WEBVTT - Does the Universe need dark matter?

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<v Speaker 1>Hey, Daniel, do you ever wonder if physics might be

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<v Speaker 1>like really wrong? Are you talking about me or like

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<v Speaker 1>the entire community? Well, I know you're never wrong, Daniel,

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<v Speaker 1>that's unthinkable, but you know, like, has physics ever gotten

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<v Speaker 1>something about the very nature of the universe? Kind of? Uh?

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<v Speaker 1>Not right? You mean, like what's the best snack food?

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<v Speaker 1>Or what colored lab coat should we wear? Hey? Yeah,

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<v Speaker 1>you know, like can I eat antimatter or not? Maybe

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<v Speaker 1>it's delicious. Physics could definitely be wrong about snacks for you. Well,

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<v Speaker 1>I mean think bigger, like, is it possible that maybe

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<v Speaker 1>things are not quite what they seem? Well, it wouldn't

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<v Speaker 1>be the first time physics is wrong, and I hope

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<v Speaker 1>it's not the last time. I am organ made cartoonists

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<v Speaker 1>and the creator of PhD comments, Hi, I'm Daniel. I'm

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<v Speaker 1>a particle physicist, and I've never been wrong about snack foods,

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<v Speaker 1>and I've never been wrong about being wrong. So I

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<v Speaker 1>think that means that I'm always wrong. I don't know,

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<v Speaker 1>but welcome to our podcast. I'm definitely right about that.

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<v Speaker 1>This is our podcast, Daniel and Jorge Explain the Universe,

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<v Speaker 1>a production of I Heart Radio. That's right. Our podcast

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<v Speaker 1>in which we take a mental tour of all the

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<v Speaker 1>crazy stuff that's out there in the universe and try

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<v Speaker 1>to bring it into your head. We try to wrap

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<v Speaker 1>up the entire universe, all those trillions and trillions of

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<v Speaker 1>stars and weird blobs of gas and dust and invisible stuff,

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<v Speaker 1>and inserted through a little hole in your ear into

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<v Speaker 1>your brain. Yeah, all of the amazing and incredible stuff

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<v Speaker 1>out there in the universe, and also all of the

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<v Speaker 1>stuff that's normal. You know, And sometimes I think when

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<v Speaker 1>you examine what's spears to be normal in your everyday lives,

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<v Speaker 1>it turns out to have all kinds of wonders and

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<v Speaker 1>all kinds of small miracles in it. Are there small

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<v Speaker 1>miracles in your snack foods? Is that what you're talking about? Like, Oh,

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<v Speaker 1>look this chocolate chips in this trail mix. Every snack

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<v Speaker 1>is a miracle, Daniel, especially banana's net. But in this podcast,

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<v Speaker 1>we go beyond the miracles of banana based snack foods

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<v Speaker 1>and talk about the incredible things that scientists are trying

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<v Speaker 1>to figure out, Because, contrary to popular perception, scientists don't

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<v Speaker 1>have it all figured out. There are lots of really

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<v Speaker 1>big mysteries out there and wondering about the universe is

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<v Speaker 1>something that belongs to everybody, including you. Yeah, so they're

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<v Speaker 1>one of the biggest mysteries out there in the universe,

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<v Speaker 1>and literally sort of like not just like because we

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<v Speaker 1>don't know it, but also because it's a huge part

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<v Speaker 1>of the universe. Is dark matter? Dark matter is a

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<v Speaker 1>little bit crazy, right, It's like twenty of the universe,

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<v Speaker 1>but we have no idea what it is. That's right

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<v Speaker 1>of the energy budget of the universe. It's a pretty

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<v Speaker 1>big slice. It's like a little bit more than a

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<v Speaker 1>quarter of all the energy in the universe. Is this

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<v Speaker 1>weird stuff and we've never seen it directly. We're pretty

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<v Speaker 1>sure it's there, but we don't really know what is it.

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<v Speaker 1>Is it made out of particles? Isn't made out of

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<v Speaker 1>black holes? Isn't made out of lost socks? Two really

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<v Speaker 1>huge mystery in modern physics. In fact, I would say

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<v Speaker 1>it's one of the biggest open questions in science. I

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<v Speaker 1>think it's just dark socks actually, but didn't that makes sense?

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<v Speaker 1>I always lose those. How many dark socks have you

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<v Speaker 1>lost for her? I mean we're talking a lot of songs. Well,

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<v Speaker 1>to be out of time a cartoonists I don't have

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<v Speaker 1>to wear dark socks very often or socks at all,

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<v Speaker 1>because I also lived in California. But yeah, dark matter,

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<v Speaker 1>I mean, it's a big deal. There's five times more

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<v Speaker 1>dark matter than there is regular matter, like planets and

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<v Speaker 1>stars and gas and dust and black holes, there's all

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<v Speaker 1>that stuff. There's actually it's only of the stuff in

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<v Speaker 1>the universe, which means the normal matter, the regular matter,

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<v Speaker 1>the stuff that you're familiar with, is not actually regular

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<v Speaker 1>or normal. It's the unusual stuff. If you just took

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<v Speaker 1>like a survey of stuff in the universe, most of

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<v Speaker 1>the stuff is dark matter. The things that make up

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<v Speaker 1>stars and planets and galaxies and hamsters and me and

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<v Speaker 1>you and bananas and snack foods. That's unusual in the universe.

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<v Speaker 1>It's a minority of what's out there in the universe.

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<v Speaker 1>And yet we still don't know what this dark matter is.

