WEBVTT - Could we reveal quantum gravity in a tabletop experiment?

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<v Speaker 1>Hey, Daniel, who do you think would win in a

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<v Speaker 1>fight theoretical or an experimental physicist?

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<v Speaker 2>That depends are we're talking arm wrestling or like integration

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<v Speaker 2>competitions into what mathematical race?

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<v Speaker 1>Then I think I would put my money into theoretical physicist.

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<v Speaker 1>I mean, no offense.

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<v Speaker 2>Maybe we have to do the experiment, or maybe you.

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<v Speaker 1>Should keep this theoretical. I don't know if you want

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<v Speaker 1>to pick a fight.

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<v Speaker 2>Well, maybe the two sides of the field just compliment

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<v Speaker 2>each other beautifully.

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<v Speaker 1>Is that all it takes us? Some compliments and you

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<v Speaker 1>guys are back as friends.

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<v Speaker 2>Theories are cheap, right, They don't need money for experiments,

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<v Speaker 2>They just need compliments in theory.

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<v Speaker 1>In my experience, hi am Warham, a cartoonist and the

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<v Speaker 1>creator of PhD comics.

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<v Speaker 2>Hi, I'm Daniel. I'm a particle physicist and a professor

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<v Speaker 2>at UC Irvine, And back in the day, I did

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<v Speaker 2>want to be a theorist.

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<v Speaker 1>Back in the day, How old were you.

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<v Speaker 2>When I started grad school? I wasn't sure if I

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<v Speaker 2>wanted to do experimental or theoretical physics, So I guess

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<v Speaker 2>I was in my early twenties, which by now is

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<v Speaker 2>pretty far back in the day.

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<v Speaker 1>Did you actually get a choice, like they offer you

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<v Speaker 1>an option of which way to go, or do you

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<v Speaker 1>have to, like, I don't know, test into it.

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<v Speaker 2>You definitely have to kind of try out and work

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<v Speaker 2>with the theorists if you want to be a theorist.

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<v Speaker 2>But you have all the options when you start grad school.

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<v Speaker 2>You could end up being an experimental particle physicist or

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<v Speaker 2>a theoretical cosmologist or whatever. All those paths are available.

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<v Speaker 2>You just gotta like it enough and be good at it.

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<v Speaker 1>So what happened? Why didn't you pick the theory?

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<v Speaker 2>I discovered I just didn't like writing down equations as

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<v Speaker 2>much as a theorist. They would sit there and like

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<v Speaker 2>develop several different mathematical fonts to write their equations in,

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<v Speaker 2>and I was like, wow, I'm just not loving this

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<v Speaker 2>as much as they're loving this.

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<v Speaker 1>It sounds like you were against the idea of it

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<v Speaker 1>in theory.

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<v Speaker 2>My experience was the experiments were more fun.

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<v Speaker 1>But anyways, Welcome to our podcast Daniel and Jorge Explain

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<v Speaker 1>the Universe, a production of iHeartRadio.

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<v Speaker 2>In which we try to blur the line between theory

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<v Speaker 2>and experiment. We want to talk about all the concepts

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<v Speaker 2>in theoretical physics that try to explain what's going on

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<v Speaker 2>in our world, but we also try to touch back

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<v Speaker 2>on the ground and understand what experiments are telling us

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<v Speaker 2>about the nature of reality, what is Nature actually saying

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<v Speaker 2>to us as she spins the story of the universe,

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<v Speaker 2>And then we try to explain all of it to you.

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<v Speaker 1>That's right, because it is a pretty storied universe, full

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<v Speaker 1>of amazing little details and facts and things to discover

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<v Speaker 1>out there that we are still puzzling over and which

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<v Speaker 1>require all kinds of scientists to figure out, theorists and experimentalists.

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<v Speaker 2>And in the history of physics we have made progress

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<v Speaker 2>in lots of different ways. Sometimes the theorists have come

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<v Speaker 2>up with a clever idea, a suspicion about how the

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<v Speaker 2>universe might work, with lots of cool directions for experimentalists.

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<v Speaker 2>Go out and check this thing, Measure how light bends

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<v Speaker 2>around the sun, see if you can find the Higgs boson.

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<v Speaker 2>Those can be wonderful directions to help unravel the mysteries

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<v Speaker 2>of the universe. But sometimes the experimentalists lead the way,

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<v Speaker 2>turning on particle smashers and discovering gobs and gobs of

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<v Speaker 2>new particles that nobody expected.

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<v Speaker 1>I guess my question, Daniel is why can't you be both?

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<v Speaker 1>Why can't you be a theoretical and an experimental physicist.

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<v Speaker 2>I'm doing my best. Actually i'm doing my best. But

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<v Speaker 2>the reality of academia these days is to get one

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<v Speaker 2>of these jobs, you have to be the world's expert

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<v Speaker 2>in some subfield. And that makes it really hard to

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<v Speaker 2>sort of live between two fields because you have to

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<v Speaker 2>be like the top person in that field that year.

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<v Speaker 2>And so if the theorists aren't sure, if you're a

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<v Speaker 2>theorist and the experimentalist aren't sure if you're an experimentalist,

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<v Speaker 2>nobody's going to give you that job. So you've got

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<v Speaker 2>to sort of get the job in one category and

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<v Speaker 2>then inch your way over to the other one if

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<v Speaker 2>you're interested. That's kind of cliquish, it's definitely very cliquiche. Absolutely,

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<v Speaker 2>these fields form and then they protect themselves and it

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<v Speaker 2>can be hard for new kinds of subfields to emerge,

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<v Speaker 2>Like right now we have the emergence of physicists who

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<v Speaker 2>are experts in machine learning, and people aren't sure is

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<v Speaker 2>that theoretical is it experimental? Because you're running a bunch

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<v Speaker 2>of calculations nobody's really sure. Everybody knows that it's valuable,

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<v Speaker 2>but we aren't quite sure where to put them.

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<v Speaker 1>That's because they're robots? Are they in disguise?

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<v Speaker 2>We're all just biological robots?

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<v Speaker 3>Man?

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<v Speaker 1>Oh, there you go.

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<v Speaker 2>Aren't you the expert in squishy robots?

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<v Speaker 1>I am, Yeah, Well I used to be, at least

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<v Speaker 1>a lifetime ago. We're a couple of lifetimes ago.

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<v Speaker 2>Now back in the day. Is there such a thing

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<v Speaker 2>as a theoretical roboticist?

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<v Speaker 1>Uh? Yeah, there's a lot of theory in robotics as well.

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<v Speaker 1>But no, as we I guess we're not as clique

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<v Speaker 1>as you're just a roboticist. If you're into robots, you're

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<v Speaker 1>just a roboticist.

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<v Speaker 2>New York because you just build your own friends. You're like, hey, look,

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<v Speaker 2>I don't need people's friends. I can build my own.

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<v Speaker 1>Yeah. But as you said, I guess you need both

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<v Speaker 1>kinds of endeavors or search. You need experimental research and

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<v Speaker 1>you need theoretical research in order to figure out how

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<v Speaker 1>things work in the universe. Because I guess you need

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<v Speaker 1>to come up with a theory so that you can

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<v Speaker 1>prove it with an experiment, and you need an experiment

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<v Speaker 1>to prove the theories. Otherwise there's no science.

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<v Speaker 2>That's sort of a theoretical way of thinking about it,

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<v Speaker 2>that we come up with the theories and improve them

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<v Speaker 2>with experiment. Remember that sometimes experiments don't just prove theories.

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<v Speaker 2>They blow up theories and tell us that the universe

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<v Speaker 2>is different from the way we understand it and operates

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<v Speaker 2>in some other way we don't yet understand. Like the

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<v Speaker 2>photoelectric effect was a demonstration that boy, we really don't

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<v Speaker 2>understand at light and how it works, and it took

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<v Speaker 2>a few years before the theorist came up with any sort

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<v Speaker 2>of explanation for it.

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<v Speaker 1>Yeah, but I guess experimenter's lunches kind of experiment blindly, right.

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<v Speaker 1>You usually have some sort of theory at hand when

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<v Speaker 1>you design your experiments, when you go out there and

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<v Speaker 1>turn stuff on.

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<v Speaker 2>It's a bit of a raging debate right now in

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<v Speaker 2>experimental physics whether we should be focused on searching for

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<v Speaker 2>the ideas that theoretical physicists are suggesting, or whether we

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<v Speaker 2>should be developing strategies that are more just exploratory that

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<v Speaker 2>leave us open to surprises. Like when you turn on

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<v Speaker 2>the Hubble Space telescope and look out into space. Sure,

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<v Speaker 2>you want to see the things that you had in

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<v Speaker 2>mind to look at, but you're also open to like

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<v Speaker 2>seeing aliens waving at you, or seeing new kinds of

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<v Speaker 2>stuff you didn't even expect to see.

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<v Speaker 1>But I guess also at the same time, we're getting

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<v Speaker 1>to a spot where you know, things are so complex

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<v Speaker 1>and so subtle and so hidden that you kind of

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<v Speaker 1>need to know what you're looking for in a way, right,

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<v Speaker 1>it's kind of hard to just like look for everything.

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<v Speaker 2>It is really hard to look for everything you really

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<v Speaker 2>put your finger on it, especially when your data is

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<v Speaker 2>very statistical. If you do like a single experiment and

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<v Speaker 2>you get some weird result, you might be able to say, hey, look,

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<v Speaker 2>there's definitely something new here. But if the data are subtle,

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<v Speaker 2>if the new things appear as like trends in your data,

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<v Speaker 2>then you're right, it can be hard to know how

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<v Speaker 2>to find them. So then you have to play some

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<v Speaker 2>clever statistical arguments and say, well, you're the kinds of

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<v Speaker 2>things that we could see, and here are the ways

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<v Speaker 2>that we could search for them. So you have to

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<v Speaker 2>do a little bit more work to define the kinds

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<v Speaker 2>of things you might be able to see. Even if

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<v Speaker 2>you aren't sure which specifically might pop up in your data.

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<v Speaker 1>Well, sometimes there are cases where both the theories and

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<v Speaker 1>the experimental lists are stumped. And that is the case

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<v Speaker 1>where non physics. There's kind of a big hole in

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<v Speaker 1>physics in terms of our knowledge of how things work

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<v Speaker 1>in the universe.

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<v Speaker 2>That's right, at the most fundamental level, we still don't

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<v Speaker 2>really understand the basic rules of physics. We have two

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<v Speaker 2>pillars of modern physics relativity that tells us about space,

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<v Speaker 2>time and gravity, and quantum mechanics that tells us about

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<v Speaker 2>particles and forces, and we just don't know how to

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<v Speaker 2>bring them together. And it's important because it has to

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<v Speaker 2>do with one of the most basic questions in physics,

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<v Speaker 2>which is what is the universe made out of? What

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<v Speaker 2>is the fundamental fabric of reality? After all?

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<v Speaker 1>Yeah? And is it soft and comfortable? Is what I

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<v Speaker 1>want to know.

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<v Speaker 2>It seems to have a little bit of spandex in it.

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<v Speaker 1>Here, you guys, long is a stretchy that can accommodate

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<v Speaker 1>all sizes.

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<v Speaker 2>Because my waste is not the size it was back

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<v Speaker 2>in the day.

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<v Speaker 1>You want the universe to kind of expand with you,

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<v Speaker 1>your mind and your waste. But yeah, there's kind of

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<v Speaker 1>a big hole in our understanding of the universe, and

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<v Speaker 1>it has to do with gravity. We're not quite sure

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<v Speaker 1>where gravity falls, whether it falls or it fits with

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<v Speaker 1>quantum mechanic skill theory, or whether it works the way

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<v Speaker 1>that Einstein envisioned in special relativity.

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<v Speaker 2>Right, that's right. Einstein's special relativity tells us about light

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<v Speaker 2>and how it propagates. His theory of general relativity tells

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<v Speaker 2>us about space time and how it bends. And these

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<v Speaker 2>two theories are in conflict and tell us very different

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<v Speaker 2>stories about the nature of the universe. But so far

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<v Speaker 2>we haven't been able to figure out a way to

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<v Speaker 2>test them without building a solar system sized particle collider

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<v Speaker 2>or peering inside a black hole. So experimental physicists have

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<v Speaker 2>not really been able to contribute to this conversation until now.

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<v Speaker 1>So the deal in the podcast, we'll be asking the question,

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<v Speaker 1>can we test quantum gravity in a tabletop experiment? And

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<v Speaker 1>right here the word tabletop I think of board games.

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<v Speaker 1>Is this what we're talking about? Like a little cardboard

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<v Speaker 1>unfolding thing with pieces, And then you test quantum gravity exactly.

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<v Speaker 2>You can download the schematics from the internet and print

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<v Speaker 2>out your own Nobel Prize winning experiment. Do you go?

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<v Speaker 1>Is it called settlers of quarks or quantum ton.

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<v Speaker 2>I'll leave you to do the branding of it. But

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<v Speaker 2>when we say tabletop experiment in physics, we basically mean

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<v Speaker 2>something not like the large Hadron collider or something that

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<v Speaker 2>doesn't require a ten billion dollar facility staffed by thousands

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<v Speaker 2>of people. We mean the kind of thing a single

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<v Speaker 2>physicist could do in their laboratory, in the basement of

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<v Speaker 2>your nearby university.

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<v Speaker 1>I see you're talking about a million dollar tabletop, not

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<v Speaker 1>a billion dollar tabletop.

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<v Speaker 2>Exactly, just like everybody has a million dollar table in

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<v Speaker 2>their kitchen. No, it's really like a single physicist experiment,

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<v Speaker 2>something you could do in a reasonable physics lab, not

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<v Speaker 2>something people are going to be doing on their kits table.

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<v Speaker 1>Well, as usually, we were wondering how many people out

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<v Speaker 1>there had thought about this question or perhaps have any

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<v Speaker 1>ideas about how to do it.

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<v Speaker 2>So thanks very much to everybody who participates in this

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<v Speaker 2>segment of the podcast. If you've been listening for years

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<v Speaker 2>and would like to hear your voice speculating about the

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<v Speaker 2>topic of the day, please write to us two questions

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<v Speaker 2>at Danielandjorge dot com everybody's welcome.

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<v Speaker 1>So think about it for a second. Do you think

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<v Speaker 1>we can test quantum gravity on somebody's table? Here's what

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<v Speaker 1>people had to say.

