WEBVTT - What is dark radiation?

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<v Speaker 1>Hey, Daniel, how do you like your coffee? Oh? I

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<v Speaker 1>like it very dark, basically black. What about your chocolate?

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<v Speaker 1>Also pretty dark? Maybe? Like? What about your wine? How

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<v Speaker 1>do you drink your wine? Well? I like a pretty

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<v Speaker 1>dark cabernet. Actually, now, are you optimistic about the fate

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<v Speaker 1>of humanity? You know, I'll be honest until we start

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<v Speaker 1>dismantling more nuclear weapons. I have a pretty dark view

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<v Speaker 1>of our future. You kind of a dark physicist. Maybe

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<v Speaker 1>you should lighten up a little, you know, try some dessert, wine,

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<v Speaker 1>some rose, maybe maybe even some white chocolate. No, no, no, man,

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<v Speaker 1>we live in a dark universe where dominated by dark matter,

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<v Speaker 1>dark energy, and dark chocolate. You know what Yoda says,

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<v Speaker 1>once you go into the dark side, forever your destiny

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<v Speaker 1>well dominate. Do you think Yoda like dark chocolate? I

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<v Speaker 1>always knew you were a dark fisicist. Daniel. Hi am

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<v Speaker 1>poor handmade cartoonists and the creator of PhD comics. Hi,

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<v Speaker 1>I'm Daniel. I'm a particle physicist and a professor UC Irvine.

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<v Speaker 1>And white chocolate is not chocolate. It is chocolate. Then

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<v Speaker 1>it's made from chocolate, made from chocolate, not the same

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<v Speaker 1>as chocolate. You just don't like it. You still want

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<v Speaker 1>to categorize this chocolate, But scientifically, I think if you

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<v Speaker 1>asked a you know, chemist, they would say it's a

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<v Speaker 1>it's chocolate. I don't know. I think it doesn't have

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<v Speaker 1>any cocoa in it. It can't be chocolate. Doesn't taste

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<v Speaker 1>like chocolate. You know, white chocolate is chocolate the same

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<v Speaker 1>way deep dish pizza is pizza. But you do know

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<v Speaker 1>it's made from chocolate, right, Like I think it uses

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<v Speaker 1>like the cocoa butter from chocolate beans. Yeah, it's sort

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<v Speaker 1>of like hangs around when chocolate is made, sort calls

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<v Speaker 1>itself chocolate nearby it's chocolate and I'll give it that much.

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<v Speaker 1>Oh man, how can it be a jacent if it

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<v Speaker 1>comes from chocolated Daniel, I think you're stretching things a

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<v Speaker 1>little bit here. My kids are coming from chocolate, but

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<v Speaker 1>they're not chocolate, right. You should be more candy inclusive, Tenny,

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<v Speaker 1>white chocolate is delicious. It's just not chocolate. But welcome

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<v Speaker 1>to our podcast. Daniel and jorhead the Bait Chocolate apparently

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<v Speaker 1>for an hour instead of talking about physics and explain

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<v Speaker 1>the universe, in which we explore all the questions out there,

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<v Speaker 1>the dark ones, the white ones, the milky ones, all

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<v Speaker 1>the questions of the universe that are rattling around in

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<v Speaker 1>your brain and in hours, the questions that make us human,

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<v Speaker 1>the questions that make us wonder why the universe is

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<v Speaker 1>this way and not some other way? Could it have

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<v Speaker 1>been this way? Did it have to turn out in

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<v Speaker 1>this particular manner? What are the rules of this universe?

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<v Speaker 1>And is it possible for them to make sense to us?

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<v Speaker 1>And is it possible for Daniel and Jorge to explain

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<v Speaker 1>them to you in less than an hour while eating chocolates? Apparently,

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<v Speaker 1>but only dark or milk? What about chocolate? Are you

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<v Speaker 1>a fan of milk chocolate? Milk chocolate is chocolate. But

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<v Speaker 1>I'm not a fan, I see, And there are different

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<v Speaker 1>categories here of exclusion for you. Oh yeah, I got

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<v Speaker 1>a whole matrix going here. But it is an amazing

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<v Speaker 1>and beautiful and sometimes even delicious universe, full of amazing

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<v Speaker 1>mysteries and tantalizing questions to answer and discover out there,

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<v Speaker 1>and fortunately humans are here for all of it, to

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<v Speaker 1>answer these questions and to wonder about the amazing things

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<v Speaker 1>that are out there. That's right, and one of the

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<v Speaker 1>most basic questions we ask about the universe is just

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<v Speaker 1>what's in it? What's out there in the universe sharing

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<v Speaker 1>this cosmos with us. There's this sense that if you

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<v Speaker 1>could like make an accounting of all the stuff, all

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<v Speaker 1>the forces in the matter, and all the particles in

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<v Speaker 1>the universe, you'd get a sense for why the universe

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<v Speaker 1>is the way that it is the way. For example,

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<v Speaker 1>if you'd like looked at the ingredients of a pizza,

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<v Speaker 1>you can get a sense for, like what makes a

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<v Speaker 1>pizza a pizza. Yeah, because for thousands of years, we

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<v Speaker 1>thought that, you know, the stuff that we were made

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<v Speaker 1>out of was all there was too stuff, you know,

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<v Speaker 1>the electron and corks and protons and neutrons that we're

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<v Speaker 1>made out of. We thought that was the whole thing

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<v Speaker 1>that was in the universe. But actually it turns out

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<v Speaker 1>that most of the universe is made out of something else,

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<v Speaker 1>something dark and mysterious. Yes, And the history of physics

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<v Speaker 1>is these waves of realization, discovering that we are not

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<v Speaker 1>at the center of the universe, we are not at

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<v Speaker 1>the center of the Solar system, we are not really

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<v Speaker 1>at the center of anything, and then discovering that our

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<v Speaker 1>kind of matter is not even that special that we

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<v Speaker 1>make up a tiny little fraction of this incredible universe pizza.

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<v Speaker 1>Oh boy, Daniel, are you saying we are universe at Jason.

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<v Speaker 1>We're not really part of the universe. We're not really

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<v Speaker 1>universe material. We're sort of dark matter adjacent, right, We're

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<v Speaker 1>around when the dark matter formed all this structure. We

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<v Speaker 1>sort of like we're followers, but we're not dark matter. Yeah.

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<v Speaker 1>Do you think there's some snob courmet I don't know,

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<v Speaker 1>universe eater out there judging us talking down about the

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<v Speaker 1>humanity and all the stars and planets and galaxies in

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<v Speaker 1>the universe, saying that's not really universe. Yeah, I hope. So,

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<v Speaker 1>I hope that there are some dark a adans out

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<v Speaker 1>there made of dark matter, with their incredibly dark dark

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<v Speaker 1>chocolate made of dark matter, and they're looking at our

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<v Speaker 1>dark chocolate. They're like, that's ridiculous. Well, I guess the

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<v Speaker 1>good news is they they're not gonna eat us, because

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<v Speaker 1>if they're there's nobby about it, like you are white chocolate.

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<v Speaker 1>That's good news for the white chocolate. Yeah. Here ago

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<v Speaker 1>you can turn anything into positive news. I appreciate that. Yeah,

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<v Speaker 1>but there is a lot of dark matter in the universe.

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<v Speaker 1>In fact, it's most of the stuff in the universe

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<v Speaker 1>is dark matter. Of the stuff in the universe. I mean,

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<v Speaker 1>that's right. Even though we can't see it directly, we

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<v Speaker 1>can tell that dark matter is there, that it's a

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<v Speaker 1>thing that is affecting the whole shape of the universe.

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<v Speaker 1>It affected their universe early on and its little wiggles

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<v Speaker 1>and jiggles. It affected the formation of structure in the universe.

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<v Speaker 1>It even shapes how galaxies spin today. So we know

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<v Speaker 1>that it's there, we know that it's out there, and

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<v Speaker 1>we know that it dominates the universe in terms of

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<v Speaker 1>like the budget of the universe is mostly dark matter,

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<v Speaker 1>not what we used to call normal matter. I e us. Yeah,

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<v Speaker 1>it's something like, what's the exact budget percentage of dark

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<v Speaker 1>matter in the universe compared to the regular stuff we're

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<v Speaker 1>made out of. It's about five to one dark matter

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<v Speaker 1>to normal matter, all right, So then that's like eight

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<v Speaker 1>percent of the universe is sort of dark matter. Yeah,

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<v Speaker 1>eighty percent of the universe. So you could almost neglect

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<v Speaker 1>our part of the universe and you still got to

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<v Speaker 1>be on your exam Befo, bueno, that's right, bueno. Barry

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<v Speaker 1>on is exactly. Yeah, you could ignore all the atoms

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<v Speaker 1>in the universe and that would only be five percent

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<v Speaker 1>of the energy in the universe or twenty percent of

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<v Speaker 1>the matter in the universe. So in some sense, the

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<v Speaker 1>question what is the universe made out of? What is

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<v Speaker 1>all this crazy stuff? Tells you that what we're made

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<v Speaker 1>out of is not a big part of it is

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<v Speaker 1>not a central element in the structure of the universe. Right,

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<v Speaker 1>And just to clarify, most of this stuff and energy

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<v Speaker 1>in the universe is dark energy, which is something totally different.

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<v Speaker 1>But if we're just talking about stuff like matter, things

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<v Speaker 1>that feel gravity, then most of it is dark matter.

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<v Speaker 1>That's right. The matter portion of the universe is about

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<v Speaker 1>and of that thirty percent, eight percent that is dark matter.

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<v Speaker 1>So if the matter portion of the universe it is

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<v Speaker 1>dark matter, well that's pretty amazing. It's almost like most

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<v Speaker 1>of the stuff in the universe is this other stuff

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<v Speaker 1>called dark matter, but we don't know actually what it is, right,

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<v Speaker 1>It's pretty mysterious. We've only know it's there, we haven't

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<v Speaker 1>actually seen it directly because it's dark. Yeah, but it's

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<v Speaker 1>a great story. You know. I got into physics for

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<v Speaker 1>exactly these kinds of realizations, discovering that the universe out

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<v Speaker 1>there is not the one that you thought it was,

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<v Speaker 1>or that scientists and deep thinkers for thousands of years

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<v Speaker 1>hadn't known the true picture of the universe. You know.

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<v Speaker 1>Physics is this incredible technique to like reveal the truth

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<v Speaker 1>about the universe, to methodically build up knowledge and tell

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<v Speaker 1>us what's actually out there. So for it to discover

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<v Speaker 1>something shocking, like an enormous plot twist, like wow, it

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<v Speaker 1>turns out most of the stuff in the universe out

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<v Speaker 1>there is something you never heard about or thought about

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<v Speaker 1>or felt before. That's fantastic and it's exactly the kind

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<v Speaker 1>of thing that I hope happens, you know, again and again,

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<v Speaker 1>overturning everything we thought we knew about the universe. Yeah,

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<v Speaker 1>we know you went into physics for dark reasons. Daniels

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<v Speaker 1>that it's pretty close to home, given that a group

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<v Speaker 1>in Los Almos where they invented nuclear weapons which are

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<v Speaker 1>now being used to threaten genocide against civilian populations. So yeah,

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<v Speaker 1>that one stings a little bit, but it might say

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<v Speaker 1>humanity even if the media ever comes towards Earth and

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<v Speaker 1>we you know, break it up with nuclear weapons, then

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<v Speaker 1>then your parents would be heroes. There you go. All right,

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<v Speaker 1>So in some scenario we are saving the Earth instead

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<v Speaker 1>of destroying it. You know, you apply the quantum physics principle.

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<v Speaker 1>You know, it's all true. It's just the different probabilities.

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<v Speaker 1>There's a little white chocolate lining to that dark chocolate cloud.

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<v Speaker 1>Oh no, that ruins it for you though. It doesn't

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<v Speaker 1>taste as good, but it goes down easier. Yeah. Yeah,

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<v Speaker 1>So most of the stuff in the universe is made

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<v Speaker 1>out of dark matter, and so it kind of makes

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<v Speaker 1>you wonder if that's all that's dark in the universe.

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<v Speaker 1>Could there be other things in the universe that we're

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<v Speaker 1>not seeing or that we can't see. And it's certainly

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<v Speaker 1>true that most of the universe are things that you

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<v Speaker 1>cannot see directly. If you look out in front of you,

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<v Speaker 1>the information that's coming to you is just from photons,

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<v Speaker 1>and photons can only interact with things that have electric charges.

