WEBVTT - What is Bose Einstein Condensate

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<v Speaker 1>Hey, Jorney, do you know who is the first person

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<v Speaker 1>to reach the South Pole? It's probably a Norwegian, wasn't

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<v Speaker 1>it someone called rolled Emson. Yeah, he's pretty famous. But

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<v Speaker 1>do you know who the second or third place finishes were.

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<v Speaker 1>I'm gonna guess rold Emonson Jr. Or rold Emonson the third.

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<v Speaker 1>I have no idea. You know, those people who came

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<v Speaker 1>in second and third, they risked their lives, literally froze

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<v Speaker 1>their butts off, and we don't even know who they are.

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<v Speaker 1>Man in this case, it was literally a raised to

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<v Speaker 1>the bottom of the world. But yeah, you're right, I

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<v Speaker 1>guess second place doesn't get much attention. And the same

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<v Speaker 1>is true in science. There's no consolation prize for the Nobel.

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<v Speaker 1>You don't get a silver Noble price. They should hand

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<v Speaker 1>out a silver and a bronze, an honorable mention. There

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<v Speaker 1>just an honor to be nominated. Hi, I'm or Hamming

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<v Speaker 1>cartoonists and the creator of PhD comments. Hi I'm Daniel.

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<v Speaker 1>I'm a particle of physicist. And if I was in

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<v Speaker 1>the running for the Nobel Prize, I wouldn't get the

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<v Speaker 1>silver or le bronze. I would get the Plywood Nobel Prize.

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<v Speaker 1>You get the thanks for Trying coupon, I get the

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<v Speaker 1>pin and ribbon on him and say thanks. Welcome to

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<v Speaker 1>our podcast, Daniel and Jorge Explained the Universe, a production

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<v Speaker 1>of I Heart Radio in which we take a tour

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<v Speaker 1>of all the incredible things that scientists have won the

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<v Speaker 1>Nobel Prize for and dive deep into all the things

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<v Speaker 1>that science has not yet figured out, all the things

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<v Speaker 1>that people want to understand, all those weird mysteries of

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<v Speaker 1>the universe that nobody has yet figured out. Because it's

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<v Speaker 1>a big, mysterious universe out there and humans are trying

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<v Speaker 1>to make sense of it and come up with theories

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<v Speaker 1>about how it all works. But it is, after all

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<v Speaker 1>a human endeavor, and so it's about humans chipping away

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<v Speaker 1>at the big unknown questions of the universe. And here

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<v Speaker 1>on the show, we like to talk about the smallest things.

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<v Speaker 1>We like to break open the universe and find out

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<v Speaker 1>what it's made out of. What are the smallest things.

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<v Speaker 1>But another sort of orthogonal way to approach discovery is

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<v Speaker 1>trying to make matter do weird stuff like you're familiar

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<v Speaker 1>with three states of matter, solids, liquids in gases, But

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<v Speaker 1>it turns out there are lots of other really weird

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<v Speaker 1>things that matter can do. Yeah, there are other states

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<v Speaker 1>of matter like super hot forms like plasma, and also

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<v Speaker 1>super cold forms. And one of these forms is a

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<v Speaker 1>pretty well known form that we're going to talk about today.

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<v Speaker 1>That's right. If you get matter into really weird configurations,

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<v Speaker 1>it will do strange stuff. And this is a great

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<v Speaker 1>way to learn about what the rules are, how does

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<v Speaker 1>it fit together, what are the forces that are involved?

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<v Speaker 1>And it's just fun to make matter be weird. Can

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<v Speaker 1>you make it shinye? Can you make it jump? Can

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<v Speaker 1>you make it super conducting? Can you make it super fluid?

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<v Speaker 1>Can you make it act as a single blob? It's

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<v Speaker 1>fun to make new kinds of Google, would that be

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<v Speaker 1>your bumper sticker, Daniel? Keep matter weird, yeah, because one

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<v Speaker 1>of the basic ways to explore the universe is just

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<v Speaker 1>to look around you and see, like what kinds of

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<v Speaker 1>stuff is there? You know, the very first people to

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<v Speaker 1>think about what is the universe made out of just

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<v Speaker 1>sort of organized the stuff around them into like you know,

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<v Speaker 1>air or fire, earth and water. And that's reflection that

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<v Speaker 1>there are different kinds of things. And even though we

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<v Speaker 1>know that the universe has made fundamentally of tying the

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<v Speaker 1>little particles. Those particles come together in really weird ways.

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<v Speaker 1>I mean, who could predict solids and gases and all

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<v Speaker 1>sorts of weird behavior from just the tiny particles. It's complicated.

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<v Speaker 1>So while it's worthwhile to like dig down deep to

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<v Speaker 1>the tiny bits, it's also really worthwhile to figure out

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<v Speaker 1>how those bits play together to make weird stuff. So

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<v Speaker 1>to the the program will be asking the question, what

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<v Speaker 1>is a Bose Einstein condensate now? M Daniel, I'm guessing

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<v Speaker 1>that's not related to both speakers or being like a BOWS.

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<v Speaker 1>I think Bose was an early investor in the Bows

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<v Speaker 1>speaker system. They're not related. The Bose family fortune came

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<v Speaker 1>from physics. No, but they are related to the Higgs boson.

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<v Speaker 1>It's the same Bows, is it? Yeah? Yes, absolutely, the

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<v Speaker 1>Bose Einstein condensate is related to the Higgs boson. It's

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<v Speaker 1>the same. Bows is a famous Indian physicist whose last

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<v Speaker 1>name is Bose, and the kind of particle that we

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<v Speaker 1>call a boson, a particle of spin one, is named

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<v Speaker 1>after both. And he's also the guy who worked together

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<v Speaker 1>with Einstein to come up with this idea of a

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<v Speaker 1>weird state of matter called the Bose Einstein content. So

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<v Speaker 1>he did rocket leg a ball And I don't know

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<v Speaker 1>if you remember, but after the Higgs boson was discovered,

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<v Speaker 1>there are a lot of folks in India who are like, hey,

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<v Speaker 1>how come Higgs is getting all the credit? After all?

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<v Speaker 1>What about bos is important contribution? His name is half

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<v Speaker 1>of Higgs boson. Why isn't he getting as much credit? Wow?

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<v Speaker 1>I guess it's lots of brand appealed, like clean X. Yeah. Well,

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<v Speaker 1>if you're gonna get your name on stuff, you know,

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<v Speaker 1>you can get your name on one individual particle like Higgs,

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<v Speaker 1>or you can get your name on like a whole

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<v Speaker 1>class of particles like bosons. Bosons are anything with integer spin.

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<v Speaker 1>That's like half the particles out there, photons, w's, z

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<v Speaker 1>s all these are boson particles. Right. Well, so today

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<v Speaker 1>this is about states of matter, and you're right, it

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<v Speaker 1>is kind of interesting that, you know, we can talk

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<v Speaker 1>about what matter is and what it does and what

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<v Speaker 1>it looks like, but we can also talk about the

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<v Speaker 1>ways it can form itself or the ways that it

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<v Speaker 1>can exist out there. Yeah, and it's incredible that we

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<v Speaker 1>can sometimes predict this. We can just like write down

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<v Speaker 1>math on a piece of paper and say, we think

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<v Speaker 1>if you put these atoms in this weird configuration that

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<v Speaker 1>do this amazing, crazy thing you can't otherwise see. And

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<v Speaker 1>then it's a game of seeing whether you can do it.

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<v Speaker 1>You know, it's an experimental challenge. And this is one

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<v Speaker 1>of those stories where the theorists were decades and decades

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<v Speaker 1>ahead of the experimentalists. They had this idea in the

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<v Speaker 1>twenties and it wasn't until the nineties that people figured

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<v Speaker 1>it out. That means that it was one of these

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<v Speaker 1>like plums hanging out there where everybody knew if you

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<v Speaker 1>could be the first one to do it, you would

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<v Speaker 1>get a Nobel Prize. And there was sort of like,

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<v Speaker 1>you know, progress for ten years, and then things ground

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<v Speaker 1>to a halt. Nobody had any good ideas, and then

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<v Speaker 1>I burst a progress and then very late in the game,

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<v Speaker 1>a quick sprint to the finish line, where you know,

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<v Speaker 1>the people who crossed the finish line first, they win

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<v Speaker 1>the Nobel Prize and everybody else just has a cold

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<v Speaker 1>gas of atoms man. So only two people are famous,

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<v Speaker 1>the people who come up with a problem and the

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<v Speaker 1>people who solve the problem. Everyone in between gets forgot

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<v Speaker 1>that's right. And if you find this kind of story inspiring,

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<v Speaker 1>you know, there are plenty of other things out there

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<v Speaker 1>which everybody knows. If you discover them, you would win

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<v Speaker 1>a Nobel Prize. And maybe we're five years, maybe we're

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<v Speaker 1>fifty years away from discovering those things and somebody getting

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<v Speaker 1>the Nobel Prize. But there is plenty of low hanging

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<v Speaker 1>fruit left in physics. All right, are you making a

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<v Speaker 1>plug for bananas, Daniel, because they're pretty low hanging In general,

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<v Speaker 1>people have discovered bananas already, sorry to first bubble well,

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<v Speaker 1>such as the case for the Bose Einstein concent And

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<v Speaker 1>as usually, we were wondering how many people out there

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<v Speaker 1>knew what this was or where familiar with what the

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<v Speaker 1>state of matter is, And so as usual, Daniel went

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<v Speaker 1>out there into the wilds of the internet to ask

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<v Speaker 1>people what is a Bose Einstein concent That's right? And

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<v Speaker 1>if you'd like to participate in our random person on

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<v Speaker 1>the Internet questions, please write to us two questions at

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<v Speaker 1>Daniel and jorgean dot com. We would love to hear

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<v Speaker 1>your thoughts for future upcoming episodes. Here's what people had

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<v Speaker 1>to say. I would imagine something to do with Albert Einstein,

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<v Speaker 1>though I don't think it has anything to do with

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<v Speaker 1>Bose audio. I would guess it might have something to

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<v Speaker 1>do with Bosn's and condensate means, maybe something with the

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<v Speaker 1>way they behave at a particular temperature or pressure. Maybe

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<v Speaker 1>it's a speaker of the vibrates water out of the

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<v Speaker 1>year and then use the hydrogen to blow up your house. Well,

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<v Speaker 1>I heard about it, but I don't remember. It's some

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<v Speaker 1>kind of state or I don't know. I think Bose

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<v Speaker 1>was a fellow that was around before Einstein who came

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<v Speaker 1>up with the initial concept, and then I think Einstein

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<v Speaker 1>sweetened the deal a little bit. But this was around

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<v Speaker 1>something hectic to do with theory of relativity and the

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<v Speaker 1>expansion of the universe and universal constants, So I think

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<v Speaker 1>it was something related to that, but I can't quite remember.

