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This is StarTalk Cosmic Queries Edition. Of course, I got
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Chuck Nice with me to make this happen. Chuck.
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What's up, Neil?
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Dude, you know, it's not often we get one of
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my own people in a Cosmic Queries. That's right. Just
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my kindred spirit. And today, we've got Professor Hair Doctor
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Brian Cox across the pond from the UK. Brian, welcome
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to StarTalk, dude. Not your first rodeo with us. No,
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it isn't.
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No, we've been doing this for a few years now.
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I think it was about 10 years ago. I've been
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a guest on your show. A couple of times I've
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been in the UK. I was there live. You got
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an audience and stuff. So that was fun. And so
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let me make sure I get your bio accurately described here.
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So you're a professor of particle physics, University of Manchester.
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That sounds very specific. You're not just a professor of physics, right? Yeah.
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Particle physics.
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Yeah.
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I mean, am I.
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My research history is I've worked at the particle accelerators
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around the world, actually, including Fermilab in Chicago, DAISY in Hamburg,
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and CERN in Geneva.
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Yeah, the big one, CERN. And so out of the UK,
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you've hosted multiple TV shows. The one I remember most
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is The Universe. And you also did one on the
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solar system, correct? Correct me if I'm wrong.
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Solar system.
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And, uh, that was the local version of that travel show.
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Yeah. This is the bit that we might be.
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Able to travel show was the universe. And you were like,
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by the way, check out this neighborhood.
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We're going to do multiverse next.
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And you've got another one, Brian Cox's adventures in space
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and time. And, uh, for me, what's most important is
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that you have come stateside. You have crossed, you've crossed
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the ocean. to give a multi-city stage theater tour of
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the universe. This is bold, hairy, and audacious. I love it.
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I love it.
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And by the time this posts, you're in the middle
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of the tour, coming up in Edmonton and Canada, Edmonton, Calgary, Vancouver,
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and then you slip down into Seattle, Portland, can't not
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do them if you're doing Canada, right? And then Sacramento,
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San Francisco, San Jose, Los Angeles, two nights in Los Angeles,
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San Diego. Then you hit up Texas.
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And it sounds like a Johnny Cash song. I've been everywhere, man.
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And you end it in Texas, Houston, Texas. So good
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luck with that tour. Oh, my gosh. What can people expect?
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Well, it's spectacular is the first thing to say. So
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we use the biggest LED screen that we can fit
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into the venues. And it was designed actually for the,
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in the fall, we're doing these huge shows in the,
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in the UK. Cause I always say to you, you know,
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people know who I am in the UK and it's
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a bit more, a bit more low key in the US.
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So the show's designed for 15,000 seat arenas. And so
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we produce these graphics of flying into black holes, a
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lot of black holes in there considering the, uh, the
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nature of life in the universe, origin of life, future
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of life, the multiverse. So all the big questions in space, time,
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black holes, cosmology. But it's essentially big graphics. And hopefully
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for everybody, I mean, I do do some complicated stuff
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in the middle about quantum entanglement and the black hole
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information paradox that we can talk about later. But the
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idea is that.
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It's a show. Of course, it wouldn't be a show
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unless you did that. Right, right, of course, duh.
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I was talking to that with my eight-year-old last night.
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It's on the tip of everybody's tongue.
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It is. I was like, sweetie, now just remember in
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the morning we'll finish this little conversation on quantum entanglement.
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In the meantime, sleep here, but not here in L.A.
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So this is not a Brian Cox lecture on stage.
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This is a performance with a hugely visually delivered messaging
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about science and physics and the universe and yeah.
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And uh there's music's a big part of it so
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it starts with um Sibelius's fifth symphony the third movement
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and uh almost a version of 2001 that I ended
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up making because I asked a friend of mine who's
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a conductor as a joke one night you know what
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said what should Stanley Kubrick have used right and he
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was kind of a joke but he immediately said he
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should have chosen this piece of music by Sibelius which
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was written in 1915. And it's at one level, it's
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about swans taking off from a lake in northern Finland.
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But at another level, it's about the deep beauty of nature.
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It's that idea, that famous quote from Einstein, that if
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you look carefully at nature, you might catch a glimpse
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of something deeply hidden, which is the structure of nature itself.
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And so it just sounded like that to me. So
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I ended up almost remaking 2001 in eight minutes, which
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to the horror of my promoter.
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So let me quantify how popular you are in the UK.
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I have a way to measure that for you. I
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don't know if I ever told you this. So right
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now in the United States, I'd be stopped by 15
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out of 20 people in the street, because they'd recognize me, whatever.
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I think for you, it's 20 out of 20, or
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21 out of 20 people. in the UK, but I
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can quantify that, okay? You were so popular there that
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no one knows who the hell I am there, so
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watch what happened. We were filming Cosmos. We're in Trafalgar Square,
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big square, and we're filming Cosmos, and we're cordoned off, okay?
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And I'm there, you know, delivering lines and things, and
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all manner of people, hey, that's Neil deGrasse Tyson. I said, oh,
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where are you from? Oh, we're from the Netherlands. Oh,
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we're from India. Oh, we're from Russia. Oh, we're from...
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Nobody stops who is from the UK.
Nobody. So either
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they're just polite and they don't, or you completely occupy
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that space in the UK. And that's what I'm thinking
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is going on there.
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Or... Brian does all of his talks in the UK,
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and instead of ending it with keep looking up, he
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ends it with don't listen to Neil deGrasse Tyson.
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I'm totally happy, okay, to swap for a few months.
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So you can have the UK. I'll have the US
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just until the end of this tour. We'll swap roles.
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That's a good deal for me.
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Here's the question, Brian.
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I can't even recite this many cities in the UK
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that you're going to do here. In the United States.
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You know what this feels like? A little bit. Because
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you've got that Beatles haircut. It feels a little bit
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like the British invasion, you know? Putting us in a
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new place that we didn't even know we could land.
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Nothing wrong with that. Yeah, nothing wrong with that. Very cool. So, Chuck,
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you collected questions from our Patreon supporters.
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Indeed, we do have them. And, of course, you know,
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our listeners are very excited. to ask Brian questions. So
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do you want to jump into this?
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Yeah, let's go straight ahead. What do you have?
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All right, this is Marcus Gustafsson, who says, hello and
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greetings from Sweden. If the strength of gravity happened to
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be a little stronger or a little bit weaker than
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it is, how different would our universe be?
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It's a good question and it's this is widely debated
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actually because um there's a question of how much you
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can change the the fundamental properties of nature so do
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you say the strength of gravity the mass of the
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electron the way the higgs field works all those things
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such that you have a radically different universe and actually
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it's quite hard because you can change some things and
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then change something else and it kind of balances the
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change out and and so it's quite a controversial area
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actually but Broadly speaking, if gravity were too strong, all
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else being equal, then things would collapse ultimately into black
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holes very quickly. So the early universe would not have
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formed extended structures like galaxies and solar systems, or stars
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may be very short-lived and so on. So you can
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change the universe such that you would not have life
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in the universe if you increase the strength of gravity
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too much. But also you can decrease it too much,
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and then stars and galaxies don't form in the early universe.
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you probably don't have a living universe. Now, the complication
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comes when you say, okay, well, what if in the
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early universe the slightly over-dense regions were a bit denser,
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which would have something to do with a theory we
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called inflation, possibly, or something the way the Big Bang was,
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and then you turn gravity down a bit. Can you
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kind of compensate? And it's true, you can. So it
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becomes an extremely difficult modelling challenge And so you'll see
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research papers on this. How can you change the things
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and fine tune things? But then broadly speaking, that's what happens.
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If it is too strong, then everything collapses into black holes.
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And if it is too weak, nothing forms at all.
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So that's the physicist answer. Okay. Now we'll give you
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the astrophysicist answer.
