WEBVTT - Can Dark Matter feel itself

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<v Speaker 1>Hey, Daniel, what's the best question anyone has ever asked

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<v Speaker 1>you about dark matter? Well, it's tough to pick. There's

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<v Speaker 1>so many good ones. But I remember a nine year

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<v Speaker 1>old who read our book once and emailed me to

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<v Speaker 1>ask is dark matter bad matter? It must be a

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<v Speaker 1>Star Wars fan. You know the dark side doesn't sound

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<v Speaker 1>very friendly. Yeah, dark matter sounds world of unfriendly and mean.

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<v Speaker 1>It's doesn't never a really good pr team. Well, you know,

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<v Speaker 1>if there are dark matter physicists out there that we

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<v Speaker 1>can't see or touch, what do you think they would

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<v Speaker 1>call us? M I guess they'll probably call us dork matter.

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<v Speaker 1>We wouldn't seem dark to them and insidious. No, actually

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<v Speaker 1>we would. I mean if they have their own dark photons,

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<v Speaker 1>they wouldn't see ours, so we would be dark to them. Man,

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<v Speaker 1>I can just imagine the conferences. You know, you just

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<v Speaker 1>spent the whole day saying you're a dark matter. No,

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<v Speaker 1>you're a dark matter. That's probably actually true. That's exactly

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<v Speaker 1>what would happen. I am, forhand, a cartoonist and the

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<v Speaker 1>creator of PhD comments. Hi, I'm Daniel Whitson, I'm a

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<v Speaker 1>particle physicist, and I'm mostly made out of dork particles. Particles,

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<v Speaker 1>dark dork particles. That's the worst. Well, mostly in the

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<v Speaker 1>summer right now. I'm not going outside very much, so

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<v Speaker 1>pale dark. My dork particles are not very dark. But

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<v Speaker 1>welcome to our podcast Daniel and Jorge Explain the Universe,

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<v Speaker 1>a production of I Heart Radio, in which we take

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<v Speaker 1>you on a mental tour of the universe, zooming down

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<v Speaker 1>to see what the universe is made out of, what

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<v Speaker 1>it looks like at its largest scale, what crazy weird

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<v Speaker 1>stuff we encounter in it, and how we can all

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<v Speaker 1>understand it because humanity is on a journey, a journey

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<v Speaker 1>to understand this universe. We started out really kind of

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<v Speaker 1>clueless about the way things work, and we slowly put

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<v Speaker 1>together little pieces of the picture. But we're here to

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<v Speaker 1>give you a tour of what we have figured out

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<v Speaker 1>and what still remains unknown. Yeah, and it turns out

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<v Speaker 1>we haven't even left the garage, it seems, Daniel, in

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<v Speaker 1>our journey of discovery, because a huge percentage of the

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<v Speaker 1>universe is made out of stuff that we have no

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<v Speaker 1>idea about. You know, twenty five percent of the universe

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<v Speaker 1>is made out of something we call dark matter, which

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<v Speaker 1>is a huge mystery. Right, that's right, And that might

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<v Speaker 1>seem a bit deflating to you, like, wow, we haven't

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<v Speaker 1>figured anything out, But to me that's exciting, Like, wow,

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<v Speaker 1>we haven't figured anything out, which means more discoveries are

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<v Speaker 1>to come, which means mind blowing revelations about the true

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<v Speaker 1>nature of the universe are in our future. You know,

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<v Speaker 1>if you haven't left the garage, that means you can

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<v Speaker 1>still go back inside. If you forget something that's positive,

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<v Speaker 1>that's right, Like you forgot to pack your banana. How

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<v Speaker 1>can you even take a journey of discovery without banana?

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<v Speaker 1>About these days, who can go anywhere? Yeah, we're talking

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<v Speaker 1>about dark matter today and it's a huge mystery and

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<v Speaker 1>it's out there. But a big question is what is

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<v Speaker 1>it made out of? What is it? Is it a fluid,

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<v Speaker 1>is it a an energy? Or is it made out

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<v Speaker 1>of particles or something totally different. That's right, Everything we've

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<v Speaker 1>ever experienced, everything you've ever eaten or touched or tasted,

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<v Speaker 1>are made out of quarks and electrons and stuff like that,

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<v Speaker 1>and so we wonder does the same thing hold for

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<v Speaker 1>dark matter. But it's a pretty big extrapolation. I mean,

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<v Speaker 1>the kind of matter that we're made out of that's

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<v Speaker 1>very familiar, is unusual in the universe, and so it

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<v Speaker 1>seems kind of odd to extrapolate from this tiny little

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<v Speaker 1>corner to a huge fraction of the universe. And so

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<v Speaker 1>particle physicists think maybe it's made of particles, but I

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<v Speaker 1>like to think, hey, maybe it's made of something totally

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<v Speaker 1>weird and new. Yeah, we really have no idea. And

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<v Speaker 1>it's there's five times more dark matter in the universe

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<v Speaker 1>than there is of the stuff that we are made

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<v Speaker 1>out of. And it really could be anything like it

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<v Speaker 1>could be something that's not even a particle. That's right,

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<v Speaker 1>we've never seen matter that's not made of particles. Everything

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<v Speaker 1>we've ever experienced can be broken down into these units.

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<v Speaker 1>But that doesn't mean that everything is like that, Right.

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<v Speaker 1>We have to be very careful about generalizing. We've seen

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<v Speaker 1>so many times in physics when we've learned something we thought, oh,

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<v Speaker 1>this must be the way everything works, and then we

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<v Speaker 1>discover it's not. Actually and there are bigger stories, is

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<v Speaker 1>a larger context, and that's the goal of science, is

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<v Speaker 1>to reveal the actual truth, not just confirm our expectations. Yeah,

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<v Speaker 1>and so one thing we know about dark matter is

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<v Speaker 1>that we know that it feels gravity, because that's how

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<v Speaker 1>we know that it's there. I mean, we can't see it,

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<v Speaker 1>it's dark, but we know it's there because of gravity.

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<v Speaker 1>It's keeping the gaxies together, it's pulling things together, and

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<v Speaker 1>it's you know, affecting the trajectories of galaxies and stars.

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<v Speaker 1>So we know it feels gravity. We certainly do. It's

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<v Speaker 1>basically an invention to explain missing gravity. It's like a

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<v Speaker 1>gravity fudge factor. Yeah. We see things in the universe

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<v Speaker 1>that gravity has done, and we don't see the source

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<v Speaker 1>of that gravity. We're like, what's this invisible thing that's

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<v Speaker 1>making this gravity? And so dark matter is basically an

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<v Speaker 1>explanation for this gravity that we do observe, and so

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<v Speaker 1>it has to feel gravity otherwise it doesn't fit the

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<v Speaker 1>bill at all. But then the question is what else

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<v Speaker 1>does it do? Does it feel anything else? Does it

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<v Speaker 1>feel lonely? Does it feel resentful that we call it

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<v Speaker 1>dark matter? Yeah, we know that it feels gravity, and

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<v Speaker 1>so the question is does it feel any other forces?

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<v Speaker 1>And I think more interestingly about this question is does

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<v Speaker 1>it feel itself like canna bump into itself? Yeah, And

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<v Speaker 1>we got a really interesting question from a listener. Here's

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<v Speaker 1>an email I god from Joe from China, who I

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<v Speaker 1>think really put his finger on the question. He says,

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<v Speaker 1>if you were to take two particles of dark matter

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<v Speaker 1>and let them go in a vacuum, the gravity would

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<v Speaker 1>attract the two particles together. But then would they pass

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<v Speaker 1>right through each other and keep moving? Eventually would they

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<v Speaker 1>settle down and be able to share the same point

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<v Speaker 1>in space like overlapping? Can too dark matter particles? But

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<v Speaker 1>I guess bump into each other or occupy the same space? Yeah?

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<v Speaker 1>Do they not into each other and push back? Do

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<v Speaker 1>they pass right through each other? Can they sit right

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<v Speaker 1>on top of each other. It's a really fascinating question,

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<v Speaker 1>and it goes right to the heart of the sort

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<v Speaker 1>of the science matter of whether dark matter feels itself?

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<v Speaker 1>This question blow your mind a little bit? Yeah, I

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<v Speaker 1>did blow my mind a little bit. I just love

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<v Speaker 1>when somebody asks a new question, a question I haven't

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<v Speaker 1>heard before, or asks it in a new way. So

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<v Speaker 1>I haven't really thought about whether dark matter feels itself? Okay,

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<v Speaker 1>so it's kind of a funny question. Does dark matter

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<v Speaker 1>feel itself? That means that you know it feels itself. Gravitationally, right,

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<v Speaker 1>if you have one bit of dark matter here and

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<v Speaker 1>a bit of dark matter, they're they're gonna be They're

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<v Speaker 1>going to feel each other. They're gonna be attracted to

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<v Speaker 1>each other by gravity. But the question is, you know

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<v Speaker 1>what happens after they feel attracted by gravity. You know,

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<v Speaker 1>they they're moving towards each other. Are they gonna bump

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<v Speaker 1>against and and repel it themselves or are they going

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<v Speaker 1>to pass through each other? Or are they going to

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<v Speaker 1>stick together? Yeah, it's a great question. I mean, if

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<v Speaker 1>you and I have gravitational attraction, if we were out

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<v Speaker 1>in the middle of space, then gravity would very slowly

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<v Speaker 1>pulls together and we would bump into each other. I

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<v Speaker 1>wouldn't phase through each other. You woul get uncomfortable really fast.

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<v Speaker 1>What you're saying more awkward than in space. No one

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<v Speaker 1>can hear you say, hey, I need more space, Daniel,

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<v Speaker 1>get off me. But you couldn't write. You'd be stuck together.

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<v Speaker 1>That's right, we need some other kind of force. But

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<v Speaker 1>you and I do have other kind of forces, right,

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<v Speaker 1>the electromagnetic force who keep us from passing through each other.

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<v Speaker 1>So it's a good way to ask the questions. Yeah,

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<v Speaker 1>so the question is does dark matter feel itself? And so,

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<v Speaker 1>as usual, we went out into the world, and in

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<v Speaker 1>this case, the Internet, to see how many people felt

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<v Speaker 1>that they knew the answer to this question. That's right,

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<v Speaker 1>So thank you to everybody who volunteered to answer random

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<v Speaker 1>Internet physics questions. If you'd like to volunteer right to

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<v Speaker 1>us at questions at Daniel and Jorge dot com. Yeah,

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<v Speaker 1>you can ask us questions or get questions from us.

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<v Speaker 1>Questions in and questions out. It's an eternal flux of questions, right.

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<v Speaker 1>But think about it for a second. If you were

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<v Speaker 1>to try to answer the question does dark matter feel itself?

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<v Speaker 1>What would you answer? And no googling, no googling? What?

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<v Speaker 1>How about? Wikipedia? Also not allowed? About calling my physicist friend?

