WEBVTT - How does gravity escape a black hole?

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<v Speaker 1>Hey, Katie, have you ever been to Las Vegas? I

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<v Speaker 1>have once, and so what did you think about America's

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<v Speaker 1>favorite adult playground?

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<v Speaker 2>Well, I can't really tell you.

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<v Speaker 1>Is that because it was so much fun you remember nothing?

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<v Speaker 2>I mean, it is a bit of an information black hole.

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<v Speaker 1>You mean, like you don't want to talk about it.

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<v Speaker 1>Like what happens in Vegas stays in Vegas.

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<v Speaker 2>It is a singular experience for sure.

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<v Speaker 1>All right, we'll leave that past. The Katie event arrived.

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<v Speaker 2>Like they're just handing out margarite?

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<v Speaker 3>Is there? What am I supposed to say?

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<v Speaker 4>Hi?

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<v Speaker 1>I'm Daniel. I'm a particle physicist and a professor at

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<v Speaker 1>UC Irvine, and I have definitely been to Vegas.

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<v Speaker 2>I am Katie Golden, I am made out of particles.

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<v Speaker 2>I host a podcast about animals, and I mostly liked

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<v Speaker 2>the food from Las Vegas, not so much the casinos.

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<v Speaker 1>I recently went to Vegas with my thirteen year old daughter,

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<v Speaker 1>which was quite an experience to see it through her eyes.

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<v Speaker 1>Definitely a place to go at least once.

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<v Speaker 2>It is a fascinating city. I regret that I have

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<v Speaker 2>not been there since they have put the giant orban.

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<v Speaker 1>Yeah, the orb is cool. There's definitely a lot of

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<v Speaker 1>stuff you can do even if you're not eighteen or

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<v Speaker 1>twenty one plus, though some of the stuff she wanted

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<v Speaker 1>to do, like drive tanks through the desert and shoot

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<v Speaker 1>automatic weapons were definitely age restricted.

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<v Speaker 2>Yeah, I have a friend who I think shot guns

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<v Speaker 2>from a helicopter in Vegas. There's a lot of things

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<v Speaker 2>you can do.

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<v Speaker 1>There's all sorts of crazy stuff you can do in Vegas,

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<v Speaker 1>stuff that helps you understand who you are and who

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<v Speaker 1>you aren't. And Welcome to the podcast Daniel and Jorge

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<v Speaker 1>Explain the Universe, in which we try to explain to

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<v Speaker 1>you what the universe is and what the universe isn't.

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<v Speaker 1>We try to pull back the curtain and help you

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<v Speaker 1>understand what's going on out there in the deepest, darkest

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<v Speaker 1>regions of.

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<v Speaker 2>Space, such as Las Vegas.

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<v Speaker 1>There is no Vegas casino yet called the black Hole,

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<v Speaker 1>but I am assuming one it will eventually open up.

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<v Speaker 2>That is a missed opportunity, or like a mini golf

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<v Speaker 2>course called the black.

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<v Speaker 1>Holes that just sucks in all the balls. Well, on

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<v Speaker 1>this podcast, we do try to explain to you black

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<v Speaker 1>holes and also how everything works on the smallest scales

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<v Speaker 1>because we don't just want to describe the universe to you.

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<v Speaker 1>We want to explain it. We want you to get

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<v Speaker 1>an understanding, a microscopic picture of how everything around you

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<v Speaker 1>actually works. We want to dive deep into the very

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<v Speaker 1>nature of reality and come out with a bottom up

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<v Speaker 1>understanding of how the universe actually works. My friend Jorge

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<v Speaker 1>can't be here today, but I'm very glad to be

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<v Speaker 1>joined by one of our regular co hosts. Thanks Katie

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<v Speaker 1>for joining us on this black Hole of an episode.

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<v Speaker 2>I am excited because no matter how many times you

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<v Speaker 2>explain to me what a black hole is, I still

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<v Speaker 2>feel like I cannot wrap my head around it. So surely,

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<v Speaker 2>surely this will be the episode where I understand black holes.

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<v Speaker 1>Well, I would say there's probably nobody out there who

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<v Speaker 1>fully deeply understands black holes, because to fully deeply understand something,

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<v Speaker 1>I think we need a particle level explanation for it.

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<v Speaker 1>You know, we need to be able to moot up

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<v Speaker 1>from the tiniest little bits and say, here's what's really

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<v Speaker 1>happening at the smallest scales when you get sucked into

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<v Speaker 1>a black hole or when photons try to escape. And

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<v Speaker 1>the reason I say that nobody understands them is that

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<v Speaker 1>we do not have a particle level understanding of black

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<v Speaker 1>hole holes. The way, for example, we can understand what

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<v Speaker 1>happens when photons go through glass, They interact with the atoms,

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<v Speaker 1>the electrons and all that stuff in there, and it

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<v Speaker 1>bends their path, and we have some way to tell

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<v Speaker 1>a story microscopically if what's happening to those photons and

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<v Speaker 1>related to what we see actually macroscopically, we can't do

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<v Speaker 1>that for black holes because we don't understand particles and gravity.

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<v Speaker 1>We have no theory of quantum gravity that tells us

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<v Speaker 1>what happens to particles when they feel gravity, and that's

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<v Speaker 1>what black holes are all about. Gravity. So we don't

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<v Speaker 1>have this sort of deep down, microscopic understanding of black holes.

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<v Speaker 1>So probably nobody understands, but that doesn't stop us from

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<v Speaker 1>asking questions and from trying to grapple with what we

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<v Speaker 1>have learned about black holes. Then, on this podcast, we

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<v Speaker 1>encourage everybody to think deeply about the universe and to

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<v Speaker 1>try to fit these ideas into their heads, to ask

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<v Speaker 1>themselves questions to see does this make sense to you?

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<v Speaker 1>Is it possible for you to grapple with what we

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<v Speaker 1>do and do not know about black holes.

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<v Speaker 2>The problem, Daniel is I have a finite number of neurons,

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<v Speaker 2>a finite sort of number of synaptic pathways in my brain,

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<v Speaker 2>and it is very difficult for those little guys to

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<v Speaker 2>understand all we know about black holes and what we

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<v Speaker 2>don't know about black holes. If we were somehow able

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<v Speaker 2>to measure everything about a black hole, do you think

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<v Speaker 2>we could even fully understand it? As humans?

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<v Speaker 1>It's a deep question in philosophy, like are we even

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<v Speaker 1>capable of describing the universe in our minds? Can we

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<v Speaker 1>understand the universe? And not a question I know the

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<v Speaker 1>answer to or I think anybody knows the answer to. Amazingly,

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<v Speaker 1>so far we have been able to do it, to

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<v Speaker 1>write these little mathematical models, tell ourselves these little stories

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<v Speaker 1>in our minds, and use them to explain everything that

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<v Speaker 1>we see and everything we experience, everything our experiments tell us.

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<v Speaker 1>Is it possible for us to understand them? The smartest

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<v Speaker 1>human I don't know. I think there probably is a

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<v Speaker 1>limit to how smart the smartest human is, and so

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<v Speaker 1>it might be that the universe it's just more complex

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<v Speaker 1>than that, and that no human, regardless of how smart

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<v Speaker 1>they are, could ever understand it. But you know, we've

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<v Speaker 1>been making a lot of progress in recent years asking

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<v Speaker 1>and answering questions about the deepest nature of the universe

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<v Speaker 1>and about black holes. So I'm kind of bullish on

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<v Speaker 1>the possibility for some humans someday to understand it. And

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<v Speaker 1>that's not just limited to like the Albert Einsteins of

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<v Speaker 1>the world. I think it's possible for basically everybody out

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<v Speaker 1>there to get some kind of intuitive grasp or how

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<v Speaker 1>black holes work. One thing I love about hearing from

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<v Speaker 1>listeners to the podcast is that it's been teaching them

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<v Speaker 1>to think like a physicist, you know, like, what does

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<v Speaker 1>that mean? To think like a physicist? It means to

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<v Speaker 1>try to understand the world around you, to tell yourself stories,

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<v Speaker 1>to ask yourself questions, to say, do I understand how

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<v Speaker 1>this works? To put these models in your head and

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<v Speaker 1>like turn them around and say, well, if that's true,

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<v Speaker 1>doesn't it mean this or how does this connect with

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<v Speaker 1>this other thing I do understand? And that's especially important

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<v Speaker 1>for weird things like black holes. So we get lots

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<v Speaker 1>of questions from listeners who're doing just that. Wh we're

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<v Speaker 1>trying to think like a physicist about black holes? To

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<v Speaker 1>try to incorporate it into the mathematical stories in their minds.

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<v Speaker 2>This podcast is Daniel's secret weapon of trying to convert

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<v Speaker 2>everyone into physicists. We are onto you, Daniel. You are

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<v Speaker 2>trying to create an army of physicists. There are so

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<v Speaker 2>many questions that I have about black holes. It's hard

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<v Speaker 2>for me to even think about how to phrase my

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<v Speaker 2>confusion about black holes into a question. So just being

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<v Speaker 2>able to ask a distinct, coherent question about black holes,

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<v Speaker 2>I think is impressive.

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<v Speaker 1>I mean, your question about black holes is like black holes,

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<v Speaker 1>what's the deal with that?

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<v Speaker 2>Yeah? My question is like, huh what.

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<v Speaker 1>That's the first step, right, is to be confused, and

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<v Speaker 1>then the second second step is to try to weave

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<v Speaker 1>together a few bits of information and say, like, what

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<v Speaker 1>parts specifically of the story don't make sense to me?

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<v Speaker 1>Which parts do I need to understand better in order

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<v Speaker 1>to have something in my mind that does work where

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<v Speaker 1>the understanding does click. Because what I'd love is for

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<v Speaker 1>people to have that moment where they're like, oh, I

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<v Speaker 1>get it. This connects with that thing, and now it

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<v Speaker 1>kind of makes sense to me, even though it's pretty

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<v Speaker 1>weird and a lot of people out there are trying

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<v Speaker 1>to do that, and many of them have run into

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<v Speaker 1>the same stumbling block. And so today on the podcast,

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<v Speaker 1>I want to answer a very common question that we

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<v Speaker 1>get about black holes. Can gravity escape a black hole?

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<v Speaker 2>I feel like I'm going crossside just trying to think

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<v Speaker 2>about this question.

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<v Speaker 1>I love this question because it reveals that people are

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<v Speaker 1>being physicists. They're thinking about what a black hole is,

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<v Speaker 1>how everything gets sucked into it, how nothing can escape.

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<v Speaker 1>But they're also thinking, hold on a second, we feel

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<v Speaker 1>gravity from a black hole. How's that possible? How can

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<v Speaker 1>the gravity get out of the black hole? And right there,

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<v Speaker 1>that's being a physicist, that's saying I was told this,

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<v Speaker 1>But there's also that how do I make this and

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<v Speaker 1>that work together? How do I put it together in

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<v Speaker 1>my head to tell a story that makes sense.

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<v Speaker 2>So what you're asking us to do is to listen

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<v Speaker 2>to what you're saying and then go hold on, Daniel,

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<v Speaker 2>you just said this. Are you lying to us?

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<v Speaker 1>Everybody's doing their best, nobody's lying to anybody. But in

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<v Speaker 1>the end, learning is a very personal experience, and an

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<v Speaker 1>explanation that makes sense to one person doesn't work for

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<v Speaker 1>somebody else. So that's why in this podcast, we often

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<v Speaker 1>try two or three different analogies or explanations or ways

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<v Speaker 1>to communicate an idea, and that's what you're here for, Katie,

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<v Speaker 1>also to make sure that what I'm saying makes sense

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<v Speaker 1>to you.

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<v Speaker 2>My method of learning is definitely food based metaphors. I'm

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<v Speaker 2>very food motivated.

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<v Speaker 1>Is your appetite something like a black hole?

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<v Speaker 2>It's something like that. Yeah, one could say I'm a

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<v Speaker 2>bit of a black hole, but yeah, I mean, it's

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<v Speaker 2>a very interesting question because it's hard for me to

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<v Speaker 2>think of gravity as like a thing, right, like a

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<v Speaker 2>thing that can escape something. Gravity to me is like, well,

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<v Speaker 2>I don't even know exactly what gravity is. I remember

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<v Speaker 2>from previous podcasts the things that you've taught me about gravity,

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<v Speaker 2>but it is so hard for me to conceptualize gravity

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<v Speaker 2>because it feels like it is like a kind of

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<v Speaker 2>thing woven into like the universe, that is not necessarily like,

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<v Speaker 2>you know, a physical matter thing, but it has everything

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<v Speaker 2>to do with physics. So it's it's a very confusing

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<v Speaker 2>kind of concept. And then you add to that the

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<v Speaker 2>black hole, which itself is quite confusing, and so this

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<v Speaker 2>question feels no pun intended, but very heavy.

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<v Speaker 1>Exactly well, you put your finger on. Really the concepts

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<v Speaker 1>here that are entertangled. You know, what do we know

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<v Speaker 1>about gravity? How is gravitation information communicated? Like? How is

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<v Speaker 1>it that you are feeling gravity from the sun even

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<v Speaker 1>though the Sun is super dup far away and not

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<v Speaker 1>touching you. Does that count as information you're getting from

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<v Speaker 1>the sun? What kind of stuff is captured by a

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<v Speaker 1>black hole? And what isn't captured by a black hole?