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All right.
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In graduate astrophysics 101, okay, one of the first calculations
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we do is, What happens to the luminosity of a
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star if you change the gravitational constant? It's a calculation
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we do. So what you do is you put a
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little parameter there and see what happens to that parameter
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as you run through the calculations for a star's luminosity.
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And what you find is that the luminosity of a
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star is extremely small. sensitive to the value of Newton's
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gravitational constant, to the seventh power. So what's
interesting about
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that is if the gravitational constant were different, slightly higher
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earlier in the universe than today, As Brian can attest,
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there are whole branches of physics that think about and
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wonder and worry about whether the constants have actually been constant.
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Forget whether we have godlike powers to just change it
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and see what happens. Were they always this good? Did
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they change over time? So you can look at how
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sensitive it is and constrain how much it could have
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possibly changed because you would see stars of enormous luminosities
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living out their lives very quickly in the early universe,
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and you don't see that. So it's to the seventh
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power of that term that the luminosity would be affected.
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And seventh power is that times that times that times
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that times that, okay, all through. So we actually find
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that number in intro astrophysics graduate school.
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And can you define luminosity for me? Because if you're
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saying that it's not just brightness.
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Oh, yeah, yeah, yeah. So here it is. It's simple luminosity.
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This example is rapidly becoming obsolete, but take a 100-watt
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light bulb, okay? Yeah, well, yeah. Okay, what is that, right? Yeah, exactly.
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In the old days, there was like the bulb.
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That's like, okay, now here's what you do first. You
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dial up your grandmother on a rotary phone.
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So the wattage is its luminosity. So no matter what
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distance I put it from you, it will always be
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a 100-watt bulb.
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Okay, gotcha.
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As I get it farther away, it gets dimmer and
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dimmer and dimmer, so that would be its brightness. That's all.
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So that's it, so okay. So you're saying that gravity
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is like a string on the light itself, kind of
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like that would be making it less?
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No, no, it would be like a knob.
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Like a knob turning it down. Increase the wattage.
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Thank you, right.
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So instead of pulling it back, it's turning down the wattage. Okay,
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that's cool, man.
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Yeah, it's a dimmer or a thing on the bulb itself. Yeah,
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let's make the universe sexy, baby. You know?
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Let's dim the lights, hey, you know. How would you
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like a little cosmic champagne?
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All right. Time to go to the next question. That's
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how you know.
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I'm enjoying this.
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You like the sexy universe, Brian?
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Yeah. I'm going to use some. I'm making notes.
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All right. Let's go to Sandra Bayani. And Sandra says,
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is it possible that the laws of physics change beyond
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our cosmic horizons so that all of our theories about
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multiverses stop working and stop making sense. Greetings, fellow Earthling.
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I cannot get enough of this show. Please, whatever you do,
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never stop this podcast.
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Oh, Chuck, did you just add that?
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No, I didn't. I really didn't.
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I mean, I love that question.
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Yeah, that's wonderful.
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I love that question because it brings in our horizon
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and multiverses and the very theories that predict a multiverse.
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work in our universe, why should they work in another?
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We're going to take a break, and when we come back,
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we will get right to the heart of that question
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with our special guest today. He's a special guest to me,
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Brian Cox from over in the UK. We'll be right back.
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We're back, StarTalk Cosmic Queries. This is everything physics, because
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I got one of my people here, one of my
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science and education brethren, Brian Cox from over in the UK,
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who They call him a rock star over there, and
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we've said this on his previous appearances, but it's worth
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repeating that this man had a number one song on
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the pop charts in the UK. So you're a literal
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and figurative rock star of science. Have I overstated that, Brian?
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No, I think you've understated it, if anything.
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So what was the name of the song again that
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you performed?
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The most famous song is a song called Things Can
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Only Get Better, which you will say correctly runs counter
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to the second law of thermodynamics.
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Oh, yes.
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So it's an inaccurate song, but yeah.
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Yeah, sometimes you got to break some eggs to make
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an omelet, you know, as they say.
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All right.
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So Chuck, we left off with a brilliant question about
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here we are in our universe that has our own
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horizon and we come up with our own theories of
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the universe. And one of them is that there might
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be a multiverse. So beyond our horizon, if it's not
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in our universe, Why should we even believe that the
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rules that predict a multiverse would even exist? There you go.
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I love that.
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There's a lot to unpick there. So our horizon, first
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of all, there is a limit to how far we
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can see, which is the fact that our universe is
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of a finite age, or let's say there's been 13.8
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billion years since the Big Bang. And so there's a
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finite distance you can see because light travels at a
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finite speed. So we are very sure that that there
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are galaxies way beyond our horizon, but essentially the light
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has not had time to reach us from them. Now, actually,
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as Neil said in the answer to the last question,
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you can say, well, observationally, do we see any evidence
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of the laws of nature? So the strength of gravity,
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for example, going back to the last question, changing as
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we look out to the most distant galaxies. And the
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answer is no. We have no evidence that they change
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in the patch of the universe we can see. So
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that's the observational point. But when you start to talk
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about the laws of nature in different regions of the universe,
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our multiverse, as you said, then it becomes more interesting.
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One multiverse, there are lots of different kinds of multiverse,
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but one of them is called the inflationary multiverse. So
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we have a theory called eternal inflation, which essentially leads
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to the idea that there are perhaps an infinite number
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of bubble universes of which ours is one. And the
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piece that we can see, the observational piece, The little
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piece we can observe is a patch in one bubble
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universe amongst perhaps an infinite number of bubble universes in
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the inflationary multiverse. And those theories do lend themselves, potentially,
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to the laws of nature in each bubble possibly being different.
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And the way I sometimes picture it is like a
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snowstorm with snowflakes. So every snowflake is different because it's
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had a different formation history. But there's something similar about
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them all. which goes to the underlying structure, which is
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to do with the water molecule itself. So there's something similar.
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There's an underlying framework, but every snowflake is different. And
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the inflationary multiverse can be like that. So you can
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imagine that the laws we see, things like the strength
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of gravity, sort of crystallize out as these bubble universes
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form from the potential, which is this thing called inflation
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that's potentially going on all the time. So it's possible.
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that different universes have different emergent laws, things like the
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strength of gravity. I think most physicists probably all expect
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that there'll be some kind of underlying framework, which could,
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something that we don't know what it is, right? Something
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like string theory or something, which underlies the whole thing.
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So that, maybe Neil wants to add, but that's my
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summary of the inflationary multiverse.
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I love your snowflake analogy, but suppose that, Do you
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have enough latitude in your eternal inflationary multiverse model to
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have a universe that has five-pointed snowflakes instead of six?
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I mean, how much room do you have to just
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make stuff up completely?
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We don't know. This goes back. It links to something
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called the string landscape, which Leonard Susskind actually wrote a
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great book called The Cosmic Landscape a while ago detailing
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this theory. So when you look at string theory.
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Just remind me, Leonard Susskind is the one who's a
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big exponent of the holographic universe. That's the same guy.
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Yeah, he's been at the cutting edge of physics for decades,
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raising it. So in the string landscape, the idea is
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that in string theory, it turns out you can have...
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There's a number that they calculate. I don't know how
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they do it, actually, but it's something... Well, I do
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know how they do it. It's something to do with
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all the extra dimensions being curled up and stuff. It
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doesn't matter. but essentially 10 to the power 500 different possibilities.
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So one with 500 noughts after it. These are the
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different ways that you can produce laws of physics like
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the ones we see from the underlying theory. And that
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was seen as a really disappointing.
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That's a lot of wiggle room right there.
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But the way I see it, it's almost like saying
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we understand DNA. So in biology, we have a theory,
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we have these things, A, C, D, T, and G.
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the four different bases that come together to form DNA.
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And it's like saying, okay, so there's an underlying theory.