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<v Speaker 1>It's a big mystery and a lot of times, you know,

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<v Speaker 1>whenever people talk about dark matter, I feel like a

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<v Speaker 1>common question we get, at least and in talks and

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<v Speaker 1>appearances is that people ask us like what if dark

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<v Speaker 1>matter doesn't exist? Like what if it's just an error

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<v Speaker 1>in the equations that you have about physics and the universe,

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<v Speaker 1>Like what if we just maybe like misunderstood gravity, or

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<v Speaker 1>haven't counted all the stars in the galaxy, or you

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<v Speaker 1>know what if there's something else that is maybe normal

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<v Speaker 1>but we just haven't thought about. And it's a great

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<v Speaker 1>question because most of the evidence we have for dark

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<v Speaker 1>matter is a little bit indirect, like because dark matter

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<v Speaker 1>is so dark and hard to interact with, we don't

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<v Speaker 1>have clear pictures of it, right, we haven't seen what

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<v Speaker 1>it's made out of. We've only sort of seen its

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<v Speaker 1>effects and sometimes second hand, and so it's tempting to

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<v Speaker 1>wonder if it's really there. You know. It's like if

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<v Speaker 1>you've only seen the footprints of an animal, are you

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<v Speaker 1>really sure it exists? Or could it be something else

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<v Speaker 1>spoofing you Until you really capture one or see one

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<v Speaker 1>in the wild, you don't really believe it exists. And

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<v Speaker 1>dark matter has been eluding our searches for decades and

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<v Speaker 1>makes people wonder like, well, maybe you people have it wrong. Yeah,

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<v Speaker 1>I mean it's kind of a crazy idea, right to

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<v Speaker 1>think that there's that much stuff out there, and conveniently

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<v Speaker 1>it's invisible and you can't see it. You know what,

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<v Speaker 1>I mean like I would be like, maybe you should

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<v Speaker 1>take your math or you know, maybe you should have

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<v Speaker 1>another grad student do the calculation. So, which do you

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<v Speaker 1>think is the conspiracy theory dark matter like there's so

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<v Speaker 1>much of it and you can't see it because it's

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<v Speaker 1>so dark and that proves that it exists, or the

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<v Speaker 1>anti dark matter conspiracy theory. Wait, anti dark matter? That's

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<v Speaker 1>another episode right there? Can you have anti dark matter Danny? Yeah,

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<v Speaker 1>that's another great question. We think probably not because then

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<v Speaker 1>they would annihilate a dark matter and turn into photons,

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<v Speaker 1>which we would see, what if it turns into dark photons? Yeah,

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<v Speaker 1>that's actually a thing, dark photon. Really? Yeah, there goes

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<v Speaker 1>my double price. You don't get credit for that one.

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<v Speaker 1>But you know which idea sounds more bonkers, right, that

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<v Speaker 1>the universe has filled with an incredible amount of invisible

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<v Speaker 1>matter nobody had detected until recently, or that it's not. Yeah.

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<v Speaker 1>So today on the podcast, we'll be asking the question

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<v Speaker 1>does the universe need dark matter? Is it an essential

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<v Speaker 1>part of the unit, Like could you have a universe

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<v Speaker 1>without dark manner? Does that make sense? Or is it

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<v Speaker 1>maybe that the universe doesn't need it? And maybe it

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<v Speaker 1>is kind of an error that we have in our

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<v Speaker 1>calculations and observations about the universe. And this kind of

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<v Speaker 1>skepticism is very healthy. When you have a crazy idea

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<v Speaker 1>you're trying to accommodate when you see results in your

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<v Speaker 1>experiments you don't understand. You need to be flexible about

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<v Speaker 1>this sort of theoretical framework with which you come at

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<v Speaker 1>the problem. You need to be open to crazy new ideas,

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<v Speaker 1>but you also need to be open to the fact

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<v Speaker 1>that maybe you got your measurements wrong. There always can

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<v Speaker 1>be an alternative explanation. So before you go big and say, wow,

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<v Speaker 1>we're going to revolutionize our understanding of the universe, you've

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<v Speaker 1>got to rule out all the more prosaic, basic, simpler explanations.

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<v Speaker 1>And so it's always a good idea to keep those

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<v Speaker 1>ideas in mind. YEA, So how sure are we that

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<v Speaker 1>dark matter exists in the universe? And could it be

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<v Speaker 1>something else? So I went out there into the internet

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<v Speaker 1>and I asked people, can we explain what we see

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<v Speaker 1>in the universe without dark matter? Are there good alternative

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<v Speaker 1>theories that don't require a new particle or a new

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<v Speaker 1>blob of stuff. Before you listen to these answers from

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<v Speaker 1>the internet. Think about it for a second. Do you

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<v Speaker 1>think dark matter is necessary in the universe or do

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<v Speaker 1>you think the universe could ignore it or live without it.

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<v Speaker 1>Here's what people had to say. I would think we

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<v Speaker 1>would be much more baffled if we didn't have dark

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<v Speaker 1>matter to explain the expansion of the universe. Oh man,

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<v Speaker 1>And this is tough because I still don't have a

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<v Speaker 1>good handle on what dark matter really is. But I

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<v Speaker 1>think I think we really don't know what dark matter is,

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<v Speaker 1>So I'm going to say, yeah, we could definitely explain

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<v Speaker 1>what we see without it, because we're kind of just

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<v Speaker 1>making up what it is. Yes, dark matter is just

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<v Speaker 1>a made a term for the stuff that's there that

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<v Speaker 1>we can't explain. So truly, any theory is under the

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<v Speaker 1>umbrella of dark matter. I have a strong suspicion that

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<v Speaker 1>the thing could be explained without dark matter, recalled Daniel,

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<v Speaker 1>saying that dark matter is just the name that we've

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<v Speaker 1>come up with for the phenomenon that we can't explain.

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<v Speaker 1>I don't know what we would see without dark matter.