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<v Speaker 4>Well, since quantum gravity is, you know, with the gravity

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<v Speaker 4>of the really small, I don't see why the experiments

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<v Speaker 4>with it couldn't be done on a tabletop. I just

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<v Speaker 4>have no idea what those experiments would even begin to

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<v Speaker 4>look like.

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<v Speaker 3>Though.

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<v Speaker 2>If yes, then it will come to our table soon.

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<v Speaker 1>But till then, I don't think it is possible at all.

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<v Speaker 2>Uh, yeah, you probably could, but probably not today.

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<v Speaker 3>I do not feel like we could test quantum gravity

0:10:52.200 --> 0:10:55.360
<v Speaker 3>in a tabletop experiment because you.

0:10:55.760 --> 0:10:59.480
<v Speaker 1>Need a lot of gravity for it to work, and

0:10:59.679 --> 0:11:02.000
<v Speaker 1>I don't think the Earth has that kind of gravity.

0:11:02.080 --> 0:11:05.120
<v Speaker 1>All right, not a lot of optimism, I like the

0:11:05.120 --> 0:11:07.880
<v Speaker 1>person who said the tabletop, I don't think so. But

0:11:08.000 --> 0:11:11.960
<v Speaker 1>maybe a desktop or on the floor, or on a shelf,

0:11:12.400 --> 0:11:16.120
<v Speaker 1>maybe mountain top maybe, yeah, tabletop on a mountain. There

0:11:16.160 --> 0:11:17.880
<v Speaker 1>you go, lower gravity.

0:11:18.080 --> 0:11:20.320
<v Speaker 2>Well, we talked recently about how to measure big g

0:11:20.520 --> 0:11:23.160
<v Speaker 2>and that experiment was definitely done on a mountain side

0:11:23.400 --> 0:11:27.720
<v Speaker 2>swinging pendulums next to a big mountain in Scotland. So yeah,

0:11:27.800 --> 0:11:30.600
<v Speaker 2>you can do funny gravity experiments on tops of mountains.

0:11:30.760 --> 0:11:33.480
<v Speaker 1>And I like the person who said probably, but not today,

0:11:33.840 --> 0:11:36.840
<v Speaker 1>Like is today a bad day for that? Were they

0:11:36.880 --> 0:11:40.360
<v Speaker 1>busy that day? How about next week? Next week work?

0:11:40.480 --> 0:11:42.439
<v Speaker 2>Please fill out this doodle pole for when we will

0:11:42.440 --> 0:11:43.439
<v Speaker 2>win a Nobel prize.

0:11:44.200 --> 0:11:48.000
<v Speaker 1>There you go. Yeah, I guess people didn't feel like

0:11:48.200 --> 0:11:51.240
<v Speaker 1>it could work. But let's find out, Daniel step us

0:11:51.240 --> 0:11:52.960
<v Speaker 1>through this. What is quantum gravity?

0:11:53.040 --> 0:11:55.800
<v Speaker 2>So when we say quantum gravity, what we mean is

0:11:55.840 --> 0:12:00.360
<v Speaker 2>a theory that explains both the quantum mechanical behavior super

0:12:00.440 --> 0:12:04.559
<v Speaker 2>tiny particles, the way like electrons and photons do things

0:12:04.679 --> 0:12:08.439
<v Speaker 2>that baseballs and basketballs and mountaintops don't do. You know,

0:12:08.480 --> 0:12:11.599
<v Speaker 2>they don't move in smooth paths. They have weird quantized

0:12:11.720 --> 0:12:15.160
<v Speaker 2>energy levels. They can be in a superposition of different states,

0:12:15.160 --> 0:12:18.040
<v Speaker 2>like maybe they're here, maybe they're there. They can interact

0:12:18.080 --> 0:12:20.319
<v Speaker 2>with each other and interfere in all sorts of complicated

0:12:20.400 --> 0:12:22.760
<v Speaker 2>ways described by their wave function. And we want a

0:12:22.800 --> 0:12:26.040
<v Speaker 2>theory that explains gravity as we know it. That things

0:12:26.080 --> 0:12:30.040
<v Speaker 2>seem to move in these inertial pass through curved space time,

0:12:30.600 --> 0:12:33.679
<v Speaker 2>and that mass in space tends to bend the path

0:12:34.040 --> 0:12:37.240
<v Speaker 2>which affects the motion of other mass. So we have

0:12:37.320 --> 0:12:40.200
<v Speaker 2>these two very different theories of the universe, and so

0:12:40.360 --> 0:12:43.920
<v Speaker 2>far we can't bring them together. So quantum gravity would

0:12:43.960 --> 0:12:48.120
<v Speaker 2>be a theory that explains both these things somehow harmoniously.

0:12:48.480 --> 0:12:50.440
<v Speaker 2>But it's not a theory that we have today.

0:12:50.640 --> 0:12:52.319
<v Speaker 1>Well, I guess maybe step us through a little bit

0:12:52.320 --> 0:12:54.520
<v Speaker 1>of what we haven't been able to bring these two

0:12:54.559 --> 0:12:56.760
<v Speaker 1>things together as far as I understand it. It's kind

0:12:56.760 --> 0:12:58.959
<v Speaker 1>of due to two things, right, Like, one is that

0:12:59.240 --> 0:13:02.719
<v Speaker 1>we haven't measure the gravitational force at the level of

0:13:03.240 --> 0:13:07.040
<v Speaker 1>quantum particles, right, that's one thing. And also we don't

0:13:07.080 --> 0:13:11.360
<v Speaker 1>know what happens to general relativity when you get down

0:13:11.400 --> 0:13:12.560
<v Speaker 1>to that small level.

0:13:12.320 --> 0:13:14.679
<v Speaker 2>Too exactly, I think you put your finger on it. Really,

0:13:14.720 --> 0:13:17.640
<v Speaker 2>we don't know what the gravity is for little particles.

0:13:17.760 --> 0:13:20.600
<v Speaker 2>The gravity for a baseball or for a moon. We

0:13:20.679 --> 0:13:22.840
<v Speaker 2>think we understand and we've been able to test that.

0:13:22.960 --> 0:13:23.120
<v Speaker 3>Right.

0:13:23.200 --> 0:13:26.760
<v Speaker 2>We see moon's orbiting planets, we see planets orbiting suns.

0:13:26.800 --> 0:13:29.600
<v Speaker 2>We see how gravity works. But that's all really really

0:13:29.640 --> 0:13:32.200
<v Speaker 2>big stuff. What we don't know is what happens when

0:13:32.240 --> 0:13:36.120
<v Speaker 2>you have gravity for particles, because particles are super duper tiny,

0:13:36.440 --> 0:13:39.720
<v Speaker 2>which makes it really complicated. For two reasons. One is

0:13:39.720 --> 0:13:42.600
<v Speaker 2>that they have almost no gravity. Remember that gravity is

0:13:42.640 --> 0:13:45.960
<v Speaker 2>like the weakest force in the universe, and so the

0:13:46.000 --> 0:13:49.520
<v Speaker 2>other forces overwhelm it. You try to do experiments with electrons,

0:13:49.559 --> 0:13:54.000
<v Speaker 2>then their charge is much more powerful than their mass. Right,

0:13:54.000 --> 0:13:57.800
<v Speaker 2>the electromagnetic force is much more powerful than the gravitational

0:13:57.840 --> 0:14:01.040
<v Speaker 2>force on an electron. So it's basically possible to measure

0:14:01.200 --> 0:14:03.160
<v Speaker 2>the gravitational force on an electron.

0:14:03.320 --> 0:14:04.640
<v Speaker 1>Can I ask why that is?

0:14:04.679 --> 0:14:04.880
<v Speaker 3>Though?

0:14:04.960 --> 0:14:09.000
<v Speaker 1>Like, couldn't I shoot an electron from here to London

0:14:09.040 --> 0:14:11.600
<v Speaker 1>and see if it curves with the curvature of the Earth.

0:14:11.840 --> 0:14:14.640
<v Speaker 2>You could try that, absolutely, I think you probably shouldn't

0:14:14.640 --> 0:14:17.200
<v Speaker 2>shoot beams across the surface of the Earth without getting

0:14:17.200 --> 0:14:20.600
<v Speaker 2>signatures from everybody who might live in between. But say

0:14:20.600 --> 0:14:22.680
<v Speaker 2>you did that, the electron would be effected by all

0:14:22.720 --> 0:14:26.400
<v Speaker 2>sorts of charged particles between here and London, right, There'd

0:14:26.400 --> 0:14:28.640
<v Speaker 2>be lots of other effects on the electron which would

0:14:28.720 --> 0:14:31.040
<v Speaker 2>swamp out any gravitational effects.

0:14:31.320 --> 0:14:34.400
<v Speaker 1>But I guess maybe, like from a satellite, I'm thinking,

0:14:34.520 --> 0:14:35.960
<v Speaker 1>you know, I just shoot a whole bunch of them,

0:14:36.120 --> 0:14:39.400
<v Speaker 1>and wouldn't the effects from other things kind of even

0:14:39.440 --> 0:14:42.000
<v Speaker 1>out If you shoot a bunch of them out, Like,

0:14:42.000 --> 0:14:45.000
<v Speaker 1>don't we have like quantum drives or like electron cannons.

0:14:45.320 --> 0:14:47.880
<v Speaker 1>What happens if I just shoot them out there in space?

0:14:48.000 --> 0:14:49.960
<v Speaker 1>Do they keep going straight or do they bend?

0:14:50.320 --> 0:14:52.840
<v Speaker 2>Yeah, you could build an electron gun and put it

0:14:52.880 --> 0:14:55.840
<v Speaker 2>in space and shoot them out, but still it would

0:14:55.880 --> 0:14:58.640
<v Speaker 2>be dominated by the effects of other particles. Remember space

0:14:58.720 --> 0:15:02.200
<v Speaker 2>is not totally empty. There's cosmic microwave background photons there,

0:15:02.280 --> 0:15:04.760
<v Speaker 2>there's other charge particles from the Sun, and all of

0:15:04.760 --> 0:15:07.440
<v Speaker 2>these would dominate the fate of that electron. Really, the

0:15:07.480 --> 0:15:10.840
<v Speaker 2>problem is that the charge is more powerful than the mass.

0:15:11.240 --> 0:15:13.320
<v Speaker 2>We talked about this once, and this is either because

0:15:13.400 --> 0:15:16.560
<v Speaker 2>gravity itself is just weaker than the other forces for

0:15:16.640 --> 0:15:20.000
<v Speaker 2>reasons we don't understand, or because electrons are just packed

0:15:20.000 --> 0:15:22.760
<v Speaker 2>with a lot of charge compared to how much mass

0:15:22.840 --> 0:15:25.280
<v Speaker 2>they have. You can think about it sort of either way.

0:15:25.320 --> 0:15:27.320
<v Speaker 2>But that just means that the effect of gravity is

0:15:27.360 --> 0:15:30.040
<v Speaker 2>tiny compared to the effect of electromagnetism. So to do

0:15:30.080 --> 0:15:33.360
<v Speaker 2>that experiment, you'd need to isolate those particles from any

0:15:33.440 --> 0:15:35.920
<v Speaker 2>sort of effect. And today we'll talk about an experiment

0:15:35.960 --> 0:15:37.480
<v Speaker 2>that's going to try to do that, all.

0:15:37.480 --> 0:15:40.200
<v Speaker 1>Right, So then that's where quantum gravity comes in. It's

0:15:40.360 --> 0:15:42.240
<v Speaker 1>kind of a is it a theory or an idea

0:15:42.320 --> 0:15:44.680
<v Speaker 1>that tries to bring these two big ideas together.

0:15:44.880 --> 0:15:47.600
<v Speaker 2>It's not a theory. It's like a category of theories.

0:15:47.640 --> 0:15:50.760
<v Speaker 2>It's like a dreamt of theory. What we want is

0:15:50.760 --> 0:15:52.920
<v Speaker 2>a theory that bring these two things together. We don't

0:15:52.920 --> 0:15:55.480
<v Speaker 2>have one. We don't know what the theory of quantum

0:15:55.560 --> 0:15:58.520
<v Speaker 2>gravity is. You know, sometimes you have like ten different

0:15:58.600 --> 0:16:00.880
<v Speaker 2>theories that describe the universe. The experiment has to go

0:16:00.880 --> 0:16:03.200
<v Speaker 2>off and tell you which one is correct. Right now,

0:16:03.240 --> 0:16:06.200
<v Speaker 2>we have zero. We have zero theories that explain quantum

0:16:06.200 --> 0:16:09.680
<v Speaker 2>mechanics and gravity at the same time. So we sort

0:16:09.720 --> 0:16:12.520
<v Speaker 2>of need an experimental result to be like, hey, this

0:16:12.680 --> 0:16:15.240
<v Speaker 2>is the right direction though where hey, here's something to

0:16:15.280 --> 0:16:17.680
<v Speaker 2>grab on to, here's a clue. But there's the second

0:16:17.720 --> 0:16:20.400
<v Speaker 2>reason why these experiments are difficult that we didn't get

0:16:20.440 --> 0:16:22.520
<v Speaker 2>to yet. One is just that gravity is so weak,

0:16:22.720 --> 0:16:25.880
<v Speaker 2>and the other is that these particles do things that

0:16:25.920 --> 0:16:28.520
<v Speaker 2>we don't know how to explain with gravity, Like particles

0:16:28.920 --> 0:16:32.000
<v Speaker 2>don't have smooth paths. It's not like the electron is

0:16:32.160 --> 0:16:35.600
<v Speaker 2>always somewhere, has some velocity. You know, you want to

0:16:35.640 --> 0:16:38.520
<v Speaker 2>calculate the gravity of an electron, you have to know

0:16:38.680 --> 0:16:41.000
<v Speaker 2>where it is, so you know how far away it is,

0:16:41.120 --> 0:16:44.200
<v Speaker 2>you can calculate it's gravity. But electrons don't have specific

0:16:44.240 --> 0:16:47.760
<v Speaker 2>locations that have probabilities, so we don't know. For example,

0:16:47.880 --> 0:16:50.080
<v Speaker 2>if an electron, when it has probabilities to be in

0:16:50.160 --> 0:16:53.080
<v Speaker 2>multiple places, does it mean it has like multiple different

0:16:53.280 --> 0:16:57.080
<v Speaker 2>possible gravities. We just don't know how to do gravity

0:16:57.120 --> 0:16:59.640
<v Speaker 2>for things that have uncertainties in their locations.