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It's pretty simple. It's the double helix. It's chemistry. Out
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of that, it's like saying, right, predict a human being. So,
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of course, you can't because there are many different combinations
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of DNA. And we have no understanding yet of which
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ones would work and which ones wouldn't and which ones
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can be realized by evolution and which ones can't.
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It's an astronomical number of combinations of just to make
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humans let alone all forms of life.
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So it's like saying we understand the basic chemistry that
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gives us that thing, DNA. But then from that, predicting
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a particular instance of that, an organism, is of course,
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it depends on its history. It depends on all sorts
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of things, and it's the same.
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If you look at that like, I don't know, an
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alphabet to create a language, can you rule out the nonsense?
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For instance, if you know English, you know that HLPPP500.
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It's not a word. Right?
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So are you able to kind of rule out the
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nonsense that, okay, these things would not happen. And so
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even though it is a possible combination, we know that
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it's kind of gibberish. How do we narrow that?
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Well, I mean, we don't. We don't know. We haven't
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got the expertise. We don't really know what the underlying
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theory is. But I mean, for example, you could imagine
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a bubble universe that forms and Gravity is so strong
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that it just collapses again in a millisecond. There may
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be many universes like that. So that might be, as
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you say, that might be a universe that we consider
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was just never got going. So it's undoubtedly true.
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That's a gibberish universe.
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That would be a gibberish universe, maybe. So it might
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just about form and then collapse again, for example.
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You'll know if you meet a life form from there
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because it's just like.
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Not only are the laws of physics gibberish, so is
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their language, right? That's what you're saying.
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I just want to emphasize, this is speculative stuff. So
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the string landscape, as I said, Leonard Susskind's book is
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great on this. And then the link, though, It's interesting
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that inflation, which Neil will know about as well, that's
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a theory that was introduced initially just to deal with
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something called the horizon problem. You mentioned the horizon. It's
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essentially the unexplained point that if you look in one
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direction out into the universe as far as you can,
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and then turn around and look in the other direction,
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then you're looking at points that emitted light that we're
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receiving now, that now... in the universe is something like
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93 billion, I think it is light years away, right?
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Because of the expansion of the universe. So you're looking
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at points that in the standard model of things could
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never have been in contact with each other and yet
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are at the same temperature. So one part in 100,000,
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which is an observation. So that means, and inflation is
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initially- Just a.
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Quick thing, Chuck, I think we did an explainer on this.
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There was something where I was talking about that the
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universe has a more uniform temperature than- Different parts of
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the same room you're in.
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Right.
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Well, that's because with that explainer, we were talking about
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redshifting is kind of how we got into it.
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Oh, that's how we got there. Because I was saying
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you have an air conditioner in a corner, you have
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a heater over there, and you're fine if it's a
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five-degree range in a room that's talking to itself thermodynamically.
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And now we have across the whole freaking universe, and
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it's within 100,000th of a degree, which is completely mind-boggling freaky.
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And we needed a freaky explanation for it.
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Yeah. So inflation was the idea that once upon a
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time they were in contact. And then the universe expanded very, very, very,
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very fast for probably a small amount of time. And
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so we thought that they couldn't have been in contact
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with each other. But in fact, they were. And so
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that's why inflation was introduced. But it ended up doing
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several things that it was not designed to do initially.
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One was that the thing that drives inflation which has
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got a fancy name called the inflating field, but it
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doesn't matter what it is.
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It's a breakdown in the supply chain.
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00:23:26.539
Oh, it makes that look trivial. Two points were doubling in,
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if you take the two points in the universe, then
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they double, the distance between them doubled every 10 to
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the minus 37 seconds in the basic models of inflation.
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So it's much worse than we're going through now with prices.
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It's an exponential expansion.
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Much worse is an understatement there, just to be clear.
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But in looking at that, Stephen Hawking actually was involved
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in this, and many physicists in the 80s found that
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these theories.
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Chuck, Chuck, last time we did this, he said, Stephen was.
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Involved in this. He's cleaning it up this time, Neil.
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He's been a little better.
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A name drop.
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We got to hear the last name here.
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Stephen, Kip, Lenny, all those people.
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This time.
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So that theory was discovered, predicted, that there would be
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ripples in the density of particles in the universe through
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the Big Bang as inflation drew to a close, which
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are the ripples that we see in the cosmic microwave
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background radiation, which you may have talked about, and also
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actually in the distribution of galaxies across the sky. So
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there's a distribution. They're not just completely random across the sky.
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There are patterns in the galactic distribution. And that was
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predicted before it was observed by this theory. So the
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theory is interesting. And textbook, you'll find it in cosmology textbooks.
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But the eternal inflation bit, which is kind of an
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add-on to that, ends up with this idea that inflation
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doesn't stop everywhere at the same time, basically. So you
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get multiple bubble universes. And then that theory was noticed
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that that's a mechanism to realize the string landscape. which
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gives you the possibility of varying the laws of nature
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in each of those bubbles. So that was the history.
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So it's not just, it sounds fantastical, but it's not
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00:25:10.920
just like somebody just dreamt it up one day and
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said this would be cool.
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I try to make that clear because otherwise they think
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we're just pulling stuff out of our ass. And it's,
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even if it is out of our ass, it's very
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carefully withdrawn.
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By the way, that's one of the universes.
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Yeah.
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With a central black hole. Time to go to the
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next question. Oh, no.
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Time to go to the next question.
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Okay, here we go. Hitty Wagemans says this. Hello, Dr.
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Tyson, Dr.
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Cox, and Lord Nice, and I bet you can't pronounce
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my name correctly. You win that bet, all right? Get
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no argument from me.
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And the name is what?
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His name is H-I-D-D-E-W-A-A-G-E-M-A-N-S. I said Hiddy Wigmans. And he's
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from the Netherlands, so he's Dutch. It's a Dutch name.
477
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That helps how to pronounce that, yeah. He de Wegmans, maybe.
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He de Wegmans, okay. Yes, if it's Dutch, it's... He says,
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00:26:20.319 --> 00:26:24.150
I'm asking myself after I watch the movie, The Atom Project,
480
00:26:24.930 --> 00:26:29.329
if you really can time travel with wormholes. By the way, oh,
481
00:26:30.009 --> 00:26:35.390
here we go. Chuck Headey is pronounced hidden without the N.
482
00:26:36.619 --> 00:26:41.170
Who knew? There you go. You've got to read to
483
00:26:41.190 --> 00:26:43.230
the end so you can help you pronounce it. People
484
00:26:43.289 --> 00:26:45.309
help you out there. That is too much work, Neil.
485
00:26:51.200 --> 00:26:55.660
So Brian, we're talking about time travel and wormholes. I presume,
486
00:26:56.680 --> 00:26:59.920
I think everyone knows with Einstein relativity, you can travel
487
00:26:59.960 --> 00:27:02.980
into a future, or at least into the future of
488
00:27:03.019 --> 00:27:05.619
where you once were. So let's confine this to can
489
00:27:05.660 --> 00:27:09.240
you go backwards in time? Do wormholes enable this at all?