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<v Speaker 1>My understanding is that we do know that there's dark

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<v Speaker 1>matter because the math doesn't work out. At some point,

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<v Speaker 1>we will have to explain the universe without dark matter,

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<v Speaker 1>because like the dark in the matter sort of implies

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<v Speaker 1>that we don't know what it is. I believe that

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<v Speaker 1>dark matter is a theory that we came up with

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<v Speaker 1>to help explain why we couldn't account for all of

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<v Speaker 1>the gravity that we see in the universe. I think

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<v Speaker 1>it's a fairly recent discovery. I don't believe Einstein knew

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<v Speaker 1>about it, so he must have had some other way

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<v Speaker 1>to account for all of the gravity. All Right, some

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<v Speaker 1>pretty good answers there, Yeah. I like the people who

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<v Speaker 1>treat dark matters just sort of like as an umbrella

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<v Speaker 1>idea for all the things we don't understand. And so

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<v Speaker 1>whatever we find out there, we just call that dark matter.

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<v Speaker 1>And I think that really touches on the sense people

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<v Speaker 1>have that we don't really have a clue what's out there.

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<v Speaker 1>We just sort of labeled it dark matter, and we're

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<v Speaker 1>talking about it as if it's a thing, but it's

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<v Speaker 1>really just a name we applied to our cluelessness. Interesting,

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<v Speaker 1>like if you put an S at d end, it

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<v Speaker 1>becomes dark matters, and then then it's sort of like

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<v Speaker 1>an umbrella term for things that are dark. That's true,

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<v Speaker 1>and you know, that is definitely true of dark energy.

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<v Speaker 1>Dark energy is another piece of the universe pie. Right,

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<v Speaker 1>the universe pie is five percent normal matter, twenty dark matter,

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<v Speaker 1>dark energy. Dark energy definitely in the category of just

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<v Speaker 1>stuff we don't understand. We gave a fancy sounding name

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<v Speaker 1>dark energy, this stuff that's making the universe expand right.

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<v Speaker 1>Dark matter, on the other hand, is much better understood,

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<v Speaker 1>is much more concrete and idea much more detailed observation.

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<v Speaker 1>So they're both called dark both things we don't understand.

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<v Speaker 1>But dark energy definitely a label for our cluelessness, while

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<v Speaker 1>dark matter is a much better founded, well described theory.

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<v Speaker 1>It's less dark. I guess we're less in the dark

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<v Speaker 1>about exactly. We are less in the dark. Our minds

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<v Speaker 1>are not quite so filled with dark shadows. All right.

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<v Speaker 1>Well that's the question for today, And that's the question is,

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<v Speaker 1>you know, do we need dark matter, like is it

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<v Speaker 1>a concept that is totally necessary for the universe to

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<v Speaker 1>make sense or is it just something weird that exists

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<v Speaker 1>out there and that maybe we could have a totally

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<v Speaker 1>wrong idea about, you know, And are there other theories

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<v Speaker 1>that are being worked on in the scientific community that

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<v Speaker 1>might explain it without needing to add some new kind

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<v Speaker 1>of stuff to the universe, darker matter, the darkest matter.

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<v Speaker 1>And you'll find that in science there are always competing voices.

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<v Speaker 1>You know, there's often like a mainstream most people think

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<v Speaker 1>the answer is X, but there's always somebody out there

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<v Speaker 1>who thinks it's why, somebody who thinks it's Z. And

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<v Speaker 1>you've got to give these people room because sometimes they're right,

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<v Speaker 1>and sometimes their ideas of the ones that turn into

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<v Speaker 1>the mainstream. That's how the mainstream became mainstream. It used

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<v Speaker 1>to once be lunatic fringe or their alternative physicists, you know,

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<v Speaker 1>French physicists. There definitely are there are people out there,

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<v Speaker 1>once they get tenure, start working on crazy Bonker's theories

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<v Speaker 1>and sometimes for decades that nobody pays attention, nobody really

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<v Speaker 1>reads their papers, that people even laugh behind their hands.

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<v Speaker 1>But sometimes they're right, you know. Literally, the history of

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<v Speaker 1>physics is filled with revolutions that start as crazy ideas,

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<v Speaker 1>and so we definitely got to pour water on some

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<v Speaker 1>of those seedlings because they could sprout into huge new

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<v Speaker 1>intellectual trees, awesome dark physics trees. I'm picturing all right, Well,

0:12:12.440 --> 0:12:15.680
<v Speaker 1>step us through um like what's the main argument for

0:12:15.960 --> 0:12:19.240
<v Speaker 1>dark matter, Like, what's the main evidence about it, and

0:12:19.480 --> 0:12:22.079
<v Speaker 1>what makes this think that, you know, it's something new

0:12:22.160 --> 0:12:24.679
<v Speaker 1>and different as opposed to maybe it's just more stuff

0:12:24.720 --> 0:12:26.240
<v Speaker 1>out there that we can't see. Yes, So if you're

0:12:26.280 --> 0:12:28.480
<v Speaker 1>going to come up with another theory of the universe,

0:12:28.520 --> 0:12:31.720
<v Speaker 1>another way to explain the way the universe works, you

0:12:31.760 --> 0:12:34.439
<v Speaker 1>have to explain what we do see, right, I mean

0:12:34.440 --> 0:12:37.200
<v Speaker 1>that's the whole idea behind making a theory of physics.

0:12:37.679 --> 0:12:39.400
<v Speaker 1>So if you're gonna come up with your theory, you

0:12:39.400 --> 0:12:41.800
<v Speaker 1>have to understand what are the observations, what are the

0:12:41.880 --> 0:12:45.440
<v Speaker 1>experiments reveal that need to be explained that you know,

0:12:45.520 --> 0:12:48.600
<v Speaker 1>what's the motivation for creating this idea of dark matter?

