all. It all. It doesn't seem like. means. But first, let's take a quick break. I'm Dr. Joy Harden-Bradford, and in session 421 of therapy for black girls, I sit down with
Starting point is 00:27:56 Dr. Ophia and Billy Shaka to explore how our hair connects to our identity, mental health, and the ways we heal. Because I think hair is a complex language system, right, in terms of it can tell how old you are, your marital status, where you're from, your spiritual belief. But I think with social media, there's like a hyper fixation and observation of our hair, right? That this is sometimes the first thing someone sees when we make a post or a reel is how our hair is styled. You talk about the important role hairstylists play in our community, the pressure to always look put together, and how breaking up with perfection can actually free us.
Starting point is 00:28:35 Plus, if you're someone who gets anxious about flying, don't miss session 418 with Dr. Angela Neil Barnett, where we dive into managing flighting. anxiety. Listen to therapy for black girls on the Iheart radio app, Apple Podcasts, or wherever you get your podcast. Have you ever wished for a change but weren't sure how to make it? Maybe you felt stuck in a job, a place, or even a relationship. I'm Emily Tish Sussman, and on she pivots, I dive into the inspiring pivots of women who have taken big leaps in their lives and careers. I'm Gretchen Whitmer, Jody Sweeten. Monica Patton. Elaine Welteroth. I'm Jessica Voss. And that's when I was like, I got to go. I don't know how, but that kicked
Starting point is 00:29:13 off the pivot of how to make the transition. Learn how to get comfortable pivoting because your life is going to be full of them. Every episode gets real about the why behind these changes and gives you the inspiration and maybe the push to make your next pivot. Listen to these women and more on She Pivots now on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. I'm Simone Boyce, host of the Brightside podcast, and on this week's episode, I'm talking to Olympian World Cup champion and podcast host Ashlyn Harris.
Starting point is 00:29:47 My worth is not wrapped up in how many things I've won. Because what I came to realize is I valued winning so much that once it was over, I got the blues and I was like, this is it. For me, it's the pursuit of greatness. It's the journey. It's the people. It's the failures. It's the heartache.
Starting point is 00:30:09 Listen to the bright side on the IHeart Radio app. Apple Podcasts, or wherever you get your podcasts. And here's Heather with the weather. Well, it's beautiful out there, sunny and 75, almost a little chilly in the shade. Now, let's get a read on the inside of your car. It is hot. You've only been parked a short time,
Starting point is 00:30:32 and it's already 99 degrees in there. Let's not leave children in the back seat while running errands. It only takes a few minutes for their body temperatures to rise, and that could be fatal. Cars get hot, fast, and can be deadly. Never leave a child in a car. A message from NHTSA and the Ad Council. All right, Dan, we're talking about the size and shape of the universe,
Starting point is 00:30:59 which seems a little rude to be asking these questions about the universe. Maybe the universe is very bashful about these things. Physics asking rude questions since 1584. Being nosy. about people's size and shape. Exactly. Upsetting the apple cart since forever. That's our goal, you know.
Starting point is 00:31:16 We don't care if the truth is offensive. We just want to know. Discarding with social conventions since the beginning of time. As if we understood social conventions, right? That's one reason we went into physics because we just don't know how to do the other stuff. Oh, man. Your meetings must be pretty interesting or not, man. Or me or not, you know, a world without subtlety might be a little boring.
Starting point is 00:31:40 No, that's a fun stereotype, but, you know, physicists are social creatures. I work in a collaboration of thousands of people and we have lots of meetings and politics and have to deal with each other and, you know, people work together and don't work together and it's all sorts of stuff. Exactly the same way you find in every other field of human endeavors. Right, right. It is a human endeavor. And we were talking about the size and shape to the universe and you were telling me that, you know,
Starting point is 00:32:04 the universe can have a shape even if I take, like, if I take out all the stuff and energy in it, put it somewhere, I don't know where, but you put it somewhere. this universe that's left over would have a shape to it. What exactly does that mean a shape? Like, does it mean it has walls and a boundary, like edges to it? It tells you how space is connected. I think about space, not as just like where stuff happens, but I think of it sort of like a fabric and it's woven together.
Starting point is 00:32:30 And if I move to the left, then I'm moving into a new bit of space. And then you can ask like, well, what happens if you keep going? You just encounter new space or potentially, space could be connected in such a way that if you keep going, you come back to where you started, right? Sort of like a Pac-Man universe. And so that's entirely possible. And that tells you something about the shape of space. So when we say like, what if space was a sphere? What do we mean by that? We don't mean that space is literally a 3D sphere. We're talking about the surface of the sphere, the 2D surface of the sphere as an analogy to our three-dimensional space because it's hard to think
Starting point is 00:33:08 about 3D surfaces of 4D spheres, but if you're on the surface of a sphere, that surface is finite. It doesn't go on forever, but it also doesn't have an edge. That's an example of how space could be connected. So really, we're talking about, like, how to weave bits of space together into a larger fabric, and then what is the shape of that fabric? Right, but I think it sounds to me like you're making an assumption about the universe, which is that it doesn't have an edge or a wall to it, right?