0:17:00.120 --> 0:17:02.160
<v Speaker 1>You mean, we don't know how to do that if

0:17:02.200 --> 0:17:06.960
<v Speaker 1>gravity was not a quantum force, right, Like you're sort

0:17:06.960 --> 0:17:10.280
<v Speaker 1>of assuming that. I guess you want gravity to be

0:17:10.560 --> 0:17:12.679
<v Speaker 1>like a quantum force like the other forces that we

0:17:12.720 --> 0:17:14.120
<v Speaker 1>know about, right.

0:17:13.960 --> 0:17:15.719
<v Speaker 2>Yeah, that's sort of one of the basic questions when

0:17:15.760 --> 0:17:17.679
<v Speaker 2>you want to build the theory of quantum gravity, like

0:17:17.800 --> 0:17:21.000
<v Speaker 2>is it a quantum force? If so, then two electrons

0:17:21.040 --> 0:17:25.480
<v Speaker 2>interacting gravitationally wouldn't like collapse each other's wave functions. Some

0:17:25.600 --> 0:17:27.720
<v Speaker 2>bits of one wave function would interact with some bits

0:17:27.760 --> 0:17:29.480
<v Speaker 2>of another wave function, and they could do all sorts

0:17:29.520 --> 0:17:32.399
<v Speaker 2>of weird quantum interactions. But if gravity is actually a

0:17:32.440 --> 0:17:35.480
<v Speaker 2>classical force and not a quantum force, then it would

0:17:35.520 --> 0:17:38.360
<v Speaker 2>collapse the wave function sort of like when you use

0:17:38.400 --> 0:17:41.240
<v Speaker 2>a detector in a double slit experiment, it forces the

0:17:41.280 --> 0:17:44.040
<v Speaker 2>particle to pick one of the options instead of the

0:17:44.080 --> 0:17:47.200
<v Speaker 2>other one. So we just don't know, like is gravity classical,

0:17:47.359 --> 0:17:49.920
<v Speaker 2>is it quantum mechanical. We just don't even know where

0:17:49.960 --> 0:17:50.359
<v Speaker 2>to begin.

0:17:50.760 --> 0:17:53.119
<v Speaker 1>And when you say classical, you mean like basically not

0:17:53.359 --> 0:17:56.920
<v Speaker 1>quantum mechanical, like not fuzzy, not uncertain.

0:17:57.040 --> 0:18:00.600
<v Speaker 2>Yeah, exactly, we mean not quantum is sort of an

0:18:00.640 --> 0:18:03.919
<v Speaker 2>overused word. Some people say classical to me, not relativistic,

0:18:04.000 --> 0:18:07.960
<v Speaker 2>like Newtonian, but today we mean not quantum mechanical. So

0:18:08.160 --> 0:18:11.000
<v Speaker 2>we don't know if gravity, like really is just classical

0:18:11.040 --> 0:18:14.440
<v Speaker 2>the way Einstein described it, thinking about space as smooth

0:18:14.560 --> 0:18:17.199
<v Speaker 2>and continuous and everything having passed, or if it is

0:18:17.240 --> 0:18:19.359
<v Speaker 2>a quantum effect, in which case it could either be

0:18:19.400 --> 0:18:23.760
<v Speaker 2>a force like you suggested, mediated by weird gravitons, or

0:18:23.800 --> 0:18:27.840
<v Speaker 2>maybe like space itself is quantum mechanical and uncertain. If

0:18:27.920 --> 0:18:31.479
<v Speaker 2>gravity is the curvature of space, maybe space itself can

0:18:31.520 --> 0:18:34.040
<v Speaker 2>be like maybe bent here and maybe bent there in

0:18:34.040 --> 0:18:38.440
<v Speaker 2>some weird quantum mechanical way. There's so many possible directions

0:18:38.440 --> 0:18:41.639
<v Speaker 2>for quantum gravity, nobody really knows which one is going

0:18:41.680 --> 0:18:45.000
<v Speaker 2>to build a viable theory that even can do calculations.

0:18:45.160 --> 0:18:47.720
<v Speaker 1>All right, well, let's get a little bit deeper into

0:18:47.760 --> 0:18:50.720
<v Speaker 1>quantum gravity and whether or not we can test it

0:18:51.000 --> 0:18:54.280
<v Speaker 1>and test it for under a billion dollars, because I

0:18:54.280 --> 0:18:57.000
<v Speaker 1>guess the cheaper the better. We'll dig into that, but first,

0:18:57.040 --> 0:19:11.480
<v Speaker 1>let's take a quick break. All right, we're talking about

0:19:11.560 --> 0:19:14.840
<v Speaker 1>quantum gravity and whether or not that is a thing

0:19:15.000 --> 0:19:18.119
<v Speaker 1>at all, whether it will bring together quantum mechanics in

0:19:18.200 --> 0:19:21.360
<v Speaker 1>general relativity to give us one theory of the universe,

0:19:21.480 --> 0:19:24.000
<v Speaker 1>and whether or not we can even design experiments to

0:19:24.160 --> 0:19:25.200
<v Speaker 1>test such a theory.

0:19:25.320 --> 0:19:27.240
<v Speaker 2>I like your threshold of a billion dollars.

0:19:27.840 --> 0:19:31.160
<v Speaker 1>Yeah, well though these days with inflation, maybe that's more

0:19:31.240 --> 0:19:31.879
<v Speaker 1>like ten billion.

0:19:31.920 --> 0:19:32.080
<v Speaker 3>Though.

0:19:33.640 --> 0:19:35.879
<v Speaker 2>You know, if we could spend a billion dollars and

0:19:35.920 --> 0:19:38.840
<v Speaker 2>get the answer to quantum gravity, I'm pretty sure we

0:19:38.840 --> 0:19:40.840
<v Speaker 2>would do it. The truth is, the experiments might cost

0:19:41.080 --> 0:19:43.000
<v Speaker 2>a lot more than one billion dollars.

0:19:43.040 --> 0:19:46.480
<v Speaker 1>All right, well, let's dig into the cost of these experiments.

0:19:46.560 --> 0:19:48.680
<v Speaker 1>How can we test quantum gravity and figure out whether

0:19:48.760 --> 0:19:49.840
<v Speaker 1>or not it's a real thing or not.

0:19:50.000 --> 0:19:51.840
<v Speaker 2>Well, you had sort of the right idea, which is like,

0:19:52.240 --> 0:19:54.560
<v Speaker 2>let's just zoom in on a quantum particle and look

0:19:54.600 --> 0:19:57.400
<v Speaker 2>at its gravity somehow. But remember the scale of things

0:19:57.440 --> 0:20:00.480
<v Speaker 2>we're talking about here, Like these particles are super duper tiny,

0:20:00.800 --> 0:20:03.359
<v Speaker 2>and the effects we're talking about what happened on really

0:20:03.440 --> 0:20:07.520
<v Speaker 2>really short distance scales. Like gravity gets more powerful when

0:20:07.520 --> 0:20:10.480
<v Speaker 2>things get closer together. In order for gravity to be

0:20:10.520 --> 0:20:13.239
<v Speaker 2>powerful enough for us to really test it, you need

0:20:13.280 --> 0:20:16.199
<v Speaker 2>to get things together to like the Plank scale distances

0:20:16.480 --> 0:20:20.000
<v Speaker 2>we're talking about, like ten to the minus thirty five meters.

0:20:20.160 --> 0:20:22.600
<v Speaker 2>So until recently it seemed like, well, the only way

0:20:22.600 --> 0:20:25.480
<v Speaker 2>to test quantum gravity is to have like a microscope

0:20:25.520 --> 0:20:27.560
<v Speaker 2>that can see effects at the scale of ten to

0:20:27.600 --> 0:20:30.920
<v Speaker 2>the minus thirty five meters, which felt almost impossible.

0:20:31.080 --> 0:20:33.320
<v Speaker 1>Now, I guess, pain me a picture here of what

0:20:33.359 --> 0:20:36.159
<v Speaker 1>it is that you would be trying to do. Like,

0:20:36.200 --> 0:20:37.840
<v Speaker 1>for example, what if I just take a bunch of

0:20:37.960 --> 0:20:41.280
<v Speaker 1>hydrogen atoms. Like a hydrogen atom is just an electron

0:20:41.320 --> 0:20:45.320
<v Speaker 1>and a proton, so it's perfectly balanced in terms of charge.

0:20:45.359 --> 0:20:47.000
<v Speaker 1>And I know that if I stick up bundle I'm

0:20:47.000 --> 0:20:50.600
<v Speaker 1>in a container, they'll sort of tend to fall down

0:20:50.640 --> 0:20:52.879
<v Speaker 1>because of gravity, right, They'll sort of accumulate the pressure

0:20:52.920 --> 0:20:55.560
<v Speaker 1>of the hydrogen tank will be higher at the bottom

0:20:55.600 --> 0:20:58.359
<v Speaker 1>than at the top. That means gravity is working on

0:20:58.400 --> 0:21:00.560
<v Speaker 1>them and it is pulling them down. Can I build

0:21:00.600 --> 0:21:03.119
<v Speaker 1>some sort of model or theory that kind of models

0:21:03.240 --> 0:21:05.720
<v Speaker 1>or tells me how it's working at the quantum level.

0:21:05.880 --> 0:21:09.399
<v Speaker 2>Well, there's the theoretical difficulty, and then there's the experimental difficulty.

0:21:09.800 --> 0:21:13.000
<v Speaker 2>On the theoretical side. Like we've tried to build those theories,

0:21:13.040 --> 0:21:16.159
<v Speaker 2>they just don't work. Gravity is complicated because everything is

0:21:16.200 --> 0:21:19.439
<v Speaker 2>affected by it. It's not like electromagnetism where you can

0:21:19.480 --> 0:21:24.680
<v Speaker 2>like shoot out photons and those photons themselves don't feel electromagnetism, right,

0:21:24.680 --> 0:21:28.920
<v Speaker 2>Photons don't interact with other photons. Gravity interacts with everything

0:21:28.960 --> 0:21:31.440
<v Speaker 2>with energy. So when you try to build a quantum

0:21:31.480 --> 0:21:35.440
<v Speaker 2>theory of gravity, like including the exchange of gravitons, those

0:21:35.480 --> 0:21:39.159
<v Speaker 2>gravitons amid other gravitons which feel those gravitons, and it

0:21:39.200 --> 0:21:41.919
<v Speaker 2>gets very hairy, very quickly. We talked once about the

0:21:42.200 --> 0:21:45.240
<v Speaker 2>strong nuclear force, which has a similar property that it's

0:21:45.359 --> 0:21:49.160
<v Speaker 2>gluons amid other gluons which affect other gluons, and it's

0:21:49.280 --> 0:21:52.720
<v Speaker 2>a nightmare to do any calculations. Gravity is even more

0:21:52.760 --> 0:21:55.439
<v Speaker 2>complex than that, and that's sort of one of the

0:21:55.480 --> 0:21:58.200
<v Speaker 2>reasons why it's been so difficult to build a theory.

0:21:58.280 --> 0:22:00.520
<v Speaker 2>So anytime people build a theory of quantum gravity, it

0:22:00.600 --> 0:22:04.200
<v Speaker 2>just sort of predicts nonsense. We just can't mathematically make

0:22:04.280 --> 0:22:07.159
<v Speaker 2>it work. And then there's the experimental challenge. And what

0:22:07.200 --> 0:22:09.119
<v Speaker 2>you're talking about is like trying to build a setup

0:22:09.160 --> 0:22:12.600
<v Speaker 2>where you can see the gravitational effects on particles. But

0:22:12.720 --> 0:22:15.240
<v Speaker 2>the experiment that you describe like a bunch of hydrogen,

0:22:15.440 --> 0:22:17.560
<v Speaker 2>you know, those are classical effects. The fact that those

0:22:17.640 --> 0:22:20.680
<v Speaker 2>hydrogen atoms are quantum particles is irrelevant to the fact

0:22:20.720 --> 0:22:22.359
<v Speaker 2>that they have more pressure on the bottom of the

0:22:22.400 --> 0:22:24.160
<v Speaker 2>tank than the top of the tank. Oh, I see.

0:22:24.200 --> 0:22:27.199
<v Speaker 1>You're trying to kind of like see what happens to

0:22:27.240 --> 0:22:31.919
<v Speaker 1>gravity at the quantum distance level. Right, that's kind of

0:22:31.920 --> 0:22:34.760
<v Speaker 1>the problem, right, Like you might be able to design

0:22:34.960 --> 0:22:37.600
<v Speaker 1>a hydrogen gun something that shoots hydrogen atoms and you

0:22:37.640 --> 0:22:40.639
<v Speaker 1>can track how the gravity affects its path, maybe, but

0:22:40.880 --> 0:22:43.560
<v Speaker 1>that doesn't necessarily tell you whether or not there's like

0:22:43.640 --> 0:22:48.560
<v Speaker 1>uncertainty or whether the there's fuzziness at the you know,

0:22:48.920 --> 0:22:49.880
<v Speaker 1>really small distance.

0:22:50.160 --> 0:22:51.800
<v Speaker 2>Exactly in the same way that like every time you

0:22:51.880 --> 0:22:55.399
<v Speaker 2>toss a baseball, and principle you're tossing quantum objects right

0:22:55.400 --> 0:22:57.439
<v Speaker 2>at a baseball. That just a bunch of quantum objects, and

0:22:57.480 --> 0:23:01.159
<v Speaker 2>definitely they're feeling gravity. We're not asking like, do electrons

0:23:01.160 --> 0:23:03.640
<v Speaker 2>and protons feel gravity? We're pretty sure they do. We're

0:23:03.640 --> 0:23:07.280
<v Speaker 2>asking is how does their quantum mechanicalness interact with their

0:23:07.320 --> 0:23:11.400
<v Speaker 2>gravitational attraction, you know, when they're doing their weird quantum stuff.

0:23:11.600 --> 0:23:14.480
<v Speaker 2>How does gravity play a role with that? You know,

0:23:14.520 --> 0:23:16.520
<v Speaker 2>if you have a particle that like has a possibility

0:23:16.560 --> 0:23:19.960
<v Speaker 2>to be here and they're simultaneously, what is its gravity?