0:12:48.760 --> 0:12:52.120
<v Speaker 1>And the short version is it's all gravity. Like everything

0:12:52.160 --> 0:12:54.400
<v Speaker 1>we see out there in the universe that we need

0:12:54.520 --> 0:12:58.440
<v Speaker 1>dark matter to explain our weird gravitational effects that we

0:12:58.559 --> 0:13:01.880
<v Speaker 1>can't explain with all the other stuff, just the gas

0:13:01.920 --> 0:13:04.520
<v Speaker 1>and the dust and the stars right with the universe

0:13:04.679 --> 0:13:08.240
<v Speaker 1>feels dark matter in terms of gravity, like it's they're

0:13:08.280 --> 0:13:10.920
<v Speaker 1>affecting the gravity of other things, but you can't see it.

0:13:11.000 --> 0:13:14.560
<v Speaker 1>That's the main evidence for it. Yeah, basically there's unexplained gravity,

0:13:14.640 --> 0:13:16.439
<v Speaker 1>like we thought we knew where all the stuff was

0:13:16.480 --> 0:13:18.719
<v Speaker 1>in the universe from the stars and the gas and

0:13:18.760 --> 0:13:21.079
<v Speaker 1>the dust, and from that you can calculate how much

0:13:21.080 --> 0:13:23.880
<v Speaker 1>gravity there should be, and we can see the effects

0:13:23.880 --> 0:13:25.840
<v Speaker 1>of gravity, and will go through in a list of

0:13:25.840 --> 0:13:28.280
<v Speaker 1>how we see the effects of gravity. But there's more

0:13:28.360 --> 0:13:31.920
<v Speaker 1>gravity than we expected. So either there's more stuff e

0:13:32.080 --> 0:13:35.600
<v Speaker 1>dark matter, or gravity is weird and different, and so

0:13:35.640 --> 0:13:38.439
<v Speaker 1>it's all about the gravity then, right, because that's kind

0:13:38.440 --> 0:13:41.120
<v Speaker 1>of at the basis of the theory about dark matter,

0:13:41.200 --> 0:13:43.720
<v Speaker 1>is that it feels gravity but not anything else exactly,

0:13:43.720 --> 0:13:47.200
<v Speaker 1>and that's why it's dark. Because if it felt electromagnetism,

0:13:47.240 --> 0:13:49.880
<v Speaker 1>it would reflect light, or it would give off light

0:13:49.960 --> 0:13:52.960
<v Speaker 1>like everything else does than the universe, it glows, or

0:13:53.040 --> 0:13:55.200
<v Speaker 1>if it felt the strong force, it would bind with

0:13:55.280 --> 0:13:58.280
<v Speaker 1>corks and form nucleons and interact with us. So it

0:13:58.280 --> 0:14:00.560
<v Speaker 1>doesn't interact with us in any way that we know

0:14:00.640 --> 0:14:03.360
<v Speaker 1>of other than gravitational And that's why we call it

0:14:03.480 --> 0:14:07.040
<v Speaker 1>matter because we think it's something that has new gravity.

0:14:07.080 --> 0:14:08.880
<v Speaker 1>But you know, it could also just be a tweak

0:14:08.920 --> 0:14:11.679
<v Speaker 1>to the way we understand gravity. But at its core,

0:14:11.720 --> 0:14:15.480
<v Speaker 1>it's really an observation that our theory of gravity doesn't

0:14:15.559 --> 0:14:20.240
<v Speaker 1>work either because there's missing mass or the theory is wrong. Right,

0:14:20.280 --> 0:14:22.520
<v Speaker 1>So those are two sides of the coin, right, Like,

0:14:22.640 --> 0:14:25.720
<v Speaker 1>according to what we know about how gravity works, there's

0:14:25.760 --> 0:14:29.760
<v Speaker 1>a lot of gravity missing, or there's too much gravity

0:14:29.760 --> 0:14:32.280
<v Speaker 1>in the universe. Almost. Yeah, there's gravity out there and

0:14:32.280 --> 0:14:35.080
<v Speaker 1>we don't have mass to explain it, and so we

0:14:35.160 --> 0:14:37.440
<v Speaker 1>have to sort of fill in those gaps. And that's

0:14:37.480 --> 0:14:39.680
<v Speaker 1>an uncomfortable feeling, right, You're like, well, you can't just

0:14:39.760 --> 0:14:42.160
<v Speaker 1>like fill in the gaps and assume that your theory

0:14:42.280 --> 0:14:45.440
<v Speaker 1>is right and add extra stuff to make it work out.

0:14:45.920 --> 0:14:49.440
<v Speaker 1>You know, that feels uncomfortable, Like there's snack food missing

0:14:49.440 --> 0:14:52.760
<v Speaker 1>from my fridge. Surely it was my son who cut

0:14:52.800 --> 0:14:54.000
<v Speaker 1>up in the middle of the night to eat it.

0:14:54.080 --> 0:14:56.920
<v Speaker 1>But you can't you can't just assume that. You can't

0:14:56.960 --> 0:14:58.920
<v Speaker 1>just assume that could have been your daughter. Maybe you

0:14:59.000 --> 0:15:01.720
<v Speaker 1>sleepwalked and aided or or And that's when you install

0:15:01.800 --> 0:15:03.440
<v Speaker 1>a camera in front of your fridge and you get

0:15:03.440 --> 0:15:06.280
<v Speaker 1>those weird videos of yourself at four am stuffing cake

0:15:06.320 --> 0:15:13.760
<v Speaker 1>in your face. Experience the hypothetically hypothetically hypathetically right, Alright,

0:15:13.760 --> 0:15:16.200
<v Speaker 1>So we think dark matter is there because of gravity.

0:15:16.240 --> 0:15:19.040
<v Speaker 1>And there are several ways that we have seen this

0:15:19.120 --> 0:15:22.320
<v Speaker 1>kind of missing gravity, right, that's in the galaxy and rotations.