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<v Speaker 1>For example, there are particles flying right in front of

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<v Speaker 1>you right now that you cannot see. Billions of neutrinos

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<v Speaker 1>coming from the Sun raining down constantly in every square

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<v Speaker 1>centimeter per second, but they are invisible to you. So

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<v Speaker 1>the true universe out there. The actual reality of the

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<v Speaker 1>universe outside your skull is vastly different from the tiny

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<v Speaker 1>slice of it that you can see. Yeah, because if

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<v Speaker 1>we can't see of the stuff in the universe, it

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<v Speaker 1>kind of makes me wonder what else it's doing or

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<v Speaker 1>what else it can do, like is it maybe radiating

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<v Speaker 1>dark forces or dark light? Exactly? Because our kind of

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<v Speaker 1>matter does all sorts of complicated things. It doesn't just

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<v Speaker 1>sit there right. It shoots off photons at each other.

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<v Speaker 1>It has electromagnetic forces and strong forces and weak forces,

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<v Speaker 1>and forms complicated things like ice cream and pizza and chocolate,

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<v Speaker 1>and so a natural question is what's going on with

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<v Speaker 1>the dark matter? What else can it do? Can it

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<v Speaker 1>interact with itself in some way? So today on the podcast,

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<v Speaker 1>we'll be asking the question what is dark radiation? Now, Daniel,

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<v Speaker 1>this sort of sounds like an oxy moron, you know,

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<v Speaker 1>you're almost asking like, what is not light light? Exactly?

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<v Speaker 1>But this is the kind of game we play in

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<v Speaker 1>physics all the time. We don't really know how to

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<v Speaker 1>grapple with the unknown, so we tend to explore it

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<v Speaker 1>in terms of the known. Like when we think about photons,

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<v Speaker 1>we don't really know how to deal with the quantum objects.

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<v Speaker 1>We say, is it a particle? Is it a wave?

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<v Speaker 1>It's kind of both. That's kind of the same. It's

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<v Speaker 1>a contradiction there, right, and so here that's what we're doing.

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<v Speaker 1>We're saying, well, we know about photons, is there like

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<v Speaker 1>another kind of like dark matter version of the photon.

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<v Speaker 1>Were extrapolating from what we know into what we don't know. Interesting, well,

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<v Speaker 1>it sounds like the plot device for a great science

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<v Speaker 1>fic to novel or the next Marvel movie. You know,

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<v Speaker 1>dark radiation. That's how you know Stephen Strange gets his

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<v Speaker 1>powers or something. That's right. And if they are like

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<v Speaker 1>what ten avengers made of normal matter, there should be like,

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<v Speaker 1>you know, forty avengers made of dark matter, the dark avengers,

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<v Speaker 1>Oh many, they can make another gazillion dark billions of dollars.

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<v Speaker 1>That's right, and my one percent cut of that is

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<v Speaker 1>going to be pretty sweet. Hopefully not you don't like

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<v Speaker 1>sweet things exactly, it'll be pretty dark. Pile up those

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<v Speaker 1>dark dollars in my dark bank account. Only pay Daniel

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<v Speaker 1>with bitter dollars. We should start some sort of dark

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<v Speaker 1>matter currency, that's right, dark chocolate coin. But it is

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<v Speaker 1>a real question in physics, what is going on with

0:11:38.400 --> 0:11:41.600
<v Speaker 1>the dark matter? Is it interacting with itself? Are dark

0:11:41.840 --> 0:11:45.960
<v Speaker 1>matter particles shooting dark photons at each other? We just

0:11:46.000 --> 0:11:49.199
<v Speaker 1>don't know. It is a dark question. And so as usual,

0:11:49.240 --> 0:11:51.160
<v Speaker 1>we were wondering how many people out there had thought

0:11:51.200 --> 0:11:55.160
<v Speaker 1>about this question or even know what these two words

0:11:55.200 --> 0:11:57.559
<v Speaker 1>put together could mean. So, as usual, Daniel went out

0:11:57.559 --> 0:12:01.559
<v Speaker 1>there into the Internet to ask people what is dark radiation?

0:12:01.720 --> 0:12:04.040
<v Speaker 1>And I'm very grateful to those of you who volunteered

0:12:04.040 --> 0:12:06.800
<v Speaker 1>to try to answer this question without having the opportunity

0:12:06.840 --> 0:12:09.160
<v Speaker 1>to look it up or Google or get a PhD

0:12:09.200 --> 0:12:11.640
<v Speaker 1>in physics first, And so thank you to all of

0:12:11.640 --> 0:12:13.680
<v Speaker 1>those of you who volunteered. And if you would like

0:12:13.760 --> 0:12:17.360
<v Speaker 1>to hear your voice speculating baselessly on the podcast, please

0:12:17.400 --> 0:12:20.200
<v Speaker 1>don't be shy right to me. Two questions at Daniel

0:12:20.240 --> 0:12:23.400
<v Speaker 1>and Jorge dot com. Has anyone tried that? They're like, oh,

0:12:23.520 --> 0:12:25.640
<v Speaker 1>that's a great question, give me a seven years, I'll

0:12:25.679 --> 0:12:27.360
<v Speaker 1>come back with a PhD and answer. Or is that

0:12:27.400 --> 0:12:29.880
<v Speaker 1>what you do to your grad students every day? Yeah?

0:12:29.920 --> 0:12:31.520
<v Speaker 1>I take the answers people give me. I'm like, oh,

0:12:31.559 --> 0:12:33.200
<v Speaker 1>that's a good idea for a project, and then I

0:12:33.200 --> 0:12:36.360
<v Speaker 1>go write a grand proposal based on it nice, and

0:12:36.360 --> 0:12:39.240
<v Speaker 1>then you get dark bitter money for it, and my

0:12:39.280 --> 0:12:41.920
<v Speaker 1>grad students spend dark bitter years working on it. Yeah.

0:12:41.960 --> 0:12:44.080
<v Speaker 1>So here's what people had to say. When I figure

0:12:44.080 --> 0:12:48.640
<v Speaker 1>of radiation, I think of waves being admitted from something,

0:12:48.679 --> 0:12:50.840
<v Speaker 1>so that could be heat radiation, or it could be

0:12:50.920 --> 0:12:56.000
<v Speaker 1>light radiation. And even when something is invisible light to

0:12:56.160 --> 0:13:01.160
<v Speaker 1>humans radiation, UM, it's still quote unquote light. So dark

0:13:01.280 --> 0:13:05.240
<v Speaker 1>radiation I imagine. I think it has something to do

0:13:05.280 --> 0:13:09.120
<v Speaker 1>with dark energy. Probably I have to give all credit

0:13:09.360 --> 0:13:11.640
<v Speaker 1>to no Degress Tyson for why I know this. But

0:13:12.320 --> 0:13:17.000
<v Speaker 1>dark radiation is the mediator of dark matter particle interaction.

0:13:17.480 --> 0:13:21.760
<v Speaker 1>Say that five times fast. The best analogy for it is, um,

0:13:21.760 --> 0:13:24.320
<v Speaker 1>it's the dark matter equivalent of a photon. I think

0:13:24.520 --> 0:13:28.760
<v Speaker 1>dark radiation is radiation coming from dark matter right away.

0:13:28.800 --> 0:13:31.880
<v Speaker 1>It makes me think of dark matter and dark energy,

0:13:31.960 --> 0:13:34.720
<v Speaker 1>and I know they both interact with regular matter only

0:13:34.720 --> 0:13:39.360
<v Speaker 1>through gravity. So I would guess that it has something

0:13:39.400 --> 0:13:45.520
<v Speaker 1>to do with how dark matter radiates away or evaporates

0:13:45.559 --> 0:13:48.360
<v Speaker 1>in the same manner regular mass does with like a

0:13:48.360 --> 0:13:52.720
<v Speaker 1>black hole. All right, some pretty good answers here, mostly questions.

0:13:53.160 --> 0:13:55.960
<v Speaker 1>I feel like people answered back with some questions too. Yeah,

0:13:55.960 --> 0:13:57.800
<v Speaker 1>and people get the sense that it has something to

0:13:57.880 --> 0:14:00.720
<v Speaker 1>do with dark matter or dark inner g right, because

0:14:00.760 --> 0:14:03.760
<v Speaker 1>people have this concept that radiation energy, and so maybe

0:14:03.760 --> 0:14:06.760
<v Speaker 1>it falls into the like energy category rather than the

0:14:06.840 --> 0:14:10.000
<v Speaker 1>dark matter category. So yeah, some great answers. Yeah, I

0:14:10.040 --> 0:14:13.040
<v Speaker 1>feel like you've really sort of branded that word dark,

0:14:13.200 --> 0:14:15.840
<v Speaker 1>Like people automatically anything you associated with the word dark,

0:14:15.920 --> 0:14:18.560
<v Speaker 1>people know it's oh dark matter or dark energy. Yeah.

0:14:18.559 --> 0:14:20.920
<v Speaker 1>The funny thing is that the word dark and physics

0:14:21.000 --> 0:14:23.800
<v Speaker 1>just means we don't know anything about it. It's like

0:14:24.000 --> 0:14:27.200
<v Speaker 1>hidden from us, something we can't see, and so like

0:14:27.240 --> 0:14:30.680
<v Speaker 1>the only relationship between dark matter and dark energy really

0:14:30.760 --> 0:14:33.000
<v Speaker 1>is that we're pretty clueless about both of them. Well,

0:14:33.040 --> 0:14:34.920
<v Speaker 1>my question is, what's gonna happen when you do discover

0:14:35.000 --> 0:14:36.680
<v Speaker 1>what it is and when you can see it. Do

0:14:36.720 --> 0:14:39.120
<v Speaker 1>you need to change the name. Oh, that's a great question.

0:14:39.280 --> 0:14:42.880
<v Speaker 1>It depends, I suppose, on whether it remains dark or not.

0:14:43.080 --> 0:14:45.280
<v Speaker 1>You know, if we find some way to communicate with

0:14:45.600 --> 0:14:48.840
<v Speaker 1>the dark sector with these dark particles, then they won't

0:14:48.960 --> 0:14:52.200
<v Speaker 1>any longer be totally dark. So yeah, because it depends

0:14:52.320 --> 0:14:54.640
<v Speaker 1>specifically on what we figure out about it. Well, you

0:14:54.720 --> 0:14:56.440
<v Speaker 1>just said that it's you call it dark when you

0:14:56.480 --> 0:14:58.120
<v Speaker 1>don't know anything about it. So if you do know

0:14:58.200 --> 0:15:00.600
<v Speaker 1>something about it and can't see it, maybe think about

0:15:00.640 --> 0:15:03.400
<v Speaker 1>changing the name to like, you know, Horhi matter or

0:15:03.760 --> 0:15:06.480
<v Speaker 1>cam matter, just saying, you know, some suggestions. We'll put

0:15:06.520 --> 0:15:08.680
<v Speaker 1>that on the list, right next to white chocolate matter. Yeah,

0:15:08.960 --> 0:15:10.520
<v Speaker 1>I just realized its kind of running for a guy

0:15:10.600 --> 0:15:13.760
<v Speaker 1>named white sun. It sounds like you have some father issues. Yeah,

0:15:13.840 --> 0:15:18.360
<v Speaker 1>self loathing matter, that's what it is. That's that's pretty dark.

0:15:18.480 --> 0:15:21.440
<v Speaker 1>That's pretty dark. I'm gonna go in some more dark

0:15:21.520 --> 0:15:23.880
<v Speaker 1>chocolate and now feel better. Alright, So Daniel, we're going

0:15:23.920 --> 0:15:26.280
<v Speaker 1>to answer this question. What is dark radiation? Which is

0:15:26.560 --> 0:15:30.239
<v Speaker 1>sounds very tantalizing, it sounds cool. It sounds maybe dangerous

0:15:30.560 --> 0:15:32.880
<v Speaker 1>dark radiation, or maybe dark radiation is good for you

0:15:32.920 --> 0:15:36.040
<v Speaker 1>because it's the opposite of regular radiation. It's not like

0:15:36.400 --> 0:15:39.080
<v Speaker 1>entire radiation like that. What you need is a dose

0:15:39.120 --> 0:15:41.600
<v Speaker 1>of dark radiation that'll cure Peter Parker, right, he'll no

0:15:41.640 --> 0:15:44.880
<v Speaker 1>longer be Spider Man. The you know, damage right out

0:15:44.880 --> 0:15:49.960
<v Speaker 1>of you. No, dark radiation is an analog to radiation,

0:15:50.400 --> 0:15:52.800
<v Speaker 1>but in dark matter. So in our kind of matter,

0:15:52.960 --> 0:15:55.240
<v Speaker 1>we have you know, electrons and quarks, and they can

0:15:55.480 --> 0:15:59.600
<v Speaker 1>radiate things like photons because there are forces between these particles,

0:15:59.720 --> 0:16:03.920
<v Speaker 1>and so dark radiation would imagine that between dark matter

0:16:04.000 --> 0:16:07.840
<v Speaker 1>particles there might be some new dark force, and that

0:16:07.960 --> 0:16:11.280
<v Speaker 1>new dark force would be capable of generating dark radiation.