490
00:27:09.740 --> 00:27:13.339
Wormholes are getting increasingly interesting, actually, particularly in the study
491
00:27:13.359 --> 00:27:16.700
of black holes. We can get onto that. So yes,
492
00:27:17.019 --> 00:27:21.900
wormholes are allowed geometries in Einstein's theory of general relativity,
493
00:27:22.180 --> 00:27:24.220
if you just take that theory alone. What do I
494
00:27:24.259 --> 00:27:27.180
mean by that? So they really are shortcuts through space
495
00:27:27.240 --> 00:27:29.740
and time. So you can imagine, you know, traveling from
496
00:27:29.809 --> 00:27:32.250
New York to Sydney, it takes a long time. You
497
00:27:32.289 --> 00:27:33.869
go around the surface of the Earth, or you could
498
00:27:33.910 --> 00:27:37.170
tunnel through, and you could get there quicker. So yes,
499
00:27:37.430 --> 00:27:41.960
if wormholes exist, and you could travel through them, and
500
00:27:42.000 --> 00:27:45.589
they were big enough and stable enough, then you can
501
00:27:45.680 --> 00:27:51.670
build a time machine. Now, virtually every physicist who works
502
00:27:51.750 --> 00:27:54.009
on this, and Kip Thorne, actually, who got the Nobel
503
00:27:54.029 --> 00:27:56.950
Prize for gravitational waves, did quite a lot of interesting
504
00:27:56.970 --> 00:27:59.759
work on this. And he was.
505
00:27:59.720 --> 00:28:01.539
The main advisor in the movie Interstellar.
506
00:28:01.619 --> 00:28:02.240
He was, yeah.
507
00:28:02.299 --> 00:28:04.819
In fact, an executive producer. And the robot in that
508
00:28:04.839 --> 00:28:05.579
movie was named Kip.
509
00:28:06.079 --> 00:28:09.319
It was, and it has a wormhole. And he also
510
00:28:09.400 --> 00:28:13.200
actually suggested to Carl Sagan in Contact that wormholes were
511
00:28:13.319 --> 00:28:14.759
used in the film.
512
00:28:14.819 --> 00:28:15.900
In the movie Contact.
513
00:28:15.920 --> 00:28:20.319
And the novel, actually, first. So when you add quantum
514
00:28:20.339 --> 00:28:23.289
mechanics into the mix, which is the theory of everything else,
515
00:28:23.640 --> 00:28:26.049
because our universe hasn't just got gravity in it, it's
516
00:28:26.069 --> 00:28:27.670
got all sorts of other things in it as well,
517
00:28:27.730 --> 00:28:31.549
obviously atoms and electromagnetic radiation and so on, then it
518
00:28:31.750 --> 00:28:35.170
seems like the wormholes are inherently unstable, the big ones.
519
00:28:35.779 --> 00:28:38.299
And if you try to travel through one, it collapses.
520
00:28:38.940 --> 00:28:40.609
So that's basic. I should say, by the way, that
521
00:28:40.640 --> 00:28:44.309
they're such an integral part of Einstein's theory. There's a
522
00:28:44.309 --> 00:28:47.210
very famous paper in the 1930s by Einstein and Rosen.
523
00:28:47.950 --> 00:28:51.549
And they were called Einstein-Rosen bridges before they were wormholes.
524
00:28:52.069 --> 00:28:56.009
And they're built into the basic description of a black hole.
525
00:28:56.170 --> 00:28:59.839
If the black hole had lived forever, it's called the
526
00:28:59.890 --> 00:29:02.279
maximally extended Schwarzschild metric, right?
527
00:29:02.319 --> 00:29:02.500
Whatever.
528
00:29:02.910 --> 00:29:07.089
It's called, but that which was discovered by Schwarzschild in 1916,
529
00:29:07.089 --> 00:29:09.710
just after the theory was published, then there's a wormhole
530
00:29:09.750 --> 00:29:12.269
in there, right?
So they're just fundamental to the theory,
531
00:29:12.730 --> 00:29:16.009
but most physicists believe, and Stephen Hawking wrote a paper
532
00:29:16.049 --> 00:29:19.990
actually called the chronology protection conjecture, conjecture, where he thought
533
00:29:20.039 --> 00:29:20.339
about this.
534
00:29:20.359 --> 00:29:21.539
Who knew he was a rapper?
535
00:29:21.559 --> 00:29:22.359
They will be unstable.
536
00:29:23.160 --> 00:29:23.359
Yeah.
537
00:29:23.700 --> 00:29:25.859
I can even say it. You can say it. I
538
00:29:25.880 --> 00:29:30.579
can't say it. Chronology protection conjecture. Yeah. But these things
539
00:29:30.599 --> 00:29:32.420
would not be stable and you can't travel through them
540
00:29:32.440 --> 00:29:36.230
so you can't build time machines. However, it's worth saying
541
00:29:36.670 --> 00:29:39.910
that wormholes are becoming very, very fashionable now in wormholes.
542
00:29:40.150 --> 00:29:44.819
called the er equals epr paradigm so einstein rosen er
543
00:29:44.880 --> 00:29:47.740
is einstein rosen this thing from the 1930s where einstein
544
00:29:47.759 --> 00:29:50.779
and rosen noticed that they these geometries exist in space
545
00:29:50.819 --> 00:29:55.559
time or can exist epr is einstein podolsky and rosen
546
00:29:55.779 --> 00:29:59.839
spooky action at a distance it's quantum entanglement And so
547
00:30:00.180 --> 00:30:03.680
what now is very fashionable and looks as one of
548
00:30:03.720 --> 00:30:06.019
the best explanations of how information gets out of a
549
00:30:06.059 --> 00:30:09.160
black hole is that this plays a role. So you can,
550
00:30:09.220 --> 00:30:11.380
there's a kind of a dual description. So we've got
551
00:30:11.420 --> 00:30:14.099
quantum entanglement, which is this spooky action at a distance
552
00:30:14.140 --> 00:30:17.079
thing where you separate things to large distances and they're
553
00:30:17.099 --> 00:30:21.119
still linked in some way. The linked in some way
554
00:30:21.319 --> 00:30:24.099
is starting to look possibly like you can describe that
555
00:30:24.140 --> 00:30:28.220
in terms of wormholes. microscopic wormholes linking them together but
556
00:30:28.240 --> 00:30:30.720
this is really this is stuff that's being done now
557
00:30:30.720 --> 00:30:34.339
2020 2022 so it's um it's on the edge but
558
00:30:34.400 --> 00:30:35.160
people are taking it.
559
00:30:35.299 --> 00:30:37.859
Okay so wait let's let's pause there and come back
560
00:30:37.960 --> 00:30:40.880
but all right now you've established that we agree we
561
00:30:40.900 --> 00:30:42.700
can think about wormholes but you haven't told us how
562
00:30:42.740 --> 00:30:45.200
to go backwards in time when we come back brian
563
00:30:45.220 --> 00:30:46.420
cox is going to tell you how to go back
564
00:30:46.819 --> 00:30:49.180
and not kill your parents okay.
565
00:30:50.369 --> 00:30:52.150
And i can tell you an even simpler way if
566
00:30:52.190 --> 00:30:54.630
you really want to go backwards in time get married
567
00:30:54.670 --> 00:30:58.130
and do something wrong Because she will never let you forget.
568
00:30:58.170 --> 00:31:02.420
Forget. Thank you, Chuck, for your marital, splitting your marital
569
00:31:02.480 --> 00:31:06.400
issues into this podcast. StarTalk will return with Brian Cox.
570
00:31:06.420 --> 00:31:08.099
We're going to find out how to go back in time.
571
00:31:08.960 --> 00:31:15.099
Be there. We're back. StarTalk, Cosmic Queries. Got Chuck, of course. Chuck,
572
00:31:15.119 --> 00:31:18.380
you're tweeting at ChuckNiceComic. Thank you, sir. You've got some
573
00:31:18.460 --> 00:31:21.539
fun stuff there that tracks current events and things. It's
574
00:31:21.559 --> 00:31:23.720
always good to see what you have to say about that.
575
00:31:24.200 --> 00:31:27.660
And Brian Cox, my friend and colleague from the UK,
576
00:31:27.769 --> 00:31:30.630
is taking the United States by storm and a little
577
00:31:30.650 --> 00:31:35.750
bit of Canada in dozens of cities. He's bringing his
578
00:31:36.210 --> 00:31:41.069
major theatrical production. Do you give it a title or
579
00:31:41.089 --> 00:31:43.130
is it just everything you want to know about where
580
00:31:43.170 --> 00:31:44.730
we are in the universe? How about that?
