WEBVTT - Could quantum clocks detect dark matter?

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<v Speaker 5>Hey, Daniel, if you were Dark Matter, where would you hide?

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<v Speaker 1>I wouldn't hide. If I was Dark Matter, I would

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<v Speaker 1>totally parade myself in front of all the scientists in

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<v Speaker 1>the galaxy.

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<v Speaker 5>Ooh, a parade You mean like a pageant queen?

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<v Speaker 1>Yeah, something like that. You know, just don't be so shy.

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<v Speaker 5>Well, if it turns out you are dark matter, we'll

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<v Speaker 5>definitely throw you a parade. But so far, it seems

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<v Speaker 5>like dark matter is kind of reclusive, right, it's kind

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<v Speaker 5>of shy, so maybe it is hiding. What would be

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<v Speaker 5>some good spots for it to hide it?

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<v Speaker 1>Well, if dark matter doesn't want a tiara and it's

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<v Speaker 1>hiding somewhere, then I don't know where it would hide.

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<v Speaker 1>I mean, if I knew, I would go and look

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<v Speaker 1>for it there.

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<v Speaker 5>What if it's somewhere kind of obvious.

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<v Speaker 1>Like what like right behind me?

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<v Speaker 5>Yeah, or right in front of you or right on

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<v Speaker 5>TV and the Matter universe contest.

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<v Speaker 1>That would be a great twist ending for the m

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<v Speaker 1>Knight Shamanlan version of this story.

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<v Speaker 5>Well, man, do you think he knows I see dark matter?

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<v Speaker 6>Hi?

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<v Speaker 5>I'm Jorge Mack, cartoonist and author of Allor's Great Big Universe.

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<v Speaker 1>Hi, I'm Daniel. I'm a particle physicist, and I wish

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<v Speaker 1>I had a dark matter tiara.

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<v Speaker 5>Oh, but it wouldn't be very shiny or bright. It

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<v Speaker 5>would be dark, So what's the point. Also, when it

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<v Speaker 5>it just fall through your head.

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<v Speaker 1>It would be hard to wear, but it'd be like

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<v Speaker 1>the greatest, most amazing piece of jewelry.

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<v Speaker 5>Ever, how would you even keep it in your house?

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<v Speaker 1>These are just like engineering details.

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<v Speaker 4>You know.

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<v Speaker 1>Once I've solved the physics of a dark matter Tiara,

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<v Speaker 1>I'll just pass that off to the engineers.

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<v Speaker 5>This is just all part of your dream to be

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<v Speaker 5>the universe's darktor universe.

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<v Speaker 1>I would like a little bit of bling. Yeah, you know,

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<v Speaker 1>physics bling would be nice. I'm not gonna win a

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<v Speaker 1>Nobel Prize anytime soon, So dark matter Tirres sounds good.

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<v Speaker 1>I see.

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<v Speaker 5>I see. You could just say you have a dark

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<v Speaker 5>matter Tierra, and they know nobody would be able to

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<v Speaker 5>see it, or feel it or detect it. They would

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<v Speaker 5>just have to believe you.

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<v Speaker 1>I need evidence, man, That's what science is all about.

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<v Speaker 1>You got to have data.

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<v Speaker 5>I don't think those beauty contests depend on data very much.

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<v Speaker 1>But I'm trying to win a science contest.

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<v Speaker 5>But anyway's welcome. Podcast Daniel and Jorge Explain the Universe,

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<v Speaker 5>a production of iHeartRadio in which we enter you in.

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<v Speaker 1>The greatest science contest of all time, the quest to

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<v Speaker 1>understand the nature of the universe. What is it, what's

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<v Speaker 1>in it? What's it made out? Of how does it

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<v Speaker 1>all work. We think these questions are deep and fundamental

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<v Speaker 1>parts of being a human being in this cosmos, and

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<v Speaker 1>unraveling these questions is a joy that everybody should share.

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<v Speaker 1>So on this podcast we take those questions apart and

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<v Speaker 1>try to share our answers and our ignorance with you.

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<v Speaker 5>That's right, because science is the greatest beauty contest in

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<v Speaker 5>the universe. We're the goal is to discover the beauty

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<v Speaker 5>of how this universe is put together, how it works,

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<v Speaker 5>and what is our place in it.

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<v Speaker 1>Over the last fifty one hundred years, we've developed a

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<v Speaker 1>pretty good sense for what's in the universe. We know

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<v Speaker 1>about stars and galaxies and all the bright and shiny

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<v Speaker 1>stuff that's out there in the universe. And we've also

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<v Speaker 1>figured out that there's a lot of the universe that

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<v Speaker 1>we can't see directly using our senses or any of

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<v Speaker 1>the forces that we've discovered except for gravity. We know

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<v Speaker 1>that a huge chunk of the stuff that's out there

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<v Speaker 1>in the universe is invisible. It's intangible, which makes it

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<v Speaker 1>very hard to discover and to figure out how to

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<v Speaker 1>make it into a tiara.

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<v Speaker 5>Yeah, because it turns out that a pretty good understanding

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<v Speaker 5>of the universe only covers about uh five percent of

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<v Speaker 5>what we know is out there. The rest, the ninety

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<v Speaker 5>five percent of the universe that we know is there,

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<v Speaker 5>we have no idea what it is or how it works.

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<v Speaker 1>That sounds like a good title for a book.

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<v Speaker 5>Yeah, I think we wrote one, Daniel, which is available

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<v Speaker 5>for us sale everywhere.

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<v Speaker 1>That's right. The kind of stuff that you and I

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<v Speaker 1>are made out of, atoms specifically, or what physicists called baryons,

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<v Speaker 1>only makes up five percent of the energy budget in

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<v Speaker 1>the universe. There's another twenty five twenty seven percent that's

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<v Speaker 1>dark matter, some kind of stuff that we know is matter.

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<v Speaker 1>We know it's out there, but we don't know what

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<v Speaker 1>it is, and we only have a very rough sense

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<v Speaker 1>of even where it is around us. The rest of

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<v Speaker 1>the universe is something we call dark energy, which is

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<v Speaker 1>contributing to the accelerating expansion of the universe, and we

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<v Speaker 1>have even less clue about what makes that up.

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<v Speaker 5>Yeah, there's a lot we don't know, and it seems

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<v Speaker 5>like these are maybe the defining mysteries of our times

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<v Speaker 5>is to figure out what the universe is actually made

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<v Speaker 5>out of. Given that what we're made out of counts

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<v Speaker 5>is so little of it.

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<v Speaker 1>Yeah, you're right, And in the last few decades there's

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<v Speaker 1>been a huge program of people looking for dark matter.

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<v Speaker 1>We've talked on the podcast about trying to make dark

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<v Speaker 1>matter in the laboratory by smashing particles together. We're searching

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<v Speaker 1>for the dark matter wind. We might be floating through

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<v Speaker 1>with very sensitive underground facilities looking for an individual piece

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<v Speaker 1>of dark matter to bump into liquid xenon, for example,

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<v Speaker 1>or maybe evidence of dark matter annihilating itself in the

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<v Speaker 1>center of the galaxy. But so far, none of these

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<v Speaker 1>experiments have found dark matter, which means we've got to

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<v Speaker 1>get creative about other ways to maybe detect this most

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<v Speaker 1>important or at least most common kind of matter in

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<v Speaker 1>the universe.

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<v Speaker 5>So to be On the podcast, we'll be tackling the

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<v Speaker 5>question could quantum clocks detect dark matter? And how many

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<v Speaker 5>jargon words can we fit into one podcast title?

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<v Speaker 1>I know it does sound like buzzword sound, you know,

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<v Speaker 1>like could we use AI generated crypto bitcoin to detect

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<v Speaker 1>dark matter?

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<v Speaker 5>You mean quantum nano matter, Yes, exactly, quantum nano matter.

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<v Speaker 1>Tiras Wow, I like quantum nanomatter. I'm going to use

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<v Speaker 1>that in a proposal.

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<v Speaker 5>That's good, that's said Daniel. Also, it's probably our on

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<v Speaker 5>sale on Amazon. There's probably some product out there with

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<v Speaker 5>that name.

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<v Speaker 1>So yeah, but you didn't say ching tm after it,

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<v Speaker 1>so I can use it.

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<v Speaker 5>No, you don't have to.

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<v Speaker 1>What I gotta brush up on my podcast property law.

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<v Speaker 5>Yeah, you better or else I'm gonna see you for

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<v Speaker 5>nano dollars for nano bitcoins, you know what?

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<v Speaker 1>Or hey, you can have all of my nano bitcoins.

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<v Speaker 5>What's the price of bitcoin these days?

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<v Speaker 1>Nano bitcoins zero? Yeah, doesn't exist.

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<v Speaker 5>But anyways, it's kind of an intriguing title. Could quantum

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<v Speaker 5>clocks detect dark matter and quantum clocks sounds like it

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<v Speaker 5>does sound like something you could buy an off of Amazon.

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<v Speaker 5>Did you check to see if it's something you can

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<v Speaker 5>just get next day?

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<v Speaker 4>Oh?

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<v Speaker 1>Yeah, it turns out Amazon will sell you something it

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<v Speaker 1>calls a quantum clock, like a quantum entanglement led wall clock.

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<v Speaker 1>But none of these things are actually quantum clocks the

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<v Speaker 1>way that we understand them.

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<v Speaker 5>Well, technically, isn't everything a quantum something? Well, I mean

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<v Speaker 5>not everything, but you know the five percent that we

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<v Speaker 5>know about in the universe, it's in it all quantum technically,

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<v Speaker 5>like this is a quantum podcast.

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<v Speaker 1>I mean, that's a really interesting philosophical question and not

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<v Speaker 1>one that we really have an answer to, because on

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<v Speaker 1>one hand, you're right that everything is made out of

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<v Speaker 1>quantum particle, so isn't the whole universe quantum. On the

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<v Speaker 1>other hand, we know that when you zoom out things

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<v Speaker 1>behave by different rules. We call that classical. We don't

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<v Speaker 1>really understand why there is that transition, but there definitely

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<v Speaker 1>is a transition. So to call everything quantum is either

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<v Speaker 1>to say that look classical is just big zoomed out quantum,

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<v Speaker 1>or is to say that clackical doesn't really matter, which

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<v Speaker 1>doesn't really sit well with me. Or what if I

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<v Speaker 1>have no class, then you probably have a lot of

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<v Speaker 1>big coin.

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<v Speaker 5>Then I'm not gonna win any beauty contest. I have poise,

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<v Speaker 5>but just no class.

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<v Speaker 1>Yeah, exactly. But you know, for example, a clock that

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<v Speaker 1>just works on mechanical parts would also work in the

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<v Speaker 1>universe where QUANTUMU didn't rule the microscopic because it's not

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<v Speaker 1>sensitive to those microscopic details, and so that wouldn't be

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<v Speaker 1>a quantum clock. For example, like a pendulum clock or

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<v Speaker 1>an old fashioned Swiss gear based.

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<v Speaker 5>Clock a discussion about now mankla Sure that's my favorite.

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<v Speaker 1>Hey you brought it up.

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<v Speaker 5>But anyways, it's a kind of an interesting question and

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<v Speaker 5>so we'll dig into it. But as usual, we were

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<v Speaker 5>wondering how many people out there have thought about putting

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<v Speaker 5>the concepts of dark matter and quantum and clocks all

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<v Speaker 5>together in one sentence.

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<v Speaker 1>So thanks very much to everybody who participates in this

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<v Speaker 1>segment of the podcast. We love that you volunteer, We

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<v Speaker 1>love hearing your thoughts, and we love sharing your voice

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<v Speaker 1>with all of the other listeners. Please chime in if

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<v Speaker 1>you'd like, write to me two questions at Danielanjorge dot

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<v Speaker 1>com and you can't participate.

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<v Speaker 5>So think about it for a second. Do you think

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<v Speaker 5>quantum clocks can be used to detect dark matter? Here's

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<v Speaker 5>what people had to say.

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<v Speaker 7>I've never heard of a quantum clock, but I'm not

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<v Speaker 7>sure how it would be able to detect dark matter

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<v Speaker 7>anymore than a regular clock could. I guess maybe even

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<v Speaker 7>with a regular clock, you could send it out into space,

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<v Speaker 7>and if it hits a huge clump of dark matter

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<v Speaker 7>and therefore gravity, maybe we could learn that there's a

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<v Speaker 7>big well of gravity out in some location that we

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<v Speaker 7>otherwise couldn't detect.

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<v Speaker 3>Not so sure.

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<v Speaker 8>I suppose it's possible, but I have no clue how

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<v Speaker 8>it would Maybe something to do with entanglement.

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<v Speaker 9>Since you're asking, the answer is probably yes, but maybe

0:11:23.200 --> 0:11:27.000
<v Speaker 9>still theoretical. I would think you'd have to use the

0:11:27.120 --> 0:11:32.199
<v Speaker 9>idea of measuring light passing through an area of more density,

0:11:32.320 --> 0:11:36.200
<v Speaker 9>thus possibly dark matter that causes curvature of space and

0:11:36.240 --> 0:11:39.560
<v Speaker 9>also time dilation. How to do that, I'm not sure.

0:11:39.800 --> 0:11:42.640
<v Speaker 1>Since we don't possess a quantum clock, it doesn't seem

0:11:42.720 --> 0:11:46.160
<v Speaker 1>unreasonable to suggest that a non existent clock cannot detect

0:11:46.280 --> 0:11:46.800
<v Speaker 1>dark matter.

0:11:47.120 --> 0:11:51.040
<v Speaker 5>All right, it's pretty uh intense answers here. I feel

0:11:51.080 --> 0:11:54.720
<v Speaker 5>like it's something that some of the listeners had heard

0:11:54.760 --> 0:11:58.280
<v Speaker 5>about before. Did you pull your professor colleagues this time?