0:16:12.400 --> 0:16:15.120
<v Speaker 1>But you know, I think technically in physics you use

0:16:15.160 --> 0:16:19.120
<v Speaker 1>the word radiation for basically any particle, any quantum particle

0:16:19.200 --> 0:16:21.360
<v Speaker 1>moving in a quantum field, right, I think that's isn't

0:16:21.400 --> 0:16:24.520
<v Speaker 1>that the technical definition? Unfortunately, we're not totally consistent that

0:16:24.680 --> 0:16:27.640
<v Speaker 1>when we talk about radiation. When we talk about radiation

0:16:27.680 --> 0:16:30.760
<v Speaker 1>sort of chemically like what is producing radiation, that can

0:16:30.800 --> 0:16:33.760
<v Speaker 1>include things like photons, but also, as you say, high

0:16:33.840 --> 0:16:36.800
<v Speaker 1>energy particles. Here, when we talk about radiation and we

0:16:36.840 --> 0:16:39.880
<v Speaker 1>distinguish it from matter, we're talking about the particles that

0:16:39.880 --> 0:16:43.160
<v Speaker 1>are associated with forces rather than the particles that are

0:16:43.160 --> 0:16:46.720
<v Speaker 1>associated with matter. So for example, a photon would be radiation,

0:16:47.000 --> 0:16:49.480
<v Speaker 1>whereas a cork would be matter. Even if a cork

0:16:49.560 --> 0:16:52.440
<v Speaker 1>moving at high speed, a chemist would call it radiation.

0:16:52.600 --> 0:16:55.000
<v Speaker 1>Oh I see, So if we're going with the chemist definition,

0:16:55.040 --> 0:16:58.360
<v Speaker 1>then radiation is just any particle moving kind of what

0:16:58.480 --> 0:17:01.200
<v Speaker 1>if you're going, if you're going with the day annual interpretation. Here,

0:17:01.400 --> 0:17:04.479
<v Speaker 1>radiation just means a force particle or like a particle

0:17:04.520 --> 0:17:07.480
<v Speaker 1>associated with a force moving through space. The idea is

0:17:07.520 --> 0:17:11.760
<v Speaker 1>that maybe dark matter also produces dark radiation. That's the idea,

0:17:11.840 --> 0:17:15.520
<v Speaker 1>and it's a really interesting area to study because you know,

0:17:15.560 --> 0:17:17.960
<v Speaker 1>we don't know what's going on with dark matter. We

0:17:18.040 --> 0:17:20.360
<v Speaker 1>just know that there's a lot of it in the universe.

0:17:20.560 --> 0:17:23.359
<v Speaker 1>But it's tempting to extrapolate from the kind of matter

0:17:23.400 --> 0:17:25.280
<v Speaker 1>that we have, right, the kind of matter we have

0:17:25.400 --> 0:17:28.520
<v Speaker 1>does all sorts of interesting crazy stuff. It feels forces,

0:17:28.800 --> 0:17:32.240
<v Speaker 1>it forms complex objects like ice cream and chocolate and pizza.

0:17:32.680 --> 0:17:34.800
<v Speaker 1>So we don't know what's going on with the dark matter.

0:17:35.000 --> 0:17:37.600
<v Speaker 1>There's various possibilities all the way from like it's totally

0:17:37.600 --> 0:17:39.920
<v Speaker 1>inert it feels no forces. It just sort of sits

0:17:39.960 --> 0:17:43.840
<v Speaker 1>there and feels gravity too. It has like seventy five

0:17:43.960 --> 0:17:47.520
<v Speaker 1>new forces we haven't even imagined. They're capable of forming intricate,

0:17:47.560 --> 0:17:52.040
<v Speaker 1>complex things that would blow our minds. And in that scenario,

0:17:52.280 --> 0:17:55.320
<v Speaker 1>those forces would be mediated by dark particles, and so

0:17:55.359 --> 0:17:58.040
<v Speaker 1>those would be dark radiation, right, Because I think all

0:17:58.080 --> 0:18:00.320
<v Speaker 1>we know about dark matter is that it it sort

0:18:00.359 --> 0:18:03.280
<v Speaker 1>of looks like it's a big giant, fuzzy clump. But

0:18:03.359 --> 0:18:04.879
<v Speaker 1>that's just what we can see of it. You know,

0:18:04.960 --> 0:18:08.359
<v Speaker 1>it could be something really detailed and organized. We just

0:18:08.400 --> 0:18:11.080
<v Speaker 1>have a very unfocused view of it. That's right, And

0:18:11.119 --> 0:18:13.840
<v Speaker 1>that's because so far, our only way to learn things

0:18:13.880 --> 0:18:16.800
<v Speaker 1>about dark matter, to interact with dark matter so as

0:18:16.840 --> 0:18:19.120
<v Speaker 1>to figure out like where it is and what it's doing,

0:18:19.560 --> 0:18:23.159
<v Speaker 1>is through gravity, and gravity is the weakest force in

0:18:23.200 --> 0:18:25.960
<v Speaker 1>the universe we've discovered, and not by a little bit,

0:18:26.000 --> 0:18:28.600
<v Speaker 1>but by like ten to the thirty six. It's like

0:18:28.720 --> 0:18:31.520
<v Speaker 1>super duper crazy week. So it's like trying to look

0:18:31.600 --> 0:18:35.040
<v Speaker 1>at dark matter, but you're looking through very very dark glasses,

0:18:35.080 --> 0:18:37.080
<v Speaker 1>so you can just barely see it. You can only

0:18:37.119 --> 0:18:39.520
<v Speaker 1>see huge clumps of it, and that gives us a

0:18:39.600 --> 0:18:42.199
<v Speaker 1>very fuzzy view of what's going on. The glasses are

0:18:42.240 --> 0:18:44.600
<v Speaker 1>made out of dark matter. I'm a little confused here.

0:18:44.960 --> 0:18:50.760
<v Speaker 1>They filter dark radiation. I think you mean like fuzzy glasses. Yeah, yeah,

0:18:50.880 --> 0:18:52.520
<v Speaker 1>all right, Well maybe for the people who are not

0:18:52.560 --> 0:18:55.080
<v Speaker 1>familiar with dark matter, maybe give us a quick refresher

0:18:55.200 --> 0:18:56.840
<v Speaker 1>of what it is and how we know it's there.

0:18:57.000 --> 0:18:59.040
<v Speaker 1>So we don't know that much about dark matter, but

0:18:59.080 --> 0:19:01.439
<v Speaker 1>we do know that it makes up most of the

0:19:01.480 --> 0:19:04.200
<v Speaker 1>stuff in the universe, and it's some kind of matter

0:19:04.520 --> 0:19:07.560
<v Speaker 1>by which we mean that it provides gravity. And you know,

0:19:07.600 --> 0:19:11.040
<v Speaker 1>we invented the idea of dark matter to explain why

0:19:11.080 --> 0:19:15.119
<v Speaker 1>there was gravity in the universe that we couldn't otherwise explain. So,

0:19:15.160 --> 0:19:18.600
<v Speaker 1>for example, we see that galaxies are rotating really really fast,

0:19:18.920 --> 0:19:21.960
<v Speaker 1>and there's apparently enough gravity to hold them together to

0:19:22.040 --> 0:19:24.920
<v Speaker 1>keep the stars from going out into interstellar space being

0:19:24.960 --> 0:19:27.760
<v Speaker 1>tossed out. But we can't explain where that gravity is

0:19:27.800 --> 0:19:30.840
<v Speaker 1>coming from, so we say probably dark matter. And if

0:19:30.840 --> 0:19:33.520
<v Speaker 1>we want to understand the structure of the universe, how

0:19:33.560 --> 0:19:36.439
<v Speaker 1>it got to have these galaxies and these superclusters and

0:19:36.440 --> 0:19:38.720
<v Speaker 1>all of this stuff. If you run a simulation of

0:19:38.760 --> 0:19:42.080
<v Speaker 1>the universe without dark matter, then it just doesn't form

0:19:42.160 --> 0:19:45.520
<v Speaker 1>galaxies and stars this quickly. You need more gravity to

0:19:45.600 --> 0:19:48.479
<v Speaker 1>pull that stuff together. So we need dark matter not

0:19:48.560 --> 0:19:51.399
<v Speaker 1>just to explain how galaxies are spinning, but also the

0:19:51.440 --> 0:19:54.440
<v Speaker 1>whole structure of the universe. And if we look in

0:19:54.520 --> 0:19:57.240
<v Speaker 1>the very early ever beginnings of the universe and we

0:19:57.280 --> 0:20:00.159
<v Speaker 1>see like how wiggles in the first plasma of the

0:20:00.280 --> 0:20:03.720
<v Speaker 1>universe formed, and how those wiggles propagated, they don't really

0:20:03.760 --> 0:20:07.720
<v Speaker 1>make sense unless you add dark matter to our calculations.

0:20:07.720 --> 0:20:09.560
<v Speaker 1>So we have a lot of evidence that dark matter

0:20:09.600 --> 0:20:11.880
<v Speaker 1>is a thing, that it's out there, that it clumps

0:20:11.960 --> 0:20:15.640
<v Speaker 1>together in these big structures that shaped our whole universe.

0:20:15.840 --> 0:20:18.040
<v Speaker 1>We just don't really know what it's made out of

0:20:18.040 --> 0:20:20.879
<v Speaker 1>other than something that gives gravity. Yeah, we we know

0:20:20.960 --> 0:20:22.880
<v Speaker 1>it's there and it has to be there to explain

0:20:22.960 --> 0:20:25.320
<v Speaker 1>what we see. But I think that's the crazy things

0:20:25.359 --> 0:20:27.840
<v Speaker 1>that we don't know what it is, Like, we really

0:20:27.840 --> 0:20:29.800
<v Speaker 1>have no idea, Like it could be a totally new

0:20:29.880 --> 0:20:32.240
<v Speaker 1>kind of thing that's not even a particle, or even

0:20:32.320 --> 0:20:35.040
<v Speaker 1>something sort of like cohesive. It could be anything, right, Yeah,

0:20:35.040 --> 0:20:37.440
<v Speaker 1>And we've done a lot of podcast episodes diving into

0:20:37.480 --> 0:20:40.560
<v Speaker 1>some of those examples. Sort Of the mainstream idea is

0:20:40.600 --> 0:20:44.439
<v Speaker 1>a whim weakly interacting massive particle that's sort of like,

0:20:44.520 --> 0:20:47.679
<v Speaker 1>you know, a generic idea like what's the simplest possible

0:20:47.680 --> 0:20:50.680
<v Speaker 1>explanation for dark matter? But there's lots of other more

0:20:50.720 --> 0:20:54.800
<v Speaker 1>exotic and fascinating ideas, from things like axions, these weird

0:20:54.920 --> 0:20:59.240
<v Speaker 1>heavy photons, to things like primordial black holes formed very

0:20:59.359 --> 0:21:02.480
<v Speaker 1>very early in the universe to things like super duper

0:21:02.560 --> 0:21:07.199
<v Speaker 1>long wave photons generated by dark stars. So we just

0:21:07.280 --> 0:21:08.880
<v Speaker 1>don't really know what it is. And as you say,

0:21:08.920 --> 0:21:12.200
<v Speaker 1>it might not even be a particle. It might be

0:21:12.280 --> 0:21:15.159
<v Speaker 1>that this whole idea of particles and fields and quantum

0:21:15.240 --> 0:21:18.000
<v Speaker 1>forces only applies to the little bit of the universe

0:21:18.040 --> 0:21:20.160
<v Speaker 1>that we've been studying for the last few hundred years,

0:21:20.200 --> 0:21:22.399
<v Speaker 1>and that you can't extrapolate to the rest of the

0:21:22.480 --> 0:21:24.679
<v Speaker 1>universe the same way you can't, like look at an

0:21:24.720 --> 0:21:27.159
<v Speaker 1>elephant's tail and assume the rest of the elephant is

0:21:27.200 --> 0:21:29.320
<v Speaker 1>like the tail. So it might be that we have

0:21:29.560 --> 0:21:33.160
<v Speaker 1>dramatic mind blowing lessons to be learned about dark matter,

0:21:33.560 --> 0:21:35.400
<v Speaker 1>or it could be super boring and just be one

0:21:35.440 --> 0:21:38.760
<v Speaker 1>particle that doesn't do anything. Some pretty extreme possibilities there.