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<v Speaker 1>Is that information? How does that all work? You know?

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<v Speaker 1>Do you need to pass little particles back and forth

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<v Speaker 1>in order to feel gravity or what. So. One of

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<v Speaker 1>the reasons I love this question is that it combines

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<v Speaker 1>all of these fun, interesting, fascinating and difficult questions together,

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<v Speaker 1>and going through it I think is really helpful to

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<v Speaker 1>clarify for people what a black hole is and what

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<v Speaker 1>a black hole isn't and how physicists think about it.

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<v Speaker 1>But before we hear about how physicists think about it,

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<v Speaker 1>I wanted to hear what everybody else out there was

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<v Speaker 1>thinking about it. So we have a nice little team

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<v Speaker 1>of volunteers who answer questions for the podcast before we

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<v Speaker 1>dig into them. Helps me understand what people are thinking

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<v Speaker 1>and helps you calibrate your thoughts against the other listeners.

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<v Speaker 1>So thanks very much to everybody who participates. You want

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<v Speaker 1>to jump in for a future episode, we would love, love,

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<v Speaker 1>love to have your voice on the team. Right to me.

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<v Speaker 1>Two questions at Danielandjorge dot com, So think about it

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<v Speaker 1>for a moment before you hear these answers. Do you

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<v Speaker 1>think gravity can escape a black hole? Here's what people

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<v Speaker 1>had to say.

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<v Speaker 5>I feel like, since it kind of depends on the

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<v Speaker 5>mass of an object, it just moves with that object,

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<v Speaker 5>so it would be dependent on the object being able

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<v Speaker 5>to escape the black hole.

0:12:31.280 --> 0:12:34.000
<v Speaker 6>It really matters what we think of as gravity. If

0:12:34.000 --> 0:12:38.000
<v Speaker 6>you think it's gravito gravitons, like with the quantum theories,

0:12:38.760 --> 0:12:41.760
<v Speaker 6>then I guess it escapes. I think, yeah, gravity can

0:12:41.960 --> 0:12:45.280
<v Speaker 6>escape black holes, otherwise I wouldn't be stucking everything in.

0:12:45.559 --> 0:12:50.640
<v Speaker 7>Gravity is a distortion in space time, So I would

0:12:50.720 --> 0:12:56.400
<v Speaker 7>say that gravity itself cannot escape. Actually it's being created

0:12:56.440 --> 0:12:59.600
<v Speaker 7>by the black hole itself. But if we are talking

0:12:59.600 --> 0:13:03.640
<v Speaker 7>about gravitational waves, I believe it can escape a black

0:13:03.640 --> 0:13:07.559
<v Speaker 7>hole if it is outside the event horizon. I even

0:13:07.640 --> 0:13:12.760
<v Speaker 7>think that gravitational waves were discovered by watching collisions of

0:13:12.880 --> 0:13:16.839
<v Speaker 7>black holes and stuff like that. So my guess is yes,

0:13:17.360 --> 0:13:21.360
<v Speaker 7>under the right circumstances, gravitational waves should be able to

0:13:21.440 --> 0:13:22.280
<v Speaker 7>escape a black hole.

0:13:22.880 --> 0:13:24.800
<v Speaker 4>I can't even wrap my head around the question.

0:13:25.200 --> 0:13:27.160
<v Speaker 5>I didn't even know those words could go together.

0:13:27.880 --> 0:13:31.040
<v Speaker 4>I guess it can escape, because isn't that kind of

0:13:31.040 --> 0:13:32.560
<v Speaker 4>what gravitational waves are.

0:13:33.160 --> 0:13:38.679
<v Speaker 2>I love all of the references to gravitational waves because

0:13:38.800 --> 0:13:40.560
<v Speaker 2>we did an episode on that recently.

0:13:40.880 --> 0:13:44.040
<v Speaker 1>We did absolutely an episode on gravitational waves, and that's

0:13:44.080 --> 0:13:47.120
<v Speaker 1>going to turn out to be crucial in understanding what

0:13:47.280 --> 0:13:51.559
<v Speaker 1>is gravitational information and what is not, what is trapped

0:13:51.600 --> 0:13:54.400
<v Speaker 1>within the black hole, and what is not trapped within

0:13:54.440 --> 0:13:57.840
<v Speaker 1>the black hole. Absolutely, so, gravitational waves are a really

0:13:57.840 --> 0:13:59.400
<v Speaker 1>helpful way to think about that.

0:13:59.559 --> 0:14:05.640
<v Speaker 2>I get the root of this question. Is this seeming paradox, right,

0:14:05.880 --> 0:14:08.520
<v Speaker 2>the idea that nothing can escape from a black hole,

0:14:09.000 --> 0:14:12.600
<v Speaker 2>and yet we do know about black holes, We get

0:14:12.720 --> 0:14:16.959
<v Speaker 2>information about black holes, But how can we receive any

0:14:17.000 --> 0:14:20.960
<v Speaker 2>information about a black hole if it is something that

0:14:21.080 --> 0:14:24.480
<v Speaker 2>is all consuming and nothing can escape it?

0:14:24.840 --> 0:14:28.720
<v Speaker 1>Boom Exactly, Adie, you were officially a physicist because you

0:14:28.800 --> 0:14:32.520
<v Speaker 1>are putting together those two ideas that you understand and saying,

0:14:32.560 --> 0:14:34.760
<v Speaker 1>how can these two things be compatible. How can we

0:14:34.760 --> 0:14:39.280
<v Speaker 1>weave them together into a singular understanding of black holes?

0:14:39.320 --> 0:14:40.760
<v Speaker 1>And what it's going to take is a little bit

0:14:40.800 --> 0:14:43.080
<v Speaker 1>of a refinement of the idea of what a black

0:14:43.080 --> 0:14:45.800
<v Speaker 1>hole is and what a black hole isn't to make

0:14:45.840 --> 0:14:47.440
<v Speaker 1>this all work together in your head.

0:14:47.520 --> 0:14:49.680
<v Speaker 2>Well, now that you have proclaimed I am a physicist,

0:14:49.760 --> 0:14:52.120
<v Speaker 2>I am just gonna waltz into like the hard drung

0:14:52.240 --> 0:14:56.880
<v Speaker 2>collider and be like physicists coming through. Let's smash some particles.

0:14:56.960 --> 0:14:57.320
<v Speaker 3>Guys.

0:14:57.680 --> 0:15:00.440
<v Speaker 1>That's right, you have officially a PhD in podcast physics

0:15:00.800 --> 0:15:03.360
<v Speaker 1>from the Daniel and Jorge University.

0:15:04.080 --> 0:15:07.080
<v Speaker 2>Worth its weight in gold. So yes, I would love

0:15:07.200 --> 0:15:12.160
<v Speaker 2>some clarification on what a black hole is. You know,

0:15:12.320 --> 0:15:17.000
<v Speaker 2>I know it's a big, sucky thing. I understand that

0:15:17.400 --> 0:15:23.320
<v Speaker 2>it has something to do with just an incredible density

0:15:24.120 --> 0:15:30.760
<v Speaker 2>of matter, and furthermore that gravity is very much a

0:15:30.800 --> 0:15:33.560
<v Speaker 2>defining characteristic of a black hole.

0:15:33.760 --> 0:15:35.400
<v Speaker 1>Then let's make sure we know what it is we're

0:15:35.440 --> 0:15:39.080
<v Speaker 1>talking about. So a black hole is a region of

0:15:39.240 --> 0:15:43.920
<v Speaker 1>space where the curvature of space is so powerful that

0:15:44.000 --> 0:15:48.800
<v Speaker 1>nothing that's inside that region can escape to outside, and

0:15:48.840 --> 0:15:51.480
<v Speaker 1>that region is defined by this threshold, not really like

0:15:51.520 --> 0:15:54.200
<v Speaker 1>a barrier, not like a physical wall. There's not got

0:15:54.200 --> 0:15:57.360
<v Speaker 1>a dotted line somebody draws in space that says beyond

0:15:57.400 --> 0:16:00.680
<v Speaker 1>this point, if you pass, then you will ever escape.

0:16:00.720 --> 0:16:03.200
<v Speaker 1>You'll be trapped within that region forever.

0:16:03.440 --> 0:16:06.600
<v Speaker 2>Someone's got to put a sign up, a warning, you know, warning,

0:16:06.680 --> 0:16:10.360
<v Speaker 2>do not pass this region. You will be spaghettified into

0:16:10.400 --> 0:16:13.160
<v Speaker 2>a black hole. But I mean, when you say space

0:16:13.280 --> 0:16:16.240
<v Speaker 2>is curved, you know, this is definitely a concept I've

0:16:16.280 --> 0:16:19.760
<v Speaker 2>been introduced to before, but it's still something that I

0:16:19.840 --> 0:16:24.160
<v Speaker 2>struggle to understand because when I think of curvature, right,

0:16:24.200 --> 0:16:27.160
<v Speaker 2>I think of like a physical object that is warped,

0:16:27.800 --> 0:16:30.160
<v Speaker 2>or like say, I think of fabric and I feel like,

0:16:30.480 --> 0:16:33.000
<v Speaker 2>you know, I think of pulling down on the fabric

0:16:33.040 --> 0:16:35.160
<v Speaker 2>and then they're being sort of a curvature and things

0:16:35.200 --> 0:16:39.000
<v Speaker 2>falling into it, and then that's how I think about gravity.

0:16:39.520 --> 0:16:43.520
<v Speaker 2>But I believe that is not really exactly the correct

0:16:44.040 --> 0:16:46.800
<v Speaker 2>understanding of it. Space is not like a piece of

0:16:46.800 --> 0:16:50.040
<v Speaker 2>fabric that you pull on and things fall into that

0:16:50.080 --> 0:16:54.080
<v Speaker 2>sort of like dip. But what exactly does curvature mean

0:16:54.280 --> 0:16:55.320
<v Speaker 2>in terms of space?

0:16:55.760 --> 0:16:58.040
<v Speaker 1>Yeah? Good, It's important to think about in terms of

0:16:58.080 --> 0:17:00.840
<v Speaker 1>curvature because I think a lot of people think about

0:17:00.840 --> 0:17:03.440
<v Speaker 1>black holes in sort of a Newtonian way, where gravity

0:17:03.520 --> 0:17:06.040
<v Speaker 1>is a force and the force of gravity is so

0:17:06.040 --> 0:17:09.120
<v Speaker 1>strong that it's sucking stuff up right, And that cartoon

0:17:09.160 --> 0:17:11.680
<v Speaker 1>model of a black hole breaks down very quickly because

0:17:11.680 --> 0:17:14.160
<v Speaker 1>it can't explain to you, like, well, why does light

0:17:14.240 --> 0:17:16.520
<v Speaker 1>get trapped by a black hole? Why can't a photon

0:17:16.920 --> 0:17:20.879
<v Speaker 1>not leave a black hole? Because the Newtonian picture of gravity,

0:17:21.160 --> 0:17:24.159
<v Speaker 1>gravity is a force between objects with mass, and photons

0:17:24.200 --> 0:17:26.480
<v Speaker 1>have no mass, so they should feel no gravity, and

0:17:26.520 --> 0:17:28.919
<v Speaker 1>so they should be able to escape. In order to

0:17:28.960 --> 0:17:31.760
<v Speaker 1>have an understanding of what black holes are, you really

0:17:31.800 --> 0:17:35.600
<v Speaker 1>have to move your thinking of gravity is from this

0:17:35.760 --> 0:17:40.760
<v Speaker 1>idea of forces between objects with mass to an apparent

0:17:40.880 --> 0:17:43.399
<v Speaker 1>force something that actually results from, as you say, the

0:17:43.480 --> 0:17:46.679
<v Speaker 1>curvature of space itself. So what do we mean by

0:17:46.720 --> 0:17:49.560
<v Speaker 1>the curvature of space itself? Means that space has a

0:17:49.720 --> 0:17:53.400
<v Speaker 1>characteristic to it that's invisible, something you can't see when

0:17:53.480 --> 0:17:55.639
<v Speaker 1>you look at it. You look at some chunk of

0:17:55.680 --> 0:17:58.800
<v Speaker 1>space and you can't tell whether or not it's curved.

0:17:59.000 --> 0:18:01.919
<v Speaker 1>But if you shine a laser beam through it, it

0:18:01.960 --> 0:18:04.320
<v Speaker 1>will either go in a straight line or it will not.

0:18:04.520 --> 0:18:06.440
<v Speaker 1>It will curve, it will bend. This way, or will

0:18:06.480 --> 0:18:10.320
<v Speaker 1>bend that way, because space has this additional, weird property

0:18:10.359 --> 0:18:13.119
<v Speaker 1>that Newton never imagined. And on the smaller scale, what

0:18:13.200 --> 0:18:16.880
<v Speaker 1>it means is that the relative distances between two points

0:18:16.960 --> 0:18:19.800
<v Speaker 1>can get changed. So when we say that like space

0:18:19.880 --> 0:18:22.439
<v Speaker 1>is curved or space is bent, it means that you

0:18:22.440 --> 0:18:25.440
<v Speaker 1>can take two locations in space, you can effectively make

0:18:25.440 --> 0:18:28.160
<v Speaker 1>them closer together, or you can make them further apart.