Starting point is 00:33:36 Like it doesn't seem like you're considering that possibility that if I just hop on a spaceship and I keep going for, you know, 90 billion light years, eventually I'm maybe going to hit a wall. Like that's not a possibility that physicists seem to consider because maybe it doesn't make sense to you. That's a possibility I'm totally open to considering. You're right that it doesn't make sense to me. It would break a lot of things and be very, very odd. That would make it super fun and interesting to discover. I wouldn't think it's something that's likely as a description of our universe because it would mean that one point, part of the universe is very different from another part of the universe. The edge would have to have
Starting point is 00:34:10 a different nature than the rest of the universe. And so far what we've seen is that every part of the universe sort of seems to be the same as every other part. But, you know, maybe it's like we're in the very center of a huge lake and we just can't see the edges, but they are there. It's possible that the universe has edges that there's another kind of space, an edgy kind of space that's different. That's a possibility. We can't rule it out that it would be weird. Right, right. So then when we're talking about the shape of space, I mean, if it does have walls and a boundary. It could be shaped like anything, right? It could be shaped like a cube or a banana or you know, like being trapped inside of a banana. That could be one way to talk about the shape of the
Starting point is 00:34:45 universe. But I think for our discussion today, what do you actually mean by the shape of the universe is like let's assume that that's not possible. Like let's assume that the universe can't have walls or boundaries. Then what are the possibilities left? Yeah. And so if you assume that every point in space is the same as every other point, right? You have like one kind of a Lego piece and you have to build a whole universe with just that one Lego piece, then what are your options? So, for example, if I only give you those flat pieces of Lego, then what can you do? You could just make a big flat sheet, right? Just like quilt together space so that every piece is just next to other pieces adjacent to it and nothing is more complicated. Space just goes on forever,
Starting point is 00:35:26 totally flat. That's one simple idea for what space might be. Right, because I think, you know, maybe a lot of people might be confused with this because, you know, if you tell me that the universe can have boundaries or like walls or edges to it, then to me I would think that it has to go on sort of forever, then to me it would seem like the only possibilities for the universe to be infinite and have no shape. But I think, you know, physicists think about it differently, like it could still be sort of infinite and continuous
Starting point is 00:35:52 without bandaries and still have a shape. No, I think you're right. If it's flat and it's infinite, that is it doesn't repeat and there's no special edges to it, then it has to be infinite. I can't think of another way to arrange. space. It is possible, though, for space to be flat and not infinite, right? Imagine the Pac-Man universe or the Asteroids universe where at some point space just repeats. You know, you get to some
Starting point is 00:36:16 point in space and it just is now connected to a spot you've already been. Without any curvature, right, it's just like the way space is. It's sort of the same way we talked about for wormholes. Space can have non-trivial connections. Like you can connect this bit of space to that bit of space and just say these two bits are now next to each other, meaning you can step for one to the other, even though in the larger fabric of space, they seem to be far apart. In that same sense, you could have like a whole seam where you connect like a whole line of space to another whole line of space, effectively making like an infinitely sized wormhole. I think what's interesting is that the idea that space can have no, it could have no boundaries,
Starting point is 00:36:54 no walls, but still have a shape. And I think what you're telling me is that the one way it can do that is if space sort of wraps around itself. Sort of like, if I keep going in one direction, I eventually come back from the other direction. Like somehow space is curved or connected to itself in a strange way so that I can keep going forever,
Starting point is 00:37:15 but I sort of keep going around circles. And in that case, the universe sort of has a shape, but it has no edges to it. And there's two possibilities there. One is space is actually curved, sort of like a sphere, right? And so it's natural to put it together in that way. that space is curved and finite
Starting point is 00:37:31 and if you keep going in one direction you come back to where you are. There's another possibility which is that space is flat. It doesn't have curvature and yet it doesn't have edges and it's finite and that's like the asteroids
Starting point is 00:37:42 or the Pac-Man universe where without space being curved it's just connected in that way. That's why local curvature is a little bit different from this question of like global topology, the connectedness or shape of space.
Starting point is 00:37:55 Right, right. But maybe let's take a step back and break it down. So it's possible for the universe to be sort of continuous all the way through, no boundaries, no edges, but still be final. And you're telling me, I think, that there are different ways in which that can happen. So one of those ways has to do with curvature and the other one doesn't. So let's maybe break it down a little bit more about what this idea of curvature is.