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<v Speaker 1>Totally allowed, totally allowed. All right, Well, here's what people

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<v Speaker 1>on the Internet had to say. I guess I'm really

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<v Speaker 1>not sure. I know that some scientists hypothesize the dark

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<v Speaker 1>matter is comprised of filaments, and if there were these

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<v Speaker 1>filaments in the dark matter, one would think that they

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<v Speaker 1>would interact in some way. I really don't think so.

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<v Speaker 1>I remember it interacting with something visible. That's a good one.

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<v Speaker 1>The interaction between light matter and dark matter is for

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<v Speaker 1>obviously still figuring that out, but I would think that

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<v Speaker 1>it does interact with itself. I don't think that turn

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<v Speaker 1>dark matter interacts with itself. Um. I think whether discussed

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<v Speaker 1>two galaxies colliding with each other, but there wasn't an

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<v Speaker 1>evidence or the details, so not itself. I would guess

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<v Speaker 1>that dark matter would interact with itself because I know

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<v Speaker 1>that one guess of what dark matter is is the

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<v Speaker 1>dark matter particle axion. And it's kind of hard to

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<v Speaker 1>visualize how a particle can pass through another particle. I

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<v Speaker 1>don't know. I've never thought about it. Okay, Um, dark

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<v Speaker 1>matter and dark energy confuse me a little bit. I

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<v Speaker 1>thought that dark matter was just a theory, and so

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<v Speaker 1>it's like we've we've seen something out there, and the

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<v Speaker 1>theory is that this dark matter, but we don't really know.

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<v Speaker 1>I don't think it can interact with normal matter. I

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<v Speaker 1>surely if it could pass through itself, we would be

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<v Speaker 1>able to see it. It might be a dark force,

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<v Speaker 1>which helps them incorrect. I know it doesn't interact with

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<v Speaker 1>regular matter. I think we don't know whether how it

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<v Speaker 1>interacts with itself. It is matter, so it has maths

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<v Speaker 1>al must interact gravitationally. I don't know. Well, I think

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<v Speaker 1>it does on some level. I don't know whether there

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<v Speaker 1>would be quantum or molecular, but I think it's got

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<v Speaker 1>to interact with itself enough to come together and blobs

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<v Speaker 1>big enough to cause gravitational lensing that we can see

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<v Speaker 1>here from Earth. I guess it's interact with yourself, since

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<v Speaker 1>it's i've gravity. All right, pretty thoughtful answers, you know,

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<v Speaker 1>people sort of thoughts through it. Yeah, there's some good

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<v Speaker 1>stuff in here. People are really thinking about what it

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<v Speaker 1>means to interact and whether gravity counts, and whether gravity

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<v Speaker 1>would make something bump or not? Does gravity count? Does

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<v Speaker 1>the Earth feel USh? Yeah? But also some people getting

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<v Speaker 1>confused about dark energy versus dark matter. That's another rabbit

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<v Speaker 1>hole there. Does dark energy feel? What is dark energy? Anyway?

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<v Speaker 1>We have no idea, all right, So the question is

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<v Speaker 1>that does dark matter feel? And so Daniel Um maybe

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<v Speaker 1>step us through what we know about dark matter and

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<v Speaker 1>it's it's not very sensitive. Unfortunately, you know, we wish

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<v Speaker 1>you would react more. Oh good, that's a good thing,

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<v Speaker 1>right as a thick skin. Well, perhaps know if you

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<v Speaker 1>want to get along with your dark matter roommate. But

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<v Speaker 1>if you want to do experiments to reveal the nature

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<v Speaker 1>of dark matter, you'd like it to respond sometimes, and

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<v Speaker 1>dark matter turns out to be very difficult to probe

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<v Speaker 1>because the only way we've been able to interact with

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<v Speaker 1>dark matter so far at all is with gravity. Like

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<v Speaker 1>we said, we've discovered dark matter because we looked at

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<v Speaker 1>how galaxies spin, and we notice that to spin as

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<v Speaker 1>fast as they do and hold all the stars in place,

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<v Speaker 1>you need a lot more gravity than is generated by

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<v Speaker 1>the stars we see, which means there must be something

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<v Speaker 1>else they're making that gravity. And we see blobs of

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<v Speaker 1>dark matter in the sky. We don't see them. We

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<v Speaker 1>deduce blobs of dark matter in the sky because they're

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<v Speaker 1>bending the light that passes through them. That's a gravitational effect.

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<v Speaker 1>So we have very concrete evidence that dark matter feels gravity.

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<v Speaker 1>That's why we call it matter, not just like dark

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<v Speaker 1>mysterious thing in the space right because it has gravity.

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<v Speaker 1>I see. It's sort of like the probervial elephant in

0:11:57.000 --> 0:11:59.520
<v Speaker 1>the room. You know it's there, everyone knows it's there,

0:12:00.080 --> 0:12:02.800
<v Speaker 1>but it's, uh, it's nobody's talking about. Sort of. It's

0:12:02.840 --> 0:12:05.160
<v Speaker 1>also sort of like the opposite of that, because the

0:12:05.240 --> 0:12:07.880
<v Speaker 1>elf in the room. Everybody is ignoring it, right though

0:12:07.880 --> 0:12:09.800
<v Speaker 1>you can all see it. In this case, we're all

0:12:09.880 --> 0:12:13.080
<v Speaker 1>desperately searching for it, but nobody can find it. It's

0:12:13.080 --> 0:12:16.200
<v Speaker 1>like you're right or right, except you're not. Well. You know,

0:12:16.360 --> 0:12:19.240
<v Speaker 1>sometimes being exactly the opposite direction is also a way

0:12:19.240 --> 0:12:23.640
<v Speaker 1>of being right. Yeah, yeah, you know up bean staff

0:12:24.000 --> 0:12:27.520
<v Speaker 1>yes times minus one. Alright, So we know it feels gravity,

0:12:27.559 --> 0:12:29.600
<v Speaker 1>but there are other forces that we know about in

0:12:29.640 --> 0:12:32.000
<v Speaker 1>the universe, and as far as we know, the dark

0:12:32.000 --> 0:12:34.360
<v Speaker 1>matter doesn't feel them. That's right. And so for example,

0:12:34.440 --> 0:12:37.200
<v Speaker 1>electromagnetism is a very powerful force and when that we

0:12:37.280 --> 0:12:40.200
<v Speaker 1>experience every day. The reason that your hand doesn't go

0:12:40.280 --> 0:12:42.320
<v Speaker 1>through the wall when you're trying to touch it is

0:12:42.400 --> 0:12:45.000
<v Speaker 1>that the wall has particles that are bound together with

0:12:45.040 --> 0:12:48.400
<v Speaker 1>electromagnetic forces, and so it does your hand and so

0:12:48.440 --> 0:12:50.400
<v Speaker 1>you think of them like a chain link fence trying

0:12:50.400 --> 0:12:53.040
<v Speaker 1>to pass through another chain link fence. That's what prevents

0:12:53.080 --> 0:12:57.080
<v Speaker 1>you from passing through another object. It's Electromagnetism is also

0:12:57.120 --> 0:13:00.280
<v Speaker 1>responsible for why things glow right, why we can see things,

0:13:01.040 --> 0:13:03.440
<v Speaker 1>or why they reflect light. To write like, it's light

0:13:03.559 --> 0:13:06.360
<v Speaker 1>hits it and then it interacts and it comes back out.

0:13:06.400 --> 0:13:08.760
<v Speaker 1>That's right. Even blobs of rock that don't glow on

0:13:08.800 --> 0:13:11.200
<v Speaker 1>their own, we can see them in the sky because

0:13:11.200 --> 0:13:14.400
<v Speaker 1>they reflect the sun's light, like the moon or like asteroids.

0:13:14.720 --> 0:13:17.160
<v Speaker 1>And so we know dark matter isn't like that because

0:13:17.200 --> 0:13:20.200
<v Speaker 1>it doesn't give off light, doesn't reflect light. Light passes

0:13:20.320 --> 0:13:24.880
<v Speaker 1>right through it. So right through it, yeah, exactly. And

0:13:25.000 --> 0:13:27.920
<v Speaker 1>I see this all the time in science fiction television,

0:13:28.320 --> 0:13:32.319
<v Speaker 1>that they encounter dark matter and it obscures their view. Right. Oh,

0:13:32.360 --> 0:13:34.520
<v Speaker 1>we can't get out of this cloud of dark matter

0:13:34.559 --> 0:13:36.959
<v Speaker 1>and we can't see where we are. What show are

0:13:36.960 --> 0:13:40.319
<v Speaker 1>you watching and seen that one? I don't remember the

0:13:40.400 --> 0:13:42.600
<v Speaker 1>name of it right now. I watched too much science fiction,

0:13:42.880 --> 0:13:44.320
<v Speaker 1>But you know that, to me, that sounds like a

0:13:44.320 --> 0:13:47.439
<v Speaker 1>fantastic situation, like, oh my gosh, look we found dark matter.

0:13:47.880 --> 0:13:50.120
<v Speaker 1>That's right home. We win the Nobel Prize. It's not like,

0:13:50.160 --> 0:13:52.640
<v Speaker 1>get out of my picture, my photo. It's like I

0:13:52.679 --> 0:13:56.000
<v Speaker 1>got a photo of dark matter. Exactly. We've been trying

0:13:56.040 --> 0:13:58.560
<v Speaker 1>to spot dark matter forever and you just figured it

0:13:58.559 --> 0:14:00.600
<v Speaker 1>out and now it seems like a hassled you. But

0:14:00.679 --> 0:14:02.320
<v Speaker 1>if you were in a cloud of dark matter, you

0:14:02.320 --> 0:14:05.240
<v Speaker 1>couldn't tell because it's invisible right. In fact, we think

0:14:05.280 --> 0:14:07.120
<v Speaker 1>we are in a cloud of dark matter. We think

0:14:07.120 --> 0:14:10.000
<v Speaker 1>the Earth is surrounded by dark matter, but we can't

0:14:10.040 --> 0:14:12.720
<v Speaker 1>see it because it doesn't reflect light. It doesn't feel

0:14:12.720 --> 0:14:15.920
<v Speaker 1>any electromagnetic forces at all. Yeah, we're swimming in dark

0:14:15.960 --> 0:14:19.160
<v Speaker 1>matter right, Like everyone who's listening to this podcast right

0:14:19.200 --> 0:14:22.240
<v Speaker 1>now is probably swimming in dark matter. Like right in

0:14:22.240 --> 0:14:25.160
<v Speaker 1>front of their eyes, is dark matter passing through or

0:14:25.560 --> 0:14:28.080
<v Speaker 1>sitting there? That's right. Dark matter, we think is spread

0:14:28.120 --> 0:14:31.440
<v Speaker 1>out through the galaxy. It's fairly dilute, so it's there's

0:14:31.440 --> 0:14:33.320
<v Speaker 1>a lot of it. There's a lot more dark matter

0:14:33.360 --> 0:14:35.480
<v Speaker 1>than normal matter, but it's much more spread out we

0:14:35.520 --> 0:14:38.280
<v Speaker 1>think the normal matter, which tends to cluster into planets

0:14:38.320 --> 0:14:40.920
<v Speaker 1>and stars and stuff. So we think there's like one

0:14:41.040 --> 0:14:44.560
<v Speaker 1>squirrel's worth of dark matter in the volume of the Earth.