0:18:28.359 --> 0:18:30.879
<v Speaker 1>And what that does is it changes the path that

0:18:30.960 --> 0:18:33.400
<v Speaker 1>light will take through that space, because light always takes

0:18:33.400 --> 0:18:37.199
<v Speaker 1>the shortest path between two points. Now you're changing what

0:18:37.280 --> 0:18:40.240
<v Speaker 1>the relative distances are between two points, and so you're

0:18:40.320 --> 0:18:43.280
<v Speaker 1>changing the path that light will take. But I think

0:18:43.320 --> 0:18:45.119
<v Speaker 1>the most intuitive way to think about it is that

0:18:45.160 --> 0:18:47.840
<v Speaker 1>like space has this additional bit to it, this characteristic

0:18:48.280 --> 0:18:50.679
<v Speaker 1>so when a photon is passing through it, basically the

0:18:50.720 --> 0:18:54.160
<v Speaker 1>space tells the photon where to go, doesn't just pass

0:18:54.240 --> 0:18:54.960
<v Speaker 1>through blindly.

0:18:55.200 --> 0:18:58.800
<v Speaker 2>It's so interesting because I think the reason it's such

0:18:58.800 --> 0:19:03.719
<v Speaker 2>a difficult concept is that as humans we deal with

0:19:03.720 --> 0:19:09.520
<v Speaker 2>physics all the time, but we can observe Newtonian physics.

0:19:09.560 --> 0:19:13.040
<v Speaker 2>We can observe that type of physics, So it's I

0:19:13.040 --> 0:19:16.400
<v Speaker 2>think easier to think of particles when even like particles

0:19:16.400 --> 0:19:19.239
<v Speaker 2>that you can't observe with the naked eye when they

0:19:19.240 --> 0:19:22.879
<v Speaker 2>are behaving according to forces, because we can on the

0:19:22.920 --> 0:19:26.280
<v Speaker 2>more macro level observe forces. You can see a ball

0:19:26.359 --> 0:19:29.160
<v Speaker 2>knocking into a ball, you can see something fall down

0:19:29.200 --> 0:19:32.399
<v Speaker 2>a hole. But with gravity, even though yes, it's true,

0:19:32.480 --> 0:19:35.080
<v Speaker 2>we can observe gravity. We see it all the time,

0:19:35.240 --> 0:19:37.280
<v Speaker 2>right because you know, you jump up, you fall down.

0:19:37.760 --> 0:19:40.280
<v Speaker 2>It's one of the main problems that we have to

0:19:40.400 --> 0:19:44.119
<v Speaker 2>encounter as a physical being in the world, and yet

0:19:44.200 --> 0:19:49.720
<v Speaker 2>we can't actually see or kind of experience this like

0:19:50.119 --> 0:19:55.200
<v Speaker 2>secret framework behind gravity, which is that what you described,

0:19:55.280 --> 0:19:58.959
<v Speaker 2>like the relative distance between two things like becoming shorter

0:19:59.520 --> 0:20:04.119
<v Speaker 2>and like the actual like you know, space like reality

0:20:04.240 --> 0:20:07.439
<v Speaker 2>sort of warping in a way. It's like so easy

0:20:07.480 --> 0:20:10.359
<v Speaker 2>to fall into that trap of thinking of it in

0:20:10.480 --> 0:20:13.280
<v Speaker 2>terms of the type of physics that we see and

0:20:13.320 --> 0:20:13.920
<v Speaker 2>we observe.

0:20:14.160 --> 0:20:18.280
<v Speaker 1>It's confusing precisely because it's invisible. You can't see this

0:20:18.359 --> 0:20:21.199
<v Speaker 1>curvature of space. You can only see its effect, and

0:20:21.240 --> 0:20:24.159
<v Speaker 1>the effect of the curvature of space looks in almost

0:20:24.240 --> 0:20:27.280
<v Speaker 1>every case as if there was a force there. It

0:20:27.359 --> 0:20:30.760
<v Speaker 1>looks like there is this force we call gravity that's

0:20:30.800 --> 0:20:34.119
<v Speaker 1>pulling on things, when really things are just following the

0:20:34.160 --> 0:20:37.720
<v Speaker 1>curvature of space. The shape of space itself is changing

0:20:37.760 --> 0:20:41.200
<v Speaker 1>the direction in which things move. And if you can't

0:20:41.280 --> 0:20:43.600
<v Speaker 1>see space doing it, it's like a bunch of stage

0:20:43.600 --> 0:20:47.000
<v Speaker 1>hands wearing black nudging stuff. Then you imagine that there's

0:20:47.000 --> 0:20:49.240
<v Speaker 1>a force there. And so that's why we call gravity

0:20:49.320 --> 0:20:51.639
<v Speaker 1>and a parent force. It's not an actual force the

0:20:51.680 --> 0:20:54.800
<v Speaker 1>way like electromagnetism is, or the weak force or the

0:20:54.840 --> 0:20:58.240
<v Speaker 1>strong force. It's just the effect of the invisible curvature

0:20:58.400 --> 0:20:59.080
<v Speaker 1>of space.

0:20:59.480 --> 0:21:02.840
<v Speaker 2>So I hop down from let's say a safe height

0:21:03.440 --> 0:21:07.119
<v Speaker 2>and land on the ground. I am not really getting

0:21:07.480 --> 0:21:11.400
<v Speaker 2>sucked into the ground, because this is an effect of gravity, right,

0:21:11.440 --> 0:21:15.840
<v Speaker 2>The gravity of Earth is affecting me, and so I'm

0:21:15.880 --> 0:21:18.920
<v Speaker 2>not really getting sucked to the ground, but I am

0:21:19.520 --> 0:21:23.640
<v Speaker 2>like sort of just following where space is curving.

0:21:24.000 --> 0:21:27.000
<v Speaker 1>Yeah, that's a great example. Let's walk through it in

0:21:27.040 --> 0:21:30.240
<v Speaker 1>the sort of Newtonian intuitive picture, and then let's move

0:21:30.280 --> 0:21:33.360
<v Speaker 1>over to the Einstein space curvature picture. You'll find that

0:21:33.440 --> 0:21:36.320
<v Speaker 1>it's a very different story about exactly the same thing.

0:21:36.920 --> 0:21:39.199
<v Speaker 1>So in the Newtonian way of thinking, where gravity is

0:21:39.200 --> 0:21:42.040
<v Speaker 1>a force, you are standing on a chair, and you

0:21:42.119 --> 0:21:44.240
<v Speaker 1>imagine that there's a force of gravity pulling you down,

0:21:44.440 --> 0:21:46.120
<v Speaker 1>and there's a force of the chair pulling you up,

0:21:46.160 --> 0:21:48.480
<v Speaker 1>and when you stand on the chair, all forces are balanced,

0:21:48.480 --> 0:21:51.000
<v Speaker 1>so you're not going anywhere. You jump off the chair

0:21:51.080 --> 0:21:52.960
<v Speaker 1>and then you fall down because all you have is

0:21:52.960 --> 0:21:55.479
<v Speaker 1>the force of gravity pulling you down. There's nothing pushing

0:21:55.520 --> 0:21:58.359
<v Speaker 1>you up until you hit the surface of the Earth,

0:21:58.440 --> 0:21:59.639
<v Speaker 1>right in the surace of the Earth, and it's now

0:21:59.680 --> 0:22:03.040
<v Speaker 1>pushing back up on you, and so the forces are

0:22:03.080 --> 0:22:05.720
<v Speaker 1>now balanced and you're not moving anymore. Cool. So that's

0:22:05.760 --> 0:22:10.160
<v Speaker 1>the Newtonian picture. Einstein says, actually that's all wrong, that jerk.

0:22:11.520 --> 0:22:13.840
<v Speaker 1>There is no force of gravity, and that when you're falling,

0:22:13.880 --> 0:22:16.680
<v Speaker 1>when you jump off that chair, what's happening is you're

0:22:16.720 --> 0:22:20.200
<v Speaker 1>following the curvature of the Earth. You're in free fall.

0:22:20.480 --> 0:22:23.320
<v Speaker 1>There is no force on you at all. And in fact,

0:22:23.640 --> 0:22:26.160
<v Speaker 1>if you are carrying a little accelerometer with you, something

0:22:26.200 --> 0:22:29.120
<v Speaker 1>which can measure whether you're accelerating, essentially if there's any

0:22:29.160 --> 0:22:31.600
<v Speaker 1>force on you. Example of an accelerometer is just like

0:22:32.040 --> 0:22:34.080
<v Speaker 1>a ball in a box, Like is the ball pushed

0:22:34.080 --> 0:22:36.960
<v Speaker 1>towards one side or the other? Where Like a bowling

0:22:37.000 --> 0:22:39.320
<v Speaker 1>ball in a truck will tell you whether you're breaking

0:22:39.440 --> 0:22:41.920
<v Speaker 1>or accelerating. If you jump off that chair and you're

0:22:41.920 --> 0:22:44.479
<v Speaker 1>holding an accelerometer, you can do this experiment. You will

0:22:44.560 --> 0:22:48.200
<v Speaker 1>not measure any acceleration. You will not measure anything because

0:22:48.240 --> 0:22:51.520
<v Speaker 1>in that case, you are not accelerating. Einstein says that

0:22:51.560 --> 0:22:54.720
<v Speaker 1>you're actually accelerating when you're standing on the chair. That

0:22:54.800 --> 0:22:57.800
<v Speaker 1>what you're doing there is you're accelerating against the curvature

0:22:57.920 --> 0:23:00.760
<v Speaker 1>of the Earth. And also when you're standing on the earth,

0:23:00.880 --> 0:23:04.200
<v Speaker 1>you're accelerating upwards against your natural path, which would be

0:23:04.240 --> 0:23:08.080
<v Speaker 1>following the curvature of gravity towards the center of the Earth.

0:23:08.200 --> 0:23:13.520
<v Speaker 2>The chair is essentially blocking where you should go naturally

0:23:13.600 --> 0:23:17.120
<v Speaker 2>go by following where space is telling you to go.

0:23:17.359 --> 0:23:19.560
<v Speaker 1>Exactly, if you jump off the chair, you're in free fall.

0:23:19.600 --> 0:23:22.040
<v Speaker 1>You're not accelerating at all. You see people who are

0:23:22.040 --> 0:23:25.639
<v Speaker 1>still on their chairs as accelerating upwards against the natural

0:23:25.680 --> 0:23:27.399
<v Speaker 1>direction gravity wants to take you.

0:23:27.760 --> 0:23:31.960
<v Speaker 2>So, if I'm holding something like a feather, say, and

0:23:32.000 --> 0:23:35.560
<v Speaker 2>I jump off a chair, the feather goes slower than me.

0:23:36.240 --> 0:23:40.120
<v Speaker 2>Is the only reason that happens because of wind resistance.

0:23:40.440 --> 0:23:43.240
<v Speaker 1>Yeah, in that case, it's the air is accelerating the

0:23:43.280 --> 0:23:46.800
<v Speaker 1>feather up. It's preventing the feather from following the curvature

0:23:46.800 --> 0:23:50.159
<v Speaker 1>of space. The air itself is pushing on the feather.

0:23:50.200 --> 0:23:55.200
<v Speaker 2>And that's why an ant can survive really high falls,

0:23:55.240 --> 0:23:58.040
<v Speaker 2>whereas a person could not. Even though the ant seems

0:23:58.119 --> 0:24:03.080
<v Speaker 2>much more structurally delicate than a human because it's so small,

0:24:03.520 --> 0:24:07.560
<v Speaker 2>The air is basically like this huge you know resistance,

0:24:07.600 --> 0:24:11.359
<v Speaker 2>this huge force that is, you know, blocking the ant

0:24:11.840 --> 0:24:15.439
<v Speaker 2>from I guess following the curvature of space.

0:24:15.880 --> 0:24:16.040
<v Speaker 7>Yeah.

0:24:16.080 --> 0:24:18.439
<v Speaker 1>I think there's also something there about the structure of

0:24:18.560 --> 0:24:21.120
<v Speaker 1>ants when they land, but I'm not a biologist.

0:24:21.400 --> 0:24:25.119
<v Speaker 2>They just stick the dismount amazingly. If you zoom in

0:24:25.200 --> 0:24:28.320
<v Speaker 2>on an ant, it does a little summrsalt, lands, and

0:24:28.400 --> 0:24:29.480
<v Speaker 2>then takes a little bow.

0:24:29.920 --> 0:24:32.439
<v Speaker 1>So this picture of gravity is this curvature in space

0:24:32.560 --> 0:24:34.760
<v Speaker 1>rather than a force, gives us a new way to

0:24:34.800 --> 0:24:37.680
<v Speaker 1>think about a black hole. It's not a very dense

0:24:37.800 --> 0:24:40.959
<v Speaker 1>mass that has very strong sucking gravity because of all

0:24:41.040 --> 0:24:43.080
<v Speaker 1>the mass in it. It's a region of space where

0:24:43.119 --> 0:24:46.200
<v Speaker 1>the curvature is such that there is no path outwards,

0:24:46.560 --> 0:24:50.280
<v Speaker 1>where every direction is towards the center of the black hole.