0:23:20.280 --> 0:23:21.879
<v Speaker 2>So you've got to get something to be showing as

0:23:21.960 --> 0:23:25.600
<v Speaker 2>quantum effects, which means really small distances and revealing its

0:23:25.640 --> 0:23:30.240
<v Speaker 2>gravitational interactions, which requires really really large masses, which is

0:23:30.280 --> 0:23:33.400
<v Speaker 2>why some people are excited to see inside black holes,

0:23:33.640 --> 0:23:36.160
<v Speaker 2>because that's where you have like, really really really big

0:23:36.200 --> 0:23:40.640
<v Speaker 2>masses squeeze down to quantum distances, and so what's going

0:23:40.640 --> 0:23:43.160
<v Speaker 2>on inside a black hole would really tell us about

0:23:43.200 --> 0:23:46.560
<v Speaker 2>the nature of quantum gravity and therefore the deepest nature

0:23:46.560 --> 0:23:49.960
<v Speaker 2>of space time itself. Of course, we can't see inside

0:23:50.040 --> 0:23:52.720
<v Speaker 2>black holes, so those secrets are hidden from us.

0:23:53.720 --> 0:23:56.760
<v Speaker 1>Yeah, you might want to let that one go. It

0:23:56.800 --> 0:23:59.359
<v Speaker 1>seems like we're never going to find out what's inside

0:23:59.400 --> 0:24:00.000
<v Speaker 1>of a black hole.

0:24:00.359 --> 0:24:04.000
<v Speaker 2>There's even a theory called cosmic censorship that suggests will

0:24:04.040 --> 0:24:06.120
<v Speaker 2>never be able to answer this because the answers are

0:24:06.160 --> 0:24:09.120
<v Speaker 2>always going to be hidden behind some weird horizon. It's

0:24:09.119 --> 0:24:10.520
<v Speaker 2>sort of a pessimistic approach.

0:24:10.880 --> 0:24:13.720
<v Speaker 1>WHOA, I didn't know there was a ratings board for

0:24:13.760 --> 0:24:14.280
<v Speaker 1>the universe.

0:24:15.280 --> 0:24:17.440
<v Speaker 2>And there are even some theorists that suggests this whole

0:24:17.600 --> 0:24:20.359
<v Speaker 2>enterprise is a waste of time. Like Freeman Dyson, the

0:24:20.359 --> 0:24:22.640
<v Speaker 2>guy who thought of Dyson's fears. He likes to think

0:24:22.640 --> 0:24:26.160
<v Speaker 2>that we live in a dualistic universe, that quantum mechanics

0:24:26.200 --> 0:24:29.040
<v Speaker 2>and gravity just sort of like rule in different regimes

0:24:29.040 --> 0:24:31.560
<v Speaker 2>and they never actually overlap at any place where they

0:24:31.640 --> 0:24:35.399
<v Speaker 2>come into contact is hidden from us by these event horizons.

0:24:35.840 --> 0:24:39.840
<v Speaker 1>Like maybe gravity is classical and it's not quantum. But

0:24:40.160 --> 0:24:42.960
<v Speaker 1>you're saying, or he's saying that at the quantum level,

0:24:43.520 --> 0:24:46.160
<v Speaker 1>there's things that are happening that you will never find out.

0:24:46.320 --> 0:24:49.000
<v Speaker 2>Yeah, exactly that maybe you don't have a single theory

0:24:49.000 --> 0:24:51.639
<v Speaker 2>at the universe. You like two theories and each have

0:24:51.720 --> 0:24:54.680
<v Speaker 2>their own regime and they never overlap anywhere we could

0:24:54.720 --> 0:24:57.159
<v Speaker 2>test them. But a lot of people don't really like

0:24:57.200 --> 0:25:00.119
<v Speaker 2>that theory. I really don't like that theory because I

0:25:00.119 --> 0:25:02.480
<v Speaker 2>want there to be one theory of the universe, one

0:25:02.520 --> 0:25:05.880
<v Speaker 2>thing that explains everything, and I'd love to see these

0:25:05.920 --> 0:25:08.600
<v Speaker 2>two different concepts battle it out. I want to force

0:25:08.640 --> 0:25:10.439
<v Speaker 2>the universe to show us what the answer is.

0:25:10.680 --> 0:25:13.359
<v Speaker 1>But I wonder couldn't they Couldn't he be right though, Like,

0:25:13.359 --> 0:25:16.400
<v Speaker 1>couldn't it just be the gravity, you know, bend space

0:25:16.880 --> 0:25:21.320
<v Speaker 1>and quantum fields and quantum particles exist in that bent space.

0:25:21.520 --> 0:25:24.160
<v Speaker 2>Yeah, he could be right. But if we can come

0:25:24.240 --> 0:25:28.280
<v Speaker 2>up with some experiments that force quantum mechanics and gravity

0:25:28.320 --> 0:25:31.359
<v Speaker 2>to speak at the same moment, to say, like, all right,

0:25:31.720 --> 0:25:34.680
<v Speaker 2>here's what happens when you have a particle that has

0:25:34.720 --> 0:25:37.879
<v Speaker 2>two possibilities and it has some gravity, then we'll know.

0:25:38.000 --> 0:25:41.320
<v Speaker 2>And maybe he's right. Maybe gravity really is classical. And

0:25:41.359 --> 0:25:44.400
<v Speaker 2>what happens when particles interact gravitationally is that their wave

0:25:44.480 --> 0:25:48.400
<v Speaker 2>functions collapse, because that's what happens when classical objects interact

0:25:48.400 --> 0:25:50.800
<v Speaker 2>with quantum objects. But it sure would be nice to know.

0:25:51.160 --> 0:25:54.480
<v Speaker 1>Yeah, gravity is pretty classic. So talk to us a

0:25:54.520 --> 0:25:57.439
<v Speaker 1>little bit about how we've been trying to study this

0:25:57.600 --> 0:25:58.960
<v Speaker 1>or get answers to this question.

0:25:59.240 --> 0:26:02.000
<v Speaker 2>So, other than wishing we could see inside a black hole,

0:26:02.440 --> 0:26:05.920
<v Speaker 2>the other typical tool in our toolkit is a particle collider.

0:26:06.320 --> 0:26:08.960
<v Speaker 2>You build a big particle smasher, you pour a lot

0:26:09.000 --> 0:26:12.320
<v Speaker 2>of energy into one tiny little spot. Then you can

0:26:12.400 --> 0:26:15.840
<v Speaker 2>like break open bonds. You can see how the pieces interact.

0:26:15.960 --> 0:26:18.960
<v Speaker 2>But in order to see gravitational effects, you would need

0:26:19.160 --> 0:26:22.919
<v Speaker 2>so much energy. You'd basically need like the Plank energy.

0:26:23.040 --> 0:26:26.000
<v Speaker 2>It would require building a collider that's like the size

0:26:26.000 --> 0:26:28.480
<v Speaker 2>of the galaxy in order to get enough energy into it.

0:26:28.600 --> 0:26:31.640
<v Speaker 2>Or some calculations suggest if you build a particle collider

0:26:31.640 --> 0:26:33.680
<v Speaker 2>that big, it would collapse into a black hole.

0:26:33.840 --> 0:26:35.600
<v Speaker 1>Wait, why do you need so much energy?

0:26:35.720 --> 0:26:38.920
<v Speaker 2>Because gravity is really really weak, which means it operates

0:26:38.920 --> 0:26:41.919
<v Speaker 2>on really small distance scales. In order to get to

0:26:42.000 --> 0:26:45.200
<v Speaker 2>small distance scales, you need a lot of energy. It's

0:26:45.200 --> 0:26:47.600
<v Speaker 2>sort of like the de Burgly wavelength, right, Like the

0:26:47.640 --> 0:26:51.119
<v Speaker 2>wavelength of a particle is inversely proportional to its momentum,

0:26:51.400 --> 0:26:54.600
<v Speaker 2>and so the more momentum an object has, the smaller

0:26:54.680 --> 0:26:56.680
<v Speaker 2>its wavelength. And you want to see like really really

0:26:56.720 --> 0:27:00.680
<v Speaker 2>short distance effects, you need really really high energy probes.

0:27:01.160 --> 0:27:04.520
<v Speaker 2>So you need like super duper high energy particle collisions

0:27:04.640 --> 0:27:07.760
<v Speaker 2>in order to see things happening at really short distance scales.

0:27:07.960 --> 0:27:10.800
<v Speaker 1>Why because I guess the more energy two particles have

0:27:10.840 --> 0:27:13.119
<v Speaker 1>when they smash into each other somehow, that gives you

0:27:13.160 --> 0:27:15.200
<v Speaker 1>more resolution in space.

0:27:15.560 --> 0:27:19.120
<v Speaker 2>Yeah, exactly, The more momentum the particle has, the smaller

0:27:19.160 --> 0:27:21.560
<v Speaker 2>the wavelength of their wave function. You can think of

0:27:21.560 --> 0:27:24.200
<v Speaker 2>the motion of every particle is described by a little

0:27:24.240 --> 0:27:26.800
<v Speaker 2>wave function that determines what happens to it, the same

0:27:26.840 --> 0:27:28.720
<v Speaker 2>way you can think of like light as a wave, right,

0:27:28.800 --> 0:27:32.440
<v Speaker 2>it's wiggling around, And if you're using light to see things,

0:27:32.560 --> 0:27:34.600
<v Speaker 2>you can only really see things that are the wavelength

0:27:34.640 --> 0:27:38.320
<v Speaker 2>of that light or larger. Anything smaller than that wavelength

0:27:38.359 --> 0:27:40.960
<v Speaker 2>the photon sort of can't interact with it. And so

0:27:41.000 --> 0:27:42.960
<v Speaker 2>you want to see really really small effects, you need

0:27:43.040 --> 0:27:46.720
<v Speaker 2>really really high energy photons or in our case, we

0:27:46.760 --> 0:27:49.440
<v Speaker 2>need really really high energy particle beams to see very

0:27:49.520 --> 0:27:52.000
<v Speaker 2>very short distance interactions.

0:27:51.640 --> 0:27:53.920
<v Speaker 1>Right, Because I guess you need things with mass, right

0:27:53.960 --> 0:27:57.240
<v Speaker 1>to test the quantum gravity or gravity at the quantum level.

0:27:57.280 --> 0:27:59.480
<v Speaker 1>And so that's also true for things with mass, Like

0:27:59.520 --> 0:28:03.920
<v Speaker 1>the faster they're going, the smaller they are, is.

0:28:03.840 --> 0:28:06.520
<v Speaker 2>That what you're saying effectively, the smaller their wavelength. Is.

0:28:06.640 --> 0:28:08.760
<v Speaker 2>Another way to think about it is that you need

0:28:08.880 --> 0:28:12.679
<v Speaker 2>enough energy in those collisions to make gravity stronger, Like

0:28:12.760 --> 0:28:15.760
<v Speaker 2>you want to overcome the electromagnetic force and the strong

0:28:15.800 --> 0:28:19.200
<v Speaker 2>force and make gravity as powerful as those other forces

0:28:19.480 --> 0:28:21.240
<v Speaker 2>so that you can see its effects. You need to

0:28:21.280 --> 0:28:23.560
<v Speaker 2>pour a lot of energy into those collisions, because the

0:28:23.560 --> 0:28:25.639
<v Speaker 2>power of gravity is linked to the mass and to

0:28:25.720 --> 0:28:28.480
<v Speaker 2>the energy of these things. So you pour enough energy

0:28:28.480 --> 0:28:32.320
<v Speaker 2>into one little location, you'll get a very strong gravitational interaction.

0:28:32.760 --> 0:28:34.760
<v Speaker 2>So if we want to see the gravitational effects on

0:28:34.840 --> 0:28:37.200
<v Speaker 2>quantum particles, you need to pour a lot of energy

0:28:37.200 --> 0:28:38.320
<v Speaker 2>into one little spot.

0:28:39.080 --> 0:28:40.720
<v Speaker 1>And is that the only way to do it through

0:28:40.720 --> 0:28:44.000
<v Speaker 1>particle colliders? Isn't there some like I don't know, like

0:28:44.080 --> 0:28:48.600
<v Speaker 1>aim your beams better approach or make smaller wavelength particles.

0:28:48.640 --> 0:28:50.400
<v Speaker 1>I don't know, Like can we do this without making

0:28:50.400 --> 0:28:51.960
<v Speaker 1>a black hole in our solar system?

0:28:52.160 --> 0:28:54.320
<v Speaker 2>The short answer is no. I mean, we do our

0:28:54.360 --> 0:28:57.560
<v Speaker 2>best with particle beam aiming already. But really the limitation

0:28:57.680 --> 0:28:59.720
<v Speaker 2>is the energy of the particles, and we have them

0:28:59.760 --> 0:29:02.800
<v Speaker 2>going as fast as we can, and the wavelength of

0:29:02.840 --> 0:29:06.160
<v Speaker 2>the particle is determined by its energy. So really sort

0:29:06.160 --> 0:29:08.560
<v Speaker 2>of at the limit there. We talked recently about other

0:29:08.600 --> 0:29:12.520
<v Speaker 2>strategies for accelerating particles that might make it smaller, faster, cheaper.

0:29:12.800 --> 0:29:16.240
<v Speaker 2>So there might be a breakthrough in accelerator technology which

0:29:16.240 --> 0:29:18.480
<v Speaker 2>could leap us up like a factor of ten or

0:29:18.520 --> 0:29:21.080
<v Speaker 2>one hundred. But we are like a factor of a

0:29:21.200 --> 0:29:24.640
<v Speaker 2>trillion away from being able to test quantum gravity in

0:29:24.680 --> 0:29:27.480
<v Speaker 2>particle colliders. So really, nowhere in the near future will

0:29:27.480 --> 0:29:29.440
<v Speaker 2>particle colliders be able to answer this question?

0:29:29.720 --> 0:29:32.000
<v Speaker 1>All right, well, I think part of what we're going

0:29:32.040 --> 0:29:34.719
<v Speaker 1>to be talking about here today are experiments that have

0:29:35.280 --> 0:29:37.880
<v Speaker 1>kind of ideas about how to test this without destroying

0:29:37.920 --> 0:29:42.840
<v Speaker 1>the Solar system. And they involve diamonds and lasers and

0:29:42.960 --> 0:29:48.360
<v Speaker 1>space lasers. No tabletop lasers in space. No, no tabletop

0:29:48.440 --> 0:29:51.560
<v Speaker 1>lasers in Pasadena. Oh that take up space in Pasadena.