581
00:31:45.470 --> 00:31:46.069
Horizons.
582
00:31:46.230 --> 00:31:47.410
Horizons. There it is.
583
00:31:49.259 --> 00:31:52.559
Billy Connell is over that way. No, which way? That way.
584
00:31:52.720 --> 00:31:55.839
There he is. And Brian Cox, you can find his
585
00:31:55.859 --> 00:32:02.750
schedule in briancoxlive.co.uk. Just do a Google on Brian Cox Live.
586
00:32:02.789 --> 00:32:05.230
It'll send you there. And you can see the whole schedule.
587
00:32:05.690 --> 00:32:10.769
And he's coming through town with a hugely visually spectacular display. Cool.
588
00:32:11.150 --> 00:32:14.150
And this is what, you know, this is what stages
589
00:32:14.210 --> 00:32:16.490
are for. If the universe is the biggest stage of
590
00:32:16.529 --> 00:32:20.470
them all, he's brought the universe together. onto into theaters.
591
00:32:20.690 --> 00:32:23.190
So Brian, welcome to town for this. So we left
592
00:32:23.369 --> 00:32:28.339
off with describing wormholes and I have to tell the story. Brian,
593
00:32:28.700 --> 00:32:31.900
I have to tell this, okay? So Brian, you just
594
00:32:32.400 --> 00:32:33.839
stay on the side while I tell this to Chuck.
595
00:32:33.859 --> 00:32:36.640
So Chuck, I'm in London and I'm a guest on
596
00:32:36.680 --> 00:32:40.369
Brian's show. We're talking about space travel and space exploration.
597
00:32:40.890 --> 00:32:44.809
And he's got a whole audience there. They're all UK people, okay?
598
00:32:44.910 --> 00:32:46.690
And they're new to me and I'm a little new
599
00:32:46.710 --> 00:32:49.220
to them, but they know Brian. And they know I'm American.
600
00:32:49.559 -->
00:32:52.160
So I talk about the future of space travel. And
601
00:32:52.220 --> 00:32:55.259
I say, maybe, you know, no, chemical rockets are not
602
00:32:55.279 --> 00:32:57.279
going to work. In order to do this, we need
603
00:32:57.299 --> 00:33:00.200
like warp drives or ideally wormholes. And then we can
604
00:33:00.220 --> 00:33:02.890
do this. And Brian kicks in and said, wormholes are
605
00:33:02.930 --> 00:33:06.569
unstable and they'll collapse and you can't do this. He's correct,
606
00:33:07.049 --> 00:33:09.509
but that's not the point. The point was the audience,
607
00:33:09.529 --> 00:33:11.430
do you remember what the audience said? The audience said,
608
00:33:12.619 --> 00:33:18.880
That's why the Americans discover everything. They're so optimistic about everything.
609
00:33:19.099 --> 00:33:21.660
That's why they went to the moon and we're stuck
610
00:33:21.700 --> 00:33:25.720
here in London. And so you lost your audience on
611
00:33:25.849 --> 00:33:29.369
that comment, Brian. And I had them from that one.
612
00:33:29.410 --> 00:33:33.509
Because they liked my American... Some of it's just me,
613
00:33:33.569 --> 00:33:37.309
but then I realized a lot of it's just American enthusiasm.
614
00:33:37.650 --> 00:33:40.089
So Brian, how do you use wormholes to actually travel
615
00:33:40.130 --> 00:33:41.210
backwards in time? Is that possible?
616
00:33:41.730 --> 00:33:46.910
Well, so... Yeah, if they were stable, or you could
617
00:33:46.950 --> 00:33:49.450
stabilize them in some way, then you could use them
618
00:33:49.490 --> 00:33:58.230
as time machines. And that's considered to be unlikely. But
619
00:33:58.750 --> 00:34:01.309
it really is true to say that we, well, it's
620
00:34:01.369 --> 00:34:03.029
very true to say we don't have what's called a
621
00:34:03.049 --> 00:34:07.490
quantum theory of gravity. So we don't really, in any sense,
622
00:34:07.569 --> 00:34:12.489
understand the deep merger of between relativity and quantum mechanics
623
00:34:12.530 --> 00:34:15.690
which you need to understand to answer that question and
624
00:34:15.710 --> 00:34:18.329
many physicists point out that we don't you know it
625
00:34:18.449 --> 00:34:20.989
feels like it's no way to build the universe we've
626
00:34:21.010 --> 00:34:22.670
all seen back to the future we all know the
627
00:34:22.710 --> 00:34:25.030
paradoxes that happen if you if time travel is a
628
00:34:25.050 --> 00:34:28.610
reality so so i think if you pushed most physicists
629
00:34:28.650 --> 00:34:30.789
and said don't be formal about it and don't say
630
00:34:30.809 --> 00:34:32.650
what i just said which is we don't understand quantum
631
00:34:32.670 --> 00:34:36.750
gravity yet um then most physicists would say okay we
632
00:34:36.849 --> 00:34:39.980
think the laws of nature will be such that There
633
00:34:40.059 --> 00:34:45.260
aren't stable, macroscopic, big wormholes. That's what I think most
634
00:34:45.320 --> 00:34:50.110
physicists would say. But actually, you mentioned interstellar. And Kip
635
00:34:50.150 --> 00:34:52.130
Thorne is one of the world experts on this, does
636
00:34:52.230 --> 00:34:55.329
point out that you can get around this. So you
637
00:34:55.429 --> 00:34:59.909
could have a universe which permitted time travel and was
638
00:34:59.980 --> 00:35:03.320
not full of contradictions if there were no free will
639
00:35:03.760 --> 00:35:08.860
at all. So the whole universe itself is completely consistent
640
00:35:08.880 --> 00:35:11.949
with And the time travel is built into the consistency.
641
00:35:12.070 --> 00:35:15.610
And that's actually what you see in Interstellar. So that
642
00:35:15.730 --> 00:35:18.980
happens in the plot of Interstellar. He can't stop it.
643
00:35:19.030 --> 00:35:21.690
I'm not spoilers, you know, but he can't stop himself
644
00:35:21.789 --> 00:35:24.150
leaving his daughter's room in the past.
645
00:35:24.230 --> 00:35:26.929
And by the way, that's also what happened in the
646
00:35:27.070 --> 00:35:30.769
story Slaughterhouse-Five by Kurt Vonnegut, which is a time travel
647
00:35:30.789 --> 00:35:32.909
story on top of being a World War II story.
648
00:35:33.489 --> 00:35:36.929
And I think Kurt Vonnegut got it right. Correct me
649
00:35:36.949 --> 00:35:39.250
if I'm wrong, Brian. He just described your life is
650
00:35:39.289 --> 00:35:42.090
always there. You're always being born. You're always dying. You're
651
00:35:42.110 --> 00:35:45.650
always in school. You're always in love. And you just
652
00:35:45.730 --> 00:35:48.989
rejoin where you were on that timeline and relive that.
653
00:35:49.340 --> 00:35:53.920
There's a Stephen Hawking's birthday party. No, it's Kip Thorne's
654
00:35:53.960 --> 00:35:57.320
birthday party. There's a proceedings. So Neil, when we go
655
00:35:57.340 --> 00:35:59.760
to scientific conferences, you have a proceedings. It's a big thing.
656
00:36:00.099 --> 00:36:03.320
And there's a proceedings. I think it's Kip's. I think
657
00:36:03.360 --> 00:36:07.780
it's his 60th birthday party. And Stephen Hawking gave a talk,
658
00:36:07.900 --> 00:36:10.579
and it's written up in the proceedings of his birthday
659
00:36:10.639 --> 00:36:14.800
party because he's so eminent. And Stephen said that Kip
660
00:36:14.960 --> 00:36:18.820
has become increasingly interested in time travel through wormholes as
661
00:36:18.900 --> 00:36:23.059
he's got older. That's how he started the paper. That's good.