0:24:50.640 --> 0:24:53.480
<v Speaker 1>Anything that's flying along is going to follow the curvature

0:24:53.520 --> 0:24:57.080
<v Speaker 1>of space, including photons. Photons in Einstein's gravity can be

0:24:57.200 --> 0:25:01.000
<v Speaker 1>bent because they follow the curvature of space, not because

0:25:01.000 --> 0:25:04.040
<v Speaker 1>of this Newtonian force between masses. So if Hodan that

0:25:04.119 --> 0:25:06.480
<v Speaker 1>goes past the event horizon is trapped by the structure

0:25:06.520 --> 0:25:09.760
<v Speaker 1>of space itself, because every path forward now takes it

0:25:09.840 --> 0:25:12.680
<v Speaker 1>towards the center of the black hole. And that's where

0:25:12.680 --> 0:25:15.640
<v Speaker 1>this apparent mental paradox comes from that you mentioned earlier.

0:25:16.160 --> 0:25:19.680
<v Speaker 1>If a black hole traps everything, if everything is encapsulated

0:25:19.720 --> 0:25:22.240
<v Speaker 1>inside the black hole because of the structure of space,

0:25:22.600 --> 0:25:24.600
<v Speaker 1>then how is it possible for us to even know

0:25:24.720 --> 0:25:28.600
<v Speaker 1>about it? How's that gravitational information leaving this trash can

0:25:28.760 --> 0:25:29.520
<v Speaker 1>of space time.

0:25:29.800 --> 0:25:33.120
<v Speaker 2>I do want to hear about sort of this idea

0:25:33.840 --> 0:25:38.680
<v Speaker 2>of information not being able to escape a black hole,

0:25:38.720 --> 0:25:41.720
<v Speaker 2>because that just it sounds weird, right to like say

0:25:41.760 --> 0:25:46.119
<v Speaker 2>like information is trapped somewhere, because when we think about information,

0:25:46.560 --> 0:25:49.000
<v Speaker 2>you know, it's like, wait, so I can't use Google

0:25:49.119 --> 0:25:51.560
<v Speaker 2>in a black hole? What does that mean? But maybe

0:25:51.560 --> 0:25:54.680
<v Speaker 2>we should take a quick break before we do that,

0:25:55.600 --> 0:25:59.240
<v Speaker 2>digest the curvature of the space. See, I need food

0:25:59.280 --> 0:26:02.720
<v Speaker 2>metaphors for me to learn and then when we get back,

0:26:02.800 --> 0:26:05.560
<v Speaker 2>I would love to learn more about what it really

0:26:05.680 --> 0:26:22.399
<v Speaker 2>means to say that information cannot escape. All right, So

0:26:22.760 --> 0:26:26.040
<v Speaker 2>I think I'm starting to get a grasp on this

0:26:26.200 --> 0:26:31.160
<v Speaker 2>idea of gravity being sort of a curvature of space,

0:26:32.200 --> 0:26:36.160
<v Speaker 2>not a force. But I do want to hear more

0:26:36.280 --> 0:26:42.600
<v Speaker 2>about what it means when information can't escape a black hole, because, like, again,

0:26:42.680 --> 0:26:45.320
<v Speaker 2>when I think of information, I'm like, well, I'm looking

0:26:45.400 --> 0:26:49.280
<v Speaker 2>on Wikipedia about how ants can stick the dismount. What

0:26:49.320 --> 0:26:52.280
<v Speaker 2>does it mean when information cannot escape a black hole?

0:26:52.440 --> 0:26:54.240
<v Speaker 1>Well, fortunately, if you fall into a black hole, you

0:26:54.320 --> 0:26:58.560
<v Speaker 1>can still access Wikipedia because information can go into Wikipedia.

0:26:58.640 --> 0:27:02.000
<v Speaker 1>You can't request specific page because we can't hear from you,

0:27:02.080 --> 0:27:04.199
<v Speaker 1>but we can send you information. We could just like

0:27:04.640 --> 0:27:07.600
<v Speaker 1>randomly send you Wikipedia pages even after you've.

0:27:07.440 --> 0:27:11.000
<v Speaker 2>Fallen in I would like to get some Netflix and

0:27:11.040 --> 0:27:13.760
<v Speaker 2>stuff if I'm in a black hole, because it seems

0:27:14.200 --> 0:27:16.919
<v Speaker 2>if I'm still alive, it seems really kind of like

0:27:17.800 --> 0:27:19.560
<v Speaker 2>a lot of time I'm going to spend in there.

0:27:19.600 --> 0:27:21.280
<v Speaker 2>I need some entertainment, you know what.

0:27:21.320 --> 0:27:24.439
<v Speaker 1>I think maybe nobody does. What everybody should do is

0:27:24.520 --> 0:27:26.880
<v Speaker 1>prepare their Like, if I fall into a black hole,

0:27:26.920 --> 0:27:29.440
<v Speaker 1>what Netflix shows. Should you beam to me the way

0:27:29.480 --> 0:27:32.840
<v Speaker 1>people like you know, prepare a will other end of

0:27:32.880 --> 0:27:35.240
<v Speaker 1>life information? Like, I'd like to know this about people

0:27:35.280 --> 0:27:37.359
<v Speaker 1>in my life, so I know what to beam to them, right.

0:27:37.400 --> 0:27:41.119
<v Speaker 2>Yeah, exactly, I need to start working on a list.

0:27:41.480 --> 0:27:44.840
<v Speaker 2>But yeah, so information can't escape a black hole? What

0:27:45.000 --> 0:27:48.000
<v Speaker 2>is going on there? And what do we mean by information?

0:27:48.119 --> 0:27:50.639
<v Speaker 1>Really? Yeah? Great? And here's where we need to zoom

0:27:50.680 --> 0:27:53.520
<v Speaker 1>back down again to the particle level when we talk

0:27:53.560 --> 0:27:56.760
<v Speaker 1>about information, Like, imagine that you are inside the black

0:27:56.800 --> 0:27:59.680
<v Speaker 1>hole and you want to request a Wikipedia page about something,

0:28:00.000 --> 0:28:02.959
<v Speaker 1>make a Sioux fla, and you want a recipe or something.

0:28:03.119 --> 0:28:05.600
<v Speaker 1>In order to request that information, you have to send

0:28:05.640 --> 0:28:09.280
<v Speaker 1>something physical outside of the black hole. The way information

0:28:09.440 --> 0:28:12.280
<v Speaker 1>works is that it's transmitted physically. The way you are

0:28:12.320 --> 0:28:16.760
<v Speaker 1>hearing this podcast right now is wiggles in electrons or

0:28:16.840 --> 0:28:20.719
<v Speaker 1>photons being beamed across the Earth. All information is transmitted

0:28:20.960 --> 0:28:23.439
<v Speaker 1>as particles or some kind of a wave. And so

0:28:23.600 --> 0:28:26.720
<v Speaker 1>if particles cannot escape a black hole, then you cannot

0:28:26.720 --> 0:28:29.320
<v Speaker 1>send information outside the black hole because to send that

0:28:29.359 --> 0:28:34.120
<v Speaker 1>information would require sending something physical, a photon, an electron,

0:28:34.280 --> 0:28:37.960
<v Speaker 1>something outside of the black hole. So that's where this

0:28:38.040 --> 0:28:40.720
<v Speaker 1>idea comes from that no information can leave a black

0:28:40.760 --> 0:28:43.719
<v Speaker 1>hole because no thing can leave a black hole, and

0:28:43.800 --> 0:28:47.280
<v Speaker 1>you need things to transmit information. Information in the end

0:28:47.480 --> 0:28:48.280
<v Speaker 1>is physical.

0:28:48.480 --> 0:28:51.000
<v Speaker 2>So I cannot order a pizza from a black hole,

0:28:51.120 --> 0:28:53.440
<v Speaker 2>which seems a little scary.

0:28:53.760 --> 0:28:56.080
<v Speaker 1>So get your pizza order in before you fall into

0:28:56.120 --> 0:28:57.760
<v Speaker 1>the black hole. That's the key. It's just a little

0:28:57.760 --> 0:28:58.360
<v Speaker 1>bit of planning.

0:28:58.600 --> 0:29:00.920
<v Speaker 2>I am writing it in sort of my black hole

0:29:01.200 --> 0:29:05.160
<v Speaker 2>instruction list, that please send pizza into the black hole.

0:29:05.200 --> 0:29:07.600
<v Speaker 2>Should I go in there.

0:29:07.560 --> 0:29:09.800
<v Speaker 1>I think you should ask for spaghetti, actually, because everything

0:29:09.840 --> 0:29:12.040
<v Speaker 1>we send in is getting spaghettified anyway, so you might

0:29:12.080 --> 0:29:13.320
<v Speaker 1>as well start with spaghetti.

0:29:13.600 --> 0:29:15.840
<v Speaker 2>You are what you eat, especially in a black hole,

0:29:15.880 --> 0:29:16.920
<v Speaker 2>if you're eating spaghetti.

0:29:17.080 --> 0:29:20.320
<v Speaker 1>But let's get specific about what we mean by information,

0:29:20.400 --> 0:29:22.640
<v Speaker 1>because this is the crux of the issue. This is

0:29:22.680 --> 0:29:25.200
<v Speaker 1>how we're going to understand later why you can feel

0:29:25.240 --> 0:29:27.960
<v Speaker 1>gravity from outside a black hole, but you can't order

0:29:28.040 --> 0:29:30.640
<v Speaker 1>pizza from within the black hole. And what we mean

0:29:30.720 --> 0:29:34.840
<v Speaker 1>by information is sort of like an update, a change

0:29:34.960 --> 0:29:38.920
<v Speaker 1>of state, so you're communicating something is different, Like if

0:29:39.000 --> 0:29:41.000
<v Speaker 1>Katie and I are across the room from each other,

0:29:41.120 --> 0:29:44.240
<v Speaker 1>she can send me information by like shooting photons at

0:29:44.280 --> 0:29:47.520
<v Speaker 1>me right. For example, if she doesn't shoot any photons

0:29:47.560 --> 0:29:50.000
<v Speaker 1>at me, I can assume like, Okay, Katie's still there.

0:29:50.040 --> 0:29:52.120
<v Speaker 1>I haven't heard from her in a while. But if

0:29:52.160 --> 0:29:54.640
<v Speaker 1>I want any new information from Katie, if you want

0:29:54.640 --> 0:29:58.240
<v Speaker 1>any updates on her situation, she wants to warn me

0:29:58.280 --> 0:30:00.320
<v Speaker 1>about something, or tell me about the pizza she wants,

0:30:00.400 --> 0:30:02.880
<v Speaker 1>or change her list of Netflix shows she wants to watch,

0:30:03.040 --> 0:30:05.440
<v Speaker 1>then she would need to send me some information, some

0:30:05.480 --> 0:30:08.640
<v Speaker 1>electrons or some photons. So information is sort of like

0:30:08.680 --> 0:30:10.600
<v Speaker 1>an update. It's like something new that.

0:30:10.560 --> 0:30:13.840
<v Speaker 2>You're learning, right, So it kind of makes me think

0:30:13.880 --> 0:30:19.280
<v Speaker 2>of like, uh, you know, the basis behind things like computers.

0:30:19.840 --> 0:30:23.400
<v Speaker 2>You have to have little on off things and you know,

0:30:23.480 --> 0:30:26.120
<v Speaker 2>this is a system inside of a computer like a

0:30:26.240 --> 0:30:30.240
<v Speaker 2>zero one an on or and off, and that change

0:30:30.640 --> 0:30:34.200
<v Speaker 2>from off to on is a sort of bit of

0:30:34.320 --> 0:30:38.280
<v Speaker 2>information that can be expanded into of course, the complexity

0:30:38.360 --> 0:30:41.040
<v Speaker 2>of computer. It's the same thing I think with you know,

0:30:41.440 --> 0:30:44.960
<v Speaker 2>in terms of the brain, where you have either a

0:30:45.400 --> 0:30:47.960
<v Speaker 2>synapse has fired or it has not, there's a little

0:30:48.040 --> 0:30:51.800
<v Speaker 2>more complexity because it's it's a large biological process. So

0:30:51.920 --> 0:30:55.400
<v Speaker 2>you have, you know, some states that are somewhat in between,

0:30:55.440 --> 0:30:59.320
<v Speaker 2>you know. But essentially it's like this on off state.

0:30:59.480 --> 0:31:02.080
<v Speaker 2>You need to you be able to clearly have an

0:31:02.200 --> 0:31:05.680
<v Speaker 2>off position and an on position and have that reach

0:31:05.840 --> 0:31:09.040
<v Speaker 2>from one you know, like be able you know, even

0:31:09.080 --> 0:31:14.520
<v Speaker 2>with like say a neuron, you are shooting neurotransmitters from

0:31:14.560 --> 0:31:17.200
<v Speaker 2>one end of a neuron to the other end of

0:31:17.280 --> 0:31:20.680
<v Speaker 2>another neuron. So it's like it's very much like in

0:31:20.800 --> 0:31:24.680
<v Speaker 2>our day to day life we experience this concept of

0:31:24.800 --> 0:31:26.280
<v Speaker 2>information exactly.

0:31:26.280 --> 0:31:28.720
<v Speaker 1>And so you could also think about information from the

0:31:28.760 --> 0:31:32.520
<v Speaker 1>sense of like affecting the future. Information is something that

0:31:32.640 --> 0:31:35.760
<v Speaker 1>somebody in the future can use to make a decision.