0:14:44.640 --> 0:14:49.240
<v Speaker 1>But it's there, it's out there. Wait, what one squirrels worth?

0:14:51.800 --> 0:14:55.160
<v Speaker 1>One squirrel? Yeah, well it's a standard international unit of mass.

0:14:55.200 --> 0:14:59.520
<v Speaker 1>One squirrel. Are you not familiar with squirrels? I don't.

0:14:59.560 --> 0:15:03.760
<v Speaker 1>I didn't usually baked with squirrels. All my favorite recipes

0:15:03.800 --> 0:15:06.440
<v Speaker 1>are in units of squirrels. You know, a third of

0:15:06.480 --> 0:15:08.840
<v Speaker 1>a squirrel of oats and you know, half a squirrel

0:15:08.840 --> 0:15:12.680
<v Speaker 1>of sugar man. That's that's the pandemic for you. It's

0:15:12.720 --> 0:15:15.760
<v Speaker 1>forcing us into a more primitive Yeah, come over to

0:15:15.800 --> 0:15:18.080
<v Speaker 1>my house sometime. We'll have a squirrel roast. So wait,

0:15:18.200 --> 0:15:20.480
<v Speaker 1>the Earth you're saying is in a pool of dark

0:15:20.480 --> 0:15:23.080
<v Speaker 1>matter that has the same amount of mass as a squirrel.

0:15:23.200 --> 0:15:25.560
<v Speaker 1>That's what it means. That's right, And there's more dark

0:15:25.600 --> 0:15:27.800
<v Speaker 1>matter than this normal matter, but the dark matter is

0:15:27.800 --> 0:15:30.360
<v Speaker 1>more diffuse, it's more spread out, and so out there

0:15:30.400 --> 0:15:33.240
<v Speaker 1>in empty space is about as much dark matter as

0:15:33.240 --> 0:15:35.520
<v Speaker 1>there is here in our solar system. You just made

0:15:35.560 --> 0:15:37.920
<v Speaker 1>me think of a giant squirrel the size of the

0:15:37.960 --> 0:15:41.720
<v Speaker 1>Earth that a dark matter. You're a very visual person,

0:15:41.760 --> 0:15:43.160
<v Speaker 1>so I'd love to see a drawing of that of

0:15:43.160 --> 0:15:47.680
<v Speaker 1>a squirrel attacking the Earth and earth size squirrel attacking us. Finally,

0:15:47.680 --> 0:15:50.520
<v Speaker 1>the aliens have come and they're just giants space squirrels.

0:15:51.280 --> 0:15:53.480
<v Speaker 1>You did it again. Just because it's a dark matter squirrel,

0:15:53.480 --> 0:15:55.800
<v Speaker 1>you assume it was bad, Daniel. Yeah, maybe it's a

0:15:55.840 --> 0:15:59.560
<v Speaker 1>friendly planet sized space squirrel. Yeah, you're right. Now, so

0:15:59.640 --> 0:16:02.320
<v Speaker 1>we we know that it doesn't feel electromagnetism, and that's

0:16:02.360 --> 0:16:05.000
<v Speaker 1>principally because it's dark, we can't see it. But there

0:16:05.000 --> 0:16:07.280
<v Speaker 1>are other forces out there, right, we talk about the

0:16:07.320 --> 0:16:11.800
<v Speaker 1>weak nuclear force. That's a very very non powerful force.

0:16:11.840 --> 0:16:15.800
<v Speaker 1>It's a weak force between particles. Neutrinos feel this force,

0:16:15.920 --> 0:16:18.400
<v Speaker 1>Leptons feel this force. All the particles we know feel

0:16:18.440 --> 0:16:21.720
<v Speaker 1>this force, but it's not very powerful. Like neutrinos pass

0:16:21.840 --> 0:16:25.040
<v Speaker 1>through a light year of lead and have a fifty

0:16:25.040 --> 0:16:28.480
<v Speaker 1>percent chance of feeling anything using the weak force. Our

0:16:28.560 --> 0:16:31.160
<v Speaker 1>particles also feeling, like the particles in my body that

0:16:31.240 --> 0:16:33.280
<v Speaker 1>they feel the weak force. Yeah, all the particles in

0:16:33.320 --> 0:16:35.800
<v Speaker 1>your body, on the electrons and the corks, they all

0:16:35.880 --> 0:16:39.600
<v Speaker 1>feel this force. It's responsible, for example, for a beta decay.

0:16:39.640 --> 0:16:42.640
<v Speaker 1>So one of the corks in a neutron can turn

0:16:42.680 --> 0:16:45.240
<v Speaker 1>into another kind of quirk which turns your neutron into

0:16:45.280 --> 0:16:48.440
<v Speaker 1>a proton. That happens through the weak force, and that's

0:16:48.440 --> 0:16:52.240
<v Speaker 1>why a little neutrinos emitted along with the electron that's created.

0:16:52.480 --> 0:16:55.000
<v Speaker 1>So all the particles in your body are sensitive to

0:16:55.000 --> 0:16:58.400
<v Speaker 1>the weak force. Neutrinos that pass through you can interact

0:16:58.400 --> 0:17:00.920
<v Speaker 1>with you. It's just very very un likely, like there's

0:17:00.920 --> 0:17:05.440
<v Speaker 1>a hundred billion newtrinos passing through your fingernail every second,

0:17:05.920 --> 0:17:07.920
<v Speaker 1>and you don't feel them well, and we know that

0:17:07.960 --> 0:17:10.080
<v Speaker 1>the dark matter doesn't feel it. We suspect that dark

0:17:10.080 --> 0:17:12.840
<v Speaker 1>matter doesn't feel it because we've looked very very carefully.

0:17:13.080 --> 0:17:16.840
<v Speaker 1>We've set up these big underground experiments filled with very quiet,

0:17:16.920 --> 0:17:20.080
<v Speaker 1>heavy liquids, and we have a lot of those atoms

0:17:20.080 --> 0:17:21.919
<v Speaker 1>in there, and we hope that a dark matter particle

0:17:21.960 --> 0:17:25.159
<v Speaker 1>would come by and bump into one of those xenon atoms,

0:17:25.200 --> 0:17:27.240
<v Speaker 1>for example, and we could spot it. And this is

0:17:27.440 --> 0:17:31.159
<v Speaker 1>similar to how newtrinos were first discovered with vast tanks

0:17:31.160 --> 0:17:34.680
<v Speaker 1>of underground liquid waiting for a little recoil from one

0:17:34.680 --> 0:17:37.280
<v Speaker 1>of those atoms. So we have a similar in spirit

0:17:37.359 --> 0:17:41.440
<v Speaker 1>kind of experiment done underground to look for passing dark

0:17:41.480 --> 0:17:44.200
<v Speaker 1>matter particles. All right, So, and there's also the strong force,

0:17:44.320 --> 0:17:46.600
<v Speaker 1>right which that one is pretty important, but dark matter

0:17:46.600 --> 0:17:48.560
<v Speaker 1>doesn't feel that one either. That's right. The strong force

0:17:48.720 --> 0:17:51.600
<v Speaker 1>is very powerful and so unlike the weak force, which

0:17:51.800 --> 0:17:53.520
<v Speaker 1>you know, if dark matter felt it, it would be

0:17:53.600 --> 0:17:57.439
<v Speaker 1>difficult but possible to detect in large underground experiments. If

0:17:57.520 --> 0:17:59.560
<v Speaker 1>dark matter felt the strong force, we would notice that

0:17:59.680 --> 0:18:02.040
<v Speaker 1>right way. I mean, it's very powerful. It wouldn't take

0:18:02.040 --> 0:18:04.760
<v Speaker 1>a very big experiment. If dark matter felt the strong force,

0:18:04.920 --> 0:18:07.400
<v Speaker 1>then it would react to almost every particle in your

0:18:07.440 --> 0:18:09.840
<v Speaker 1>body and every particle in the Earth. It wouldn't be

0:18:09.840 --> 0:18:12.080
<v Speaker 1>hard to notice. It would break up particles all the time.

0:18:12.119 --> 0:18:14.280
<v Speaker 1>It would be a very powerful force. All right. So

0:18:14.320 --> 0:18:17.359
<v Speaker 1>then those are the four main forces that we know about,

0:18:17.680 --> 0:18:20.560
<v Speaker 1>and as far as we know, dark matter only feels gravity.

0:18:21.160 --> 0:18:24.719
<v Speaker 1>And so the question is what what happens to dark matter? Then?

0:18:24.720 --> 0:18:27.680
<v Speaker 1>Does it bump into itself or does it ignore it

0:18:27.760 --> 0:18:30.760
<v Speaker 1>even itself? And so let's get into the question of

0:18:30.840 --> 0:18:33.600
<v Speaker 1>does dark matter feel itself? But first let's take a

0:18:33.680 --> 0:18:49.480
<v Speaker 1>quick break right there. We're talking about dark matter and

0:18:49.520 --> 0:18:52.760
<v Speaker 1>whether it can feel itself, and so we know it

0:18:52.800 --> 0:18:56.280
<v Speaker 1>feels gravity, and we know it doesn't feel the other forces.

