WEBVTT - Why is the universe inflating?

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<v Speaker 1>Hey, Daniel, did you have a good holiday break? Oh?

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<v Speaker 1>I did, but you know, as usual, I ate too much.

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<v Speaker 1>You mean you ate cosmically too much? Yeah, I totally

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<v Speaker 1>overdid it. I'm like on the verge of becoming a

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<v Speaker 1>black hole myself. Would you say your waistline is inflating,

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<v Speaker 1>I'd say a few more bites and I'd be risking

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<v Speaker 1>becoming my own personal big bang big Daniel. I'm talking

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<v Speaker 1>dark matter here people. Oh no, let's cut to the

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<v Speaker 1>theme song. Cut to the theme song. Hi am or

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<v Speaker 1>handmade cartoonist and the creator of PhD comics. Hi, I'm Daniel,

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<v Speaker 1>I'm a particle physicist, and I am actually full of

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<v Speaker 1>dark matter. Welcome to our podcast, Daniel and Jorge Explain

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<v Speaker 1>the Universe, a production of I Heart Radio in which

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<v Speaker 1>we examine all things fascinating and amazing and bonkers about

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<v Speaker 1>our universe and explain them to you in a way

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<v Speaker 1>that you can actually understand. So it's a new decade here,

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<v Speaker 1>and so, Daniel, what do we have to look forward

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<v Speaker 1>to in physics? What do we have to look forward

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<v Speaker 1>to in physics? Wow? So much? There are all sorts

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<v Speaker 1>of new exciting telescopes coming online that will let us

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<v Speaker 1>see further and further into the ancient past. The Large

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<v Speaker 1>Hadron Collider is going to keep running and maybe discover

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<v Speaker 1>some crazy new particles. But you know the best thing

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<v Speaker 1>about looking forward in physics is that we have no

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<v Speaker 1>idea what we're going to discover. There are always surprises

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<v Speaker 1>out there waiting for us. There are surprises everywhere. Yeah,

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<v Speaker 1>that's awesome. Yeah there might be Hey, a new kind

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<v Speaker 1>of plantain or a strawberry flavored banana discovered by scientists somewhere.

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<v Speaker 1>You never know science. It's what's for dinner, and so

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<v Speaker 1>there's a lot of good stuff to look forward to.

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<v Speaker 1>I look forward to in looking back and thinking, Man,

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<v Speaker 1>those folks in had no idea what was coming. Interesting.

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<v Speaker 1>You look forward to the future so you can laugh

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<v Speaker 1>at the past. Yeah, it's a wonderful feeling to think,

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<v Speaker 1>look at what we know about the universe, and look

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<v Speaker 1>at how the people before us, including ourselves ten years ago,

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<v Speaker 1>really had no clue what was coming. And that's exciting

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<v Speaker 1>to me because it makes me enthusiastic about the next

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<v Speaker 1>ten years. You know, the mind blowing discoveries that physics

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<v Speaker 1>and the rest of science will reveal. Man, you're making

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<v Speaker 1>me feel bad about humans. They were so clueless, oh man,

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<v Speaker 1>with their like new Facebook craze and they didn't even

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<v Speaker 1>have TikTok or Instagram. No, but we learned a lot

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<v Speaker 1>about the universe in the twenty tens. You know, we

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<v Speaker 1>saw a whole bunch of new exo planets and discovered

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<v Speaker 1>the Higgs boson, and you are there really some pretty

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<v Speaker 1>big shifts that our understanding of the universe in the

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<v Speaker 1>last ten years. And since science is just accelerating exponentially,

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<v Speaker 1>then I look forward to even more mind blowing stuff

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<v Speaker 1>in the decade to come. Yeah, and technically we have

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<v Speaker 1>more universe now than we had in Right, the universe

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<v Speaker 1>is constantly expanding and getting bigger. There's new space being created,

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<v Speaker 1>so we have also that to look forward to. Right

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<v Speaker 1>in the future, there there will be even more space.

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<v Speaker 1>That's right, in the future, you will occupy a smaller

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<v Speaker 1>fraction of the universe because the universe is inflating. Oh no, wait,

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<v Speaker 1>so you're saying that the people in were more significant

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<v Speaker 1>than we are. Well, you know, what's the fraction of

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<v Speaker 1>infinity is still zero so relatively speaking. But you know,

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<v Speaker 1>I had a listener right in and make a really

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<v Speaker 1>fascinating point about the expansion of the universe that I

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<v Speaker 1>had never thought of before. Yeah, And they said, well,

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<v Speaker 1>what about in time travel books, if you go back

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<v Speaker 1>in time, then doesn't your body occupy a smaller space

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<v Speaker 1>in the universe back then than it does now? And

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<v Speaker 1>how do you account for that? And it's true, you know,

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<v Speaker 1>the space that you occupied twenty years ago has expanded

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<v Speaker 1>to a larger space, and so somehow you have to

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<v Speaker 1>factor that into your time travel novel. WHOA like if

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<v Speaker 1>you if you send your consciousness back, it has to

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<v Speaker 1>somehow fit into a smaller package or something. Yeah, it

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<v Speaker 1>has to shrink exactly. You gotta squeeze your way back

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<v Speaker 1>into the universe from ten years ago or twenty years ago.

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<v Speaker 1>On today's episode, we are going to not look forward

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<v Speaker 1>in time, but we're going to try to look backwards

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<v Speaker 1>in time almost as much as you can look backwards. Right,

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<v Speaker 1>that's right. We're gonna try to rewind all the way

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<v Speaker 1>back to the very beginning. Because I've noticed that in

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<v Speaker 1>conversations with listeners and just with folks around campus, that

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<v Speaker 1>there's still a lot of misunderstandings about the very beginning

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<v Speaker 1>of the universe. Right, because right now we have a

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<v Speaker 1>lot of space, there's a lot of universe, but at

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<v Speaker 1>some point in the past there was very little of

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<v Speaker 1>the universe. I don't know. I mean, I think right

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<v Speaker 1>now the universe is pretty dilute, but in the past,

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<v Speaker 1>the universe was more dense. It could be that the

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<v Speaker 1>universe has been infinite since its conception. So in that sense,

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<v Speaker 1>it doesn't really make sense to talk about having less universe.

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<v Speaker 1>It's just more compact, right, A denser infinity, yes, a

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<v Speaker 1>denser infinity exactly, versus a water down infinity, which you know,

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<v Speaker 1>it just doesn't taste as good. That's right. But I

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<v Speaker 1>think a lot of people when you talk about the

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<v Speaker 1>beginning of the universe and the Big Bang, they have

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<v Speaker 1>sort of an old idea in their head of what

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<v Speaker 1>the Big Bang was like this just this big explosion

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<v Speaker 1>from a singularity, and that's not really the modern view. Wait,

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<v Speaker 1>you're saying the name big bang doesn't actually describe the

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<v Speaker 1>Big Bang. I think it was pretty big and it

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<v Speaker 1>might have been a bang, so you know, from that

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<v Speaker 1>point of view. But I think the ideas in people's

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<v Speaker 1>heads need updating. I see, it's it's a kind of

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<v Speaker 1>big bang, yes, exactly. Big Bang and compass is like

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<v Speaker 1>a whole spectrum of ideas and physics has moved on,

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<v Speaker 1>while popular conception is sort of stuck in the eighties version, right,

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<v Speaker 1>And so this is a question that you said to me.

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<v Speaker 1>A lot of listeners asked wrote in to ask about

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<v Speaker 1>a lot of people are wondering and asking us to

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<v Speaker 1>explain what this idea is. Yeah, and so, as usually,

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<v Speaker 1>we want to cater to our listeners. We want to

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<v Speaker 1>answer the questions that are in your minds, and we

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<v Speaker 1>want to bring you to the forefront of science. We

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<v Speaker 1>want you to understand what scientists out there, who are

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<v Speaker 1>experts in this field, who know the most that any

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<v Speaker 1>human is ever known about the beginning of the universe,

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<v Speaker 1>what they are thinking about. We want to explain it

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<v Speaker 1>to you in a way that makes sense. So that's

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<v Speaker 1>our goal. So today on the episode, we'll be asking

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<v Speaker 1>the question, what is cosmic inflation? Inflation? Inflation? That's right,

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<v Speaker 1>it's not controlled by the Federal Reserve. It's not the

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<v Speaker 1>reason why your bank account is emptying. Wait, you mean

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<v Speaker 1>cosmic interest rate? Don't don't make a difference here. No,

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<v Speaker 1>we can't borrow money from the other universe. Orything can

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<v Speaker 1>my cosmic debt somehow bring it down? That's your karmic debt, actually,

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<v Speaker 1>and there's nothing you can do about that. Then do

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<v Speaker 1>good things for people, like explain the universe to them.

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<v Speaker 1>I think that's definitely a positive on the karmic debt,

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<v Speaker 1>right right, But today we're talking about cosmic inflation, and

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<v Speaker 1>that kind of sounds simple. It just means that the

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<v Speaker 1>cosmos is getting bigger or got bigger. But in this case,

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<v Speaker 1>scientists use this phrase for something very specific, right, like

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<v Speaker 1>a very specific moment in time right after the Big Bang.

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<v Speaker 1>Sort Of, it's both a specific moment in time that's

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<v Speaker 1>after the Big Bang, it's also sort of our modern

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<v Speaker 1>view of what the Big Bang was, and and it's

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<v Speaker 1>also connects the like primordial inflation, these first moments when

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<v Speaker 1>the universe is expanding with the current inflation, and it

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<v Speaker 1>says maybe these things are connected. So it's sort of

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<v Speaker 1>like saying the Big Bang wasn't the moment of creation.

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<v Speaker 1>It happened just afterwards. And it's saying maybe the Big

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<v Speaker 1>Bang is still banging. We're still banging, yes, exactly, that's

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<v Speaker 1>how big this bang is. Well, it sounds like it's

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<v Speaker 1>it's pretty interesting and maybe there are a lot of

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<v Speaker 1>subtle ideas here, so we'll get into all of that.

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<v Speaker 1>But first, as usual, we were wondering how many people

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<v Speaker 1>out there heard of the phrase cosmic inflation and if

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<v Speaker 1>they knew what it was. That's right. And so since

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<v Speaker 1>it was winter break and you see, Irvine was closed,

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<v Speaker 1>I walked around coffee shops in Irvine and I asked

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<v Speaker 1>random strangers who were amenable to being interrogated about physics

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<v Speaker 1>topics while on their holiday break if they knew anything

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<v Speaker 1>about cosmic inflation. Here's what they had to say. Oh,

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<v Speaker 1>I feel like I've heard the term, but I do

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<v Speaker 1>not know what it means. Um, cosmic inflation is that

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<v Speaker 1>like the theory where everything in space is like constantly

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<v Speaker 1>moving away from itself, like there's an explosion and everything's

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<v Speaker 1>still expanding. Yeah, I have no idea. I think it

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<v Speaker 1>means that just like crowding together, maybe like everything's coming together,

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<v Speaker 1>but I don't know. The universe is expanding and getting

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<v Speaker 1>bigger with each but as time passes, so something that's

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<v Speaker 1>happening now or in the past, it's still happening from

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<v Speaker 1>the universe. That's something that's happening now or in the

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<v Speaker 1>beginning the universe, or it's always been happening. Yes, what

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<v Speaker 1>is it? That's essentially the basis of the big bank theory? Okay, Um,

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<v Speaker 1>when did it happen fourteen point three billion years ago?

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<v Speaker 1>We might have more more satellites of space, space stations

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<v Speaker 1>or something. I have no idea. I mean it sounds

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<v Speaker 1>like the expansion of space, cosmic inflation. No, alright, a

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<v Speaker 1>lot of knows I feel, not a lot of inflated

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<v Speaker 1>answers here. No, no, no, and confusion people thinking like

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<v Speaker 1>space is getting smaller or the Earth is getting more crowded.