0:31:35.920 --> 0:31:38.280
<v Speaker 1>Like if I could tell you what the Powerball winning

0:31:38.360 --> 0:31:41.840
<v Speaker 1>numbers are, you can be a billionaire tomorrow because you

0:31:41.840 --> 0:31:44.280
<v Speaker 1>would know exactly what numbers to put in. So if

0:31:44.320 --> 0:31:46.720
<v Speaker 1>I have information, I can send it to somebody and

0:31:46.760 --> 0:31:48.800
<v Speaker 1>they can use that to make a decision. It can

0:31:48.880 --> 0:31:51.880
<v Speaker 1>like change the future if I am sending them information.

0:31:52.560 --> 0:31:55.360
<v Speaker 1>This is closely connected with another concept we've talked about

0:31:55.400 --> 0:31:58.520
<v Speaker 1>on the podcast a lot, which is this causal link, right,

0:31:58.600 --> 0:32:02.760
<v Speaker 1>like causes and effects how they can be connected. Because

0:32:02.760 --> 0:32:05.880
<v Speaker 1>there's already a limit to how you can affect the

0:32:05.880 --> 0:32:09.360
<v Speaker 1>future in the universe. Like, for example, I can't change

0:32:09.440 --> 0:32:13.360
<v Speaker 1>the future in Andromeda tomorrow. Andromeda is so many light

0:32:13.440 --> 0:32:16.640
<v Speaker 1>years away that any information I send to Andromeda will

0:32:16.640 --> 0:32:20.239
<v Speaker 1>not arrive for millions of years, and so nothing I

0:32:20.360 --> 0:32:24.760
<v Speaker 1>do today can get any information to Andromeda by tomorrow.

0:32:24.880 --> 0:32:28.720
<v Speaker 2>So we cannot get a pizza from or to Andromeda

0:32:29.440 --> 0:32:30.280
<v Speaker 2>anytime soon.

0:32:31.040 --> 0:32:34.480
<v Speaker 1>That's right. We can't even tell Andromeda about what kind

0:32:34.480 --> 0:32:37.520
<v Speaker 1>of pizzas they should order, which in principle could travel

0:32:37.560 --> 0:32:41.320
<v Speaker 1>at the maximum speed of information, which is light speed.

0:32:41.840 --> 0:32:44.440
<v Speaker 1>And so we have this concept we call a light cone,

0:32:44.920 --> 0:32:48.080
<v Speaker 1>which tells you where in the universe your information can reach.

0:32:48.560 --> 0:32:51.520
<v Speaker 1>You can send signals, you can turn on flashing lights,

0:32:51.760 --> 0:32:54.560
<v Speaker 1>but people outside your light cone will not see it,

0:32:55.120 --> 0:32:57.600
<v Speaker 1>and so the light cone expands as time goes on.

0:32:57.960 --> 0:33:01.600
<v Speaker 1>You send a flare. Now that information propagates through the

0:33:01.720 --> 0:33:04.760
<v Speaker 1>universe and eventually will reach the edges of the universe.

0:33:04.840 --> 0:33:08.360
<v Speaker 1>Your light cone is expanding in time from every moment.

0:33:08.640 --> 0:33:11.120
<v Speaker 1>But there is a limitation there, right, There are already

0:33:11.200 --> 0:33:15.400
<v Speaker 1>parts of the universe that your information cannot reach at

0:33:15.400 --> 0:33:18.600
<v Speaker 1>an arbitrary time, So there's a limit to the information.

0:33:18.840 --> 0:33:21.840
<v Speaker 1>You can't send any information to people outside your light cone.

0:33:21.960 --> 0:33:24.320
<v Speaker 2>I don't know if this is a pretty rudimentary question,

0:33:24.400 --> 0:33:30.080
<v Speaker 2>but from Earth, right, we can't see every star in existence,

0:33:30.200 --> 0:33:33.400
<v Speaker 2>can we? Or are we able to see, like get

0:33:33.560 --> 0:33:37.080
<v Speaker 2>light information from every star in existence? From Earth?

0:33:37.240 --> 0:33:39.640
<v Speaker 1>We can't because the universe is not old enough. Right,

0:33:39.640 --> 0:33:42.320
<v Speaker 1>The universe is finite age, So there are some stars

0:33:42.360 --> 0:33:44.840
<v Speaker 1>that are so distant that light from them has not

0:33:45.000 --> 0:33:47.720
<v Speaker 1>had time to arrive here. Plus you've got a factor

0:33:47.760 --> 0:33:50.520
<v Speaker 1>in the expansion or the universe. It gets much more complicated.

0:33:50.720 --> 0:33:53.480
<v Speaker 1>But no, there definitely starts who have sent photons towards

0:33:53.560 --> 0:33:55.400
<v Speaker 1>us but have not yet arrived.

0:33:55.520 --> 0:33:59.520
<v Speaker 2>So it is a matter of timing where because like

0:33:59.560 --> 0:34:02.440
<v Speaker 2>all this stars that we see right now, like that

0:34:02.600 --> 0:34:06.920
<v Speaker 2>information is really old, that light information that we're receiving now,

0:34:07.080 --> 0:34:07.840
<v Speaker 2>that's exactly right.

0:34:07.920 --> 0:34:10.160
<v Speaker 1>Yeah, that information is very old, and it's a matter

0:34:10.239 --> 0:34:13.280
<v Speaker 1>of timing. And if space was simple, space was always flat,

0:34:13.320 --> 0:34:16.000
<v Speaker 1>if there was no curvature, photons always traveled in a

0:34:16.040 --> 0:34:18.160
<v Speaker 1>straight direction and at the speed of light, then the

0:34:18.200 --> 0:34:21.239
<v Speaker 1>only limit to information would be timing. But the curvature

0:34:21.280 --> 0:34:24.799
<v Speaker 1>of space changes things. And in curved space, your light

0:34:24.880 --> 0:34:27.440
<v Speaker 1>cone is not a simple cone. It gets bent, it

0:34:27.440 --> 0:34:30.320
<v Speaker 1>gets distorted. Near a black hole or anywhere where space

0:34:30.360 --> 0:34:33.440
<v Speaker 1>is curved. Your light cone gets twisted because it changes

0:34:33.760 --> 0:34:36.680
<v Speaker 1>where photons go. Right, you send out a flash of light.

0:34:36.960 --> 0:34:39.200
<v Speaker 1>Now they're going in some directions, not in other directions.

0:34:39.200 --> 0:34:41.439
<v Speaker 1>They get twisted, they get bent. Once you pass over

0:34:41.480 --> 0:34:44.560
<v Speaker 1>the event horizon, your light cone is now just pointed

0:34:44.640 --> 0:34:47.919
<v Speaker 1>towards the center of the singularity. Any flare you set off,

0:34:48.280 --> 0:34:51.600
<v Speaker 1>all photons are going to end up going towards the singularity.

0:34:51.920 --> 0:34:54.320
<v Speaker 1>So your light cone is now sort of trapped behind

0:34:54.520 --> 0:34:57.439
<v Speaker 1>this barrier. And that's what we mean when we say

0:34:57.520 --> 0:35:00.760
<v Speaker 1>information cannot escape a black hole. I mean that nobody

0:35:00.760 --> 0:35:03.840
<v Speaker 1>passed that threshold can ever send you a photon that

0:35:04.000 --> 0:35:04.919
<v Speaker 1>arrives to you.

0:35:05.080 --> 0:35:08.640
<v Speaker 2>If a photon approaches a black hole but doesn't pass

0:35:08.760 --> 0:35:11.959
<v Speaker 2>the event horizon, can its light cones still get bent,

0:35:12.400 --> 0:35:14.799
<v Speaker 2>but not fall into the black hole.

0:35:14.880 --> 0:35:17.120
<v Speaker 1>Oh yeah. In fact, there's a region near black holes

0:35:17.160 --> 0:35:20.440
<v Speaker 1>where photons can orbit. They can get trapped and forever

0:35:20.560 --> 0:35:23.600
<v Speaker 1>loop around a black hole, which is pretty cool, or

0:35:23.640 --> 0:35:26.160
<v Speaker 1>they can do other weird things like pass around the

0:35:26.200 --> 0:35:28.160
<v Speaker 1>backside of a black hole and then come back. So

0:35:28.200 --> 0:35:30.120
<v Speaker 1>you can shoot it like a laser beam just above

0:35:30.120 --> 0:35:32.520
<v Speaker 1>a black hole and kind of come around the backside

0:35:32.560 --> 0:35:35.319
<v Speaker 1>and zap you in the eyeball from below the black hole.

0:35:36.000 --> 0:35:37.600
<v Speaker 2>It's like a laser boomerang.

0:35:37.760 --> 0:35:40.320
<v Speaker 1>So the key thing to understand there is that information

0:35:40.480 --> 0:35:44.360
<v Speaker 1>is about changes of state, how things change, getting updates

0:35:44.400 --> 0:35:47.520
<v Speaker 1>about what's going on, decisions that are made, new facts

0:35:47.520 --> 0:35:51.040
<v Speaker 1>that arise. Information is about changes of state.

0:35:51.320 --> 0:35:56.879
<v Speaker 2>So with gravity, Now, I thought that we had talked

0:35:56.920 --> 0:36:00.480
<v Speaker 2>about a previous episode about how with gravity there is

0:36:00.520 --> 0:36:04.799
<v Speaker 2>a phenomenon known as gravitational waves, which would indicate that

0:36:04.840 --> 0:36:09.080
<v Speaker 2>gravity can change. Right, you can have changes in gravity.

0:36:09.239 --> 0:36:12.840
<v Speaker 2>So why would it be considered that gravity is not

0:36:13.320 --> 0:36:14.680
<v Speaker 2>a form of information.

0:36:15.160 --> 0:36:19.080
<v Speaker 1>Yes, great example, So gravitational wave is a great example

0:36:19.160 --> 0:36:22.960
<v Speaker 1>of gravity changing. Right. We talked about gravity in terms

0:36:23.040 --> 0:36:25.560
<v Speaker 1>of the curvature of space. So imagine space has some

0:36:25.760 --> 0:36:28.520
<v Speaker 1>curvature because of the arrangements of masses in it. So

0:36:28.560 --> 0:36:30.760
<v Speaker 1>space has that curvature, and that curvature is just fixed,

0:36:30.800 --> 0:36:34.080
<v Speaker 1>it's constant. Right. Now, take one of those masses, the

0:36:34.120 --> 0:36:37.239
<v Speaker 1>Sun maybe, and wiggle it. You put your finger on it,

0:36:37.280 --> 0:36:39.479
<v Speaker 1>you shake it back and forth. If you wiggle the Sun,

0:36:39.520 --> 0:36:42.440
<v Speaker 1>you're changing where the mass is. You're changing how space

0:36:42.600 --> 0:36:44.520
<v Speaker 1>is bent. So what's happening to there is the curvature

0:36:44.560 --> 0:36:46.239
<v Speaker 1>is changing. You're moving the Sun to the left, and

0:36:46.280 --> 0:36:47.799
<v Speaker 1>you're moving it to the right, and you're moving it

0:36:47.800 --> 0:36:49.439
<v Speaker 1>to the left again, you're moving it to the right,

0:36:49.560 --> 0:36:53.640
<v Speaker 1>and that's information and that information propagates out at the

0:36:53.680 --> 0:36:56.200
<v Speaker 1>speed of light. And so if you're far away from

0:36:56.200 --> 0:36:58.759
<v Speaker 1>the Sun when somebody's wiggling it, you don't feel those

0:36:58.880 --> 0:37:02.439
<v Speaker 1>changes instantly. It takes time for that information to get

0:37:02.440 --> 0:37:05.880
<v Speaker 1>to you. So Katie wiggles the Sun. Eight minutes later,

0:37:06.040 --> 0:37:09.080
<v Speaker 1>I feel the gravity on Earth shaking a little bit.

0:37:09.400 --> 0:37:11.400
<v Speaker 1>It gets stronger, it gets weaker, it gets stronger, it

0:37:11.400 --> 0:37:15.879
<v Speaker 1>gets weaker. That's a gravitational wave. That's information moving through

0:37:15.880 --> 0:37:18.840
<v Speaker 1>the gravitational field. So I think that's sort of a

0:37:18.840 --> 0:37:21.080
<v Speaker 1>long answer to your question, which is can you send

0:37:21.120 --> 0:37:23.600
<v Speaker 1>information through gravity? And the answer is yes, And that's

0:37:23.600 --> 0:37:27.560
<v Speaker 1>what gravitational waves are. There's information sent through the gravitational field.

0:37:27.880 --> 0:37:31.360
<v Speaker 1>The crucial thing is that that's all about a change

0:37:31.440 --> 0:37:35.200
<v Speaker 1>in the gravitational field. There's no information being propagated when

0:37:35.200 --> 0:37:37.879
<v Speaker 1>the sun is static. The field is not changing. There's

0:37:37.880 --> 0:37:40.640
<v Speaker 1>no information there. When you move the sun, when you've

0:37:40.680 --> 0:37:43.239
<v Speaker 1>wiggled it, that's sending information.