0:29:52.720 --> 0:29:53.840
<v Speaker 2>A table near you?

0:29:54.160 --> 0:29:56.520
<v Speaker 1>All right, Well, to dig into it, Daniel, What is

0:29:56.520 --> 0:29:57.840
<v Speaker 1>the first of these experiments?

0:29:57.960 --> 0:30:01.280
<v Speaker 2>So the first of the experiments involves diamonds, and the

0:30:01.360 --> 0:30:04.880
<v Speaker 2>goal here essentially is to create a situation where a

0:30:05.000 --> 0:30:08.880
<v Speaker 2>particle has the probability of being in two places at once,

0:30:09.200 --> 0:30:11.719
<v Speaker 2>and then you test its gravity. You see, if it's

0:30:11.800 --> 0:30:14.480
<v Speaker 2>gravity really is sort of like split between its two

0:30:14.520 --> 0:30:18.160
<v Speaker 2>possible locations, or if when you probe it with gravity,

0:30:18.280 --> 0:30:21.840
<v Speaker 2>it somehow collapses into just having one possible location. Because

0:30:21.880 --> 0:30:24.440
<v Speaker 2>remember this, quantum particles can do this weird thing. They

0:30:24.480 --> 0:30:27.280
<v Speaker 2>can be in a superposition like if there's two possibilities

0:30:27.320 --> 0:30:30.440
<v Speaker 2>for an electron, it doesn't have to choose A or B.

0:30:30.880 --> 0:30:35.120
<v Speaker 2>It can maintain both possibilities until something interacts with it classically,

0:30:35.200 --> 0:30:38.120
<v Speaker 2>which forces it to choose. That's the weird thing about

0:30:38.160 --> 0:30:41.080
<v Speaker 2>quantum mechanics and something we don't understand. So this is

0:30:41.160 --> 0:30:43.640
<v Speaker 2>very hard, of course, because particles are very small and

0:30:43.680 --> 0:30:46.040
<v Speaker 2>they're very delicate. But they've come up with a clever

0:30:46.080 --> 0:30:48.960
<v Speaker 2>way that they think might be possible, and it involves

0:30:49.080 --> 0:30:52.000
<v Speaker 2>electrons embedded in falling diamonds.

0:30:52.400 --> 0:30:54.680
<v Speaker 1>Sounds like a rap video where there's like money and

0:30:54.760 --> 0:30:58.200
<v Speaker 1>diamonds falling from the sky. Break it down for us.

0:30:58.280 --> 0:30:59.480
<v Speaker 1>How does his experiment work?

0:31:00.160 --> 0:31:02.800
<v Speaker 2>Is you take a very tiny diamond and has a

0:31:02.920 --> 0:31:06.480
<v Speaker 2>nitrogen added inside of it, like embedded inside the diamond.

0:31:06.600 --> 0:31:09.080
<v Speaker 2>And this has a cool property, which is that if

0:31:09.120 --> 0:31:11.680
<v Speaker 2>you zap it with a laser, the electrons have a

0:31:11.720 --> 0:31:14.520
<v Speaker 2>probability to absorb that photon, which case they flip their

0:31:14.560 --> 0:31:17.239
<v Speaker 2>spin to be up, or to ignore that photon and

0:31:17.240 --> 0:31:19.880
<v Speaker 2>flip their spin to be down. So you shoot a

0:31:19.960 --> 0:31:22.480
<v Speaker 2>laser at this diamond, and now it's in a quantum

0:31:22.560 --> 0:31:26.560
<v Speaker 2>superposition of two possibilities. Maybe the electron inside there on

0:31:26.600 --> 0:31:29.720
<v Speaker 2>the nitrogen is spin up, and maybe it's spin down.

0:31:29.880 --> 0:31:32.480
<v Speaker 2>So you have your particle now in a quantum superposition.

0:31:32.600 --> 0:31:34.080
<v Speaker 2>But what you need is for it to be in

0:31:34.080 --> 0:31:37.640
<v Speaker 2>a quantum superposition of two locations rather than two spins.

0:31:37.800 --> 0:31:40.120
<v Speaker 2>So then you pass it to a little magnetic field.

0:31:40.320 --> 0:31:43.760
<v Speaker 2>The magnetic field will push it left or right based

0:31:43.800 --> 0:31:46.320
<v Speaker 2>on the spin. So you have this falling diamond which

0:31:46.360 --> 0:31:49.000
<v Speaker 2>passes through a magnetic field and it either moves left

0:31:49.120 --> 0:31:51.880
<v Speaker 2>or it moves right. Now if it's in a quantum superposition,

0:31:52.040 --> 0:31:54.680
<v Speaker 2>and then it has both possibilities to move left and

0:31:54.800 --> 0:31:59.520
<v Speaker 2>to move right. So now it's location depends on this quantumness.

0:32:00.000 --> 0:32:03.080
<v Speaker 2>It's the same thing for another diamond nearby. Now you

0:32:03.080 --> 0:32:06.040
<v Speaker 2>have this pair of falling diamonds, each of which has

0:32:06.040 --> 0:32:09.320
<v Speaker 2>the possibility to be in two slightly different locations, and

0:32:09.360 --> 0:32:12.440
<v Speaker 2>you see how they interact. Do the possibilities for one

0:32:12.440 --> 0:32:15.360
<v Speaker 2>diamond interact with the possibilities for the other diamond, or

0:32:15.400 --> 0:32:18.280
<v Speaker 2>do the two diamonds like collapse each other's wave functions.

0:32:18.880 --> 0:32:21.240
<v Speaker 1>I see, So you embed a little nitrogen atom into

0:32:21.240 --> 0:32:25.080
<v Speaker 1>the diamond Ezaly with a laser, and now the nirogen

0:32:25.160 --> 0:32:28.680
<v Speaker 1>atom has quantumn certainty, which kind of extends to the

0:32:28.720 --> 0:32:31.360
<v Speaker 1>whole diamond. Is basically what you're saying, right like if

0:32:31.360 --> 0:32:35.160
<v Speaker 1>I don't know, there's quantum certainty about the electron into nitrogen,

0:32:35.200 --> 0:32:37.720
<v Speaker 1>and that means there's quantum certainty about the whole diamond

0:32:38.040 --> 0:32:40.640
<v Speaker 1>because it could be swinging right or left. And now

0:32:40.800 --> 0:32:43.320
<v Speaker 1>if you put two of them together really close, they

0:32:43.320 --> 0:32:46.000
<v Speaker 1>should interact with gravity. And so now you have the

0:32:46.040 --> 0:32:50.120
<v Speaker 1>system where you have two quantum objects interacting with gravity exactly.

0:32:50.120 --> 0:32:52.440
<v Speaker 2>And they have some really clever mathematical way to tell

0:32:52.480 --> 0:32:55.680
<v Speaker 2>if the two diamonds interacted in a quantum way or

0:32:55.720 --> 0:32:58.640
<v Speaker 2>if the two diamonds interacted in a classical way, Like

0:32:58.680 --> 0:33:01.760
<v Speaker 2>if they interacted in a quanti when you measure the

0:33:01.840 --> 0:33:04.720
<v Speaker 2>spins of those electrons after they fall far enough in

0:33:04.760 --> 0:33:08.040
<v Speaker 2>your experiment, they'll have some cool correlation to them, and

0:33:08.080 --> 0:33:10.600
<v Speaker 2>if they interact it in a classical way, then they'll

0:33:10.600 --> 0:33:13.160
<v Speaker 2>be uncorrelated, like whether they're spin up or down will

0:33:13.200 --> 0:33:15.640
<v Speaker 2>just be random, and so because of the weird rules

0:33:15.640 --> 0:33:18.959
<v Speaker 2>of quantum mechanics, you can tell whether quantum mechanics has

0:33:19.040 --> 0:33:22.080
<v Speaker 2>been at play in the gravitational interaction, Like did gravity

0:33:22.360 --> 0:33:24.600
<v Speaker 2>cancel out the quantum mechanic effects because it's really just

0:33:24.640 --> 0:33:28.640
<v Speaker 2>a classical force, or did it allow the quantum uncertainty

0:33:28.920 --> 0:33:32.080
<v Speaker 2>to be maintained, meaning that gravity would be a quantum

0:33:32.280 --> 0:33:34.720
<v Speaker 2>mechanical effect not a classical effect.

0:33:34.920 --> 0:33:38.600
<v Speaker 1>Well, I guess quantum mechanics aside. Can you measure gravity

0:33:38.640 --> 0:33:41.160
<v Speaker 1>the force of gravity by just dropping two diamonds together

0:33:41.280 --> 0:33:43.680
<v Speaker 1>and seeing if they attract each other? Is that like

0:33:43.760 --> 0:33:44.680
<v Speaker 1>a real thing you can do.

0:33:44.840 --> 0:33:47.200
<v Speaker 2>It's a real thing you can try to do. That's very,

0:33:47.320 --> 0:33:51.640
<v Speaker 2>very difficult because little diamonds have very very gentle gravity,

0:33:51.720 --> 0:33:53.600
<v Speaker 2>and so this is not something we think we can

0:33:53.640 --> 0:33:56.640
<v Speaker 2>do today. There's a group in the UK that thinks

0:33:56.640 --> 0:33:58.120
<v Speaker 2>that they can figure out how to do this, and

0:33:58.120 --> 0:34:01.880
<v Speaker 2>there's lots of complicated steps involved and they're hoping to

0:34:01.920 --> 0:34:04.680
<v Speaker 2>maybe pull this off sometime in the next ten years.

0:34:05.560 --> 0:34:08.560
<v Speaker 2>There's a lot of really complicated moving parts involvement getting

0:34:08.600 --> 0:34:12.000
<v Speaker 2>the nitrogen inside the diamond, flipping its spin with a laser,

0:34:12.040 --> 0:34:15.920
<v Speaker 2>beam getting two pairs of diamonds to fall simultaneously close

0:34:16.040 --> 0:34:18.600
<v Speaker 2>enough each other that maybe they have a gravitational interaction.

0:34:18.760 --> 0:34:20.759
<v Speaker 2>Now you don't actually have to see any sort of

0:34:20.800 --> 0:34:24.120
<v Speaker 2>like gravitational pull. You're not measuring like how far did

0:34:24.120 --> 0:34:27.040
<v Speaker 2>the diamond move because of gravity. You're just bringing them

0:34:27.080 --> 0:34:30.320
<v Speaker 2>close enough together that you think gravity is at play.

0:34:30.360 --> 0:34:32.960
<v Speaker 2>The gravity like wakes up and says, ooh, there's something

0:34:33.000 --> 0:34:35.279
<v Speaker 2>going on here. You don't have to measure the gravity.

0:34:35.560 --> 0:34:37.560
<v Speaker 2>You just have to see if gravity messes up the

0:34:37.640 --> 0:34:39.000
<v Speaker 2>quantum state. I see.

0:34:39.040 --> 0:34:41.120
<v Speaker 1>But to measure the quantum state at the end, wouldn't

0:34:41.120 --> 0:34:44.080
<v Speaker 1>you be doing something like measuring that whether or not

0:34:44.160 --> 0:34:47.480
<v Speaker 1>the two diamonds were attracted to each other gravitationally or not.

0:34:47.840 --> 0:34:49.960
<v Speaker 2>No, all you need to do is measure the spins

0:34:50.000 --> 0:34:53.960
<v Speaker 2>of those electrons embedded inside the nitrogen atoms in the diamonds.

0:34:54.080 --> 0:34:56.399
<v Speaker 2>You don't have to see the gravitational effects directly. It's

0:34:56.440 --> 0:34:58.040
<v Speaker 2>sort of like in the double slit experiment when you

0:34:58.080 --> 0:35:01.000
<v Speaker 2>add a detector and that ruins the interface spearance. We're

0:35:01.040 --> 0:35:03.880
<v Speaker 2>adding gravity to a quantum interaction and seeing if it

0:35:03.960 --> 0:35:05.480
<v Speaker 2>ruins the interference or not.

0:35:05.960 --> 0:35:10.440
<v Speaker 1>M But would that necessarily tell you anything about quantum

0:35:10.520 --> 0:35:12.080
<v Speaker 1>gravity or gravitons.

0:35:12.120 --> 0:35:13.799
<v Speaker 2>It wouldn't tell you that much, but it would be

0:35:13.800 --> 0:35:16.520
<v Speaker 2>a powerful clue. It would tell you if gravity is

0:35:16.600 --> 0:35:20.919
<v Speaker 2>classical or quantum mechanical. Like, if gravity is classical, it'll

0:35:20.960 --> 0:35:23.560
<v Speaker 2>act like a detector and it'll collapse those wave functions

0:35:23.600 --> 0:35:27.279
<v Speaker 2>and destroy this interference. If gravity is quantum mechanical, it won't,

0:35:27.320 --> 0:35:30.120
<v Speaker 2>and everything quantum mechanical will stay quantum mechanical, and you

0:35:30.120 --> 0:35:32.800
<v Speaker 2>get all sorts of weird interference. So that just tells

0:35:32.800 --> 0:35:35.720
<v Speaker 2>you if gravity is classical or quantum mechanical. It doesn't

0:35:35.719 --> 0:35:38.200
<v Speaker 2>tell you like, oh, space is quantized, or oh there

0:35:38.239 --> 0:35:41.320
<v Speaker 2>are gravitons. It doesn't tell you which theory of quantum gravity,

0:35:41.600 --> 0:35:43.800
<v Speaker 2>but it is a powerful clue. It would mean, for example,

0:35:43.840 --> 0:35:46.680
<v Speaker 2>if we know gravity is quantum mechanical, the Freeman Dyson

0:35:46.840 --> 0:35:50.479
<v Speaker 2>is wrong about classical gravity and quantum mechanics being able

0:35:50.480 --> 0:35:51.160
<v Speaker 2>to play together.

0:35:52.640 --> 0:35:54.400
<v Speaker 1>Yeah, he could be wrong, in which case he might

0:35:54.440 --> 0:35:58.879
<v Speaker 1>need to stick to them making vacuum tees. All right, Well,

0:35:59.480 --> 0:36:02.279
<v Speaker 1>that's one experiment, and I guess it's in progress. I

0:36:02.280 --> 0:36:04.600
<v Speaker 1>guess they're designing it or making it. Where are they

0:36:04.680 --> 0:36:04.880
<v Speaker 1>with that?