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<v Speaker 1>That maybe they thought space was getting devalued. Maybe there's

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<v Speaker 1>the there's the negative flip side to it that surprised.

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<v Speaker 1>The market for space is sad oversaturated. So better spend

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<v Speaker 1>your space now before it's worth nothing. Better use it up. Better,

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<v Speaker 1>eat more so you can take up more space. That's

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<v Speaker 1>that's my New Year's resolution. Eat more dark matter, take

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<v Speaker 1>up more space, make more dark better. But there were

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<v Speaker 1>some some core ideas here. You know, people have heard

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<v Speaker 1>of some connection to the Big Bang or some ideas

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<v Speaker 1>for things that happened in the early universe. So there's

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<v Speaker 1>definitely some nuggets there Yeah. A lot of people said

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<v Speaker 1>it related to the expansion of the universe, which is

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<v Speaker 1>I guess not a big stretch, right. Inflation and expansion

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<v Speaker 1>sort of sound the same. Yeah, And in fact I

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<v Speaker 1>think they're right. It is related to the expansion of

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<v Speaker 1>the universe as far as we know, which is not

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<v Speaker 1>very much, it turns out, you know, and this is

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<v Speaker 1>fascinating to me because it's something where we've made a

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<v Speaker 1>lot of progress in the last twenty years coming up

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<v Speaker 1>with new, crazy ideas about the universe, but something that

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<v Speaker 1>we're also still puzzled over, Like there are huge unanswered

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<v Speaker 1>questions about the Big Bang and cosmic inflation. There are

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<v Speaker 1>things that scientists are arguing about. You know, the guy

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<v Speaker 1>who came up with inflation, one of the architects of

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<v Speaker 1>the theory, Paul Steinhardt, is now the guy arguing against

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<v Speaker 1>the theory most Yeah, he's trying to deflate inflation, that's right.

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<v Speaker 1>He's trying to pop the bubble of his own creation.

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<v Speaker 1>So what's interesting I think is that, you know, if

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<v Speaker 1>you had asked what is the Big Bang, a lot

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<v Speaker 1>of people might have said, yes, it has had some

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<v Speaker 1>ideas about that. It's about the beginning of the universe,

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<v Speaker 1>but cosmic inflation, which is almost as important, doesn't have

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<v Speaker 1>the same kind of market recognition. Yeah, and that's what

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<v Speaker 1>we're going to try to correct today on the podcast.

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<v Speaker 1>We're gonna bring some panash to cosmic inflation. We're gonna

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<v Speaker 1>show people how big bang is sort of the old

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<v Speaker 1>busted theory and cosmic inflation is the new hotness. M

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<v Speaker 1>it's a new bang. It's the new bang. That's right

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<v Speaker 1>out with the old bang, in with it's climb. Are

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<v Speaker 1>you still banging the old way? Man? What's wrong with you? Try?

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<v Speaker 1>Are you physics bace banging? Yeah? I don't know what

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<v Speaker 1>advertisers are going to go for that. Somebody out there

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<v Speaker 1>has got a product that fits that. Alright, Diana, So

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<v Speaker 1>let's get into it. Let's get into this idea of

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<v Speaker 1>cosmic inflation. So, first of all, what is how would

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<v Speaker 1>you define inflation in a physics way? Basically, inflation is

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<v Speaker 1>the expansion of space. It's saying, let's take space and

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<v Speaker 1>stretch it. Let's make space bigger and it it's important

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<v Speaker 1>there to understand that it's not the moving of stuff

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<v Speaker 1>through space. It's really the stretching of space itself. So

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<v Speaker 1>are we stretching space or creating new space both both.

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<v Speaker 1>That is how you stretch spaces and you create new space.

0:12:56.120 --> 0:12:57.959
<v Speaker 1>I see, like there's more meters. It's not like the

0:12:58.040 --> 0:13:01.400
<v Speaker 1>meter got bigger, so it's just more meters of space. Yeah,

0:13:01.520 --> 0:13:04.320
<v Speaker 1>there are more meters of space. So stuff can be

0:13:04.520 --> 0:13:08.160
<v Speaker 1>further apart without moving through space. Right. It's like if

0:13:08.240 --> 0:13:11.520
<v Speaker 1>you take a ruler and you put a penny on

0:13:11.600 --> 0:13:13.880
<v Speaker 1>the one meter and on the two m and then

0:13:13.920 --> 0:13:16.760
<v Speaker 1>you stretch the ruler. The ruler itself is like may

0:13:16.840 --> 0:13:19.480
<v Speaker 1>out of elastic, and you stretch the rulers to make

0:13:19.480 --> 0:13:22.160
<v Speaker 1>it longer than the two pennies are further apart even

0:13:22.160 --> 0:13:26.679
<v Speaker 1>though they haven't moved relative to the ruler. That's expansion

0:13:26.720 --> 0:13:30.400
<v Speaker 1>of space. That's inflation of space. Right. But it's not

0:13:30.480 --> 0:13:32.720
<v Speaker 1>just that the ruler expanded. It's like the wood of

0:13:32.760 --> 0:13:36.400
<v Speaker 1>the ruler got bigger. You definitely add more to the ruler. Okay,

0:13:36.440 --> 0:13:39.760
<v Speaker 1>And so that's different than kind of the old idea

0:13:39.800 --> 0:13:44.520
<v Speaker 1>of how the Big Bank happened after the beginning of time. Yeah,

0:13:44.559 --> 0:13:46.840
<v Speaker 1>so let's dig into that in that way. Let's like

0:13:47.080 --> 0:13:50.280
<v Speaker 1>define what I think most people think the Big Bang

0:13:50.520 --> 0:13:52.640
<v Speaker 1>was and the sort of old idea of what the

0:13:52.720 --> 0:13:55.360
<v Speaker 1>universe was, and then let's contrast it with with sort

0:13:55.360 --> 0:13:57.640
<v Speaker 1>of what they should replace in their heads with. Okay,

0:13:57.720 --> 0:14:00.640
<v Speaker 1>so what's the old thing. The old thing, I think

0:14:00.960 --> 0:14:03.280
<v Speaker 1>is this idea that the universe started from a point

0:14:03.400 --> 0:14:08.520
<v Speaker 1>like a singularity and infinitely dense dot primordial atom, which

0:14:08.600 --> 0:14:10.880
<v Speaker 1>was a point in space. It was like somewhere and

0:14:10.920 --> 0:14:14.240
<v Speaker 1>it was infinitely dense. And remember, like nobody has in

0:14:14.280 --> 0:14:16.520
<v Speaker 1>the idea where this thing might have come from, what

0:14:16.640 --> 0:14:18.760
<v Speaker 1>could have created it. But that's sort of just like

0:14:18.840 --> 0:14:21.400
<v Speaker 1>swept under the rug, you know, the primordial rug, Like well,

0:14:21.680 --> 0:14:23.360
<v Speaker 1>you know, we don't know what came before, but let's

0:14:23.360 --> 0:14:25.720
<v Speaker 1>just start from there. Right, it was like a little tiny,

0:14:25.800 --> 0:14:30.480
<v Speaker 1>infinitely energetic package in sitting in space actually right like

0:14:30.520 --> 0:14:33.520
<v Speaker 1>it was. People think it was like a grenade sitting there.

0:14:33.880 --> 0:14:36.480
<v Speaker 1>It was really really small, exactly, And that's really key

0:14:36.480 --> 0:14:39.520
<v Speaker 1>insight there that space was already created. You already had space,

0:14:39.560 --> 0:14:41.640
<v Speaker 1>and you just had this dot in space. And then

0:14:41.680 --> 0:14:45.560
<v Speaker 1>it exploded and that stuff then flew out and it

0:14:45.760 --> 0:14:49.560
<v Speaker 1>spread out and slowly got more and more dilute, right

0:14:49.680 --> 0:14:53.120
<v Speaker 1>less dense like an explosion would, and spread out to

0:14:53.200 --> 0:14:56.880
<v Speaker 1>eventually form of the universe, and that's the stuff moving

0:14:57.000 --> 0:14:59.440
<v Speaker 1>through space. And that's what we call in science the

0:14:59.480 --> 0:15:02.000
<v Speaker 1>hot big Bang model. The hot big Bang is now

0:15:02.040 --> 0:15:05.320
<v Speaker 1>the old Big Bang. It's right, you know, it's like

0:15:05.400 --> 0:15:07.480
<v Speaker 1>your ex girlfriend and boyfriends. You still think they're hot,

0:15:07.680 --> 0:15:11.880
<v Speaker 1>but it's not really for you anymore. Man. So that's

0:15:11.920 --> 0:15:14.440
<v Speaker 1>probably the idea most people have in their heads when

0:15:14.480 --> 0:15:17.120
<v Speaker 1>you say big bang or creation in the universe. And

0:15:17.440 --> 0:15:20.080
<v Speaker 1>I think that's what I thought that the Big Bang was,

0:15:20.480 --> 0:15:22.440
<v Speaker 1>you know, way before, when I was in high school

0:15:22.560 --> 0:15:25.560
<v Speaker 1>or before I started hanging out with physicists, was that

0:15:25.640 --> 0:15:27.400
<v Speaker 1>the Big Bang is really just like a bang, Like

0:15:28.080 --> 0:15:30.160
<v Speaker 1>everything that we know about was in a small spot

0:15:30.200 --> 0:15:32.720
<v Speaker 1>and then it just exploded. And now all the stars

0:15:32.720 --> 0:15:34.800
<v Speaker 1>and galaxies and dust that was in that little bit

0:15:34.880 --> 0:15:38.640
<v Speaker 1>doot are now flying through space outwards. Yeah. And you know,

0:15:38.680 --> 0:15:41.840
<v Speaker 1>when you started hanging out with physicists, basically the moment

0:15:41.920 --> 0:15:45.200
<v Speaker 1>your universe was created. Everything else before that is like, oh,

0:15:45.800 --> 0:15:50.760
<v Speaker 1>waste of time. I see you. You created my universe, Daniel,

0:15:51.040 --> 0:15:53.880
<v Speaker 1>my universe started. There's nothing before I met you. There

0:15:54.000 --> 0:15:58.160
<v Speaker 1>you're supposed to go with you complete my universe. You're

0:15:58.200 --> 0:16:02.280
<v Speaker 1>saying you made my universe. Then that's even more romantic. Wow.