0:21:39.119 --> 0:21:41.000
<v Speaker 1>But but are you saying that maybe, like maybe even

0:21:41.080 --> 0:21:44.400
<v Speaker 1>quantum mechanics only applies to a small part of the universe.

0:21:44.640 --> 0:21:46.560
<v Speaker 1>I think that's true. Yeah, All of the tests that

0:21:46.600 --> 0:21:49.879
<v Speaker 1>we've done of quantum mechanics use our kind of matter

0:21:50.080 --> 0:21:52.320
<v Speaker 1>and our kind of forces, and so we have a

0:21:52.320 --> 0:21:56.000
<v Speaker 1>pretty good quantum description of quantum particles, but we don't

0:21:56.000 --> 0:21:59.399
<v Speaker 1>really have a quantum description of gravity and gravity is

0:21:59.440 --> 0:22:01.439
<v Speaker 1>our poor to dark matter. The only thing we know

0:22:01.480 --> 0:22:04.359
<v Speaker 1>about dark matter is that it does feel gravity, and

0:22:04.400 --> 0:22:06.800
<v Speaker 1>so it could be some other new, weird kind of

0:22:06.920 --> 0:22:11.119
<v Speaker 1>thing that generates gravity but doesn't otherwise follow the rules

0:22:11.119 --> 0:22:15.520
<v Speaker 1>of quantum mechanics. Well, all right, so that's a dark matter. Now,

0:22:15.560 --> 0:22:18.800
<v Speaker 1>what would you say is a dark force? Besides the

0:22:18.840 --> 0:22:22.600
<v Speaker 1>obvious Star Wars reference, a dark force would be anybody

0:22:22.600 --> 0:22:26.280
<v Speaker 1>who tries to force me to eat white chocolate, the

0:22:26.400 --> 0:22:29.320
<v Speaker 1>dark force in my life. Now, a dark force would

0:22:29.320 --> 0:22:32.159
<v Speaker 1>be in the assumption that dark matter is made of

0:22:32.200 --> 0:22:36.280
<v Speaker 1>particles that follow the rules of quantum mechanics like our particles,

0:22:36.720 --> 0:22:39.240
<v Speaker 1>then you might imagine that they also feel some dark

0:22:39.320 --> 0:22:43.000
<v Speaker 1>forces between them. You know that too. Dark matter particles

0:22:43.000 --> 0:22:47.040
<v Speaker 1>can exchange some like dark photon or dark z boson

0:22:47.240 --> 0:22:50.199
<v Speaker 1>or dark higgs boson that they can like push or

0:22:50.240 --> 0:22:52.159
<v Speaker 1>pull on each other. They can do more than just

0:22:52.280 --> 0:22:55.679
<v Speaker 1>feel each other's gravity. Maybe there's some additional dark forces

0:22:55.760 --> 0:22:58.200
<v Speaker 1>and they're passing particles back and forth as a way

0:22:58.200 --> 0:23:01.040
<v Speaker 1>to mediate those forces. Rights. Even the matter in our

0:23:01.119 --> 0:23:04.280
<v Speaker 1>universe is sort of selective about which forces it feels

0:23:04.359 --> 0:23:07.760
<v Speaker 1>or which forces they give out, right, Like some particles

0:23:07.800 --> 0:23:11.679
<v Speaker 1>in our type of matter only feel like the magnetic forces,

0:23:11.800 --> 0:23:14.159
<v Speaker 1>or they don't feel the strong force and things like that. Right,

0:23:14.280 --> 0:23:17.800
<v Speaker 1>that's exactly right. Neutrinos, for example, only feel the weak force.

0:23:17.960 --> 0:23:22.440
<v Speaker 1>They ignore the strong force, they ignore electromagnetism. Electrons they

0:23:22.560 --> 0:23:25.719
<v Speaker 1>do feel electromagnetism and the weak force, but they ignore

0:23:25.760 --> 0:23:28.680
<v Speaker 1>the strong force. Only the corks feel all of the forces,

0:23:28.800 --> 0:23:32.040
<v Speaker 1>including the strong force. And so for an individual particle,

0:23:32.119 --> 0:23:34.680
<v Speaker 1>you can ask, like whether it has a charge for

0:23:34.760 --> 0:23:38.720
<v Speaker 1>that force. So electromagnetism only interact with particles that have

0:23:38.840 --> 0:23:41.960
<v Speaker 1>electric charges. For example, we know that dark matter doesn't

0:23:41.960 --> 0:23:44.600
<v Speaker 1>have electric charges, and it doesn't have weak charges, or

0:23:44.640 --> 0:23:47.680
<v Speaker 1>it doesn't have strong charges, but it might have charges

0:23:47.760 --> 0:23:51.199
<v Speaker 1>for other forces we haven't yet discovered. Wow, like there

0:23:51.240 --> 0:23:54.000
<v Speaker 1>could be a whole different category of forces that we

0:23:54.119 --> 0:23:56.680
<v Speaker 1>just don't happen to feel in our kind of matter,

0:23:57.040 --> 0:23:59.359
<v Speaker 1>but that maybe dark matter it does feel exactly So

0:23:59.400 --> 0:24:02.359
<v Speaker 1>there could be like one or forty new forces that

0:24:02.400 --> 0:24:05.480
<v Speaker 1>we haven't yet discovered because our particles don't feel those,

0:24:05.800 --> 0:24:09.000
<v Speaker 1>or maybe more, not just forty, maybe four thousand exactly.

0:24:11.119 --> 0:24:13.200
<v Speaker 1>All right, Well, let's dig into what this new kind

0:24:13.200 --> 0:24:16.000
<v Speaker 1>of force might be, this dark force and what it

0:24:16.080 --> 0:24:17.960
<v Speaker 1>could all mean and whether or not we can never

0:24:18.000 --> 0:24:20.760
<v Speaker 1>hope to see it or feel it. But first let's

0:24:20.760 --> 0:24:35.920
<v Speaker 1>take a quick break. All right, we're talking about dark radiation,

0:24:36.080 --> 0:24:37.919
<v Speaker 1>and in this case, the word radiation sort of is

0:24:37.920 --> 0:24:40.920
<v Speaker 1>associated with the word force. So really we're asking does

0:24:41.000 --> 0:24:45.080
<v Speaker 1>dark matter feel dark forces that maybe are out there,

0:24:45.080 --> 0:24:47.399
<v Speaker 1>but that we in our kind of matter can feel

0:24:47.480 --> 0:24:49.960
<v Speaker 1>or touch or detect. But then maybe it is maybe

0:24:50.160 --> 0:24:53.720
<v Speaker 1>organizing dark matter into structures or maybe you know, even

0:24:53.800 --> 0:24:57.400
<v Speaker 1>making dark matter particles and Adams exactly. And it's part

0:24:57.440 --> 0:25:00.439
<v Speaker 1>of this imagination game we play, you know, we wonder

0:25:00.520 --> 0:25:03.320
<v Speaker 1>what's going on out there in the dark universe. Is

0:25:03.320 --> 0:25:06.600
<v Speaker 1>it simple, is it fascinating, is it complex? What is

0:25:06.640 --> 0:25:09.320
<v Speaker 1>going on? What is they're out there to learn? And

0:25:09.560 --> 0:25:11.879
<v Speaker 1>usually when we go out and explore the universe, we

0:25:11.960 --> 0:25:16.120
<v Speaker 1>find that things are crazier and more fascinating and richer

0:25:16.280 --> 0:25:19.120
<v Speaker 1>than we ever imagined. And so we're at this point

0:25:19.160 --> 0:25:21.240
<v Speaker 1>where we really don't know about most of the universe.

0:25:21.280 --> 0:25:22.840
<v Speaker 1>But at some point in the future, I hope a

0:25:22.920 --> 0:25:25.000
<v Speaker 1>hundred years, five hundred years from now, we will know

0:25:25.040 --> 0:25:27.600
<v Speaker 1>what's going on in the dark sector and those people

0:25:27.680 --> 0:25:31.159
<v Speaker 1>will look back at our ideas as ridiculous. Probably you

0:25:31.240 --> 0:25:34.080
<v Speaker 1>might think of us as the Dark Ages physics. They

0:25:34.280 --> 0:25:36.800
<v Speaker 1>like the really dark ages, not that the trial run

0:25:36.840 --> 0:25:40.760
<v Speaker 1>in the Middle Ages, but more serious. Yes, back when

0:25:40.760 --> 0:25:45.359
<v Speaker 1>people ate white chocolate, that's right. Maybe we're looking forward

0:25:45.400 --> 0:25:50.000
<v Speaker 1>to an age of dark enlightenment, in the age of oxymorons.

0:25:50.160 --> 0:25:52.719
<v Speaker 1>But yeah, So in our kind of matter, we feel

0:25:52.880 --> 0:25:56.879
<v Speaker 1>the electromagnetic force, which is what basically holds our atoms together.

0:25:57.040 --> 0:25:58.760
<v Speaker 1>And what you know when you touch something, when you

0:25:58.800 --> 0:26:01.199
<v Speaker 1>touch the table or you hold the banana, that's the

0:26:01.200 --> 0:26:04.479
<v Speaker 1>force you're feeling. And that force is transmitted by a

0:26:04.520 --> 0:26:07.199
<v Speaker 1>particle called the photon. So the photon is not just

0:26:07.320 --> 0:26:10.960
<v Speaker 1>lighted Tosso what transmits the electromagnetic force? And so the

0:26:11.040 --> 0:26:13.919
<v Speaker 1>question daniel I guess is does dark matter have the

0:26:13.960 --> 0:26:17.520
<v Speaker 1>equivalent of a photon or at least an electromagnetic force field.

0:26:17.680 --> 0:26:20.000
<v Speaker 1>We just don't know, and so we're playing this game

0:26:20.040 --> 0:26:22.639
<v Speaker 1>of trying to extrapolate from what we do know. And

0:26:22.640 --> 0:26:25.280
<v Speaker 1>in the same way that we imagine maybe dark matter

0:26:25.560 --> 0:26:28.399
<v Speaker 1>is made of a particle, because we're made of particles,

0:26:28.520 --> 0:26:31.480
<v Speaker 1>we wonder if there are dark forces that look like

0:26:31.600 --> 0:26:34.800
<v Speaker 1>our forces. And so one of the simplest forces to

0:26:34.880 --> 0:26:38.520
<v Speaker 1>understand is electromagnetism because it just has like one particle

0:26:38.600 --> 0:26:41.159
<v Speaker 1>and it interacts with lots of stuff, and so a

0:26:41.280 --> 0:26:44.600
<v Speaker 1>simple proposals to say, well, what if dark matter has

0:26:44.640 --> 0:26:48.840
<v Speaker 1>a dark electromagnetism, meaning a dark photon. This would be

0:26:48.880 --> 0:26:51.399
<v Speaker 1>a particle that has a lot of properties similar to

0:26:51.560 --> 0:26:54.639
<v Speaker 1>our photon, but it would be different. You know, those

0:26:54.720 --> 0:26:58.160
<v Speaker 1>dark matter particles would have like a dark electric charge

0:26:58.480 --> 0:27:01.080
<v Speaker 1>and the dark photon, but only interact with particles with

0:27:01.160 --> 0:27:04.760
<v Speaker 1>a dark electric charge, not ones with our electric charge

0:27:05.040 --> 0:27:09.080
<v Speaker 1>and our normal vanilla photons wouldn't interact with dark matter

0:27:09.160 --> 0:27:12.040
<v Speaker 1>because they don't have an electric charge, only a dark

0:27:12.160 --> 0:27:16.080
<v Speaker 1>electric charge. But it wouldn't necessarily be the same or

0:27:16.119 --> 0:27:19.000
<v Speaker 1>the sort of the analog of light. Right you're just

0:27:19.000 --> 0:27:21.199
<v Speaker 1>saying like, maybe it's a force, and let's why not

0:27:21.359 --> 0:27:23.960
<v Speaker 1>let's qual it the dark electromagnetic force. It doesn't have

0:27:24.040 --> 0:27:26.040
<v Speaker 1>to be, and it could be the dark matter fields

0:27:26.080 --> 0:27:28.439
<v Speaker 1>forces that are more similar to like our weak force,

0:27:28.800 --> 0:27:31.040
<v Speaker 1>or forces that are more similar to our strong force,

0:27:31.400 --> 0:27:34.000
<v Speaker 1>or forces that are totally different from these forces and

0:27:34.080 --> 0:27:37.560
<v Speaker 1>have other new weird capacities. Right before we discovered the

0:27:37.600 --> 0:27:41.399
<v Speaker 1>strong force, who could have imagined this crazy force, you know,

0:27:41.440 --> 0:27:43.960
<v Speaker 1>where it gets stronger as things get further apart, and

0:27:43.960 --> 0:27:46.639
<v Speaker 1>it has like eight different kinds of gluons pulling it together.