0:18:56.320 --> 0:18:58.680
<v Speaker 1>So I guess the question is, you know what happens

0:18:58.680 --> 0:19:00.959
<v Speaker 1>when too dark matter? Part of goals if they are

0:19:01.040 --> 0:19:03.920
<v Speaker 1>particles get attracted to each other, what's going to happen

0:19:03.960 --> 0:19:05.760
<v Speaker 1>and are they gonna bump into each other or just

0:19:05.840 --> 0:19:07.960
<v Speaker 1>totally ignore each other. It's a really fun sort of

0:19:07.960 --> 0:19:10.919
<v Speaker 1>thought experiment. This is exactly what Joe is asking. And

0:19:11.000 --> 0:19:14.119
<v Speaker 1>so you know, let's assume for the dark matter only

0:19:14.160 --> 0:19:17.479
<v Speaker 1>feels gravity, that no other forces we don't know about

0:19:17.600 --> 0:19:20.280
<v Speaker 1>that are involved, that it's just a gravitational thing. And

0:19:20.440 --> 0:19:23.359
<v Speaker 1>you know, that is totally possible. It's possible for a

0:19:23.400 --> 0:19:26.399
<v Speaker 1>particle to have mass and no other interactions. It's sort

0:19:26.440 --> 0:19:28.560
<v Speaker 1>of incredible, but it would be something that we've never

0:19:28.600 --> 0:19:32.199
<v Speaker 1>seen before. But hey, this physics is full of surprises. Well,

0:19:32.240 --> 0:19:35.320
<v Speaker 1>because we know about neutrinos, right, Neutrinos are also sort

0:19:35.320 --> 0:19:37.880
<v Speaker 1>of selective about which forces it feels. Yeah, we don't

0:19:37.960 --> 0:19:40.879
<v Speaker 1>understand that at all, Like why do neutrinos only feel

0:19:40.960 --> 0:19:43.159
<v Speaker 1>the weak force? You know, why don't they feel the

0:19:43.200 --> 0:19:46.160
<v Speaker 1>strong force? Why don't electrons feel the strong force. It's

0:19:46.200 --> 0:19:48.680
<v Speaker 1>just sort of like a thing we observe. We notice

0:19:48.720 --> 0:19:51.600
<v Speaker 1>these things. All the corks feel the strong force. None

0:19:51.600 --> 0:19:54.160
<v Speaker 1>of the electrons or neutrinos or muans or towels, those

0:19:54.160 --> 0:19:57.440
<v Speaker 1>particles feel it. Why not? I mean, we don't know.

0:19:57.800 --> 0:20:01.399
<v Speaker 1>We know that neutrinos don't feel elect a magnetism because

0:20:01.400 --> 0:20:03.840
<v Speaker 1>they don't have a charge. Only things with electric charge

0:20:03.880 --> 0:20:06.679
<v Speaker 1>can feel that. But we don't understand this. It's just

0:20:06.760 --> 0:20:09.120
<v Speaker 1>it's something we observe, something that we hope one day

0:20:09.119 --> 0:20:12.199
<v Speaker 1>to explain From the bottoms of principle. But at this

0:20:12.240 --> 0:20:15.760
<v Speaker 1>point we're pretty clueless. All right, So then what happens,

0:20:15.920 --> 0:20:18.600
<v Speaker 1>Like Joe put it, What if I take two particles

0:20:18.600 --> 0:20:21.399
<v Speaker 1>of dark matter in an empty universe, said I'm a

0:20:21.440 --> 0:20:24.040
<v Speaker 1>meter apart, and then I let go. Well, they attract

0:20:24.080 --> 0:20:26.840
<v Speaker 1>each other, right, gravity pulls them together. But then now

0:20:26.880 --> 0:20:29.680
<v Speaker 1>imagine what happens when sort of their edges meet, right,

0:20:29.680 --> 0:20:32.399
<v Speaker 1>what happens that one blob versus the other blob. Now,

0:20:32.440 --> 0:20:35.719
<v Speaker 1>if this was normal matter, when their edges meet, then

0:20:35.760 --> 0:20:38.440
<v Speaker 1>they would repel each other. They would bump, literally, because

0:20:38.440 --> 0:20:41.520
<v Speaker 1>they have forces to push against each other with. But

0:20:42.280 --> 0:20:46.320
<v Speaker 1>if all you have is gravity, gravity can't push. Gravity

0:20:46.400 --> 0:20:50.480
<v Speaker 1>only pulls. Right, you have two objects with positive mass,

0:20:50.520 --> 0:20:53.280
<v Speaker 1>they only pull on each other unless you have negative

0:20:53.320 --> 0:20:56.040
<v Speaker 1>mass particles. And we have a whole other podcast episode

0:20:56.080 --> 0:20:59.120
<v Speaker 1>about that. Gravity can only attract. So there's no way

0:20:59.119 --> 0:21:02.040
<v Speaker 1>for gravity to put ish, which means these particles just

0:21:02.080 --> 0:21:06.119
<v Speaker 1>get closer and closer. There's no repelling force, and eventually

0:21:06.200 --> 0:21:08.919
<v Speaker 1>they pass through each other. Right, Because there I guess

0:21:09.320 --> 0:21:11.840
<v Speaker 1>point particles right, Well, we don't know if they're made

0:21:11.840 --> 0:21:14.480
<v Speaker 1>of particles, right, but imagine they are mative particles. So

0:21:14.520 --> 0:21:16.399
<v Speaker 1>I think these arguments hold even if they're made of

0:21:16.440 --> 0:21:19.120
<v Speaker 1>some weird other kind of thing that you know isn't

0:21:19.119 --> 0:21:23.120
<v Speaker 1>divided up into little particles. But they can basically cohabitate

0:21:23.200 --> 0:21:25.840
<v Speaker 1>the same space. Right. The only thing that prevents things

0:21:25.840 --> 0:21:29.760
<v Speaker 1>from overlapping are the forces. Right. The reason that one

0:21:29.800 --> 0:21:32.200
<v Speaker 1>proton doesn't want to be next to another proton isn't

0:21:32.200 --> 0:21:35.679
<v Speaker 1>because the stuff in them is like you're crowding me

0:21:35.800 --> 0:21:38.240
<v Speaker 1>or something. It's all about the forces. As you said,

0:21:38.240 --> 0:21:40.920
<v Speaker 1>if you imagined that their point particles, they have zero volume.

0:21:41.480 --> 0:21:44.000
<v Speaker 1>So the only thing that gives distance to things are

0:21:44.040 --> 0:21:46.920
<v Speaker 1>forces that repel, and gravity can't do that. Well. I

0:21:46.920 --> 0:21:49.480
<v Speaker 1>think what's interesting to think about is that you know

0:21:49.480 --> 0:21:52.159
<v Speaker 1>they wouldn't share the same space for very long, right,

0:21:52.359 --> 0:21:54.640
<v Speaker 1>because if you set them a meter apart, they're gonna

0:21:54.640 --> 0:21:56.359
<v Speaker 1>ask some velocity by the time that you get to

0:21:56.400 --> 0:21:58.240
<v Speaker 1>the center, and so they'll just keep going. Yeah, they

0:21:58.280 --> 0:22:00.640
<v Speaker 1>pass through each other, but then gravity will slow them down,

0:22:01.280 --> 0:22:03.239
<v Speaker 1>stop them, turn them around, and they'll come through each

0:22:03.280 --> 0:22:06.320
<v Speaker 1>other again. So like slash back and forth forever and

0:22:06.440 --> 0:22:10.320
<v Speaker 1>right forever, right, because there's nothing, nothing would be making

0:22:10.320 --> 0:22:13.600
<v Speaker 1>you lose energy. Yeah, in your hypothetical universe where there

0:22:13.760 --> 0:22:16.520
<v Speaker 1>is nothing else, then they would slash back and forth forever.

0:22:17.080 --> 0:22:19.760
<v Speaker 1>If they had some other way to lose energy. There's

0:22:19.800 --> 0:22:22.520
<v Speaker 1>like larger blobs of dark matter that are sort of

0:22:22.720 --> 0:22:25.320
<v Speaker 1>you know, equilibrating them or something. Then eventually they would

0:22:25.359 --> 0:22:27.679
<v Speaker 1>slow down and then stop and sit right in the

0:22:27.720 --> 0:22:31.560
<v Speaker 1>same place. But maybe not dark matter what you're saying.

0:22:31.560 --> 0:22:34.120
<v Speaker 1>In in the real universe, that would it is possible

0:22:34.160 --> 0:22:36.880
<v Speaker 1>out there that dark matter has settled. Yeah, it is possible.

0:22:36.960 --> 0:22:39.000
<v Speaker 1>In fact, we think that dark matter is not moving

0:22:39.080 --> 0:22:41.680
<v Speaker 1>very much. There's two theories of dark matter. There's warm

0:22:41.760 --> 0:22:44.880
<v Speaker 1>dark matter and cold dark matter. And warm dark matter

0:22:44.960 --> 0:22:47.480
<v Speaker 1>just means that the dark matter sort of zipping around everywhere.

0:22:47.520 --> 0:22:50.720
<v Speaker 1>It's like has high velocity, and cold dark matter means

0:22:50.920 --> 0:22:54.040
<v Speaker 1>it's mostly sitting around. It's like sluggist chilling and not

0:22:54.119 --> 0:22:58.240
<v Speaker 1>moving very fast. It's chilling matter exactly, chill dark matter.

0:23:00.160 --> 0:23:03.159
<v Speaker 1>That's for a statement of its feelings. Man. Yeah, so

0:23:03.200 --> 0:23:06.200
<v Speaker 1>we think the dark matter is cold. It's cold dark matter,

0:23:06.200 --> 0:23:08.119
<v Speaker 1>and so it's not moving very much. But yeah, if

0:23:08.119 --> 0:23:11.359
<v Speaker 1>you imagine so, like a gravitational well constructed by something else,

0:23:11.400 --> 0:23:14.520
<v Speaker 1>some larger object than two pieces of dark matter in

0:23:14.560 --> 0:23:17.000
<v Speaker 1>that well would fall together to the bottom of it,

0:23:17.040 --> 0:23:18.879
<v Speaker 1>and then they could just sit on top of each other.

0:23:19.280 --> 0:23:21.320
<v Speaker 1>And I guess the same would happen with dark matter

0:23:21.400 --> 0:23:25.280
<v Speaker 1>and regular matter, right, they would technically, like we only

0:23:25.320 --> 0:23:28.240
<v Speaker 1>interact with gravity with dark matter, and so therefore we

0:23:28.480 --> 0:23:30.720
<v Speaker 1>would just pass through us back and forth. Oh that's

0:23:30.720 --> 0:23:32.240
<v Speaker 1>a good point. Yeah, And I think you're right, And

0:23:32.240 --> 0:23:34.800
<v Speaker 1>I think dark matter is passing through us right now,

0:23:35.000 --> 0:23:37.720
<v Speaker 1>or we're passing through dark matter in the same way

0:23:37.720 --> 0:23:40.440
<v Speaker 1>that like neutrinos passed through us. But if there literally

0:23:40.640 --> 0:23:44.080
<v Speaker 1>is no interaction other than gravity, then you're right. Dark

0:23:44.080 --> 0:23:46.080
<v Speaker 1>matter can be in you and you can be in

0:23:46.200 --> 0:23:48.800
<v Speaker 1>dark matter. Oh man, I feel like now we're getting

0:23:49.040 --> 0:23:52.919
<v Speaker 1>ethereal here about dark matter and spiritual It's in you,

0:23:53.480 --> 0:23:56.480
<v Speaker 1>in all of us, and it's not just a hypothetical question.