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<v Speaker 1>I know it was mentioned on the podcast recently. It

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<v Speaker 1>was the state of matter, I think from dron The

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<v Speaker 1>scientists in the s S lab found it in some

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<v Speaker 1>udom cold lab that in the one name and they

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<v Speaker 1>discoded it's been theoretical so far, and so first them

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<v Speaker 1>there's something you exist in that state of matter? All right, Well,

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<v Speaker 1>it sounds like a lot of people knew was a

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<v Speaker 1>state of matter. Yeah, except for the folks who thought

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<v Speaker 1>it was a speaker that vibrates water out of the

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<v Speaker 1>air and blows up your house. Wow. Where did that

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<v Speaker 1>one come from? Right? I don't know. That must have

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<v Speaker 1>been like an awesome installation of massive bows speakers that

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<v Speaker 1>chattered somebody's windows or something, And I like somebody made

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<v Speaker 1>that connection to the Boson particle. Yeah, exactly. So there's

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<v Speaker 1>some good general knowledge out there. Good job listeners. Yeah,

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<v Speaker 1>so bose, Einstein, condensate, Daniel, let's dig into it. What

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<v Speaker 1>is it? I'm guessing it has something to do with

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<v Speaker 1>Einstein and maybe condensed milk? Is that the sweet and

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<v Speaker 1>condensed milk? Yes, it's a recipe for lemon bars by

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<v Speaker 1>Boz and only if you get it cold enough and

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<v Speaker 1>only the first bite. Yeah. So what it is is

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<v Speaker 1>a new state of matter, another state of matter different

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<v Speaker 1>and from liquid, solid, or gas or even plasma. And

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<v Speaker 1>as you said before, those are the states of matter

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<v Speaker 1>sort of organized in terms of temperature increasing, right, solid, liquid, gas, plasma.

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<v Speaker 1>And what happens there is the particles are disassociating as

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<v Speaker 1>they get hotter and hotter, they tend to move around more,

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<v Speaker 1>they have less restrictions. But there are these phase differences, right,

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<v Speaker 1>Things don't go smoothly from solid to liquid and liquid

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<v Speaker 1>to gas. They're these transitions where suddenly things behave different Wait,

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<v Speaker 1>isn't there a middle state called the smoothie or a

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<v Speaker 1>carbonated drink. That's right, it's called the margarita. That's the

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<v Speaker 1>state of matter you discover after you win the Nogo process. Right, Yeah,

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<v Speaker 1>it's made of dacorns. Now, So they're these interesting transitions,

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<v Speaker 1>and that's fascinating, right that these particles tend to work

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<v Speaker 1>in one way and then you cross them over a

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<v Speaker 1>threshold and they tend to work in another way, Like

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<v Speaker 1>there are different rules for gases and liquids and solids

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<v Speaker 1>and lasmas, right. And it has something to do with

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<v Speaker 1>the forces that bind atoms together and particles together, right, Like,

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<v Speaker 1>at some point their energy is more than the that bond,

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<v Speaker 1>and so they start arranging themselves in different ways exactly,

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<v Speaker 1>And so you have to understand it from the microscopic

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<v Speaker 1>You say, well, what's the dominant force? And just like

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<v Speaker 1>you said, when things get cold with the dominant force,

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<v Speaker 1>is this crystal structure of the atoms that are holding

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<v Speaker 1>them together. And after that, the dominant energetic contribution is

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<v Speaker 1>the kinetic energy of the objects. But there's still some bonds, right,

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<v Speaker 1>the bonds between atoms and a liquid or what give

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<v Speaker 1>you things like surface pressure and constant volume and stuff.

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<v Speaker 1>And so you have to understand, like what are the

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<v Speaker 1>dominant forces and how are they playing together? And so

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<v Speaker 1>you take these little atoms and you try to think

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<v Speaker 1>what are their emergent properties. And this is a really

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<v Speaker 1>hard thing to do, to go from the microscopic like

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<v Speaker 1>I have a few little particles to understanding the whole thing.

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<v Speaker 1>It's like why hurricanes are difficult. You know, we understand

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<v Speaker 1>how particles of water move through the atmosphere, it's not hard,

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<v Speaker 1>But how do you understand ten trillion of them swirling

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<v Speaker 1>around in really complex situations? So this kind of theory

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<v Speaker 1>is very difficult. And Bows and Einstein we're playing around

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<v Speaker 1>with the math and they figured out a new phase.

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<v Speaker 1>They're like, oh, here's a way if you arrange the

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<v Speaker 1>particles in this special way, you can get completely different

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<v Speaker 1>behavior from anything we've seen. Well, I guess you're saying

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<v Speaker 1>it's sort of like an emergent property that means that

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<v Speaker 1>it's like how they all behave collectively, and you're saying

0:12:31.600 --> 0:12:33.800
<v Speaker 1>that it doesn't you know, like you can't talk about

0:12:34.080 --> 0:12:36.920
<v Speaker 1>one atom being solid, liquid or gas, right, you have

0:12:36.960 --> 0:12:39.160
<v Speaker 1>to talk about like a collection of them, That's right.

0:12:39.160 --> 0:12:41.559
<v Speaker 1>You have to talk about the state of like many particles,

0:12:41.880 --> 0:12:44.160
<v Speaker 1>you know. I think about physics sort of like in layers. Right,

0:12:44.160 --> 0:12:47.319
<v Speaker 1>we have rules for how the solar system operates, and

0:12:47.360 --> 0:12:49.840
<v Speaker 1>we think about the planets as like an individual blob.

0:12:50.120 --> 0:12:52.959
<v Speaker 1>But then we also have rules for how winds move

0:12:53.040 --> 0:12:55.880
<v Speaker 1>and fluid dynamics, and then we have on another layer

0:12:55.920 --> 0:12:59.120
<v Speaker 1>we have rules for individual particles, and then deeper down

0:12:59.160 --> 0:13:01.560
<v Speaker 1>we have rules for like how the quarks move inside

0:13:01.559 --> 0:13:04.200
<v Speaker 1>those particles. That in principle, all you need to know

0:13:04.360 --> 0:13:08.160
<v Speaker 1>is the sort of lowest level stuff, the tiniest particles.

0:13:08.200 --> 0:13:12.960
<v Speaker 1>Those really do determine everything else. But in practice it's hard.

0:13:13.040 --> 0:13:15.360
<v Speaker 1>It's a hard way to do stuff, Like it's hard

0:13:15.360 --> 0:13:18.400
<v Speaker 1>to predict how a hurricane works, even if you understand

0:13:18.520 --> 0:13:21.800
<v Speaker 1>wind and water. And the amazing thing is how much

0:13:21.880 --> 0:13:26.160
<v Speaker 1>interesting stuff you discover that's not fundamental like tiny particles,

0:13:26.160 --> 0:13:29.640
<v Speaker 1>but comes out at the higher levels like hurricanes, And

0:13:29.720 --> 0:13:33.240
<v Speaker 1>this stuff can be simply described by new laws of

0:13:33.280 --> 0:13:36.240
<v Speaker 1>physics that work at that higher level, Like you don't

0:13:36.280 --> 0:13:39.480
<v Speaker 1>need to know about particles to understand how cannonball flies,

0:13:39.520 --> 0:13:42.440
<v Speaker 1>and have a math formula that describes it. And that's

0:13:42.480 --> 0:13:47.719
<v Speaker 1>why phases of matter are super fascinating, not because they're fundamental,

0:13:47.920 --> 0:13:51.679
<v Speaker 1>but because they emerge. All right, So then Einstein got

0:13:51.720 --> 0:13:55.240
<v Speaker 1>together with this scientist called Bows and they hung out

0:13:55.280 --> 0:13:57.160
<v Speaker 1>and worked out the math together. Or how did they

0:13:57.240 --> 0:13:59.640
<v Speaker 1>work together? I think Bo's actually worked out the basic

0:13:59.720 --> 0:14:03.080
<v Speaker 1>idea at first, and then Einstein reads paper and extended it,

0:14:03.440 --> 0:14:06.240
<v Speaker 1>and the result was this prediction that if you took

0:14:06.280 --> 0:14:08.839
<v Speaker 1>atoms and you made them not super hot like you

0:14:08.840 --> 0:14:11.880
<v Speaker 1>would need to get a plasma, but super duper duper cold,

0:14:12.400 --> 0:14:15.480
<v Speaker 1>then they would do something really interesting, but only if

0:14:15.520 --> 0:14:18.200
<v Speaker 1>there were a certain kind of particle, a particle called

0:14:18.240 --> 0:14:21.120
<v Speaker 1>a boson. Oh. I see, so this is not about atoms.

0:14:21.120 --> 0:14:25.200
<v Speaker 1>It's more like when we're talking about particular particles. Well,

0:14:25.200 --> 0:14:27.840
<v Speaker 1>there's two kinds of particles. There are fermions and there

0:14:27.840 --> 0:14:31.000
<v Speaker 1>are bosons. Fermions are particles that have a certain kind

0:14:31.040 --> 0:14:33.560
<v Speaker 1>of spin half an integer that can have spin one

0:14:33.600 --> 0:14:36.560
<v Speaker 1>half or minus one half, and bosons are particles that

0:14:36.640 --> 0:14:38.640
<v Speaker 1>have spin that are an integer. So they can have

0:14:38.680 --> 0:14:41.680
<v Speaker 1>spin like one zero or minus one. Now that's not

0:14:41.720 --> 0:14:44.400
<v Speaker 1>really a big deal, it doesn't really matter. But every atom,

0:14:44.440 --> 0:14:47.200
<v Speaker 1>for example, is either a fermion or boson depending on

0:14:47.480 --> 0:14:49.840
<v Speaker 1>how you build it up out of the little particles.

0:14:49.880 --> 0:14:53.440
<v Speaker 1>So for example, rubidium is a boson because of the

0:14:53.480 --> 0:14:57.160
<v Speaker 1>particles it's made out of. You can also have fermionic atoms. Oh,

0:14:57.440 --> 0:15:01.440
<v Speaker 1>what are electrons? But are electron? Electrons are emions, and

0:15:01.600 --> 0:15:05.000
<v Speaker 1>quarks are bosons. Right, Electrons are fermions and quarks are fermions.

0:15:05.400 --> 0:15:08.480
<v Speaker 1>At the particle level, the smallest level, all of the

0:15:08.520 --> 0:15:14.800
<v Speaker 1>matter particles quarks and leptons are fermions, while the force particles, photons, etcetera.

0:15:14.880 --> 0:15:19.560
<v Speaker 1>Are bosons. But you can combine fermions together to make boson.

0:15:19.680 --> 0:15:23.920
<v Speaker 1>So like two electrons together can make a bosonic pair

0:15:24.200 --> 0:15:26.360
<v Speaker 1>because the one has can add up to an integer.

0:15:26.920 --> 0:15:29.920
<v Speaker 1>And that's why, for example, you can make bosons out

0:15:29.920 --> 0:15:33.840
<v Speaker 1>of fermions. Some really complicated spin arithmetic there that we

0:15:33.840 --> 0:15:36.000
<v Speaker 1>probably don't want to get into. And vocabulary. I feel

0:15:36.000 --> 0:15:40.160
<v Speaker 1>like you're confusing me with vocabulary again, Daniel. But like Higgs,

0:15:40.200 --> 0:15:42.400
<v Speaker 1>boson then is made out of other things, or is

0:15:42.440 --> 0:15:44.920
<v Speaker 1>the higgs boson and boson bosons don't have to be

0:15:45.040 --> 0:15:47.640
<v Speaker 1>made the fermions. They can be fundamental like the higgs,

0:15:47.680 --> 0:15:50.560
<v Speaker 1>but all the force particles like the higgs, boson, the photon,

0:15:50.640 --> 0:15:54.840
<v Speaker 1>the w d z fundamentally are boson. But fermions can

0:15:54.880 --> 0:15:59.560
<v Speaker 1>get together and become like boson. Yes, absolutely, you can

0:15:59.640 --> 0:16:03.640
<v Speaker 1>combine find the half spin lego pieces to make integer

0:16:03.680 --> 0:16:06.360
<v Speaker 1>spin pieces. I see, but they have to come in

0:16:06.440 --> 0:16:08.760
<v Speaker 1>like in pairs. I guess right, Yeah, you have to

0:16:08.800 --> 0:16:10.440
<v Speaker 1>combine them the right way. So does it have to

0:16:10.440 --> 0:16:12.480
<v Speaker 1>do with like if the atom has an even number

0:16:12.520 --> 0:16:17.880
<v Speaker 1>of electrons or yes, exactly, so you can make bosons,

0:16:18.000 --> 0:16:20.640
<v Speaker 1>you can make fermions. Every atom can be fermions, you

0:16:20.680 --> 0:16:24.240
<v Speaker 1>can have bosons, etcetera. But there's an important difference because

0:16:24.280 --> 0:16:28.200
<v Speaker 1>bosons can do something that fermions cannot do, which is

0:16:28.280 --> 0:16:31.360
<v Speaker 1>hang out together. You're saying, yes, they can hang out together.