0:36:05.160 --> 0:36:08.239
<v Speaker 2>This physicist at University College London who's leading a team

0:36:08.280 --> 0:36:10.960
<v Speaker 2>of researchers who are trying to make this work. And

0:36:11.080 --> 0:36:13.799
<v Speaker 2>there's folks in Santa Barbara as well, and they're trying

0:36:13.800 --> 0:36:15.080
<v Speaker 2>to work on this. But you know, there's a lot

0:36:15.160 --> 0:36:18.120
<v Speaker 2>of complicated steps and making this thing do its stance

0:36:18.160 --> 0:36:20.360
<v Speaker 2>and being sure you know, what they're doing is a

0:36:20.400 --> 0:36:24.200
<v Speaker 2>lot of pieces involved, lots of complicated experimental cleverness really

0:36:24.200 --> 0:36:26.880
<v Speaker 2>required just to be able to do this test. So

0:36:26.920 --> 0:36:28.960
<v Speaker 2>they're hoping sometime in the next ten years to be

0:36:29.000 --> 0:36:29.879
<v Speaker 2>able to pull this off.

0:36:30.000 --> 0:36:31.919
<v Speaker 1>All right, Well, let's get to the second of these

0:36:31.960 --> 0:36:35.400
<v Speaker 1>potential experiments to measure quantum gravity. We'll dig into that,

0:36:35.480 --> 0:36:50.520
<v Speaker 1>but first let's take another quick break. All right, we're

0:36:50.560 --> 0:36:54.239
<v Speaker 1>talking about quantum gravity and whether or not it's a thing,

0:36:54.480 --> 0:36:59.400
<v Speaker 1>whether gravity is quantum mechanical or is it pretty and

0:36:59.480 --> 0:37:03.920
<v Speaker 1>classical and doesn't care about quantum mechanics and this weirdness

0:37:04.440 --> 0:37:07.040
<v Speaker 1>of things being uncertain, And so we talked about one

0:37:07.080 --> 0:37:10.640
<v Speaker 1>possible experiment that it might look at that using falling diamonds.

0:37:10.800 --> 0:37:15.320
<v Speaker 1>And there's another interesting potential experiments happening also, right.

0:37:15.280 --> 0:37:17.800
<v Speaker 2>That's right, And this one is being developed and built

0:37:17.880 --> 0:37:18.480
<v Speaker 2>in your.

0:37:18.360 --> 0:37:20.600
<v Speaker 1>Backyard, like literally my backyard.

0:37:21.239 --> 0:37:22.040
<v Speaker 2>Look at your window.

0:37:22.080 --> 0:37:22.279
<v Speaker 3>Man.

0:37:22.400 --> 0:37:23.840
<v Speaker 2>You ever wonder what those people are told you?

0:37:23.920 --> 0:37:24.160
<v Speaker 1>What?

0:37:25.480 --> 0:37:27.840
<v Speaker 2>No, it's at cal Tech. Both the theorists and the

0:37:27.880 --> 0:37:31.760
<v Speaker 2>experimental list are at Caltech, and it's a really cool idea.

0:37:31.960 --> 0:37:34.840
<v Speaker 2>And what they're trying to do in this experiment's completely

0:37:34.840 --> 0:37:37.319
<v Speaker 2>different from the other one is try to see if

0:37:37.440 --> 0:37:41.319
<v Speaker 2>space itself is quantum mechanical. Like, if gravity is quant

0:37:41.400 --> 0:37:44.920
<v Speaker 2>mechanical and there are gravitons, then that would mean that

0:37:45.040 --> 0:37:48.040
<v Speaker 2>graviton should be like popping out of the vacuum all

0:37:48.080 --> 0:37:50.879
<v Speaker 2>the time, the same way that other quantum particles are.

0:37:51.160 --> 0:37:53.200
<v Speaker 2>Like if you go out in the middle of empty space,

0:37:53.239 --> 0:37:56.120
<v Speaker 2>there's nothing there, there's still always a little bit of

0:37:56.280 --> 0:37:59.200
<v Speaker 2>energy in the quantum fields, which means that like those

0:37:59.200 --> 0:38:02.080
<v Speaker 2>fields can turn into particles briefly and then back into

0:38:02.160 --> 0:38:06.160
<v Speaker 2>potential energy. So if space itself is quantum mechanical, if

0:38:06.200 --> 0:38:10.280
<v Speaker 2>gravity is quantum mechanical, then gravitons should also be popping

0:38:10.320 --> 0:38:13.160
<v Speaker 2>out of the vacuum. There should be like effectively tiny

0:38:13.360 --> 0:38:18.560
<v Speaker 2>little ripples in space making quantum size gravitational waves.

0:38:19.239 --> 0:38:21.719
<v Speaker 1>WHOA wait, I think you just confused me a little bit.

0:38:21.800 --> 0:38:24.000
<v Speaker 1>So I thought there were two possibilities. Either gravity is

0:38:24.080 --> 0:38:28.040
<v Speaker 1>quantum mechanical or space is quantized. Which one are you

0:38:28.120 --> 0:38:28.799
<v Speaker 1>talking about here?

0:38:28.840 --> 0:38:31.680
<v Speaker 2>Here, we're talking about gravity being quantum mechanical, that there

0:38:31.719 --> 0:38:35.520
<v Speaker 2>exist gravitons which mediate the force of gravity, which in

0:38:35.560 --> 0:38:38.359
<v Speaker 2>this theory would be a quantum force like the other

0:38:38.440 --> 0:38:39.640
<v Speaker 2>forces in the universe.

0:38:39.920 --> 0:38:43.120
<v Speaker 1>Okay, so we're not talking about quantizing space itself.

0:38:42.880 --> 0:38:45.360
<v Speaker 2>That's right. We're not talking about quantizing space and like

0:38:45.400 --> 0:38:48.360
<v Speaker 2>a space foam. But we're talking about space being filled

0:38:48.400 --> 0:38:51.440
<v Speaker 2>with a quantum force of gravity, which would have fluctuations

0:38:51.480 --> 0:38:54.960
<v Speaker 2>in it, right, And those fluctuations would be like quantum

0:38:54.960 --> 0:38:59.240
<v Speaker 2>gravitons popping in and out of the quantum gravitational field.

0:39:00.360 --> 0:39:02.560
<v Speaker 1>I see. So anything that is quantum or has a

0:39:02.640 --> 0:39:05.879
<v Speaker 1>quantum field, by its nature, by its kind of statistical

0:39:05.960 --> 0:39:09.840
<v Speaker 1>random nature, has these particles popping out of nothingness. But

0:39:09.880 --> 0:39:11.920
<v Speaker 1>doesn't it need some sort of like energy to it.

0:39:11.920 --> 0:39:14.680
<v Speaker 2>It does, But quantum fields always have energy to them.

0:39:14.680 --> 0:39:18.320
<v Speaker 2>They can never relax down to zero because the uncertainty principle,

0:39:18.560 --> 0:39:21.160
<v Speaker 2>the minimum energy level of a quantum field is always

0:39:21.200 --> 0:39:24.080
<v Speaker 2>above zero energy, which is why there's always energy in

0:39:24.160 --> 0:39:26.680
<v Speaker 2>quantum fields, which is why there's energy in all of

0:39:26.719 --> 0:39:28.520
<v Speaker 2>space because of its quantum nature.

0:39:28.640 --> 0:39:30.840
<v Speaker 1>Well, that's kind of an odd idea, Like what happens

0:39:30.880 --> 0:39:33.480
<v Speaker 1>if a graviton appears out of nothingness, well.

0:39:33.280 --> 0:39:36.360
<v Speaker 2>Mostly almost nothing, because gravitons would be super duper tiny,

0:39:36.520 --> 0:39:39.319
<v Speaker 2>gravity is super duper weak, and so it would be

0:39:39.480 --> 0:39:42.239
<v Speaker 2>basically impossible to see these things what have effects on

0:39:42.320 --> 0:39:45.600
<v Speaker 2>super tiny distance scales we typically can't probe. But a

0:39:45.680 --> 0:39:49.240
<v Speaker 2>theorist that Caltech, Catherine Zurich, came up with this idea

0:39:49.280 --> 0:39:52.799
<v Speaker 2>that maybe gravitons can all work together. Instead of just

0:39:52.840 --> 0:39:55.640
<v Speaker 2>looking for one graviton, maybe you can look for like

0:39:55.800 --> 0:39:58.640
<v Speaker 2>larger effects of graviton sort of working together to make

0:39:58.719 --> 0:40:03.040
<v Speaker 2>something else emerge from this quantum craziness. And she designed

0:40:03.080 --> 0:40:04.600
<v Speaker 2>an experiment to maybe see that.

0:40:05.160 --> 0:40:09.640
<v Speaker 1>Hmmm, interesting, Well, we actually have an interview of Daniel

0:40:09.760 --> 0:40:13.080
<v Speaker 1>talking with professor Catherine Zurich from cal Tech about her

0:40:13.160 --> 0:40:14.560
<v Speaker 1>idea for this experiment.

0:40:14.640 --> 0:40:16.319
<v Speaker 2>That's right. Kathy and I have known each other since

0:40:16.360 --> 0:40:18.120
<v Speaker 2>we were POSTOCX, and so I called her up and

0:40:18.160 --> 0:40:21.000
<v Speaker 2>asked her about her crazy idea to not build a

0:40:21.000 --> 0:40:22.120
<v Speaker 2>black hole in Pasadena.

0:40:22.160 --> 0:40:23.759
<v Speaker 1>I feel like it's a little says, you have to

0:40:23.760 --> 0:40:27.320
<v Speaker 1>throw that disclaimer in there, it's like, what are you

0:40:27.320 --> 0:40:31.239
<v Speaker 1>guys doing? I am not destroying your town if that's

0:40:31.239 --> 0:40:34.759
<v Speaker 1>what you're asking. First of all, let's get that clear.

0:40:35.040 --> 0:40:36.360
<v Speaker 2>That didn't make you feel any better.

0:40:37.320 --> 0:40:40.640
<v Speaker 1>Nobody asked I wasn't something I was concerned about before.

0:40:41.160 --> 0:40:41.440
<v Speaker 3>All right.

0:40:41.480 --> 0:40:44.000
<v Speaker 2>In that case, I'm also not testing any nuclear weapons

0:40:44.040 --> 0:40:44.680
<v Speaker 2>in Pasadena.

0:40:44.840 --> 0:40:47.480
<v Speaker 1>Oh good, thank you. What else are you not doing

0:40:47.480 --> 0:40:52.000
<v Speaker 1>in Pasadena? Let's go down the list. All right. Well,

0:40:52.040 --> 0:40:55.439
<v Speaker 1>here is Daniel's interview with Professor Catherine Zurich from cal Tech.

0:40:55.719 --> 0:41:00.160
<v Speaker 2>All right, so it's my pleasure to welcome Professor Katherin Zurchod.

0:41:00.440 --> 0:41:02.160
<v Speaker 2>Thank you very much for chatting with us.

0:41:02.520 --> 0:41:04.000
<v Speaker 3>It's my pleasure to join you.

0:41:04.360 --> 0:41:07.360
<v Speaker 2>So help me understand, first of all, how it's possible

0:41:07.520 --> 0:41:11.200
<v Speaker 2>at all to see effects of quantum gravity. We understood

0:41:11.239 --> 0:41:12.840
<v Speaker 2>for a long time that these things were just on

0:41:12.880 --> 0:41:15.680
<v Speaker 2>the plank scale. How do they sort of work together

0:41:15.800 --> 0:41:19.280
<v Speaker 2>to emerge to some signal we can see experimentally.

0:41:19.520 --> 0:41:22.280
<v Speaker 3>So it's just like smoke. So if you ask yourself

0:41:22.280 --> 0:41:27.239
<v Speaker 3>the question how to smoke spread? So there are interactions

0:41:27.280 --> 0:41:30.880
<v Speaker 3>of molecules on very short distance scales, much shorter than

0:41:30.920 --> 0:41:33.279
<v Speaker 3>what we can observe and yet you can see the

0:41:33.320 --> 0:41:38.279
<v Speaker 3>effects of those short distance interactions simply by waiting a

0:41:38.360 --> 0:41:44.640
<v Speaker 3>while for the effects of those short range interactions to

0:41:44.680 --> 0:41:50.799
<v Speaker 3>accumulate over time. So that's a physical analogy for what

0:41:50.840 --> 0:41:55.320
<v Speaker 3>we're interested in doing. So we have these quantum fluctuations

0:41:55.360 --> 0:41:58.440
<v Speaker 3>on very short distance scales. So in this case it's

0:41:58.480 --> 0:42:00.479
<v Speaker 3>the plank length, which is about to into the minus

0:42:00.520 --> 0:42:06.280
<v Speaker 3>thirty five meters. And the idea is that if those

0:42:06.680 --> 0:42:13.680
<v Speaker 3>quantum fluctuations accumulate over long times, then we can observe them.

0:42:14.000 --> 0:42:17.160
<v Speaker 3>They're still very small, but we can observe them then

0:42:17.280 --> 0:42:21.320
<v Speaker 3>with sufficiently precise instruments.

0:42:21.680 --> 0:42:25.080
<v Speaker 2>So what makes quantum fluctuations add up to make a

0:42:25.120 --> 0:42:29.480
<v Speaker 2>microscopic effect and what makes them not because sometimes they don't. Right,

0:42:29.560 --> 0:42:31.400
<v Speaker 2>you have like a bunch of electrons in a baseball,

0:42:31.400 --> 0:42:34.080
<v Speaker 2>they have all such fluctuations those average out to nothing.

0:42:34.120 --> 0:42:37.479
<v Speaker 2>You can see what makes these guys add up over

0:42:37.880 --> 0:42:39.080
<v Speaker 2>longer distance scales.