Starting point is 00:38:16 Like, what does curvature mean for you? Like, for me, curvature means that the ground is uneven or has a slope to it. But what does it mean in terms of space? In terms of space, locally it means what is the path of a photon? If you shine a laser beam through a chunk of space, where does it go? And if space is curved, then you can't see that curvature, but it affects the flight of the photon. And so the photon will bend. It's taking what's actually the shortest distance through that space, right?
Starting point is 00:38:45 Because photons always take the shortest path. But the shortest path is now something that looks bent to you because you can't see the relationships between those bits of space. Remember, the curvature of space is intrinsic, meaning it just changes the relative distances between bits of space. So that's what I mean by the curvature of space. I mean like the path of a photon through that piece of space. And again, I think you mean space time, right? Or I guess do you lump it all together?
Starting point is 00:39:11 Yeah, well, relativity definitely mixes space and time together. There's a lot of connected effects there. But you know, space and time are also different. You know, space has these properties that time doesn't have. And here we're talking specifically about the spatial part of it. of space time. But yeah, you can't really think about space without thinking about the 4D structure that it sits in, which is space time. Well, another thing that I think I've read is that, you know, this idea of curvature is not just about whether one foot, like if you shoot one photon and it
Starting point is 00:39:37 sort of leans to the right or to the left, it's more about like if you shoot two photons, do they curve away from each other or towards each other? That's really more about the curvature of space, right? Yeah, one way to measure the curvature of space is to look at the path of two photons. Another way which is equivalent is to like draw a triangle and ask like what are the angles of that triangle? If you draw a triangle on a flat surface, then its angles add up to 180. If you draw a triangle on the surface of a sphere, its angles are bigger than 180. And that's the same notion, right? If you shoot two photons and they have to move along the surface of a sphere, then they can appear to curve towards each other, for example. And if you're on a parabola,
Starting point is 00:40:16 then they appear to curve away from each other. And it's equivalent to saying that a triangle on that surface as angles less than 180 degrees. Well, it's kind of strange to think about spheres and convert between 2D and 4D and 3D. But I think what you're saying is like if the curvature of the universe is flat or at least around this, things are flat. It means that if I shoot two photons, they're not going to curve or at least they're going to curve together maybe. But they're not going to sort of move away from each other or move towards each other, right?
Starting point is 00:40:45 They're just going to keep going in the same direction, side by side forever. That's what it means for space to be flat, right? that's a way to test it in flat space two photons moving in parallel will not approach each other whereas in curved space two photons initially moving what appears to be parallel to you will either approach each other or divert from each other same way as if you're on the equator of the earth which is a curved surface and you and your friend both walk north do north which feels like you know we're moving parallel you'll notice that you get closer and closer to each other because eventually you're going to hit the same point so motion constrained along a curved
Starting point is 00:41:19 surface or motion through curved space can make things that initially were parallel moved towards each other. So the earth is not flat. The earth is not flat. Newsflash, it's not flat. Right? I mean, if the earth was flat and you and I started walking in one direction, we would keep
Starting point is 00:41:35 walking at the same distance from each other all the time. But that doesn't happen on Earth, right? That's one way we know the Earth is not flat. Exactly. Although I don't know what North would mean on an infinite flat Earth, though. I'm sure the Flat Earth Earth Earth has figured that out somehow. All right, so that's a flat universe. And you're seeing a curved universe means that the two photons would eventually either collide or move away from each other forever.
Starting point is 00:41:58 Depending on the sign of the curvature. So if you're on a sphere, for example, then those photons eventually will hit each other. They'll come closer to each other. If you're on a parabola or in 3D, it's called a hyperbolic paraboloid, then they will eventually move away from each other. Right. And that's what you mean by like positive curvature and negative curvature. Like if the universe has positive curvature, then two photons would eventually hit each other, even if you should. and parallel to each other.
Starting point is 00:42:21 And if it has negative curvature, they'll just diverge and never hit each other. Exactly. But that's curvature. What does that tell us about the shape of the universe? Because the curvature of space determines what shapes are possible. Like if the curvature is positive,
Starting point is 00:42:35 like on the surface of a sphere, then you are building up your universe. You can't make a parabola. You can't make an infinite flat universe. You can make a sphere. You could make a donut. You can make a donut with more holes in it. You have to build a universe.