0:16:31.400 --> 0:16:35.640
<v Speaker 1>So fermions, for a reason that nobody really understands, can

0:16:35.720 --> 0:16:39.120
<v Speaker 1>never share a quantum state. Like that's the reason why

0:16:39.280 --> 0:16:42.640
<v Speaker 1>electrons which are fermions don't all lie in the ground

0:16:42.720 --> 0:16:44.720
<v Speaker 1>state of an atom, like you have an atom with

0:16:44.760 --> 0:16:47.120
<v Speaker 1>ten electrons in it. They don't all just lie in

0:16:47.160 --> 0:16:50.240
<v Speaker 1>the lowest energy level. They stack on top of each other.

0:16:50.400 --> 0:16:52.560
<v Speaker 1>The energy levels are a ladder. You can only have

0:16:52.680 --> 0:16:56.360
<v Speaker 1>one electron per layer of the ladder because their fermions

0:16:56.360 --> 0:16:59.400
<v Speaker 1>bosons are happy to all hang out at the bottom

0:16:59.480 --> 0:17:02.560
<v Speaker 1>level in the nuts. In many configurations, like you can

0:17:02.600 --> 0:17:04.680
<v Speaker 1>have a laser, which is a bunch of photons which

0:17:04.680 --> 0:17:07.840
<v Speaker 1>are bosons, all in the same quantum states. And so

0:17:08.160 --> 0:17:12.240
<v Speaker 1>we have two kinds of particles, bosons and fermions. And

0:17:12.480 --> 0:17:16.000
<v Speaker 1>we understand sort of mathematically why this happens. It emerges

0:17:16.359 --> 0:17:18.840
<v Speaker 1>from the math, but we don't really fundamentally and tutially

0:17:18.920 --> 0:17:21.800
<v Speaker 1>understand why bosons can all hang out in the same

0:17:21.800 --> 0:17:25.280
<v Speaker 1>state and formons just will not Like this, this famous

0:17:25.280 --> 0:17:28.000
<v Speaker 1>story about how somebody asked Fineman he find me, can

0:17:28.040 --> 0:17:31.560
<v Speaker 1>you explain this to us why bosons can all hang

0:17:31.560 --> 0:17:34.119
<v Speaker 1>out in the same state and formons can't. And he

0:17:34.160 --> 0:17:35.960
<v Speaker 1>came back and he said, you know, I don't have

0:17:36.000 --> 0:17:39.120
<v Speaker 1>an explanation that I can use on like eighteen year olds,

0:17:39.160 --> 0:17:42.520
<v Speaker 1>which means I don't really understand it. That's right. He's

0:17:43.040 --> 0:17:47.760
<v Speaker 1>famous for saying nobody understands quantum physics, right, yeah, exactly,

0:17:48.200 --> 0:17:50.520
<v Speaker 1>and you know it does come out of the mathematics,

0:17:50.520 --> 0:17:52.840
<v Speaker 1>but we don't intuitively understand it. It's just a weird

0:17:52.920 --> 0:17:56.359
<v Speaker 1>fact about the universe. But it means that if you

0:17:56.440 --> 0:18:00.119
<v Speaker 1>put a bunch of Boson particles together, they can in

0:18:00.440 --> 0:18:04.879
<v Speaker 1>all hang out in the coldest, lowest quantum state, and

0:18:04.960 --> 0:18:08.840
<v Speaker 1>that is the Einstein bos concit. Yes, so they predicted

0:18:08.840 --> 0:18:10.920
<v Speaker 1>that if you get a bunch of these particles together

0:18:11.119 --> 0:18:13.480
<v Speaker 1>and you get them really cold, they can all be

0:18:13.520 --> 0:18:16.680
<v Speaker 1>in the same quantum state. And then something really weird

0:18:16.720 --> 0:18:20.080
<v Speaker 1>would happen that because they would be so close together

0:18:20.480 --> 0:18:25.640
<v Speaker 1>and so cold that the size of their quantum wavelength

0:18:25.960 --> 0:18:28.600
<v Speaker 1>would be larger than the distance between them, and so

0:18:28.640 --> 0:18:31.680
<v Speaker 1>they would basically merge and all have the same quantum

0:18:31.720 --> 0:18:35.320
<v Speaker 1>state and act like one big quantum particle. Alright, cool,

0:18:35.440 --> 0:18:37.640
<v Speaker 1>let's get into it a little bit more and how

0:18:37.680 --> 0:18:40.600
<v Speaker 1>that all works. But first let's take a quick break.

0:18:53.200 --> 0:18:56.320
<v Speaker 1>All right, we're talking about the Bose Einstein condensate, and

0:18:56.359 --> 0:18:59.159
<v Speaker 1>you're saying that it's related to this idea that bosons

0:18:59.280 --> 0:19:01.399
<v Speaker 1>can hang out to other and they can share a

0:19:01.480 --> 0:19:04.760
<v Speaker 1>quantum state. I guess maybe some people might be wondering

0:19:04.920 --> 0:19:07.280
<v Speaker 1>what does that mean, Like they're sharing a quantum state.

0:19:07.320 --> 0:19:09.640
<v Speaker 1>Does that mean that they have all the same quantum

0:19:09.680 --> 0:19:12.240
<v Speaker 1>properties and are sitting in the same spot. It means

0:19:12.240 --> 0:19:13.800
<v Speaker 1>that they sit on top of each other. They can

0:19:13.840 --> 0:19:16.040
<v Speaker 1>be in the same location and they can share all

0:19:16.040 --> 0:19:19.280
<v Speaker 1>the same quantum properties. And this is really interesting because

0:19:19.520 --> 0:19:22.639
<v Speaker 1>usually you have just one particle in a quantum state,

0:19:23.000 --> 0:19:25.080
<v Speaker 1>and you know, we know the quantum state is sort

0:19:25.080 --> 0:19:28.440
<v Speaker 1>of a thing that controls what happens to one particle.

0:19:28.640 --> 0:19:30.520
<v Speaker 1>It's like a list of all the possibilities for what

0:19:30.720 --> 0:19:33.280
<v Speaker 1>that particle can do. But since you only ever have

0:19:33.400 --> 0:19:35.760
<v Speaker 1>one particle in a quantum state, you don't really see

0:19:35.800 --> 0:19:39.000
<v Speaker 1>the full distribution. But if you have a bunch of

0:19:39.040 --> 0:19:42.479
<v Speaker 1>particles and they're all in that same one quantum state,

0:19:43.040 --> 0:19:45.199
<v Speaker 1>then you can see sort of the whole distribution. You

0:19:45.200 --> 0:19:48.840
<v Speaker 1>can like physically look at this thing and see, oh,

0:19:48.880 --> 0:19:51.960
<v Speaker 1>here's the distribution of all the possible things that could

0:19:52.000 --> 0:19:54.919
<v Speaker 1>happen to this particle. Because you have ten million particles

0:19:54.960 --> 0:19:57.239
<v Speaker 1>and they're all in the same quantum states, you get

0:19:57.280 --> 0:19:59.879
<v Speaker 1>to see sort of all the outcomes at once. A

0:20:00.119 --> 0:20:01.960
<v Speaker 1>only if there are boson. Only if there are boson

0:20:02.040 --> 0:20:04.800
<v Speaker 1>because only bosons can do this. Permons can only have

0:20:04.880 --> 0:20:08.040
<v Speaker 1>one particle per quantum state. Bosons you can have any

0:20:08.160 --> 0:20:11.399
<v Speaker 1>number of particles all in the lowest quantum state. Now,

0:20:11.560 --> 0:20:13.280
<v Speaker 1>how do you get a bunch of particles in the

0:20:13.400 --> 0:20:16.239
<v Speaker 1>same quantum state. Well, the only way really to do

0:20:16.280 --> 0:20:18.960
<v Speaker 1>that is to push them up against the wall of temperature.

0:20:19.280 --> 0:20:20.800
<v Speaker 1>But you can't get them all in the same quantum

0:20:20.840 --> 0:20:23.280
<v Speaker 1>state if they're at two hundred degrees because there's a

0:20:23.280 --> 0:20:25.760
<v Speaker 1>billion different quantum states. So what you do is you

0:20:25.840 --> 0:20:29.399
<v Speaker 1>make them really really cold, so there's only one of

0:20:29.480 --> 0:20:32.280
<v Speaker 1>state available to them, the lowest one, and then they

0:20:32.320 --> 0:20:35.159
<v Speaker 1>all pile up in that quantum state. And Einstein and

0:20:35.200 --> 0:20:37.480
<v Speaker 1>Bows predicted that if you did that, you would get

0:20:37.520 --> 0:20:41.480
<v Speaker 1>this blob where the particles sort of lose their individuality.

0:20:41.560 --> 0:20:45.240
<v Speaker 1>They become a macroscopically size like you could see it

0:20:45.720 --> 0:20:48.960
<v Speaker 1>quantum mechanically behaving conject I guess maybe I'm getting tripped

0:20:49.000 --> 0:20:51.760
<v Speaker 1>up because I'm thinking of these things as particles. It's

0:20:51.840 --> 0:20:54.400
<v Speaker 1>like little things. But maybe you know, if you think

0:20:54.440 --> 0:20:57.000
<v Speaker 1>of them as waves, then it maybe makes more sense.

0:20:57.080 --> 0:20:59.879
<v Speaker 1>Like you know, fermions, you can't have a wave on

0:21:00.040 --> 0:21:02.800
<v Speaker 1>top of another wave, but bosons they're happy to stack

0:21:02.880 --> 0:21:05.360
<v Speaker 1>together as waves. It's that kind of what you're saying. Yeah,

0:21:05.400 --> 0:21:07.320
<v Speaker 1>And every time you think about these things, you should

0:21:07.359 --> 0:21:10.520
<v Speaker 1>not be thinking about a tiny, little spinning ball of matter, right,

0:21:10.560 --> 0:21:13.680
<v Speaker 1>because that's not what they are. They're weird quantum mechanical objects.

0:21:14.000 --> 0:21:16.720
<v Speaker 1>And the intuition you usually have about how a particle,

0:21:16.760 --> 0:21:20.239
<v Speaker 1>a little thing moves through space doesn't work. But you're right,

0:21:20.280 --> 0:21:23.040
<v Speaker 1>and you can apply that intuition to the waves because

0:21:23.040 --> 0:21:26.520
<v Speaker 1>the waves follow all those rules, like waves are deterministic

0:21:26.560 --> 0:21:29.919
<v Speaker 1>and their future can be predicted and actually move through space.