0:15:22.400 --> 0:15:25.600
<v Speaker 1>The way galaxies rotade is kind of one of the

0:15:25.600 --> 0:15:28.000
<v Speaker 1>first one, maybe even Yeah, one of the most dramatic

0:15:28.160 --> 0:15:31.880
<v Speaker 1>and earliest pieces of evidence that there was more gravity

0:15:31.880 --> 0:15:35.040
<v Speaker 1>in the universe than we expected was looking at how

0:15:35.120 --> 0:15:38.640
<v Speaker 1>galaxies rotate. And we can add up all the mass

0:15:38.680 --> 0:15:41.560
<v Speaker 1>of the stars and the stuff in the galaxy and say, okay,

0:15:41.840 --> 0:15:44.320
<v Speaker 1>we know how much gravity there should be, and then

0:15:44.360 --> 0:15:48.080
<v Speaker 1>we can calculate how fast those galaxies are rotating. And

0:15:48.120 --> 0:15:50.720
<v Speaker 1>you know, for a galaxy, when it's rotating, it's trying

0:15:50.760 --> 0:15:52.960
<v Speaker 1>to push stuff off. It's trying to throw stuff off

0:15:53.000 --> 0:15:55.480
<v Speaker 1>the edge. Like if you put ping pong balls on

0:15:55.520 --> 0:15:57.480
<v Speaker 1>a merry go round and spin it, the ping pong

0:15:57.520 --> 0:16:00.680
<v Speaker 1>balls fly out. The thing that keeps the galaxy from

0:16:00.680 --> 0:16:03.760
<v Speaker 1>tearing itself apart from throwing those ping pong balls out

0:16:03.840 --> 0:16:07.440
<v Speaker 1>into inter galactic space, is the gravity. So you can

0:16:07.480 --> 0:16:10.880
<v Speaker 1>ask how fast is the galaxy spinning and is there

0:16:11.000 --> 0:16:14.200
<v Speaker 1>enough gravity to hold it together, because the faster spins,

0:16:14.200 --> 0:16:16.080
<v Speaker 1>the more gravity unied. Right. Yeah, It's kind of like

0:16:16.080 --> 0:16:18.160
<v Speaker 1>our solar system, right, like you know, the mass of

0:16:18.160 --> 0:16:20.000
<v Speaker 1>the Sun is what keeps all the planets kind of

0:16:20.000 --> 0:16:22.600
<v Speaker 1>spinning around it. But what if, like the planets for

0:16:22.680 --> 0:16:25.280
<v Speaker 1>spinning faster than what you could explain by the mass

0:16:25.280 --> 0:16:27.720
<v Speaker 1>of the Sun. You would need some other explanations, that's right,

0:16:27.760 --> 0:16:30.560
<v Speaker 1>You need more force to hold them into their orbits.

0:16:30.840 --> 0:16:32.920
<v Speaker 1>And so you say, well, maybe there's extra gravity or

0:16:32.960 --> 0:16:35.400
<v Speaker 1>some other force or something. And so we know there's

0:16:35.440 --> 0:16:40.200
<v Speaker 1>something else holding the galaxy together. And so the first explanations,

0:16:40.240 --> 0:16:43.040
<v Speaker 1>oh well, what if there's more invisible mass. It's just

0:16:43.080 --> 0:16:46.440
<v Speaker 1>some stuff in the galaxy that's providing gravity and we

0:16:46.560 --> 0:16:50.400
<v Speaker 1>just can't see it. And you can explain these rotation

0:16:50.480 --> 0:16:53.640
<v Speaker 1>curves the way the stars move around centers of galaxies.

0:16:53.960 --> 0:16:56.560
<v Speaker 1>If you distribute a bunch of mass sort of smoothly,

0:16:56.560 --> 0:16:58.440
<v Speaker 1>it's like a big clump in the middle, and then

0:16:58.440 --> 0:17:01.200
<v Speaker 1>sort of smoothly outpass the edge of the galaxy into

0:17:01.280 --> 0:17:04.280
<v Speaker 1>a big halo that's even actually bigger than the galaxy.

0:17:04.480 --> 0:17:06.800
<v Speaker 1>That explains to this as that would give you the

0:17:06.920 --> 0:17:09.239
<v Speaker 1>kind of gravity that we are seeing, right, because if

0:17:09.280 --> 0:17:12.160
<v Speaker 1>you look at a galaxy doesn't have that enough mass, right,

0:17:12.200 --> 0:17:14.639
<v Speaker 1>like there aren't enough stars or planets in it that

0:17:14.680 --> 0:17:16.520
<v Speaker 1>you can see. That's right. We count up all the

0:17:16.600 --> 0:17:19.520
<v Speaker 1>visible stuff and we say how much mass does it have?

0:17:19.640 --> 0:17:22.480
<v Speaker 1>And that just doesn't give us enough gravity to explain

0:17:22.640 --> 0:17:25.800
<v Speaker 1>how those galaxies are holding themselves together. And that was

0:17:25.840 --> 0:17:27.439
<v Speaker 1>the sort of genesis of it. I mean, for a

0:17:27.480 --> 0:17:30.080
<v Speaker 1>long time people were like, well, wow, that's must be

0:17:30.119 --> 0:17:32.639
<v Speaker 1>a mistake, you know, because coming to the idea that

0:17:32.680 --> 0:17:36.240
<v Speaker 1>there's five times as much mass as you can see

0:17:36.359 --> 0:17:38.760
<v Speaker 1>is a really big idea. It's not something people just

0:17:38.800 --> 0:17:41.880
<v Speaker 1>came to an afternoon and then accepted, Yeah, it doesn't

0:17:41.920 --> 0:17:44.240
<v Speaker 1>seem likely. It does not seem likely. It seems more

0:17:44.320 --> 0:17:47.480
<v Speaker 1>likely that you mismeasured something that you got the velocity

0:17:47.560 --> 0:17:50.000
<v Speaker 1>is wrong, or you know your grad student is pranking

0:17:50.040 --> 0:17:52.520
<v Speaker 1>you or something. It's a big idea, right, It's like