0:27:46.920 --> 0:27:49.640
<v Speaker 1>It's bonkers. Nobody would have written that into the script.

0:27:49.880 --> 0:27:52.320
<v Speaker 1>So it's possible that there are other kinds of forces.

0:27:52.440 --> 0:27:54.960
<v Speaker 1>But if there is a dark force that's very similar

0:27:55.040 --> 0:27:58.360
<v Speaker 1>to electromagnetism, then that dark photon would have properties very

0:27:58.359 --> 0:28:01.399
<v Speaker 1>similar to our photon, because those properties come from the

0:28:01.400 --> 0:28:04.800
<v Speaker 1>structure of the force, all right. And also it makes

0:28:04.800 --> 0:28:07.560
<v Speaker 1>for a cool name, dark photon, because it kind of

0:28:07.600 --> 0:28:09.840
<v Speaker 1>it trips up your brain, right, Like, how can a

0:28:09.840 --> 0:28:13.080
<v Speaker 1>photon which transmits light be dark? That's right, because it

0:28:13.119 --> 0:28:18.200
<v Speaker 1>transmits dark light into dark eyeballs. Oh yeah, I feel

0:28:18.200 --> 0:28:20.119
<v Speaker 1>like you should maybe just call it something different. What

0:28:20.160 --> 0:28:23.240
<v Speaker 1>would you call it the dark on the invisible photon?

0:28:23.320 --> 0:28:25.240
<v Speaker 1>I don't know, dark on is good, But then what

0:28:25.280 --> 0:28:27.679
<v Speaker 1>do you find another force? Yeah, we'll have to be

0:28:27.720 --> 0:28:30.320
<v Speaker 1>even more creative with our names. We'll just have, you know,

0:28:30.400 --> 0:28:32.560
<v Speaker 1>a brainstorming session with lots of chocolate, and we'll come

0:28:32.640 --> 0:28:35.080
<v Speaker 1>up with something good and then and then who knows

0:28:35.080 --> 0:28:36.840
<v Speaker 1>what you'll get out of it? Maybe a heart attack,

0:28:37.080 --> 0:28:39.640
<v Speaker 1>all right? So dark matter might feel this new kind

0:28:39.680 --> 0:28:42.360
<v Speaker 1>of or strange new kind of force, a dark force.

0:28:42.600 --> 0:28:44.960
<v Speaker 1>So how would we ever detected Daniel, would we ever

0:28:45.000 --> 0:28:47.480
<v Speaker 1>hope to feel it or you know, know it's there

0:28:47.520 --> 0:28:49.600
<v Speaker 1>if we can't touch it or see it. So in

0:28:49.640 --> 0:28:53.080
<v Speaker 1>the end, this question is really asking what dark matter

0:28:53.200 --> 0:28:56.640
<v Speaker 1>does to itself? You know, can we speculate about what's

0:28:56.640 --> 0:28:59.400
<v Speaker 1>going on in the dark sector beyond these particles existing

0:28:59.680 --> 0:29:02.920
<v Speaker 1>can like touch each other and become sticky and do stuff,

0:29:03.000 --> 0:29:05.160
<v Speaker 1>And so we have sort of two ways to probe this.

0:29:05.360 --> 0:29:07.400
<v Speaker 1>The first category is sort of like indirect ways to

0:29:07.440 --> 0:29:10.120
<v Speaker 1>look at it, and broadly speaking, we can tell that

0:29:10.240 --> 0:29:13.040
<v Speaker 1>dark matter is doing things because of its gravity. And

0:29:13.240 --> 0:29:15.840
<v Speaker 1>even though it's not a great way to study dark matter,

0:29:16.120 --> 0:29:19.040
<v Speaker 1>we can use its gravitational effects to ask questions like

0:29:19.440 --> 0:29:22.680
<v Speaker 1>is it clumping? Is it interacting with itself? Because if

0:29:22.680 --> 0:29:25.400
<v Speaker 1>it interacts with itself, it forms sort of different structures

0:29:25.400 --> 0:29:27.840
<v Speaker 1>that have different gravity. So we can sort of ask

0:29:27.920 --> 0:29:30.800
<v Speaker 1>questions about whether dark matter is feeling itself by trying

0:29:30.840 --> 0:29:33.960
<v Speaker 1>to look to see how it organizes itself in the universe.

0:29:34.240 --> 0:29:36.840
<v Speaker 1>I see, we can't maybe see it directly or touch

0:29:37.000 --> 0:29:40.200
<v Speaker 1>dark matter, but if we can somehow kind of know

0:29:40.280 --> 0:29:42.120
<v Speaker 1>what it's doing, And if we see it doing stuff

0:29:42.120 --> 0:29:44.400
<v Speaker 1>to itself, then we know that it's there must be

0:29:44.440 --> 0:29:47.280
<v Speaker 1>some kind of force that it does interact with exactly.

0:29:47.360 --> 0:29:50.080
<v Speaker 1>For example, if dark matter felt a version of the

0:29:50.120 --> 0:29:53.120
<v Speaker 1>strong force, if it interacted with itself very very strongly

0:29:53.200 --> 0:29:56.400
<v Speaker 1>and could like clump together very very very sticky ways,

0:29:56.600 --> 0:29:59.200
<v Speaker 1>then it would form much denser objects than we see

0:29:59.240 --> 0:30:03.000
<v Speaker 1>currently in the universe. Currently, dark matter looks really big

0:30:03.040 --> 0:30:06.640
<v Speaker 1>and fluffy, like the dark matter in our galaxy isn't

0:30:06.640 --> 0:30:09.400
<v Speaker 1>nearly as compact as the normal matter in our galaxy.

0:30:09.440 --> 0:30:12.320
<v Speaker 1>It spreads out much further out. It's a big, fluffy

0:30:12.360 --> 0:30:16.000
<v Speaker 1>cloud hasn't collapsed nearly as much, and we think that's

0:30:16.040 --> 0:30:19.640
<v Speaker 1>because it's not as sticky as our matter. We think

0:30:19.640 --> 0:30:22.400
<v Speaker 1>that it doesn't feel like a super powerful force that

0:30:22.520 --> 0:30:25.000
<v Speaker 1>sticks it together, because that would help it like form

0:30:25.120 --> 0:30:28.640
<v Speaker 1>denser objects like dark planets and dark stars. So we

0:30:28.680 --> 0:30:32.520
<v Speaker 1>already know very broadly something about how dark matter can't

0:30:32.640 --> 0:30:35.840
<v Speaker 1>feel itself because it stays sort of fluffy and doesn't

0:30:35.880 --> 0:30:38.040
<v Speaker 1>seem to clump as much as normal matter. Right, But

0:30:38.080 --> 0:30:40.160
<v Speaker 1>I wonder you know it sort of looks fluffy to

0:30:40.240 --> 0:30:42.280
<v Speaker 1>us because we don't have a good way of seeing it.

0:30:42.360 --> 0:30:44.560
<v Speaker 1>You know, we talked earlier about having we kind of

0:30:44.600 --> 0:30:47.000
<v Speaker 1>have a fuzzy lens when we look at dark matter

0:30:47.360 --> 0:30:50.040
<v Speaker 1>because we can only see it through gravity. You know,

0:30:50.160 --> 0:30:52.600
<v Speaker 1>is it maybe even possible that there are dark matter

0:30:52.640 --> 0:30:55.760
<v Speaker 1>stars out there, which is don't have the resolution to

0:30:55.840 --> 0:30:58.040
<v Speaker 1>see them. You know, absolutely, there's a very big loophole

0:30:58.040 --> 0:30:59.840
<v Speaker 1>in this argument that you allude to, which is that

0:31:00.040 --> 0:31:02.040
<v Speaker 1>you can see sort of the bulk of dark matter,

0:31:02.080 --> 0:31:04.960
<v Speaker 1>but we can't tell what it's doing in detail. In

0:31:04.960 --> 0:31:08.040
<v Speaker 1>an episode recently about where is the dark matter, and

0:31:08.080 --> 0:31:09.880
<v Speaker 1>we talked about how we can tell sort of the

0:31:10.000 --> 0:31:12.600
<v Speaker 1>dark matters in these big fluffy clouds, but we also

0:31:12.720 --> 0:31:15.280
<v Speaker 1>can't really tell if it is forming clumps. So you

0:31:15.280 --> 0:31:17.920
<v Speaker 1>could imagine that dark matter maybe it's made out of

0:31:17.960 --> 0:31:20.320
<v Speaker 1>a few different kinds of things. So most of it,

0:31:20.360 --> 0:31:22.160
<v Speaker 1>maybe like you know, half of the dark matter or

0:31:22.160 --> 0:31:24.440
<v Speaker 1>three fourths of the dark matter, is some big, fluffy

0:31:24.480 --> 0:31:26.840
<v Speaker 1>stuff that hardly interacts with itself. But there could be

0:31:26.880 --> 0:31:30.160
<v Speaker 1>a component of the dark matter that does do interesting,

0:31:30.280 --> 0:31:34.280
<v Speaker 1>complicated things and has crazy interactions and forms dark stars

0:31:34.280 --> 0:31:36.760
<v Speaker 1>and dark planets and dark life, and that would not

0:31:36.920 --> 0:31:39.920
<v Speaker 1>mess up the distribution of dark matter, because remember, there's

0:31:40.000 --> 0:31:43.360
<v Speaker 1>like so much dark matter out there that even like

0:31:43.640 --> 0:31:46.640
<v Speaker 1>if a quarter of it does more interesting stuff, that's

0:31:46.680 --> 0:31:49.320
<v Speaker 1>still more than all of our kind of matter. So

0:31:49.360 --> 0:31:51.760
<v Speaker 1>there's plenty of room to have like a component that

0:31:51.800 --> 0:31:55.760
<v Speaker 1>has complex interactions without missing up these constraints about the

0:31:55.840 --> 0:31:58.120
<v Speaker 1>big picture of dark matter. So I feel like dark

0:31:58.120 --> 0:31:59.960
<v Speaker 1>matter could be in the shape of I don't know,

0:32:00.120 --> 0:32:03.640
<v Speaker 1>like rubber duckies. It's just that they're sort of distributed

0:32:03.640 --> 0:32:06.440
<v Speaker 1>out in space, these rubber duckies, and to us it

0:32:06.440 --> 0:32:08.920
<v Speaker 1>just seems like a big fluffy cloud. Yeah, most of

0:32:08.960 --> 0:32:10.840
<v Speaker 1>it has to be pretty big and fluffy to form

0:32:10.880 --> 0:32:13.720
<v Speaker 1>that big fluffy cloud. It can't stick to itself. But

0:32:13.800 --> 0:32:16.480
<v Speaker 1>it could be that inside that big fluffy cloud there

0:32:16.520 --> 0:32:19.040
<v Speaker 1>are like rubber duckies made out of like a special

0:32:19.160 --> 0:32:21.080
<v Speaker 1>kind of dark matter, you know, the way they like

0:32:21.160 --> 0:32:23.800
<v Speaker 1>our matter. There's lots of different kinds is electrons, is

0:32:23.840 --> 0:32:27.360
<v Speaker 1>different kinds of quarks. Right, we have twelve different matter particles.

0:32:27.720 --> 0:32:30.240
<v Speaker 1>Dark matter could have like fifty different kinds of particles,

0:32:30.240 --> 0:32:32.520
<v Speaker 1>and maybe most of them don't interact and make a

0:32:32.520 --> 0:32:35.160
<v Speaker 1>big fluffy cloud, but one or two of them form

0:32:35.320 --> 0:32:37.840
<v Speaker 1>dark rubber duckies that are floating out there in the universe,

0:32:37.840 --> 0:32:40.080
<v Speaker 1>and we couldn't tell the difference because the only way

0:32:40.120 --> 0:32:43.640
<v Speaker 1>we can see them is through their overall gravitational interaction.

0:32:43.680 --> 0:32:46.240
<v Speaker 1>I'm pretty sure that's what dark Vader uses in his bathtuff.