0:21:30.040 --> 0:21:32.960
<v Speaker 1>So yes, you can imagine all those bosonic waves sort

0:21:32.960 --> 0:21:34.760
<v Speaker 1>of stacking on top of each other. They're all doing

0:21:34.760 --> 0:21:37.760
<v Speaker 1>the same thing, right, whereas like a fermion, a bunch

0:21:37.760 --> 0:21:40.400
<v Speaker 1>of waves, they would all sort of avoid each other. Yeah, exactly,

0:21:40.440 --> 0:21:42.720
<v Speaker 1>like droplets that repel each other. Yeah, or sort of

0:21:42.760 --> 0:21:45.000
<v Speaker 1>like a game of connect for you know, you slide

0:21:45.040 --> 0:21:47.240
<v Speaker 1>the pieces in and they stack on top of each other,

0:21:47.600 --> 0:21:49.320
<v Speaker 1>and once you got one in a slot, you can't

0:21:49.359 --> 0:21:51.399
<v Speaker 1>get another one in a slot, whereas boson is that

0:21:51.520 --> 0:21:53.639
<v Speaker 1>just like slide right past each other, and they're all

0:21:53.680 --> 0:21:56.320
<v Speaker 1>happy to go down to the very lowest level. So

0:21:56.359 --> 0:21:58.880
<v Speaker 1>you couldn't play connect forward with bosons, they all stack

0:21:58.920 --> 0:22:01.720
<v Speaker 1>at the bottom. That would be a hard game to win.

0:22:01.800 --> 0:22:05.120
<v Speaker 1>There's right, unless it's connect one, in which case it's

0:22:05.160 --> 0:22:08.680
<v Speaker 1>over instantly, all right. So einstand and bos figured out

0:22:08.680 --> 0:22:11.080
<v Speaker 1>that if you cool atoms, you make them cold enough,

0:22:11.359 --> 0:22:14.879
<v Speaker 1>then with bosons then they all sort of like merge

0:22:14.920 --> 0:22:17.280
<v Speaker 1>together all their wave functions. I think you were telling

0:22:17.280 --> 0:22:20.120
<v Speaker 1>me that, like you go over some threshold, like their

0:22:20.240 --> 0:22:23.520
<v Speaker 1>quantum wave functions starts to overlap. The key thing is

0:22:23.560 --> 0:22:26.320
<v Speaker 1>to get them so cold. That's the size of their

0:22:26.359 --> 0:22:29.440
<v Speaker 1>wave function. The thing that controls where they are is

0:22:29.480 --> 0:22:33.440
<v Speaker 1>about the same as the mean difference in the spacing

0:22:33.520 --> 0:22:36.760
<v Speaker 1>between them, so that their wave functions actually overlaps. And

0:22:36.760 --> 0:22:38.840
<v Speaker 1>you have like atom number one over here and I'm

0:22:38.920 --> 0:22:41.199
<v Speaker 1>number two over there. They're not literally on top of

0:22:41.240 --> 0:22:44.560
<v Speaker 1>each other, but their wave functions are now over and

0:22:44.600 --> 0:22:46.000
<v Speaker 1>the more you can get them on top of each

0:22:46.040 --> 0:22:48.760
<v Speaker 1>other the better. But there's this sort of threshold where

0:22:48.760 --> 0:22:51.680
<v Speaker 1>their wave functions are now overlapping. And they think that's

0:22:51.680 --> 0:22:54.440
<v Speaker 1>when the faith transition occurs, and you get this new

0:22:54.480 --> 0:22:57.880
<v Speaker 1>weird kind of blob that should behave differently, and we'll

0:22:58.040 --> 0:23:00.399
<v Speaker 1>they can do exactly what this thing can do, but

0:23:00.440 --> 0:23:04.760
<v Speaker 1>it should behave differently than liquids or gases or solid Oh.

0:23:04.800 --> 0:23:07.520
<v Speaker 1>I see, it's kind of like normally the particles or

0:23:07.560 --> 0:23:09.960
<v Speaker 1>the atoms are are bouncing around, they're moving too fast,

0:23:10.080 --> 0:23:12.320
<v Speaker 1>really far apart from each other. But once you cool it,

0:23:12.440 --> 0:23:15.640
<v Speaker 1>they start to come together and at some point their

0:23:15.680 --> 0:23:19.280
<v Speaker 1>wave functions overlap. They synchronize. I guess is a good

0:23:19.280 --> 0:23:22.040
<v Speaker 1>way to put it. Yeah, they synchronize. They all follow

0:23:22.080 --> 0:23:24.760
<v Speaker 1>the same rules, they're all in the same state. They

0:23:24.760 --> 0:23:27.840
<v Speaker 1>can have different actual outcomes because remember there's still a

0:23:27.920 --> 0:23:30.680
<v Speaker 1>random element there, but they all have the same wave functions.

0:23:30.720 --> 0:23:34.760
<v Speaker 1>They're all determined by the same fundamental and dynamics. Wait,

0:23:34.880 --> 0:23:38.080
<v Speaker 1>there's like one overall wave function that sort of controls

0:23:38.119 --> 0:23:39.800
<v Speaker 1>all of them. Yeah, that's right. And you know, there's

0:23:39.840 --> 0:23:42.439
<v Speaker 1>nothing stopping you from writing a wave function down for

0:23:42.480 --> 0:23:44.720
<v Speaker 1>two particles that have nothing to do with each other.

0:23:45.040 --> 0:23:47.480
<v Speaker 1>But those way functions factorized. It's just like a product

0:23:47.560 --> 0:23:50.320
<v Speaker 1>of the two. But when they overlap, when they synchronize,

0:23:50.359 --> 0:23:52.439
<v Speaker 1>like you said, then you have a single wave function

0:23:52.480 --> 0:23:55.480
<v Speaker 1>that describes both particles. And so if you get a

0:23:55.480 --> 0:23:57.919
<v Speaker 1>bunch of particles you cool them, they will start to

0:23:58.000 --> 0:24:00.680
<v Speaker 1>overlap and suddenly it's like you have a giant article. Right,

0:24:00.720 --> 0:24:03.200
<v Speaker 1>that's kind of the idea, and that's they're all sort

0:24:03.240 --> 0:24:06.360
<v Speaker 1>of like moving together, but they're not really moving, they're

0:24:06.400 --> 0:24:10.200
<v Speaker 1>just sort of existing in a quantum way together. Yes,

0:24:10.280 --> 0:24:12.720
<v Speaker 1>and then together they can do quantum things that you

0:24:12.840 --> 0:24:16.880
<v Speaker 1>usually can only see on tiny microscopic particles. But now

0:24:16.960 --> 0:24:20.800
<v Speaker 1>you can see a giant, millimeter sized blob doing these

0:24:20.880 --> 0:24:24.640
<v Speaker 1>quantum things. A giant, like a millimeter sized quantum object.

0:24:24.720 --> 0:24:27.879
<v Speaker 1>That's yes, huge, that's huge. Yeah, I mean in a

0:24:27.960 --> 0:24:31.840
<v Speaker 1>literal and also significance. And it's not like it has

0:24:31.960 --> 0:24:35.160
<v Speaker 1>great you know, military applications or it's going to revolutionize

0:24:35.160 --> 0:24:37.600
<v Speaker 1>the Internet. You're not going to see like Bose Einstein

0:24:37.640 --> 0:24:41.119
<v Speaker 1>computing or whatever. It's mostly just cool, like, can we

0:24:41.160 --> 0:24:44.199
<v Speaker 1>make a new weird kind of Google, especially one that

0:24:44.320 --> 0:24:47.560
<v Speaker 1>reveals the fundamental quantum nature of the universe in a

0:24:47.600 --> 0:24:51.800
<v Speaker 1>way that's just totally unambiguous and observable. I guess because

0:24:51.800 --> 0:24:54.000
<v Speaker 1>you can look at it. Yeah, people like to see stuff,

0:24:54.040 --> 0:24:56.480
<v Speaker 1>and so here this is quantum mechanics you can see,

0:24:56.760 --> 0:24:58.439
<v Speaker 1>and so what kind of weird stuff can it do?

0:24:58.520 --> 0:25:04.040
<v Speaker 1>Can it's like teleport or well, it can interfere. So

0:25:04.119 --> 0:25:07.160
<v Speaker 1>you can have like two of these things with different

0:25:07.200 --> 0:25:09.760
<v Speaker 1>way functions, and then you sort of overlap them and

0:25:09.800 --> 0:25:13.240
<v Speaker 1>you see an interference pattern. Like rather than having a

0:25:13.280 --> 0:25:15.720
<v Speaker 1>single particle and it's got a probability going here or there,

0:25:15.960 --> 0:25:18.880
<v Speaker 1>you get these waves in the blob, You get these

0:25:19.000 --> 0:25:21.639
<v Speaker 1>interference patterns, these patterns of dark and light in the

0:25:21.720 --> 0:25:25.840
<v Speaker 1>single blob, and you can do quantum mechanical tunneling. Yeah,

0:25:25.840 --> 0:25:28.920
<v Speaker 1>that's what I mean by teleporting is that they can

0:25:28.960 --> 0:25:32.240
<v Speaker 1>cross impossible barrier. A single particle can have a way

0:25:32.240 --> 0:25:35.280
<v Speaker 1>function that exists on both sides of a barrier, right

0:25:35.560 --> 0:25:38.760
<v Speaker 1>like in a potential well, and across a barrier to

0:25:38.840 --> 0:25:40.919
<v Speaker 1>the other side of the well. So it can't be

0:25:41.000 --> 0:25:42.919
<v Speaker 1>in between, but has a possibility to be on the

0:25:43.000 --> 0:25:45.280
<v Speaker 1>left and the right. We did a whole fun podcast

0:25:45.320 --> 0:25:48.520
<v Speaker 1>episode about quantum tunneling and the reason that that can

0:25:48.600 --> 0:25:50.680
<v Speaker 1>happen is that the particle has a probability to be

0:25:50.720 --> 0:25:52.720
<v Speaker 1>on the left and the probability to be on the right.

0:25:52.880 --> 0:25:56.159
<v Speaker 1>And particles aren't limited to classical paths. They don't have

0:25:56.240 --> 0:25:58.680
<v Speaker 1>to go from where they were to where they are.

0:25:58.960 --> 0:26:01.480
<v Speaker 1>They just have these snap shots. So if your probability

0:26:01.480 --> 0:26:03.560
<v Speaker 1>to be on the left and then on the right later.

0:26:03.880 --> 0:26:06.119
<v Speaker 1>That's no problem. You can do that. That's quantum tunnel.

0:26:06.119 --> 0:26:08.159
<v Speaker 1>And so that's why would happen with the blob. It

0:26:08.160 --> 0:26:10.920
<v Speaker 1>would suddenly appear on the other side of a wall. Yeah,

0:26:11.080 --> 0:26:12.600
<v Speaker 1>you can have part of the blob on the left

0:26:12.600 --> 0:26:14.520
<v Speaker 1>and then suddenly have part of the blob on the right,

0:26:14.840 --> 0:26:18.000
<v Speaker 1>even though it can't go in between. So it can teleport.