0:17:52.760 --> 0:17:55.200
<v Speaker 1>jumping to the conclusion right away that maybe there are

0:17:55.200 --> 0:17:57.560
<v Speaker 1>five ghosts in my house eating my snacks. You know,

0:17:57.680 --> 0:18:00.480
<v Speaker 1>that's like a big that's a big leap from like, hey,

0:18:00.520 --> 0:18:04.280
<v Speaker 1>maybe it's just your u. And so it took other

0:18:04.359 --> 0:18:08.040
<v Speaker 1>pieces of evidence before dark matter became mainstream. Right, all right,

0:18:08.080 --> 0:18:10.400
<v Speaker 1>let's get into those other ways that we know dark

0:18:10.440 --> 0:18:13.520
<v Speaker 1>matter is there, and let's get into whether or not

0:18:14.080 --> 0:18:16.359
<v Speaker 1>it is there, or me we just have gravity wrong.

0:18:16.480 --> 0:18:31.119
<v Speaker 1>But first, let's take a quick break, all right, Daniel,

0:18:31.119 --> 0:18:34.879
<v Speaker 1>we're talking about whether dark matter is necessary in the

0:18:35.000 --> 0:18:37.560
<v Speaker 1>universe or you know, maybe it's just the hanger on

0:18:37.720 --> 0:18:40.639
<v Speaker 1>and the universe could care less about dark matter. But

0:18:40.840 --> 0:18:42.800
<v Speaker 1>we we know it's definitely there because we see it

0:18:42.880 --> 0:18:46.040
<v Speaker 1>from the rotation of galaxies and also we've set off

0:18:46.280 --> 0:18:48.280
<v Speaker 1>kind of can see it, right, We can see it

0:18:48.320 --> 0:18:51.120
<v Speaker 1>in the way that distorts the light from other far

0:18:51.160 --> 0:18:53.679
<v Speaker 1>away stars. That's right. These days, we have a good

0:18:53.720 --> 0:18:58.000
<v Speaker 1>handful of ways to indirectly detect dark matter, and one

0:18:58.000 --> 0:19:01.320
<v Speaker 1>of the coolest is seeing it act like a lens

0:19:01.440 --> 0:19:05.920
<v Speaker 1>in the sky because dark matter only has gravitational forces,

0:19:05.920 --> 0:19:09.359
<v Speaker 1>but gravity can bend space, right, It's a bending of

0:19:09.400 --> 0:19:11.719
<v Speaker 1>space and time. So if you have a big blob

0:19:11.800 --> 0:19:15.520
<v Speaker 1>of invisible stuff in the sky, it will curve the

0:19:15.560 --> 0:19:18.440
<v Speaker 1>space it's in, so that photon is traveling through it

0:19:18.480 --> 0:19:21.560
<v Speaker 1>will get bent as if they're moving through a huge lens. Right,

0:19:21.840 --> 0:19:24.040
<v Speaker 1>So if there's a big blob of dark matter between

0:19:24.080 --> 0:19:27.200
<v Speaker 1>you and some really far away galaxy, it will distort

0:19:27.240 --> 0:19:31.040
<v Speaker 1>that galaxy, creating duplicates of it, stretching it just as

0:19:31.040 --> 0:19:33.040
<v Speaker 1>if there was a huge lens in the sky, right,

0:19:33.119 --> 0:19:35.040
<v Speaker 1>and then we can see that, like if you look

0:19:35.040 --> 0:19:37.800
<v Speaker 1>at pictures as a sky, you see these kind of distortions,

0:19:37.840 --> 0:19:40.600
<v Speaker 1>these ripples, these lensing effects. You can sort of see

0:19:40.680 --> 0:19:42.880
<v Speaker 1>dark matter almost, you can definitely see it. And there's

0:19:42.880 --> 0:19:45.840
<v Speaker 1>sort of two categories. There's strong lensing, like there's a

0:19:45.840 --> 0:19:49.040
<v Speaker 1>big dense blob and it's distorting the galaxies and it's

0:19:49.080 --> 0:19:51.720
<v Speaker 1>pretty hard to explain that kind of lensing in any

0:19:51.760 --> 0:19:54.920
<v Speaker 1>other way. And then there's weak lensing. We just sort

0:19:54.960 --> 0:19:57.919
<v Speaker 1>of like look at all the galaxies out there to see, like,

0:19:58.000 --> 0:19:59.960
<v Speaker 1>are any of them sort of just a little distorted?

0:20:00.000 --> 0:20:02.359
<v Speaker 1>They're just looking a little tweaked. And from that we

0:20:02.400 --> 0:20:04.439
<v Speaker 1>can get sort of like a map of where in

0:20:04.440 --> 0:20:07.360
<v Speaker 1>the sky we think the dark matter is just by

0:20:07.359 --> 0:20:10.520
<v Speaker 1>looking at small distortions. And that's how we've gotten a

0:20:10.560 --> 0:20:13.439
<v Speaker 1>pretty good map for where we think this missing mass is.