Starting point is 00:42:49 where every piece of space has that curvature and sort of like have it all fit together without any edges there are only a few shapes that are possible the curvature of the universe on the large scales determines the shapes that are possible so if you measure the curvature doesn't tell you the shape it tells you what shapes are allowed I see so you're saying like if it's positively curved everywhere then there's only one sort of shape ish that the universe can be which is a sphere or closed right like something that wraps around itself. Although it could be other shapes than just a sphere like a donut. But note here, there's a bit of a subtle point of geometry. The picture you have in your mind of a donut has lots of spots on it with positive curvature. They sort of bend away from you. But not everywhere on the donut has positive curvature.
Starting point is 00:43:39 There are spots there with negative curvature. And if you talk to professional geometers like mathematicians, they think of a donut is actually like a flat plane. connected on itself like the Pac-Man universe we were talking about. So there's the donut you eat, which has curvature, and then there's a mathematical donut which is actually flat on the surface. And we could also consider more exotic shapes, like a donut with two holes in it. I don't even know what you call that, like a double bagel.
Starting point is 00:44:05 But yes, it couldn't be totally flat if space is curved positively. I see. But if we measured space to be flat, then there's no shape it can be. It has to be infinite, kind of. That's right. If space is flat, then it can't be a sphere. It could still be that weird Pac-Man universe, or as you say, it could have a weird edge to it, right, beyond what we're measuring, but it can't be a sphere or it can't be a paraboloid or a hypobloid or anything like that. So measuring the curvature of space does rule out some possibilities for the shape of space.
Starting point is 00:44:34 Okay, so depending on the curvature that we measure around us and in all space, they'll determine whether the universe is shaped like an infinite sort of space sheet or whether it's shaped maybe close like a ball, like a sphere, or whether it's shaped maybe close like a ball, like a sphere, or whether it's. it has a more interesting shape like a donut. And so let's talk about what we've measured out there, whether the universe is flat or curved. But first, let's take another quick break. I'm Dr. Joy Harden Bradford. And in session 421 of Therapy for Black Girls, I sit down with Dr. Athea and Billy Shaka
Starting point is 00:45:08 to explore how our hair connects to our identity, mental health, and the ways we heal. Because I think hair is a complex language system, right? in terms of it can tell how old you are, your marital status, where you're from, you're a spiritual belief. But I think with social media, there's like a hyperfixation and observation of our hair, right? That this is sometimes the first thing someone sees when we make a post or a reel is how our hair is styled. You talk about the important role hairstylists play in our community, the pressure to always look put together, and how breaking up with perfection can actually free us.
Starting point is 00:45:44 Plus, if you're someone who gets anxious about flying, don't miss session 418 with Dr. Angela Neil Barnett, where we dive into managing flight anxiety. Listen to therapy for black girls on the IHeart Radio app, Apple Podcasts, or wherever you get your podcast. I'm Simone Boyce, host of the Brightside podcast, and on this week's episode, I'm talking to Olympian, World Cup champion, and podcast host Ashlyn Harris. My worth is not wrapped up in how many things I've won because what I came to realize is I valued winning so much that once it was over, I got the blues and I was like, this is it. For me, it's the pursuit of greatness. It's the journey. It's the people.
Starting point is 00:46:29 It's the failures. It's the heartache. Listen to the bright side on the IHeartRadio app, Apple Podcasts, or wherever you get your podcasts. And here's Heather with the weather. Well, it's beautiful out there, sunny and 75, almost a little chilly in the shade. Now, let's get a read on the inside of your car. It is hot.
Starting point is 00:46:54 You've only been parked a short time, and it's already 99 degrees in there. Let's not leave children in the back seat while running errands. It only takes a few minutes for their body temperatures to rise, and that could be fatal. Cars get hot, fast, and can be deadly. Never leave a child in a car. A message from Nitsa and the Ad Council. Have you ever wished for a change but weren't sure how to make it? Maybe you felt stuck in a job, a place, or even a relationship.
Starting point is 00:47:19 I'm Emily Tish Sussman, and on she pivots, I dive into the inspiring pivots of women who have taken big leaps in their lives and careers. I'm Gretchen Whitmer, Jody Sweetie. Monica Patton. Elaine Welter-A. I'm Jessica Voss. And that's when I was like, I got to go. I don't know how, but that kicked off the pivot of how to make the transition. Learn how to get comfortable pivoting because your life is going to be full of them.
Starting point is 00:47:42 Every episode gets real about the why behind these changes and gives you the inspiration and maybe the push to make your next pivot. Listen to these women and more on She Pivots now on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. Okay, Dinah, we are talking about the size and shapes of the universe. and now we're doing something even ruder, which is actually measuring the size and shape of the universe. Like, wouldn't that be rude if somebody came out to me like, hey, I wonder how big you are. Let me measure you.