0:32:46.560 --> 0:32:48.760
<v Speaker 1>But I guess the question is, you know, isn't the

0:32:48.800 --> 0:32:51.000
<v Speaker 1>fact that dark matter does seem to be sort of

0:32:51.040 --> 0:32:53.720
<v Speaker 1>fluffy and doesn't seem to stick to itself. Is that

0:32:53.760 --> 0:32:57.120
<v Speaker 1>evidence that maybe it doesn't interact with itself other than

0:32:57.160 --> 0:32:59.880
<v Speaker 1>with gravity. It's evidence that it doesn't interact with itself

0:33:00.160 --> 0:33:03.200
<v Speaker 1>very very strongly. But again, the loophole is that some

0:33:03.360 --> 0:33:05.880
<v Speaker 1>component of it might be able to Now. The way

0:33:05.880 --> 0:33:08.080
<v Speaker 1>to probe that a little bit more deeply is to

0:33:08.080 --> 0:33:11.040
<v Speaker 1>do experiments. Is to take like two big clouds of

0:33:11.120 --> 0:33:13.960
<v Speaker 1>dark matter and throw them against each other and see

0:33:14.320 --> 0:33:16.560
<v Speaker 1>if they pass right through each other, or if maybe

0:33:16.560 --> 0:33:19.200
<v Speaker 1>they stick together and make them like dark explosions. That

0:33:19.280 --> 0:33:22.080
<v Speaker 1>kind of experiment is pretty tough to do, but we

0:33:22.080 --> 0:33:24.320
<v Speaker 1>were lucky and the universe did it for us. It

0:33:24.480 --> 0:33:28.760
<v Speaker 1>collided two huge clusters of galaxies, each of which have

0:33:28.880 --> 0:33:32.320
<v Speaker 1>their own dark matter associated with them, smashed them together

0:33:32.400 --> 0:33:34.200
<v Speaker 1>millions of years ago, and we got to see what

0:33:34.280 --> 0:33:36.400
<v Speaker 1>happened and what did happen, and so this is called

0:33:36.400 --> 0:33:38.200
<v Speaker 1>the bullet cluster. You can go ahead and look at

0:33:38.240 --> 0:33:41.480
<v Speaker 1>these pictures online if you're interested. It's really beautiful. What

0:33:41.600 --> 0:33:44.880
<v Speaker 1>happened is that the stars in these galaxy clusters mostly

0:33:44.920 --> 0:33:47.920
<v Speaker 1>passed through themselves because stars are pretty sparse, so it's

0:33:47.920 --> 0:33:50.480
<v Speaker 1>like two clouds of sand passing through each other. The

0:33:50.600 --> 0:33:53.320
<v Speaker 1>gas and the dust that were in these galaxies smashed

0:33:53.360 --> 0:33:55.800
<v Speaker 1>together and admitted a lot of light and radiation. But

0:33:55.840 --> 0:33:59.120
<v Speaker 1>the dark matter looks like it basically passed right through itself.

0:33:59.520 --> 0:34:01.360
<v Speaker 1>You might ask school like, how could we know where

0:34:01.360 --> 0:34:03.240
<v Speaker 1>the dark matter is? We can see the dark matter

0:34:03.280 --> 0:34:06.040
<v Speaker 1>because it distorts the stuff behind it. From the dark

0:34:06.080 --> 0:34:09.240
<v Speaker 1>matter is matter, it feels gravity, so it bends space

0:34:09.280 --> 0:34:12.759
<v Speaker 1>a little bit, which creates like gravitational distortions in the

0:34:12.840 --> 0:34:15.960
<v Speaker 1>light that passes through it. So from this bullet cluster,

0:34:16.040 --> 0:34:18.719
<v Speaker 1>it looks like these two clouds mostly passed right through

0:34:18.760 --> 0:34:21.840
<v Speaker 1>each other. So not it doesn't have any strong interactions

0:34:21.840 --> 0:34:24.200
<v Speaker 1>with itself, but it could still have some interactions with itself,

0:34:24.239 --> 0:34:27.200
<v Speaker 1>which would maybe give rise to something like a dark photon.

0:34:27.360 --> 0:34:30.000
<v Speaker 1>That's right, and so people often cite the bullet cluster

0:34:30.080 --> 0:34:32.760
<v Speaker 1>is evidence that dark matter can't feel anything with itself,

0:34:32.840 --> 0:34:35.600
<v Speaker 1>and that's not exactly true, because, as you say, there's

0:34:35.600 --> 0:34:38.240
<v Speaker 1>still room in there for some kind of interaction. Because

0:34:38.320 --> 0:34:41.640
<v Speaker 1>remember that the stars, which do definitely feel each other,

0:34:41.800 --> 0:34:45.040
<v Speaker 1>also passed right through themselves. Right. The star is hardly collided,

0:34:45.280 --> 0:34:47.960
<v Speaker 1>and that's just because it's pretty sparse, and so could

0:34:48.000 --> 0:34:50.719
<v Speaker 1>be that dark matter forms the structures, but they didn't

0:34:50.719 --> 0:34:53.439
<v Speaker 1>collide with each other because just like the stars, they're

0:34:53.480 --> 0:34:56.160
<v Speaker 1>pretty sparse and space is pretty big. And it could

0:34:56.200 --> 0:34:58.919
<v Speaker 1>also be that some components of the dark matter did

0:34:58.960 --> 0:35:01.600
<v Speaker 1>collide with itself, did get stuck sort of in the

0:35:01.600 --> 0:35:04.080
<v Speaker 1>middle there. But we don't really have the resolution to tell.

0:35:04.160 --> 0:35:07.600
<v Speaker 1>We can't very precisely measure how much dark matter passed

0:35:07.600 --> 0:35:09.640
<v Speaker 1>through and how much stuck. We can just tell that

0:35:09.680 --> 0:35:12.600
<v Speaker 1>a lot of it passed through, but some component could

0:35:12.600 --> 0:35:14.920
<v Speaker 1>have gotten stuck and could be doing like crazy stuff

0:35:14.920 --> 0:35:17.000
<v Speaker 1>there in the middle. I see, like maybe the Rubert

0:35:17.040 --> 0:35:19.279
<v Speaker 1>duckies didn't all crash into each other, but some just

0:35:19.360 --> 0:35:22.040
<v Speaker 1>kept going. I think the key point to understand is

0:35:22.040 --> 0:35:25.080
<v Speaker 1>that there's so much dark matter out there that even

0:35:25.080 --> 0:35:27.680
<v Speaker 1>if a tiny fraction of it is doing interesting things

0:35:28.000 --> 0:35:30.520
<v Speaker 1>we couldn't tell, and that tiny fraction would still be

0:35:30.560 --> 0:35:32.960
<v Speaker 1>more stuff than all of the stars and gas and

0:35:33.040 --> 0:35:34.920
<v Speaker 1>dust in the universe that we know. All right, well,

0:35:35.000 --> 0:35:36.680
<v Speaker 1>let's get into other ways that we might be able

0:35:36.719 --> 0:35:39.839
<v Speaker 1>to detect this dark radiation and maybe even see these

0:35:39.920 --> 0:35:42.319
<v Speaker 1>dark or not see these dark photons. I'm a little

0:35:42.320 --> 0:35:44.960
<v Speaker 1>confused about how he might see are not photon But

0:35:45.000 --> 0:35:59.799
<v Speaker 1>first let's take another quick break. All right, we're talking

0:35:59.800 --> 0:36:03.560
<v Speaker 1>abot dark gradiation and dark photons, which it might be

0:36:03.680 --> 0:36:06.560
<v Speaker 1>what dark matter sees and feels with itself when dark

0:36:06.600 --> 0:36:08.319
<v Speaker 1>matter looks in the mirror. That's what they would see

0:36:08.400 --> 0:36:12.440
<v Speaker 1>dark photons. Yeah, exactly. I hope they haven't eating too

0:36:12.480 --> 0:36:15.000
<v Speaker 1>much dark chocolate. But to us it's pretty elusive because

0:36:15.000 --> 0:36:18.279
<v Speaker 1>we can see or feel the dark matter or maybe

0:36:18.320 --> 0:36:20.719
<v Speaker 1>even these forces. So, Daniel, what are some of the

0:36:20.760 --> 0:36:23.360
<v Speaker 1>other ways that we might hope to detect whether or

0:36:23.360 --> 0:36:26.200
<v Speaker 1>not dark matter has these dark interactions. There are a

0:36:26.320 --> 0:36:30.360
<v Speaker 1>couple other indirect ways, basically again using gravity. One of

0:36:30.360 --> 0:36:34.360
<v Speaker 1>them is looking at neutron stars. Neutron stars are these

0:36:34.440 --> 0:36:37.880
<v Speaker 1>crazy dense objects that are the remnants of stars that

0:36:37.920 --> 0:36:40.640
<v Speaker 1>have blown up and left this very very compact core,

0:36:41.200 --> 0:36:44.399
<v Speaker 1>and sometimes neutron stars come in pairs and then those

0:36:44.440 --> 0:36:47.279
<v Speaker 1>pairs spin around each other in this sort of like

0:36:47.360 --> 0:36:50.400
<v Speaker 1>death spiral before they collide, and when they do that,

0:36:50.440 --> 0:36:53.839
<v Speaker 1>they create gravitational waves that we can see here from Earth.

0:36:53.880 --> 0:36:57.239
<v Speaker 1>This is like the shaking of space itself. If you're

0:36:57.520 --> 0:36:59.200
<v Speaker 1>interested in learning more about that, we have a couple

0:36:59.200 --> 0:37:02.239
<v Speaker 1>of episodes about gravitational waves. It's really cool because the

0:37:02.280 --> 0:37:06.360
<v Speaker 1>gravitational waves reveal in detail how these stars are spiraling

0:37:06.480 --> 0:37:09.560
<v Speaker 1>towards the center, how they're losing energy, and we can

0:37:09.560 --> 0:37:12.520
<v Speaker 1>calculate with great precision how fast they should be going

0:37:12.560 --> 0:37:14.960
<v Speaker 1>and how much energy they're losing. And so this is

0:37:14.960 --> 0:37:17.120
<v Speaker 1>a really nice test of sort of like what's going

0:37:17.200 --> 0:37:19.840
<v Speaker 1>on with this kind of matter, Because if these neutron

0:37:19.960 --> 0:37:24.080
<v Speaker 1>stars were capable, for example, of feeling this dark radiation

0:37:24.200 --> 0:37:27.320
<v Speaker 1>at some level, if the particles in there could feel

0:37:27.320 --> 0:37:29.839
<v Speaker 1>this force at all, then they would radiate a little

0:37:29.840 --> 0:37:32.400
<v Speaker 1>bit of those dark photons and it would change the

0:37:32.440 --> 0:37:34.920
<v Speaker 1>way this inspiral happens, and we would be able to

0:37:34.920 --> 0:37:37.880
<v Speaker 1>see that by looking at the gravitational waves. Wait, so

0:37:38.000 --> 0:37:40.439
<v Speaker 1>these neutron stars would be made out of regular matter,

0:37:40.560 --> 0:37:42.160
<v Speaker 1>the kind we're made out of. But you're saying that

0:37:42.200 --> 0:37:45.240
<v Speaker 1>even though the regular matter it might admit this dark radiation,

0:37:45.560 --> 0:37:48.200
<v Speaker 1>how is that possible. It might be that our matter

0:37:48.480 --> 0:37:50.920
<v Speaker 1>can feel these sort of like new forces, just at

0:37:50.960 --> 0:37:53.440
<v Speaker 1>a very very low level. We don't know, and so

0:37:53.520 --> 0:37:55.480
<v Speaker 1>this is like, you know, one way to look for

0:37:55.560 --> 0:37:57.840
<v Speaker 1>it under the assumption that our kind of matter could

0:37:57.880 --> 0:38:00.239
<v Speaker 1>feel these dark forces, which is not something we know.