0:16:02.720 --> 0:16:04.480
<v Speaker 1>Well all right, yeah, I think on the back pedal

0:16:04.520 --> 0:16:06.440
<v Speaker 1>on that a little bit, But no, you're right, and

0:16:06.480 --> 0:16:09.400
<v Speaker 1>I think that's what most people think um as sort

0:16:09.440 --> 0:16:11.400
<v Speaker 1>of how the universe began, and you know, there's lots

0:16:11.400 --> 0:16:14.400
<v Speaker 1>of questions there um. But one big problem with that

0:16:14.440 --> 0:16:17.600
<v Speaker 1>conception is that it has a center, has a place

0:16:17.600 --> 0:16:20.520
<v Speaker 1>where the Big Bang happened. And if you were looking

0:16:20.560 --> 0:16:23.040
<v Speaker 1>at the explosion from any point of view, you would

0:16:23.080 --> 0:16:26.640
<v Speaker 1>see stuff sort of flying sideways, unless you happen to

0:16:26.760 --> 0:16:29.760
<v Speaker 1>be at the center, then everything would be flying in

0:16:29.800 --> 0:16:32.560
<v Speaker 1>a certain direction, right, and you could tell maybe where

0:16:32.560 --> 0:16:34.880
<v Speaker 1>the center of the universe was just by looking at

0:16:35.200 --> 0:16:38.360
<v Speaker 1>where all the things were, and you're flying away from

0:16:38.360 --> 0:16:42.680
<v Speaker 1>precisely and as a foreshadowing moment, that's not what we

0:16:42.760 --> 0:16:45.480
<v Speaker 1>see when we look out into space. Yeah. So at

0:16:45.520 --> 0:16:50.400
<v Speaker 1>some point a humanity physicist and scientists decided or started

0:16:50.680 --> 0:16:53.400
<v Speaker 1>to realize that this old model of the big band

0:16:53.640 --> 0:16:56.760
<v Speaker 1>was not the right one. Yeah. I mean it's a

0:16:56.760 --> 0:16:59.400
<v Speaker 1>good first draft. Like we're thinking about the universe, is

0:16:59.440 --> 0:17:01.680
<v Speaker 1>expanding what could have created it. You know, we don't

0:17:01.680 --> 0:17:04.400
<v Speaker 1>want to criticize those scientists, is being dumb or something

0:17:04.440 --> 0:17:06.520
<v Speaker 1>It's just sort of like science evolves, and this is

0:17:06.560 --> 0:17:08.840
<v Speaker 1>how it evolves. You have an idea, you compare it

0:17:08.840 --> 0:17:11.159
<v Speaker 1>to what you see. Doesn't quite work, so you improved

0:17:11.200 --> 0:17:16.199
<v Speaker 1>the idea. Right, They did a bang up job. It

0:17:16.280 --> 0:17:19.520
<v Speaker 1>was a big project. But but what I guess what

0:17:19.560 --> 0:17:21.720
<v Speaker 1>I mean is it at what point did we start

0:17:21.760 --> 0:17:24.439
<v Speaker 1>to sort of realize maybe this view was not the

0:17:24.480 --> 0:17:27.439
<v Speaker 1>correct one. Well, there's been a lot of problems with

0:17:27.480 --> 0:17:30.120
<v Speaker 1>the Big Bang basically since early on. You know when

0:17:30.280 --> 0:17:33.320
<v Speaker 1>ed when Hubble looked out into the universe and realized

0:17:33.359 --> 0:17:36.719
<v Speaker 1>it's like a hundred years ago that the universe was expanding,

0:17:37.320 --> 0:17:39.480
<v Speaker 1>That's sort of what gave birth to this concept of

0:17:39.480 --> 0:17:42.760
<v Speaker 1>a big Bang. He's the one who discovered that everything

0:17:42.840 --> 0:17:45.200
<v Speaker 1>was moving away from us, and everything was moving away

0:17:45.200 --> 0:17:47.480
<v Speaker 1>from us sort of the same speed in every direction

0:17:47.520 --> 0:17:50.159
<v Speaker 1>you looked. So this is an outstanding problem for the

0:17:50.200 --> 0:17:53.639
<v Speaker 1>Big Bang for a long time, and it wasn't until

0:17:54.040 --> 0:17:57.440
<v Speaker 1>this idea of inflation came along that it helped solve it.

0:17:57.520 --> 0:18:00.760
<v Speaker 1>So the Big Bang was not like totally accepted for

0:18:01.240 --> 0:18:04.280
<v Speaker 1>many many decades. And one problem what with it was,

0:18:04.720 --> 0:18:06.679
<v Speaker 1>you know, are we at the center? Why does it

0:18:06.760 --> 0:18:09.480
<v Speaker 1>look like we are at the center. Oh, I see.

0:18:09.560 --> 0:18:12.119
<v Speaker 1>He tried to figure out where the center of the

0:18:12.160 --> 0:18:15.520
<v Speaker 1>grenade was, and so he looked around and he found

0:18:15.560 --> 0:18:18.520
<v Speaker 1>that the center was us, which is weird, which was like,

0:18:18.600 --> 0:18:22.000
<v Speaker 1>too coincidental. It's too coincidental. Any time in science you

0:18:22.040 --> 0:18:23.760
<v Speaker 1>appear to be at the center of the universe, you

0:18:23.840 --> 0:18:28.520
<v Speaker 1>gotta wonder my biased or I'm just thinking about this wrong.

0:18:28.560 --> 0:18:31.000
<v Speaker 1>You know, you want to avoid coincidences. You want to

0:18:31.000 --> 0:18:35.359
<v Speaker 1>avoid things that are really unlikely, or especially things that

0:18:35.400 --> 0:18:38.320
<v Speaker 1>put humanity in the very important place in the cosmos.

0:18:38.400 --> 0:18:42.680
<v Speaker 1>Because we've made that mistake before, right, Like before we thought,

0:18:42.800 --> 0:18:44.639
<v Speaker 1>we like the Earth with decent was the center of

0:18:44.680 --> 0:18:46.600
<v Speaker 1>the Solar system. More than that, we thought it was

0:18:46.600 --> 0:18:49.240
<v Speaker 1>the center of the cosmos, right without everything was created

0:18:49.280 --> 0:18:52.520
<v Speaker 1>around the Earth, Yeah, right, right, And then it turns

0:18:52.520 --> 0:18:54.480
<v Speaker 1>out that the Sun, not even the Sun, is the

0:18:54.520 --> 0:18:57.960
<v Speaker 1>center of the universe. It's like just one star in

0:18:58.000 --> 0:19:02.359
<v Speaker 1>the rotating galaxy, which is part of something even bigger. Yeah,

0:19:02.440 --> 0:19:04.800
<v Speaker 1>And we like to think more democratically now. We like

0:19:04.880 --> 0:19:07.920
<v Speaker 1>to think that every point in space is equal, not

0:19:07.960 --> 0:19:10.560
<v Speaker 1>because they're voting or anything, but just that you know,

0:19:10.600 --> 0:19:13.760
<v Speaker 1>there should be no special locations because special locations require

0:19:13.840 --> 0:19:17.160
<v Speaker 1>special explanations. It just makes the most sense if everywhere

0:19:17.160 --> 0:19:20.000
<v Speaker 1>in space follows the same rules and is the same.

0:19:20.320 --> 0:19:21.720
<v Speaker 1>And that's why I like the Big Bang is a

0:19:21.760 --> 0:19:23.639
<v Speaker 1>point never really made sense to me, because then you

0:19:23.640 --> 0:19:26.159
<v Speaker 1>can always ask, like, well, why they're why did the

0:19:26.160 --> 0:19:28.400
<v Speaker 1>Big Bang start there and not like a meter over

0:19:28.680 --> 0:19:30.640
<v Speaker 1>or over there or a light year in the other direction,

0:19:31.040 --> 0:19:34.000
<v Speaker 1>why they're nowhere else? And so you avoid those questions

0:19:34.040 --> 0:19:36.240
<v Speaker 1>if you say, everywhere in the universe is the same.

0:19:36.400 --> 0:19:39.560
<v Speaker 1>All right, So that's the old bang, the old hot bang,

0:19:40.160 --> 0:19:43.320
<v Speaker 1>and now let's talk about the new hotter bang, I guess,

0:19:43.600 --> 0:19:47.520
<v Speaker 1>and in terms of trendiness um and why why we

0:19:47.560 --> 0:19:49.639
<v Speaker 1>think it happened and why is it still a mystery?

0:19:49.760 --> 0:20:06.200
<v Speaker 1>But first let's take a quick break. Okay, So Danny

0:20:06.640 --> 0:20:09.320
<v Speaker 1>telling me that the universe, the Big Bang is not

0:20:09.440 --> 0:20:11.760
<v Speaker 1>like a grenade that exploded that was full stuff and

0:20:11.760 --> 0:20:14.840
<v Speaker 1>then exploded, But the universe, the Big Bang is actually

0:20:14.880 --> 0:20:18.600
<v Speaker 1>something different where new space is being created and space

0:20:18.680 --> 0:20:22.040
<v Speaker 1>is being stretched. It's not an explosion, that's right. And

0:20:22.080 --> 0:20:24.120
<v Speaker 1>we still have to reconcile the fact that we think

0:20:24.160 --> 0:20:27.479
<v Speaker 1>the universe was more dense in the past than it

0:20:27.600 --> 0:20:29.840
<v Speaker 1>is today, and that makes you want to go to

0:20:29.920 --> 0:20:32.840
<v Speaker 1>the explosion explanation because you know, like, how else could

0:20:32.880 --> 0:20:37.040
<v Speaker 1>it happen? Right, because the grenade was denser before the explosion,

0:20:38.280 --> 0:20:41.760
<v Speaker 1>So you might be tempted to apply to our universe. Yeah,

0:20:41.880 --> 0:20:44.760
<v Speaker 1>So another approach and a better way to think about

0:20:44.760 --> 0:20:48.600
<v Speaker 1>it that it requires swallowing a really big idea, is

0:20:48.640 --> 0:20:52.800
<v Speaker 1>that the Big Bang essentially happened everywhere all at once.

0:20:53.400 --> 0:20:56.840
<v Speaker 1>That the universe wasn't created as a tiny singularity which

0:20:56.880 --> 0:21:01.359
<v Speaker 1>then exploded, but that the entire uni verse, an infinite

0:21:01.440 --> 0:21:05.960
<v Speaker 1>universe filled with an infinite amount of stuff, was created somehow,

0:21:06.240 --> 0:21:09.760
<v Speaker 1>we don't know how, in a very dense state, and

0:21:09.800 --> 0:21:12.520
<v Speaker 1>the Big Bang was the expansion of that state, the

0:21:12.600 --> 0:21:16.400
<v Speaker 1>stretching of space itself to make that stuff more dilute.

0:21:16.560 --> 0:21:19.840
<v Speaker 1>But that it was created everywhere and happened everywhere all

0:21:19.880 --> 0:21:23.000
<v Speaker 1>at once. So like that's an infinitely big bang. Okay,

0:21:23.040 --> 0:21:26.720
<v Speaker 1>So you're saying that the universe was has always been infinite.

0:21:26.720 --> 0:21:28.600
<v Speaker 1>It's not like it started as a point and became

0:21:28.720 --> 0:21:32.600
<v Speaker 1>exploited into infinity. You're saying that the universe was always infinite,

0:21:33.040 --> 0:21:35.760
<v Speaker 1>but that before it was like a dance and compact

0:21:35.800 --> 0:21:39.000
<v Speaker 1>infinite infinity but now it's more of a bigger and

0:21:40.240 --> 0:21:43.800
<v Speaker 1>more expanded infinity. Precisely, that's the idea. And of course

0:21:43.800 --> 0:21:46.119
<v Speaker 1>we don't know the size of the universe, and we

0:21:46.160 --> 0:21:48.480
<v Speaker 1>don't even know it's shape, but this is the idea.

0:21:48.480 --> 0:21:52.639
<v Speaker 1>It explains what we see, an infinite universe created infinitely

0:21:52.680 --> 0:21:55.480
<v Speaker 1>big and always filled with an infinite amount of stuff.

0:21:55.520 --> 0:21:58.359
<v Speaker 1>There's no edge to the matter, and there's no edge

0:21:58.400 --> 0:22:01.439
<v Speaker 1>to the universe, and just started out really hot and

0:22:01.480 --> 0:22:05.800
<v Speaker 1>dense and then stretched out right, But that's only one possibility, right,

0:22:06.200 --> 0:22:08.400
<v Speaker 1>that it's infinite. It could also be that the universe

0:22:08.560 --> 0:22:11.480
<v Speaker 1>is finite as far as we know. Right, it could

0:22:11.480 --> 0:22:13.600
<v Speaker 1>be right, but it at least has to be big

0:22:13.720 --> 0:22:18.840
<v Speaker 1>enough to fill our observable universe with a homogeneous stuff. Right.

0:22:18.880 --> 0:22:22.000
<v Speaker 1>If there is an edge to the stuff in the universe,

0:22:22.400 --> 0:22:24.439
<v Speaker 1>we don't see that, and so it has to be

0:22:24.560 --> 0:22:27.800
<v Speaker 1>really really big and and pretty uniform, at least in

0:22:27.840 --> 0:22:31.480
<v Speaker 1>our neighborhood. So it's possible that there's an edge to

0:22:31.520 --> 0:22:34.960
<v Speaker 1>the stuff in the universe. But it's sort of simpler somehow.