Starting point is 00:48:17 Well, you know, I think if you're a tailor, for example, you ask somebody to waste size and then you measure it because you want to deliver a suit that fits, not an aspirational suit that they hope to one day fit into it. Oh, I see. Are physicists the tailors of the universe? What kind of suit are we making for the universe? I don't know, but if we ask the universe,
Starting point is 00:48:35 it's size and he gave us an answer, I'd still want to go out and measure just to make. make sure it wasn't being modest. Oh, man, you think the universe is lying to you, maybe. You always got to double check, and then double check your double checks. I guess the universe could have been eating more dark chocolate than it thought, and, you know, its measurements are outdated. That's right.
Starting point is 00:48:53 Maybe in between the time it's sent in its measurements, it had a bunch more snacks. And so, hey, we just want to make sure to make a suit that fits. We were talking about how knowing the curvature space tells you, at least not maybe the total or exact shape of the universe, is tell you kind of what kinds of shape the universe can be, whether it's sort of closed like a sphere or open like an infinite sheet or maybe has some weird shape like a donut or a hyperbola. And so I guess the big question now is how do we measure the curvature of space?
Starting point is 00:49:21 Like how do we measure if it's curving one way or another? Yeah, the best way to do it would be to have a huge triangle, right? To draw at a huge triangle in space and to measure its angles. You know, shoot photons in straight lines between three points. and then measure the opening angles between those photons. And that would tell you, just like if you did that on the surface of the earth, you could literally measure the curvature of the earth because you would measure that a triangle actually has more than 180 degrees in it
Starting point is 00:49:49 if you laid it out on the surface of the earth. So that would be the best way to do it, you know, huge lasers, really, really far apart, deep in space. Oh, I see. You send out three satellites, put it, arrange them in a triangle, and you shoot lasers at each other? Yeah, you make sure they're in a triangle. angle by shooting lasers at each other. This is totally fantastical, right?
Starting point is 00:50:09 You never actually do it. Imagine one satellite in this galaxy and one in an adromeda, one in another galaxy, and they shoot lasers at each other. So, you know, they're lined up, and then you just measure the angles between those lasers. So, like, if I'm shooting an Andromeda from here and I'm shooting at alphas, you know, another galaxy from here,
Starting point is 00:50:25 I would literally just take like a protractor and measure the angle between the lasers that would tell me whether the universe is curved? Yeah, in the same way you could on the surface of the Earth, right? You got two friends, you guys stand in a triangle, and you spool out string between yourselves, you could just measure the angle between those strings, and that would tell you the curvature of the Earth. Same way you could do it with photons deep in space. What you want is a really, really big triangle because the curvature, if it exists, is going to be pretty small.
Starting point is 00:50:53 Just like on the surface of the Earth, you'd want a really big triangle because it's pretty hard to measure the curvature of the Earth in just your bedroom. I see. Well, technically you could do it in your bedroom. you just need like a super precise protractor, right? Yeah, but then you're also measuring the curvature of your bedroom instead of the earth. But if your bedroom follows the perfect curvature of the earth, then yes. And so that's what you'd like to do ideally. Obviously, we can't do that.
Starting point is 00:51:17 So what we have to do is sort of look for existing triangles in space. Like, you know, is there a place where two photons were sent to us from really distant locations and we can sort of reconstruct like an existing cosmic triangle? Mm. So meaning like looking at galaxies or looking at sort of like the background of the universe? Yeah. So the oldest light in the universe is a really helpful resource for this. So we're talking about light from the cosmic microwave background. Back when the universe was really hot and really dense and only a few hundred thousand years old, there was a moment when those particles came together and became transparent.
Starting point is 00:51:54 And we still see light from that plasma glowing. That light is really, really helpful because it's so old. So it's traversed a lot of the universe. And we can kind of put it together in a sort of cosmic triangle to get a sense for whether the universe is curved in one way or another or whether it's flat. Right. And this light is kind of interesting
Starting point is 00:52:12 because it's like the earliest light in the universe. So it's very kind of like primal, right? Like it's sort of like the OG light, like the original light of the universe. Like when it was born, did it have a curvature to it? And you can tell from the, you said the wiggles of this light. What we do is we look in this light for,
Starting point is 00:52:29 lumps. We don't really just measure the angles between things. What we look for is the size of lumps that are evidenced in the cosmic microwave background light. So if you look in one direction, if you look in another direction, you see this light, but it turns out this light has slightly different temperatures if you look in different directions. It's really, really minute. It's like one part in tens of thousands. Mostly it's just the same, but there are these little wiggles. And if you look for the size of those wiggles, like how big is a hot spot or how big is a cold spot, you can use the apparent size of those wiggles to tell you, whether the universe is curved and how it's curved.