0:20:13.440 --> 0:20:15.399
<v Speaker 1>How we know that it's mostly in the center of

0:20:15.400 --> 0:20:18.040
<v Speaker 1>the galaxy and how far out past the edge of

0:20:18.080 --> 0:20:21.040
<v Speaker 1>the visible galaxy the dark matter halo might go. So

0:20:21.080 --> 0:20:23.560
<v Speaker 1>it's a really powerful technique, right, And so that's kind

0:20:23.560 --> 0:20:26.200
<v Speaker 1>of how dark matter entered in kind of our view

0:20:26.240 --> 0:20:30.080
<v Speaker 1>of the universe was these first initial ways. But since

0:20:30.119 --> 0:20:32.600
<v Speaker 1>then and we sort of have put more nails into

0:20:32.680 --> 0:20:35.200
<v Speaker 1>sort of the coffin of whether or not dark matter

0:20:35.320 --> 0:20:38.159
<v Speaker 1>is out there, right, I mean, it's now sort of

0:20:38.240 --> 0:20:41.120
<v Speaker 1>shows up in pictures of the universe, the early universe,

0:20:41.119 --> 0:20:44.280
<v Speaker 1>it kind of shows up in our calculations about all

0:20:44.320 --> 0:20:46.560
<v Speaker 1>of the energy in the universe. Right, It's gotten more

0:20:46.600 --> 0:20:48.960
<v Speaker 1>and more convincing that there's something there that's right, it

0:20:49.000 --> 0:20:52.120
<v Speaker 1>becomes very difficult to explain the universe you see without

0:20:52.240 --> 0:20:55.640
<v Speaker 1>dark matter. For example, we see the influence of dark

0:20:55.680 --> 0:20:59.119
<v Speaker 1>matter on the formation of structures in the universe. Like

0:20:59.200 --> 0:21:02.280
<v Speaker 1>the universe be in as a sort of diffuse cloud,

0:21:02.440 --> 0:21:04.920
<v Speaker 1>you know, just of gas, mostly hydrogen, and then it

0:21:05.000 --> 0:21:08.840
<v Speaker 1>started clumping together, and that clumping comes from gravity. Right,

0:21:08.840 --> 0:21:11.359
<v Speaker 1>So gravity is the thing that draws these things together

0:21:11.400 --> 0:21:14.560
<v Speaker 1>and eventually gives you stars and galaxies and planets and

0:21:14.600 --> 0:21:16.560
<v Speaker 1>all that cool stuff. If you run a stimulation of

0:21:16.600 --> 0:21:19.200
<v Speaker 1>the universe without any dark matter, then you don't get

0:21:19.280 --> 0:21:22.000
<v Speaker 1>galaxies in the first ten billion years. It takes like

0:21:22.040 --> 0:21:25.400
<v Speaker 1>another ten or twenty billion years. So it's dark matter

0:21:25.480 --> 0:21:29.119
<v Speaker 1>that's that's created these like gravitational wells for stuff to

0:21:29.160 --> 0:21:32.480
<v Speaker 1>fall into to make the stars in the galaxies and us.

0:21:33.080 --> 0:21:35.359
<v Speaker 1>So just like the whole structure of the universe would

0:21:35.359 --> 0:21:39.800
<v Speaker 1>look very different without some kind of gravitational stuff out there,

0:21:40.760 --> 0:21:43.119
<v Speaker 1>and we should have just called them dark clumps or

0:21:43.880 --> 0:21:47.520
<v Speaker 1>dark do it. And even earlier in the universe, like

0:21:47.560 --> 0:21:51.120
<v Speaker 1>we've talked on this program about the cosmic microwave background radiation.

0:21:51.600 --> 0:21:54.760
<v Speaker 1>Those are photons from the very very early universe, three

0:21:54.880 --> 0:21:58.359
<v Speaker 1>hundred thousand years after the universe was created, the first

0:21:58.359 --> 0:22:01.879
<v Speaker 1>moment when the universe became Rand's parent to light. Before

0:22:01.920 --> 0:22:04.720
<v Speaker 1>that it was thick and soupy and light got reabsorbed,

0:22:04.920 --> 0:22:06.800
<v Speaker 1>and after that it was cool enough that light could

0:22:06.800 --> 0:22:10.439
<v Speaker 1>travel through the universe without being absorbed. And the shape

0:22:10.440 --> 0:22:13.439
<v Speaker 1>of that plasma that gave off that light was affected

0:22:13.480 --> 0:22:16.000
<v Speaker 1>by dark matter and how much dark matter there was

0:22:16.080 --> 0:22:18.679
<v Speaker 1>and much normal matter there was, and that stuff like

0:22:18.920 --> 0:22:22.040
<v Speaker 1>bounced off each other and oscillated and like squeezed and

0:22:22.080 --> 0:22:25.560
<v Speaker 1>squished that plasma. So the amount of dark matter in

0:22:25.640 --> 0:22:28.880
<v Speaker 1>that moment of the universe affects the shape of that light,

0:22:28.960 --> 0:22:31.320
<v Speaker 1>the currents, the sort of patterns we see in that

0:22:31.400 --> 0:22:34.960
<v Speaker 1>light in a very very precise way that's hard to

0:22:35.000 --> 0:22:38.400
<v Speaker 1>describe in any other way other than there's some other

0:22:38.520 --> 0:22:42.200
<v Speaker 1>kind of stuff out there. So that's giving us this graphic. Yeah,

0:22:42.240 --> 0:22:44.679
<v Speaker 1>you can see like it's imprint in the light from

0:22:44.720 --> 0:22:48.359
<v Speaker 1>the early universe, Like it's visually and like tangibly and like,

0:22:49.040 --> 0:22:51.679
<v Speaker 1>you know, you can calculate it the storts that light.

0:22:51.760 --> 0:22:53.920
<v Speaker 1>That's right. And so if you just take the universe

0:22:53.920 --> 0:22:56.920
<v Speaker 1>and you add to it a new particle, a particle

0:22:56.920 --> 0:22:59.720
<v Speaker 1>that doesn't move really fast, we call it cold and

0:22:59.800 --> 0:23:03.399
<v Speaker 1>doesn't feel anything but gravity, it explains all of this stuff.