0:11:59.000 --> 0:12:02.360
<v Speaker 1>No, these are our listeners online. You know. There's some

0:12:02.400 --> 0:12:07.920
<v Speaker 1>good answers here about entanglement and light passing through areas

0:12:07.960 --> 0:12:10.520
<v Speaker 1>with dark matter density in them, and just in general

0:12:10.640 --> 0:12:12.160
<v Speaker 1>sense that this is a hard problem.

0:12:12.280 --> 0:12:14.960
<v Speaker 5>Maybe you should ask a bunch of beauty queens next time,

0:12:15.760 --> 0:12:17.439
<v Speaker 5>or make it one of the standard questions in a

0:12:17.480 --> 0:12:21.120
<v Speaker 5>beauty pageant. Forget howdy, how would you save the world?

0:12:21.240 --> 0:12:24.040
<v Speaker 5>Or how would you know make things better? What do

0:12:24.040 --> 0:12:25.439
<v Speaker 5>you think about quantum clocks?

0:12:27.040 --> 0:12:29.040
<v Speaker 1>Well, where is the dark matter? Yeah, I'd love to

0:12:29.040 --> 0:12:30.439
<v Speaker 1>hear that answer in the beauty pageant.

0:12:32.080 --> 0:12:35.200
<v Speaker 5>Not that it couldn't happen, of course, no, absolutely. All right, Well,

0:12:35.280 --> 0:12:39.200
<v Speaker 5>let's dig into this intriguing question of whether dark matter

0:12:39.240 --> 0:12:42.440
<v Speaker 5>can be detected by quantum clocks, and let's start with

0:12:42.480 --> 0:12:45.560
<v Speaker 5>the basics. Daniel, what do we know about dark matter?

0:12:45.640 --> 0:12:47.480
<v Speaker 1>So there's a lot that we do and do not

0:12:47.679 --> 0:12:50.679
<v Speaker 1>know about dark matter. So let's start with what we

0:12:50.760 --> 0:12:53.360
<v Speaker 1>do know. We know that it's out there, and we

0:12:53.400 --> 0:12:56.360
<v Speaker 1>know that it's here as well. We know that dark

0:12:56.400 --> 0:12:58.760
<v Speaker 1>matter is something that exists in the universe. And then

0:12:58.800 --> 0:13:01.520
<v Speaker 1>it's matter. We know that because we see its gravity.

0:13:02.000 --> 0:13:05.440
<v Speaker 1>We see it holding galaxies together as they spin. There

0:13:05.520 --> 0:13:07.880
<v Speaker 1>isn't enough gravity from the stars and the gas and

0:13:08.000 --> 0:13:10.960
<v Speaker 1>dust that make up those galaxies to keep the stars

0:13:11.000 --> 0:13:13.320
<v Speaker 1>in place as they swirl around the center of the

0:13:13.320 --> 0:13:16.959
<v Speaker 1>galaxy at very high speeds, and yet they do stay

0:13:16.960 --> 0:13:20.680
<v Speaker 1>in place. Galaxies are mostly not throwing stars out into

0:13:20.720 --> 0:13:23.560
<v Speaker 1>intergalactic space, and so we infer that there must be

0:13:23.600 --> 0:13:27.360
<v Speaker 1>some matter there to hold that galaxy together. But it's

0:13:27.400 --> 0:13:30.200
<v Speaker 1>more than just that one inference, that one fudge factor

0:13:30.240 --> 0:13:33.360
<v Speaker 1>to make that particular equation work. We see evidence for

0:13:33.440 --> 0:13:36.000
<v Speaker 1>dark matter all over the history of the universe, from

0:13:36.000 --> 0:13:39.000
<v Speaker 1>the very first few moments when the early universe plasma

0:13:39.080 --> 0:13:42.360
<v Speaker 1>is slashing around and you have dark matter and normal

0:13:42.400 --> 0:13:45.920
<v Speaker 1>matter and photons all acting very differently and creating different

0:13:45.960 --> 0:13:49.720
<v Speaker 1>slashing patterns. From looking at that slashing in the cosmic

0:13:49.760 --> 0:13:53.040
<v Speaker 1>microwave background radiation, we can figure out that there was

0:13:53.160 --> 0:13:55.560
<v Speaker 1>dark matter and even measure how much of it there is,

0:13:55.920 --> 0:13:58.520
<v Speaker 1>and we can trace the history of dark matter's gravity

0:13:58.559 --> 0:14:01.240
<v Speaker 1>as it shapes the structure formation of the whole universe

0:14:01.559 --> 0:14:04.160
<v Speaker 1>why we have galaxies at all this early in the

0:14:04.240 --> 0:14:06.880
<v Speaker 1>history of the universe, And so dark matter is definitely

0:14:06.880 --> 0:14:08.840
<v Speaker 1>out there as a kind of matter, but we don't

0:14:08.840 --> 0:14:12.719
<v Speaker 1>know really what it is or very specifically where it is,

0:14:12.840 --> 0:14:16.680
<v Speaker 1>because it's so hard to see since it only feels gravity.

0:14:16.679 --> 0:14:19.360
<v Speaker 1>It doesn't feel any of the other forces that we've discovered.

0:14:19.720 --> 0:14:22.360
<v Speaker 5>And we can also sort of see dark matter right like,

0:14:22.400 --> 0:14:23.840
<v Speaker 5>we can see it in the same way that you

0:14:23.840 --> 0:14:26.280
<v Speaker 5>can see a lens or glass lens or example. You

0:14:26.280 --> 0:14:29.360
<v Speaker 5>can see how it distorts the light behind it, right.

0:14:29.280 --> 0:14:32.440
<v Speaker 1>Yeah, exactly. We can see dark matter through gravity, and

0:14:32.480 --> 0:14:35.720
<v Speaker 1>so that means we can see stuff bending around dark matter.

0:14:35.960 --> 0:14:38.680
<v Speaker 1>We can see it holding galaxies together, and that even

0:14:38.760 --> 0:14:41.880
<v Speaker 1>impacts how light moves in the vicinity of dark matter.

0:14:42.000 --> 0:14:44.880
<v Speaker 1>If you have a big blob of dark matter between

0:14:44.880 --> 0:14:48.160
<v Speaker 1>you and some distant galaxy, for example, the photons from

0:14:48.200 --> 0:14:50.880
<v Speaker 1>that distant galaxy will bend as they move through that

0:14:51.040 --> 0:14:54.480
<v Speaker 1>dark matter, creating apparent distortions in your image. You can

0:14:54.520 --> 0:14:57.680
<v Speaker 1>even sometimes see the same galaxy twice in the sky

0:14:57.920 --> 0:15:01.240
<v Speaker 1>because of this gravitational lensing. And so we know that

0:15:01.280 --> 0:15:03.160
<v Speaker 1>it's out there, and we can use some techniques like

0:15:03.200 --> 0:15:06.760
<v Speaker 1>that to sometimes tell roughly where it is. But because

0:15:06.880 --> 0:15:10.520
<v Speaker 1>dark matter is so weak it's particles only feel gravity,

0:15:10.560 --> 0:15:13.440
<v Speaker 1>we think it's very difficult to figure out what exactly

0:15:13.560 --> 0:15:16.440
<v Speaker 1>is made out of to isolate one piece of dark matter,

0:15:16.680 --> 0:15:20.040
<v Speaker 1>because gravity is so weak that essentially a particle's gravity

0:15:20.320 --> 0:15:21.960
<v Speaker 1>is almost impossible to measure.

0:15:22.160 --> 0:15:24.560
<v Speaker 5>Yeah, and dark matter is also something that's not just

0:15:24.720 --> 0:15:27.920
<v Speaker 5>out there in space. It's sort of like all around us,

0:15:28.000 --> 0:15:30.440
<v Speaker 5>right like it's floating through us right now, sort of

0:15:30.480 --> 0:15:32.880
<v Speaker 5>like the fourth you know, it flows through us, binds

0:15:32.920 --> 0:15:36.440
<v Speaker 5>us all together. It's made out of medtichlorians.

0:15:36.480 --> 0:15:40.600
<v Speaker 1>Perhaps perhaps, yeah, exactly, you'll only really understand it after

0:15:40.720 --> 0:15:43.440
<v Speaker 1>nine hundred years of study. That's a really good question,

0:15:43.520 --> 0:15:46.200
<v Speaker 1>and that's sort of the central question of this episode

0:15:46.320 --> 0:15:49.760
<v Speaker 1>is exactly where is the dark matter? And can we

0:15:49.800 --> 0:15:53.000
<v Speaker 1>find like concentrations of it? Can we map it out?

0:15:53.760 --> 0:15:57.640
<v Speaker 1>Because dark matter is so weakly interacting like only gravity,

0:15:57.680 --> 0:16:00.360
<v Speaker 1>it takes huge amounts of it to feel anything, and

0:16:00.440 --> 0:16:02.880
<v Speaker 1>so that makes it very hard to tell exactly where

0:16:02.920 --> 0:16:05.400
<v Speaker 1>the dark matter is. It might be that it's mostly

0:16:05.480 --> 0:16:08.240
<v Speaker 1>spread out evenly through the galaxy. It might be more

0:16:08.320 --> 0:16:11.480
<v Speaker 1>clumpy than that depends a lot on your particular theory

0:16:11.640 --> 0:16:14.800
<v Speaker 1>of dark matter. Where it exactly is. So it could

0:16:14.800 --> 0:16:16.840
<v Speaker 1>be that we are in a dark matter wind as

0:16:16.880 --> 0:16:19.120
<v Speaker 1>the Earth orbits the Sun and the Sun moves through

0:16:19.120 --> 0:16:22.080
<v Speaker 1>the galaxy. We could also be in a dark matter

0:16:22.200 --> 0:16:25.560
<v Speaker 1>liss bubble, a bubble of space in which there's comparatively

0:16:25.680 --> 0:16:27.960
<v Speaker 1>little dark matter. Or it could be that dark matter

0:16:28.000 --> 0:16:29.560
<v Speaker 1>is fairly dense in our area.

0:16:29.720 --> 0:16:31.000
<v Speaker 5>You know, I have to say, every time you say

0:16:31.080 --> 0:16:34.640
<v Speaker 5>dark matter wind, it makes me think of dark parts.

0:16:37.280 --> 0:16:39.320
<v Speaker 1>Elevating the discourse every week.

0:16:41.760 --> 0:16:43.120
<v Speaker 5>That's my job. That's why I'm here.

0:16:43.320 --> 0:16:43.960
<v Speaker 1>Smells.

0:16:43.680 --> 0:16:48.080
<v Speaker 5>It's all grounded or grounded or you know, flat as

0:16:48.120 --> 0:16:51.600
<v Speaker 5>in fletch wents. But anyways, so it's sort of all

0:16:51.640 --> 0:16:53.440
<v Speaker 5>around this, and I guess I'm wondering, like, if it

0:16:53.480 --> 0:16:56.440
<v Speaker 5>is all around us, would we be able to tell, Like,

0:16:56.600 --> 0:16:58.600
<v Speaker 5>you know, if let's say dark matter is flowing through

0:16:58.640 --> 0:17:01.080
<v Speaker 5>the Earth right now, or say it wasn't, would you

0:17:01.120 --> 0:17:02.200
<v Speaker 5>be able to tell the difference.

0:17:02.440 --> 0:17:05.359
<v Speaker 1>That's exactly what these experiments are trying to measure. And

0:17:05.440 --> 0:17:08.240
<v Speaker 1>to give you a sense of the difficulty the challenge

0:17:08.240 --> 0:17:11.280
<v Speaker 1>of this, think about like why we didn't discover dark

0:17:11.320 --> 0:17:14.760
<v Speaker 1>matter earlier, just in studying how our Solar system moves.

0:17:15.119 --> 0:17:18.080
<v Speaker 1>We have now very precise measurements of the orbit of

0:17:18.160 --> 0:17:20.679
<v Speaker 1>Jupiter and Mars and all the planets and all the

0:17:20.720 --> 0:17:23.960
<v Speaker 1>little pieces of the Solar System as they orbit the Sun.

0:17:24.320 --> 0:17:26.080
<v Speaker 1>You might think, hey, if dark matter is here in

0:17:26.080 --> 0:17:28.960
<v Speaker 1>our Solar system and it has gravity, wouldn't it change

0:17:29.000 --> 0:17:31.399
<v Speaker 1>the way those things orbit? Shouldn't we be able to

0:17:31.480 --> 0:17:33.720
<v Speaker 1>detect it? But because we think dark matter might be

0:17:33.920 --> 0:17:37.800
<v Speaker 1>spread very thin, probably there isn't that much dark matter

0:17:37.880 --> 0:17:40.520
<v Speaker 1>in the vicinity of our Solar system. So even those

0:17:40.640 --> 0:17:43.639
<v Speaker 1>very very precise measurements you know, like knowing the motion

0:17:43.760 --> 0:17:47.639
<v Speaker 1>of Jupiter to meters or centimeters, can't detect dark matter

0:17:47.960 --> 0:17:50.200
<v Speaker 1>because it would be very thin and very spread out

0:17:50.240 --> 0:17:53.399
<v Speaker 1>and mostly we think homogeneous, which in the end doesn't

0:17:53.440 --> 0:17:56.680
<v Speaker 1>give much gravitational pull on the objects in the Solar System.

0:17:57.040 --> 0:18:00.399
<v Speaker 1>So it takes a very specialized, highly sensitive device to

0:18:00.400 --> 0:18:02.200
<v Speaker 1>be able to detect this dark matter.

0:18:02.400 --> 0:18:04.199
<v Speaker 5>Yeah, and then don't we say once like, if you

0:18:04.240 --> 0:18:07.000
<v Speaker 5>take all the dark matter that is potentially floating through

0:18:07.040 --> 0:18:09.439
<v Speaker 5>the Earth right now, it would only weigh about as

0:18:09.520 --> 0:18:11.680
<v Speaker 5>much as a squirrel or something like that.