0:26:18.200 --> 0:26:22.960
<v Speaker 1>So we can do weird. Yeah, quantum teleportation. Sure, So

0:26:23.040 --> 0:26:25.160
<v Speaker 1>you just have to be cool and you can teleport

0:26:26.119 --> 0:26:29.640
<v Speaker 1>super duper cool like nano cool. All right, And are

0:26:29.680 --> 0:26:33.119
<v Speaker 1>there any other interesting things that can do or interesting

0:26:33.119 --> 0:26:35.400
<v Speaker 1>applications we can use these for. Well, we talked about

0:26:35.440 --> 0:26:38.080
<v Speaker 1>this once that you can do weird stuff to light.

0:26:38.280 --> 0:26:41.840
<v Speaker 1>Bose Einstein condensate, because of its weird properties, can slow

0:26:41.880 --> 0:26:45.720
<v Speaker 1>down light to like the speed of a bicycle. Usually

0:26:45.800 --> 0:26:49.080
<v Speaker 1>light travels, you know, three hundred million meters per second,

0:26:49.760 --> 0:26:52.240
<v Speaker 1>but you can slow down light if it goes into

0:26:52.280 --> 0:26:55.480
<v Speaker 1>various media and boze Einstein content sates can slow it

0:26:55.520 --> 0:26:58.120
<v Speaker 1>down to like the speed of somebody riding a bicycle.

0:26:58.480 --> 0:27:00.600
<v Speaker 1>And there's a group of Harvor that even was able

0:27:00.640 --> 0:27:04.440
<v Speaker 1>to stop light inside of Bose Einstein condensate. Right, Yeah,

0:27:04.480 --> 0:27:07.439
<v Speaker 1>we talked about light going in and then bouncing around

0:27:07.720 --> 0:27:10.520
<v Speaker 1>kind of or interacting with the Bose Einstein concert and

0:27:10.680 --> 0:27:14.000
<v Speaker 1>essentially slowing down light. Yeah, slowing down light or even

0:27:14.000 --> 0:27:16.320
<v Speaker 1>stopping it. Like they can have a laser pulse go

0:27:16.440 --> 0:27:19.080
<v Speaker 1>into the Bose Einstein condensate and then they can just

0:27:19.160 --> 0:27:21.040
<v Speaker 1>wait and they can move it somewhere else and then

0:27:21.080 --> 0:27:24.000
<v Speaker 1>they can have it re emit the exact same laser pulse.

0:27:24.680 --> 0:27:27.200
<v Speaker 1>So that's kind of cool. They're working on using Bose

0:27:27.240 --> 0:27:30.480
<v Speaker 1>Einstein condensates to build an atom laser. So usually you

0:27:30.520 --> 0:27:33.399
<v Speaker 1>have a laser made of photons, right, You're shooting beams

0:27:33.400 --> 0:27:36.800
<v Speaker 1>of light made of tiny little photons. But people are

0:27:36.840 --> 0:27:40.120
<v Speaker 1>interested in shooting beams of atoms, atoms that are all

0:27:40.160 --> 0:27:42.840
<v Speaker 1>in the same quantum state, and that can do the

0:27:42.880 --> 0:27:45.360
<v Speaker 1>same kind of thing as a laser, like enhance and

0:27:45.600 --> 0:27:47.840
<v Speaker 1>resonate with each other. And it has all sorts of

0:27:47.840 --> 0:27:51.119
<v Speaker 1>weird applications. Plus it just seems kind of cool. And

0:27:51.280 --> 0:27:55.080
<v Speaker 1>so people are building atom lasers using Boze Einstein condensates.

0:27:55.119 --> 0:27:58.240
<v Speaker 1>That is a really weird thing that matter can do. Right,

0:27:58.280 --> 0:28:00.359
<v Speaker 1>I guess it's all because of quantum acount. It's like

0:28:00.880 --> 0:28:04.640
<v Speaker 1>you know, solid gas, liquid plasma. Those you can sort

0:28:04.640 --> 0:28:09.119
<v Speaker 1>of imagine from classical physics, right, but this one is

0:28:09.160 --> 0:28:12.199
<v Speaker 1>like a very unique quantum state of matter. Yeah, this

0:28:12.280 --> 0:28:15.720
<v Speaker 1>one you couldn't do if matter really was tiny little

0:28:15.760 --> 0:28:19.639
<v Speaker 1>classical balls. So you really need a microscopic quantum understanding

0:28:19.800 --> 0:28:21.520
<v Speaker 1>to make any sense of this. And it's sort of

0:28:21.560 --> 0:28:24.399
<v Speaker 1>awesome that they just use the map to predict it, right,

0:28:24.440 --> 0:28:26.960
<v Speaker 1>to say, like, oh, here's how we think this should work.

0:28:27.000 --> 0:28:29.199
<v Speaker 1>I'm really in all of those kinds of accomplishment. This

0:28:29.280 --> 0:28:31.879
<v Speaker 1>is a really interesting story. And so let's get into that.

0:28:32.119 --> 0:28:35.439
<v Speaker 1>Einstein and Bows figured out this possible quantum state of

0:28:35.440 --> 0:28:39.560
<v Speaker 1>matter and then it took seventy years to actually sort

0:28:39.560 --> 0:28:42.280
<v Speaker 1>of do it. Yeah, it took seventy years. And the

0:28:42.360 --> 0:28:44.360
<v Speaker 1>reason is that they knew it had to be really,

0:28:44.400 --> 0:28:48.800
<v Speaker 1>really cold. And so this basically just traces the technology

0:28:48.840 --> 0:28:52.400
<v Speaker 1>available to make stuff super duper cold. A story of

0:28:52.440 --> 0:28:55.920
<v Speaker 1>refrigerations what you're saying, Yeah, it's like the race to

0:28:55.960 --> 0:28:57.880
<v Speaker 1>the South Pole in that sense, right, It's a race

0:28:57.920 --> 0:29:01.000
<v Speaker 1>to the bottom of the temperature scale. How call did

0:29:01.000 --> 0:29:02.560
<v Speaker 1>it need to be? It needed to be down to

0:29:02.640 --> 0:29:07.240
<v Speaker 1>like nano kelvin, like really nano kelvins, like zero point

0:29:07.320 --> 0:29:12.880
<v Speaker 1>zero zero zero twelve zeros one kelvin. Yeah, And very

0:29:12.920 --> 0:29:14.800
<v Speaker 1>early on in the race, people were able to do

0:29:14.840 --> 0:29:18.040
<v Speaker 1>stuff like get down to a few degrees kelvin, you know,

0:29:18.120 --> 0:29:20.080
<v Speaker 1>tens of degrees kelvin, and you can do things like

0:29:20.320 --> 0:29:24.360
<v Speaker 1>super fluid helium, which we think now has a small

0:29:24.440 --> 0:29:27.960
<v Speaker 1>element of Bose Einstein condensate in it, but people really

0:29:28.000 --> 0:29:31.520
<v Speaker 1>wanted to get like a pure Bose Einstein condensate something

0:29:31.560 --> 0:29:33.880
<v Speaker 1>where most of the atoms were in that state, so

0:29:33.960 --> 0:29:36.920
<v Speaker 1>it was like unambiguous, and for that to happen, you

0:29:36.920 --> 0:29:39.600
<v Speaker 1>really have to get the whole thing down to really

0:29:39.600 --> 0:29:42.800
<v Speaker 1>really cold temperature, to nano kelvin. And so you're saying

0:29:42.800 --> 0:29:44.720
<v Speaker 1>then that even in the twenties and thirties they could

0:29:44.880 --> 0:29:47.560
<v Speaker 1>go down to a few kelvin, but I guess you

0:29:47.640 --> 0:29:51.400
<v Speaker 1>needed like a super special technology to go even further. Yeah,

0:29:51.440 --> 0:29:54.480
<v Speaker 1>And so fast forward to like the nineties, and people

0:29:54.480 --> 0:29:56.840
<v Speaker 1>have been trying to do this and using various techniques,

0:29:56.880 --> 0:29:59.080
<v Speaker 1>and you know, we had atomic physics and you could

0:29:59.080 --> 0:30:02.400
<v Speaker 1>trap individual a ms and do clever stuff. But people

0:30:02.480 --> 0:30:05.360
<v Speaker 1>were struggling, right, they sort of hit a wall, and

0:30:05.400 --> 0:30:07.400
<v Speaker 1>there was a lab at m I T that was

0:30:07.440 --> 0:30:10.160
<v Speaker 1>trying to use hydrogen. They're like, let's just start with hydrogen.

0:30:10.520 --> 0:30:12.880
<v Speaker 1>And this is Dan Kletner his lab at m I T.

0:30:13.360 --> 0:30:15.200
<v Speaker 1>And he sort of hit a wall in the nineties

0:30:15.480 --> 0:30:18.120
<v Speaker 1>and couldn't really make much more progress. But that's when

0:30:18.160 --> 0:30:21.840
<v Speaker 1>the breakthrough happened. He couldn't teleport to the other side. Yeah.

0:30:22.040 --> 0:30:25.160
<v Speaker 1>Then people made two really big advances, and there's actually

0:30:25.160 --> 0:30:29.280
<v Speaker 1>his students that made these advances. Two advances were laser

0:30:29.360 --> 0:30:34.600
<v Speaker 1>cooling and magnetic evaporation. Is the two technologies that let

0:30:34.640 --> 0:30:38.000
<v Speaker 1>them super cool these atoms down to the levels they

0:30:38.040 --> 0:30:41.640
<v Speaker 1>need to. All great combinations of words that you sound

0:30:41.920 --> 0:30:46.120
<v Speaker 1>impressive in the physics sense, magnetic evaporation and laser cooling.

0:30:46.440 --> 0:30:48.640
<v Speaker 1>All right, let's get into the details of how they

0:30:48.920 --> 0:30:52.520
<v Speaker 1>finally found a Bose Einstein concert and let's talk about

0:30:52.520 --> 0:30:54.480
<v Speaker 1>what awesome things we can do with it. But first

0:30:54.560 --> 0:31:10.080
<v Speaker 1>let's take another quick break. Okay, So there's a raise

0:31:10.200 --> 0:31:14.160
<v Speaker 1>Daniel to get the coldest thing possible so that it

0:31:14.240 --> 0:31:19.400
<v Speaker 1>can snap into the Bose Einstein state of matter, conside,

0:31:20.080 --> 0:31:22.600
<v Speaker 1>and so they figured out how to do magnetic evaporation

0:31:22.880 --> 0:31:24.880
<v Speaker 1>to do that. What does that mean. What that means

0:31:25.080 --> 0:31:27.320
<v Speaker 1>is you have a bunch of atoms and you want

0:31:27.360 --> 0:31:29.440
<v Speaker 1>to get it colder. How do you do that? Well,

0:31:29.960 --> 0:31:32.840
<v Speaker 1>one way is to actually make all the atoms each

0:31:32.920 --> 0:31:36.960
<v Speaker 1>individually slow down. Another way is to just sort of

0:31:37.120 --> 0:31:40.280
<v Speaker 1>take out its kinetic energy. Yeah, because remember temperature is

0:31:40.320 --> 0:31:43.400
<v Speaker 1>basically kinetic energy. The faster these things are moving, the

0:31:43.480 --> 0:31:46.400
<v Speaker 1>hotter the gas is. The Other way to do it

0:31:46.440 --> 0:31:48.920
<v Speaker 1>is to start with a larger sample and then just

0:31:49.080 --> 0:31:52.520
<v Speaker 1>pick out the slower moving ones, like boil off the

0:31:52.600 --> 0:31:55.960
<v Speaker 1>hot parts. Selectively pick out the slow ones. Then you

0:31:56.040 --> 0:31:58.800
<v Speaker 1>end up with somebody which is on average colder than

0:31:58.840 --> 0:32:00.920
<v Speaker 1>what you started, right. That's kind of what happens to

0:32:01.000 --> 0:32:02.760
<v Speaker 1>a glass of water when you leave it out right,

0:32:02.920 --> 0:32:06.040
<v Speaker 1>Like it's actually a little bit cooler than ambient temperature

0:32:06.040 --> 0:32:09.280
<v Speaker 1>because all the hot water atoms fly off. Yeah, I

0:32:09.280 --> 0:32:11.280
<v Speaker 1>think that's true. Where it's sort of like you know,

0:32:11.320 --> 0:32:13.440
<v Speaker 1>say you had a glass of ice water and you

0:32:13.480 --> 0:32:15.720
<v Speaker 1>wanted it colder. Well, one thing you do is put

0:32:15.720 --> 0:32:17.840
<v Speaker 1>it in the freezer and actually cool it all down.