662
00:36:23.079 --> 00:36:23.739
That's good. That's good.
663
00:36:23.760 --> 00:36:24.429
Chuck, this is how.
664
00:36:33.860 --> 00:36:36.840
Third of three segments. Give me a few, see if
665
00:36:36.860 --> 00:36:38.010
you can slip in a few more questions.
666
00:36:38.030 --> 00:36:42.869
All right, here we go. This is Catherine Cellarini-Moore who says, Dr. Tyson, Dr. Cox,
667
00:36:42.969 --> 00:36:47.269
Lord Nice, hoping that you can hear Dr. Cox
elaborate
668
00:36:47.429 --> 00:36:50.789
on he alluded to in his YouTube video regarding time
669
00:36:50.829 --> 00:36:54.860
and space not being the stuff from which everything else
670
00:36:54.920 --> 00:36:59.500
is derived. Rather, that time and space may be derivative
671
00:36:59.780 --> 00:37:02.940
of something much bigger, much deeper.
672
00:37:02.960 --> 00:37:03.360
Or deeper.
673
00:37:04.280 --> 00:37:09.699
This comes from the study of black holes primarily. And
674
00:37:10.679 --> 00:37:13.800
I would say it looks like space and time emerge
675
00:37:13.860 --> 00:37:18.219
from quantum entanglement. So we mentioned entanglement before. I should
676
00:37:18.260 --> 00:37:19.380
say what it is, by the way. Should I say
677
00:37:19.400 --> 00:37:21.059
what it is? Should I give the one minute introduction
678
00:37:21.099 --> 00:37:21.559
to entanglement?
679
00:37:21.599 --> 00:37:22.519
Sure, sure, sure.
680
00:37:22.780 --> 00:37:26.000
So imagine you have a coin and you can toss
681
00:37:26.079 --> 00:37:28.840
it and it can come up heads and tails. If
682
00:37:28.880 --> 00:37:31.460
it was a quantum coin and there's two of them,
683
00:37:32.050 --> 00:37:34.730
they can be in what we call a state. such
684
00:37:34.789 --> 00:37:37.889
that you could separate these coins out across the Milky
685
00:37:37.929 --> 00:37:41.289
Way to the edges of the universe. And you just
686
00:37:41.329 --> 00:37:43.010
look at one of them and you could toss it
687
00:37:43.090 --> 00:37:45.369
and it would be heads and tails. You can look
688
00:37:45.409 --> 00:37:46.630
at it and it's heads. You look at it again,
689
00:37:46.650 --> 00:37:50.530
it's tails. 50% of the time looks completely normal. But actually,
690
00:37:51.090 --> 00:37:53.849
if you got back together after doing lots of experiments
691
00:37:53.949 --> 00:37:56.960
on this thing, you would find that the coins never
692
00:37:57.039 --> 00:37:59.860
came up heads at the same time or tails at
693
00:37:59.880 --> 00:38:03.159
the same time. They're always heads, tails, plus tails, heads.
694
00:38:03.909 --> 00:38:06.789
Head to tails or tail centric. They're always opposite. So
695
00:38:06.809 --> 00:38:10.469
you can build a quantum state like that. That's called entanglement.
696
00:38:10.969 --> 00:38:15.000
So it's an interesting thing. It's like the information, all
697
00:38:15.039 --> 00:38:18.619
the information contained in this system of two coins is
698
00:38:18.719 --> 00:38:22.800
somehow spread between them and they don't behave as individual entities,
699
00:38:22.900 --> 00:38:26.239
even if you separate them to vast distances. So that's entanglement.
700
00:38:26.469 --> 00:38:29.070
Because they're not just coins, they're also waves. And the
701
00:38:29.130 --> 00:38:32.210
waves know about each other outside of the local place
702
00:38:32.610 --> 00:38:35.369
Were the coins getting flipped? No, it's... If that's the truth,
703
00:38:35.409 --> 00:38:37.190
then I've been saying it wrong all these years.
704
00:38:37.429 --> 00:38:41.530
No, no, they... Really, they are... The best way to
705
00:38:41.570 --> 00:38:46.010
consider it is it's a single system. And the information,
706
00:38:46.090 --> 00:38:48.090
the structure of the system is a property of the
707
00:38:48.110 --> 00:38:48.590
whole thing.
708
00:38:48.809 --> 00:38:49.489
Why is that the wave function?
709
00:38:49.510 --> 00:38:50.530
That's the best way to think about it.
710
00:38:50.530 --> 00:38:51.550
That's got to be the wave function.
711
00:38:51.730 --> 00:38:52.650
Oh, it is the wave, yeah.
712
00:38:52.710 --> 00:38:54.030
Oh, that's what I'm trying to say.
713
00:38:54.429 --> 00:38:57.829
The wave function, you'd write it down. It'd be heads, tails,
714
00:38:57.909 --> 00:39:00.829
plus tails, heads. is an example of a wave function.
715
00:39:01.070 --> 00:39:02.889
And for the geeks there, we can have a one
716
00:39:02.949 --> 00:39:05.230
over root two there in front of each one if
717
00:39:05.250 --> 00:39:05.489
we want.
718
00:39:06.190 --> 00:39:07.429
You've gone too far, Brian.
719
00:39:07.550 --> 00:39:10.429
The key point is it's.
720
00:39:10.449 --> 00:39:12.429
You had me at wave, you lost me at one
721
00:39:12.489 --> 00:39:13.610
over root whatever.
722
00:39:13.869 --> 00:39:14.250
Well, 50%.
723
00:39:14.250 --> 00:39:18.730
So you can have lots of different... Anyway, so that's
724
00:39:18.750 --> 00:39:19.769
an entangled system.
725
00:39:20.929 --> 00:39:24.690
Deep in there is that there's a term that's squared
726
00:39:24.789 --> 00:39:26.349
in the wave function. So he's got to put the
727
00:39:26.389 --> 00:39:28.400
square root of two. so that when you square that,
728
00:39:28.550 --> 00:39:29.389
it becomes a half.
729
00:39:29.750 --> 00:39:31.920
Yeah, if I want 50-50.
730
00:39:32.110 --> 00:39:34.539
That was a missing piece of what he was saying there.
731
00:39:34.780 --> 00:39:40.199
It's the amplitude, right? So that's entanglement. It's a fundamentally
732
00:39:40.300 --> 00:39:43.119
quantum mechanical thing, and it's very well understood, and we
733
00:39:43.199 --> 00:39:46.159
use it in technology and quantum cryptography and so on.
734
00:39:46.199 --> 00:39:48.360
So it's a thing. This is how the universe works.
735
00:39:49.179 --> 00:39:52.579
And it does seem as if, as I mentioned before,
736
00:39:52.639 --> 00:39:55.440
the idea that you can also interpret that as having
737
00:39:55.559 --> 00:39:58.070
wormholes connecting these things together.
738
00:39:58.150 --> 00:39:58.449
I love it.
739
00:39:58.730 --> 00:40:03.730
Essentially what you're seeing is that entanglement and space are
740
00:40:03.869 --> 00:40:07.929
intimately related. That's the modern way of looking at this,
741
00:40:07.969 --> 00:40:11.789
the very modern way. And I think it's fair to
742
00:40:11.849 --> 00:40:14.099
say that most physicists would say
that the entanglement is
743
00:40:14.119 --> 00:40:17.940
the fundamental thing. And so we're beginning to think now
744
00:40:18.670 --> 00:40:21.570
that you have a theory of quantum mechanics, quantum field
745
00:40:21.610 --> 00:40:25.980
theories on some surface or something, and then the entanglement
746
00:40:26.179 --> 00:40:29.760
actually produces the space. I mean, it's true to say
747
00:40:29.800 --> 00:40:33.099
that entanglement, I've seen it said, which is a beautiful
748
00:40:33.119 --> 00:40:35.539
thing to say, that entanglement is sort of the glue
749
00:40:35.619 --> 00:40:41.489
that keeps space together. And so entanglement is fundamentally related
750
00:40:41.530 --> 00:40:47.320
to space. And therefore, time. but it's more obscure.