0:38:00.280 --> 0:38:02.000
<v Speaker 1>It's just sort of like a guess. We do this

0:38:02.080 --> 0:38:04.279
<v Speaker 1>in physics a lot. We're like, we don't know if

0:38:04.280 --> 0:38:06.479
<v Speaker 1>it's possible to see it this way, but let's check,

0:38:06.600 --> 0:38:09.360
<v Speaker 1>because if it does feel this force, if neutron stars

0:38:09.440 --> 0:38:12.239
<v Speaker 1>can make these dark photons, we would be able to

0:38:12.280 --> 0:38:15.160
<v Speaker 1>see that. I see neutron stars are so it's such

0:38:15.200 --> 0:38:17.320
<v Speaker 1>an extreme event when they crash into each other that

0:38:17.320 --> 0:38:21.120
<v Speaker 1>that's one possible, you know, crazy scenario where it might

0:38:21.200 --> 0:38:23.440
<v Speaker 1>make dark gradiations exactly. And it's a place where we

0:38:23.440 --> 0:38:26.920
<v Speaker 1>can make very very precise calculations about the gravitational waves

0:38:26.920 --> 0:38:29.960
<v Speaker 1>and compare them to very very detailed data. So it's

0:38:29.960 --> 0:38:33.200
<v Speaker 1>an opportunity to look for like very small deviations, you know,

0:38:33.320 --> 0:38:35.320
<v Speaker 1>things that the neutron stars are doing that we can't

0:38:35.360 --> 0:38:40.399
<v Speaker 1>otherwise explain that might be explainable through dark photons. I see,

0:38:40.480 --> 0:38:42.440
<v Speaker 1>all right, what are some other ways we could maybe

0:38:42.520 --> 0:38:45.160
<v Speaker 1>feel this dark force? All the most generic ways you

0:38:45.320 --> 0:38:47.800
<v Speaker 1>just use gravity the kind of tests that we did before,

0:38:47.960 --> 0:38:49.680
<v Speaker 1>But there are some other approaches to look for these

0:38:49.719 --> 0:38:53.160
<v Speaker 1>dark photons, hoping that there's some connection between our kind

0:38:53.160 --> 0:38:56.120
<v Speaker 1>of matter and the dark matter, Like hoping that somehow

0:38:56.200 --> 0:39:00.680
<v Speaker 1>maybe these dark photons can turn into normal photon very

0:39:00.800 --> 0:39:04.120
<v Speaker 1>very rarely, and then we could detect that what how

0:39:04.120 --> 0:39:06.600
<v Speaker 1>can a dark photon turn into a regular photon. It

0:39:06.640 --> 0:39:09.000
<v Speaker 1>turns out that if you have another kind of force

0:39:09.040 --> 0:39:11.319
<v Speaker 1>that's very similar to the photon, has sort of like

0:39:11.480 --> 0:39:15.560
<v Speaker 1>a similar mathematical structure, that these forces like to talk

0:39:15.600 --> 0:39:17.960
<v Speaker 1>to each other, that there's like it's very easy to

0:39:18.000 --> 0:39:20.960
<v Speaker 1>build a physics model in which another kind of photon

0:39:21.120 --> 0:39:25.640
<v Speaker 1>can turn into our photon wha like spontaneously or only

0:39:25.680 --> 0:39:29.040
<v Speaker 1>in like high energy completions or you know, moments where

0:39:29.040 --> 0:39:32.240
<v Speaker 1>you have kind of this a state of pure energy.

0:39:32.320 --> 0:39:34.799
<v Speaker 1>It would be spontaneous, and in order for that to happen,

0:39:34.840 --> 0:39:37.160
<v Speaker 1>they would have to be some kind of particle in

0:39:37.200 --> 0:39:41.280
<v Speaker 1>the universe that has both kinds of charges. So imagine

0:39:41.360 --> 0:39:44.839
<v Speaker 1>some new kind, very very rare dark matter that does

0:39:44.960 --> 0:39:48.160
<v Speaker 1>have electric charges and also has some new kind of

0:39:48.280 --> 0:39:51.839
<v Speaker 1>dark electric charge. That particle could effectively be like a

0:39:51.880 --> 0:39:56.040
<v Speaker 1>portal that connects our photons to these other photons, and

0:39:56.080 --> 0:39:58.759
<v Speaker 1>it might be that these particles never really exist in

0:39:58.800 --> 0:40:01.960
<v Speaker 1>the universe, the way like top corks almost never exist

0:40:02.000 --> 0:40:04.400
<v Speaker 1>in the universe on their own, but they're sort of

0:40:04.440 --> 0:40:07.000
<v Speaker 1>like on the list of possibilities. As long as it's

0:40:07.000 --> 0:40:10.759
<v Speaker 1>on the list of possibilities, then dark photons can use

0:40:10.800 --> 0:40:14.640
<v Speaker 1>that as a portal to become normal photons and vice versa.

0:40:14.760 --> 0:40:18.160
<v Speaker 1>This allows them to spontaneously turn from one into the other. Whoa,

0:40:18.320 --> 0:40:21.680
<v Speaker 1>So that wouldn't make dark matter not dark, right, It

0:40:21.680 --> 0:40:23.680
<v Speaker 1>would mean that you can sort of see them. It would,

0:40:23.680 --> 0:40:25.920
<v Speaker 1>but these particles again wouldn't actually have to exist in

0:40:25.960 --> 0:40:29.279
<v Speaker 1>the universe. So imagine now the dark sector is some

0:40:29.360 --> 0:40:31.840
<v Speaker 1>kind of particle that's actually out there, that most of

0:40:31.840 --> 0:40:33.920
<v Speaker 1>the dark matter is made out of this particle. And

0:40:33.960 --> 0:40:37.040
<v Speaker 1>then there's the possibility for this other particle that has

0:40:37.160 --> 0:40:40.239
<v Speaker 1>electric charges and dark charges, even though it's never really

0:40:40.239 --> 0:40:43.080
<v Speaker 1>out there in the universe, as long as the possibility

0:40:43.200 --> 0:40:46.360
<v Speaker 1>for it to exist is part of sort of nature's menu.

0:40:47.000 --> 0:40:50.879
<v Speaker 1>That possibility allows dark photons to turn into photons. It's

0:40:50.880 --> 0:40:54.759
<v Speaker 1>called kinetic mixing because we see it happening with regular matter, right,

0:40:54.840 --> 0:40:57.520
<v Speaker 1>Like our photons turned into other kinds of stuff all

0:40:57.560 --> 0:41:00.400
<v Speaker 1>the time, yes, exactly, Like photons turned into pairs of

0:41:00.480 --> 0:41:04.239
<v Speaker 1>particles electrons and positrons, and then those can turn into

0:41:04.320 --> 0:41:08.680
<v Speaker 1>z bosons, right because z's also interact with electrons impositron.

0:41:08.800 --> 0:41:11.520
<v Speaker 1>So even if there weren't a single electron or positron

0:41:11.560 --> 0:41:14.239
<v Speaker 1>in the universe, a photon could still turn into a

0:41:14.320 --> 0:41:17.080
<v Speaker 1>z boson. And in the same way, as long as

0:41:17.120 --> 0:41:20.319
<v Speaker 1>there's the possibility for some virtual particle that connects these

0:41:20.320 --> 0:41:23.480
<v Speaker 1>two forces to exist, then photons could turn into dark

0:41:23.480 --> 0:41:26.840
<v Speaker 1>photons and vice versa. And that's kind of our only

0:41:26.880 --> 0:41:29.799
<v Speaker 1>hope of seeing this dark force directly. That's the best

0:41:29.840 --> 0:41:32.960
<v Speaker 1>way to see these dark forces directly, exactly, And so

0:41:33.080 --> 0:41:35.440
<v Speaker 1>people have built really cool experiments to try to like

0:41:35.880 --> 0:41:38.560
<v Speaker 1>make this happen more often, try to like create the

0:41:38.640 --> 0:41:43.319
<v Speaker 1>scenarios that would help induce dark photons to spontaneously turn

0:41:43.400 --> 0:41:47.040
<v Speaker 1>into photons. They have these resonant cavities at Fermilab, for example,

0:41:47.160 --> 0:41:50.000
<v Speaker 1>that should enhance the rate of this happening. If you

0:41:50.120 --> 0:41:52.719
<v Speaker 1>like build something with the right shape and size, it

0:41:52.760 --> 0:41:56.319
<v Speaker 1>creates a situation where this kind of spontaneous transformation is

0:41:56.320 --> 0:41:58.759
<v Speaker 1>more likely to happen. And so they look for this

0:41:58.880 --> 0:42:02.360
<v Speaker 1>kind of signature. Wait, that's being built right now, Like

0:42:02.400 --> 0:42:06.480
<v Speaker 1>there are people building basically dark forest boxes. These things

0:42:06.520 --> 0:42:09.360
<v Speaker 1>exist already and they are being run and they're just

0:42:09.400 --> 0:42:11.080
<v Speaker 1>building them bigger and bigger. It's sort of like the

0:42:11.080 --> 0:42:13.000
<v Speaker 1>way people are looking for a dark matter. They look

0:42:13.040 --> 0:42:15.480
<v Speaker 1>in these containers underground, and they started with small ones,

0:42:15.480 --> 0:42:17.480
<v Speaker 1>and then they're making bigger and bigger and bigger ones.

0:42:17.719 --> 0:42:20.359
<v Speaker 1>Nobody's seeing a dark photon yet, but they're hoping as

0:42:20.360 --> 0:42:23.760
<v Speaker 1>they make these cavities more precise and larger to induce

0:42:23.800 --> 0:42:27.200
<v Speaker 1>a dark photon to turn into a normal photon. Cool,

0:42:27.360 --> 0:42:29.160
<v Speaker 1>and how else can you look for these? Another way

0:42:29.160 --> 0:42:32.000
<v Speaker 1>to look for these is to look for particles appearing

0:42:32.040 --> 0:42:34.480
<v Speaker 1>where they shouldn't be. So one of my favorite kind

0:42:34.480 --> 0:42:37.520
<v Speaker 1>of experiments, it's called a beam dump experiment, where you

0:42:37.560 --> 0:42:39.479
<v Speaker 1>take a particle beam you were using for something else

0:42:39.520 --> 0:42:41.480
<v Speaker 1>and you dump it, meaning you just like shoot it

0:42:41.480 --> 0:42:45.000
<v Speaker 1>into a huge block of concrete or into a mountain side,

0:42:45.280 --> 0:42:47.000
<v Speaker 1>just because you know, it's got to go somewhere. You

0:42:47.000 --> 0:42:50.080
<v Speaker 1>don't want to like sprayed over the neighborhood because it's dangerous, right,

0:42:50.120 --> 0:42:51.840
<v Speaker 1>just shoot it through the earth at people on the

0:42:51.880 --> 0:42:54.120
<v Speaker 1>other side of the earth. Is that what you're saying, Yeah, exactly.

0:42:54.520 --> 0:42:56.319
<v Speaker 1>And so Sho didn't do a mountain. It was on

0:42:56.360 --> 0:42:59.799
<v Speaker 1>the other side of Daniel. It's not California, is I'm

0:43:00.000 --> 0:43:02.480
<v Speaker 1>to have to look that up. But if you shoot

0:43:02.520 --> 0:43:05.239
<v Speaker 1>this particle beam into a mountain, for example, and then

0:43:05.280 --> 0:43:08.200
<v Speaker 1>you put a particle detector on the other side of

0:43:08.280 --> 0:43:10.919
<v Speaker 1>the mountain, none of the particles should make it through

0:43:10.920 --> 0:43:14.319
<v Speaker 1>the mountain, but you might see particles appearing in your

0:43:14.360 --> 0:43:16.920
<v Speaker 1>detector on the other side of the mountain, because dark

0:43:17.000 --> 0:43:19.960
<v Speaker 1>photons might make it through the mountain because they basically

0:43:20.000 --> 0:43:22.600
<v Speaker 1>see the mountain is invisible as transparent. The ideas if

0:43:22.640 --> 0:43:27.600
<v Speaker 1>your beam sometimes occasionally produces dark photons, those dark photons

0:43:27.600 --> 0:43:30.359
<v Speaker 1>would make it through the mountain. And so essentially it's

0:43:30.480 --> 0:43:33.520
<v Speaker 1>like looking for light shining through walls or I see

0:43:33.520 --> 0:43:35.359
<v Speaker 1>so many the ideas that you send this beam out

0:43:35.360 --> 0:43:38.520
<v Speaker 1>into the mountain, some of it turns into dark photons,

0:43:38.760 --> 0:43:42.040
<v Speaker 1>and then somehow it turns back into regular photons before

0:43:42.080 --> 0:43:44.640
<v Speaker 1>it hits your detector. Yeah, that's exactly right. And so

0:43:44.800 --> 0:43:48.399
<v Speaker 1>you're hoping that sometimes those dark photons turned back into

0:43:48.440 --> 0:43:51.040
<v Speaker 1>normal photons. So you're assuming a lot of things here.

0:43:51.080 --> 0:43:54.319
<v Speaker 1>You're assuming that maybe sometimes dark photons are created in

0:43:54.320 --> 0:43:57.640
<v Speaker 1>your beam, and that sometimes they turn back into normal photons. Right,

0:43:57.640 --> 0:43:59.799
<v Speaker 1>But if they turn back into regular photons, how would

0:43:59.840 --> 0:44:02.120
<v Speaker 1>you know they turned into dark photons in the middle. Yeah,

0:44:02.160 --> 0:44:04.160
<v Speaker 1>you wouldn't know for sure. You would just know that

0:44:04.440 --> 0:44:07.680
<v Speaker 1>something passed through the mountain that typically shouldn't be able to.