Starting point is 00:53:02 Yeah, this is pretty cool because I was thinking about this. It's almost like the universe is acting like a lens, right? Like if the universe is curved in one way, positively, say, for example, and maybe the universe is sort of like a sphere, then the universe could have acts like a magnifying glass, right? So you should see these spots in the background radiation kind of bigger than they actually are. Exactly.
Starting point is 00:53:23 And we have an idea for how big we expect those spots to be, right? That's key. we have some idea for like how matter and dark matter and the photons we're all sloshing back and forth together against each other how big should those lumps be we can predict how big they should be and then we can go and measure how big they are and as you say if the universe is curved then photons for example from really far apart will curve towards each other and so those lumps will appear to be slightly bigger than they actually are because you look in one direction you look in another direction you'll be seeing like two sides of the same lump, but really those edges were closer than what you're
Starting point is 00:54:01 seeing. Space is flat, then the photons are just flying straight. And so that's sort of like a cosmic triangle because you have these like two different sources of light all coming at you. And you can look at the angle basically between those photons and tell whether they've been bent together or bent apart or flown true. Right. And like if the universe is has negative curvature, then it sort of acts like a what's the opposite of a magnifying glass? A glass if you're near-sided or something. A demagnifying glass? You know, like a piece of glass that has the opposite kind of curve,
Starting point is 00:54:32 like the curves inwards in the middle. Then things sort of looked smaller through it, right? So the spots should look smaller. And we can do these simulations. We say, here's where the hot spots and cold spots should look like if the universe was flat. And then we can dial up the curvature of the universe. And in our simulations, we can say, oh, look, the spots get bigger.
Starting point is 00:54:49 And then we can dial down the curvature to negative. We say, oh, look, the spots get smaller. And then we go out and we look in the actual universe. And we say, which of these best describes what we see? You know, is the universe look like it's flat or does it look like it's curved one way or the other? So this is a very powerful way to measure the curve to the universe over a very, very large scale. Because even though those photons started out not that far apart from each other, they traversed a huge amount of the universe because of that expansion.
Starting point is 00:55:19 Right, yeah. So is the universe amplifying or shrinking the cosmic microwave background? And so what we found when we measure this is that the universe seems to be very, very close to flat. Within 0.4% it's flat. Like this is a number we measure. So it's not an exact thing. You can never get like 0.000000 with infinite zeros. What we measure is 0.004 curvature.
Starting point is 00:55:44 Meaning that as far as we think, the universe is not curved. It's flat. That's right. It's consistent with zero that we measure something a little bit above zero. It's like if you flipped a coin, a thousand. thousand times and it's a fair coin, you'd expect on average to get 50% of those to be heads. But, you know, sometimes you get a fluctuation up or down. So that's what we see here.
Starting point is 00:56:04 Space is either perfectly flat or it's slightly positively curved, but it's consistent with flat. But I guess, you know, one question I would have as a skeptic is that you just told me that this is based on our measurement of the universe compared to what we expect, but isn't what we expect also sort of warped by our view of the universe? Like what we expect is somehow distorted too. Absolutely. This could be wrong, right? It's one measurement.
Starting point is 00:56:27 And there are always assumptions built into any measurement. We have other ways to measure the curvature of the universe. And those other ways agree with this measurement. Another way to measure the curvature of the universe is to go back to something we were talking about earlier, like what stuff is there in the universe? You sort of like weigh the whole universe, like add up all the mass of all the stuff that's in the universe, the matter, the dark matter, the dark energy. And that'll tell you like, is there.
Starting point is 00:56:51 enough stuff in the universe to be consistent with flat or is there too much stuff in the universe that the universe has to be closed, has to have positive curvature. And so that's another completely separate, totally independent way to measure the curvature of the universe. And that also comes up consistent with flat. Well, wait, you told me earlier that the curvature of the universe doesn't depend on the stuff in it. Well, the overall shape, the way it's connected, whether it's infinite or looped or finite, that cannot be changed by the stuff in the universe. But the stuff in the universe can change the amount of curvature, collapsing a large sphere into a smaller one, for example, if it has more than the critical density. And knowing the amount of stuff in the universe
Starting point is 00:57:31 helps us measure the curvature, which determines what shapes it can be. I see. So, okay, so we've measured out the cosmic microwave background and we, it fits our predictions for a flat universe, which means that probably the universe is flat. What does that mean for the shape of the universe. Probably the universe is flat, which means probably it's infinite and boring in that sense and goes on forever in that sort of naive sense. But, you know, people look at these measurements and they see some weird stuff in there. Like, first of all, it's flat, but, you know, there's a little bit of positive curvature there. So maybe it's something different. And when they look in more detail at these wiggles, they see something a little bit unexpected, something a little surprising,
Starting point is 00:58:15 which makes them think about donuts. Are you sure that's something? It's just because it's lunchtime, maybe, or you need to sugar fix. But wait, let's like a setback. You said, so we've measured the universe to be probably flat, mostly flat. And what does that mean for the shape of the universe? Like, if it is flat, what does that mean? It means it doesn't have a shape, right? It means that it can only be infinite and go on forever, meaning it doesn't have a shape.