0:23:56.560 --> 0:23:59.880
<v Speaker 1>We sort of did this experiment on a massive cause,

0:24:00.000 --> 0:24:02.159
<v Speaker 1>a logical scale. Oh yeah, we did it. Oh we

0:24:02.280 --> 0:24:03.800
<v Speaker 1>didn't sort of do what I mean, as much as

0:24:03.800 --> 0:24:06.800
<v Speaker 1>astronomers do anything. They just sort of watched the universe

0:24:06.840 --> 0:24:10.600
<v Speaker 1>do stuff. You say, astronomers don't do anything, Well, they

0:24:10.600 --> 0:24:13.679
<v Speaker 1>don't construct experiments, right, They don't go like, let's build

0:24:13.680 --> 0:24:17.080
<v Speaker 1>a sun that has these properties and distribute these planets

0:24:17.119 --> 0:24:18.760
<v Speaker 1>around it and let it go. Right. They don't do

0:24:18.800 --> 0:24:22.160
<v Speaker 1>that except in simulations, but they just look around and

0:24:22.320 --> 0:24:25.359
<v Speaker 1>find that situation because the universe is so vast and

0:24:25.400 --> 0:24:28.359
<v Speaker 1>so varied that they can usually find whatever they're looking for.

0:24:28.440 --> 0:24:33.160
<v Speaker 1>The shoppers, not doers. I love astronomers. Nothing I say

0:24:33.200 --> 0:24:38.040
<v Speaker 1>should be construed as negative towards astronomy or astronomers. But yeah,

0:24:38.200 --> 0:24:42.560
<v Speaker 1>they're mostly observers, right, And what they found was these

0:24:42.640 --> 0:24:46.680
<v Speaker 1>two clusters of galaxies that had slammed into each other. Yeah,

0:24:46.800 --> 0:24:49.879
<v Speaker 1>it's called the Bullet cluster. Right, it's called the Bullet cluster.

0:24:50.160 --> 0:24:51.960
<v Speaker 1>And this is a collision that happened a long long

0:24:52.000 --> 0:24:55.600
<v Speaker 1>time ago. And by galaxy cluster, we just mean literally

0:24:55.640 --> 0:24:59.040
<v Speaker 1>a group of galaxies, because galaxies orbit each other and

0:24:59.080 --> 0:25:00.879
<v Speaker 1>are sort of grouped to either the same way that

0:25:01.000 --> 0:25:04.920
<v Speaker 1>like stars are grouped together into a galaxy, galaxies themselves

0:25:04.920 --> 0:25:08.480
<v Speaker 1>are grouped together into clusters of galaxies, and sometimes these

0:25:08.480 --> 0:25:12.359
<v Speaker 1>things collide. Right. Dark energy is pushing the whole universe apart,

0:25:12.440 --> 0:25:15.800
<v Speaker 1>creating spaces between things, but there are still forces and

0:25:15.840 --> 0:25:19.240
<v Speaker 1>still directions that can pull things together. And so gravity

0:25:19.280 --> 0:25:22.920
<v Speaker 1>pulled these two clusters together and they slammed into each other,

0:25:23.520 --> 0:25:26.320
<v Speaker 1>and so we basically got to see this experiment happened. Yeah,

0:25:26.320 --> 0:25:28.840
<v Speaker 1>you can look it up online if you google bullet cluster,

0:25:29.000 --> 0:25:32.320
<v Speaker 1>and they're pretty spectacular images. Like, imagine a cluster of

0:25:32.320 --> 0:25:35.520
<v Speaker 1>galaxies slamming into another cluster of galaxies. It's like a

0:25:35.560 --> 0:25:39.000
<v Speaker 1>special effects bonanza. It's like a large hadron collider on

0:25:39.080 --> 0:25:45.440
<v Speaker 1>the biggest scale possible, the largest, the large gaxy collider collider. Yeah,

0:25:45.520 --> 0:25:48.360
<v Speaker 1>and of course you can't see it happen in real time.

0:25:48.400 --> 0:25:51.080
<v Speaker 1>The whole collision took, you know, hundreds of millions of years.

0:25:51.320 --> 0:25:53.040
<v Speaker 1>What we're looking at when we see it in the sky,

0:25:53.520 --> 0:25:56.040
<v Speaker 1>it's just the after effects, and we can reconstruct what

0:25:56.080 --> 0:25:58.920
<v Speaker 1>we think happened from what we're seeing now. And so,

0:25:59.240 --> 0:26:01.080
<v Speaker 1>you know, the clusters are made of sort of three

0:26:01.119 --> 0:26:03.679
<v Speaker 1>basic constituents. You have the stars, of course, so the

0:26:03.720 --> 0:26:06.359
<v Speaker 1>things that are visible in the galaxy, and then between

0:26:06.400 --> 0:26:09.160
<v Speaker 1>the stars you have gas, the things that make the stars.

0:26:09.400 --> 0:26:12.000
<v Speaker 1>And then of course each one has dark matter, these

0:26:12.119 --> 0:26:15.040
<v Speaker 1>huge blobs of dark matter. Remember that most of the

0:26:15.080 --> 0:26:17.480
<v Speaker 1>things that are out there in the sky, the visible galaxies,

0:26:17.760 --> 0:26:21.320
<v Speaker 1>have these halos of dark matter around them. So wherever

0:26:21.400 --> 0:26:23.760
<v Speaker 1>you see stuff in the sky is probably where the

0:26:23.840 --> 0:26:26.360
<v Speaker 1>dark matter is. They tend to follow each other. We've

0:26:26.359 --> 0:26:28.919
<v Speaker 1>never seen or have we seen dark matter by itself.

0:26:29.119 --> 0:26:32.040
<v Speaker 1>We have noticed some clumps, like that's what gravitational lensing is,

0:26:32.359 --> 0:26:35.080
<v Speaker 1>so it is distributed. It goes out further past the

0:26:35.160 --> 0:26:37.639
<v Speaker 1>edge of the galaxy, Like each galaxy has a halo

0:26:37.800 --> 0:26:40.960
<v Speaker 1>that's longer and wider and larger than the galaxy itself.

0:26:41.200 --> 0:26:43.480
<v Speaker 1>And we have seen blobs of dark matter in the

0:26:43.560 --> 0:26:46.919
<v Speaker 1>universe by themselves. They do this gravitational lensing, but for

0:26:46.960 --> 0:26:49.680
<v Speaker 1>the most part, the structure they follow each other. And

0:26:49.720 --> 0:26:52.560
<v Speaker 1>that's not an accident. That's because of gravity. The structure

0:26:52.600 --> 0:26:55.679
<v Speaker 1>of dark matter created the structure of normal matter, like

0:26:55.840 --> 0:26:59.200
<v Speaker 1>created these gravitational wells for normal matter to fall into.

0:26:59.400 --> 0:27:03.040
<v Speaker 1>That's why we have galaxies and stars and planets and squirrels.

0:27:03.160 --> 0:27:05.520
<v Speaker 1>It's like, which came first, the dark matter or the galaxies,

0:27:05.560 --> 0:27:07.639
<v Speaker 1>And the answer is the dark matter. Yeah, well, all

0:27:07.680 --> 0:27:09.520
<v Speaker 1>the matter was created, i think at the same time,

0:27:09.560 --> 0:27:11.840
<v Speaker 1>but dark matter there's more of it, and so it

0:27:11.880 --> 0:27:15.280
<v Speaker 1>has a huge influence on the shape of the universe.

0:27:15.880 --> 0:27:18.359
<v Speaker 1>So we saw this collision happen and we looked at it,

0:27:18.400 --> 0:27:21.560
<v Speaker 1>and what we noticed is that when these two galaxy

0:27:21.720 --> 0:27:24.879
<v Speaker 1>clusters passed through each other, the gas reacted like you

0:27:24.920 --> 0:27:28.000
<v Speaker 1>would expect what to happen when two huge piles of

0:27:28.000 --> 0:27:30.800
<v Speaker 1>stuff hit each other, right, big special effects, explosions, lots

0:27:30.800 --> 0:27:33.280
<v Speaker 1>of friction and radiation at the edges and all that

0:27:33.320 --> 0:27:35.719
<v Speaker 1>kind of stuff. And so you could see the gas

0:27:35.720 --> 0:27:37.959
<v Speaker 1>not just kind of mixing with itself but actually like

0:27:38.119 --> 0:27:42.280
<v Speaker 1>violently reacting. Oh yeah, these things are moving really fast. Absolutely,

0:27:42.320 --> 0:27:44.920
<v Speaker 1>like if you shoot gas really fast and another cloud

0:27:44.960 --> 0:27:47.399
<v Speaker 1>of gas, then things would happen. Things will happen, and

0:27:47.440 --> 0:27:49.359
<v Speaker 1>they slow down, right, And so that energy had to

0:27:49.400 --> 0:27:51.879
<v Speaker 1>go somewhere, and that energy went to heating up the

0:27:51.880 --> 0:27:53.560
<v Speaker 1>gas and then it radiates, and you have all this

0:27:53.680 --> 0:27:57.280
<v Speaker 1>friction between these two colliding clouds of gas. But the

0:27:57.359 --> 0:28:00.679
<v Speaker 1>dark matter in these clusters got stripped way. It passed

0:28:00.800 --> 0:28:04.080
<v Speaker 1>right through. It went right through the clouds of gas

0:28:04.280 --> 0:28:06.879
<v Speaker 1>and right through the clouds of dark matter from the

0:28:06.920 --> 0:28:10.040
<v Speaker 1>other galaxy and passed through to the other side like

0:28:10.080 --> 0:28:12.440
<v Speaker 1>it went through the windshield or you know, thinking maybe

0:28:12.440 --> 0:28:14.760
<v Speaker 1>like in the matrix, remember when they're fighting those ghosts

0:28:15.040 --> 0:28:17.080
<v Speaker 1>and they're in the car and they slammed the brakes

0:28:17.119 --> 0:28:19.640
<v Speaker 1>and the ghosts just keep going. Yeah, kind of like that,

0:28:19.920 --> 0:28:21.920
<v Speaker 1>or like you're walking down the sidewalk with your kid

0:28:22.359 --> 0:28:24.480
<v Speaker 1>and they notice something interesting and they stop and you

0:28:24.640 --> 0:28:26.520
<v Speaker 1>just on your phone, and so you don't even pay

0:28:26.520 --> 0:28:28.359
<v Speaker 1>attention to a block later, you're like, wait a second,

0:28:28.359 --> 0:28:32.600
<v Speaker 1>where's my kid? I mean, that's never happened to me.

0:28:32.800 --> 0:28:35.359
<v Speaker 1>They're reacting with some gas or is it running to

0:28:35.400 --> 0:28:38.719
<v Speaker 1>another kid that you didn't spot? Right, there's the analogy,

0:28:38.800 --> 0:28:40.960
<v Speaker 1>and the two parents just keep going looking at their phone.

0:28:41.880 --> 0:28:44.720
<v Speaker 1>We're really modeling responsible parenting. I know, we're really talking

0:28:44.720 --> 0:28:47.400
<v Speaker 1>about our feelings. And so we can see the dark

0:28:47.440 --> 0:28:50.360
<v Speaker 1>matter came at the other side because we use gravitational lensing,

0:28:50.400 --> 0:28:53.600
<v Speaker 1>we can see it distorting the light from background galaxies.