751
00:40:47.360 --> 00:40:51.559
So that's the next sci-fi frontier, because the latest Doctor
752
00:40:51.599 --> 00:40:55.840
Strange is madness through the multiverse or something. So they
753
00:40:55.860 --> 00:40:58.829
got the multiverse in there, and he's opening up portals,
754
00:40:58.889 --> 00:41:03.489
which are basically wormholes, as he jiggles his hand. So
755
00:41:03.550 --> 00:41:05.409
now we've got to somehow get down into the very
756
00:41:05.469 --> 00:41:08.090
fabric of the space and time itself. That would be good.
757
00:41:08.429 --> 00:41:08.949
All right.
758
00:41:09.250 --> 00:41:09.389
Cool.
759
00:41:09.840 --> 00:41:11.239
Chuck, we got just a couple, but see if we
760
00:41:11.260 --> 00:41:14.530
can go into like lightning mode. Okay, if we can. Okay, go.
761
00:41:14.750 --> 00:41:22.829
Well, let's lighten things up here with Lindahl Freese, who says, Dr. Tyson, Dr. Cox, Chuck,
762
00:41:22.889 --> 00:41:25.469
here is, is there a parameter edge of the universe?
763
00:41:25.869 --> 00:41:28.179
And where in relation to that edge is the Earth
764
00:41:28.260 --> 00:41:31.099
or the Milky Way located? Are we closer or farther
765
00:41:31.139 --> 00:41:33.639
to the center of the universe? Also, how do we
766
00:41:33.719 --> 00:41:36.480
know the universe is expanding? And is it just that
767
00:41:36.539 --> 00:41:39.480
our instruments are getting stronger?
768
00:41:39.500 --> 00:41:39.579
Sure.
769
00:41:40.480 --> 00:41:42.019
Okay, so we need that in a soundbite.
770
00:41:43.619 --> 00:41:46.429
I can do it. So no, we're not at the
771
00:41:46.469 --> 00:41:47.889
center of the universe. We're at the center of the
772
00:41:47.929 --> 00:41:50.969
observable universe because that's just a piece that we can see.
773
00:41:51.570 --> 00:41:55.150
But the universe extends way beyond that horizon. And so
774
00:41:55.510 --> 00:41:56.750
it could be infinite in extent.
775
00:41:57.489 --> 00:41:57.889
We don't know.
776
00:41:58.809 --> 00:42:00.360
But it's much bigger, I think, than the piece we
777
00:42:00.380 --> 00:42:02.219
can see. So no, we're not at the center of
778
00:42:02.280 --> 00:42:05.179
the universe. It might be an infinite universe. We know
779
00:42:05.219 --> 00:42:07.780
it's expanding just very simply because we look at light
780
00:42:07.800 --> 00:42:12.190
from distant objects and that light is stretched. And the
781
00:42:12.230 --> 00:42:15.320
explanation is that light is a wave, and it's traveling
782
00:42:15.360 --> 00:42:19.500
through expanding space. And so it gets stretched as it journeys.
783
00:42:19.539 --> 00:42:22.280
And the basic observation, all the way back to Hubble,
784
00:42:22.860 --> 00:42:24.400
is that the further away you see.
785
00:42:24.460 --> 00:42:26.199
Hubble, the person. Edwin Hubble.
786
00:42:26.489 --> 00:42:28.909
All the way back to Edwin Hubble. The further away
787
00:42:28.949 --> 00:42:30.750
the thing is, the more the light is stretched when
788
00:42:30.789 --> 00:42:33.150
it reaches us. And that's what you would expect if
789
00:42:33.190 --> 00:42:36.789
space were expanding. Essentially, at a uniform rate, it's actually
790
00:42:36.829 --> 00:42:38.809
changing a bit. It's expanding a bit faster now.
791
00:42:40.780 --> 00:42:44.460
So if we said, I want to go to my horizon. Chuck,
792
00:42:44.500 --> 00:42:45.320
let's leave tomorrow.
793
00:42:45.530 --> 00:42:45.719
Yes.
794
00:42:46.239 --> 00:42:47.449
What would we see?
795
00:42:48.489 --> 00:42:50.829
You'd see the same universe as far as we know.
796
00:42:51.250 --> 00:42:54.989
So you could go to the horizon and look around
797
00:42:55.130 --> 00:42:58.800
and you'd see a completely uniform universe. with the same
798
00:42:58.860 --> 00:43:01.469
kind of distribution of galaxies. So like if it's C,
799
00:43:01.559 --> 00:43:04.320
it's carrying its horizon with it, basically. So yes, that's
800
00:43:04.380 --> 00:43:06.400
a good example. If you go to the horizon on
801
00:43:06.639 --> 00:43:09.039
your boat and go to the horizon 20 miles away,
802
00:43:09.079 --> 00:43:12.030
whatever it is, and then I probably got that number wrong,
803
00:43:12.050 --> 00:43:13.750
and now all the flat Earth people will go, C,
804
00:43:13.789 --> 00:43:14.289
didn't know.
805
00:43:16.170 --> 00:43:19.329
There is a horizon, whatever it is. It's way closer
806
00:43:19.349 --> 00:43:21.809
than 20 miles unless you're in a crow's nest. Okay, right.
807
00:43:23.030 --> 00:43:24.869
So you go to the horizon, and you just see ocean.
808
00:43:25.090 --> 00:43:26.909
And you go to the next horizon, you just see ocean.
809
00:43:27.170 --> 00:43:29.340
And that's what the universe is like as far as
810
00:43:29.380 --> 00:43:29.880
we can tell.
811
00:43:29.889 --> 00:43:30.219
Yeah.
812
00:43:30.679 --> 00:43:32.519
I mean, that's as simple as going to the top
813
00:43:32.559 --> 00:43:35.119
of a hill. You experience that any time? Like you're
814
00:43:35.159 --> 00:43:37.320
driving up a hill or on a bike, you look
815
00:43:37.360 --> 00:43:38.719
at the top of the hill, and it just looks
816
00:43:38.760 --> 00:43:40.699
like that's the
end. You get at the top of
817
00:43:40.719 --> 00:43:42.079
the hill, and it's just more of the same.
818
00:43:42.099 --> 00:43:43.460
It's just more and more and more.
819
00:43:43.559 --> 00:43:44.539
This time you're looking down.
820
00:43:44.579 --> 00:43:45.000
More of the same.
821
00:43:45.079 --> 00:43:45.780
That's cool. Yeah.
822
00:43:46.079 --> 00:43:49.699
All right. Let's go to Alain Bredeau, who says.
823
00:43:49.719 --> 00:43:51.710
This might be the last question we have time for. Okay, go.
824
00:43:52.190 --> 00:43:58.219
Alain says this. Hey, Neil, Chuck, and Professor Cox, we
825
00:43:58.300 --> 00:44:02.519
have electron microscopes to probe smaller stuff than with regular
826
00:44:02.619 --> 00:44:06.159
light microscopes. Do you think somebody is going to come
827
00:44:06.219 --> 00:44:10.250
up with a quark microscope or something of that nature
828
00:44:10.289 --> 00:44:13.550
that will enable us to see even smaller or get
829
00:44:13.650 --> 00:44:20.820
closer microscopes? to those strings that theorists fantasize about.