0:18:11.880 --> 0:18:14.879
<v Speaker 1>Yeah, exactly, though that's very speculative, right. That assumes that

0:18:15.000 --> 0:18:18.520
<v Speaker 1>dark matter is essentially equally spread out in our galaxy,

0:18:18.600 --> 0:18:21.520
<v Speaker 1>which we don't believe is true. But if you assume

0:18:21.640 --> 0:18:24.880
<v Speaker 1>that there is, then we know our galaxy, for example,

0:18:25.080 --> 0:18:28.640
<v Speaker 1>is ninety five percent dark matter. That means for every

0:18:28.720 --> 0:18:31.720
<v Speaker 1>kilogram of matter made out of atoms like hydrogen and

0:18:31.720 --> 0:18:35.400
<v Speaker 1>helium or whatever, there's nineteen kilograms of matter made out

0:18:35.400 --> 0:18:38.320
<v Speaker 1>of whatever dark matter is made out of. And so

0:18:38.440 --> 0:18:41.679
<v Speaker 1>it's like nineteen to one in our galaxy.

0:18:41.280 --> 0:18:44.119
<v Speaker 5>Which sounds like a lot, but I guess also galaxies

0:18:44.240 --> 0:18:47.600
<v Speaker 5>kind of very empty mostly right, like it's probably like

0:18:47.680 --> 0:18:48.840
<v Speaker 5>ninety nine percent empty.

0:18:48.960 --> 0:18:51.960
<v Speaker 1>Yeah exactly. Now, normal matter clumps up a lot, right,

0:18:52.400 --> 0:18:56.080
<v Speaker 1>Like the Sun is an extraordinarily dense collection of normal matter.

0:18:56.160 --> 0:18:59.119
<v Speaker 1>Normal matter is not spread evenly through the galaxy. But

0:18:59.160 --> 0:19:01.640
<v Speaker 1>if you take dark man and spread it evenly through

0:19:01.640 --> 0:19:05.040
<v Speaker 1>the galaxy, you get a pretty small density. It's like

0:19:05.240 --> 0:19:08.680
<v Speaker 1>ten to the twenty six kilograms per cubic light year,

0:19:08.880 --> 0:19:12.240
<v Speaker 1>which is a huge volume, which means it's like ten

0:19:12.280 --> 0:19:16.280
<v Speaker 1>to the negative twenty two kilograms per cubic meter. So

0:19:16.320 --> 0:19:18.119
<v Speaker 1>then if you add up all the cubic meters in

0:19:18.160 --> 0:19:20.840
<v Speaker 1>the Earth, that adds up to about two thirds of

0:19:20.880 --> 0:19:24.480
<v Speaker 1>a kilogram of dark matter inside the volume of the Earth. Again,

0:19:24.560 --> 0:19:28.160
<v Speaker 1>assuming that dark matter is evenly spread throughout the galaxy,

0:19:28.160 --> 0:19:30.280
<v Speaker 1>which it probably isn't, but it might be.

0:19:30.320 --> 0:19:33.920
<v Speaker 5>Roughly, which is about the size or mass of a squirrel.

0:19:34.080 --> 0:19:37.240
<v Speaker 1>Yeah exactly, So one squirrel of dark matter inside the

0:19:37.280 --> 0:19:39.560
<v Speaker 1>volume of the Earth compared to you know, the many,

0:19:39.600 --> 0:19:42.679
<v Speaker 1>many millions and billions of kilograms of normal matter inside

0:19:42.680 --> 0:19:45.680
<v Speaker 1>the volume of the Earth. That sounds the importance of clumping, right,

0:19:45.680 --> 0:19:49.040
<v Speaker 1>Because normal matter clumps together, it's gravity is much more powerful.

0:19:49.200 --> 0:19:52.080
<v Speaker 1>In our local neighborhood, than dark matter. Even though dark

0:19:52.119 --> 0:19:55.480
<v Speaker 1>matter outweighs normal matter by nineteen to one, if it's

0:19:55.560 --> 0:19:58.160
<v Speaker 1>much more thinly spread out, the local effects of its

0:19:58.200 --> 0:19:59.880
<v Speaker 1>gravity are much harder to detect.

0:20:00.000 --> 0:20:02.240
<v Speaker 5>I think maybe what you're saying is that dark matter,

0:20:02.840 --> 0:20:06.160
<v Speaker 5>in terms of the universe scale, it mostly hangs out

0:20:06.200 --> 0:20:08.120
<v Speaker 5>in galaxies. Like you don't see a lot of dark

0:20:08.160 --> 0:20:10.680
<v Speaker 5>matter floating out there on its own between galaxies.

0:20:10.760 --> 0:20:12.720
<v Speaker 1>Yeah, we can do really precise measurements of where dark

0:20:12.720 --> 0:20:15.400
<v Speaker 1>matter is on the galaxy scale, because galaxies are really

0:20:15.440 --> 0:20:18.359
<v Speaker 1>really big. If we can tell how galaxies are orbiting

0:20:18.400 --> 0:20:20.600
<v Speaker 1>around each other, just the way we can tell how

0:20:20.680 --> 0:20:23.879
<v Speaker 1>stars are moving through the galaxy, so enormous clumps of

0:20:23.960 --> 0:20:26.840
<v Speaker 1>dark matter, absolutely, we can measure their gravity. But when

0:20:26.840 --> 0:20:29.040
<v Speaker 1>you zoom in in a really fine grained way and

0:20:29.080 --> 0:20:31.639
<v Speaker 1>want to say, hey, is there a moon sized blob

0:20:31.680 --> 0:20:34.000
<v Speaker 1>of dark matter anywhere in our solar system, that's a

0:20:34.000 --> 0:20:35.080
<v Speaker 1>tough question to answer.

0:20:35.160 --> 0:20:37.840
<v Speaker 5>So then within the galaxy, you're saying, like, there's a

0:20:37.880 --> 0:20:39.880
<v Speaker 5>lot of dark matter within our galaxy. Ninety five percent

0:20:39.920 --> 0:20:42.199
<v Speaker 5>of the mass of our galaxy is dark matter, And

0:20:42.240 --> 0:20:44.320
<v Speaker 5>what does it look like. Does it look like, you know,

0:20:44.600 --> 0:20:47.439
<v Speaker 5>an intense dense ball of dark matter in the middle,

0:20:48.000 --> 0:20:51.000
<v Speaker 5>is it evenly distributed? And also, like our galaxy looks

0:20:51.040 --> 0:20:53.119
<v Speaker 5>like a disc sort of like a flat disk, is

0:20:53.240 --> 0:20:55.040
<v Speaker 5>dark matter also shaped like a flat disk.

0:20:55.280 --> 0:20:57.560
<v Speaker 1>So we have the best answers the more we zoom out,

0:20:57.600 --> 0:21:00.000
<v Speaker 1>and then as we zoom in things get literally funny.

0:21:00.280 --> 0:21:02.560
<v Speaker 1>But on the scale of the galaxy we have some ideas.

0:21:02.920 --> 0:21:05.040
<v Speaker 1>We think that dark matter is like a big halo.

0:21:05.400 --> 0:21:08.680
<v Speaker 1>So imagine the visible galaxy right the edge of the stars.

0:21:09.160 --> 0:21:11.920
<v Speaker 1>Dark matter is a big halo that goes out beyond

0:21:12.040 --> 0:21:15.440
<v Speaker 1>the visible stars, and it's bigger and fuzzier. It hasn't

0:21:15.440 --> 0:21:17.919
<v Speaker 1>collapsed the way normal matter has because it just doesn't

0:21:17.920 --> 0:21:20.520
<v Speaker 1>clump right. In order to clump, things need other kinds

0:21:20.520 --> 0:21:23.119
<v Speaker 1>of interaction other than gravity. Like if you have two

0:21:23.200 --> 0:21:25.919
<v Speaker 1>dark matter particles they attract each other gravitationally and then

0:21:26.000 --> 0:21:28.240
<v Speaker 1>just passed right through each other. They're just gonna zig

0:21:28.280 --> 0:21:30.919
<v Speaker 1>and zag back and forth oscillate forever. They're not going

0:21:31.000 --> 0:21:34.000
<v Speaker 1>to clump together. To do that, you need like electromagnetism

0:21:34.080 --> 0:21:36.240
<v Speaker 1>or the strong force or something that wants to grab

0:21:36.280 --> 0:21:39.600
<v Speaker 1>onto each other. So dark matter stays a big puffy

0:21:39.640 --> 0:21:42.800
<v Speaker 1>halo and the galaxy is sort of embedded in that halo,

0:21:43.200 --> 0:21:45.800
<v Speaker 1>and that's not a coincidence. Right. The reason the galaxy

0:21:45.840 --> 0:21:49.080
<v Speaker 1>exists is because of a big dark matter blob there

0:21:49.280 --> 0:21:53.800
<v Speaker 1>that's gathered together all the hydrogen helium gravitationally and made

0:21:53.800 --> 0:21:56.720
<v Speaker 1>it into a galaxy. It's the reason we have stars, etc.

0:21:57.240 --> 0:21:59.960
<v Speaker 5>Now, when you say halo, you don't actually mean like

0:22:00.040 --> 0:22:02.520
<v Speaker 5>an angel's halo that looks like a ring. You actually

0:22:02.600 --> 0:22:04.000
<v Speaker 5>mean just like a blob, right.

0:22:03.960 --> 0:22:07.159
<v Speaker 1>Yeah, exactly, like a big fuzzy blob that extends out

0:22:07.200 --> 0:22:10.119
<v Speaker 1>further along the disc and then further above and below

0:22:10.200 --> 0:22:13.080
<v Speaker 1>the disc. But even that we know already is not

0:22:13.160 --> 0:22:14.080
<v Speaker 1>evenly distributed.

0:22:14.160 --> 0:22:16.800
<v Speaker 5>Is it like football shaped? Is it kind of flat?

0:22:16.960 --> 0:22:18.040
<v Speaker 5>Or is it a perfect sphere.

0:22:18.320 --> 0:22:20.840
<v Speaker 1>It's more like a hockey puck, right, It's flat, but

0:22:20.920 --> 0:22:22.920
<v Speaker 1>not as flat as the galaxy itself.

0:22:23.040 --> 0:22:23.879
<v Speaker 5>What made it flat?

0:22:24.000 --> 0:22:26.120
<v Speaker 1>Yeah, maybe a hockey puck is the wrong analogy. It's

0:22:26.119 --> 0:22:29.360
<v Speaker 1>not quite that flat. It's more like a big ellipsoid.

0:22:29.560 --> 0:22:31.280
<v Speaker 5>You mean like a slightly squished ball.

0:22:31.600 --> 0:22:35.800
<v Speaker 1>Yeah exactly. It's like a big basketball that somebody's sitting

0:22:35.840 --> 0:22:36.440
<v Speaker 1>on or something.

0:22:36.600 --> 0:22:38.960
<v Speaker 5>All right, Well, let's get a little bit more into

0:22:39.160 --> 0:22:41.600
<v Speaker 5>the details of what we know about dark matter, how

0:22:41.680 --> 0:22:43.600
<v Speaker 5>much of it can we see, how much can we

0:22:43.720 --> 0:22:47.720
<v Speaker 5>discern about what it's doing in our universe? And we'll

0:22:47.720 --> 0:22:50.080
<v Speaker 5>answer the question of whether you can use a quantum

0:22:50.119 --> 0:22:54.600
<v Speaker 5>clock from Amazon dot com to detect it. So we'll

0:22:54.640 --> 0:22:57.359
<v Speaker 5>get to those questions, but first let's take a quick break.

0:23:02.000 --> 0:23:05.000
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0:26:18.240 --> 0:26:21.360
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0:26:21.440 --> 0:26:25.480
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0:26:25.520 --> 0:26:28.119
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0:26:44.920 --> 0:26:48.359
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0:26:48.400 --> 0:26:51.200
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0:27:23.160 --> 0:27:25.400
<v Speaker 5>All right, we're asking the question can you use quantum

0:27:25.400 --> 0:27:29.080
<v Speaker 5>clocks to deteg dark matter? And we've been recapping a

0:27:29.080 --> 0:27:32.040
<v Speaker 5>little bit about what we know about dark matter, Daniel.

0:27:32.280 --> 0:27:34.520
<v Speaker 5>How much of the details of it can we see?

0:27:34.640 --> 0:27:38.080
<v Speaker 1>Not really very much. We have this sense of a big,

0:27:38.200 --> 0:27:42.919
<v Speaker 1>fuzzy halo that surrounds the galaxy, and we can also

0:27:43.000 --> 0:27:46.200
<v Speaker 1>measure the density as a function of distance from the center.

0:27:46.359 --> 0:27:48.800
<v Speaker 1>So if you're a star, for example, orbiting the center

0:27:48.840 --> 0:27:52.119
<v Speaker 1>of the galaxy, the speed at which you orbit depends

0:27:52.240 --> 0:27:55.600
<v Speaker 1>on the force that's holding you in that orbit. So

0:27:55.640 --> 0:27:58.639
<v Speaker 1>the stronger the force, the faster you can go, or

0:27:58.720 --> 0:28:00.520
<v Speaker 1>the faster you can go, the stronger the force that's

0:28:00.600 --> 0:28:03.240
<v Speaker 1>needed to hold you in that orbit. So by measuring

0:28:03.240 --> 0:28:06.159
<v Speaker 1>the speed of a given star, we can essentially measure

0:28:06.160 --> 0:28:08.720
<v Speaker 1>the mass of all that stuff that's holding on to

0:28:08.840 --> 0:28:10.800
<v Speaker 1>that star. So then if you look at stars at

0:28:10.800 --> 0:28:14.280
<v Speaker 1>different distances from the center, you can basically map out

0:28:14.359 --> 0:28:17.320
<v Speaker 1>the density of stuff in the galaxy as you go

0:28:17.560 --> 0:28:20.080
<v Speaker 1>further and closer to the center of the galaxy.

0:28:20.400 --> 0:28:23.359
<v Speaker 5>Like, if dark matter was super condensed in the middle

0:28:23.359 --> 0:28:26.400
<v Speaker 5>of the galaxy, then the stars in the galaxy we'd

0:28:26.440 --> 0:28:29.400
<v Speaker 5>be rotating a certain way. Or if the dark matter

0:28:29.520 --> 0:28:32.080
<v Speaker 5>was more spread out then the stars in the galaxy

0:28:32.080 --> 0:28:33.760
<v Speaker 5>we'd be rotating in a different way.