0:42:39.280 --> 0:42:43.320
<v Speaker 3>So it's really the fact that you're losing information. Any

0:42:43.560 --> 0:42:48.440
<v Speaker 3>measurement that you make is over a finite time. So

0:42:48.800 --> 0:42:50.960
<v Speaker 3>you know, I turn on my instrument, let's say it's

0:42:50.960 --> 0:42:54.560
<v Speaker 3>in an intraferometer, and the light goes out. It comes

0:42:54.600 --> 0:42:56.799
<v Speaker 3>back and I make a measurement of it. And so

0:42:57.080 --> 0:42:59.840
<v Speaker 3>what it does, what an instrument does, is it defines

0:43:00.080 --> 0:43:02.920
<v Speaker 3>what we call a horizon. So there's a region of

0:43:02.920 --> 0:43:04.840
<v Speaker 3>the space time that I measure and there's a region

0:43:04.880 --> 0:43:07.160
<v Speaker 3>of the space time that I don't, and so that

0:43:07.280 --> 0:43:12.399
<v Speaker 3>leads to a quantum mismeasurement effect that accumulates over time.

0:43:12.920 --> 0:43:16.919
<v Speaker 3>So you're absolutely right that, you know, normal systems, where

0:43:16.920 --> 0:43:21.640
<v Speaker 3>we can confine all of our information to a particular region,

0:43:22.000 --> 0:43:24.960
<v Speaker 3>there's no information that's going to accumulate over time. But

0:43:25.080 --> 0:43:29.520
<v Speaker 3>in this case, we can't actually confine quantum fluctuations. There's

0:43:29.560 --> 0:43:31.760
<v Speaker 3>just part of the space time that we can't measure,

0:43:32.080 --> 0:43:36.680
<v Speaker 3>and so what we're doing now is quantifying how much

0:43:36.800 --> 0:43:41.120
<v Speaker 3>of that information is lost over the period of time

0:43:41.120 --> 0:43:42.280
<v Speaker 3>that I make that measurement.

0:43:42.680 --> 0:43:46.160
<v Speaker 2>Very cool, and so what kind of models of quantum

0:43:46.200 --> 0:43:49.279
<v Speaker 2>space time is as sensitive to generally any kind of

0:43:49.320 --> 0:43:53.360
<v Speaker 2>model where space time has quantum fluctuations or only specific

0:43:53.400 --> 0:43:55.000
<v Speaker 2>sort of kinds of ideas.

0:43:55.280 --> 0:43:59.320
<v Speaker 3>So what we're trying to show is that this effect

0:44:00.280 --> 0:44:08.200
<v Speaker 3>occurs very generally across the space of theoretical ideas that

0:44:09.080 --> 0:44:14.160
<v Speaker 3>people explore, you know, commonly, So what do I mean

0:44:14.200 --> 0:44:17.440
<v Speaker 3>by that exactly, So we're still trying to understand a

0:44:18.280 --> 0:44:21.880
<v Speaker 3>precisely what are the minimal sets of requirements that you need.

0:44:22.239 --> 0:44:26.120
<v Speaker 3>At minimum, we need quantum fluctuations at the plank scale,

0:44:26.880 --> 0:44:32.400
<v Speaker 3>so that has to be there, and those quantum fluctuations

0:44:32.400 --> 0:44:37.440
<v Speaker 3>have to accumulate into the infrared. And there are various

0:44:37.520 --> 0:44:39.719
<v Speaker 3>ways that we can see that. We can see it

0:44:39.800 --> 0:44:43.240
<v Speaker 3>actually coming out in a quite broad range of theories

0:44:43.320 --> 0:44:46.640
<v Speaker 3>where we can just write down some general properties of

0:44:46.680 --> 0:44:49.160
<v Speaker 3>the theory and then crank through it and we see

0:44:49.200 --> 0:44:53.520
<v Speaker 3>this effect come out. So we think it's pretty generic.

0:44:53.760 --> 0:44:57.719
<v Speaker 2>Wonderful, And so why can't existing interchometers like LEGO, which

0:44:57.760 --> 0:45:01.080
<v Speaker 2>is already very very precise, why can't it's signatures of

0:45:01.120 --> 0:45:02.080
<v Speaker 2>this quantum fluctuation.

0:45:02.560 --> 0:45:04.919
<v Speaker 3>So we actually think that LEGO is not very far

0:45:05.000 --> 0:45:07.400
<v Speaker 3>from being able to see it. But one of the

0:45:07.440 --> 0:45:11.360
<v Speaker 3>reasons why LEGO is not optimally sensitive to this signal

0:45:11.719 --> 0:45:17.359
<v Speaker 3>is because they recycle their light by which I mean

0:45:17.960 --> 0:45:21.120
<v Speaker 3>the light beam goes out and it comes back, and

0:45:21.160 --> 0:45:24.080
<v Speaker 3>they don't make a measurement of it. After one round trick,

0:45:24.400 --> 0:45:27.240
<v Speaker 3>it actually goes out and comes back many times before

0:45:27.239 --> 0:45:30.200
<v Speaker 3>they make a measurement of it. And so for the

0:45:30.239 --> 0:45:34.120
<v Speaker 3>signals that they're interested in, which come from you know,

0:45:34.239 --> 0:45:38.040
<v Speaker 3>let's say black holes merging, that's fine because there's a

0:45:38.080 --> 0:45:41.920
<v Speaker 3>classical source that generates a wave at some frequency. In

0:45:42.080 --> 0:45:45.719
<v Speaker 3>this case, we're also interested in gravitational waves, but they're

0:45:45.719 --> 0:45:50.840
<v Speaker 3>gravitational waves that come from the vacuum fluctuating, and they're uncorrelated.

0:45:51.160 --> 0:45:55.040
<v Speaker 3>If I measured the system over time scales that are

0:45:55.120 --> 0:45:57.759
<v Speaker 3>long in comparison to the light crossing time, So the

0:45:57.840 --> 0:46:01.760
<v Speaker 3>fact that ligo weights and beam goes out and comes

0:46:01.800 --> 0:46:04.480
<v Speaker 3>back many times before they measure it means that they're

0:46:04.480 --> 0:46:07.000
<v Speaker 3>actually averaging down their signal, and so they have a

0:46:07.040 --> 0:46:10.640
<v Speaker 3>reduced sensitivity to it in comparison to if they had

0:46:10.640 --> 0:46:14.000
<v Speaker 3>this same that they could measure the same space time fluctuation.

0:46:14.200 --> 0:46:16.239
<v Speaker 3>But they did it after the light just went out

0:46:16.320 --> 0:46:19.440
<v Speaker 3>and came back. Then we claim that you can actually

0:46:19.440 --> 0:46:20.200
<v Speaker 3>see this signal.

0:46:20.320 --> 0:46:23.640
<v Speaker 2>Do these space time fluctuations look different from a gravitational

0:46:23.760 --> 0:46:26.360
<v Speaker 2>way you could get from black hole collisions, for example.

0:46:26.360 --> 0:46:29.120
<v Speaker 3>Yeah, they do. So one thing that's different about this

0:46:29.280 --> 0:46:31.839
<v Speaker 3>signal in comparison to what you would get from let's

0:46:31.840 --> 0:46:34.760
<v Speaker 3>say black hole mergers is in that case, the signal

0:46:34.840 --> 0:46:37.520
<v Speaker 3>is the signal. It doesn't depend on my measuring apparatus.

0:46:37.800 --> 0:46:40.000
<v Speaker 3>If I have a gravitational way of coming in at

0:46:40.040 --> 0:46:43.680
<v Speaker 3>some frequency. It's like your radio station is broadcasting something

0:46:43.840 --> 0:46:46.480
<v Speaker 3>and it has a frequency, and that's just you know,

0:46:46.520 --> 0:46:49.920
<v Speaker 3>you tune it to some station, and that's what it is.

0:46:50.200 --> 0:46:54.840
<v Speaker 3>In this case, what you measure actually depends on your apparatus,

0:46:54.880 --> 0:46:58.800
<v Speaker 3>like your interferometer. So if I have a smaller apparatus,

0:46:59.760 --> 0:47:02.400
<v Speaker 3>my signal is going to be coming in at a

0:47:02.520 --> 0:47:07.799
<v Speaker 3>higher number radio station. Then if I have a bigger apparatus,

0:47:07.880 --> 0:47:10.239
<v Speaker 3>then it comes in at a lower frequency station. The

0:47:10.280 --> 0:47:14.000
<v Speaker 3>reason for that is because it's the quantum mismeasurement. And

0:47:14.000 --> 0:47:16.440
<v Speaker 3>of course how much you're mismeasuring the space time depends

0:47:16.440 --> 0:47:19.000
<v Speaker 3>on how big you know, the volume of space time.

0:47:18.840 --> 0:47:21.240
<v Speaker 2>You're measuring affects your horizon.

0:47:21.520 --> 0:47:23.719
<v Speaker 3>Yeah, it depends on the size of your horizon. That's

0:47:23.719 --> 0:47:25.680
<v Speaker 3>another way of saying it. It depends on the size

0:47:25.680 --> 0:47:28.200
<v Speaker 3>of your horizon, depends on how many quantum degrees of

0:47:28.239 --> 0:47:33.120
<v Speaker 3>freedom are fluctuating inside your volume, which depends on how

0:47:33.160 --> 0:47:35.799
<v Speaker 3>big your horizon is. And so as a result, you know,

0:47:35.920 --> 0:47:38.279
<v Speaker 3>you would really know about this signal. First of all,

0:47:38.280 --> 0:47:41.359
<v Speaker 3>it would have a very particular shape, but it would

0:47:41.360 --> 0:47:44.080
<v Speaker 3>depend on your measuring apparatus, So you could compare between

0:47:44.080 --> 0:47:46.880
<v Speaker 3>different instruments and then start to tell what the source

0:47:46.920 --> 0:47:47.520
<v Speaker 3>of it would be.

0:47:47.719 --> 0:47:50.799
<v Speaker 2>And can you also see things unexpected, like if there's

0:47:50.800 --> 0:47:53.719
<v Speaker 2>a general enough detector that you might see things that

0:47:53.960 --> 0:47:57.359
<v Speaker 2>aren't these quantum fluctuations, then aren't gravitational away some black

0:47:57.360 --> 0:47:59.960
<v Speaker 2>holes but something else, you know, surprise?

0:48:00.600 --> 0:48:03.800
<v Speaker 3>Yeah. Sure, So these instruments that were interested in building,

0:48:03.840 --> 0:48:07.640
<v Speaker 3>they can be sensitive to anything that's generating gravitational waves

0:48:07.640 --> 0:48:11.919
<v Speaker 3>in that same frequency range. So the signal definitely has

0:48:11.960 --> 0:48:14.600
<v Speaker 3>to be predictive enough to be able to tell apart

0:48:14.760 --> 0:48:18.520
<v Speaker 3>different sources. And our claim is that the signal has

0:48:18.680 --> 0:48:22.480
<v Speaker 3>very particular you know, frequencies that it's peaked at. It

0:48:22.600 --> 0:48:26.040
<v Speaker 3>has angular correlations, like it depends on the angle between

0:48:26.080 --> 0:48:29.880
<v Speaker 3>the arms and your interferometer. So therefore you'll be able

0:48:29.960 --> 0:48:33.360
<v Speaker 3>to tell what the source of these gravitational waves.

0:48:33.080 --> 0:48:35.520
<v Speaker 2>Are and what's the sort of timeline like best case

0:48:35.560 --> 0:48:38.200
<v Speaker 2>scenario when you guys can build this thing and discover

0:48:38.320 --> 0:48:39.000
<v Speaker 2>quantum gravity.

0:48:39.239 --> 0:48:45.600
<v Speaker 3>Yeah yeah, So we've got the first bit of funding

0:48:45.840 --> 0:48:50.560
<v Speaker 3>to come in and my colleague Lemacullor who's spearheading this

0:48:50.719 --> 0:48:55.080
<v Speaker 3>effort here at Caltech. You know, his lab is ramping

0:48:55.160 --> 0:49:00.080
<v Speaker 3>up on this. There are some technological objectives that they

0:49:00.080 --> 0:49:01.840
<v Speaker 3>have to demonstrate, and they have to do R and

0:49:01.960 --> 0:49:07.439
<v Speaker 3>D because they're proposing a novel readout scheme for these interferometer.

0:49:09.040 --> 0:49:13.840
<v Speaker 3>What we have proposed is to have a demonstrator apparatus

0:49:14.719 --> 0:49:19.919
<v Speaker 3>that would kind of scrape the signal. Okay, we're talking

0:49:19.960 --> 0:49:24.880
<v Speaker 3>about two sigma kind of sensitivity in five years, so

0:49:24.960 --> 0:49:28.440
<v Speaker 3>I think to really start to see this, you know,

0:49:28.600 --> 0:49:32.239
<v Speaker 3>like five sigma, you're just really confident you can start

0:49:32.239 --> 0:49:35.760
<v Speaker 3>to test various aspects of it. I think we're probably

0:49:35.800 --> 0:49:37.799
<v Speaker 3>talking the ten year timescale.

0:49:37.880 --> 0:49:40.359
<v Speaker 2>So I've read your paper. There's a lot of nice

0:49:40.400 --> 0:49:43.520
<v Speaker 2>theoretical maneuvers in there. My question to you is, do

0:49:43.560 --> 0:49:45.320
<v Speaker 2>you believe this is going to be real? Like you

0:49:45.440 --> 0:49:47.759
<v Speaker 2>turn this thing on in ten years? Nature tales you

0:49:47.800 --> 0:49:51.040
<v Speaker 2>an answer. What's your confidence that this is out there

0:49:51.080 --> 0:49:51.799
<v Speaker 2>that you're going to see it?

0:49:52.200 --> 0:49:55.800
<v Speaker 3>Yeah, so it doesn't seem to be going away. Let's

0:49:55.800 --> 0:49:59.040
<v Speaker 3>put it that way. When you see something in a calculation,

0:50:00.120 --> 0:50:03.440
<v Speaker 3>you know, you try to test it by doing a

0:50:03.440 --> 0:50:07.840
<v Speaker 3>different calculation that behaves differently. You know, it has different

0:50:07.880 --> 0:50:11.239
<v Speaker 3>theoretical systematics, and the kinds of things that you could

0:50:11.320 --> 0:50:14.640
<v Speaker 3>mess up in the calculation are different, so on and

0:50:14.640 --> 0:50:17.520
<v Speaker 3>so forth. And then you also check for whether it's

0:50:17.560 --> 0:50:21.840
<v Speaker 3>in conflict with anything that you know. And through the

0:50:21.920 --> 0:50:25.120
<v Speaker 3>process of doing this, you know, based on my experience,

0:50:25.120 --> 0:50:27.920
<v Speaker 3>when you try to build a theory, oftentimes it'll fail

0:50:28.480 --> 0:50:30.280
<v Speaker 3>and then you try to fix it up by adding

0:50:30.320 --> 0:50:33.360
<v Speaker 3>other things to it. This has not been like that.