0:22:34.960 --> 0:22:37.560
<v Speaker 1>It's weird. It's weird. It's simpler to imagine an infinite

0:22:37.640 --> 0:22:39.520
<v Speaker 1>universe with infinite stuff because then you don't have to

0:22:39.520 --> 0:22:43.199
<v Speaker 1>explain the edges. Even though I can't explain how you

0:22:43.240 --> 0:22:45.480
<v Speaker 1>create an infinite universe with an infinite amount of stuff

0:22:45.480 --> 0:22:50.159
<v Speaker 1>in it either, well, nobody can explain it finite universe either. Right,

0:22:50.240 --> 0:22:52.920
<v Speaker 1>All this stuff defies explanation. But you know it's it's

0:22:52.960 --> 0:22:55.880
<v Speaker 1>like pushing the rock further up the hill. You don't

0:22:55.920 --> 0:22:58.159
<v Speaker 1>have to have the answer to every question. You just

0:22:58.200 --> 0:23:00.119
<v Speaker 1>have to ask have the answer to this question in

0:23:00.440 --> 0:23:02.680
<v Speaker 1>and then it gives you the next question. Like if

0:23:02.760 --> 0:23:06.480
<v Speaker 1>you say, let's assume the universe started infinitely large, filled

0:23:06.520 --> 0:23:08.920
<v Speaker 1>with an infinite amount of stuff, then what would have happened?

0:23:09.119 --> 0:23:11.159
<v Speaker 1>And you can show that that's consistent with what we

0:23:11.200 --> 0:23:13.320
<v Speaker 1>see so far, then you get to go back to

0:23:13.359 --> 0:23:15.800
<v Speaker 1>that other question, say, okay, let's roll up our sleeves

0:23:15.800 --> 0:23:19.320
<v Speaker 1>and figure out how it's possible to create an infinite universe. Um.

0:23:19.520 --> 0:23:22.119
<v Speaker 1>So that is that your approach to teaching as well, Daniel,

0:23:22.280 --> 0:23:25.160
<v Speaker 1>Just make it up as you go along, push all

0:23:25.160 --> 0:23:28.160
<v Speaker 1>the problems off until tomorrow. That's my approach to life.

0:23:28.440 --> 0:23:34.800
<v Speaker 1>Yes to my inbox as well. Yeah, and so the

0:23:34.840 --> 0:23:38.679
<v Speaker 1>idea is you create an infinite universe filled with an

0:23:38.720 --> 0:23:41.480
<v Speaker 1>infinite amount of stuff, but it's very hot and dense. Right,

0:23:41.520 --> 0:23:44.520
<v Speaker 1>it's like a huge singularity essentially. Okay, so I think

0:23:44.560 --> 0:23:46.159
<v Speaker 1>you're saying that the best way to think about the

0:23:46.160 --> 0:23:48.840
<v Speaker 1>big band it's not as like a little point that exploded,

0:23:49.320 --> 0:23:52.320
<v Speaker 1>but just as an infinity going from a really dense

0:23:52.359 --> 0:23:57.640
<v Speaker 1>infinity to a bigger infinity. Yeah, And that's what cosmic

0:23:57.640 --> 0:24:01.840
<v Speaker 1>inflation is, is taking that really dense um infinity and

0:24:02.000 --> 0:24:06.320
<v Speaker 1>stretching it out to a much more dilute infinity, because

0:24:06.320 --> 0:24:09.040
<v Speaker 1>that is what we see, that's what we have evidence for, right,

0:24:09.080 --> 0:24:12.640
<v Speaker 1>Like we see that the universe is really sparse and

0:24:12.760 --> 0:24:15.159
<v Speaker 1>I'm kind of empty now, and and we see that

0:24:15.200 --> 0:24:19.320
<v Speaker 1>everything used to be much much denser. Yeah, we need

0:24:19.400 --> 0:24:21.879
<v Speaker 1>to have inflation order to explain a bunch of stuff

0:24:21.880 --> 0:24:24.120
<v Speaker 1>that we see in the universe. And we can get

0:24:24.119 --> 0:24:26.240
<v Speaker 1>into that in a few minutes if you like. But

0:24:26.520 --> 0:24:30.000
<v Speaker 1>this explains why the universe looks the way that it does.

0:24:30.440 --> 0:24:34.119
<v Speaker 1>And without inflation, the universe doesn't really make sense. Like

0:24:34.480 --> 0:24:38.200
<v Speaker 1>if you just create the universe at this current density

0:24:38.240 --> 0:24:41.920
<v Speaker 1>and said it expanding now um ten billion years ago,

0:24:42.160 --> 0:24:44.400
<v Speaker 1>it wouldn't make sense. It doesn't explain what we see.

0:24:44.440 --> 0:24:47.040
<v Speaker 1>So you need to have this inflationary period in order

0:24:47.040 --> 0:24:49.040
<v Speaker 1>to get all the sort of the clumpiness and the

0:24:49.080 --> 0:24:52.840
<v Speaker 1>structure that we see in the temperature of stuff all correct. Okay,

0:24:52.840 --> 0:24:55.920
<v Speaker 1>So I think that's another key concept about inflation, which

0:24:55.960 --> 0:24:59.160
<v Speaker 1>is that it's not you know, the universe went from

0:24:59.640 --> 0:25:03.560
<v Speaker 1>a as infinity to a wider infinity, but it didn't

0:25:03.600 --> 0:25:06.119
<v Speaker 1>do it sort of evenly, right, like there were there

0:25:06.200 --> 0:25:08.400
<v Speaker 1>was a period of time where it was really expanding

0:25:08.400 --> 0:25:11.159
<v Speaker 1>really fast, and now it's expanding but not as fast.

0:25:11.800 --> 0:25:14.239
<v Speaker 1>And so what do you call inflation? Is it that

0:25:14.440 --> 0:25:16.600
<v Speaker 1>rapid expansion or is it the whole thing, or is

0:25:16.600 --> 0:25:20.760
<v Speaker 1>it that's still kind of undecided. That's a little bit fuzzy. Yeah,

0:25:20.760 --> 0:25:23.800
<v Speaker 1>I think if you talk to most cosmologists, they would

0:25:23.800 --> 0:25:27.600
<v Speaker 1>think about inflation as this very narrow period from tend

0:25:27.640 --> 0:25:31.320
<v Speaker 1>to the minus thirty six seconds after somehow the universe

0:25:31.600 --> 0:25:34.440
<v Speaker 1>was created, to tend to the minus thirty two seconds

0:25:34.640 --> 0:25:37.119
<v Speaker 1>after the universe was created, in which you had this

0:25:37.359 --> 0:25:40.480
<v Speaker 1>enormous expansion in the universe. It seems like a factor

0:25:40.520 --> 0:25:43.520
<v Speaker 1>of ten to the twenty six. That's what they would

0:25:43.520 --> 0:25:46.240
<v Speaker 1>think of as inflation. But I'd also like to think

0:25:46.280 --> 0:25:48.480
<v Speaker 1>about what, you know, what expansion is still happening, and

0:25:48.520 --> 0:25:50.760
<v Speaker 1>so maybe this is still really part of inflation. But

0:25:50.920 --> 0:25:53.640
<v Speaker 1>that was the most dramatic moment, and so I think,

0:25:54.119 --> 0:25:56.000
<v Speaker 1>you know, if you talk about inflation, that's the moment

0:25:56.040 --> 0:25:58.520
<v Speaker 1>that people are thinking about. Oh, I see, like we're

0:25:58.560 --> 0:26:01.480
<v Speaker 1>maybe it's just at the air party of the inflation,

0:26:01.880 --> 0:26:05.160
<v Speaker 1>but you could technically maybe still call it inflation night,

0:26:05.280 --> 0:26:07.840
<v Speaker 1>you know, like the Oscar's Night. That's right, is the

0:26:07.840 --> 0:26:10.600
<v Speaker 1>celebration after the super Bowl part of the super Bowl. Yeah,

0:26:10.920 --> 0:26:14.639
<v Speaker 1>you know, but it's nothing like yeah, like the tailgating

0:26:14.680 --> 0:26:18.719
<v Speaker 1>counts as part of the event, surely, yeah, exactly. The

0:26:18.720 --> 0:26:21.359
<v Speaker 1>tailgating created the whole thing. It's only because the fans

0:26:21.400 --> 0:26:23.880
<v Speaker 1>and you can even have a super Bowl. So there

0:26:23.920 --> 0:26:26.000
<v Speaker 1>you go. And one of my favorite things about inflation

0:26:26.119 --> 0:26:28.880
<v Speaker 1>is just sort of the mind boggling numbers. We're talking

0:26:28.880 --> 0:26:31.320
<v Speaker 1>about a really brief amount of time. Tend to the

0:26:31.400 --> 0:26:35.120
<v Speaker 1>minus thirty two seconds. It's like impossible to think about.

0:26:35.119 --> 0:26:38.680
<v Speaker 1>We talked recently on a podcast about how long particles live,

0:26:39.160 --> 0:26:41.000
<v Speaker 1>and I said that they last like ten to the

0:26:41.040 --> 0:26:45.439
<v Speaker 1>minus twenty three seconds, which seems impossibly short, but you know,

0:26:45.480 --> 0:26:48.000
<v Speaker 1>compared to tend to the minus thirty six. That's a

0:26:48.119 --> 0:26:50.720
<v Speaker 1>huge amount of time. The ideas that the universe went

0:26:50.800 --> 0:26:57.400
<v Speaker 1>from almost or actually infinitely dense and infinitely dense infinity

0:26:58.000 --> 0:27:02.480
<v Speaker 1>to a less infinite lead dance infinity in a matter

0:27:02.520 --> 0:27:06.879
<v Speaker 1>of seconds or fractions of fractions of a second. And

0:27:06.920 --> 0:27:10.080
<v Speaker 1>the expansion also is incredible. I mean ten to the

0:27:10.160 --> 0:27:13.760
<v Speaker 1>twenty six expansion is hard to get your mind around. Yeah,

0:27:13.840 --> 0:27:18.120
<v Speaker 1>it would take one meter and expanded to ten billion

0:27:18.359 --> 0:27:20.760
<v Speaker 1>light years. That's what happened at the beginning of time.

0:27:21.240 --> 0:27:24.120
<v Speaker 1>Is that a meter, Like suddenly a meter became ten

0:27:24.119 --> 0:27:26.960
<v Speaker 1>billion light years. Yeah, so the stuff that's in a

0:27:27.000 --> 0:27:30.000
<v Speaker 1>meter of space got stretched out and spread out over

0:27:30.160 --> 0:27:33.560
<v Speaker 1>ten billion light years in a matter of ten to

0:27:33.760 --> 0:27:36.640
<v Speaker 1>minus thirty two seconds. Yeah, one pachinko second or whatever

0:27:36.680 --> 0:27:41.240
<v Speaker 1>that unit is second. You know, if you're a cosmology is,

0:27:41.280 --> 0:27:43.680
<v Speaker 1>you get to make up whatever terms like because you're

0:27:43.960 --> 0:27:47.440
<v Speaker 1>this is uncharted territory in terms of scientific prefixes. Right,

0:27:47.600 --> 0:27:49.199
<v Speaker 1>I think I think you should claim it right now,

0:27:49.640 --> 0:27:52.320
<v Speaker 1>go online to chink that's the sound of me claiming

0:27:52.359 --> 0:27:56.240
<v Speaker 1>pachinko second and then gaining royalties from it. Then you

0:27:56.280 --> 0:27:59.240
<v Speaker 1>get to change seconds and the other thing to wrap

0:27:59.280 --> 0:28:01.400
<v Speaker 1>your mind around is that this is stuff that's happening

0:28:01.520 --> 0:28:04.439
<v Speaker 1>faster than the speed of light. You know, light can't

0:28:04.480 --> 0:28:07.719
<v Speaker 1>travel ten billion light years in ten to the minus

0:28:07.760 --> 0:28:10.840
<v Speaker 1>thirty two seconds, obviously, right, it would take ten billion

0:28:10.920 --> 0:28:14.880
<v Speaker 1>light years years to cross that distance. That's right, even

0:28:14.880 --> 0:28:17.040
<v Speaker 1>Han Solo would take twelve par Sex to get that far.