0:28:33.920 --> 0:28:36.720
<v Speaker 1>Yeah, exactly, if all the dark matter in the galaxy

0:28:36.880 --> 0:28:39.040
<v Speaker 1>was at the center, then everything would act in a

0:28:39.040 --> 0:28:41.000
<v Speaker 1>certain way, would just go like one over are squared.

0:28:41.000 --> 0:28:42.880
<v Speaker 1>It's sort of like the way the Solar system orbits

0:28:42.920 --> 0:28:44.960
<v Speaker 1>the Sun. But if you take some of that mass

0:28:44.960 --> 0:28:47.800
<v Speaker 1>and you spread it out through the galaxy instead, then

0:28:47.800 --> 0:28:50.160
<v Speaker 1>the dark matter that's further out than a given star

0:28:50.240 --> 0:28:53.440
<v Speaker 1>doesn't affect its orbit because it's gravity all cancels out.

0:28:53.680 --> 0:28:56.880
<v Speaker 1>So that changes the rotation speed of those stars, and

0:28:56.920 --> 0:28:59.720
<v Speaker 1>that's in fact how we first discover dark matter. Was

0:28:59.720 --> 0:29:02.600
<v Speaker 1>by looking at these rotation speeds of stars around the

0:29:02.600 --> 0:29:05.320
<v Speaker 1>center of the galaxy and seeing that we couldn't explain

0:29:05.360 --> 0:29:07.640
<v Speaker 1>it by mapping all the mass from the stars and

0:29:07.680 --> 0:29:09.560
<v Speaker 1>the gas and the dust. And that's exactly how you

0:29:09.560 --> 0:29:12.120
<v Speaker 1>can tell where you need to add more mass to

0:29:12.200 --> 0:29:14.960
<v Speaker 1>explain these rotation speeds. It's not just like, hey, add

0:29:14.960 --> 0:29:16.840
<v Speaker 1>a big blob of the center. You need to add

0:29:16.840 --> 0:29:18.920
<v Speaker 1>some of the center and also some further out and

0:29:19.000 --> 0:29:22.720
<v Speaker 1>some further out, and so precise measurements of those velocities

0:29:22.880 --> 0:29:25.160
<v Speaker 1>give you a fairly accurate picture of where the dark

0:29:25.200 --> 0:29:28.160
<v Speaker 1>matter is in the galaxy. And it's not evenly spread out.

0:29:28.320 --> 0:29:31.280
<v Speaker 1>It's more densely clumped at the center, which is something you'd.

0:29:31.080 --> 0:29:34.360
<v Speaker 5>Expect because it is affected by gravity, right.

0:29:34.200 --> 0:29:36.440
<v Speaker 1>It is, in the end affected by gravity, and so

0:29:36.560 --> 0:29:39.520
<v Speaker 1>it's pulled itself together. And the whole reason that this

0:29:39.680 --> 0:29:44.440
<v Speaker 1>exists is because of some like early universe perturbation where

0:29:44.440 --> 0:29:47.360
<v Speaker 1>you had a denser blob of dark matter that created

0:29:47.400 --> 0:29:50.240
<v Speaker 1>this whole well, gathered together the other dark matter and

0:29:50.280 --> 0:29:53.320
<v Speaker 1>created this over density which then pulled in hydrogen, helium

0:29:53.320 --> 0:29:56.440
<v Speaker 1>and whatever was around to make a galaxy. So it's

0:29:56.440 --> 0:29:58.600
<v Speaker 1>a little bit denser at the center, though it's not

0:29:58.840 --> 0:30:02.560
<v Speaker 1>very well understood, like if we do calculations simulations to

0:30:02.640 --> 0:30:05.160
<v Speaker 1>describe what we think should happen. If you have a

0:30:05.160 --> 0:30:06.920
<v Speaker 1>bunch of dark matter and you give it a few

0:30:06.960 --> 0:30:09.720
<v Speaker 1>billion years to fall together and to form some structure,

0:30:09.800 --> 0:30:12.880
<v Speaker 1>it describes what astronomers call a cusp, which means like

0:30:13.120 --> 0:30:14.959
<v Speaker 1>a point of high density of the center and then

0:30:15.080 --> 0:30:17.680
<v Speaker 1>very steeply falling should like drop off quickly. But if

0:30:17.680 --> 0:30:21.680
<v Speaker 1>you go out and measure the actual distributions of stars velocities,

0:30:21.960 --> 0:30:24.320
<v Speaker 1>you see something that looks like a bigger core. It's

0:30:24.320 --> 0:30:27.040
<v Speaker 1>not like it's pointing near the center. It's more spread

0:30:27.040 --> 0:30:30.600
<v Speaker 1>out in the inner galaxy. It's like flatter, and so

0:30:30.720 --> 0:30:32.760
<v Speaker 1>this is not something we understand very well. And it

0:30:32.760 --> 0:30:34.760
<v Speaker 1>also gives you a sense of like the scale of

0:30:34.840 --> 0:30:36.880
<v Speaker 1>which we can figure this stuff out. We're talking about

0:30:36.920 --> 0:30:40.000
<v Speaker 1>over light years distances, right, We're not resolving dark matter

0:30:40.080 --> 0:30:44.240
<v Speaker 1>in meters or even in aus with very very coarse

0:30:44.280 --> 0:30:47.120
<v Speaker 1>ways to measure where the dark matter is again, because

0:30:47.160 --> 0:30:48.360
<v Speaker 1>its gravity is so weak.

0:30:48.480 --> 0:30:51.000
<v Speaker 5>Are you saying like the beginning of the universe, dark

0:30:51.040 --> 0:30:53.760
<v Speaker 5>matter was more evenly spread out, like you know, all

0:30:53.800 --> 0:30:56.560
<v Speaker 5>those light years of empty space between US and Andromeda

0:30:56.600 --> 0:30:59.080
<v Speaker 5>and other galaxies was all filled with dark matter, and

0:30:59.120 --> 0:31:01.600
<v Speaker 5>then it all colleutes through certain clusters.

0:31:01.760 --> 0:31:04.600
<v Speaker 1>Yeah, it definitely gathered itself together. The early universe had

0:31:04.640 --> 0:31:08.360
<v Speaker 1>initial density fluctuations, and that's a whole big question about

0:31:08.400 --> 0:31:11.920
<v Speaker 1>where exactly that came from. And then those seated gravity

0:31:11.960 --> 0:31:15.360
<v Speaker 1>to pull things together. So gravity does form structure, but

0:31:15.440 --> 0:31:17.960
<v Speaker 1>it takes time. And so yeah, dark matter was more

0:31:18.000 --> 0:31:19.920
<v Speaker 1>spread out and now it's less spread out.

0:31:19.960 --> 0:31:21.880
<v Speaker 5>Why would dark matter stay stuck together?

0:31:22.080 --> 0:31:24.400
<v Speaker 1>Well, it's not that dark matter is sticking together. It's

0:31:24.440 --> 0:31:26.480
<v Speaker 1>not like it's bonded to itself. And again we don't

0:31:26.480 --> 0:31:29.080
<v Speaker 1>really know because we don't have a microscopic picture of

0:31:29.160 --> 0:31:31.800
<v Speaker 1>the dark matter. But I think you're asking, like, why

0:31:31.880 --> 0:31:34.880
<v Speaker 1>does dark matter form even gravitational structures? Like why does

0:31:34.920 --> 0:31:37.400
<v Speaker 1>it get more dense in some places and then in others?

0:31:37.520 --> 0:31:38.280
<v Speaker 1>Is that what you're asking?

0:31:38.480 --> 0:31:40.600
<v Speaker 5>Yeah, Like I'm imagining at the beginning of the universe

0:31:40.600 --> 0:31:43.440
<v Speaker 5>there's a bit of dark matter that was, you know,

0:31:43.560 --> 0:31:45.640
<v Speaker 5>let's say, ten light years away, and then it got

0:31:45.640 --> 0:31:48.760
<v Speaker 5>attracted to our galaxy, so it flew over here. But

0:31:48.840 --> 0:31:51.200
<v Speaker 5>then why didn't just keep flying to the other side.

0:31:51.360 --> 0:31:53.800
<v Speaker 1>Yeah, So as that distant piece of dark matter approaches

0:31:53.840 --> 0:31:58.040
<v Speaker 1>the galaxy, it gains velocity. Right, it's exchanging gravitational potential

0:31:58.120 --> 0:32:01.120
<v Speaker 1>energy for kinetic energy. And then you're imagining like the

0:32:01.120 --> 0:32:03.040
<v Speaker 1>way a ball rolls down a valley, why doesn't it

0:32:03.120 --> 0:32:05.800
<v Speaker 1>roll back up the other side? And it will, yes,

0:32:05.880 --> 0:32:08.760
<v Speaker 1>but then it comes back right, And so gravity in

0:32:08.800 --> 0:32:12.320
<v Speaker 1>the end is organizing something. There's the second piece to that,

0:32:12.440 --> 0:32:15.640
<v Speaker 1>which is that it doesn't completely roll back up the

0:32:15.640 --> 0:32:19.480
<v Speaker 1>other side. You know, anything that's accelerating is emitting gravitational

0:32:19.560 --> 0:32:22.960
<v Speaker 1>radiation for example. So the reason, for example, two black

0:32:23.000 --> 0:32:26.680
<v Speaker 1>holes orbiting each other will eventually spiral in and collapse

0:32:27.000 --> 0:32:29.960
<v Speaker 1>is that they're emitting gravitational energy. So none of these

0:32:30.000 --> 0:32:32.880
<v Speaker 1>things are really stable. So over long periods of time,

0:32:33.120 --> 0:32:37.320
<v Speaker 1>even without inelastic interactions like electromagnetism or whatever, these things

0:32:37.360 --> 0:32:41.680
<v Speaker 1>will form very large structures and they will gradually collapse

0:32:41.760 --> 0:32:43.200
<v Speaker 1>due to gravitational radiation.

0:32:43.560 --> 0:32:45.800
<v Speaker 5>All right, so we kind of have a fuzzy picture

0:32:45.840 --> 0:32:48.480
<v Speaker 5>of where it is in the universe. So now the

0:32:48.520 --> 0:32:51.280
<v Speaker 5>question of the episode is can we use quantum clocks

0:32:51.600 --> 0:32:55.000
<v Speaker 5>to detect dark matter? How do quantum clocks fit into this?

0:32:55.280 --> 0:32:57.920
<v Speaker 1>So quantum clocks might give us a sense for where

0:32:57.920 --> 0:33:00.560
<v Speaker 1>the dark matter is if we can find a place

0:33:00.640 --> 0:33:03.360
<v Speaker 1>where it's like clumpy, if we can find a place

0:33:03.520 --> 0:33:06.840
<v Speaker 1>in our solar system where it's like gathered together for

0:33:06.880 --> 0:33:09.440
<v Speaker 1>some reason. And that would be really cool, because not

0:33:09.480 --> 0:33:11.960
<v Speaker 1>only would it help us detect what dark matter is,

0:33:12.160 --> 0:33:14.880
<v Speaker 1>but it would help us understand where it is. It's

0:33:14.880 --> 0:33:16.960
<v Speaker 1>a really deep mystery. I think, not just because we

0:33:16.960 --> 0:33:18.960
<v Speaker 1>want to understand dark matter, but because we want like

0:33:18.960 --> 0:33:22.000
<v Speaker 1>a map. You know, humans are visual creatures. We want

0:33:22.040 --> 0:33:24.080
<v Speaker 1>to know like where the stuff is, and just not

0:33:24.320 --> 0:33:27.600
<v Speaker 1>knowing where dark matter is in the universe really bugs me.

0:33:27.680 --> 0:33:29.720
<v Speaker 1>So I would love to know where it is, and

0:33:30.200 --> 0:33:33.880
<v Speaker 1>understanding its map on a finer scale would be really helpful.

0:33:33.920 --> 0:33:36.400
<v Speaker 1>And quantum clocks might be able to help us map

0:33:36.600 --> 0:33:38.760
<v Speaker 1>where dark matter is if we can send them out

0:33:38.840 --> 0:33:42.640
<v Speaker 1>into space and if they're sensitive to dark matter, if

0:33:42.680 --> 0:33:45.680
<v Speaker 1>their operation changes as they pass through dark matter.

0:33:45.800 --> 0:33:47.280
<v Speaker 5>Okay, I think you're saying that you know, at the

0:33:47.320 --> 0:33:50.280
<v Speaker 5>galaxy level, we know that it looks like a big blob.

0:33:50.320 --> 0:33:52.360
<v Speaker 5>It's sort of like a switch ball. It's sort of

0:33:52.560 --> 0:33:55.120
<v Speaker 5>more intense or more dense in the center of the galaxy.

0:33:55.320 --> 0:33:57.440
<v Speaker 5>But I think maybe you're saying, can we know in

0:33:57.560 --> 0:34:02.360
<v Speaker 5>finer detail what it looks like between stars within the galaxy,

0:34:02.440 --> 0:34:05.200
<v Speaker 5>like is it clumpy, is it chunky, or is it

0:34:05.240 --> 0:34:06.040
<v Speaker 5>like peanut butter.

0:34:06.000 --> 0:34:10.480
<v Speaker 1>Smooth exactly, And people have tackled this problem in the past,

0:34:10.680 --> 0:34:13.600
<v Speaker 1>Like people use the technique you mentioned gravitation lensing to

0:34:13.640 --> 0:34:16.520
<v Speaker 1>look for blobs of dark matter, and that works, and

0:34:16.560 --> 0:34:19.400
<v Speaker 1>it's powerful, but only if you have like a really

0:34:19.480 --> 0:34:22.799
<v Speaker 1>nice galaxy behind the blob of dark matter that can

0:34:22.840 --> 0:34:25.040
<v Speaker 1>show you that it's there, so that tells us a

0:34:25.080 --> 0:34:27.200
<v Speaker 1>little bit about the dark matter density. But there aren't

0:34:27.239 --> 0:34:29.400
<v Speaker 1>like galaxies in all the right places to like X

0:34:29.520 --> 0:34:31.920
<v Speaker 1>ray the whole Solar system and figure out where it is.