0:37:43.800 --> 0:37:49.920
<v Speaker 2>So Earth has gravity, obviously, but when the Earth moves,

0:37:50.320 --> 0:37:53.760
<v Speaker 2>you're getting some change in gravity, and so you're getting

0:37:53.840 --> 0:37:57.600
<v Speaker 2>gravitational waves. And so that change of the Earth moving

0:37:58.440 --> 0:38:03.360
<v Speaker 2>is sending out information in terms of the change in gravity.

0:38:03.560 --> 0:38:06.480
<v Speaker 1>Absolutely, And when the Earth orbits the Sun, because it's

0:38:06.480 --> 0:38:10.320
<v Speaker 1>effectively moving through space and changing the Earth's gravitational field,

0:38:10.600 --> 0:38:14.680
<v Speaker 1>we are generating gravitational waves. Our orbit around the Sun

0:38:14.800 --> 0:38:18.840
<v Speaker 1>generates gravitational waves, and it actually contributes to the decay

0:38:18.960 --> 0:38:23.040
<v Speaker 1>of Earth's orbit because gravitational waves contain energy, so we're

0:38:23.160 --> 0:38:26.040
<v Speaker 1>radiating away some of our energy every time we go

0:38:26.080 --> 0:38:27.800
<v Speaker 1>around the Sun. You just did an episode about this

0:38:27.840 --> 0:38:30.160
<v Speaker 1>about how stable is the Earth's orbit, and it turns

0:38:30.160 --> 0:38:32.880
<v Speaker 1>out that's a very very small effect in terms of

0:38:32.920 --> 0:38:35.719
<v Speaker 1>the stability of the Earth's orbit. But in principle, yes,

0:38:36.040 --> 0:38:39.480
<v Speaker 1>we are generating gravitational waves which contain information, and if

0:38:39.520 --> 0:38:42.760
<v Speaker 1>you had a sensitive enough gravitational wave detector, you could

0:38:42.760 --> 0:38:45.520
<v Speaker 1>pick up those wiggles in space time that are telling

0:38:45.600 --> 0:38:47.600
<v Speaker 1>you about how the Earth is moving.

0:38:47.960 --> 0:38:52.279
<v Speaker 2>So gravity can convey information. It can be considered a

0:38:52.320 --> 0:38:55.880
<v Speaker 2>form of information if it is a change in the gravity.

0:38:56.200 --> 0:38:59.680
<v Speaker 2>So with a black hole, why aren't we seeing a

0:38:59.760 --> 0:39:02.719
<v Speaker 2>chain in gravity, because I would assume if we're not

0:39:02.760 --> 0:39:06.719
<v Speaker 2>getting gravitational information from a black hole, that would mean

0:39:07.120 --> 0:39:10.560
<v Speaker 2>that there is not a change in the gravity of

0:39:10.600 --> 0:39:11.279
<v Speaker 2>a black hole.

0:39:11.520 --> 0:39:13.359
<v Speaker 1>Yes, exactly, and so now I think we have all

0:39:13.400 --> 0:39:15.880
<v Speaker 1>the pieces in place to try to answer this question,

0:39:16.400 --> 0:39:19.240
<v Speaker 1>which is a black hole does of course have gravity,

0:39:19.400 --> 0:39:22.640
<v Speaker 1>and you can feel its gravity from a distance. You

0:39:22.719 --> 0:39:24.759
<v Speaker 1>are a light year from a black hole, you will

0:39:24.800 --> 0:39:29.120
<v Speaker 1>feel its gravity. But what you can't feel are changes

0:39:29.160 --> 0:39:32.400
<v Speaker 1>to its gravity. So if there's something going on inside

0:39:32.480 --> 0:39:35.720
<v Speaker 1>the event horizon, Katie's in there and she's doing a dance,

0:39:36.120 --> 0:39:39.280
<v Speaker 1>or she's rearranging her living room or whatever, you can't

0:39:39.320 --> 0:39:42.800
<v Speaker 1>get that kind of information. If you change the configuration

0:39:43.000 --> 0:39:46.440
<v Speaker 1>of the masses inside the black hole, in principle, that

0:39:46.520 --> 0:39:50.760
<v Speaker 1>generates gravitational waves, but those are trapped within the event horizon.

0:39:51.200 --> 0:39:54.000
<v Speaker 1>So nothing that's happening within the event horizon is generating

0:39:54.080 --> 0:39:57.960
<v Speaker 1>any gravitational information that's escaping. All you're feeling is the

0:39:58.000 --> 0:40:01.319
<v Speaker 1>static field of the black hole, the one that was

0:40:01.360 --> 0:40:04.120
<v Speaker 1>created when it was formed. So you have a black

0:40:04.120 --> 0:40:07.279
<v Speaker 1>hole and it has a static gravitational field. Nothing is

0:40:07.360 --> 0:40:11.360
<v Speaker 1>changing and anything that happens inside the event horizon is

0:40:11.440 --> 0:40:14.520
<v Speaker 1>going to generate gravitational waves, but they don't leave the

0:40:14.600 --> 0:40:18.360
<v Speaker 1>black hole. So you can have gravity outside the black

0:40:18.360 --> 0:40:21.799
<v Speaker 1>hole from its original formation without knowing what's going on

0:40:21.920 --> 0:40:26.000
<v Speaker 1>later inside the event horizon, without getting any information from

0:40:26.120 --> 0:40:29.600
<v Speaker 1>inside the event horizon. The only information you have is

0:40:29.640 --> 0:40:32.480
<v Speaker 1>the existence of the black hole from when it was created,

0:40:32.600 --> 0:40:35.839
<v Speaker 1>which is not information from inside the event horizon. Another

0:40:35.880 --> 0:40:38.359
<v Speaker 1>way to think about it is you create the black hole,

0:40:38.560 --> 0:40:42.680
<v Speaker 1>you're then freezing that gravitational field. Nothing that happens pas

0:40:42.719 --> 0:40:46.440
<v Speaker 1>the event horizon can then change the gravitational field outside

0:40:46.520 --> 0:40:49.040
<v Speaker 1>the black hole. Now, that's all if the black hole

0:40:49.120 --> 0:40:52.080
<v Speaker 1>is not moving and so it has a static, unchanging

0:40:52.239 --> 0:40:55.279
<v Speaker 1>gravitational field. If you wiggle a black hole or if

0:40:55.320 --> 0:40:59.280
<v Speaker 1>black holes merge, that motion creates ripples in the gravitational field,

0:40:59.400 --> 0:41:01.760
<v Speaker 1>just like a d when the Sun or the Earth moves.

0:41:01.880 --> 0:41:05.400
<v Speaker 1>But that's motion of the event horizon. It's not information

0:41:05.520 --> 0:41:09.120
<v Speaker 1>from inside the event horizon about what's going on within it.

0:41:09.239 --> 0:41:11.400
<v Speaker 1>Another way to say it is that from the outside

0:41:11.480 --> 0:41:14.440
<v Speaker 1>you can see if the black hole is wiggling, but

0:41:14.520 --> 0:41:17.520
<v Speaker 1>that's not information from inside the event horizon. You can't

0:41:17.560 --> 0:41:20.680
<v Speaker 1>tell if things inside are wiggling, only if the whole

0:41:20.760 --> 0:41:21.800
<v Speaker 1>thing is moving.

0:41:22.000 --> 0:41:25.120
<v Speaker 2>I mean that's interesting because it's like, I suspect this

0:41:25.200 --> 0:41:27.680
<v Speaker 2>might be the wrong way to conceptualize it, but in

0:41:27.719 --> 0:41:31.040
<v Speaker 2>my head, I'm thinking of sort of a Russian nesting doll,

0:41:31.400 --> 0:41:34.560
<v Speaker 2>where it's like the black hole is the main one,

0:41:34.840 --> 0:41:39.439
<v Speaker 2>the main sort of gravitational field, and inside you could

0:41:39.440 --> 0:41:42.440
<v Speaker 2>have like the little tiny doll dancing around doing stuff,

0:41:42.440 --> 0:41:45.360
<v Speaker 2>but none of that is reaching outside of this nesting

0:41:45.640 --> 0:41:50.239
<v Speaker 2>doll because like the bigger one is essentially this like

0:41:50.360 --> 0:41:56.719
<v Speaker 2>static large gravitational field, and nothing is getting outside of it.

0:41:56.800 --> 0:41:58.640
<v Speaker 1>Yeah, I think that's a great way to think about it.

0:41:58.960 --> 0:42:01.920
<v Speaker 1>Another useful thing to think through is how a black

0:42:01.920 --> 0:42:04.719
<v Speaker 1>hole gets formed, the moment in which a black hole

0:42:04.840 --> 0:42:07.399
<v Speaker 1>is created. I think that can really help people crystallize

0:42:07.520 --> 0:42:10.560
<v Speaker 1>how that information is propagated through the universe and why

0:42:10.719 --> 0:42:14.440
<v Speaker 1>no more information is ever sent out from that object.

0:42:14.520 --> 0:42:17.600
<v Speaker 2>All right, let's take a quick break as I mentally

0:42:17.680 --> 0:42:21.240
<v Speaker 2>prepare my mind to be blown. I'll lay out a tarp,

0:42:21.480 --> 0:42:24.240
<v Speaker 2>and then when we get back, please tell me how

0:42:24.360 --> 0:42:40.480
<v Speaker 2>a black hole is created. All right, So I'm officially

0:42:40.560 --> 0:42:45.960
<v Speaker 2>ready for my brain to explode from the information of

0:42:46.400 --> 0:42:48.520
<v Speaker 2>how a black hole is formed.

0:42:48.640 --> 0:42:49.919
<v Speaker 1>So all you have to do to form a black

0:42:49.960 --> 0:42:53.400
<v Speaker 1>hole is just order enough pizzas. Really, that's all it takes. Okay,

0:42:55.120 --> 0:42:56.799
<v Speaker 1>So we know that there are black holes out there

0:42:56.800 --> 0:42:59.560
<v Speaker 1>in the universe and that they are created, right, they're

0:42:59.560 --> 0:43:02.080
<v Speaker 1>a black holes that have not existed since the beginning

0:43:02.080 --> 0:43:04.680
<v Speaker 1>of the universe. So there has to be some moment

0:43:04.760 --> 0:43:06.880
<v Speaker 1>when there wasn't a black hole and when there is

0:43:06.920 --> 0:43:09.319
<v Speaker 1>a black hole. And I think the thinking through that

0:43:09.440 --> 0:43:12.719
<v Speaker 1>moment really can help people understand what we're talking about

0:43:12.719 --> 0:43:14.319
<v Speaker 1>when we say a black hole, what it means for

0:43:14.360 --> 0:43:16.759
<v Speaker 1>information to be trapped within it. And so there's lots

0:43:16.800 --> 0:43:18.440
<v Speaker 1>of ways that a black hole can be made in

0:43:18.480 --> 0:43:20.480
<v Speaker 1>the universe, But let's try to think about like the

0:43:20.520 --> 0:43:24.480
<v Speaker 1>simplest possible configuration and in general relativity, one very frequently

0:43:24.560 --> 0:43:27.560
<v Speaker 1>used example is like a sphere of rocks. Imagine you

0:43:27.600 --> 0:43:30.000
<v Speaker 1>have like tiny little bits of dust or pebbles, and

0:43:30.000 --> 0:43:33.040
<v Speaker 1>you have a perfectly symmetrical sphere of it. Okay, and

0:43:33.080 --> 0:43:35.520
<v Speaker 1>now gravity is pulling it and so it's collapsing. It's

0:43:35.560 --> 0:43:38.080
<v Speaker 1>going to pull towards itself and get denser and denser

0:43:38.120 --> 0:43:39.879
<v Speaker 1>and denser. Now, how do you make a black hole.

0:43:39.920 --> 0:43:42.200
<v Speaker 1>You make a black hole by having enough stuff in

0:43:42.239 --> 0:43:45.920
<v Speaker 1>a small enough space. It's all about the density of matter.

0:43:46.280 --> 0:43:47.920
<v Speaker 1>You could take the Earth and squeeze it into a

0:43:47.960 --> 0:43:49.960
<v Speaker 1>peanut to get a black hole. You could take the

0:43:50.000 --> 0:43:53.040
<v Speaker 1>Sun and squeeze it into like a three kilometer wide object.

0:43:53.120 --> 0:43:55.080
<v Speaker 1>To get a black hole. You could take a huge

0:43:55.080 --> 0:43:57.279
<v Speaker 1>blob of stuff and squeeze it. The point is to

0:43:57.280 --> 0:43:59.840
<v Speaker 1>get high enough density. So now you have this hollow

0:44:00.120 --> 0:44:03.319
<v Speaker 1>fear of pebbles. Right, everything's like the same distance from

0:44:03.360 --> 0:44:06.799
<v Speaker 1>the center, and it's collapsing slowly. At some point it's

0:44:06.840 --> 0:44:09.160
<v Speaker 1>going to be dense enough to pass this threshold and

0:44:09.200 --> 0:44:11.240
<v Speaker 1>become a black hole. It's going to be a moment

0:44:11.280 --> 0:44:14.400
<v Speaker 1>before it passes that threshold where it's just like a

0:44:14.480 --> 0:44:16.880
<v Speaker 1>sphere of stuff that has gravity, and then a moment

0:44:17.000 --> 0:44:20.120
<v Speaker 1>after passes that threshold, now it's a black hole.