Starting point is 00:58:37 Well, I mean, that is a shape, right? Mathematically speaking, that's a shape, if the universe is flat and has no boundaries and goes on forever, that's a shape. Yeah. I see. And if it was closed, if it had positive courage, it would be a sphere, but we are not measuring that. Yeah, although remember, positive curvature can also be consistent with a donut. A donut is positively curved on its surface.
Starting point is 00:58:58 That's for a physical donut. A mathematically donut is technically flat. So remember that little subtlety. Okay, so we're measuring the universe to be a little positive curvature. Is that what you're saying? It has a little bit of a positive curvature. A little bit of a positive curvature. And also some details in the cosmic microwave background radiation are really interesting and tantalizing.
Starting point is 00:59:17 And it led some people to suspect that, that may be a donut is the best description of our universe. As the universe expands, we get these lumps in the cosmic microwave background, right? These lumps come from quantum fluctuations in the very early universe during inflation. But as the universe is inflating, you're getting fluctuations all the time.
Starting point is 00:59:35 So you should see lumps at all different sizes. This is like a biggest lump, and that's the one we're using to measure the curvature. You should see big lumps, you should see small lumps. You should see very, very small lumps. And so when we look at these fluctuations, the amounts of lumpiness in the universe, we should see big lumps and small lumps and smaller lumps and even smaller lumps.
Starting point is 00:59:53 And so when people go out and measure this stuff, they see that mostly, but they see that sort of like at the biggest scales, some of those lumps seem to be missing. Like you don't see necessarily correlations between things that are as far apart as you expect. Wait, let's maybe take a step back. We measure the universe to be a little bit positive curvature, which means that it can still be a sphere. Couldn't it still be a sphere?
Starting point is 01:00:15 Could be a sphere, yeah. I see. But there's something about the donut that makes it makes you think that it could be donut. What's special about a donut that would fit what you're seeing? Well, what we're seeing is that at very, very large angles, there aren't as many correlations as we expect. You know, we're talking about a very small effect here. And above 60 degrees in the sky, we should see fluctuations about 100 microcalvins, but what we see is fluctuations like 20 microcalvins. So it's a small effect. But a donut topology turns out to suppress these large scale fluctuations because it
Starting point is 01:00:48 makes the universe finite and donuts have a sort of a smaller radius than a sphere for the same curvature a donut has sort of like shorter length scales right than a sphere does well i guess maybe we need to talk about the differences between donuts and meatballs daniel like because a donut is interesting right because it's it's a close shape um but it has a hole in it and it's kind of interesting because like if you go in one direction like around the wide rim of the donut you go in a circle and also if you go towards the center of the donut you also go in a circle so it sort of loops around in all directions sort of like a sphere but it's not a sphere it's more like a like a closed cylinder yeah and it's got two different length scales as you say it's got like the one way around
Starting point is 01:01:29 and the other way around whereas a sphere only has one length scale it's just the radius and you know even if the universe is curved and it's a sphere or a donut we're talking about something very slightly curved so really really huge right really on enormous scales just it's just a no Nobody is confused. We're not like the little prints here standing on a tiny donut. It's a ginormous donut. Yeah, but they did a bunch of simulations and they discovered that a donut is better at causing the sort of lack of ripples that they see in CMB.
Starting point is 01:01:57 In the cosmic microwave background radiation, we don't see some of the bigger ripples that we expect. And a donut is better at suppressing those because it has these two length scales, the long way around and the short way around. And so you just sort of like don't get as big lumps on a donut as you do on a sphere. And so that makes people wonder, maybe the universe is shaped. like a donut. Right. So it's the difference between these length scales that is giving you the clues. Like you're seeing some weird kind of like oblong shaped in the cosmic microwave background.
Starting point is 01:02:25 Yes, the fact that you don't see as big lumps as you expect from a flat universe or even from a spherical universe. It's not impossible to suppress these long distance effects on a sphere. It's just that you would need a radius of curvature that's not consistent with what we have measured. A donut gives you another length scale to play with. So it's easier to suppress the long distance correlations. Now this is not a smoking gun. This is like a weird little hint that could just be random noise, right? It could be theorists getting too excited and eating too much chocolate and thinking about donuts. But it's sort of like a fun hint. And we'll get more data and we'll see if this holds up. But it's fascinating to me that this question is the universe
Starting point is 01:03:06 flat or is it a sphere or is it even a donut is still unanswered. It's still something we don't know the actual answer to. Whoa. But it seems like we have a sort of a big clue, which is that the universe seems flat around us. Could it be that we're just measuring local curvature? Like, are we just a dimple, like a flat spot in a, you know, teacup shape universe? Absolutely. You know, what we're doing is we're assuming that the curvature we measure here is the same as the curvature we're measuring somewhere else.