0:34:32.000 --> 0:34:34.000
<v Speaker 1>And that technique isn't always powerful enough. You need like

0:34:34.040 --> 0:34:36.759
<v Speaker 1>a really big blob of dark matter. Another technique people

0:34:36.760 --> 0:34:40.000
<v Speaker 1>have used is to look for dwarf galaxies. Essentially, our

0:34:40.040 --> 0:34:43.560
<v Speaker 1>galaxy is formed by the combination of lots of galaxies, right,

0:34:43.760 --> 0:34:46.160
<v Speaker 1>we think galaxies formed kind of small and then grew

0:34:46.200 --> 0:34:49.480
<v Speaker 1>together with all sorts of absorptions and collisions. That means

0:34:49.520 --> 0:34:53.279
<v Speaker 1>that our galaxy has other like mini galaxies embedded within it.

0:34:53.680 --> 0:34:56.360
<v Speaker 1>Some of these we call dwarf galaxies because they're small,

0:34:56.560 --> 0:34:59.800
<v Speaker 1>and we think they're like very high dark matter density

0:34:59.400 --> 0:35:02.759
<v Speaker 1>therew stars, and so we can look at the motion

0:35:02.800 --> 0:35:05.480
<v Speaker 1>of the stars inside those little galaxies to get sensors

0:35:05.560 --> 0:35:08.080
<v Speaker 1>for like where those blobs are. But we don't have

0:35:08.120 --> 0:35:10.480
<v Speaker 1>a great way to like X ray the Solar System

0:35:10.520 --> 0:35:12.640
<v Speaker 1>and figure out, like where is the dark matter in

0:35:12.640 --> 0:35:15.239
<v Speaker 1>our Solar system? Is it hanging out by Jupiter? Is

0:35:15.239 --> 0:35:18.000
<v Speaker 1>it spread evenly like peanut butter? What's going on?

0:35:18.480 --> 0:35:21.120
<v Speaker 5>You want to know it's distribution at the Solar system

0:35:21.120 --> 0:35:21.880
<v Speaker 5>scale exactly.

0:35:21.960 --> 0:35:23.600
<v Speaker 1>That's what I want to do. And I read a

0:35:23.640 --> 0:35:26.239
<v Speaker 1>recent paper which was very clever, which is looking at

0:35:26.280 --> 0:35:29.520
<v Speaker 1>asteroids and trying to track asteroid trajectories and see if

0:35:29.560 --> 0:35:33.120
<v Speaker 1>like tiny little deviations in the trajectory of asteroids or

0:35:33.160 --> 0:35:36.480
<v Speaker 1>comets as they move through the Solar System could reveal

0:35:36.520 --> 0:35:38.960
<v Speaker 1>the presence of dark matter. It's very difficult to do

0:35:39.000 --> 0:35:41.640
<v Speaker 1>because if dark matter is evenly spread out or only

0:35:41.680 --> 0:35:44.560
<v Speaker 1>a little bit clumpy, that'd be basically no effect on

0:35:44.640 --> 0:35:47.080
<v Speaker 1>those asteroids. But it's the kind of thing that we're

0:35:47.160 --> 0:35:49.359
<v Speaker 1>just on the verge of being able to potentially do

0:35:49.480 --> 0:35:52.680
<v Speaker 1>now that we have better measurements and better computational tools

0:35:52.719 --> 0:35:56.640
<v Speaker 1>to try to like infer this information from really specific measurements.

0:35:56.719 --> 0:35:58.800
<v Speaker 5>All right, So then how would you use a quantum

0:35:58.800 --> 0:36:00.520
<v Speaker 5>clock to deteg dark matter?

0:36:00.640 --> 0:36:02.799
<v Speaker 1>So when we talk about a quantum clock, really what

0:36:02.840 --> 0:36:06.000
<v Speaker 1>we mean is something which is based on fundamental quantum

0:36:06.000 --> 0:36:08.719
<v Speaker 1>mechanical principles. And you know it sounds fancy, but even

0:36:08.800 --> 0:36:11.799
<v Speaker 1>just like an atomic clock, is a quantum clock. An

0:36:11.840 --> 0:36:14.440
<v Speaker 1>atomic clock is something that looks at like the oscillation

0:36:14.520 --> 0:36:17.480
<v Speaker 1>of electron between two energy levels and a caesium atom,

0:36:17.760 --> 0:36:21.840
<v Speaker 1>which is a very precise, very very regular process that

0:36:21.920 --> 0:36:25.160
<v Speaker 1>we can use essentially to tell how time has passed,

0:36:25.760 --> 0:36:29.320
<v Speaker 1>and so on Earth, we have extraordinarily precise atomic clocks

0:36:29.360 --> 0:36:31.960
<v Speaker 1>which now set the standard and in fact define what

0:36:32.000 --> 0:36:34.120
<v Speaker 1>we mean by a second. A second used to have

0:36:34.200 --> 0:36:36.960
<v Speaker 1>a different definition, but now a second is defined as

0:36:37.040 --> 0:36:39.800
<v Speaker 1>like a certain number of cycle of a specific kind

0:36:39.840 --> 0:36:44.200
<v Speaker 1>of atom. That's literally how we measure time now, and

0:36:44.280 --> 0:36:45.640
<v Speaker 1>so it's the standard.

0:36:46.120 --> 0:36:48.120
<v Speaker 5>It's like the minute, like it used to be like

0:36:48.160 --> 0:36:50.600
<v Speaker 5>a minute with sixty seconds, but now people say, oh,

0:36:50.640 --> 0:36:53.560
<v Speaker 5>it's been a minute to really mean something totally different.

0:36:57.560 --> 0:37:02.360
<v Speaker 1>Yes, it's just like that exactly, and we call it

0:37:02.360 --> 0:37:05.120
<v Speaker 1>a quantum clock because this really is a quantum process

0:37:05.120 --> 0:37:08.400
<v Speaker 1>we're talking about quantum particles. There's an electron, there's an atom.

0:37:08.600 --> 0:37:11.640
<v Speaker 1>The electron is moving in the potential well of the atom,

0:37:11.719 --> 0:37:15.120
<v Speaker 1>so it's interacting electromagnetically with the nucleus. And the way

0:37:15.120 --> 0:37:17.720
<v Speaker 1>that it's moving, the way it oscillates between energy levels,

0:37:17.920 --> 0:37:21.120
<v Speaker 1>is completely controlled by quantum processes. This is not a

0:37:21.120 --> 0:37:23.680
<v Speaker 1>clock that you could have in a perfectly classical universe.

0:37:23.920 --> 0:37:26.320
<v Speaker 1>You know, if we lived in a universe where electrons

0:37:26.320 --> 0:37:28.799
<v Speaker 1>really were tiny little balls that went to orbits and

0:37:28.840 --> 0:37:31.960
<v Speaker 1>had smooth classical paths the way planets do, then this

0:37:32.000 --> 0:37:34.680
<v Speaker 1>clock could not exist. And so that's when we meet

0:37:34.719 --> 0:37:35.800
<v Speaker 1>by quantum clock.

0:37:36.040 --> 0:37:38.160
<v Speaker 5>But I guess, if it's a quantum clock, doesn't it

0:37:38.239 --> 0:37:41.560
<v Speaker 5>have a certain amount of uncertainty to it or unknowability?

0:37:41.840 --> 0:37:45.280
<v Speaker 5>How can it be precise if there's the Heisenberg uncertainty principle.

0:37:46.560 --> 0:37:49.920
<v Speaker 1>Yeah, you're right, there's no absolutely precise quantum clock. But

0:37:50.080 --> 0:37:52.520
<v Speaker 1>this is about as regular as it gets. And amazingly,

0:37:52.640 --> 0:37:56.120
<v Speaker 1>these quantum clocks are more precise than mechanical clocks, which

0:37:56.120 --> 0:37:58.880
<v Speaker 1>of course also have uncertainty in them, because no mechanical

0:37:58.920 --> 0:38:02.040
<v Speaker 1>device is perfect created, right, And so this is as

0:38:02.080 --> 0:38:04.520
<v Speaker 1>accurate as they've been able to make them, and recently

0:38:04.520 --> 0:38:07.920
<v Speaker 1>they've been even able to make them small and transportable.

0:38:08.160 --> 0:38:10.279
<v Speaker 1>You might think of an atomic clock as like some

0:38:10.480 --> 0:38:13.839
<v Speaker 1>huge device in the basement of a laboratory in Colorado

0:38:14.080 --> 0:38:16.520
<v Speaker 1>that weighs like ten tons and fills a room. But

0:38:16.640 --> 0:38:18.840
<v Speaker 1>actually these things can be made quite small.

0:38:19.120 --> 0:38:21.680
<v Speaker 5>So a quantum clock is really just an atomic clock

0:38:21.800 --> 0:38:24.160
<v Speaker 5>or is there another kind that doesn't use atoms?

0:38:24.239 --> 0:38:26.480
<v Speaker 1>There's no atomic clock that's not a quantum clock. So

0:38:26.560 --> 0:38:29.280
<v Speaker 1>quantum clock is just a fancier sounding name for atomic clock.

0:38:29.360 --> 0:38:31.800
<v Speaker 5>Yes, can you have a quantum clock that maybe doesn't

0:38:31.880 --> 0:38:34.799
<v Speaker 5>use an atom, that maybe just relies on electrons or

0:38:34.960 --> 0:38:35.800
<v Speaker 5>quarks or something.

0:38:35.960 --> 0:38:38.840
<v Speaker 1>Yeah, sure, you're not limited to atoms. You can imagine

0:38:38.920 --> 0:38:42.280
<v Speaker 1>quantum clocks made out of like photons interacting or splitting

0:38:42.360 --> 0:38:45.760
<v Speaker 1>or bouncing or something like that. In some sense, lego

0:38:46.000 --> 0:38:49.320
<v Speaker 1>is a clock because it's measuring the time for photons

0:38:49.360 --> 0:38:52.680
<v Speaker 1>to travel along its legs, right, it's just converting that

0:38:52.760 --> 0:38:55.440
<v Speaker 1>to a distance measurement. And so you could have other

0:38:55.520 --> 0:38:58.000
<v Speaker 1>quantum clocks that are not based on atoms. Yes, And

0:38:58.040 --> 0:39:00.000
<v Speaker 1>one day, when we discover dark matter, maybe we could

0:39:00.080 --> 0:39:01.640
<v Speaker 1>build a clock out of dark.

0:39:01.440 --> 0:39:04.759
<v Speaker 5>Matter, which may or may not tell you the time.

0:39:05.120 --> 0:39:07.120
<v Speaker 1>And may or may not smell like flatulence.

0:39:07.320 --> 0:39:09.000
<v Speaker 5>Well, I guess maybe give us an example of, like

0:39:09.040 --> 0:39:12.800
<v Speaker 5>what's a typical or popular or a commonly used quantum

0:39:12.800 --> 0:39:13.879
<v Speaker 5>clock and how does it work.

0:39:14.160 --> 0:39:16.920
<v Speaker 1>Well, the most precise quantum clock is based on the

0:39:16.920 --> 0:39:20.080
<v Speaker 1>caesium one thirty three atom. That's the one that's actually

0:39:20.120 --> 0:39:23.360
<v Speaker 1>used to define what a second is. And so here

0:39:23.400 --> 0:39:26.400
<v Speaker 1>we have two states of electrons. There's a small splitting

0:39:26.440 --> 0:39:28.840
<v Speaker 1>in an energy in state here. It's called a hyper

0:39:28.880 --> 0:39:31.640
<v Speaker 1>fine splitting because the difference is very very small, and

0:39:31.680 --> 0:39:33.439
<v Speaker 1>when the electron sits in there, it sort of goes

0:39:33.480 --> 0:39:36.320
<v Speaker 1>back and forth between the two different states.

0:39:36.120 --> 0:39:39.400
<v Speaker 5>Meaning like, this is an electron that's orbiting around the

0:39:39.440 --> 0:39:40.240
<v Speaker 5>caesium atom.

0:39:40.480 --> 0:39:42.520
<v Speaker 1>Yeah, I wouldn't say orbiting if we want to be

0:39:42.560 --> 0:39:45.360
<v Speaker 1>really really technical, But it's captured by the caesium atom.

0:39:45.560 --> 0:39:47.840
<v Speaker 5>And you're saying it's switching energy levels. Why would it

0:39:47.840 --> 0:39:48.880
<v Speaker 5>switch energy levels?

0:39:49.080 --> 0:39:51.279
<v Speaker 1>So you have this caesium atom and you embed the

0:39:51.280 --> 0:39:53.839
<v Speaker 1>whole thing in some microwave radiation that can lift those

0:39:53.880 --> 0:39:56.799
<v Speaker 1>electrons up from the lower state to the higher.

0:39:56.480 --> 0:39:58.600
<v Speaker 5>State, meaning you like put it in a microwave or

0:39:58.680 --> 0:40:00.600
<v Speaker 5>you shoot it with it like a light gun.

0:40:01.560 --> 0:40:03.799
<v Speaker 1>There's not a difference, right, that's what a microwave is.

0:40:03.840 --> 0:40:06.960
<v Speaker 1>A microwave is shooting microwave radiation at your food, and

0:40:07.080 --> 0:40:10.640
<v Speaker 1>microwaves are lights. Though basically a microwave is a light gun.

0:40:10.880 --> 0:40:13.240
<v Speaker 5>Sounds hot. So then you have this atom and you

0:40:13.239 --> 0:40:14.280
<v Speaker 5>you stick it in the microwave.