0:44:20.440 --> 0:44:25.600
<v Speaker 2>How does the incredible density cause Essentially, what I'm imagining

0:44:25.719 --> 0:44:30.440
<v Speaker 2>is like pinching the curvature of space such that everything

0:44:30.520 --> 0:44:34.800
<v Speaker 2>is going towards that point, Like, how does density cause

0:44:34.880 --> 0:44:35.640
<v Speaker 2>that to happen?

0:44:35.840 --> 0:44:38.040
<v Speaker 1>We talked about how gravity is actually just the curvature

0:44:38.040 --> 0:44:40.399
<v Speaker 1>of space. We didn't talk about how you make that

0:44:40.440 --> 0:44:43.640
<v Speaker 1>curvature why bits of space are curved here or not

0:44:43.760 --> 0:44:47.320
<v Speaker 1>curved there. So the missing piece is density energy density.

0:44:47.760 --> 0:44:49.560
<v Speaker 1>If you have a chunk of space with a lot

0:44:49.600 --> 0:44:52.960
<v Speaker 1>of energy in it, be it mass or photons or

0:44:53.000 --> 0:44:56.600
<v Speaker 1>any kind of energy, then that space gets curved. So

0:44:56.640 --> 0:45:00.840
<v Speaker 1>the simplest version of general relativity is mass tells space

0:45:00.880 --> 0:45:04.200
<v Speaker 1>how to bend. Space tells mass how to move, and

0:45:04.239 --> 0:45:06.759
<v Speaker 1>so it's that first bit that mass tells space how

0:45:06.800 --> 0:45:09.479
<v Speaker 1>to bend. The more energy density, usually in the form

0:45:09.520 --> 0:45:12.040
<v Speaker 1>of mass, that you pile into a little chunk of space,

0:45:12.120 --> 0:45:16.000
<v Speaker 1>the more curvature you get. When you cross past some threshold,

0:45:16.320 --> 0:45:19.600
<v Speaker 1>then you have so much curvature that nothing can escape anymore.

0:45:19.680 --> 0:45:21.640
<v Speaker 1>So that's the moment you become a black hole. So

0:45:21.719 --> 0:45:24.200
<v Speaker 1>you take this sphere of dust again, it's a hollow sphere.

0:45:24.200 --> 0:45:26.640
<v Speaker 1>It's not filled on the center. If it's really really big,

0:45:26.680 --> 0:45:28.359
<v Speaker 1>then you have a lot of empty space. Also, you're

0:45:28.360 --> 0:45:31.239
<v Speaker 1>including density is very very low, you don't have a

0:45:31.280 --> 0:45:34.760
<v Speaker 1>black hole. As you collapse it, the radius gets smaller

0:45:34.760 --> 0:45:37.000
<v Speaker 1>and smaller. All the bits get closer and closer together.

0:45:37.120 --> 0:45:40.800
<v Speaker 1>Eventually you pass over the short siled radius, the radius

0:45:40.800 --> 0:45:43.839
<v Speaker 1>of an event horizon for that amount of stuff, and

0:45:43.880 --> 0:45:46.759
<v Speaker 1>then you have enough density that there's enough curvature that

0:45:46.800 --> 0:45:47.839
<v Speaker 1>you've got a black hole.

0:45:48.120 --> 0:45:51.800
<v Speaker 2>So mass which we can observe is sort of tied

0:45:51.880 --> 0:45:57.280
<v Speaker 2>to this hidden world of gravity which we cannot see.

0:45:57.880 --> 0:46:00.359
<v Speaker 2>We can feel the effects of, but we cannot see

0:46:00.360 --> 0:46:03.520
<v Speaker 2>the curvature of space. But that curvature of space has

0:46:03.640 --> 0:46:09.400
<v Speaker 2>direct connections to all the mass that we can directly observe.

0:46:09.719 --> 0:46:13.279
<v Speaker 1>Yeah, that's exactly right. And remember that's not just mass.

0:46:13.400 --> 0:46:16.759
<v Speaker 1>Right in Newton's physics, it's just mass, but in Einstein's

0:46:16.760 --> 0:46:20.320
<v Speaker 1>relativity it's energy density. That's why photons and other massless

0:46:20.360 --> 0:46:23.440
<v Speaker 1>things can actually contribute to the curvature of space. You

0:46:23.480 --> 0:46:26.720
<v Speaker 1>can actually just make a black hole by overlapping powerful

0:46:26.800 --> 0:46:30.920
<v Speaker 1>laser beams. Pure photons can make a black hole in theory.

0:46:31.200 --> 0:46:33.239
<v Speaker 2>Okay, how do you know that, Daniel, or are you

0:46:33.320 --> 0:46:35.680
<v Speaker 2>working on that? Are you doing that?

0:46:35.960 --> 0:46:38.560
<v Speaker 1>I can either deny nor confirm those experiments.

0:46:38.719 --> 0:46:44.719
<v Speaker 2>That's incredible that just through light, if you cram enough

0:46:44.840 --> 0:46:48.160
<v Speaker 2>light into a small enough area, not only are you

0:46:48.200 --> 0:46:50.719
<v Speaker 2>going to like blow out your retinas, you're going to

0:46:50.800 --> 0:46:52.000
<v Speaker 2>create a black hole.

0:46:52.320 --> 0:46:55.000
<v Speaker 1>So now let's go back to our collapsing sphere of

0:46:55.040 --> 0:46:58.960
<v Speaker 1>pebbles or dust or rocks or whatever. What happens when

0:46:58.960 --> 0:47:01.840
<v Speaker 1>it creates a black hole? What is changing in space

0:47:02.000 --> 0:47:04.319
<v Speaker 1>the moment before it creates a black hole? What do

0:47:04.400 --> 0:47:06.200
<v Speaker 1>you have? What you have gravity?

0:47:06.400 --> 0:47:06.560
<v Speaker 2>Right?

0:47:06.920 --> 0:47:08.759
<v Speaker 1>If somebody is going to shoot a photon or a

0:47:08.760 --> 0:47:11.719
<v Speaker 1>particle near it, it's going to be bending space and

0:47:11.760 --> 0:47:13.920
<v Speaker 1>it's going to affect the path of that stuff. Right,

0:47:13.920 --> 0:47:16.919
<v Speaker 1>You're going to feel the effective force of gravity from

0:47:16.960 --> 0:47:19.440
<v Speaker 1>this sphere of rocks, right, because it has mass, it's

0:47:19.480 --> 0:47:22.279
<v Speaker 1>curving space. It's giving you that effect. No big deal,

0:47:22.320 --> 0:47:25.400
<v Speaker 1>no surprise there. What happens when it crosses that threshold

0:47:25.440 --> 0:47:29.200
<v Speaker 1>and becomes a black hole? Well, nothing changes from that

0:47:29.280 --> 0:47:32.440
<v Speaker 1>point of view, right, because the mass hasn't changed, the

0:47:32.520 --> 0:47:35.239
<v Speaker 1>overall energy hasn't changed. So if you're in the outside,

0:47:35.760 --> 0:47:40.080
<v Speaker 1>when this sphere becomes a black hole, nothing changes gravitationally,

0:47:40.120 --> 0:47:43.480
<v Speaker 1>the gravitational field is still the same. And that makes sense, right.

0:47:43.560 --> 0:47:46.200
<v Speaker 1>It's not like the gravity disappears when the thing becomes

0:47:46.200 --> 0:47:49.440
<v Speaker 1>a black hole. It changes from a big sphere of

0:47:49.520 --> 0:47:51.440
<v Speaker 1>dust to a black hole. But if it has the

0:47:51.440 --> 0:47:54.160
<v Speaker 1>same mass, it has the same gravity as before it

0:47:54.239 --> 0:47:55.160
<v Speaker 1>became a black hole.

0:47:55.320 --> 0:47:59.480
<v Speaker 2>Okay, so you have this amount of gravity that just

0:47:59.600 --> 0:48:02.760
<v Speaker 2>before sure the black hole is created, and then once

0:48:02.880 --> 0:48:06.920
<v Speaker 2>the black hole happens, that gravity is the same. So

0:48:07.000 --> 0:48:10.520
<v Speaker 2>can you not add any more gravity to a black hole?

0:48:10.560 --> 0:48:13.400
<v Speaker 2>Like you cannot, Like say, you put more stuff into

0:48:13.440 --> 0:48:16.680
<v Speaker 2>a black hole, you put more particles into that black hole,

0:48:16.719 --> 0:48:19.560
<v Speaker 2>you shoot some lasers. There's no more gravity that you

0:48:19.600 --> 0:48:20.239
<v Speaker 2>can add to that.

0:48:20.440 --> 0:48:23.040
<v Speaker 1>That's a great question, actually really illustrates this point very nicely.

0:48:23.360 --> 0:48:26.120
<v Speaker 1>Absolutely you can. Right, if you shoot a laser into

0:48:26.120 --> 0:48:27.759
<v Speaker 1>the black hole, or you throw a more mast in

0:48:27.800 --> 0:48:30.560
<v Speaker 1>the black hole, you are going to increase its gravity,

0:48:30.960 --> 0:48:34.160
<v Speaker 1>and that information will propagate outwards. Right, you add to

0:48:34.200 --> 0:48:36.200
<v Speaker 1>a black hole, you add to its gravity. You can

0:48:36.280 --> 0:48:39.760
<v Speaker 1>feel more gravity now somewhere else. That information will propagate

0:48:39.760 --> 0:48:43.720
<v Speaker 1>outwards as a gravitational waves, a change in the gravitational

0:48:43.800 --> 0:48:47.400
<v Speaker 1>field of the black hole. But that's external, right, that's

0:48:47.440 --> 0:48:50.760
<v Speaker 1>not information coming from within the black hole. That stuff

0:48:50.760 --> 0:48:53.000
<v Speaker 1>you're adding from the outside. If you have just a

0:48:53.000 --> 0:48:55.560
<v Speaker 1>black hole and it's collapsed and you're not changing its

0:48:55.600 --> 0:48:58.960
<v Speaker 1>gravitational field, then what does it mean for information to

0:48:59.040 --> 0:49:01.880
<v Speaker 1>not be able to aesc if you're still feeling its gravity?

0:49:02.280 --> 0:49:04.560
<v Speaker 1>What that means, is that anything that's happening to that

0:49:04.719 --> 0:49:08.280
<v Speaker 1>stuff that fell into the black hole, you can't tell. Basically,

0:49:08.320 --> 0:49:11.759
<v Speaker 1>the gravitation field is just frozen from that stuff. If

0:49:11.800 --> 0:49:14.040
<v Speaker 1>that stuff goes in and does a funny dance or

0:49:14.080 --> 0:49:18.160
<v Speaker 1>becomes a singularity, or becomes a quantum fuzzball, or does whatever,

0:49:18.760 --> 0:49:21.240
<v Speaker 1>you can't ever see. It can't ever tell you anything

0:49:21.280 --> 0:49:24.240
<v Speaker 1>about it. You can't ever learn anything about the configuration

0:49:24.480 --> 0:49:27.720
<v Speaker 1>of the mass within the event horizon. The gravitational field

0:49:27.760 --> 0:49:31.360
<v Speaker 1>of that stuff still exists, but it's now frozen in time.

0:49:31.719 --> 0:49:34.279
<v Speaker 1>You will get no more updates. If you take that

0:49:34.320 --> 0:49:37.080
<v Speaker 1>stuff inside the black hole and wiggle it around, generating

0:49:37.120 --> 0:49:40.439
<v Speaker 1>a bunch of gravitational waves within the event horizon, those

0:49:40.480 --> 0:49:44.040
<v Speaker 1>waves are trapped within the event horizon. Outside you will

0:49:44.080 --> 0:49:47.399
<v Speaker 1>still see the same exact gravitational field. And that's why

0:49:47.440 --> 0:49:50.600
<v Speaker 1>we made the distinction earlier about information being about updates,

0:49:51.000 --> 0:49:53.880
<v Speaker 1>because that gravitational field can be static. There's no information

0:49:54.000 --> 0:49:57.120
<v Speaker 1>escaping from within the black hole. It's just sort of

0:49:57.160 --> 0:50:00.279
<v Speaker 1>like think about the event horizon itself as having that

0:50:00.360 --> 0:50:03.840
<v Speaker 1>gravity or the last information you got about this stuff

0:50:03.920 --> 0:50:06.640
<v Speaker 1>was just before it falls into the black hole. It's

0:50:06.800 --> 0:50:11.359
<v Speaker 1>that gravitational field. You're feeling no updates, no information means

0:50:11.360 --> 0:50:13.640
<v Speaker 1>that gravitational field is effectively frozen.

0:50:13.880 --> 0:50:16.640
<v Speaker 2>So would it be fair to say that we can

0:50:17.120 --> 0:50:21.839
<v Speaker 2>get information from the existence of a black hole, and

0:50:21.920 --> 0:50:26.000
<v Speaker 2>we can get information by shooting information into a black

0:50:26.040 --> 0:50:30.239
<v Speaker 2>hole and then that sort of changing the characteristics of

0:50:30.239 --> 0:50:33.600
<v Speaker 2>the black hole. But we cannot get any information from

0:50:33.640 --> 0:50:37.240
<v Speaker 2>anything that is already inside of the black hole.