0:28:18.600 --> 0:28:20.159
<v Speaker 1>Which hand Solo though? That do you want here? The

0:28:20.200 --> 0:28:24.600
<v Speaker 1>old of course, the old one, the original? And I

0:28:24.600 --> 0:28:26.320
<v Speaker 1>want to get a shout out to all those fans

0:28:26.359 --> 0:28:28.960
<v Speaker 1>out there who wrote in and gave me an explanation

0:28:29.240 --> 0:28:32.239
<v Speaker 1>for why Han Solo quoted his Kessel run time in

0:28:32.320 --> 0:28:36.240
<v Speaker 1>par Sex because he found a shortcut. He wasn't using

0:28:36.240 --> 0:28:38.240
<v Speaker 1>it as a measure of time. He was referring to

0:28:38.280 --> 0:28:40.520
<v Speaker 1>the fact that he took a trip near some gravitational well,

0:28:40.560 --> 0:28:43.440
<v Speaker 1>which basically shortened his trip through space. So thank you

0:28:43.480 --> 0:28:45.880
<v Speaker 1>to all those fans who educated me on the physics

0:28:45.960 --> 0:28:48.560
<v Speaker 1>of Star Wars. Sounds like a whole episode we should do,

0:28:48.920 --> 0:28:52.520
<v Speaker 1>We should, certainly. But the idea here is that space

0:28:52.560 --> 0:28:55.040
<v Speaker 1>expanded faster than the speed of light. And so for

0:28:55.080 --> 0:28:57.880
<v Speaker 1>those of you physics afficionados who are thinking, what nothing

0:28:57.920 --> 0:29:00.240
<v Speaker 1>can go fast in the speed of light, you're night

0:29:00.280 --> 0:29:02.360
<v Speaker 1>that nothing can go faster than the speed of light

0:29:02.520 --> 0:29:06.800
<v Speaker 1>through space. But there's no limit to how fast space

0:29:06.840 --> 0:29:09.600
<v Speaker 1>can expand really no limit. You think you think space

0:29:09.640 --> 0:29:14.440
<v Speaker 1>can expand infinitely. Well, it made a pretty impressive expansion

0:29:14.440 --> 0:29:16.280
<v Speaker 1>in the first few moments of the universe. I mean,

0:29:16.360 --> 0:29:18.680
<v Speaker 1>I'm impressed we are not aware of a limit. I

0:29:18.680 --> 0:29:20.840
<v Speaker 1>mean there could be a limit, but you know, we

0:29:20.880 --> 0:29:25.280
<v Speaker 1>have evidence that this expansion happened in a mind boggling speed.

0:29:25.320 --> 0:29:27.360
<v Speaker 1>So things that used to be close by, they used

0:29:27.400 --> 0:29:30.280
<v Speaker 1>to be like a meter apart, where all of a sudden,

0:29:30.880 --> 0:29:35.120
<v Speaker 1>cosmically separated. They were in their own essentially observable universes.

0:29:35.160 --> 0:29:37.280
<v Speaker 1>You know, they could no longer see each other or

0:29:37.280 --> 0:29:42.280
<v Speaker 1>communicate with each other. That's a little sad. You know,

0:29:42.440 --> 0:29:45.480
<v Speaker 1>something tore them apart. Yeah, something tore them apart. And

0:29:45.560 --> 0:29:48.720
<v Speaker 1>that's actually an important clue as to why we think

0:29:48.800 --> 0:29:52.280
<v Speaker 1>inflation happened. And you know, this kind of expansion is

0:29:52.400 --> 0:29:55.200
<v Speaker 1>the same kind of expansion that we're talking about now

0:29:55.320 --> 0:29:58.120
<v Speaker 1>that we're talking about for dark energy. You know, people

0:29:58.240 --> 0:30:01.160
<v Speaker 1>in the interviews who said, huh, in space expanding now

0:30:01.280 --> 0:30:06.320
<v Speaker 1>is cosmic inflation talking about the current expansion of the universe. Maybe, right,

0:30:06.400 --> 0:30:09.120
<v Speaker 1>that there's no difference in the kind of expansion we're

0:30:09.160 --> 0:30:12.120
<v Speaker 1>seeing now that's driven by dark energy and the kind

0:30:12.120 --> 0:30:15.280
<v Speaker 1>of expansion that we're talking about for cosmic inflation. They're

0:30:15.320 --> 0:30:20.360
<v Speaker 1>the same expansion of space, right, And so so this was,

0:30:20.840 --> 0:30:25.400
<v Speaker 1>um what we that short, super crazy period happened near

0:30:25.440 --> 0:30:29.560
<v Speaker 1>the beginning of time, and it happened really fast, but

0:30:29.600 --> 0:30:32.680
<v Speaker 1>we don't know kind of why it happened, right, We

0:30:32.720 --> 0:30:35.160
<v Speaker 1>don't know what happened, and we don't know why it

0:30:35.280 --> 0:30:38.000
<v Speaker 1>stopped happening and sort of cool off for a while,

0:30:38.480 --> 0:30:40.920
<v Speaker 1>and then we don't know why it started happening a

0:30:40.960 --> 0:30:44.520
<v Speaker 1>little bit again five billion years ago when dark energy

0:30:44.600 --> 0:30:47.120
<v Speaker 1>sort of started taking over the universe. So yeah, we

0:30:47.160 --> 0:30:50.520
<v Speaker 1>don't understand the mechanism of it at all, right, but

0:30:50.560 --> 0:30:52.920
<v Speaker 1>it is pretty crazy, and maybe that is that kind

0:30:52.920 --> 0:30:55.080
<v Speaker 1>of where the idea of a big band came from,

0:30:55.160 --> 0:30:58.400
<v Speaker 1>Like from this crazy expansion. It's almost like an explosion

0:30:58.440 --> 0:31:01.080
<v Speaker 1>of space, right, you might call it or a bang

0:31:01.120 --> 0:31:04.000
<v Speaker 1>of space, or I think the original name big Bang

0:31:04.080 --> 0:31:06.400
<v Speaker 1>came as a sort of a joke trying to mock

0:31:06.480 --> 0:31:09.440
<v Speaker 1>somebody else's scientific theory, and that was thinking of the

0:31:09.480 --> 0:31:13.040
<v Speaker 1>universe is starting from a point and an explosion through space.

0:31:13.360 --> 0:31:15.600
<v Speaker 1>And people were like, what are you suggesting as a

0:31:15.680 --> 0:31:18.200
<v Speaker 1>theory of the whole universe? Something as whimsical as that

0:31:18.320 --> 0:31:21.280
<v Speaker 1>Big Bang? You know, I think probably said with a

0:31:21.280 --> 0:31:25.560
<v Speaker 1>snotty British accident, you know exactly what the sneer, right,

0:31:26.400 --> 0:31:29.840
<v Speaker 1>the curled lip, but it caught on it like the

0:31:29.880 --> 0:31:34.680
<v Speaker 1>Big mag like the Big mag. It was catchy precisely,

0:31:34.720 --> 0:31:37.280
<v Speaker 1>and you know it has its own special sauce. And

0:31:38.960 --> 0:31:41.120
<v Speaker 1>but it is sort of it is sort incredible that

0:31:41.360 --> 0:31:43.160
<v Speaker 1>I mean, it's sort of like if you were alive

0:31:43.200 --> 0:31:45.479
<v Speaker 1>back then, it would you would not survive that, right,

0:31:45.520 --> 0:31:47.800
<v Speaker 1>It would feel like an explosion. It would feel like

0:31:47.840 --> 0:31:52.840
<v Speaker 1>this crazy violent, uh you know, sudden thing that it

0:31:52.960 --> 0:31:55.920
<v Speaker 1>just happened suddenly. Yeah, if you're two ms high, then

0:31:55.920 --> 0:31:59.840
<v Speaker 1>you would suddenly become a twenty billion light year long

0:32:00.160 --> 0:32:03.720
<v Speaker 1>staying on the universe. Right, I feel like I'm a

0:32:03.760 --> 0:32:06.480
<v Speaker 1>staying in the universe now that yeah, but you're localized,

0:32:06.880 --> 0:32:10.760
<v Speaker 1>like infinitely stayed. Do you want to be a cosmic

0:32:10.880 --> 0:32:13.719
<v Speaker 1>smear in the universe? You know? And if you are

0:32:13.760 --> 0:32:16.600
<v Speaker 1>reading that time travel device, be careful don't go back

0:32:16.600 --> 0:32:21.120
<v Speaker 1>to far because you do not want to experience cosmic inflation, right,

0:32:21.120 --> 0:32:23.640
<v Speaker 1>but you know it's it's space and time are tied together.

0:32:23.800 --> 0:32:27.000
<v Speaker 1>So is this was time also moving slower or was

0:32:27.120 --> 0:32:31.000
<v Speaker 1>time moving? Is this all measured at the same time scale?

0:32:31.480 --> 0:32:33.400
<v Speaker 1>Oh yeah, that's a great question and a deep one,

0:32:33.600 --> 0:32:36.040
<v Speaker 1>and we don't really understand. But we're measuring these things

0:32:36.080 --> 0:32:39.959
<v Speaker 1>according to our time, so our proper time. You know

0:32:40.040 --> 0:32:42.800
<v Speaker 1>what when you have experienced in terms of time, if

0:32:42.840 --> 0:32:46.040
<v Speaker 1>you're living through that period, I don't know. And we

0:32:46.040 --> 0:32:49.080
<v Speaker 1>don't really have a mechanism for explaining how this happened.

0:32:49.080 --> 0:32:51.120
<v Speaker 1>We just sort of sort of describing that it did.

0:32:51.680 --> 0:32:53.960
<v Speaker 1>And so we don't understand, like, is this part of

0:32:54.000 --> 0:32:56.480
<v Speaker 1>general relativity, there's some term you can add to the

0:32:56.480 --> 0:32:59.720
<v Speaker 1>equations of general realtivity that create this expansion, or is

0:32:59.720 --> 0:33:02.719
<v Speaker 1>it some totally different than it is stretching space? And

0:33:02.800 --> 0:33:05.000
<v Speaker 1>so the answer to how it affects time depends a

0:33:05.040 --> 0:33:07.960
<v Speaker 1>little bit on the details of what's doing it, whether

0:33:08.000 --> 0:33:12.240
<v Speaker 1>it's part of general relativity or not. I think time

0:33:12.280 --> 0:33:16.200
<v Speaker 1>itself cost inflation about that? Is that a new idea?