0:40:14.320 --> 0:40:16.640
<v Speaker 1>Uh huh, yeah, So you stick in the microwave and

0:40:16.719 --> 0:40:18.839
<v Speaker 1>you measure how often it jumps up and then down

0:40:18.920 --> 0:40:19.840
<v Speaker 1>and then up and then.

0:40:19.719 --> 0:40:23.000
<v Speaker 5>Down because the light, as the light passes through it,

0:40:23.000 --> 0:40:25.319
<v Speaker 5>it knocks the electron up and down or what.

0:40:25.560 --> 0:40:28.319
<v Speaker 1>Yeah, the light is tuned to exactly the frequency for

0:40:28.360 --> 0:40:31.680
<v Speaker 1>the electron to jump up into the higher energy level. Remember,

0:40:31.719 --> 0:40:33.920
<v Speaker 1>electrons can go from a lower to a higher energy

0:40:33.960 --> 0:40:36.520
<v Speaker 1>level if a photon of the right energy comes along.

0:40:36.880 --> 0:40:40.320
<v Speaker 1>So they've tuned this microwave to exactly that energy level.

0:40:40.520 --> 0:40:43.320
<v Speaker 1>So electrons and the lower level can absorb these photons

0:40:43.400 --> 0:40:45.640
<v Speaker 1>jump up to the higher level. But then they'll naturally

0:40:45.680 --> 0:40:49.120
<v Speaker 1>decay down because the universe likes to spread energy out

0:40:49.320 --> 0:40:51.880
<v Speaker 1>and so the time of these oscillations turns out to

0:40:51.920 --> 0:40:55.000
<v Speaker 1>be very very regular, Like an electron will do this

0:40:55.239 --> 0:40:58.840
<v Speaker 1>nine point one nine two billion times per second.

0:40:59.000 --> 0:41:01.359
<v Speaker 5>And it doesn't depend on the frequency of the light,

0:41:01.480 --> 0:41:01.879
<v Speaker 5>or it does.

0:41:02.000 --> 0:41:03.920
<v Speaker 1>It definitely depends on the frequency of the light. If

0:41:03.920 --> 0:41:06.239
<v Speaker 1>the frequency of the light is not correct, then it

0:41:06.239 --> 0:41:08.080
<v Speaker 1>won't even absorb it, right, it won't happen.

0:41:08.360 --> 0:41:11.080
<v Speaker 5>Oh, but then don't you need to make that frequency

0:41:11.239 --> 0:41:11.960
<v Speaker 5>super precise?

0:41:12.120 --> 0:41:14.600
<v Speaker 1>Yeah, exactly, And this is one source of uncertainty in

0:41:14.640 --> 0:41:18.000
<v Speaker 1>these clocks, right, making those accurate. And you can measure

0:41:18.000 --> 0:41:20.200
<v Speaker 1>these things, like you build two independent ones, you can

0:41:20.239 --> 0:41:23.279
<v Speaker 1>see how their counts drift relative to each other. And

0:41:23.680 --> 0:41:26.000
<v Speaker 1>that's how you measure the accuracy of clocks. In general.

0:41:26.040 --> 0:41:28.279
<v Speaker 1>There's no absolute standard by which you can tell like, oh,

0:41:28.280 --> 0:41:30.120
<v Speaker 1>this clock is off or that clock is off. You

0:41:30.239 --> 0:41:31.719
<v Speaker 1>just build a few of them and you measure them

0:41:31.760 --> 0:41:34.160
<v Speaker 1>relative to each other. And this is something that we

0:41:34.280 --> 0:41:36.520
<v Speaker 1>know well enough. We know how to design the mean

0:41:36.640 --> 0:41:39.120
<v Speaker 1>of the physics and the engineering that you can build

0:41:39.120 --> 0:41:43.160
<v Speaker 1>these things so that atomic clocks in independent locations agree

0:41:43.520 --> 0:41:46.879
<v Speaker 1>to zero point three nanoseconds per day. It's really very

0:41:46.880 --> 0:41:47.880
<v Speaker 1>incredibly precise.

0:41:48.320 --> 0:41:51.000
<v Speaker 5>WHOA, so what are you measuring? How are you measuring

0:41:51.040 --> 0:41:53.000
<v Speaker 5>whether these electrons are going up and down?

0:41:53.080 --> 0:41:55.919
<v Speaker 1>When the electron goes back down. It emits radiation, right,

0:41:55.960 --> 0:41:57.920
<v Speaker 1>and so you can gather that as well.

0:41:57.880 --> 0:41:59.960
<v Speaker 5>Like it shoots off light like an a blink.

0:41:59.680 --> 0:42:01.800
<v Speaker 1>Basically exactly little flash.

0:42:01.920 --> 0:42:04.040
<v Speaker 5>All right. So then, and you're saying you can build

0:42:04.160 --> 0:42:06.520
<v Speaker 5>these things now to be the size of a toaster

0:42:07.080 --> 0:42:09.160
<v Speaker 5>or a microwave oven.

0:42:09.760 --> 0:42:12.760
<v Speaker 1>A quantum toaster. They have them now and they've deployed

0:42:12.800 --> 0:42:15.480
<v Speaker 1>them out in space. They actually built the Deep Space

0:42:15.560 --> 0:42:18.359
<v Speaker 1>Atomic Clock Mission and they sent an atomic clock out

0:42:18.400 --> 0:42:20.759
<v Speaker 1>into space to see, like, hey, can we operate one

0:42:20.840 --> 0:42:23.080
<v Speaker 1>of these things out in space? And you might wonder

0:42:23.120 --> 0:42:25.319
<v Speaker 1>like is this just a bunch of nerds trying to

0:42:25.360 --> 0:42:29.160
<v Speaker 1>do something that seems cool? Yes, is always the answer.

0:42:28.920 --> 0:42:31.879
<v Speaker 5>Like can we shoot a microwave into space and will

0:42:31.880 --> 0:42:35.319
<v Speaker 5>it still heat up my burrito? My season Burritoah? Is

0:42:35.320 --> 0:42:35.960
<v Speaker 5>that the challenge?

0:42:35.960 --> 0:42:38.160
<v Speaker 1>That's the challenge. But also if we want to do

0:42:38.280 --> 0:42:42.120
<v Speaker 1>things like navigate in space, navigation needs timing. You need

0:42:42.160 --> 0:42:44.480
<v Speaker 1>to know like how long you're going in one direction.

0:42:44.719 --> 0:42:46.319
<v Speaker 1>If you want to do dead reckoning, you want to

0:42:46.360 --> 0:42:49.480
<v Speaker 1>know where you are. Timing is absolutely crucial. Or if

0:42:49.480 --> 0:42:53.200
<v Speaker 1>you want to use like nearby pulsars to triangulate your position,

0:42:53.440 --> 0:42:55.799
<v Speaker 1>I have whole episode about how that works. You also

0:42:55.880 --> 0:42:58.319
<v Speaker 1>need very accurate timing so you can measure the time

0:42:58.360 --> 0:43:01.400
<v Speaker 1>between the pulses. So this was like a technological challenge

0:43:01.440 --> 0:43:03.840
<v Speaker 1>that's going to lay the groundwork for all sorts of

0:43:03.840 --> 0:43:06.919
<v Speaker 1>cool innovations, and this was totally successful in this deep

0:43:06.960 --> 0:43:08.360
<v Speaker 1>space atomic clock mission.

0:43:08.560 --> 0:43:11.000
<v Speaker 5>Well, let's get into how you would actually use these

0:43:11.239 --> 0:43:14.759
<v Speaker 5>and how the timing might tell you where dark matter

0:43:14.880 --> 0:43:18.760
<v Speaker 5>is within our Solar system and maybe even within the Earth.

0:43:18.880 --> 0:43:21.320
<v Speaker 5>So let's dig into that. But first, let's take another

0:43:21.360 --> 0:43:22.160
<v Speaker 5>quick break.

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0:44:10.200 --> 0:44:12.000
<v Speaker 1>When you pop a piece of cheese into your mouth

0:44:12.120 --> 0:44:15.240
<v Speaker 1>or enjoy a rich spoonful of Greek yogurt, you're probably

0:44:15.280 --> 0:44:19.320
<v Speaker 1>not thinking about the environmental impact of each and every bite,

0:44:19.360 --> 0:44:22.000
<v Speaker 1>But the people in the dairy industry are. US Dairy

0:44:22.040 --> 0:44:26.319
<v Speaker 1>has set themselves some ambitious sustainability goals, including being greenhouse

0:44:26.360 --> 0:44:28.919
<v Speaker 1>gas neutral by twenty to fifty. That's why they're working

0:44:28.960 --> 0:44:31.279
<v Speaker 1>hard every day to find new ways to reduce waste,

0:44:31.360 --> 0:44:35.600
<v Speaker 1>conserve natural resources, and drive down greenhouse gas emissions. Take water,

0:44:35.640 --> 0:44:38.720
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<v Speaker 5>All right. We're talking about using a microwave stuck inside

0:46:53.400 --> 0:46:55.920
<v Speaker 5>of a microwave to the tech dark matter so you

0:46:55.960 --> 0:46:59.120
<v Speaker 5>can win a Tierra for being the prettiest scientist.

0:47:00.080 --> 0:47:02.600
<v Speaker 1>Exactly does it take longer to heat up your burrito

0:47:02.680 --> 0:47:04.120
<v Speaker 1>when there's dark matter around?

0:47:04.400 --> 0:47:06.799
<v Speaker 5>So the idea is that you take these atomic or

0:47:07.080 --> 0:47:09.759
<v Speaker 5>basically an atomic clock, which is a quantum clock. But

0:47:10.640 --> 0:47:13.480
<v Speaker 5>it seems like the most popular ones use atoms, and

0:47:13.520 --> 0:47:15.560
<v Speaker 5>so you shrink them down to the size of a

0:47:15.600 --> 0:47:17.560
<v Speaker 5>toaster or microwave, and then you shoot them in space.

0:47:17.600 --> 0:47:19.680
<v Speaker 5>And then how does that help you measure dark matter?

0:47:20.440 --> 0:47:22.400
<v Speaker 1>Well, there were a bunch of physicists who thought, Okay,

0:47:22.440 --> 0:47:25.040
<v Speaker 1>this is cool because now we not only have all

0:47:25.120 --> 0:47:28.319
<v Speaker 1>some super precise atomic clocks, but now we have them

0:47:28.320 --> 0:47:30.960
<v Speaker 1>spread out through the Solar system, like in principle the

0:47:30.960 --> 0:47:32.880
<v Speaker 1>way we like scent devices near the Sun with a

0:47:32.920 --> 0:47:35.439
<v Speaker 1>Parker solar probe. People are like, what if we built

0:47:35.480 --> 0:47:37.319
<v Speaker 1>a bunch of these things and we spread them out

0:47:37.360 --> 0:47:39.640
<v Speaker 1>in the Solar system? Could they give us a picture

0:47:39.680 --> 0:47:42.320
<v Speaker 1>of where the dark matter is in the Solar system?

0:47:42.760 --> 0:47:46.040
<v Speaker 1>If they operate differently when there's dark matter around, like

0:47:46.040 --> 0:47:48.880
<v Speaker 1>if they're sensitive to the dark matter density, Like if

0:47:48.920 --> 0:47:52.319
<v Speaker 1>your atomic clock gets off if it drifts when there's

0:47:52.360 --> 0:47:54.960
<v Speaker 1>more or less dark matter around, than having a bunch

0:47:55.000 --> 0:47:57.760
<v Speaker 1>of these atomic clocks spread out through the Solar system

0:47:57.880 --> 0:48:00.000
<v Speaker 1>could give you a picture for where in the Solar

0:48:00.080 --> 0:48:01.359
<v Speaker 1>System the dark matter is.

0:48:02.040 --> 0:48:05.160
<v Speaker 5>But I guess what's the mechanism by which dark matter

0:48:05.200 --> 0:48:07.520
<v Speaker 5>would affect the timing of these clocks.

0:48:07.719 --> 0:48:10.600
<v Speaker 1>Yeah, so mostly it wouldn't For many theories of dark matter.

0:48:10.680 --> 0:48:13.880
<v Speaker 1>Dark matter is just some whimp. It's a massive particle

0:48:13.920 --> 0:48:17.120
<v Speaker 1>that only interacts gravitationally, and so it has essentially no

0:48:17.239 --> 0:48:20.960
<v Speaker 1>effect on these clocks except for gravitational time dilation. We

0:48:21.040 --> 0:48:23.759
<v Speaker 1>know the areas with greater mass have more curvature, and

0:48:23.840 --> 0:48:26.440
<v Speaker 1>a curvature causes time dilation, but that would be very,

0:48:26.520 --> 0:48:29.200
<v Speaker 1>very difficult to measure even with these quantum clocks.

0:48:29.239 --> 0:48:30.800
<v Speaker 5>But wait, why would it be difficult.

0:48:30.880 --> 0:48:33.880
<v Speaker 1>You can measure gravitational time dilation with quantum clocks, and

0:48:33.880 --> 0:48:36.040
<v Speaker 1>we've done that. You can do it on the surface

0:48:36.040 --> 0:48:37.960
<v Speaker 1>of the Earth, for example, and you can put a

0:48:38.040 --> 0:48:41.040
<v Speaker 1>quantum clock one meter above another one and you can

0:48:41.120 --> 0:48:43.680
<v Speaker 1>see the difference between them because one of them is

0:48:43.760 --> 0:48:46.840
<v Speaker 1>deeper in the curvature than the other. Super duper awesome,

0:48:47.080 --> 0:48:49.120
<v Speaker 1>but that's because the Earth has a huge amount of

0:48:49.120 --> 0:48:52.880
<v Speaker 1>gravity and this significant curvature. Here. Dark matter doesn't contribute

0:48:52.880 --> 0:48:56.600
<v Speaker 1>significantly to the curvature because it's pretty spread out. And

0:48:56.719 --> 0:48:59.560
<v Speaker 1>we would already know if dark matter wasn't pretty spread out,

0:48:59.680 --> 0:49:02.239
<v Speaker 1>because we would have seen deviations and like Jupiter's orbit

0:49:02.320 --> 0:49:05.000
<v Speaker 1>and whatever. So in principle you can, but we don't

0:49:05.040 --> 0:49:06.719
<v Speaker 1>think it's going to be very sensitive. If you had

0:49:06.760 --> 0:49:09.160
<v Speaker 1>a lot of quantum clocks and there were much more sensitive,

0:49:09.320 --> 0:49:12.879
<v Speaker 1>then you could probably detect dark matter local density variations

0:49:13.160 --> 0:49:14.120
<v Speaker 1>using that principle.