0:32:17.880 --> 0:32:19.840
<v Speaker 1>The other thing is you could just fish the ice

0:32:19.880 --> 0:32:21.520
<v Speaker 1>out of it and be like, oh look now I

0:32:21.560 --> 0:32:24.760
<v Speaker 1>have ice, right, and you just leave the hot parts behind.

0:32:25.040 --> 0:32:28.040
<v Speaker 1>So magnetic evaporations sort of works like that. It says,

0:32:28.320 --> 0:32:31.000
<v Speaker 1>let's just pick out the coldest bits, so start with

0:32:31.040 --> 0:32:34.240
<v Speaker 1>more than your need, right, and has a distribution. Some

0:32:34.400 --> 0:32:36.400
<v Speaker 1>are hot, some are cold, and you pick out the

0:32:36.400 --> 0:32:38.440
<v Speaker 1>cold bits. In the way they do it is they

0:32:38.480 --> 0:32:40.960
<v Speaker 1>put it in a magnetic bowl. So they put it

0:32:40.960 --> 0:32:42.680
<v Speaker 1>in a bowl so that you need to have enough

0:32:42.840 --> 0:32:45.120
<v Speaker 1>energy to get out of the bowl, and you just

0:32:45.200 --> 0:32:47.080
<v Speaker 1>let it sit there for a little while and the

0:32:47.080 --> 0:32:49.320
<v Speaker 1>hot ones will get over the lip of the bowl

0:32:49.440 --> 0:32:51.400
<v Speaker 1>and the cold ones will get stuck in the bottom,

0:32:51.520 --> 0:32:55.200
<v Speaker 1>and eventually you're left with only the cold one. Gradually

0:32:55.240 --> 0:32:57.600
<v Speaker 1>lower the sides of the bowl and so they can

0:32:57.640 --> 0:33:00.160
<v Speaker 1>tune the temperature that they get. Well, so that's one

0:33:00.160 --> 0:33:02.640
<v Speaker 1>way to cool example. And then you also said they

0:33:02.640 --> 0:33:05.360
<v Speaker 1>can use lasers. Yeah, they use lasers. And this is

0:33:05.360 --> 0:33:07.600
<v Speaker 1>sort of mind blowing because you imagine, if you're gonna

0:33:07.600 --> 0:33:10.200
<v Speaker 1>cool something down, you probably shouldn't shoot it with high

0:33:10.320 --> 0:33:13.680
<v Speaker 1>energy lasers, right, So this is really counted to it if.

0:33:13.680 --> 0:33:15.600
<v Speaker 1>I don't know how anybody came up with this idea,

0:33:16.040 --> 0:33:18.160
<v Speaker 1>but the way it works is that you shoot a

0:33:18.240 --> 0:33:20.880
<v Speaker 1>laser at these atoms and you shoot a laser at

0:33:20.880 --> 0:33:25.000
<v Speaker 1>them at just above the energy that they like to absorb. Remember,

0:33:25.160 --> 0:33:28.280
<v Speaker 1>adams can't just absorb any photon. They have to absorb

0:33:28.360 --> 0:33:31.960
<v Speaker 1>photons of certain energies to have this spectrum that they

0:33:31.960 --> 0:33:34.400
<v Speaker 1>can jump up and down to. So they need a

0:33:34.440 --> 0:33:37.360
<v Speaker 1>photon that has exactly the right gap between the energy

0:33:37.400 --> 0:33:39.560
<v Speaker 1>level they're at and the one they can go to.

0:33:40.240 --> 0:33:43.520
<v Speaker 1>So if you shine an arbitrary energy laser through a gas,

0:33:43.600 --> 0:33:46.160
<v Speaker 1>probably won't even absorb anything. You have to sort of

0:33:46.200 --> 0:33:49.800
<v Speaker 1>tune the laser to where the gas likes to drink

0:33:49.840 --> 0:33:53.080
<v Speaker 1>its light. But wouldn't that make it absorbed then the light,

0:33:53.360 --> 0:33:55.680
<v Speaker 1>how does that make it give off energy? So what

0:33:55.720 --> 0:33:58.360
<v Speaker 1>they do is they tune the laser to just above

0:33:59.040 --> 0:34:01.560
<v Speaker 1>where it likes to absorb the light. And what this

0:34:01.640 --> 0:34:05.600
<v Speaker 1>means is that atoms moving towards the laser, we'll see

0:34:05.640 --> 0:34:09.120
<v Speaker 1>the laser doppler shifted. It will change the wavelength of

0:34:09.120 --> 0:34:11.560
<v Speaker 1>the light to be the one that they like to absorb.

0:34:11.960 --> 0:34:15.200
<v Speaker 1>So adams moving towards the laser will preferentially absorb this

0:34:15.280 --> 0:34:18.640
<v Speaker 1>laser light, which will slow them down because they're moving

0:34:18.680 --> 0:34:20.799
<v Speaker 1>towards the laser. So you pick the ones that are

0:34:20.800 --> 0:34:23.440
<v Speaker 1>moving towards the light and you give them a push

0:34:23.680 --> 0:34:26.719
<v Speaker 1>and that basically slows them down a little. And then

0:34:26.760 --> 0:34:29.759
<v Speaker 1>the opposite happens for the atoms going the other way. Yes,

0:34:29.760 --> 0:34:32.160
<v Speaker 1>and so what you do is you shoot laser beams

0:34:32.200 --> 0:34:35.640
<v Speaker 1>at this thing slightly above the wavelength that they should absorb,

0:34:35.960 --> 0:34:38.799
<v Speaker 1>and that preferentially slows down the atoms moving away from

0:34:38.800 --> 0:34:41.279
<v Speaker 1>the center of the block. It's like a quantum hack.

0:34:42.920 --> 0:34:45.920
<v Speaker 1>It's really cool. It's mind blowing. And you know, they

0:34:45.960 --> 0:34:48.160
<v Speaker 1>do absorb this and then they give off the light

0:34:48.440 --> 0:34:50.160
<v Speaker 1>and so they slow back down, but they end up

0:34:50.160 --> 0:34:52.520
<v Speaker 1>going in a different direction. And so you've taken a

0:34:52.560 --> 0:34:56.239
<v Speaker 1>particle which was shooting towards the laser and you've modified

0:34:56.400 --> 0:34:58.720
<v Speaker 1>its angle a little bit, and that in effect slows

0:34:58.760 --> 0:35:01.640
<v Speaker 1>it down because the overall magnitude of its philosophy is

0:35:01.680 --> 0:35:03.879
<v Speaker 1>now smaller. I see. It's kind of like a wall

0:35:03.920 --> 0:35:06.440
<v Speaker 1>that slows and Adam down, but only in one direction. Yeah.

0:35:06.480 --> 0:35:08.680
<v Speaker 1>It's like you've got a bunch of sheep and you've got,

0:35:08.680 --> 0:35:10.239
<v Speaker 1>you know, a dog on each side, and it's like

0:35:10.320 --> 0:35:12.799
<v Speaker 1>finding the single sheep that are running away from the

0:35:12.800 --> 0:35:14.840
<v Speaker 1>herd and sort of like turning them around and pushing

0:35:14.840 --> 0:35:17.040
<v Speaker 1>them back in, and eventually sheep come together and make

0:35:17.080 --> 0:35:23.720
<v Speaker 1>a Bose Einstein content sheep. That's such a bad joke, Danny.

0:35:24.440 --> 0:35:26.560
<v Speaker 1>All right. So the race was on to be the

0:35:26.600 --> 0:35:29.960
<v Speaker 1>coolest physicist on the planet to get the Bose Einstein

0:35:30.000 --> 0:35:32.839
<v Speaker 1>contestant going. And we were at M I T and

0:35:32.880 --> 0:35:36.400
<v Speaker 1>then somebody discovered these two techniques. Yes, so Dan Kleptner

0:35:36.560 --> 0:35:38.520
<v Speaker 1>was doing it at hydrogen with M I T but

0:35:38.560 --> 0:35:41.919
<v Speaker 1>sort of hit a wall. And then his students went

0:35:41.960 --> 0:35:45.200
<v Speaker 1>out to NIST into you See Boulder and they started

0:35:45.200 --> 0:35:48.640
<v Speaker 1>a lab out there. These are Cornell and Wyman. I

0:35:48.680 --> 0:35:51.840
<v Speaker 1>believe it's See You Boulder. Then I just want to

0:35:51.840 --> 0:35:54.399
<v Speaker 1>insult the whole campus as people. Thank you. Yeah, I'm

0:35:54.400 --> 0:35:56.239
<v Speaker 1>biased because I'm at the Universe of Californ in this,

0:35:56.360 --> 0:35:58.680
<v Speaker 1>I think, you see. And they had an idea to

0:35:58.760 --> 0:36:02.279
<v Speaker 1>try heavier out of instead of using hydrogen, which had

0:36:02.280 --> 0:36:05.120
<v Speaker 1>this certain interaction between them that made it hard for

0:36:05.160 --> 0:36:07.279
<v Speaker 1>them to stay in the magnetic trap. They said, well,

0:36:07.320 --> 0:36:10.200
<v Speaker 1>let's use rubidium. Rubidium is still a boson, but it's

0:36:10.239 --> 0:36:14.240
<v Speaker 1>a little heavier. And so people hadn't tried these heavier

0:36:14.280 --> 0:36:18.720
<v Speaker 1>alkali atoms before, and so they made a better magnetic trap,

0:36:19.120 --> 0:36:22.920
<v Speaker 1>and they had this cool idea to use really cheap lasers,

0:36:22.960 --> 0:36:25.160
<v Speaker 1>like other folks were trying to get their lasers to

0:36:25.200 --> 0:36:28.320
<v Speaker 1>work and buying like a hundred and fifty dollar laser systems.