0:44:07.920 --> 0:44:10.839
<v Speaker 1>So you calculate, like how often should particles be able

0:44:10.840 --> 0:44:14.399
<v Speaker 1>to pass through the mountain and turn into photons? And

0:44:14.520 --> 0:44:17.319
<v Speaker 1>if that happens more often than you expect, then you

0:44:17.320 --> 0:44:20.040
<v Speaker 1>know there's something else and new there, maybe a dark photon,

0:44:20.120 --> 0:44:22.399
<v Speaker 1>maybe something else. But you know, that's often the case

0:44:22.440 --> 0:44:25.680
<v Speaker 1>with particle physics. We find something new, we're not exactly

0:44:25.719 --> 0:44:28.480
<v Speaker 1>sure what it is, and then we study it in detail,

0:44:28.520 --> 0:44:30.839
<v Speaker 1>we try to characterize exactly what it is, just like

0:44:31.040 --> 0:44:33.719
<v Speaker 1>with the Higgs boson. First thing, we saw some new

0:44:33.760 --> 0:44:36.960
<v Speaker 1>particle decaying into two photons, and we weren't sure is

0:44:37.000 --> 0:44:38.759
<v Speaker 1>this the Higgs boson or is it something else? We

0:44:38.760 --> 0:44:41.200
<v Speaker 1>didn't expect, and over decades of study we sort of

0:44:41.239 --> 0:44:43.160
<v Speaker 1>pinned down what it must be because of all of

0:44:43.200 --> 0:44:45.880
<v Speaker 1>its behaviors. I see, it's like, the only way it

0:44:45.880 --> 0:44:48.839
<v Speaker 1>could have made it through the mountain to and out

0:44:48.880 --> 0:44:51.760
<v Speaker 1>into California to hit us it was if it turned

0:44:51.760 --> 0:44:56.520
<v Speaker 1>into something invisible like dark photons somewhere in the middle.

0:44:56.760 --> 0:44:58.719
<v Speaker 1>Otherwise it wouldn't have made it through. Exactly, I have

0:44:58.840 --> 0:45:01.120
<v Speaker 1>to phase through the mountain by turning into something that

0:45:01.160 --> 0:45:04.040
<v Speaker 1>doesn't interact with mountains. All right, cool, Well, what are

0:45:04.120 --> 0:45:05.800
<v Speaker 1>some other ways we might be able to see these

0:45:05.880 --> 0:45:08.400
<v Speaker 1>dark forces? A lot of the other experiments are very similar.

0:45:08.680 --> 0:45:13.279
<v Speaker 1>There's one at CERN called Phaser Forward Search Experiment. It's

0:45:13.320 --> 0:45:16.520
<v Speaker 1>a pretty tortured acronym, but a really cool idea for

0:45:17.480 --> 0:45:19.720
<v Speaker 1>I don't even know what is there an A actually

0:45:19.760 --> 0:45:23.080
<v Speaker 1>in the name, there's an A and forward and an

0:45:23.239 --> 0:45:27.760
<v Speaker 1>R experiment. Oh man, it's a really cool idea because

0:45:27.800 --> 0:45:31.400
<v Speaker 1>they're taking an already existing experiment Atlas where we collide

0:45:31.400 --> 0:45:35.040
<v Speaker 1>protons together and they're wondering like maybe dark photons are

0:45:35.040 --> 0:45:37.680
<v Speaker 1>created and shoot down the beam. So they built a

0:45:37.719 --> 0:45:41.160
<v Speaker 1>detector like really far down along the beam past where

0:45:41.160 --> 0:45:44.000
<v Speaker 1>the collisions happen to see if maybe dark photons are

0:45:44.040 --> 0:45:47.040
<v Speaker 1>created in those collisions and then fly along the beam

0:45:47.160 --> 0:45:49.680
<v Speaker 1>and then turn into something that they can see sort

0:45:49.680 --> 0:45:53.319
<v Speaker 1>of downstream. So they added this little bit to the

0:45:53.360 --> 0:45:55.960
<v Speaker 1>detector that can do something totally novel and new. It's

0:45:55.960 --> 0:45:58.240
<v Speaker 1>actually led by a team here at you see Irvine,

0:45:58.360 --> 0:46:00.480
<v Speaker 1>m M, I see. But we don't actually know if

0:46:00.560 --> 0:46:03.440
<v Speaker 1>dark matter can switch back and forth that easily, right,

0:46:03.640 --> 0:46:05.640
<v Speaker 1>We don't know. And again, it could be that dark

0:46:05.640 --> 0:46:09.160
<v Speaker 1>matter is only some inert particle that feels gravity and

0:46:09.200 --> 0:46:11.319
<v Speaker 1>nothing else and there are no dark forces and no

0:46:11.440 --> 0:46:14.360
<v Speaker 1>way to interact. It could also be that dark matter

0:46:14.480 --> 0:46:17.640
<v Speaker 1>does feel some new dark force, but can only interact

0:46:17.680 --> 0:46:20.359
<v Speaker 1>with itself, and none of those dark forces can ever

0:46:20.520 --> 0:46:24.480
<v Speaker 1>turn into normal matter or normal photons. Here, we're just guessing.

0:46:24.480 --> 0:46:27.640
<v Speaker 1>We're trying to like study the various possibilities in the

0:46:27.719 --> 0:46:32.080
<v Speaker 1>various ways that those possibilities might manifesto well, And so

0:46:32.160 --> 0:46:33.960
<v Speaker 1>what does it all mean? Do you think we will

0:46:34.000 --> 0:46:37.399
<v Speaker 1>find it has interactions with itself or do you think

0:46:37.440 --> 0:46:40.279
<v Speaker 1>it just represents this whole part of the universe that

0:46:40.320 --> 0:46:42.759
<v Speaker 1>we will never be able to see or touch or

0:46:42.800 --> 0:46:45.319
<v Speaker 1>even confirm that it's there. You know, like we could

0:46:45.320 --> 0:46:50.120
<v Speaker 1>be swimming in dark rubber duckies and never ever ever, Yeah,

0:46:50.239 --> 0:46:52.120
<v Speaker 1>part of it comes down to what you think is

0:46:52.160 --> 0:46:54.440
<v Speaker 1>more natural. Does it make sense to you to have

0:46:54.560 --> 0:46:57.920
<v Speaker 1>a huge component of the universe be sort of simple

0:46:58.160 --> 0:47:00.960
<v Speaker 1>and inert and not really doing any being interesting, or

0:47:01.000 --> 0:47:03.680
<v Speaker 1>does this seem more natural for it to be complex

0:47:03.680 --> 0:47:06.680
<v Speaker 1>and interactive the way that our matter is. Now, what

0:47:06.800 --> 0:47:09.239
<v Speaker 1>I know is that the universe doesn't follow what we

0:47:09.360 --> 0:47:12.600
<v Speaker 1>think is natural. Our conceptions of how the universe should

0:47:12.640 --> 0:47:14.680
<v Speaker 1>work don't seem to be very well aligned with how

0:47:14.719 --> 0:47:17.440
<v Speaker 1>it usually does work, and so I suspect there are

0:47:17.480 --> 0:47:19.880
<v Speaker 1>some surprises out there. The other side of that question

0:47:19.960 --> 0:47:22.120
<v Speaker 1>is what you asked, is might we ever be able

0:47:22.160 --> 0:47:24.160
<v Speaker 1>to tell? And it could be that dark matter doesn't

0:47:24.160 --> 0:47:26.240
<v Speaker 1>feel any of our forces, and none of these forces

0:47:26.239 --> 0:47:28.560
<v Speaker 1>can talk to our forces, and we can never find

0:47:28.719 --> 0:47:31.840
<v Speaker 1>these dark rubber duckies. But I have faith in physicists

0:47:31.880 --> 0:47:34.640
<v Speaker 1>and engineers to come up with clever ways to probe

0:47:34.680 --> 0:47:37.799
<v Speaker 1>these things, ways that we can't even today. Imagine kinds

0:47:37.840 --> 0:47:40.439
<v Speaker 1>of experiments that people might think of in ten years

0:47:40.520 --> 0:47:43.200
<v Speaker 1>or twenty years, experiments thought up by you know, clever

0:47:43.320 --> 0:47:46.560
<v Speaker 1>Listeners to this podcast who aren't constrained by the kind

0:47:46.560 --> 0:47:49.359
<v Speaker 1>of thinking that academic physicists have been trained to do.

0:47:49.560 --> 0:47:51.120
<v Speaker 1>I think I know how you can do it, Daniel,

0:47:51.239 --> 0:47:54.960
<v Speaker 1>Dark Chocolate collisions. You just gotta want it enough. You know,

0:47:55.320 --> 0:47:58.360
<v Speaker 1>you have to really want it, because, as Yoda says,

0:47:58.400 --> 0:48:01.960
<v Speaker 1>you know, wanting these to pain and pain needs to suffering,

0:48:02.680 --> 0:48:05.359
<v Speaker 1>and suffering leads to the dark side, and so that's

0:48:05.360 --> 0:48:07.560
<v Speaker 1>that's how you can get there faster. Maybe, Yeah, there

0:48:07.640 --> 0:48:09.640
<v Speaker 1>is no try. I should just do it, that's right,

0:48:09.719 --> 0:48:15.120
<v Speaker 1>Just I mean, do it? You should, yes, all right.

0:48:15.160 --> 0:48:16.439
<v Speaker 1>I don't know why I didn't think of that before.

0:48:16.480 --> 0:48:18.040
<v Speaker 1>I'm just gonna go do it right after we're done

0:48:18.080 --> 0:48:20.239
<v Speaker 1>with this podcast, or not do it. I guess we're

0:48:20.239 --> 0:48:23.040
<v Speaker 1>doing in the dark. Gosh, I'm so confused. But to me,

0:48:23.080 --> 0:48:25.840
<v Speaker 1>it really touches on these deep mysteries of physics that

0:48:25.960 --> 0:48:28.520
<v Speaker 1>we know the universe out there is telling stories that

0:48:28.560 --> 0:48:31.200
<v Speaker 1>we haven't heard yet. We're desperate to hear those stories.

0:48:31.480 --> 0:48:33.760
<v Speaker 1>We have hints that we know the shape of those stories,

0:48:33.760 --> 0:48:35.759
<v Speaker 1>but we don't know any of the details yet, and

0:48:35.840 --> 0:48:37.480
<v Speaker 1>I just hope that one day we'll be able to

0:48:37.520 --> 0:48:39.839
<v Speaker 1>fill those in. Yeah, it's almost like there's a whole

0:48:39.960 --> 0:48:42.440
<v Speaker 1>universe out there, sitting right in front of us that

0:48:42.520 --> 0:48:45.480
<v Speaker 1>we have yet to discover, and that anyone listening to

0:48:45.520 --> 0:48:47.840
<v Speaker 1>this could become part of that search. That's right. So

0:48:47.880 --> 0:48:50.560
<v Speaker 1>there's plenty more of the universe to find out, and

0:48:50.560 --> 0:48:54.120
<v Speaker 1>we desperately need new ideas. And whether the universe counts

0:48:54.120 --> 0:48:56.960
<v Speaker 1>as dark chocolate or not, that's for other people to debate.

0:48:57.719 --> 0:49:00.440
<v Speaker 1>That's right. And if you love white chocolate, take my apologies.

0:49:00.480 --> 0:49:03.440
<v Speaker 1>I love all of them. You love listeners more than

0:49:03.480 --> 0:49:07.239
<v Speaker 1>you love your chocolate, exactly, And if you eat white

0:49:07.280 --> 0:49:11.000
<v Speaker 1>chocolate while listen to this podcast, I forgive you because

0:49:11.120 --> 0:49:13.440
<v Speaker 1>he can't see your or feel you, so it doesn't

0:49:13.440 --> 0:49:17.799
<v Speaker 1>matter to exactly. Please accept my dark apologies. All right, Well,

0:49:17.840 --> 0:49:20.239
<v Speaker 1>we hope you enjoyed that. Thanks for joining us, See

0:49:20.239 --> 0:49:30.680
<v Speaker 1>you next time. Thanks for listening, and remember that Daniel

0:49:30.719 --> 0:49:33.239
<v Speaker 1>and Jorge Explain the Universe is a production of I

0:49:33.480 --> 0:49:36.919
<v Speaker 1>Heart Radio. For more podcast for my heart Radio, visit

0:49:36.920 --> 0:49:40.440
<v Speaker 1>the I heart Radio app, Apple Podcasts, or wherever you

0:49:40.520 --> 0:49:47.799
<v Speaker 1>listen to your favorite shows. Yeah,