Starting point is 01:03:34 And we're hoping that that's true because we're measuring in lots of different ways. And we're trying to measure in different directions. But in the end, our vantage point is limited, right? And so it could be that we're a flat spot on a very large donut or that we could be a slightly curved spot on an otherwise flat universe. You know, we can't really confidently extrapolate path what we can see. Though remember that the CMB measurements do cover a lot of space. It's not that local. Interesting.
Starting point is 01:04:03 Or so you're saying kind of stay tuned. Like we actually don't know what the shape of the universe is. That's right. If you're betting, I think flat is the best bet. It's the simplest. It's harmonious. It's what most physicists believe. If you ask them, is the universe flat, they would say yes.
Starting point is 01:04:19 But, you know, the data say it's either flat or slightly positively curved. And there are these interesting wiggles that are more consistent with a donut shape than a sphere or a flat universe. So, yeah, stay tuned. We still got big realizations ahead of us. So if you're the gambling type, maybe invest in donuts, is what you're saying. And if you win, eat a donut. And if you lose, eat a donut. Either way, you win.
Starting point is 01:04:43 I thought he said, if you don't win, you don't it. You win, you don't or you donut? Don't donut if you win. If the universe is filled with dark chocolate, how would that change the coverage or Daniel? I think we'd make it more closed. Exactly. Dark chocolate's pretty dense stuff and so we tend to compact on itself. And that would mean the universe is not infinitely filled with chocolate and eventually my snacking days must end.
Starting point is 01:05:05 Right. But if it's closed, then there's a finite amount of dark chocolate. So eventually you might eat, physicists might eat it all. That's right. better go out and get started on my snack. You might want to buy some new belts, too, or pants. Assuming you wear pants, I mean, we talked about social conventions and physicists. Yeah.
Starting point is 01:05:21 Who knows, right? We talked about not making assumptions, right? You know, we're exploring the universe here. That's right. What shape is Daniel, are Daniels pants? He doesn't have pants, maybe. It's a good question. There actually is a pants diagram for black hole mergers.
Starting point is 01:05:35 We're going to talk about it a few weeks. All right. Is that rude to ask what shape that black hole's pants are? We'll find out. Are they bell bottoms or tapered, low-rising? They wear shorts over their socks and sandals probably. Me, their mom jeans. Or dad cargo pants.
Starting point is 01:05:54 All right. Well, it's interesting to think that, you know, from our little spot in the universe, we can, you know, have these conversations about what the shape of the universe is when it's so far away, you know, 90, 60 billion light years away. We're still, we can still have conversations about it. And we might be right, which is the crazy thing. Yeah. And thank you very much to Professor. Professor's Leo Stein and Evans Kennepeakeko for consulting with us on this tricky topic.
Starting point is 01:06:18 Any remaining inaccuracies and ambiguities are our responsibility not theirs. And no matter how big and how crazy the question is, we can eventually always think about some way to try to answer it, some clever wrinkle in the nature of the universe that forces it to answer our questions, but even the biggest, hardest, craziest questions with the craziest answers. That's right, even the tasty and crazy answers about the universe. Well, we hope you enjoyed that. Thanks for joining us. See you next time.
Starting point is 01:07:10 I'm Dr. Scott Barry Kaufman, 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 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. I'm Simone Boyce, host of the Brightside podcast, and on this week's episode, I'm talking to Olympian, World Cup champion, and podcast host, Ashlyn Harris.
Starting point is 01:08:00 My worth is not wrapped up in how many things I've won, because what I came to realize is I valued winning so much that once it was over, I got the blues, and I was like, this is it. For me, it's the pursuit of greatness. It's the journey. It's the people. It's the failures. It's the heartache. Listen to the bright side on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. And here's Heather with the weather. Well, it's beautiful out there, sunny and 75, almost a little chilly in the shade. Now, let's get a read on the internet. inside of your car. It is hot. You've only been parked a short time and it's already 99 degrees in there. Let's not leave children in the back seat while running errands. It only takes a few minutes for
Starting point is 01:08:52 their body temperatures to rise and that could be fatal. Cars get hot, fast, and can be deadly. Never leave a child in a car. A message from NHTSA and the ad council. This is an iHeart podcast.

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