0:49:14.320 --> 0:49:18.520
<v Speaker 5>Meaning these clocks would tick at a different frequency depending

0:49:18.680 --> 0:49:21.920
<v Speaker 5>on how close it was to big sources of mass

0:49:22.040 --> 0:49:24.640
<v Speaker 5>or even light sources of mass, because that's just how

0:49:24.719 --> 0:49:25.560
<v Speaker 5>relativity works.

0:49:25.680 --> 0:49:27.920
<v Speaker 1>Yeah, that's how relativity works. Remember, in relativity, it is

0:49:27.960 --> 0:49:30.840
<v Speaker 1>two kinds of time dilation. One is based on speed.

0:49:30.840 --> 0:49:33.279
<v Speaker 1>If you see a clock moving quickly, then you see

0:49:33.280 --> 0:49:36.719
<v Speaker 1>it ticking slowly, and that's very confusing because it's relative,

0:49:36.760 --> 0:49:39.160
<v Speaker 1>and so it depends on two observers. But there's another

0:49:39.280 --> 0:49:42.759
<v Speaker 1>kind of time dilation, gravitational, which is absolute. It just

0:49:42.800 --> 0:49:46.280
<v Speaker 1>says anybody in curature their clock is going to tick slowly,

0:49:46.480 --> 0:49:48.360
<v Speaker 1>no matter who's looking at it, and everybody's going to

0:49:48.440 --> 0:49:51.359
<v Speaker 1>agree about whose clock is ticking slowly. So that's very

0:49:51.400 --> 0:49:54.520
<v Speaker 1>powerful and that's something you can use to measure just

0:49:54.600 --> 0:49:57.680
<v Speaker 1>like how much stuff is there in general, because clocks

0:49:57.680 --> 0:50:01.080
<v Speaker 1>tick slower near stuff. Really kind of awesome feature of.

0:50:01.040 --> 0:50:03.120
<v Speaker 5>The universe, meaning like if I had two of these

0:50:03.120 --> 0:50:05.000
<v Speaker 5>atomic clocks and one of them is out there in

0:50:05.000 --> 0:50:07.400
<v Speaker 5>the middle of empty space, and the other one is

0:50:07.480 --> 0:50:09.520
<v Speaker 5>near a big blob of dark matter. The one near

0:50:09.560 --> 0:50:13.080
<v Speaker 5>the blob of dark matter would take slower.

0:50:12.800 --> 0:50:14.560
<v Speaker 1>Right, Yeah, that's exactly right.

0:50:14.600 --> 0:50:16.719
<v Speaker 5>And so you might like start them out in the

0:50:16.760 --> 0:50:20.480
<v Speaker 5>same spot. But then after being for a while and

0:50:20.480 --> 0:50:22.360
<v Speaker 5>two different spots, one near the dark matter, and you

0:50:22.400 --> 0:50:24.080
<v Speaker 5>brun them back, you would see that one of them

0:50:24.600 --> 0:50:26.040
<v Speaker 5>take more ticks than the other.

0:50:26.239 --> 0:50:28.719
<v Speaker 1>Yeah. And so now imagine like a grid, you have

0:50:28.760 --> 0:50:32.239
<v Speaker 1>a quantum clock every ten meters in the solar system, right,

0:50:32.320 --> 0:50:34.000
<v Speaker 1>you start them all out at the same time, and

0:50:34.000 --> 0:50:36.200
<v Speaker 1>then you monitor it, and by measuring the difference in

0:50:36.239 --> 0:50:39.160
<v Speaker 1>that number of ticks after a year on your reference clock,

0:50:39.200 --> 0:50:41.399
<v Speaker 1>the one that's hanging out with you, you can tell

0:50:41.440 --> 0:50:43.799
<v Speaker 1>where stuff is in the solar system.

0:50:43.680 --> 0:50:47.440
<v Speaker 5>Like which spots in the solar system have slower time.

0:50:47.280 --> 0:50:51.120
<v Speaker 1>Yes, exactly, because slower time means more matter, more curvature,

0:50:51.239 --> 0:50:52.200
<v Speaker 1>more energy density.

0:50:52.239 --> 0:50:54.600
<v Speaker 5>Really, I guess, on top of what you already know

0:50:54.719 --> 0:50:57.839
<v Speaker 5>about the Solar system right like right now, even if

0:50:57.880 --> 0:51:01.000
<v Speaker 5>we didn't have dark matter, a clock near the Sun

0:51:01.040 --> 0:51:03.120
<v Speaker 5>would takes lower than a clock here exactly.

0:51:03.320 --> 0:51:05.640
<v Speaker 1>And we've done some basic version of this, as I

0:51:05.680 --> 0:51:08.919
<v Speaker 1>said earlier, if a few clocks on Earth at different altitudes.

0:51:09.360 --> 0:51:11.560
<v Speaker 1>Those are different distances from the matter of the Earth,

0:51:11.600 --> 0:51:14.840
<v Speaker 1>and the ones closer do ticks more slowly, And satellites

0:51:14.960 --> 0:51:18.440
<v Speaker 1>up in space their clocks tick faster than atomic clocks

0:51:18.440 --> 0:51:19.680
<v Speaker 1>here on the surface of the Earth, And you've got

0:51:19.719 --> 0:51:22.560
<v Speaker 1>to take that new account famously when you're doing GPS,

0:51:22.600 --> 0:51:23.040
<v Speaker 1>et cetera.

0:51:23.239 --> 0:51:26.360
<v Speaker 5>But you're saying, we're not going to be using this effect,

0:51:26.560 --> 0:51:29.799
<v Speaker 5>this time dilation from relativity to measure dark matter. Dark

0:51:29.840 --> 0:51:30.960
<v Speaker 5>matter is just too weak.

0:51:31.120 --> 0:51:32.759
<v Speaker 1>Dark matter is too weak, and we think it's not

0:51:32.880 --> 0:51:34.960
<v Speaker 1>cluppy enough to really detect that, though it would be

0:51:35.000 --> 0:51:38.320
<v Speaker 1>super awesome. There's a special kind of dark matter which

0:51:38.520 --> 0:51:41.480
<v Speaker 1>might give much larger effects, which would be much easier

0:51:41.520 --> 0:51:44.880
<v Speaker 1>to discover. And this is a theory called fuzzy dark matter.

0:51:45.280 --> 0:51:50.080
<v Speaker 5>Sounds fuzzy. But wait, so you're saying, like this idea

0:51:50.080 --> 0:51:53.120
<v Speaker 5>of using atomic clocks to measure dark matter would only

0:51:53.160 --> 0:51:59.800
<v Speaker 5>work for a certain theoretical meaning guessie type of dark matter,

0:52:00.000 --> 0:52:01.880
<v Speaker 5>which we don't know whether it's true or not, or

0:52:01.920 --> 0:52:02.440
<v Speaker 5>exist or not.

0:52:02.560 --> 0:52:03.000
<v Speaker 4>Mm hmmm.

0:52:03.239 --> 0:52:06.600
<v Speaker 5>So this is a huge sources in white scheme that

0:52:07.480 --> 0:52:08.879
<v Speaker 5>you don't really know if it's going to work.

0:52:08.960 --> 0:52:10.879
<v Speaker 1>You know, you were talking about nomenclature and now you're

0:52:10.920 --> 0:52:13.680
<v Speaker 1>using the words guess and scheme, you know, really kind

0:52:13.680 --> 0:52:15.920
<v Speaker 1>of undermine the credibility of science. But you know, this

0:52:16.120 --> 0:52:18.359
<v Speaker 1>is good faith stuff. This is like, hey, what if

0:52:18.400 --> 0:52:21.319
<v Speaker 1>dark matter is this other weird particular thing, how could

0:52:21.320 --> 0:52:23.239
<v Speaker 1>we see that? And yet it'd be best if we

0:52:23.280 --> 0:52:25.960
<v Speaker 1>had experiments which could detect any kind of dark matter,

0:52:26.080 --> 0:52:27.839
<v Speaker 1>But you know, there might be kinds of dark matter

0:52:27.880 --> 0:52:30.400
<v Speaker 1>which we could only detect in certain ways or easier

0:52:30.440 --> 0:52:32.239
<v Speaker 1>to spot in some ways. And so it's good to

0:52:32.239 --> 0:52:35.200
<v Speaker 1>be creative and think about how we could detect specific

0:52:35.360 --> 0:52:37.640
<v Speaker 1>kinds of dark matter as well, even though we don't

0:52:37.680 --> 0:52:40.160
<v Speaker 1>know what dark matter is. And if this theory is at.

0:52:40.040 --> 0:52:42.880
<v Speaker 5>All correct, well, I'm just trying to understand the scheme.

0:52:45.080 --> 0:52:47.279
<v Speaker 5>So are you saying there's a theoretical kind of dark

0:52:47.320 --> 0:52:49.359
<v Speaker 5>matter called fuzzy dark matter? So what is it?

0:52:49.400 --> 0:52:49.520
<v Speaker 4>So?

0:52:49.640 --> 0:52:53.400
<v Speaker 1>Fuzzy dark matter suggests that maybe dark matter isn't very massive,

0:52:53.800 --> 0:52:56.279
<v Speaker 1>like some people suggest that dark matter could be like

0:52:56.320 --> 0:52:58.920
<v Speaker 1>one hundred GeV like the mass of a w or

0:52:58.960 --> 0:53:01.640
<v Speaker 1>a z boson, like one hundred times the mass of

0:53:01.640 --> 0:53:05.040
<v Speaker 1>a proton, a pretty hefty particle, almost as massive as

0:53:05.040 --> 0:53:08.040
<v Speaker 1>a Higgs. That's sort of the classic strategy, and there's

0:53:08.080 --> 0:53:10.960
<v Speaker 1>reasons for that. There's something called the Wimp miracle. Check

0:53:11.000 --> 0:53:14.239
<v Speaker 1>on our podcast about that, which argues strongly that dark

0:53:14.280 --> 0:53:16.839
<v Speaker 1>matter should be around one hundred gv based on how

0:53:16.920 --> 0:53:19.200
<v Speaker 1>much of it there is in the universe. But people

0:53:19.200 --> 0:53:20.719
<v Speaker 1>are like, well, maybe that's all wrong, and there's an

0:53:20.760 --> 0:53:23.240
<v Speaker 1>assumption there that's wrong. What if dark matter is super

0:53:23.360 --> 0:53:26.759
<v Speaker 1>duper light, like a trilliance the mass of an electron.

0:53:26.960 --> 0:53:30.320
<v Speaker 1>So now there's an enormous number of these dark matter particles,

0:53:30.360 --> 0:53:33.000
<v Speaker 1>so many more than you could even imagine, because you

0:53:33.040 --> 0:53:35.799
<v Speaker 1>have to somehow make like a big fraction of the

0:53:35.800 --> 0:53:38.600
<v Speaker 1>mass of the universe out of particles that are a

0:53:38.640 --> 0:53:41.319
<v Speaker 1>tiny fraction in the mass of the electron, which is

0:53:41.360 --> 0:53:42.680
<v Speaker 1>already very very light.

0:53:42.880 --> 0:53:45.040
<v Speaker 5>Well, first of all, I think this whole podcast is

0:53:45.080 --> 0:53:49.000
<v Speaker 5>a Wimp miracle, Daniel. But I think you're saying, like

0:53:49.239 --> 0:53:52.360
<v Speaker 5>this version of dark matter, instead of being maybe marble

0:53:52.440 --> 0:53:56.160
<v Speaker 5>sized particles, they're like super tiny BB sized particles, And

0:53:56.239 --> 0:53:57.480
<v Speaker 5>some of that makes it fuzzier.

0:53:57.600 --> 0:53:59.759
<v Speaker 1>Yeah, it makes it fuzzier because if they're very very

0:53:59.760 --> 0:54:03.480
<v Speaker 1>low mass, then their wavelengths are more spread out. Some

0:54:03.520 --> 0:54:05.720
<v Speaker 1>of these things can have a wavelength like the size

0:54:05.760 --> 0:54:06.480
<v Speaker 1>of the galaxy.

0:54:06.760 --> 0:54:07.759
<v Speaker 5>What do you mean a wavelength.

0:54:07.960 --> 0:54:10.400
<v Speaker 1>The wavelength of a particle is like the distance on

0:54:10.440 --> 0:54:14.239
<v Speaker 1>which these quantum interference effects appear, and so you can

0:54:14.280 --> 0:54:17.520
<v Speaker 1>calculate this quantity. It's called the Debrogely wavelength. You'll see

0:54:17.560 --> 0:54:21.160
<v Speaker 1>wave like effects for a particle when you interact over

0:54:21.200 --> 0:54:24.320
<v Speaker 1>these kinds of distances, and that's the wavelength of a particle.

0:54:24.120 --> 0:54:25.560
<v Speaker 5>Meaning sort of like the size of it.

0:54:25.680 --> 0:54:27.880
<v Speaker 1>Kind of right, sort of, Yeah, it's when it stops

0:54:27.880 --> 0:54:30.560
<v Speaker 1>acting like a blob like a particle and starts acting

0:54:30.600 --> 0:54:34.080
<v Speaker 1>more like a wave. Things that have wavelike behaviors. Really

0:54:34.120 --> 0:54:36.120
<v Speaker 1>it's always acting like a wave. It's just that when

0:54:36.120 --> 0:54:38.880
<v Speaker 1>you zoom out you can approximate it as a particle.