0:33:17.800 --> 0:33:21.320
<v Speaker 1>Lame Craig lame credit to that high fi novel. That's right,

0:33:21.360 --> 0:33:24.880
<v Speaker 1>that is officially your idea. And look forward to seeing

0:33:24.920 --> 0:33:28.280
<v Speaker 1>the paper you're writing on it. All right, let's get

0:33:28.320 --> 0:33:31.480
<v Speaker 1>into why we think costmic inflation even happened in the

0:33:31.520 --> 0:33:33.960
<v Speaker 1>first place, and let's get into what is still a

0:33:34.000 --> 0:33:50.000
<v Speaker 1>big mystery about it. But first let's take another break. Okay,

0:33:50.080 --> 0:33:53.960
<v Speaker 1>Daniel Lid we're talking about cosmic inflation, which is the

0:33:54.040 --> 0:33:56.160
<v Speaker 1>new Big Bang? Should we just call it the big

0:33:56.480 --> 0:34:03.440
<v Speaker 1>inflationary Bang, the Biggest Bang? Maybe the bangie inflation. But

0:34:03.560 --> 0:34:05.800
<v Speaker 1>so that's a crazy idea, that this idea that the

0:34:05.960 --> 0:34:11.320
<v Speaker 1>universe went from an infinitely dense infinity to a less

0:34:11.440 --> 0:34:15.600
<v Speaker 1>infinitely dense infinity in less than ten to the twenty

0:34:15.640 --> 0:34:18.760
<v Speaker 1>six seconds. That's crazy. It's crazy. But you know, the

0:34:18.880 --> 0:34:23.560
<v Speaker 1>universe and reality are no stranger to absurdity, right, They

0:34:23.560 --> 0:34:26.480
<v Speaker 1>don't care what your definition of crazy is. Yeah, and

0:34:26.640 --> 0:34:29.240
<v Speaker 1>crazy stuff has happened. And that's one of my favorite

0:34:29.239 --> 0:34:32.560
<v Speaker 1>things about physics is learning that the universe is bonkers,

0:34:32.600 --> 0:34:37.040
<v Speaker 1>bonkers beyond our imagination sometimes so it stretches our concept

0:34:37.120 --> 0:34:39.640
<v Speaker 1>of reality completely. I guess my question to you is

0:34:40.040 --> 0:34:43.160
<v Speaker 1>why do scientists think that so much happen is such

0:34:43.160 --> 0:34:46.200
<v Speaker 1>a short amount of time? You know, basically, why do

0:34:46.239 --> 0:34:49.440
<v Speaker 1>we think that the Big Bang or the inflation happened

0:34:49.440 --> 0:34:51.920
<v Speaker 1>in the first place. Yeah, well, it solves some problems.

0:34:52.000 --> 0:34:54.000
<v Speaker 1>It explains some of the things that we see that

0:34:54.120 --> 0:34:56.480
<v Speaker 1>we can't otherwise resolve. I mean, you might come up

0:34:56.480 --> 0:34:59.879
<v Speaker 1>with another theory that explains what we see out there,

0:35:00.000 --> 0:35:01.719
<v Speaker 1>but it has to explain all the stuff that we

0:35:01.760 --> 0:35:04.279
<v Speaker 1>see and tie up all the loose ends. And one

0:35:04.280 --> 0:35:06.440
<v Speaker 1>of the things is what we mentioned earlier on is

0:35:06.480 --> 0:35:08.719
<v Speaker 1>that we seem to be at the center of the

0:35:08.840 --> 0:35:11.719
<v Speaker 1>universe and that doesn't make sense. And the the hot Big

0:35:11.760 --> 0:35:14.440
<v Speaker 1>Bang model we have a point that explodes out, but

0:35:14.520 --> 0:35:17.719
<v Speaker 1>it does explain what we see if the whole universe

0:35:17.840 --> 0:35:21.320
<v Speaker 1>was infinite and expanded out everywhere at once, because then

0:35:21.440 --> 0:35:24.000
<v Speaker 1>everywhere looks like it's at the center of the universe.

0:35:24.400 --> 0:35:26.080
<v Speaker 1>It's like you're in the middle of a loaf of

0:35:26.120 --> 0:35:29.040
<v Speaker 1>bread and all the reasons as it's baking, all the

0:35:29.080 --> 0:35:31.479
<v Speaker 1>reasons are moving away from you. That's true, no matter

0:35:31.520 --> 0:35:34.760
<v Speaker 1>where you are in this infinite loaf of bread. Yeah,

0:35:34.840 --> 0:35:37.120
<v Speaker 1>it's like being in a rubber sheet. Right when you

0:35:37.160 --> 0:35:40.200
<v Speaker 1>stretch it out wherever you stand, it looks like everything's

0:35:40.200 --> 0:35:44.320
<v Speaker 1>blooming away from you. Yeah, exactly, And and that's pretty compelling.

0:35:44.719 --> 0:35:46.680
<v Speaker 1>But then you might ask, all right, well, that just

0:35:46.800 --> 0:35:49.120
<v Speaker 1>requires that the universe is infinite and it is filled

0:35:49.160 --> 0:35:51.000
<v Speaker 1>with an infor amount of stuff. Why do you think

0:35:51.040 --> 0:35:54.720
<v Speaker 1>it had this crazy expansion? And part of that comes

0:35:54.800 --> 0:35:56.840
<v Speaker 1>with what we see out there in the universe is

0:35:56.880 --> 0:35:59.839
<v Speaker 1>that the universe is pretty smooth. I mean, there are

0:36:00.040 --> 0:36:02.880
<v Speaker 1>clumps and galaxies and solar systems. Will get into that

0:36:02.960 --> 0:36:05.560
<v Speaker 1>in a moment, but if you average out over it,

0:36:05.920 --> 0:36:09.000
<v Speaker 1>it looks pretty smooth. And most specifically, if you look

0:36:09.040 --> 0:36:13.120
<v Speaker 1>at this cosmic microwave background radiation, this light we've talked

0:36:13.120 --> 0:36:16.400
<v Speaker 1>about that comes from like three hundred thousand years after

0:36:16.800 --> 0:36:19.440
<v Speaker 1>the Big Bang, when the universe was a hot plasma.

0:36:19.960 --> 0:36:22.040
<v Speaker 1>We see that light and we use that light to

0:36:22.080 --> 0:36:24.680
<v Speaker 1>measure it's sort of the temperature of the universe by

0:36:24.719 --> 0:36:29.760
<v Speaker 1>the frequency of the light. And it's really really, really smooth.

0:36:30.320 --> 0:36:32.839
<v Speaker 1>Like it looks like the universe was basically the same

0:36:32.960 --> 0:36:36.960
<v Speaker 1>temperature everywhere. And that's weird. It's it's very even, right,

0:36:37.040 --> 0:36:39.640
<v Speaker 1>It's like it it all, it all looks the same

0:36:39.719 --> 0:36:42.919
<v Speaker 1>almost from every direction. Yeah, it looks like a smooth bath,

0:36:43.480 --> 0:36:46.719
<v Speaker 1>you know. It looks like the temperature varies by one

0:36:46.840 --> 0:36:48.960
<v Speaker 1>part in a hundred thousand or one part in ten

0:36:49.080 --> 0:36:51.880
<v Speaker 1>thousand from here to there to the other place. And

0:36:51.960 --> 0:36:55.200
<v Speaker 1>you might be thinking, well, what what's weird about that? Right, Well,

0:36:55.280 --> 0:36:57.800
<v Speaker 1>it's weird from the point of view that those things

0:36:58.120 --> 0:37:02.080
<v Speaker 1>are cosmically far upon heart. If you look at light

0:37:02.160 --> 0:37:04.800
<v Speaker 1>that's coming to us from one direction in the cosmic

0:37:04.880 --> 0:37:08.120
<v Speaker 1>micro background radiation, it's been traveling the whole history of

0:37:08.120 --> 0:37:10.759
<v Speaker 1>the universe, just got here. If you look from the

0:37:10.840 --> 0:37:13.920
<v Speaker 1>other direction, life coming from the other direction has also

0:37:14.000 --> 0:37:16.759
<v Speaker 1>been traveling the whole history universe and just got here.

0:37:17.080 --> 0:37:19.359
<v Speaker 1>So it's the first time they ever met, right from

0:37:19.400 --> 0:37:22.120
<v Speaker 1>different ends of the universe. Right, one of them came

0:37:22.160 --> 0:37:24.200
<v Speaker 1>from the left edge of the universe and the other

0:37:24.239 --> 0:37:27.160
<v Speaker 1>one came from the right edge of the right. Yeah, well,

0:37:27.200 --> 0:37:29.760
<v Speaker 1>even if there aren't any edges, they came from totally

0:37:29.840 --> 0:37:32.600
<v Speaker 1>separated spots, spots that have not had time to talk

0:37:32.680 --> 0:37:35.200
<v Speaker 1>to each other or communicate in any way since the

0:37:35.280 --> 0:37:40.640
<v Speaker 1>beginning of the universe. Right, that's weird. That's weird because

0:37:40.719 --> 0:37:42.759
<v Speaker 1>they're the same temperature, and the only way you can

0:37:42.840 --> 0:37:45.520
<v Speaker 1>get stuff to be the same temperature is to let

0:37:45.600 --> 0:37:48.440
<v Speaker 1>it mix, Right, Like if you put an ice cube

0:37:48.760 --> 0:37:52.160
<v Speaker 1>into hot water, then you have a cold spot in

0:37:52.320 --> 0:37:54.919
<v Speaker 1>your water, and you have to wait for things to mix,

0:37:55.000 --> 0:37:57.520
<v Speaker 1>for the temperature to get so even. And so it

0:37:57.719 --> 0:38:00.320
<v Speaker 1>looks like the universe had a chance to mix. It

0:38:00.440 --> 0:38:05.000
<v Speaker 1>looks like the temperature smoothed out. But how did that happen?

0:38:05.160 --> 0:38:07.239
<v Speaker 1>Because these things have never had a chance to talk

0:38:07.280 --> 0:38:09.640
<v Speaker 1>to each other before. Why what? What if it touch

0:38:09.680 --> 0:38:13.000
<v Speaker 1>is how the universe was before? Yeah, it could be.

0:38:13.360 --> 0:38:16.920
<v Speaker 1>You know, a lot of these problems are sort of aesthetic.

0:38:17.200 --> 0:38:19.200
<v Speaker 1>You're like, well, I don't really get it. I don't

0:38:19.280 --> 0:38:21.520
<v Speaker 1>like that assumption. And so you could say, well, the

0:38:21.600 --> 0:38:25.319
<v Speaker 1>universe were just created like perfectly smooth. Yeah, just came

0:38:25.400 --> 0:38:29.719
<v Speaker 1>off the factory floor, nice and nice and toasty. Yeah,

0:38:29.880 --> 0:38:33.800
<v Speaker 1>nice and toasty. It's not exactly smooth. We see little

0:38:33.960 --> 0:38:37.640
<v Speaker 1>clumps in there, and the distribution of those clumps is

0:38:37.680 --> 0:38:40.640
<v Speaker 1>another thing that's explained by inflation. But you're right, this,

0:38:41.000 --> 0:38:45.920
<v Speaker 1>you know, by itself, this smoothness problem is not completely bulletproof. Right.

0:38:45.920 --> 0:38:49.240
<v Speaker 1>You could say, maybe the universe was just created almost

0:38:49.280 --> 0:38:52.640
<v Speaker 1>perfectly smooth, like maybe when photons are creative at the beginning,

0:38:53.080 --> 0:38:55.600
<v Speaker 1>they all have the same temperature. There would be another

0:38:55.600 --> 0:38:57.000
<v Speaker 1>way to explain it. There would be another way to

0:38:57.040 --> 0:39:00.080
<v Speaker 1>explain it. But the explanation that comes from inflation and

0:39:00.760 --> 0:39:03.879
<v Speaker 1>is that these things did once have a chance to mix.

0:39:04.000 --> 0:39:07.440
<v Speaker 1>That you know, before inflation, these photons, which were ten

0:39:07.520 --> 0:39:10.480
<v Speaker 1>billion light years apart, were only a meter apart. And

0:39:10.600 --> 0:39:13.040
<v Speaker 1>so there's a lot of time in this early plasma

0:39:13.120 --> 0:39:15.359
<v Speaker 1>for stuff to slash around and for things to get

0:39:15.440 --> 0:39:18.160
<v Speaker 1>smoothed out and for the universe to get to an

0:39:18.239 --> 0:39:23.239
<v Speaker 1>even temperature before things got inflated. Right, And so I

0:39:23.320 --> 0:39:25.920
<v Speaker 1>think I remember this that the the the way that

0:39:26.000 --> 0:39:28.640
<v Speaker 1>this explains it. It is that you need this kind

0:39:28.680 --> 0:39:33.560
<v Speaker 1>of rapid and violent expansion of space to basically take

0:39:33.640 --> 0:39:38.160
<v Speaker 1>the left edge photon and the right edge photon far

0:39:38.360 --> 0:39:42.120
<v Speaker 1>enough apart where it makes sense now. Yeah, so these

0:39:42.160 --> 0:39:45.000
<v Speaker 1>two have had to been inside the same sort of

0:39:45.200 --> 0:39:49.600
<v Speaker 1>cosmic horizon before, and now they're outside the cosmic horizon.