0:36:28.719 --> 0:36:30.399
<v Speaker 1>But you know, this is the era when you could

0:36:30.400 --> 0:36:33.000
<v Speaker 1>buy like a laser for two dollars because they were

0:36:33.040 --> 0:36:36.400
<v Speaker 1>in CD players right in DVD readers, laser pointers and

0:36:36.480 --> 0:36:39.440
<v Speaker 1>laser pointers. So lasers have become really cheap. And they

0:36:39.480 --> 0:36:41.480
<v Speaker 1>figured out a way to use really cheap lasers and

0:36:41.480 --> 0:36:44.279
<v Speaker 1>that combine them in this cool way to make it

0:36:44.360 --> 0:36:47.000
<v Speaker 1>very flexible but very powerful. So there's sort of like

0:36:47.040 --> 0:36:50.600
<v Speaker 1>this experimental cleverness and they were the first ones to

0:36:50.600 --> 0:36:54.320
<v Speaker 1>do it. They combined this magnetic evaporation with this laser

0:36:54.400 --> 0:36:58.280
<v Speaker 1>cooling and it was in that they were able to

0:36:58.400 --> 0:37:01.600
<v Speaker 1>get this thing down to a d seventy nano kelvin

0:37:02.000 --> 0:37:06.080
<v Speaker 1>and they actually saw this Bose Einstein condensate in their device.

0:37:06.600 --> 0:37:08.200
<v Speaker 1>What did it look like like? Does it look like

0:37:08.239 --> 0:37:10.160
<v Speaker 1>a blog? Yeah, it looks like a blog. Can you

0:37:10.200 --> 0:37:12.040
<v Speaker 1>actually see it or is it too small? You can

0:37:12.080 --> 0:37:14.360
<v Speaker 1>actually see it? It looks like a blob. It's like

0:37:14.440 --> 0:37:18.960
<v Speaker 1>millimeters across. It lasted for about fifteen seconds. It had

0:37:19.000 --> 0:37:22.480
<v Speaker 1>like two thousand atoms in it. And you know what

0:37:22.560 --> 0:37:25.319
<v Speaker 1>happens is it's getting colder and colder and colder, and

0:37:25.400 --> 0:37:27.480
<v Speaker 1>each atom is sort of doing its own thing. And

0:37:27.520 --> 0:37:29.200
<v Speaker 1>when you have a bunch of atoms doing their own thing,

0:37:29.239 --> 0:37:31.439
<v Speaker 1>you get like a distribution, like some are a little faster,

0:37:31.600 --> 0:37:33.879
<v Speaker 1>some a little slower. All of a sudden, when they

0:37:33.880 --> 0:37:37.600
<v Speaker 1>crossed this threshold, this temperature threshold, they all snapped into place,

0:37:37.840 --> 0:37:40.440
<v Speaker 1>and we're all doing the same thing. Like they all

0:37:40.480 --> 0:37:43.400
<v Speaker 1>had the same velocity and they were in the same place,

0:37:43.440 --> 0:37:47.120
<v Speaker 1>and they acted like one mega particle. And you can

0:37:47.160 --> 0:37:49.520
<v Speaker 1>see this in their paper. They show like there's a blob,

0:37:49.560 --> 0:37:51.520
<v Speaker 1>there's a blob boom, there's a spike in the middle,

0:37:51.920 --> 0:37:54.640
<v Speaker 1>and that's a phase transition. That's when matters like doing

0:37:54.760 --> 0:37:58.240
<v Speaker 1>something really different. That's when it clicks. That's when it clicks. Yeah.

0:37:58.640 --> 0:38:00.480
<v Speaker 1>The sort of tragic thing is that you and see it,

0:38:00.520 --> 0:38:03.120
<v Speaker 1>but the only way to see it is to shine

0:38:03.160 --> 0:38:05.120
<v Speaker 1>a laser at it. Right, this is really small and

0:38:05.239 --> 0:38:07.720
<v Speaker 1>really cold, can just like see it with your naked eye.

0:38:08.000 --> 0:38:09.600
<v Speaker 1>So they had to shine a laser at it, which

0:38:09.640 --> 0:38:12.560
<v Speaker 1>destroys it. So they can prove that it's there, but

0:38:12.640 --> 0:38:15.919
<v Speaker 1>only by destroying And is that why it only last

0:38:15.960 --> 0:38:18.040
<v Speaker 1>fifteen seconds because you're trying to look at it at

0:38:18.040 --> 0:38:20.080
<v Speaker 1>the same time, or what's the time limit here? The

0:38:20.120 --> 0:38:21.799
<v Speaker 1>time limb is just how long they can keep this

0:38:21.840 --> 0:38:25.200
<v Speaker 1>thing cold and trapped. Eventually the atoms will fall out

0:38:25.400 --> 0:38:28.160
<v Speaker 1>of their trap. And the way they made their magnetic

0:38:28.239 --> 0:38:30.360
<v Speaker 1>bowl has a bit of a hole in the bottom

0:38:30.640 --> 0:38:32.520
<v Speaker 1>they had, so they were struggling with that a little bit,

0:38:32.760 --> 0:38:34.239
<v Speaker 1>and so it's hard for them to get a lot

0:38:34.280 --> 0:38:36.000
<v Speaker 1>of atoms in there and for it to last a

0:38:36.040 --> 0:38:38.320
<v Speaker 1>long time. It's a leaky bowl, a little bit of

0:38:38.320 --> 0:38:40.160
<v Speaker 1>a leaky bowl. But hey, they were the first ones

0:38:40.200 --> 0:38:42.320
<v Speaker 1>to do it. Because at m I T there was

0:38:42.360 --> 0:38:45.560
<v Speaker 1>a follow up lab, a lab led by Wolfgang Keaderly

0:38:45.880 --> 0:38:48.600
<v Speaker 1>that was sort of inheriting what Kleppner had done and

0:38:48.640 --> 0:38:50.840
<v Speaker 1>also trying to use heavier atoms. And there was a

0:38:50.920 --> 0:38:53.920
<v Speaker 1>race between this lab at U C Boulder and this

0:38:54.000 --> 0:38:56.719
<v Speaker 1>lab at M I T, and then also a lab

0:38:56.760 --> 0:38:58.880
<v Speaker 1>at Rice University, where I was happening to be an

0:38:58.920 --> 0:39:02.160
<v Speaker 1>undergraduate at this very moment, right you're telling me you

0:39:02.239 --> 0:39:04.560
<v Speaker 1>knew one of the scientists in this race trying to

0:39:04.600 --> 0:39:06.799
<v Speaker 1>get it to work first. Yeah, so everybody sort of

0:39:06.800 --> 0:39:09.000
<v Speaker 1>figured this out, and everybody knew that like this was

0:39:09.040 --> 0:39:11.320
<v Speaker 1>going to happen, and it was going to happen soon. Really,

0:39:11.719 --> 0:39:13.359
<v Speaker 1>like everyone knew that they were close to the finish

0:39:13.760 --> 0:39:17.240
<v Speaker 1>because they'd be giving presentations at conferences and these ideas

0:39:17.239 --> 0:39:19.680
<v Speaker 1>have been sort of coalescing, and these guys were the

0:39:19.760 --> 0:39:22.080
<v Speaker 1>leaders in the field, and it was really about like

0:39:22.239 --> 0:39:24.840
<v Speaker 1>making it work and getting it done. So the ideas

0:39:24.840 --> 0:39:26.799
<v Speaker 1>were out there, everybody knew how to do it. There

0:39:26.800 --> 0:39:29.400
<v Speaker 1>are a few slightly different approaches, like the guys that

0:39:29.520 --> 0:39:31.600
<v Speaker 1>m I T had a cool way to plug the

0:39:31.640 --> 0:39:35.240
<v Speaker 1>hole in the bottom of their magnetic well using another laser,

0:39:35.480 --> 0:39:37.600
<v Speaker 1>and the guys at Rice course, and the guys at

0:39:37.680 --> 0:39:40.200
<v Speaker 1>Rice were using lithium to try to get it done.

0:39:40.440 --> 0:39:43.080
<v Speaker 1>And I remember at this time because I was taking

0:39:43.239 --> 0:39:47.080
<v Speaker 1>thermodynamics as a physics major and the person teaching it

0:39:47.160 --> 0:39:50.000
<v Speaker 1>was Professor Randy Hewlett, and he was engaged in this

0:39:50.200 --> 0:39:53.240
<v Speaker 1>three way race for the Nobel Prize. These three labs

0:39:53.239 --> 0:39:55.360
<v Speaker 1>were all trying to make this happen at the same time.

0:39:55.880 --> 0:39:59.160
<v Speaker 1>I remember specifically because he almost never showed up to class,

0:39:59.200 --> 0:40:01.880
<v Speaker 1>like he was off giving talks, or he was in

0:40:01.880 --> 0:40:04.800
<v Speaker 1>the lab, or he sent his grad student or canceled lecture.

0:40:05.160 --> 0:40:06.960
<v Speaker 1>At the time, I was like, what is this guy

0:40:07.000 --> 0:40:10.800
<v Speaker 1>doing these things? He's so important. He was racing to

0:40:10.920 --> 0:40:13.279
<v Speaker 1>get the Nobel Prize. He wasn't on the clock. He

0:40:13.360 --> 0:40:16.040
<v Speaker 1>was on the clock where you know, days and weeks

0:40:16.080 --> 0:40:18.920
<v Speaker 1>make a difference between winning the Nobel Prize and just

0:40:18.960 --> 0:40:24.279
<v Speaker 1>being like also mentioned on the podcast years later by

0:40:24.320 --> 0:40:27.799
<v Speaker 1>one of your students that you ignored. Oh no, but

0:40:27.880 --> 0:40:31.000
<v Speaker 1>if the people at T Boulder did it first, who

0:40:31.000 --> 0:40:33.280
<v Speaker 1>got the Nobel Prize? We'll see you Boulder did it first.

0:40:33.640 --> 0:40:35.480
<v Speaker 1>And then M I T did it a couple of

0:40:35.480 --> 0:40:37.839
<v Speaker 1>months later, and they put out their paper. I think

0:40:37.840 --> 0:40:39.239
<v Speaker 1>this is so M I T. They put out their

0:40:39.280 --> 0:40:42.640
<v Speaker 1>paper the Monday after Thanksgiving, which means they must have

0:40:42.640 --> 0:40:48.399
<v Speaker 1>worked all Thanksgiving. Break them. Yeah, it was a few

0:40:48.400 --> 0:40:50.839
<v Speaker 1>months later, but it was a lot bigger, Like they

0:40:50.840 --> 0:40:53.239
<v Speaker 1>plugged that hole and they were able to get a

0:40:53.400 --> 0:40:56.520
<v Speaker 1>lot of atoms like you know, many many more atoms

0:40:56.520 --> 0:40:59.160
<v Speaker 1>that lasted a lot longer than to see you Boulder one.

0:40:59.160 --> 0:41:01.000
<v Speaker 1>So it was really like a big step forward in

0:41:01.040 --> 0:41:04.560
<v Speaker 1>another demonstration, and then you know, Rice did it also

0:41:04.680 --> 0:41:07.760
<v Speaker 1>in lithium. But it was later, and so they didn't

0:41:07.840 --> 0:41:10.480
<v Speaker 1>get included in the Nobel Prize. They went to MT

0:41:11.120 --> 0:41:16.239
<v Speaker 1>and see you Boulder, but Rice just got a cold gas. Well,

0:41:16.320 --> 0:41:18.560
<v Speaker 1>but Rice did it. They just did it even later,

0:41:18.920 --> 0:41:21.279
<v Speaker 1>and so the Nobel price compantee said, all right, we'll

0:41:21.320 --> 0:41:24.000
<v Speaker 1>cut it off at a couple of months after the discovery.