0:54:38.560 --> 0:54:41.359
<v Speaker 5>Because they have low mass. What's the relationship between having

0:54:41.360 --> 0:54:43.960
<v Speaker 5>low mass and being having big wavelengths.

0:54:44.200 --> 0:54:46.800
<v Speaker 1>Well, the wavelength depends on your momentum and your mass.

0:54:47.000 --> 0:54:50.719
<v Speaker 1>So lower mass just means a larger wavelength because it's

0:54:50.760 --> 0:54:53.600
<v Speaker 1>really like a ratio between the momentum and the mass.

0:54:53.640 --> 0:54:55.759
<v Speaker 1>When things have a lot of kinetic energy relative to

0:54:55.760 --> 0:54:58.480
<v Speaker 1>their mass, they act more like light because light is

0:54:58.560 --> 0:55:01.960
<v Speaker 1>pure kinetic energy. Have very small amounts of energy relative

0:55:02.000 --> 0:55:04.600
<v Speaker 1>to their mass their stationary so they act more like

0:55:04.760 --> 0:55:07.600
<v Speaker 1>bits of sand like particles. And so it's just sort

0:55:07.640 --> 0:55:10.760
<v Speaker 1>of a rough way to understand where that transition happens.

0:55:11.040 --> 0:55:13.040
<v Speaker 5>Okay, so then if dark matter is this kind of

0:55:13.040 --> 0:55:15.920
<v Speaker 5>fuzzy kind of dark matter, you're saying that each particle

0:55:15.920 --> 0:55:18.839
<v Speaker 5>would be super super light, and it would also have

0:55:19.080 --> 0:55:22.560
<v Speaker 5>huge variations in their size. That's what you mean by fuzzy.

0:55:22.600 --> 0:55:24.520
<v Speaker 5>It's like they might be some of them might be

0:55:24.600 --> 0:55:26.240
<v Speaker 5>super big and somewhere might be super small.

0:55:26.520 --> 0:55:29.000
<v Speaker 1>Yeah, well, the wavelengths could be very very large, which

0:55:29.040 --> 0:55:31.879
<v Speaker 1>means they can interact over long distances. The fascinating thing

0:55:32.000 --> 0:55:34.800
<v Speaker 1>is that in simulations of this dark matter, it predicts

0:55:35.080 --> 0:55:37.880
<v Speaker 1>like a mini halo of dark matter in our Solar system,

0:55:37.960 --> 0:55:40.719
<v Speaker 1>essentially that this stuff would be clumped up in and

0:55:41.040 --> 0:55:43.520
<v Speaker 1>near the Sun. That most of the dark matter in

0:55:43.560 --> 0:55:46.839
<v Speaker 1>the Solar System might be like clumped up near the Sun.

0:55:46.920 --> 0:55:48.720
<v Speaker 1>It might be like hiding in the Sun.

0:55:49.320 --> 0:55:51.359
<v Speaker 5>And if it wasn't this kind of fuzzy dark matter,

0:55:51.400 --> 0:55:51.960
<v Speaker 5>it wouldn't.

0:55:52.200 --> 0:55:54.479
<v Speaker 1>Now, this kind of fuzzy dark matter is the kind

0:55:54.520 --> 0:55:57.280
<v Speaker 1>we think would clump up like a halo near the Sun.

0:55:57.400 --> 0:55:58.480
<v Speaker 5>And the other kinds wouldn't.

0:55:58.520 --> 0:56:01.000
<v Speaker 1>Yeah, the other kinds wouldn't. As I mean, I've heard

0:56:01.040 --> 0:56:03.560
<v Speaker 1>of other theories of dark matter clumping in the Sun.

0:56:03.600 --> 0:56:06.840
<v Speaker 1>There's all sorts of theories, but this particular one tends

0:56:06.840 --> 0:56:09.680
<v Speaker 1>to make a halo near the Sun and would affect

0:56:09.719 --> 0:56:13.080
<v Speaker 1>the operation of quantum clocks because of its special fuzziness.

0:56:13.200 --> 0:56:16.600
<v Speaker 1>It can also slightly interact with electrons through sort of

0:56:16.600 --> 0:56:19.200
<v Speaker 1>like a back door in quantum mechanics, which would change

0:56:19.200 --> 0:56:21.760
<v Speaker 1>the way a quantum clock operates. It's like it changes

0:56:21.800 --> 0:56:25.320
<v Speaker 1>the electrons' mass and how it responds to photons because

0:56:25.320 --> 0:56:29.160
<v Speaker 1>of oscillations in this fuzzy dark matter field, and so

0:56:29.280 --> 0:56:32.839
<v Speaker 1>effectively it changes the frequency of these clocks. And so

0:56:32.920 --> 0:56:35.960
<v Speaker 1>you can detect in principle whether you're near a dense

0:56:36.040 --> 0:56:39.239
<v Speaker 1>blob of this ultra light dark matter by looking at

0:56:39.280 --> 0:56:42.160
<v Speaker 1>a quantum clock and counting its ticks very carefully. And

0:56:42.200 --> 0:56:44.120
<v Speaker 1>this would be a bigger effect than the effect we

0:56:44.400 --> 0:56:46.600
<v Speaker 1>talked about earlier, the gravitational curvature.

0:56:46.719 --> 0:56:49.320
<v Speaker 5>But I thought that dark matter couldn't interact with regular

0:56:49.360 --> 0:56:51.920
<v Speaker 5>matter only through it could only do it through gravity.

0:56:52.000 --> 0:56:54.400
<v Speaker 1>Yeah, it could only do it through gravity in general,

0:56:54.440 --> 0:56:56.680
<v Speaker 1>But this one takes a back door through the Higgs field.

0:56:57.000 --> 0:56:59.200
<v Speaker 1>It like interacts with the Higgs field and it changes

0:56:59.239 --> 0:57:01.880
<v Speaker 1>how the Higgs field works. And so near the presence

0:57:01.920 --> 0:57:04.600
<v Speaker 1>of this ultra light dark matter, electrons effectively have a

0:57:04.600 --> 0:57:05.440
<v Speaker 1>different mass.

0:57:06.440 --> 0:57:08.680
<v Speaker 5>But I guess if that was true, wouldn't we see

0:57:08.920 --> 0:57:11.840
<v Speaker 5>it affect regular matter on a larger scale.

0:57:11.880 --> 0:57:13.760
<v Speaker 1>You would see it happen, but it's a subtle effect,

0:57:13.960 --> 0:57:16.000
<v Speaker 1>and so you need to be near a dense clump

0:57:16.080 --> 0:57:18.920
<v Speaker 1>of it. So the idea is, take something that's very

0:57:19.000 --> 0:57:21.560
<v Speaker 1>very sensitive to the electron mass, like a quantum clock,

0:57:21.720 --> 0:57:23.760
<v Speaker 1>and try to put it near a dense clump of

0:57:23.800 --> 0:57:26.800
<v Speaker 1>this special ultra light dark matter, maybe near the Sun.

0:57:27.400 --> 0:57:29.240
<v Speaker 1>So that's the idea is, like launch a bunch of

0:57:29.320 --> 0:57:31.919
<v Speaker 1>quantum clocks, have them orbit near the Sun, and look

0:57:31.960 --> 0:57:35.160
<v Speaker 1>for deviations in their timekeeping and see if that's evidence

0:57:35.280 --> 0:57:38.560
<v Speaker 1>for ultra light dark matter interfering with the masses of

0:57:38.560 --> 0:57:40.520
<v Speaker 1>the electrons in these quantum clocks.

0:57:40.640 --> 0:57:42.520
<v Speaker 5>We mean that you would maybe like throw a bunch

0:57:42.600 --> 0:57:45.360
<v Speaker 5>of the sun, have them kind of form a half

0:57:45.480 --> 0:57:48.320
<v Speaker 5>ring around the Sun to see if time changes there,

0:57:48.520 --> 0:57:50.640
<v Speaker 5>sort of like a giant tirra.

0:57:50.880 --> 0:57:53.960
<v Speaker 1>Like a giant tr a quantum cosmic tiara.

0:57:54.160 --> 0:57:56.200
<v Speaker 5>All right, but I guess which one would you be proving.

0:57:56.240 --> 0:57:59.240
<v Speaker 5>Would you be proving that dark matter is fuzzy or

0:57:59.320 --> 0:58:02.320
<v Speaker 5>would you be proved that it's there? Or are they

0:58:02.320 --> 0:58:02.960
<v Speaker 5>both related?

0:58:03.160 --> 0:58:04.000
<v Speaker 1>They're both related.

0:58:04.040 --> 0:58:04.200
<v Speaker 4>Though.

0:58:04.280 --> 0:58:06.560
<v Speaker 1>You know, if we saw this thing, there would instantly

0:58:06.600 --> 0:58:09.360
<v Speaker 1>be like fifty other theories to explain it as well.

0:58:09.640 --> 0:58:12.320
<v Speaker 1>It probably wouldn't be a unique prediction of this kind

0:58:12.360 --> 0:58:14.960
<v Speaker 1>of dark matter. Theories are very very clever people, and

0:58:14.960 --> 0:58:17.240
<v Speaker 1>they'll always come up with another way to explain the

0:58:17.320 --> 0:58:20.120
<v Speaker 1>data that we're seeing. But it's cool because it's a

0:58:20.120 --> 0:58:22.480
<v Speaker 1>prediction that this theory makes and we go out and

0:58:22.520 --> 0:58:24.920
<v Speaker 1>we see it. That's really fascinating, and then we can

0:58:24.960 --> 0:58:27.440
<v Speaker 1>think about ways to distinguish all the different ideas that

0:58:27.520 --> 0:58:30.880
<v Speaker 1>might also explain this kind of observation. It would just

0:58:30.880 --> 0:58:33.360
<v Speaker 1>be cool to see something different. Currently, all of our

0:58:33.440 --> 0:58:37.120
<v Speaker 1>dark matter experiments basically see nothing. It would be cool

0:58:37.160 --> 0:58:38.400
<v Speaker 1>to have a signal somewhere.

0:58:39.280 --> 0:58:41.040
<v Speaker 5>So you're thinking, hey, let's put up a bunch of

0:58:41.040 --> 0:58:43.880
<v Speaker 5>microways in space and see if at sticks exactly.

0:58:43.960 --> 0:58:45.880
<v Speaker 1>Let's see if one burrito is a little bit colder

0:58:45.880 --> 0:58:46.360
<v Speaker 1>than another.

0:58:46.680 --> 0:58:49.360
<v Speaker 5>All right, Well, an interesting idea for how we could

0:58:49.360 --> 0:58:54.200
<v Speaker 5>maybe possibly crack sort of a theoretical version of one

0:58:54.240 --> 0:58:55.960
<v Speaker 5>of the biggest mysteries in the universe.

0:58:56.160 --> 0:58:58.480
<v Speaker 1>That's right. Physicists are being very creative and trying to

0:58:58.480 --> 0:59:00.840
<v Speaker 1>come up with new theories of dark matter and new

0:59:00.880 --> 0:59:04.680
<v Speaker 1>ways to discover them, including using super duper sets in

0:59:04.680 --> 0:59:08.240
<v Speaker 1>and quantum clocks distributed through the solar system, which also

0:59:08.400 --> 0:59:09.400
<v Speaker 1>would just be fun to do.

0:59:09.720 --> 0:59:11.520
<v Speaker 5>You just want to parade, Daniel, I.

0:59:11.480 --> 0:59:14.200
<v Speaker 1>Just want a tiara? Is that too much to ask?

0:59:16.200 --> 0:59:17.760
<v Speaker 5>How about we just buy you a tiara?

0:59:18.200 --> 0:59:20.040
<v Speaker 1>Is it made of dark matter? Are you using your bitcoin?

0:59:20.200 --> 0:59:22.120
<v Speaker 5>It can be, but in any way that you want.

0:59:23.120 --> 0:59:26.360
<v Speaker 5>But if it saves tax dollars billions of dollars, you know,

0:59:26.400 --> 0:59:27.600
<v Speaker 5>it would be a pretty good investment.

0:59:27.680 --> 0:59:29.840
<v Speaker 1>Yeah, there we go. That was my scheme the whole time.

0:59:30.000 --> 0:59:33.280
<v Speaker 5>Yeah, to get us to buy you a tiara without

0:59:33.280 --> 0:59:35.080
<v Speaker 5>actually having to run in a beauty contest.

0:59:36.520 --> 0:59:37.160
<v Speaker 1>I'm busted.

0:59:38.240 --> 0:59:42.120
<v Speaker 5>Well, you are the most beautiful podcaster with a show

0:59:42.160 --> 0:59:44.960
<v Speaker 5>called Daniel Jorge is playing the universe. So whose name

0:59:45.000 --> 0:59:45.600
<v Speaker 5>is Daniels?

0:59:45.760 --> 0:59:47.920
<v Speaker 1>I'll take very highly qualified compliments, thank you.

0:59:49.280 --> 0:59:53.320
<v Speaker 5>It's a very specific tiara based on a very theoretical

0:59:54.040 --> 0:59:55.320
<v Speaker 5>model of the.

0:59:55.320 --> 0:59:57.040
<v Speaker 1>Universe fuzzy compliments from Warhead.

0:59:57.240 --> 0:59:59.320
<v Speaker 5>All right, well, we hope you enjoyed that. Thanks for

0:59:59.400 --> 1:00:01.400
<v Speaker 5>joining us. See you next time.

1:00:06.120 --> 1:00:09.000
<v Speaker 1>For more science and curiosity, come find us on social

1:00:09.000 --> 1:00:14.000
<v Speaker 1>media where we answer questions and post videos. We're on Twitter, Disport, Instant,

1:00:14.040 --> 1:00:17.840
<v Speaker 1>and now TikTok. Thanks for listening and remember that Daniel

1:00:17.880 --> 1:00:21.320
<v Speaker 1>and Jorge Explain the Universe is a production of iHeartRadio.

1:00:21.600 --> 1:00:26.760
<v Speaker 1>For more podcasts from iHeartRadio, visit the iHeartRadio app, Apple Podcasts,

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