0:39:50.160 --> 0:39:53.719
<v Speaker 1>Cosmic horizon is something that is so far away that

0:39:54.000 --> 0:39:56.839
<v Speaker 1>you have not seen it because light from it has

0:39:56.920 --> 0:39:59.600
<v Speaker 1>never reached you in the history of the universe. Right,

0:39:59.640 --> 0:40:02.200
<v Speaker 1>there's a no way they could have talked before, And

0:40:02.320 --> 0:40:05.719
<v Speaker 1>yet it seems like they had have talked before. And

0:40:05.880 --> 0:40:08.319
<v Speaker 1>the expansion of space faster than the speed of light

0:40:08.440 --> 0:40:09.839
<v Speaker 1>is the thing that can do that. It can take

0:40:09.920 --> 0:40:13.239
<v Speaker 1>things that were inside the same cosmic horizon, right, that

0:40:13.280 --> 0:40:15.400
<v Speaker 1>are close enough to interact and talk to each other,

0:40:15.480 --> 0:40:18.359
<v Speaker 1>and smooth them become the same temperature, and push them

0:40:18.400 --> 0:40:21.359
<v Speaker 1>apart into their own separate cosmic horizons so that they

0:40:21.680 --> 0:40:24.120
<v Speaker 1>can no longer interact. And so that's what we think

0:40:24.160 --> 0:40:27.160
<v Speaker 1>we see now is that light from this from two

0:40:27.239 --> 0:40:30.839
<v Speaker 1>directions in the universe is now the same temperature, even

0:40:30.920 --> 0:40:33.640
<v Speaker 1>though without cosmic inflation, we don't think that they could

0:40:33.719 --> 0:40:36.360
<v Speaker 1>ever have met, right, It's like it's like a crazy

0:40:36.440 --> 0:40:38.400
<v Speaker 1>thing you've see in the universe that can only be

0:40:38.520 --> 0:40:43.200
<v Speaker 1>explained apparently by this crazy idea of inflation. Yeah, precisely.

0:40:43.719 --> 0:40:47.520
<v Speaker 1>That's one reason why we like inflation. It explains that.

0:40:48.280 --> 0:40:52.440
<v Speaker 1>And more specifically, the universe is not all the same temperature.

0:40:52.560 --> 0:40:55.200
<v Speaker 1>If you look at the cosmic microwave background radiation, this

0:40:55.400 --> 0:40:57.960
<v Speaker 1>light from the early universe, we said, it's like the

0:40:58.080 --> 0:41:00.239
<v Speaker 1>same too, within one in ten thousand, one in a

0:41:00.320 --> 0:41:04.319
<v Speaker 1>hundred thousand. Those wiggles are actually important. Those those deviations

0:41:04.440 --> 0:41:07.640
<v Speaker 1>from being exactly the same temperature are really important, and

0:41:08.080 --> 0:41:11.240
<v Speaker 1>we study those really carefully because those are the seeds

0:41:11.440 --> 0:41:13.880
<v Speaker 1>of the rest of the universe, right, that they're the

0:41:14.080 --> 0:41:18.600
<v Speaker 1>wrinkles that came from basically this giant stretching of the universe. Yeah,

0:41:18.680 --> 0:41:22.080
<v Speaker 1>those those wrinkles came from the giant stretching. And you

0:41:22.160 --> 0:41:25.400
<v Speaker 1>might wonder, like, all right, say the universe was created

0:41:25.560 --> 0:41:28.520
<v Speaker 1>perfectly smoothly, like you were saying earlier, Right, why couldn't

0:41:28.560 --> 0:41:31.400
<v Speaker 1>just come off the factory floor, like totally homogeneous. Well,

0:41:31.440 --> 0:41:33.960
<v Speaker 1>if you have a universe like that, then you never

0:41:34.120 --> 0:41:36.800
<v Speaker 1>get any sort of clumping. You don't get anything like

0:41:37.080 --> 0:41:41.000
<v Speaker 1>solar systems and hamsters and galaxies and stuff, because everything

0:41:41.120 --> 0:41:44.439
<v Speaker 1>is perfectly smooth and there's no place where things start

0:41:44.520 --> 0:41:47.280
<v Speaker 1>to clump together. To get any sort of clumping or structure,

0:41:47.600 --> 0:41:50.600
<v Speaker 1>you need something and that's not homogeneous, right, And so

0:41:50.960 --> 0:41:54.800
<v Speaker 1>you're saying, inflation is our only explanation for why the

0:41:54.960 --> 0:41:59.640
<v Speaker 1>universe is smooth and clumpy just the right amount that

0:41:59.840 --> 0:42:02.120
<v Speaker 1>we see it right now. That's right, because in physics

0:42:02.200 --> 0:42:06.200
<v Speaker 1>we have only one way to introduce random clumpiness, and

0:42:06.320 --> 0:42:09.840
<v Speaker 1>that's quantum mechanics. So the idea is the universe was

0:42:09.880 --> 0:42:14.719
<v Speaker 1>really really dense and perfectly smooth, and then quantum fluctuations

0:42:14.760 --> 0:42:16.440
<v Speaker 1>just like created a few particles here and a few

0:42:16.480 --> 0:42:19.400
<v Speaker 1>particles there. Now, normally, when that happens, and it's happening

0:42:19.440 --> 0:42:21.360
<v Speaker 1>all the time, it's not a big deal because there

0:42:21.400 --> 0:42:23.440
<v Speaker 1>are the quantum level so you don't see them. But

0:42:24.160 --> 0:42:27.400
<v Speaker 1>what if just when you're making those fluctuations, the universe

0:42:27.480 --> 0:42:30.759
<v Speaker 1>decides I'm gonna blow this up to ten billion light years?

0:42:31.160 --> 0:42:34.480
<v Speaker 1>Then all of a sudden, tiny little quantum fluctuations become

0:42:34.560 --> 0:42:39.200
<v Speaker 1>really big cosmic fluctuations, right, they become spread out over

0:42:39.320 --> 0:42:43.600
<v Speaker 1>the whole cosmos. Then they're big enough to seed gravity,

0:42:43.680 --> 0:42:46.840
<v Speaker 1>to get things moving, to clump stuff together. Right and

0:42:46.960 --> 0:42:51.000
<v Speaker 1>if so, so, if an inflation was not as dramatic,

0:42:51.600 --> 0:42:55.319
<v Speaker 1>then we wouldn't see those quantum fluctuations, right, because let's

0:42:55.360 --> 0:43:00.640
<v Speaker 1>say that inflation had actually taken longer than you wouldn't

0:43:00.840 --> 0:43:03.799
<v Speaker 1>you know, it wouldn't stretch those quantum fluctuations because things

0:43:03.840 --> 0:43:07.080
<v Speaker 1>would even out before you stretch out to the to

0:43:07.200 --> 0:43:09.120
<v Speaker 1>what we see now. Yeah, And that's why you need

0:43:09.160 --> 0:43:11.600
<v Speaker 1>to have inflation happened at the scale that had happened

0:43:11.680 --> 0:43:14.719
<v Speaker 1>like so dramatically and so quickly. You've got to catch

0:43:15.040 --> 0:43:20.160
<v Speaker 1>those quantum fluctuations with their pants down. Otherwise it doesn't

0:43:20.200 --> 0:43:23.520
<v Speaker 1>explain the universe were in. That's right, Their cosmic embarrassment

0:43:23.640 --> 0:43:27.160
<v Speaker 1>is the reason why we are here. Yeah, that's sort

0:43:27.200 --> 0:43:30.200
<v Speaker 1>of basically right, right, Like, it's like you needed to

0:43:30.280 --> 0:43:33.160
<v Speaker 1>catch the universe just the right time with this crazy

0:43:33.239 --> 0:43:37.000
<v Speaker 1>expansion like this photograph in order to explain what we

0:43:37.080 --> 0:43:39.400
<v Speaker 1>see now. Yeah, And we talked on the podcast recently

0:43:39.440 --> 0:43:43.040
<v Speaker 1>about another possibility, another different idea, which was cosmic strings.

0:43:43.120 --> 0:43:45.840
<v Speaker 1>People thought, maybe cosmic strings are the reason why we

0:43:45.920 --> 0:43:48.240
<v Speaker 1>see this sort of distribution of stuff in the universe,

0:43:48.600 --> 0:43:50.719
<v Speaker 1>but people look at them more carefully and it doesn't work.

0:43:50.920 --> 0:43:53.520
<v Speaker 1>You don't get this sort of the right kind of wiggles,

0:43:53.560 --> 0:43:55.880
<v Speaker 1>you don't get the right distribution of stuff here and

0:43:55.920 --> 0:43:59.680
<v Speaker 1>stuff there. But inflation gets it just right. Inflation says,

0:44:00.000 --> 0:44:02.480
<v Speaker 1>if you had that really dense plasma and then you

0:44:02.560 --> 0:44:04.960
<v Speaker 1>blew it up really quickly, you would expect to get

0:44:05.160 --> 0:44:07.359
<v Speaker 1>just the right density of stuff to form the kind

0:44:07.440 --> 0:44:10.480
<v Speaker 1>of structure that we see today, And there's no other

0:44:10.600 --> 0:44:13.440
<v Speaker 1>way to explain it in such fine detail that we know.

0:44:13.719 --> 0:44:16.160
<v Speaker 1>I mean, there are some other crazier ideas, but none

0:44:16.160 --> 0:44:18.160
<v Speaker 1>of them work as well as inflation, right, Yeah, Like,

0:44:18.239 --> 0:44:21.240
<v Speaker 1>if inflation at lasts it tended to the negative thirty

0:44:21.360 --> 0:44:24.360
<v Speaker 1>one seconds instead of tend to negative thirty two seconds,

0:44:24.920 --> 0:44:27.479
<v Speaker 1>then you and I wouldn't be here. Yeah, it would

0:44:27.480 --> 0:44:30.080
<v Speaker 1>be some other podcasts which would be not nearly as funny.

0:44:32.000 --> 0:44:34.560
<v Speaker 1>It would probably be over quicker. But there's a there's

0:44:34.600 --> 0:44:37.080
<v Speaker 1>some something else there. There's a real randomness right, Like

0:44:37.520 --> 0:44:39.839
<v Speaker 1>it tells you that the structure to universe, Like why

0:44:39.880 --> 0:44:44.239
<v Speaker 1>does a galaxy here comes from some like electron fluctuating

0:44:44.280 --> 0:44:47.120
<v Speaker 1>out of the vacuum fourteen billion years ago, And if

0:44:47.120 --> 0:44:49.080
<v Speaker 1>it had fluctuated in a different direction, we'd have a

0:44:49.200 --> 0:44:53.120
<v Speaker 1>different galaxy somewhere else. Like those tiny little quantum rolls

0:44:53.160 --> 0:44:57.440
<v Speaker 1>of the dye determine the specific structure of our universe today.

0:44:57.920 --> 0:45:02.000
<v Speaker 1>It mind boggling to think about. And they're super sensitive, right,

0:45:02.040 --> 0:45:06.440
<v Speaker 1>and totally random, super sensitive and totally random. Yeah. Wow.