0:50:37.160 --> 0:50:41.640
<v Speaker 1>Exactly, because that would require communicating something physically. Right, if

0:50:41.680 --> 0:50:44.200
<v Speaker 1>you wanted to send information from within the black hole,

0:50:44.520 --> 0:50:47.560
<v Speaker 1>you'd need to like take a bowling ball and wiggle it,

0:50:47.640 --> 0:50:50.759
<v Speaker 1>which would generate gravitational waves. But I can't feel that

0:50:50.800 --> 0:50:53.320
<v Speaker 1>from the outside. What I feel is the gravitational field

0:50:53.360 --> 0:50:55.799
<v Speaker 1>of the stuff the moment it became a black hole.

0:50:55.880 --> 0:50:58.400
<v Speaker 1>That's when it got frozen in time. All the gravitational

0:50:58.440 --> 0:51:01.759
<v Speaker 1>waves generated inside of it, an updates to that gravitational

0:51:01.800 --> 0:51:04.239
<v Speaker 1>field are now trapped the same way that like if

0:51:04.239 --> 0:51:06.800
<v Speaker 1>you shoot photons or if you shoot electrons. Right, I remember,

0:51:06.840 --> 0:51:10.400
<v Speaker 1>information is physical. None of that physical information.

0:51:10.000 --> 0:51:12.640
<v Speaker 2>Can leave all right, But now hear me out. If

0:51:12.640 --> 0:51:15.800
<v Speaker 2>you had a really long string and you were sitting

0:51:15.840 --> 0:51:19.719
<v Speaker 2>here on Earth with a dixie cup attached to your end,

0:51:20.280 --> 0:51:22.719
<v Speaker 2>and I'm all the way in a black hole with

0:51:22.840 --> 0:51:25.799
<v Speaker 2>that string and a dixie cup on my end. No,

0:51:26.080 --> 0:51:30.680
<v Speaker 2>I cannot communicate any information to you, even if somehow

0:51:30.719 --> 0:51:34.200
<v Speaker 2>that string was strong enough to survive the black hole.

0:51:34.400 --> 0:51:34.600
<v Speaker 7>Right.

0:51:34.640 --> 0:51:37.359
<v Speaker 1>Well, there, you're creating a new paradox because there is

0:51:37.440 --> 0:51:40.279
<v Speaker 1>no string strong enough to survive the black hole. Right

0:51:40.560 --> 0:51:43.440
<v Speaker 1>Because as you zoom in microscopically to that string, it's

0:51:43.480 --> 0:51:47.239
<v Speaker 1>really just a bunch of particles transmitting information to each

0:51:47.280 --> 0:51:51.920
<v Speaker 1>other using electrons or using photons, and those photons cannot

0:51:52.040 --> 0:51:54.960
<v Speaker 1>escape the black hole. But you know, electrons and photons

0:51:55.000 --> 0:51:57.960
<v Speaker 1>are a great way to think about this information. Also,

0:51:58.560 --> 0:52:00.480
<v Speaker 1>like say you take an electron and you just have

0:52:00.480 --> 0:52:03.719
<v Speaker 1>an electron in space. Electron has an electric field, right,

0:52:04.000 --> 0:52:06.600
<v Speaker 1>a static field all through space. It gets stronger as

0:52:06.600 --> 0:52:09.759
<v Speaker 1>you're closer to it, and weaker as you get further away. Now,

0:52:09.760 --> 0:52:12.400
<v Speaker 1>what happens if you shake that electron. You shake that electron,

0:52:12.520 --> 0:52:15.960
<v Speaker 1>you're changing the electric field. And that change is a photon.

0:52:16.000 --> 0:52:19.960
<v Speaker 1>It's physical information. It's changing the field of the electron

0:52:20.120 --> 0:52:24.759
<v Speaker 1>that is transmitting the information. The static, frozen constant existence

0:52:24.840 --> 0:52:27.920
<v Speaker 1>of the field is not information, which is why stationary

0:52:27.960 --> 0:52:31.239
<v Speaker 1>electrons don't generate photons in the same way that like,

0:52:31.280 --> 0:52:34.320
<v Speaker 1>the existence of the black hole and its gravitational field

0:52:34.680 --> 0:52:37.080
<v Speaker 1>is sort of like old information from before it became

0:52:37.120 --> 0:52:40.040
<v Speaker 1>a black hole when it was created. Any new information

0:52:40.239 --> 0:52:43.520
<v Speaker 1>created within it by moving the stuff inside is not

0:52:43.560 --> 0:52:47.640
<v Speaker 1>going to be transmitted. So information gravitational waves or photons

0:52:47.680 --> 0:52:50.719
<v Speaker 1>really are about changes in the field, not about the

0:52:50.760 --> 0:52:52.480
<v Speaker 1>existence of the field itself.

0:52:52.800 --> 0:52:56.440
<v Speaker 2>So in my string and cup analogy, of course the

0:52:56.440 --> 0:53:00.200
<v Speaker 2>string would not survive. But you know, with a hypothetical string,

0:53:00.280 --> 0:53:02.479
<v Speaker 2>I could be shaken it, I could be talking into

0:53:02.480 --> 0:53:06.719
<v Speaker 2>the Dixie cup. But as soon as that information, you know,

0:53:07.000 --> 0:53:10.920
<v Speaker 2>is basically the part of the hypothetical string outside of

0:53:10.960 --> 0:53:15.560
<v Speaker 2>the event horizon is getting nothing from the string inside.

0:53:15.960 --> 0:53:18.080
<v Speaker 2>From within the event horizon.

0:53:17.840 --> 0:53:20.080
<v Speaker 1>Exactly, your string is going to be dangling towards the

0:53:20.120 --> 0:53:22.600
<v Speaker 1>center of the black hole. All the information you create

0:53:22.960 --> 0:53:25.319
<v Speaker 1>is going to get funneled towards the center of the

0:53:25.320 --> 0:53:25.920
<v Speaker 1>black hole.

0:53:26.239 --> 0:53:30.080
<v Speaker 2>Wow. Well, I'm gonna really emphasize that if I am

0:53:30.080 --> 0:53:35.120
<v Speaker 2>in a black hole. Pepperoni pizza is good. Also, do

0:53:35.160 --> 0:53:40.239
<v Speaker 2>a nice carbonara, just keep them common for eternity. I

0:53:40.280 --> 0:53:42.440
<v Speaker 2>suppose that sounds good.

0:53:42.480 --> 0:53:44.919
<v Speaker 1>It's good to get that information now before you fall

0:53:44.920 --> 0:53:45.759
<v Speaker 1>into the black hole.

0:53:45.960 --> 0:53:49.280
<v Speaker 2>Right could happen any day. We are sponsored by black

0:53:49.280 --> 0:53:53.400
<v Speaker 2>Hole Insurance. Make sure to set up your affares before

0:53:53.440 --> 0:53:56.120
<v Speaker 2>you get sucked into a black hole, or should I say,

0:53:56.200 --> 0:53:59.400
<v Speaker 2>not sucked into a black hole, but follow the curvature

0:53:59.440 --> 0:54:01.520
<v Speaker 2>of space into a black hole.

0:54:01.600 --> 0:54:05.040
<v Speaker 1>So you should think about black holes as barriers to information.

0:54:05.200 --> 0:54:07.200
<v Speaker 1>But I hope this podcast has helped you understand a

0:54:07.200 --> 0:54:10.759
<v Speaker 1>little bit more what that means, what information really is,

0:54:11.239 --> 0:54:15.200
<v Speaker 1>because what's inside a black hole can affect what's outside

0:54:15.200 --> 0:54:18.080
<v Speaker 1>a black hole. The creation of the black hole itself

0:54:18.360 --> 0:54:21.640
<v Speaker 1>affects space time near the black hole. But sort of

0:54:21.640 --> 0:54:24.280
<v Speaker 1>in a simplified way. We can only know a few

0:54:24.360 --> 0:54:26.200
<v Speaker 1>things about the black hole. We can know it's mass,

0:54:26.200 --> 0:54:28.200
<v Speaker 1>we can know it's charge, we can know its spin.

0:54:28.640 --> 0:54:31.560
<v Speaker 1>Anything else that happens within the black hole can't change

0:54:31.560 --> 0:54:35.400
<v Speaker 1>what's happening on the outside. The changes behind the barrier,

0:54:35.680 --> 0:54:38.439
<v Speaker 1>wiggles and rearrangements of the stuff within the black hole

0:54:38.520 --> 0:54:42.279
<v Speaker 1>can't influence things on the outside. So I think the

0:54:42.320 --> 0:54:45.640
<v Speaker 1>crucial concept there is that information really is about changing

0:54:45.680 --> 0:54:49.160
<v Speaker 1>the internal arrangements. That's what you're prevented from knowing not

0:54:49.239 --> 0:54:51.319
<v Speaker 1>the existence of the black hole, but what's going on

0:54:51.600 --> 0:54:52.359
<v Speaker 1>inside of it.

0:54:52.600 --> 0:54:56.360
<v Speaker 2>So I could be inside of the black hole, drunk

0:54:56.360 --> 0:55:00.800
<v Speaker 2>off of Martini's, standing on the black hole jack table

0:55:01.120 --> 0:55:05.359
<v Speaker 2>and screaming out the lyrics to a Katie Perry song,

0:55:05.600 --> 0:55:06.959
<v Speaker 2>and no one would ever know.

0:55:07.160 --> 0:55:09.800
<v Speaker 1>Only people within the black hole and closer to the center.

0:55:10.480 --> 0:55:13.480
<v Speaker 1>But hopefully what happens inside a black hole stays inside

0:55:13.480 --> 0:55:14.040
<v Speaker 1>a black hole.

0:55:14.200 --> 0:55:18.160
<v Speaker 2>Yeah, well that's good information to know, because I know

0:55:18.360 --> 0:55:21.080
<v Speaker 2>now where I'm going to do my next Vegas trip

0:55:21.960 --> 0:55:23.520
<v Speaker 2>and it's not in Vegas.

0:55:23.280 --> 0:55:25.640
<v Speaker 1>All right. Well, I want everybody out there to keep

0:55:25.719 --> 0:55:28.960
<v Speaker 1>thinking like a physicist, trying to bring pieces of understanding

0:55:29.000 --> 0:55:32.040
<v Speaker 1>together and weave them into a deeper, more profound model

0:55:32.080 --> 0:55:34.879
<v Speaker 1>in your head about how the universe works, how these

0:55:34.920 --> 0:55:38.520
<v Speaker 1>things all interact, and when things don't jive together, when

0:55:38.560 --> 0:55:40.239
<v Speaker 1>they don't make sense to you, or when you feel

0:55:40.239 --> 0:55:42.960
<v Speaker 1>like you have hit upon a contradition right to us,

0:55:43.080 --> 0:55:46.800
<v Speaker 1>we will help you figure it out. Questions at Danielanjorge

0:55:46.920 --> 0:55:50.320
<v Speaker 1>dot com. Our goal is to turn everybody into a physicist.

0:55:50.680 --> 0:55:53.560
<v Speaker 2>You and your army of physicists. What are you planning?

0:55:53.760 --> 0:55:56.640
<v Speaker 1>I can neither confirm nor deny our plan. Thanks very

0:55:56.719 --> 0:55:59.360
<v Speaker 1>much Katie for joining me on this path towards the

0:55:59.400 --> 0:56:03.040
<v Speaker 1>center of understanding following the curvature of explanations.

0:56:03.280 --> 0:56:05.680
<v Speaker 2>Thank you for all the information. I'm glad we're not

0:56:05.800 --> 0:56:08.680
<v Speaker 2>broadcasting from a black hole where nobody would.

0:56:08.560 --> 0:56:11.359
<v Speaker 1>Know, and thanks everybody for listening. Tune in next time.

0:56:12.320 --> 0:56:14.280
<v Speaker 4>Hey, this is Joege from the podcast and I'm super

0:56:14.280 --> 0:56:17.320
<v Speaker 4>excited to announce that my new book, Oliver's Great Big Universe,

0:56:17.480 --> 0:56:20.400
<v Speaker 4>is out now. It has humor, cartoons, a fun story,

0:56:20.440 --> 0:56:23.160
<v Speaker 4>and lots of awesome signs, and it's perfect for kids

0:56:23.160 --> 0:56:25.120
<v Speaker 4>that are into science, but also kids who are not

0:56:25.200 --> 0:56:28.080
<v Speaker 4>into science yet. There are chapters about black holes the

0:56:28.120 --> 0:56:30.680
<v Speaker 4>planet's dark energy, but at the heart of it is

0:56:30.680 --> 0:56:33.160
<v Speaker 4>a story about friendship and figuring out your place in

0:56:33.200 --> 0:56:34.839
<v Speaker 4>the world, so please check it out. You can get

0:56:34.840 --> 0:56:38.319
<v Speaker 4>it in stores, online, and at Great Big Universe dot net.

0:56:46.239 --> 0:56:49.040
<v Speaker 1>Thanks for listening, and remember that Daniel and Jorge explain

0:56:49.120 --> 0:56:53.120
<v Speaker 1>the universe is a productive of iHeartRadio. For more podcasts

0:56:53.120 --> 0:56:57.040
<v Speaker 1>from my Heart Radio, visit the iHeartRadio app, Apple Podcasts,

0:56:57.200 --> 0:57:10.680
<v Speaker 1>or wherever you listen to your favorite