0:28:54.360 --> 0:28:58.200
<v Speaker 1>So dark matter passed right through normal matter, gas, etcetera.

0:28:58.520 --> 0:29:01.880
<v Speaker 1>Collided and so they got separated. So we really can't

0:29:01.880 --> 0:29:03.840
<v Speaker 1>see in that case, this is a you know, collidab

0:29:03.920 --> 0:29:06.040
<v Speaker 1>lab of dark matter with another lav of dark matter.

0:29:06.120 --> 0:29:10.320
<v Speaker 1>What happens, Well, they massed right through nothing exactly, nothing happens.

0:29:10.320 --> 0:29:14.880
<v Speaker 1>It just it just passes right through at least exciting collision. Ever, Well,

0:29:14.920 --> 0:29:16.800
<v Speaker 1>I'm sure if it's exciting for them to lose their

0:29:16.880 --> 0:29:20.160
<v Speaker 1>kids A few blocks back. All right. So we know

0:29:20.360 --> 0:29:24.360
<v Speaker 1>then for sure through observational experiments that dark matter doesn't

0:29:24.400 --> 0:29:26.240
<v Speaker 1>seem to feel itself, at least not in the way

0:29:26.280 --> 0:29:28.840
<v Speaker 1>that we know about or with any forces that we

0:29:28.920 --> 0:29:31.440
<v Speaker 1>know about. And so the question is, is there maybe

0:29:32.040 --> 0:29:34.440
<v Speaker 1>another way that dark matter can feel itself that we

0:29:34.520 --> 0:29:36.760
<v Speaker 1>don't know about? And so let's get into that. But

0:29:36.840 --> 0:29:51.960
<v Speaker 1>first let's take a quick break. All right, Daniel, have

0:29:52.000 --> 0:29:54.719
<v Speaker 1>you have you find your child yet? I've got your

0:29:54.800 --> 0:29:56.920
<v Speaker 1>child and still looking for mine. Oh well no, wait,

0:29:56.960 --> 0:30:01.160
<v Speaker 1>this one looks like, oh man, what take mishap here? Yeah,

0:30:01.240 --> 0:30:03.560
<v Speaker 1>it's like parent trapped galaxy style. All right. So we're

0:30:03.600 --> 0:30:05.360
<v Speaker 1>talking about dark matter and whether or not it can

0:30:05.480 --> 0:30:08.320
<v Speaker 1>feel itself. And we know you can feel itself with gravity,

0:30:08.360 --> 0:30:12.120
<v Speaker 1>but gravity doesn't help you really, you know, permanently feel

0:30:12.240 --> 0:30:14.760
<v Speaker 1>or clump or things like that. And so the question

0:30:14.840 --> 0:30:16.760
<v Speaker 1>is it could there be maybe another way that dark

0:30:16.800 --> 0:30:19.760
<v Speaker 1>matter interacts with itself that we don't know? There absolutely

0:30:19.840 --> 0:30:22.240
<v Speaker 1>could be, I mean, the existence of dark matter and

0:30:22.280 --> 0:30:26.000
<v Speaker 1>the existence of dark energy, and our sheer ignorance about

0:30:26.000 --> 0:30:28.640
<v Speaker 1>how the universe works, how it begins, and what controls

0:30:28.680 --> 0:30:31.200
<v Speaker 1>its largest dynamics tells us that there's a lot to

0:30:31.280 --> 0:30:34.080
<v Speaker 1>learn about the universe, and so there's certainly could be

0:30:34.120 --> 0:30:37.960
<v Speaker 1>a whole other force out there, some force we've never discovered,

0:30:38.280 --> 0:30:41.040
<v Speaker 1>some force that only dark matter feels and feels with

0:30:41.240 --> 0:30:43.880
<v Speaker 1>other dark matter, and that might be the reason we've

0:30:43.920 --> 0:30:46.960
<v Speaker 1>never seen it, the dark side of the force. Yeah,

0:30:47.000 --> 0:30:50.720
<v Speaker 1>there's nothing preventing another kind of force from existing. It's

0:30:50.720 --> 0:30:53.440
<v Speaker 1>not like we have any idea as to the number

0:30:53.480 --> 0:30:56.360
<v Speaker 1>of forces that there could be, or is any limit

0:30:56.480 --> 0:30:58.120
<v Speaker 1>to how many forces there are. It's just sort of

0:30:58.160 --> 0:31:01.160
<v Speaker 1>like a list of stuff we've seen so far in

0:31:01.200 --> 0:31:04.959
<v Speaker 1>our attempt to understand it. And so that's it. That

0:31:05.000 --> 0:31:08.160
<v Speaker 1>list is almost certainly incomplete, the way our list of

0:31:08.280 --> 0:31:12.959
<v Speaker 1>particles is incomplete, or the list of Beatles is incomplete. Right,

0:31:13.040 --> 0:31:15.320
<v Speaker 1>Like every year he's scovered like a a thousand new kinds

0:31:15.320 --> 0:31:23.640
<v Speaker 1>of Beatle. It's amazing. Yeah, Ringo, Paul Bob Robert And

0:31:23.720 --> 0:31:26.360
<v Speaker 1>that was such a bad joke. I'm sorry. I did

0:31:26.440 --> 0:31:28.880
<v Speaker 1>learn about a new Beatle last week. Actually, I discovered

0:31:28.920 --> 0:31:31.959
<v Speaker 1>that they brought Ringo in, that they fired the original drummer,

0:31:31.960 --> 0:31:34.040
<v Speaker 1>and he's still kind of better about the fifth One

0:31:34.040 --> 0:31:36.920
<v Speaker 1>of the fifth Beatles is usually refers to their producer.

0:31:37.120 --> 0:31:39.560
<v Speaker 1>But yeah, that the Ringo was not the original drummer. Yeah,

0:31:39.560 --> 0:31:42.160
<v Speaker 1>not a music podcast, So let's stick to our strengths

0:31:42.160 --> 0:31:49.080
<v Speaker 1>here matters. Yeah, well, this is a really interesting idea.

0:31:49.160 --> 0:31:51.240
<v Speaker 1>I think that the you know, because it's it's like

0:31:51.320 --> 0:31:53.760
<v Speaker 1>totally possible for there to be a whole another universe

0:31:53.800 --> 0:31:56.040
<v Speaker 1>on top of us, right, Like there could be a

0:31:56.080 --> 0:31:59.120
<v Speaker 1>whole set of other particles to feel, a whole other

0:31:59.200 --> 0:32:01.520
<v Speaker 1>set of forces, but we just can't see them or

0:32:01.600 --> 0:32:04.000
<v Speaker 1>feeling or touch them. Yeah, there's a whole party going on,

0:32:04.120 --> 0:32:06.680
<v Speaker 1>and we weren't invited, and even if we had been invited,

0:32:06.720 --> 0:32:10.560
<v Speaker 1>we couldn't even really attend because it just ignores us completely, right,

0:32:11.040 --> 0:32:13.080
<v Speaker 1>And we know that there's a lot going out there

0:32:13.080 --> 0:32:15.360
<v Speaker 1>that we can't see. Right, what we see in the

0:32:15.480 --> 0:32:19.040
<v Speaker 1>universe is a tiny fraction what's actually happening, even just

0:32:19.160 --> 0:32:22.240
<v Speaker 1>here on Earth with your eyeballs. Your eyeballs see a

0:32:22.440 --> 0:32:26.200
<v Speaker 1>little sliver of all the electromagnetic radiation that's out there.

0:32:26.360 --> 0:32:28.200
<v Speaker 1>There's a lot of stuff going on you can't see.

0:32:28.600 --> 0:32:31.280
<v Speaker 1>And imagine if you could see, you know, cell phone

0:32:31.320 --> 0:32:35.200
<v Speaker 1>signals and television signals and radio waves, the world would

0:32:35.200 --> 0:32:38.160
<v Speaker 1>be a much different looking place. And so we see

0:32:38.200 --> 0:32:41.840
<v Speaker 1>a little fraction of what's actually happening. Wow, and good

0:32:41.880 --> 0:32:45.400
<v Speaker 1>thing to write like it be overwhelmed me. I mean,

0:32:45.440 --> 0:32:48.080
<v Speaker 1>you can get Netflix in the Hulu for free, but

0:32:49.800 --> 0:32:52.200
<v Speaker 1>you know, cloud based delivery would be a different kind

0:32:52.200 --> 0:32:54.120
<v Speaker 1>of thing. All right, So there could be another force

0:32:54.160 --> 0:32:57.040
<v Speaker 1>out there, and it's im possible the dark matter feels

0:32:57.080 --> 0:32:59.720
<v Speaker 1>it then when we see it in these collisions, that

0:33:00.080 --> 0:33:02.440
<v Speaker 1>was interacting with itself in another way. Yeah. So there's

0:33:02.440 --> 0:33:06.000
<v Speaker 1>sort of two different categories of ideas. One is, could

0:33:06.040 --> 0:33:09.560
<v Speaker 1>there be another force that dark matter feels and uses

0:33:09.640 --> 0:33:12.800
<v Speaker 1>to interact with our kind of matter, some new kind

0:33:12.800 --> 0:33:15.840
<v Speaker 1>of force we've never seen before that mediates the interaction

0:33:15.920 --> 0:33:18.800
<v Speaker 1>between those two kinds of particles and that we're looking

0:33:18.840 --> 0:33:21.320
<v Speaker 1>for and we haven't ever seen, and we're looking for

0:33:21.400 --> 0:33:23.640
<v Speaker 1>that in the same way we're looking for like its

0:33:23.640 --> 0:33:26.280
<v Speaker 1>interaction via the weak force. We have these big tanks

0:33:26.280 --> 0:33:29.200
<v Speaker 1>of underground normal matter particles and we wait for dark

0:33:29.240 --> 0:33:31.880
<v Speaker 1>matter to bump into It doesn't matter if it's the

0:33:31.920 --> 0:33:34.360
<v Speaker 1>weak force or some other new kind of force. Like

0:33:34.440 --> 0:33:36.640
<v Speaker 1>would it be really hard to, for example, to take

0:33:36.840 --> 0:33:40.760
<v Speaker 1>one squirrel that's flying through the earth. Yes, And now

0:33:40.800 --> 0:33:44.400
<v Speaker 1>you're talking about one squirrel particle and it's flying through

0:33:44.480 --> 0:33:48.680
<v Speaker 1>like a ton of liquid zenon. These are very difficult experiments,

0:33:49.040 --> 0:33:52.440
<v Speaker 1>and they're done underground, like a kilometer underground to keep

0:33:52.480 --> 0:33:55.880
<v Speaker 1>them cold and isolated from all of the sources of background.