0:50:35.239 --> 0:50:37.440
<v Speaker 3>If it seems like it's going to fail for some reason,

0:50:38.200 --> 0:50:40.440
<v Speaker 3>it means that you should just stop and wait and

0:50:40.480 --> 0:50:44.560
<v Speaker 3>try to understand what's there better, because it fixes itself.

0:50:44.960 --> 0:50:49.160
<v Speaker 3>So to me, that's an indication that there's something there.

0:50:49.880 --> 0:50:54.040
<v Speaker 3>It hangs together in a very self consistent way, and

0:50:54.120 --> 0:50:57.239
<v Speaker 3>so from that point of view, I find it theoretically

0:50:57.360 --> 0:51:01.719
<v Speaker 3>very attractive, very interesting. It's right now, I don't want

0:51:01.760 --> 0:51:05.400
<v Speaker 3>to tell nature what to do. Right. Nature gets to decide.

0:51:05.800 --> 0:51:07.560
<v Speaker 3>You know, there are some things that go in right,

0:51:07.560 --> 0:51:10.719
<v Speaker 3>there's this fundamental fluctuations and then space time you know,

0:51:10.840 --> 0:51:12.800
<v Speaker 3>needs to remember right, so there needs to be the

0:51:12.920 --> 0:51:15.560
<v Speaker 3>sense in which you're losing information. And if those two

0:51:15.600 --> 0:51:19.240
<v Speaker 3>things are there in nature, and we certainly know lots

0:51:19.280 --> 0:51:24.080
<v Speaker 3>of analogous physical systems where that happens, then we'll see it.

0:51:24.480 --> 0:51:28.319
<v Speaker 3>But at the end of the day, nature decides. And

0:51:28.360 --> 0:51:30.440
<v Speaker 3>that's one of the things I really like about this

0:51:30.520 --> 0:51:32.600
<v Speaker 3>problem is I can write these things down on paper

0:51:32.680 --> 0:51:36.000
<v Speaker 3>and they're beautiful, and I'm understanding more things about it

0:51:36.040 --> 0:51:38.520
<v Speaker 3>from a mathematical perspective. But at the end of the day,

0:51:38.880 --> 0:51:39.960
<v Speaker 3>nature gets to decide.

0:51:40.200 --> 0:51:42.879
<v Speaker 2>All right, Well, we look forward to hearing nature's side

0:51:42.880 --> 0:51:45.200
<v Speaker 2>of the story. Thanks very much for joining us today.

0:51:45.760 --> 0:51:48.280
<v Speaker 1>All right, pretty interesting. I'm super impressed you can talk

0:51:48.320 --> 0:51:51.000
<v Speaker 1>to a theorist. I thought you guys spoke different languages

0:51:51.040 --> 0:51:52.520
<v Speaker 1>and didn't like each other.

0:51:52.760 --> 0:51:55.719
<v Speaker 2>They mostly speak in Greek symbols exactly, but sometimes I

0:51:55.760 --> 0:51:58.160
<v Speaker 2>can translate. These days, I'm trying to move a little

0:51:58.160 --> 0:52:00.560
<v Speaker 2>bit in the direction of theoretical physics, so it's really

0:52:00.600 --> 0:52:02.560
<v Speaker 2>fun for me to talk to these folks. But yeah,

0:52:02.600 --> 0:52:05.160
<v Speaker 2>they think on a whole different plane of existence. But

0:52:05.200 --> 0:52:08.760
<v Speaker 2>what's really cool are theorists who propose experiments, who develop

0:52:08.920 --> 0:52:12.720
<v Speaker 2>new techniques and new ideas that allow experimentalists to maybe

0:52:12.760 --> 0:52:16.160
<v Speaker 2>force the universe to reveal something about its nature. And

0:52:16.200 --> 0:52:18.240
<v Speaker 2>the story of this one is similar to the story

0:52:18.280 --> 0:52:21.960
<v Speaker 2>of a very similar experiment, which is LIGO, the innerferometer

0:52:22.080 --> 0:52:25.960
<v Speaker 2>that looked for classical gravitational waves. That was originally just

0:52:26.000 --> 0:52:29.120
<v Speaker 2>a theoretical idea, and experimentalists were like, all right, let's

0:52:29.120 --> 0:52:30.719
<v Speaker 2>try to build it, see if we can find it,

0:52:30.760 --> 0:52:33.799
<v Speaker 2>and they did. This is like the quantum version of it,

0:52:34.160 --> 0:52:37.600
<v Speaker 2>which would look for little quantum ripples in space time,

0:52:37.719 --> 0:52:42.360
<v Speaker 2>basically little quantum gravitational waves. And the experiment itself is similar.

0:52:42.440 --> 0:52:45.840
<v Speaker 2>It's a little innerferometer. Like shoot laser beams back and forth,

0:52:46.200 --> 0:52:48.160
<v Speaker 2>see how they overlap, and see if you can catch

0:52:48.160 --> 0:52:51.480
<v Speaker 2>a graviton interfering with those laser beams.

0:52:51.840 --> 0:52:55.279
<v Speaker 1>Hmmm, because the gravit times would be sort of like

0:52:55.400 --> 0:52:59.000
<v Speaker 1>bedding space, is that the idea? Because gravity can't interact

0:52:59.000 --> 0:53:01.960
<v Speaker 1>with footon or candy.

0:53:01.680 --> 0:53:04.400
<v Speaker 2>Gravity doesn't interact with photons in a sort of Newtonian

0:53:04.440 --> 0:53:07.520
<v Speaker 2>way because photons have no mass, but gravity does bend space,

0:53:07.560 --> 0:53:10.759
<v Speaker 2>and photons move through that bend space, and so yeah,

0:53:10.800 --> 0:53:14.680
<v Speaker 2>you're exactly right, Like a little gravitational quantum fluctuation the

0:53:14.800 --> 0:53:18.320
<v Speaker 2>kind she's looking for, would affect the shape of space

0:53:18.400 --> 0:53:20.560
<v Speaker 2>for one of these beams and would sort of knock

0:53:20.600 --> 0:53:23.160
<v Speaker 2>a photon out of the path. And that's what they're

0:53:23.200 --> 0:53:23.640
<v Speaker 2>looking for.

0:53:24.440 --> 0:53:26.480
<v Speaker 1>The idea is that like a graviton would pop out

0:53:26.480 --> 0:53:29.520
<v Speaker 1>of nowhere, it pops out, it bends space around it,

0:53:29.600 --> 0:53:32.040
<v Speaker 1>and maybe it will deflect the photon. Is that the idea.

0:53:32.200 --> 0:53:34.719
<v Speaker 2>That's the idea. But it's not one single graviton that

0:53:34.760 --> 0:53:37.520
<v Speaker 2>would be totally invisible. It's this effect where a lot

0:53:37.560 --> 0:53:41.160
<v Speaker 2>of gravitons are working together. And the super duper weird

0:53:41.200 --> 0:53:44.000
<v Speaker 2>thing is that this effect only happens when you're making

0:53:44.040 --> 0:53:47.200
<v Speaker 2>a measurement. It's a quantum effect. It comes from not

0:53:47.239 --> 0:53:50.600
<v Speaker 2>being able to see the whole universe. So she's imagining

0:53:50.640 --> 0:53:53.399
<v Speaker 2>space filled with all these gravitons, and when you make

0:53:53.440 --> 0:53:55.319
<v Speaker 2>this measurement, it can only be affected by like a

0:53:55.360 --> 0:53:58.520
<v Speaker 2>certain bubble of the universe, a bubble of the universe

0:53:58.560 --> 0:54:00.960
<v Speaker 2>that's like close enough to you that light can travel

0:54:01.000 --> 0:54:04.480
<v Speaker 2>to you. Because you create this information horizon, you limit

0:54:04.640 --> 0:54:07.520
<v Speaker 2>like the wavelengths of these gravitons, and so only some

0:54:07.600 --> 0:54:09.759
<v Speaker 2>of them can talk to your experiment, and that's what

0:54:09.880 --> 0:54:12.600
<v Speaker 2>creates this weird effect. And I'll be totally honest, there's

0:54:12.640 --> 0:54:14.920
<v Speaker 2>a lot of math there that I just don't even understand.

0:54:15.120 --> 0:54:17.560
<v Speaker 2>But she's been trying to prove to herself that this

0:54:17.640 --> 0:54:20.000
<v Speaker 2>works or that this doesn't work, and the math just

0:54:20.120 --> 0:54:22.719
<v Speaker 2>keeps holding together no matter how she probes it. So,

0:54:22.840 --> 0:54:25.280
<v Speaker 2>as you heard maybe in the interview, she really believes

0:54:25.320 --> 0:54:25.879
<v Speaker 2>this is real.

0:54:26.280 --> 0:54:28.120
<v Speaker 1>And so the idea is that you could maybe build

0:54:28.160 --> 0:54:31.440
<v Speaker 1>this experiment on a tabletop like it could be, you know,

0:54:31.520 --> 0:54:34.320
<v Speaker 1>a small experiment to prove a huge thing like quantum

0:54:34.360 --> 0:54:35.360
<v Speaker 1>gravity exactly.

0:54:35.600 --> 0:54:40.319
<v Speaker 2>Lego classical gravitational wave experiment is like kilometers long and

0:54:40.360 --> 0:54:42.879
<v Speaker 2>cost billions of dollars. This would be like meters long.

0:54:42.920 --> 0:54:45.319
<v Speaker 2>You literally could build it in a lab in the

0:54:45.360 --> 0:54:48.920
<v Speaker 2>basement at Caltech, and if it works, they could see

0:54:49.080 --> 0:54:52.680
<v Speaker 2>quantum gravitational effects on these beams of light and they

0:54:52.680 --> 0:54:55.640
<v Speaker 2>could prove that gravitons are out there and that they're

0:54:55.719 --> 0:54:58.759
<v Speaker 2>dancing together to make these little tiny ripples in space time.

0:54:59.200 --> 0:55:02.239
<v Speaker 1>Cool. Well, she's welcome to hang out in my backyard

0:55:02.320 --> 0:55:06.000
<v Speaker 1>and do the experiment here. That could be exciting.

0:55:07.800 --> 0:55:09.719
<v Speaker 2>I don't think she wants her experiment it sprayed by

0:55:09.719 --> 0:55:11.320
<v Speaker 2>the hose or like doused with water.

0:55:11.160 --> 0:55:15.920
<v Speaker 1>Balloons, yeah, or have screaming kids running all around it

0:55:15.960 --> 0:55:19.080
<v Speaker 1>that you usually it tends to make gravitons shy.

0:55:19.120 --> 0:55:21.560
<v Speaker 2>I tend to dampen the effects of your experiment.

0:55:21.920 --> 0:55:24.760
<v Speaker 1>All right, well, pretty exciting. Thank you to doctor Catherine

0:55:24.880 --> 0:55:28.880
<v Speaker 1>Zurich for talking about her research. What does this all mean, Daniel,

0:55:29.160 --> 0:55:32.640
<v Speaker 1>Are we far or near proving the idea of quantum gravity?

0:55:33.120 --> 0:55:35.600
<v Speaker 2>I think we're still pretty far from figuring anything out.

0:55:35.680 --> 0:55:37.880
<v Speaker 2>The theorists are working hard and making progress all the

0:55:37.920 --> 0:55:41.200
<v Speaker 2>time about building their theories. But now it's exciting that

0:55:41.280 --> 0:55:44.759
<v Speaker 2>we have experimental efforts which maybe in the next five, ten,

0:55:44.880 --> 0:55:47.759
<v Speaker 2>fifteen years could provide us with really valuable clues to

0:55:47.800 --> 0:55:50.680
<v Speaker 2>tell us, Oh, gravity is classical or nope, gravity is

0:55:50.760 --> 0:55:53.360
<v Speaker 2>quantum mechanical. You better figure it out. That would be

0:55:53.400 --> 0:55:57.359
<v Speaker 2>really powerful indication for sort of which direction to go theoretically.

0:55:57.760 --> 0:56:00.760
<v Speaker 2>And I love this dance between experimental and the radical physics.

0:56:00.760 --> 0:56:03.200
<v Speaker 2>You know, the ideas flourish and then experiments kill them,

0:56:03.440 --> 0:56:07.000
<v Speaker 2>or sometimes experiments discover something weird which inspires lots of

0:56:07.040 --> 0:56:10.279
<v Speaker 2>new theoretical ideas. It's really beautiful to see the interplay

0:56:10.280 --> 0:56:14.360
<v Speaker 2>of these two different avenues of exploration. It's like a

0:56:14.480 --> 0:56:17.680
<v Speaker 2>theoretical tango exactly. Even the physicists don't really know how

0:56:17.680 --> 0:56:19.879
<v Speaker 2>to flirt. And I think the tango is pretty flirtatious.

0:56:20.040 --> 0:56:23.280
<v Speaker 1>All right, Well, it sounds like the answer is stay tuned.

0:56:23.520 --> 0:56:25.719
<v Speaker 1>In theory, it might be ten to fifteen years, but

0:56:25.880 --> 0:56:28.879
<v Speaker 1>in reality, who knows. It could be that we may

0:56:28.920 --> 0:56:31.399
<v Speaker 1>never answer this question, or it could be that we'll

0:56:31.440 --> 0:56:33.160
<v Speaker 1>answer it within our lifetimes.

0:56:33.400 --> 0:56:36.560
<v Speaker 2>That's right, we could be flirting with understanding or confusion.

0:56:36.880 --> 0:56:39.600
<v Speaker 1>We hope you enjoyed that. Thanks for joining us, See

0:56:39.640 --> 0:56:40.160
<v Speaker 1>you next time.

0:56:48.080 --> 0:56:50.880
<v Speaker 2>Thanks for listening, and remember that Daniel and Jorge Explain

0:56:50.920 --> 0:56:54.200
<v Speaker 2>the Universe is a production of iHeart Radio. For more

0:56:54.280 --> 0:56:59.080
<v Speaker 2>podcasts from iHeartRadio, visit the iHeartRadio app, Apple Podcasts, or

0:56:59.120 --> 0:57:01.360
<v Speaker 2>wherever you listen into your favorite shows.

0:57:06.680 --> 0:57:09.400
<v Speaker 3>M hm h