0:41:24.160 --> 0:41:26.920
<v Speaker 1>That kind of it seems a little totally arbitrary, but

0:41:26.960 --> 0:41:29.600
<v Speaker 1>there is this rule about Nobel Prizes you can only

0:41:29.640 --> 0:41:32.160
<v Speaker 1>share it among three people. And so there are two

0:41:32.160 --> 0:41:35.440
<v Speaker 1>p I s leading the lab at SEU Boulder slash

0:41:35.520 --> 0:41:37.440
<v Speaker 1>Mist and one leading the lab at m I T

0:41:37.760 --> 0:41:41.479
<v Speaker 1>And so that was sort of a natural cut off. Yeah, man,

0:41:41.600 --> 0:41:44.520
<v Speaker 1>you know, so you know, if those grad students in

0:41:44.560 --> 0:41:46.960
<v Speaker 1>the lab at Rice had just worked over Thanksgiving or

0:41:47.120 --> 0:41:50.120
<v Speaker 1>giving up their Christmas break or not taking vacation, or

0:41:50.120 --> 0:41:53.319
<v Speaker 1>if they didn't have to teach your class, maybe they

0:41:53.320 --> 0:41:55.080
<v Speaker 1>didn't have to grade. Like, oh, I almost got it,

0:41:55.120 --> 0:41:57.560
<v Speaker 1>but I gotta go teach this freshman the physics class.

0:41:57.800 --> 0:42:00.640
<v Speaker 1>I gotta grade this sloppy homework. May in I can't

0:42:00.640 --> 0:42:02.920
<v Speaker 1>even read this, writing up all night trying to decide

0:42:02.960 --> 0:42:06.279
<v Speaker 1>for this kid's homework. So basically, Daniel you're claimed to fame.

0:42:06.360 --> 0:42:09.280
<v Speaker 1>Is that not only did you know the second place

0:42:09.320 --> 0:42:12.279
<v Speaker 1>finisher for the both iceland concept, you were maybe a

0:42:12.360 --> 0:42:17.600
<v Speaker 1>participant slowing this person down. I definitely had interactions with

0:42:17.640 --> 0:42:20.799
<v Speaker 1>this person. No. I I know Randy Hewlett. He's a

0:42:20.800 --> 0:42:24.040
<v Speaker 1>great physicist and I admire him, and he's a great teacher,

0:42:24.360 --> 0:42:26.440
<v Speaker 1>and I think it's exciting to be on the forefront

0:42:26.520 --> 0:42:28.839
<v Speaker 1>and so close to the cutting edge. I do have

0:42:28.880 --> 0:42:32.200
<v Speaker 1>some sympathy for being so close and not quite being

0:42:32.239 --> 0:42:34.640
<v Speaker 1>included in the upper echelon of folks who win the

0:42:34.680 --> 0:42:37.239
<v Speaker 1>Nobel Prize. Yeah, I mean it seems kind of arbitrary, right,

0:42:37.680 --> 0:42:40.080
<v Speaker 1>Like you get the Nobel Prize, you don't get the prize,

0:42:40.120 --> 0:42:41.680
<v Speaker 1>but they were all sort of in it together. Yeah,

0:42:41.719 --> 0:42:43.799
<v Speaker 1>And what's really the difference between a few months here

0:42:43.880 --> 0:42:45.440
<v Speaker 1>or there. I think a lot of times people in

0:42:45.480 --> 0:42:48.439
<v Speaker 1>science make way too big a deal about somebody who's

0:42:48.520 --> 0:42:50.960
<v Speaker 1>one day ahead or the second day. You know, it's

0:42:50.960 --> 0:42:53.920
<v Speaker 1>important that everybody has done their own individual work. If

0:42:53.920 --> 0:42:56.000
<v Speaker 1>somebody has published a result and you just go and

0:42:56.239 --> 0:43:00.000
<v Speaker 1>replicate it, that's not the same thing as individual independent

0:43:00.040 --> 0:43:03.560
<v Speaker 1>in contribution. These are different lines of research, different ideas,

0:43:03.880 --> 0:43:07.920
<v Speaker 1>different strategies, really independent efforts that were in parallel. Sure,

0:43:07.920 --> 0:43:10.320
<v Speaker 1>one finished a few weeks or months ahead of the other,

0:43:10.560 --> 0:43:13.200
<v Speaker 1>but they all made contributions around the same time. So

0:43:13.800 --> 0:43:15.960
<v Speaker 1>in a better world, we would have recognized all of

0:43:15.960 --> 0:43:18.560
<v Speaker 1>them and think about his accomplishments. I mean, he taught you,

0:43:18.760 --> 0:43:21.880
<v Speaker 1>and now here you are teaching thousands and thousands and

0:43:21.880 --> 0:43:24.560
<v Speaker 1>thousands of people. Yeah, that's a I hope that's enough

0:43:24.560 --> 0:43:26.560
<v Speaker 1>for you. You didn't get to meet the King of Sweden.

0:43:26.760 --> 0:43:29.120
<v Speaker 1>You got to be talked about on my podcast. All right,

0:43:29.160 --> 0:43:31.960
<v Speaker 1>Well that was pretty exciting for such a cool topic,

0:43:32.400 --> 0:43:36.759
<v Speaker 1>such a chill topic. Yeah, and so people are continuing

0:43:37.080 --> 0:43:39.640
<v Speaker 1>and now they make Bose Einstein condensates all the time.

0:43:39.680 --> 0:43:43.080
<v Speaker 1>They even made it once on the space station, kidding like,

0:43:43.400 --> 0:43:46.480
<v Speaker 1>you can make a Bose Einstein maker that you can

0:43:46.480 --> 0:43:48.920
<v Speaker 1>take to space. Yeah, exactly. They put together a lab

0:43:48.960 --> 0:43:51.800
<v Speaker 1>on the International Space Station that made a Bose Einstein

0:43:51.840 --> 0:43:55.799
<v Speaker 1>condensate in space, which is pretty cool. Could they also

0:43:55.840 --> 0:44:00.520
<v Speaker 1>make bar garded and smooth only on Fridays? Very cool

0:44:00.520 --> 0:44:02.560
<v Speaker 1>that Bose and Einstein thought of this and that it

0:44:02.600 --> 0:44:05.360
<v Speaker 1>actually came to pass. That's pretty awesome. And now it

0:44:05.400 --> 0:44:07.520
<v Speaker 1>gives us a new window, a new kind of stuff

0:44:07.560 --> 0:44:10.040
<v Speaker 1>to poke and to play with. And you know, now

0:44:10.120 --> 0:44:12.160
<v Speaker 1>we can make these things and they last a long time,

0:44:12.200 --> 0:44:14.319
<v Speaker 1>so you can do things like stir them and make

0:44:14.400 --> 0:44:18.360
<v Speaker 1>vortices in them, and watch quantum vortices be created and

0:44:18.640 --> 0:44:21.319
<v Speaker 1>overlap them and and launch them into each other, and

0:44:21.360 --> 0:44:25.240
<v Speaker 1>see interference effects on macroscopic objects. So you can recreate

0:44:25.239 --> 0:44:28.120
<v Speaker 1>a lot of the cool quantum mechanical experiments that used

0:44:28.120 --> 0:44:31.880
<v Speaker 1>to only work on tiny, invisible microscopic particles. Now you

0:44:31.880 --> 0:44:35.760
<v Speaker 1>can do them on macroscopic blobs of stuff. That's pretty amazing.

0:44:35.920 --> 0:44:37.839
<v Speaker 1>So are there any other states of matter we should

0:44:37.880 --> 0:44:39.920
<v Speaker 1>be looking out for or that we might discover in

0:44:39.960 --> 0:44:41.920
<v Speaker 1>the future. You know, there are lots of other states

0:44:41.920 --> 0:44:45.160
<v Speaker 1>of matter that people theorize about, you know, tetracorks and

0:44:45.200 --> 0:44:49.040
<v Speaker 1>hexa corks and all sorts of weird combinations. Because matter

0:44:49.200 --> 0:44:52.480
<v Speaker 1>is complex and it has lots of really complicated interactions

0:44:52.760 --> 0:44:56.120
<v Speaker 1>and in various configurations and pressure and density. You know,

0:44:56.160 --> 0:44:58.120
<v Speaker 1>you can do all sorts of weird stuff, like we

0:44:58.239 --> 0:45:01.000
<v Speaker 1>talked about quirk matter and strang age matter. You know,

0:45:01.040 --> 0:45:03.360
<v Speaker 1>what might happen in the core of a neutron star.

0:45:04.000 --> 0:45:05.720
<v Speaker 1>And I'm sure there are lots of things we haven't

0:45:05.760 --> 0:45:09.000
<v Speaker 1>even imagined. One day, I hope we'll discover something before

0:45:09.120 --> 0:45:10.840
<v Speaker 1>we think about it, so we'll have a triumph for

0:45:10.960 --> 0:45:14.400
<v Speaker 1>experimental physics rather than just for theoretical physics. Well, and

0:45:14.440 --> 0:45:16.520
<v Speaker 1>maybe somebody out there listening could be the person to

0:45:16.560 --> 0:45:19.399
<v Speaker 1>discover this new state of matter. That's right. There's lots

0:45:19.400 --> 0:45:22.360
<v Speaker 1>more to discover, lots more weird kinds of good that

0:45:22.400 --> 0:45:25.200
<v Speaker 1>we can make matter to do. And hopefully you'll start

0:45:25.239 --> 0:45:28.960
<v Speaker 1>a lab and zap matter into doing something weird and

0:45:29.000 --> 0:45:33.600
<v Speaker 1>then chill out with your Nobel Prize and your Margarita

0:45:33.920 --> 0:45:36.719
<v Speaker 1>or at or your silver Bibel Prize. What did you

0:45:36.760 --> 0:45:43.680
<v Speaker 1>call it, the Plywood Nobel Prize? Plywood not as valuable,

0:45:43.719 --> 0:45:46.239
<v Speaker 1>but very tough. It's very hearty, that's right. Yeah, and

0:45:46.280 --> 0:45:49.640
<v Speaker 1>it's got the description written in a sharpie. All right. Well,

0:45:49.680 --> 0:45:51.440
<v Speaker 1>we hope you enjoyed that, and you we hope that

0:45:51.520 --> 0:45:55.080
<v Speaker 1>you joined this amazing race to discover new kinds of matter.

0:45:55.160 --> 0:45:57.759
<v Speaker 1>And thanks for listening. If you're interested in hearing more

0:45:57.800 --> 0:46:00.000
<v Speaker 1>about this kind of stuff, please send us a suggestion

0:46:00.080 --> 0:46:02.960
<v Speaker 1>two questions at Daniel and Jorge dot com and come

0:46:03.000 --> 0:46:05.800
<v Speaker 1>interact with us. We're on Twitter at Dale and Jorge

0:46:05.840 --> 0:46:08.680
<v Speaker 1>where we answer questions and make jokes, so come and

0:46:08.760 --> 0:46:11.560
<v Speaker 1>check us out. Thanks for joining us, see you next time.

0:46:19.280 --> 0:46:22.160
<v Speaker 1>Thanks for listening, and remember that Daniel and Jorge explained.

0:46:22.160 --> 0:46:25.080
<v Speaker 1>The Universe is a production of I Heart Radio. Or

0:46:25.200 --> 0:46:28.120
<v Speaker 1>more podcast from my heart Radio, visit the I heart

0:46:28.200 --> 0:46:31.799
<v Speaker 1>Radio app, Apple Podcasts, or wherever you listen to your

0:46:31.840 --> 0:46:32.560
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