0:33:56.200 --> 0:33:59.360
<v Speaker 1>They're very hard experiments, and they haven't seen anything so far. Right,

0:33:59.680 --> 0:34:02.240
<v Speaker 1>But can you say it conclusively, like there's a pink

0:34:02.400 --> 0:34:05.280
<v Speaker 1>squirrel out there with the purple polka dots, but we

0:34:05.320 --> 0:34:07.920
<v Speaker 1>haven't found it on Earth, so therefore it must not exist.

0:34:07.960 --> 0:34:09.799
<v Speaker 1>You're right. We can't say it does not exist. We

0:34:09.840 --> 0:34:14.320
<v Speaker 1>can say it's less common than one squirrel per cubic

0:34:14.400 --> 0:34:17.720
<v Speaker 1>volume per year. Right, We can just say how likely

0:34:17.719 --> 0:34:20.320
<v Speaker 1>it is to exist at a certain level, and so

0:34:20.680 --> 0:34:22.520
<v Speaker 1>it could still be there. And people are still running

0:34:22.560 --> 0:34:25.279
<v Speaker 1>these experiments, and the longer we run them, the more

0:34:25.320 --> 0:34:27.719
<v Speaker 1>we can push those limits. We can say, if this

0:34:27.760 --> 0:34:31.920
<v Speaker 1>force does exist between standard model A matter and dark matter,

0:34:32.120 --> 0:34:35.239
<v Speaker 1>that it must be even weaker than this limit, than

0:34:35.280 --> 0:34:37.320
<v Speaker 1>this limit, than this lem We keep pushing that down.

0:34:37.840 --> 0:34:40.200
<v Speaker 1>But there's a whole other category, which is like maybe

0:34:40.280 --> 0:34:43.759
<v Speaker 1>dark matter just feel stuff with itself, not with our experiments,

0:34:43.760 --> 0:34:46.960
<v Speaker 1>not with our bodies, but just between itself, like is

0:34:47.000 --> 0:34:49.720
<v Speaker 1>it possible that dark matter bumps into itself and feels

0:34:49.719 --> 0:34:54.879
<v Speaker 1>something right or repels each other with because you're telling

0:34:54.880 --> 0:34:57.880
<v Speaker 1>me that this idea that it only feels gravity is

0:34:58.280 --> 0:35:02.520
<v Speaker 1>sort of on thin nice like maybe there's evidence that

0:35:02.560 --> 0:35:04.440
<v Speaker 1>maybe it does feel something else. Yeah, And this is

0:35:04.480 --> 0:35:07.800
<v Speaker 1>really hard to probe because you can't do experiments using

0:35:08.280 --> 0:35:13.040
<v Speaker 1>normal matter material to probe dark matters interactions with itself.

0:35:13.080 --> 0:35:15.799
<v Speaker 1>You need to like build your experiment out of dark matter, right,

0:35:16.239 --> 0:35:18.400
<v Speaker 1>So all we can do is look at how the

0:35:18.480 --> 0:35:20.799
<v Speaker 1>dark matter is laid out in the universe, like where

0:35:20.840 --> 0:35:23.040
<v Speaker 1>did it end up, and then try to see is

0:35:23.080 --> 0:35:26.120
<v Speaker 1>that consistent with how it should end up if it

0:35:26.160 --> 0:35:29.200
<v Speaker 1>only feels gravity, because if it is bumping into itself,

0:35:29.320 --> 0:35:31.719
<v Speaker 1>that will change the way it's laid out, just like

0:35:32.040 --> 0:35:34.440
<v Speaker 1>if it's hot or cold, if it's fast or slow,

0:35:34.640 --> 0:35:37.680
<v Speaker 1>will also change the distribution of dark matter. So we

0:35:37.719 --> 0:35:39.840
<v Speaker 1>look at the distribution and try to ask is it

0:35:39.880 --> 0:35:43.000
<v Speaker 1>consistent with gravity only or do we need another piece

0:35:43.040 --> 0:35:44.840
<v Speaker 1>of the puzzle aid And what do we see do

0:35:44.920 --> 0:35:47.800
<v Speaker 1>we see out there in the universe that maybe it

0:35:47.800 --> 0:35:50.919
<v Speaker 1>does feel another force? We see that mostly gets things

0:35:51.040 --> 0:35:54.040
<v Speaker 1>right sort of on the scale of galaxies, and larger

0:35:54.560 --> 0:35:57.560
<v Speaker 1>like the distribution of galaxies and how they cluster together

0:35:57.680 --> 0:36:00.400
<v Speaker 1>and superclusters. That all seems right, and you run a

0:36:00.400 --> 0:36:03.319
<v Speaker 1>simulation of the universe with dark matter and normal matter

0:36:03.560 --> 0:36:06.239
<v Speaker 1>and dark matter is only gravity, it mostly gets that right.

0:36:06.560 --> 0:36:08.320
<v Speaker 1>But then if you zoom in, like on the smaller

0:36:08.360 --> 0:36:12.000
<v Speaker 1>scale here, smaller scales like less than a galaxy siza,

0:36:12.400 --> 0:36:16.400
<v Speaker 1>then sub galaxy, then it's not quite right. It doesn't

0:36:16.400 --> 0:36:20.680
<v Speaker 1>predict things the way we see them. For example, we

0:36:20.719 --> 0:36:22.760
<v Speaker 1>know that we have a big blob of dark matter

0:36:22.800 --> 0:36:24.960
<v Speaker 1>in our galaxy, and we know it's the densest at

0:36:24.960 --> 0:36:28.280
<v Speaker 1>the center just because of gravity, But the exact shape

0:36:28.320 --> 0:36:31.200
<v Speaker 1>of that blob is not something that we understand, like

0:36:31.680 --> 0:36:34.279
<v Speaker 1>dark matter with only gravity predicts it sort of like

0:36:34.400 --> 0:36:36.520
<v Speaker 1>peaked right at the center, that the center is like

0:36:36.640 --> 0:36:39.120
<v Speaker 1>a hot spot for dark matter. But we go out

0:36:39.120 --> 0:36:40.960
<v Speaker 1>and measure it, we see it's much more spread out

0:36:41.000 --> 0:36:43.520
<v Speaker 1>than that. It's like much more of a rod core,

0:36:43.680 --> 0:36:46.600
<v Speaker 1>not so much like peaked like a cusp, and so

0:36:47.080 --> 0:36:51.000
<v Speaker 1>that's not something we understand. Fuzzier than what you would expect.

0:36:51.040 --> 0:36:54.040
<v Speaker 1>You would expect it to sort of cluster more, but

0:36:54.440 --> 0:36:57.240
<v Speaker 1>it's actually kind of fuzzy it's like a big fuzzy squirrel,

0:36:57.320 --> 0:37:01.440
<v Speaker 1>not a little tiny intense squirrel. Yeah, it's a hedgehog

0:37:01.600 --> 0:37:04.400
<v Speaker 1>or or something like that rather than a tiny little squirrel.

0:37:04.960 --> 0:37:07.919
<v Speaker 1>And if you change your simulations and you add a

0:37:07.960 --> 0:37:09.960
<v Speaker 1>little bit of bumping this like a little bit like

0:37:10.080 --> 0:37:13.600
<v Speaker 1>maybe sometimes dark matter does bump into itself, that describes

0:37:13.600 --> 0:37:15.520
<v Speaker 1>what we see better, meaning like a little bit of

0:37:15.560 --> 0:37:19.120
<v Speaker 1>a repulsive force with itself. You just add in a

0:37:19.160 --> 0:37:21.440
<v Speaker 1>made up force. You're like, we don't know, but let's

0:37:21.480 --> 0:37:24.279
<v Speaker 1>see if it describes a situation, just like we made

0:37:24.360 --> 0:37:27.600
<v Speaker 1>up dark matter to describe this gravity we were seeing.

0:37:27.880 --> 0:37:30.280
<v Speaker 1>We're like, all right, well, now let's give another force

0:37:30.360 --> 0:37:32.880
<v Speaker 1>to these particles that are creating the gravity, so that

0:37:32.960 --> 0:37:35.560
<v Speaker 1>the distribution of gravity is the way we are seeing it.

0:37:35.640 --> 0:37:37.680
<v Speaker 1>Let's make something up about something that we've made up.

0:37:39.600 --> 0:37:42.600
<v Speaker 1>You're talking about all the physics, now, man, we'll come

0:37:42.600 --> 0:37:46.440
<v Speaker 1>to science. What if that thing we made up for

0:37:46.520 --> 0:37:50.200
<v Speaker 1>the thing we made up, that's something else we make up. Yeah,

0:37:50.239 --> 0:37:51.960
<v Speaker 1>and so this is sort of the state of the art.

0:37:52.000 --> 0:37:55.280
<v Speaker 1>Now we're like looking really carefully trying to understand where

0:37:55.440 --> 0:37:57.800
<v Speaker 1>is the dark matter? Does it agree with what we

0:37:57.920 --> 0:38:00.839
<v Speaker 1>predict and it turns out it doesn't quite agree, and

0:38:00.880 --> 0:38:04.720
<v Speaker 1>there are other little details that the gravity only theory

0:38:05.280 --> 0:38:08.440
<v Speaker 1>is getting wrong, so that they're sort of strong maybe

0:38:08.640 --> 0:38:11.600
<v Speaker 1>or at least a hint of an indication that maybe

0:38:11.640 --> 0:38:14.759
<v Speaker 1>dark matter does feel a whole new force or could

0:38:14.760 --> 0:38:16.279
<v Speaker 1>it be one of the old force. It couldn't be

0:38:16.320 --> 0:38:17.799
<v Speaker 1>one of the old forces. It would have to be

0:38:17.880 --> 0:38:20.840
<v Speaker 1>some sort of self interaction. So this theory is called

0:38:21.120 --> 0:38:24.160
<v Speaker 1>self interacting dark matter, and it solves some of these

0:38:24.440 --> 0:38:27.720
<v Speaker 1>nagging problems that we've had in the gravity only theory

0:38:27.760 --> 0:38:30.120
<v Speaker 1>of dark matter. So that makes it compelling. It's not

0:38:30.200 --> 0:38:33.560
<v Speaker 1>proof at all that this is happening, but it's like, huh,

0:38:33.600 --> 0:38:36.120
<v Speaker 1>we've had this problem. We add this new idea. It

0:38:36.160 --> 0:38:39.200
<v Speaker 1>gives a better explanation. That's cool. And you always have

0:38:39.280 --> 0:38:42.359
<v Speaker 1>to be careful when you're adding more stuff to your theory. Right,

0:38:42.400 --> 0:38:46.239
<v Speaker 1>you'd like the simplest possible explanation, but if that doesn't work,

0:38:46.280 --> 0:38:48.360
<v Speaker 1>then you have to add a little widget to your theory,

0:38:48.880 --> 0:38:52.120
<v Speaker 1>like maybe what if there are two kinds of squirrels matter? Yeah,

0:38:52.160 --> 0:38:54.600
<v Speaker 1>and and that's a whole other idea, right, Like if

0:38:54.680 --> 0:38:57.080
<v Speaker 1>dark matter made of particles, is it one kind of particles?