0:45:06.920 --> 0:45:09.120
<v Speaker 1>So we we are lucky to have the universe we

0:45:09.239 --> 0:45:12.120
<v Speaker 1>have right now, and you listeners are lucky to have us, frankly,

0:45:12.840 --> 0:45:15.680
<v Speaker 1>and we are lucky to have you. We are very

0:45:15.719 --> 0:45:18.479
<v Speaker 1>glad that you fluctuated into existence. We are all lucky

0:45:18.560 --> 0:45:21.239
<v Speaker 1>to have each other. I think is the new theme

0:45:21.280 --> 0:45:24.799
<v Speaker 1>for Okay cool. I feel like I really understand there's

0:45:24.800 --> 0:45:27.160
<v Speaker 1>a little bit more, you know. It's it's like this

0:45:27.360 --> 0:45:32.200
<v Speaker 1>idea of an infinite infinity going less dense is and

0:45:32.480 --> 0:45:34.319
<v Speaker 1>very quickly in order to explain what we have now.

0:45:35.280 --> 0:45:37.479
<v Speaker 1>So does that mean, Daniel, that we know everything about

0:45:37.520 --> 0:45:39.560
<v Speaker 1>inflation and what happened at the beginning of time? Or

0:45:39.640 --> 0:45:42.160
<v Speaker 1>are there still things we don't know? There's not an

0:45:42.280 --> 0:45:44.800
<v Speaker 1>infinite amount of stuff that we don't know about inflation,

0:45:45.920 --> 0:45:48.200
<v Speaker 1>infinitely amount of stuff we don't know about an infinite

0:45:48.719 --> 0:45:51.880
<v Speaker 1>lead dance infinity that gets less infinite. Yeah, as our

0:45:52.000 --> 0:45:54.440
<v Speaker 1>knowledge grows, it feels like our ignorance is also growing,

0:45:54.560 --> 0:45:57.439
<v Speaker 1>or like our knowledge of our ignorance is inflating as well,

0:45:57.600 --> 0:46:00.400
<v Speaker 1>you know. But that's the fun part about science. I

0:46:00.520 --> 0:46:03.880
<v Speaker 1>think the biggest mystery about inflation is like what caused it?

0:46:04.040 --> 0:46:07.520
<v Speaker 1>What made it happen? What could possibly expand space at

0:46:07.600 --> 0:46:10.920
<v Speaker 1>this crazy rate? Right? Like why didn't the universe just

0:46:11.040 --> 0:46:13.239
<v Speaker 1>stay the way it was before? Why did it have

0:46:13.440 --> 0:46:16.239
<v Speaker 1>to have this crazy expansion? Yeah, and why did the

0:46:16.280 --> 0:46:19.520
<v Speaker 1>expansion stop? And so as usual, we don't have any idea,

0:46:19.560 --> 0:46:22.879
<v Speaker 1>but we've already given it a name, and of course yeah,

0:46:22.880 --> 0:46:27.960
<v Speaker 1>we've we've called it the infloton not a joke. I

0:46:28.040 --> 0:46:31.120
<v Speaker 1>know it sounds like I'm making that up. But created

0:46:31.200 --> 0:46:33.839
<v Speaker 1>this field called the infloton field, which would have an

0:46:33.840 --> 0:46:37.279
<v Speaker 1>infloton particle, and the ideas that this field causes this

0:46:37.480 --> 0:46:40.840
<v Speaker 1>crazy expansion. It sort of just puts off the question like,

0:46:40.920 --> 0:46:43.560
<v Speaker 1>all right, well, what creates the inflotton field and what

0:46:43.680 --> 0:46:46.160
<v Speaker 1>controls it? Well, we have no idea, but it's just

0:46:46.239 --> 0:46:49.280
<v Speaker 1>sort of like a place to put our ideas. Interesting,

0:46:49.640 --> 0:46:52.320
<v Speaker 1>So we owe our existence and our universe to the

0:46:52.480 --> 0:46:55.239
<v Speaker 1>infloton Yeah, and the infloton The idea there is like

0:46:55.600 --> 0:46:58.560
<v Speaker 1>the universe is filled with this infloton field, which expands

0:46:58.640 --> 0:47:04.000
<v Speaker 1>space and sort of decays into ordinary matter. And that's

0:47:04.000 --> 0:47:06.359
<v Speaker 1>how you get ordinary matter. You have in photon field,

0:47:06.360 --> 0:47:09.719
<v Speaker 1>which then turns into corks and electrons and other kinds

0:47:09.760 --> 0:47:13.240
<v Speaker 1>of fields. Um. And we don't know like what would

0:47:13.400 --> 0:47:16.000
<v Speaker 1>cause that decay, Like that's when inflation stops, is when

0:47:16.040 --> 0:47:18.440
<v Speaker 1>it turns into normal matter. But we don't know like

0:47:18.719 --> 0:47:21.319
<v Speaker 1>why would it stopped and or why was it there

0:47:21.360 --> 0:47:23.200
<v Speaker 1>in the first place? Yeah, what was there first place?

0:47:23.400 --> 0:47:27.200
<v Speaker 1>And also did it stop? Like there might be it

0:47:27.320 --> 0:47:30.000
<v Speaker 1>might be that inflation sort of stopped in our part

0:47:30.040 --> 0:47:33.080
<v Speaker 1>of the universe, but it's still going on in other

0:47:33.239 --> 0:47:35.840
<v Speaker 1>parts of the universe. Could be the rest of the universe.

0:47:35.880 --> 0:47:38.360
<v Speaker 1>We're like in a little bubble, a pocket universe, and

0:47:38.440 --> 0:47:41.320
<v Speaker 1>the rest of the universe is still inflating. And imagine

0:47:41.320 --> 0:47:43.640
<v Speaker 1>how far If it got that far in ten of

0:47:43.680 --> 0:47:45.800
<v Speaker 1>the minus thirty two seconds, imagine what it could do

0:47:45.880 --> 0:47:50.160
<v Speaker 1>in fourteen billion years. Wow. So you're saying that maybe

0:47:50.320 --> 0:47:55.120
<v Speaker 1>we are even more insignificant than we had previously imagined. Yeah,

0:47:55.200 --> 0:47:57.760
<v Speaker 1>that's this idea. It's called eternal inflation. That the universe

0:47:57.920 --> 0:48:02.480
<v Speaker 1>is continuously inflating, and occasionally the inflation sort of decays

0:48:02.560 --> 0:48:04.279
<v Speaker 1>into normal matter, and then you get the kind of

0:48:04.360 --> 0:48:06.880
<v Speaker 1>universe we're familiar with, but that most of the universe

0:48:07.280 --> 0:48:11.840
<v Speaker 1>is just this massively expanding infloton field. Wait, are you saying, Daniel,

0:48:11.880 --> 0:48:15.719
<v Speaker 1>that the infloton works in mysterious ways? I'm saying exactly that,

0:48:16.200 --> 0:48:18.600
<v Speaker 1>mostly because we don't understand it at all, And so

0:48:19.080 --> 0:48:21.200
<v Speaker 1>can I start a new religion based on the infloton?

0:48:22.760 --> 0:48:25.120
<v Speaker 1>Are you the high priest of the inflation here? Yeah,

0:48:25.400 --> 0:48:27.920
<v Speaker 1>because I am both the high priest and the parishioner

0:48:28.400 --> 0:48:31.200
<v Speaker 1>of my church of the Inflaton. Yes, please donate to

0:48:31.440 --> 0:48:35.720
<v Speaker 1>the Church of the Inflaton. I think we just replaced

0:48:35.760 --> 0:48:39.080
<v Speaker 1>the spagetti master. Yeah, and so of course this feels

0:48:39.120 --> 0:48:41.040
<v Speaker 1>like a big place holder because it is we don't know,

0:48:41.239 --> 0:48:44.680
<v Speaker 1>and so it's just a way to say, if inflation happened,

0:48:45.160 --> 0:48:47.239
<v Speaker 1>what's a possible way it might have happened. And then

0:48:47.320 --> 0:48:50.120
<v Speaker 1>let's start to get to work on, you know, figuring

0:48:50.160 --> 0:48:52.440
<v Speaker 1>out how that theory has to look. Step one, give

0:48:52.480 --> 0:48:56.319
<v Speaker 1>it a science names and then figure it out. Step

0:48:56.400 --> 0:49:02.919
<v Speaker 1>to get ridiculed by Jorge. Step three, get to work alright. Cool,

0:49:02.920 --> 0:49:05.320
<v Speaker 1>It sounds like there's still lots of answers to be

0:49:05.480 --> 0:49:08.360
<v Speaker 1>found in this and these are important answers, right, I

0:49:08.400 --> 0:49:11.640
<v Speaker 1>mean they're they're about the beginning of the universe and

0:49:11.840 --> 0:49:14.000
<v Speaker 1>why are things the way they are? And are things

0:49:14.040 --> 0:49:16.320
<v Speaker 1>going to change in the future. And you know, I

0:49:16.400 --> 0:49:18.279
<v Speaker 1>think in ten years or in twenty years, people will

0:49:18.280 --> 0:49:20.600
<v Speaker 1>look back at these ideas and think, oh, my gosh,

0:49:20.680 --> 0:49:23.800
<v Speaker 1>how absurd. I can't believe they really believe that stuff.

0:49:24.320 --> 0:49:26.839
<v Speaker 1>Because we're going to learn things about inflation, and we're

0:49:26.840 --> 0:49:28.640
<v Speaker 1>going to learn things about the history of the universe

0:49:28.680 --> 0:49:30.640
<v Speaker 1>and its current expansion that are going to give us

0:49:30.880 --> 0:49:33.759
<v Speaker 1>better ideas, even crazier ideas that are going to be

0:49:33.840 --> 0:49:37.320
<v Speaker 1>even more correct. And so this is the perfect example

0:49:37.400 --> 0:49:40.400
<v Speaker 1>of how our knowledge of the universe is constantly expanding.

0:49:40.480 --> 0:49:43.160
<v Speaker 1>We look back and think, wow, how silly. Yeah, you

0:49:43.200 --> 0:49:47.640
<v Speaker 1>know they say twenties smart physicists are twenty thirties ignoratons.

0:49:48.640 --> 0:49:52.480
<v Speaker 1>That's right, Yeah, I have twenty twenty vision, which means

0:49:52.600 --> 0:49:54.839
<v Speaker 1>I look back at ten and think one a bunch

0:49:54.880 --> 0:50:00.759
<v Speaker 1>of ideas. Well, I can't wait to have visions. That's

0:50:00.800 --> 0:50:02.480
<v Speaker 1>what happens in our old age, right, we all get

0:50:02.520 --> 0:50:06.000
<v Speaker 1>reading to us is all right? Well, maybe we'll get

0:50:06.040 --> 0:50:08.840
<v Speaker 1>into these mysteries a little bit deeper in the future podcast,

0:50:09.000 --> 0:50:11.279
<v Speaker 1>but for now, thanks for joining us. We hope you

0:50:11.360 --> 0:50:13.799
<v Speaker 1>enjoyed that. We hope we inflated your mind and took

0:50:13.840 --> 0:50:16.200
<v Speaker 1>you on a tour of the early universe. Thank you

0:50:16.320 --> 0:50:26.360
<v Speaker 1>very much. Before you still have a question after listening

0:50:26.400 --> 0:50:29.439
<v Speaker 1>to all these explanations, please drop us a line. We'd

0:50:29.560 --> 0:50:32.320
<v Speaker 1>love to hear from you. You can find us on Facebook, Twitter,

0:50:32.440 --> 0:50:36.080
<v Speaker 1>and Instagram at Daniel and Jorge that's one word, or

0:50:36.239 --> 0:50:39.600
<v Speaker 1>email us at Feedback at Daniel and Jorge dot com.

0:50:40.200 --> 0:50:43.000
<v Speaker 1>Thanks for listening, and remember that Daniel and Jorge Explain

0:50:43.080 --> 0:50:45.920
<v Speaker 1>the Universe is a production of I heart Radio. For

0:50:46.080 --> 0:50:49.000
<v Speaker 1>more podcast from my heart Radio, visit the i heart

0:50:49.120 --> 0:50:52.680
<v Speaker 1>Radio app, Apple Podcasts, or wherever you listen to your

0:50:52.719 --> 0:50:53.440
<v Speaker 1>favorite shows.