830
00:44:20.960 --> 00:44:23.420
It's an old trickle.
831
00:44:23.460 --> 00:44:25.380
Let me just set that up just real quick. So
832
00:44:25.739 --> 00:44:30.500
regular microscopes use visible light and visible light has certain wavelengths.
833
00:44:31.409 --> 00:44:33.690
So if you really think about it, a visible light
834
00:44:33.710 --> 00:44:37.550
telescope can't see anything smaller than the wavelength of light
835
00:44:37.590 --> 00:44:40.670
you're using because the light would just wash over it
836
00:44:40.750 --> 00:44:43.070
and wouldn't be able to bring it into focus. So
837
00:44:43.639 --> 00:44:48.320
electron microscopes use basically, I think, Brian, is it X-rays?
838
00:44:48.739 --> 00:44:52.460
Because electrons and X-rays are the same thing at certain,
839
00:44:52.900 --> 00:44:55.110
you can beam electrons to have an energy level of
840
00:44:55.139 --> 00:44:59.030
that of an X-ray, and X-rays have really small wavelengths.
841
00:44:59.710 --> 00:45:02.510
So now you can see detail way smaller than visible light.
842
00:45:02.530 --> 00:45:06.230
So this questioner knows this about electron microscopes and wants
843
00:45:06.250 --> 00:45:07.190
to take it another step.
844
00:45:07.590 --> 00:45:10.349
And there's a really great fundamental point to make here,
845
00:45:10.389 --> 00:45:14.489
which goes to black hole physics, actually, again. So as
846
00:45:16.070 --> 00:45:19.110
you take the wavelength down, quantum mechanics allows you to
847
00:45:19.170 --> 00:45:22.010
think of light as a wave or as a stream
848
00:45:22.030 --> 00:45:25.239
of particles called photons. And as you shrink the wavelength,
849
00:45:25.280 --> 00:45:27.780
the energy of the photon goes up. So that's just
850
00:45:27.880 --> 00:45:30.539
basic quantum mechanics. So the smaller the wavelength, the higher
851
00:45:30.579 --> 00:45:33.340
the energy. So you get to a point where if
852
00:45:33.360 --> 00:45:36.969
you want to probe smaller and smaller distances, what actually
853
00:45:37.010 --> 00:45:40.190
happens is you make a black hole. Because you put
854
00:45:40.250 --> 00:45:42.650
so much energy into the small piece of space that
855
00:45:42.670 --> 00:45:45.050
a black hole forms. And then as you put more
856
00:45:45.110 --> 00:45:48.719
energy in, the black hole grows. And so you end
857
00:45:48.760 --> 00:45:53.360
up reversing that process. Because as the black hole grows,
858
00:45:53.380 --> 00:45:57.440
then you get less and less resolution again. So there's
859
00:45:57.480 --> 00:46:00.329
a limit to how small you can see.
860
00:46:00.349 --> 00:46:03.409
So I'll step in here because Chuck didn't. You kept
861
00:46:03.469 --> 00:46:06.400
talking after you said, yeah, first you make the black
862
00:46:06.460 --> 00:46:09.420
hole and then you continue.
863
00:46:09.480 --> 00:46:11.360
So you put more and more energy in.
864
00:46:11.380 --> 00:46:13.820
I'm saying this sounds dangerous, Brian.
865
00:46:15.119 --> 00:46:16.699
It's an in principle argument.
866
00:46:16.739 --> 00:46:19.260
Oh, it's a thought experiment.
867
00:46:19.280 --> 00:46:20.929
The point is that you get to a point where
868
00:46:20.949 --> 00:46:23.670
if you try to cram more and more energy into
869
00:46:23.710 --> 00:46:26.389
a smaller and smaller amount of space, which you have
870
00:46:26.429 --> 00:46:28.369
to do to see the small thing, you have to
871
00:46:28.409 --> 00:46:30.289
get more energy in, right? The smaller wavelength.
872
00:46:30.429 --> 00:46:32.969
Because you're using photons that are... Higher and higher energy.
873
00:46:33.070 --> 00:46:35.590
Or anything, yes. Or anything, electrons or whatever it is.
874
00:46:36.130 --> 00:46:38.610
Then you form, there comes a point where you form
875
00:46:38.650 --> 00:46:40.369
a black hole in that region.
876
00:46:40.409 --> 00:46:42.750
And then you can't say anything because your microscope got
877
00:46:42.829 --> 00:46:48.469
sucked into it. Because you dayed.
878
00:46:48.530 --> 00:46:53.099
You'll have less resolution. So it's called, now Leonard Susskind
879
00:46:53.119 --> 00:46:53.820
writes about it.
880
00:46:54.000 --> 00:46:58.079
Ignoring the complication that you'd be dead. Ignoring the complication
881
00:46:58.099 --> 00:47:00.250
that you'd be dead and you'd destroy the Earth. You'd
882
00:47:00.269 --> 00:47:01.789
have less resolution on your microscope.
883
00:47:01.809 --> 00:47:04.849
No, you wouldn't because it'd be a tiny, tiny black hole.
884
00:47:04.889 --> 00:47:08.860
So you wouldn't notice it, except you'd stop seeing. So
885
00:47:08.900 --> 00:47:12.679
you can't probe smaller and smaller distances forever. I think
886
00:47:12.719 --> 00:47:17.039
Susskind calls it the UVIR connection, ultraviolet infrared connection. I
887
00:47:17.079 --> 00:47:20.389
think that's what he calls it. But it's a fundamental
888
00:47:20.530 --> 00:47:23.809
property of the universe. So black holes stop you from
889
00:47:24.010 --> 00:47:26.420
doing that. going to smaller and smaller and smaller and
890
00:47:26.440 --> 00:47:27.199
smaller distances.
891
00:47:27.260 --> 00:47:28.079
Pesky black hole.
892
00:47:28.139 --> 00:47:28.440
Yes.
893
00:47:28.639 --> 00:47:32.059
Yeah. And again, it's fundamental. It's, it's, it's pointing to
894
00:47:32.099 --> 00:47:34.670
fundamental physics. So we go all the way back to
895
00:47:34.710 --> 00:47:36.989
this idea of space and time and the link to
896
00:47:37.030 --> 00:47:37.590
quantum theory.
897
00:47:38.510 --> 00:47:40.570
Dude, we got to wrap it up there. Oh my gosh.
898
00:47:40.809 --> 00:47:41.130
Wow.
899
00:47:41.590 --> 00:47:45.889
Cover the universe here. Whoa, Brian, this has been a delight. Uh,
900
00:47:46.369 --> 00:47:48.750
I know you're active on Twitter. Where else are you active?
901
00:47:48.769 --> 00:47:51.920
Cause you're prof Brian Cox on Twitter. Uh, where else
902
00:47:52.000 --> 00:47:52.219
are you?
903
00:47:52.679 --> 00:47:56.260
Yeah, I'm on Facebook as well. Um, But Twitter is
904
00:47:56.300 --> 00:48:01.079
my usual mode of communication. I don't know why. It's
905
00:48:01.360 --> 00:48:02.139
just a habit.
906
00:48:02.380 --> 00:48:04.679
I suppose. Yeah, it's a habit. It's quick and easy
907
00:48:04.949 --> 00:48:09.030
and sharp. And so, Brian, always great to see you
908
00:48:09.130 --> 00:48:12.289
and hear from you. And we'll connect again. Chuck, love you, man.
909
00:48:12.309 --> 00:48:12.829
Love you, too.
910
00:48:12.869 --> 00:48:13.409
Always a pleasure.
911
00:48:13.449 --> 00:48:17.639
All right. Neil deGrasse Tyson here, your personal astrophysicist. As always,
912
00:48:17.659 --> 00:48:18.710
keep looking out.