0:38:57.160 --> 0:38:59.480
<v Speaker 1>Is it two or is it ten? Didn't they decay

0:38:59.520 --> 0:39:01.920
<v Speaker 1>from one kind particle to the other? Do only some

0:39:02.000 --> 0:39:04.200
<v Speaker 1>of them have self interactions? I mean, look at the

0:39:04.200 --> 0:39:06.560
<v Speaker 1>particles that make up our kind of matter. There's all

0:39:06.600 --> 0:39:10.200
<v Speaker 1>sorts of complicated interactions with weird rules we don't understand.

0:39:10.560 --> 0:39:13.240
<v Speaker 1>Why would we imagine dark matter would be like simpler.

0:39:13.280 --> 0:39:16.480
<v Speaker 1>It could be different shades of dark matter, the darkest

0:39:16.520 --> 0:39:21.520
<v Speaker 1>matters squirrels and cats. And and then then you wonder, like,

0:39:21.600 --> 0:39:24.520
<v Speaker 1>all right, well, maybe dark matter could feel itself and

0:39:24.520 --> 0:39:27.239
<v Speaker 1>that would explain like the weird distribution of gravity that

0:39:27.239 --> 0:39:30.240
<v Speaker 1>we're seeing. But what about the bullet cluster? Right? Didn't

0:39:30.280 --> 0:39:34.080
<v Speaker 1>we do this experiment because the two clouds of dark

0:39:34.120 --> 0:39:36.960
<v Speaker 1>matter didn't repel each other. They didn't repel each other.

0:39:37.440 --> 0:39:39.880
<v Speaker 1>But people went back and looked at that again, and

0:39:39.920 --> 0:39:42.879
<v Speaker 1>they said, all right, well, can we explain this and

0:39:43.040 --> 0:39:46.520
<v Speaker 1>have some amount of interaction in there, because it's not

0:39:46.600 --> 0:39:49.359
<v Speaker 1>easy to tell exactly where all the dark matter is

0:39:49.680 --> 0:39:52.719
<v Speaker 1>very precisely, like maybe some of it did interact and

0:39:52.760 --> 0:39:55.280
<v Speaker 1>got sort of stuck in the middle. Most of it didn't,

0:39:55.520 --> 0:39:58.640
<v Speaker 1>but maybe some of it did. You know. It's like

0:39:58.680 --> 0:40:00.320
<v Speaker 1>we made it up in the first place when we

0:40:00.400 --> 0:40:03.160
<v Speaker 1>just you know, it's like there's a first pass and

0:40:03.200 --> 0:40:05.960
<v Speaker 1>there's a more precise test, right, you know, first you

0:40:06.000 --> 0:40:08.359
<v Speaker 1>try to understand the broad strokes. Then you really dig

0:40:08.400 --> 0:40:10.640
<v Speaker 1>in and see if it gets the details right. And

0:40:10.640 --> 0:40:12.239
<v Speaker 1>the other thing is it turns out that this is

0:40:12.360 --> 0:40:17.000
<v Speaker 1>not a great dark matter collider. It's too big dark matter. Well,

0:40:17.080 --> 0:40:19.800
<v Speaker 1>dark matter is very dilute, and so if you throw

0:40:20.239 --> 0:40:23.680
<v Speaker 1>a huge, very dilute cloud of dark matter at another one,

0:40:23.800 --> 0:40:26.200
<v Speaker 1>most of it's just going to pass through anyway. Like,

0:40:26.280 --> 0:40:28.960
<v Speaker 1>dark matter is not as dense as these gas clouds.

0:40:29.360 --> 0:40:31.759
<v Speaker 1>It's sort of like like the stars. Like if you

0:40:31.840 --> 0:40:35.600
<v Speaker 1>have two galaxies that pass through each other, mostly the

0:40:35.640 --> 0:40:39.320
<v Speaker 1>stars don't collide because the stars are embedded in huge,

0:40:39.520 --> 0:40:43.360
<v Speaker 1>vast empty spaces, and so they don't really collide with

0:40:43.360 --> 0:40:45.080
<v Speaker 1>each other head to head. So you were saying, like,

0:40:45.120 --> 0:40:47.279
<v Speaker 1>if I take two dark matter squirrels and I throw

0:40:47.320 --> 0:40:50.000
<v Speaker 1>them at each other, they might repel one against the other.

0:40:50.040 --> 0:40:53.040
<v Speaker 1>But if I take a whole cloud of squirrels that

0:40:53.120 --> 0:40:55.719
<v Speaker 1>are really far apart, they might just pass through each

0:40:55.719 --> 0:40:58.160
<v Speaker 1>other like we've seen in the cluster. Yeah, and they

0:40:58.200 --> 0:41:01.279
<v Speaker 1>would mostly miss, just like the large Hadron collider what

0:41:01.320 --> 0:41:04.840
<v Speaker 1>we do is we collide to clouds of protons against

0:41:04.880 --> 0:41:07.760
<v Speaker 1>each other, because one proton will never hit another proton,

0:41:07.800 --> 0:41:10.000
<v Speaker 1>they're too small. So we have like ten to the

0:41:10.040 --> 0:41:12.279
<v Speaker 1>ten protons and one cloud and ten to the ten

0:41:12.360 --> 0:41:14.719
<v Speaker 1>to the other, and we get you know, ten or

0:41:14.800 --> 0:41:18.560
<v Speaker 1>twenty or fifty collisions. And so it's not that easy

0:41:18.680 --> 0:41:22.120
<v Speaker 1>to make things collide. And so it turns out the

0:41:22.120 --> 0:41:25.760
<v Speaker 1>bullet cluster is actually also consistent with dark matter feeling

0:41:25.800 --> 0:41:28.680
<v Speaker 1>itself at sort of a low level of tweak how

0:41:28.719 --> 0:41:30.399
<v Speaker 1>you look at it. Yeah, and so you know, the

0:41:30.440 --> 0:41:33.120
<v Speaker 1>game here is come up with a theory um model

0:41:33.400 --> 0:41:36.920
<v Speaker 1>that explains everything that we do see all the same time.

0:41:37.320 --> 0:41:40.000
<v Speaker 1>And so you have to add some of this stuff

0:41:40.000 --> 0:41:43.120
<v Speaker 1>to explain the distribution of dark matter and the core

0:41:43.400 --> 0:41:45.680
<v Speaker 1>versus cup effect to the center of the galaxy, but

0:41:45.760 --> 0:41:47.840
<v Speaker 1>not too much that you mess up the description of

0:41:47.840 --> 0:41:49.719
<v Speaker 1>the bullet cluster. So you sort of hemmed in on

0:41:49.800 --> 0:41:53.480
<v Speaker 1>both sides there. Interesting, But I guess maybe the takeaways

0:41:53.520 --> 0:41:57.520
<v Speaker 1>that the answer is, yes, maybe dark matter does feel itself.

0:41:57.600 --> 0:42:00.560
<v Speaker 1>It's totally possible, and there might be some indication out

0:42:00.560 --> 0:42:03.319
<v Speaker 1>there that it does. Yeah, it's a new idea and

0:42:03.320 --> 0:42:06.840
<v Speaker 1>it's gaining traction in the community self interacting dark matter.

0:42:07.280 --> 0:42:10.120
<v Speaker 1>So it's possible that yes, dark matter could feel itself

0:42:10.160 --> 0:42:13.040
<v Speaker 1>and there could be multiple forces that it feels all right,

0:42:13.160 --> 0:42:16.239
<v Speaker 1>So maybe dark matter does have feelings, Daniel, It might

0:42:16.280 --> 0:42:18.719
<v Speaker 1>have a lot more feelings than we could ever understand.

0:42:19.120 --> 0:42:22.280
<v Speaker 1>Shades and shades of nuance. Well, I think it's all again,

0:42:22.320 --> 0:42:24.520
<v Speaker 1>just all of this is just an interesting example of

0:42:24.560 --> 0:42:27.719
<v Speaker 1>how there are things in the universe happening that we

0:42:27.960 --> 0:42:31.560
<v Speaker 1>don't really know about or see or feel or effective.

0:42:31.680 --> 0:42:34.600
<v Speaker 1>We're only seeing a tiny fraction of this grand play

0:42:34.600 --> 0:42:38.120
<v Speaker 1>of the universe, and we're making huge, broad conclusions about

0:42:38.160 --> 0:42:40.880
<v Speaker 1>how the universe works from this tiny little corner of

0:42:40.880 --> 0:42:43.200
<v Speaker 1>the stage. And there's a lot going on that we

0:42:43.280 --> 0:42:46.480
<v Speaker 1>haven't ever observed. And at least we know now. We

0:42:46.520 --> 0:42:49.280
<v Speaker 1>know that we're ignorant, so we know to be humble

0:42:49.320 --> 0:42:52.799
<v Speaker 1>and we know not to over generalize our ideas. But

0:42:52.880 --> 0:42:55.399
<v Speaker 1>it also is tantalizing because you hope that one day

0:42:55.440 --> 0:42:57.160
<v Speaker 1>we will see the rest of the action, We will

0:42:57.160 --> 0:42:59.719
<v Speaker 1>get a glimpse for what's really happening. We might all

0:42:59.760 --> 0:43:04.920
<v Speaker 1>be swimming in a giant squirrel up mr. I like

0:43:04.960 --> 0:43:08.160
<v Speaker 1>to think of myself as a physics raccoon, because it's

0:43:08.160 --> 0:43:10.440
<v Speaker 1>sneaking late at night to steal other people's garbage with

0:43:10.520 --> 0:43:14.000
<v Speaker 1>dark circles on your eyes. That makes sense eating garbage.

0:43:16.080 --> 0:43:19.600
<v Speaker 1>All right, Well that's pretty interesting and cool and or

0:43:19.680 --> 0:43:22.960
<v Speaker 1>chill um, and so we hope you enjoyed that discussion.

0:43:23.040 --> 0:43:25.200
<v Speaker 1>Thanks Joe for writing with your question. And if you

0:43:25.280 --> 0:43:27.719
<v Speaker 1>have a question you'd like us to explore on the podcast,

0:43:27.960 --> 0:43:31.440
<v Speaker 1>please write to us. We love your questions. Two questions

0:43:31.520 --> 0:43:35.239
<v Speaker 1>at Daniel and Jorge dot com. A bit mysterious. See

0:43:35.280 --> 0:43:46.040
<v Speaker 1>you next time. Thanks for listening, and remember that Daniel

0:43:46.040 --> 0:43:48.600
<v Speaker 1>and Jorge Explain the Universe is a production of I

0:43:48.800 --> 0:43:52.239
<v Speaker 1>Heart Radio. For more podcast from my Heart Radio, visit

0:43:52.280 --> 0:43:56.120
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