0:23:03.440 --> 0:23:06.760
<v Speaker 1>It explains why galaxies rotate the way they do, why

0:23:06.800 --> 0:23:09.880
<v Speaker 1>the cosmic microwave background rediation looks the way it does,

0:23:10.200 --> 0:23:13.880
<v Speaker 1>why the structure of the universe has this structure at

0:23:13.880 --> 0:23:17.600
<v Speaker 1>this time in the universe. And also there are very specific,

0:23:17.880 --> 0:23:20.919
<v Speaker 1>awesome experiments that the universe has done to sort of

0:23:20.960 --> 0:23:24.399
<v Speaker 1>demonstrate dark matter to us. Yeah, I guess, you know,

0:23:24.480 --> 0:23:27.160
<v Speaker 1>I think maybe a question that a lot of people have,

0:23:27.280 --> 0:23:29.520
<v Speaker 1>and I'm sure if physicists had at the beginning, was,

0:23:29.960 --> 0:23:32.800
<v Speaker 1>you know, why does it need to be something special?

0:23:32.920 --> 0:23:35.200
<v Speaker 1>Like why does it need to be a new kind

0:23:35.200 --> 0:23:39.680
<v Speaker 1>of particle or matter? Couldn't it also just be something regular?

0:23:39.760 --> 0:23:41.560
<v Speaker 1>But that you just can't see, Like, you know, what

0:23:41.600 --> 0:23:44.040
<v Speaker 1>if there's a whole bunch of black asteroids out there

0:23:44.119 --> 0:23:46.720
<v Speaker 1>that are hard to see, or you know, a lot

0:23:46.800 --> 0:23:49.359
<v Speaker 1>of small dust that we can see, or maybe even

0:23:49.400 --> 0:23:51.560
<v Speaker 1>like a whole bunch of little black holes kind of

0:23:51.600 --> 0:23:53.919
<v Speaker 1>spread around the universe. Yeah, that's a great question, like

0:23:53.960 --> 0:23:56.040
<v Speaker 1>why do we know it's a new kind of thing.

0:23:56.200 --> 0:23:57.920
<v Speaker 1>Why can't it just be more of the same but

0:23:58.040 --> 0:24:01.080
<v Speaker 1>just kind of dark, right? Yeah, yeah, Well we don't

0:24:01.080 --> 0:24:04.640
<v Speaker 1>really know anything in our current set of particles that

0:24:04.880 --> 0:24:08.440
<v Speaker 1>is that dark. I mean, other than neutrinos. Everything else

0:24:08.520 --> 0:24:11.200
<v Speaker 1>has some kind of interaction, like if it's a black

0:24:11.359 --> 0:24:14.240
<v Speaker 1>rock or something, well that does reflect light, it does

0:24:14.359 --> 0:24:16.639
<v Speaker 1>give off light. So if it's made out of the

0:24:16.680 --> 0:24:18.560
<v Speaker 1>normal kind of matter, it's going to have the kind

0:24:18.560 --> 0:24:22.320
<v Speaker 1>of interactions we have, and therefore we would be able

0:24:22.359 --> 0:24:26.360
<v Speaker 1>to see it, except of course, neutrinos. Neutrinos were candidate

0:24:26.400 --> 0:24:28.239
<v Speaker 1>for dark matter for a long time. The problem is

0:24:28.359 --> 0:24:31.879
<v Speaker 1>neutrinos move away too fast, they zoom around the universe

0:24:31.920 --> 0:24:34.280
<v Speaker 1>because they're so light, so they don't give the same

0:24:34.280 --> 0:24:37.200
<v Speaker 1>sort of structure to the universe that dark matter does.

0:24:37.240 --> 0:24:39.439
<v Speaker 1>You need this thing to be sort of slow moving

0:24:39.480 --> 0:24:42.399
<v Speaker 1>and cold in order to stick around long enough to

0:24:42.480 --> 0:24:46.240
<v Speaker 1>give the structure of galaxies. Could you have cold neutrinos

0:24:46.320 --> 0:24:48.560
<v Speaker 1>like slow moving neutrinos. Then we talk about that the

0:24:48.600 --> 0:24:51.800
<v Speaker 1>other in another episode. Could you have cold neutrinos, Yes,

0:24:52.160 --> 0:24:55.240
<v Speaker 1>but we don't think that neutrinos are that cold. We

0:24:55.320 --> 0:24:58.600
<v Speaker 1>haven't seen cold neutrinos. Neutrinos are so light they have

0:24:58.680 --> 0:25:02.240
<v Speaker 1>almost no mass that they essentially almost always travel near

0:25:02.280 --> 0:25:05.080
<v Speaker 1>the speed of light. They're always in a rush, They're

0:25:05.080 --> 0:25:08.040
<v Speaker 1>always in a hurry. Yes, neutrinos are hot, as we

0:25:08.119 --> 0:25:12.800
<v Speaker 1>call them in particle physics. And it literally and figuratively

0:25:12.920 --> 0:25:15.840
<v Speaker 1>is it's it's a pretty big trend right now, that's right,

0:25:15.880 --> 0:25:18.040
<v Speaker 1>all right? Well, I guess if it's not maybe something

0:25:18.080 --> 0:25:20.119
<v Speaker 1>we know about, could it be that just maybe we

0:25:20.160 --> 0:25:23.280
<v Speaker 1>have our theories wrong about how things work, Like, you know,

0:25:23.320 --> 0:25:25.320
<v Speaker 1>maybe it's not a new particle or a new kind

0:25:25.359 --> 0:25:28.439
<v Speaker 1>of matter, but maybe we just have gravity wrong. Like

0:25:28.520 --> 0:25:31.320
<v Speaker 1>maybe gravity doesn't work the way we think it is.

0:25:31.320 --> 0:25:36.080
<v Speaker 1>And maybe these larger universe size scales could gravity, you know,

0:25:36.160 --> 0:25:38.320
<v Speaker 1>could there be a different theory of gravity that would

0:25:38.320 --> 0:25:40.920
<v Speaker 1>maybe account for what we think is dark matter. It's

0:25:40.960 --> 0:25:44.560
<v Speaker 1>definitely something to consider, right, because all these observations are

0:25:44.640 --> 0:25:48.080
<v Speaker 1>just observations of gravity. And what we're doing is we're saying,

0:25:48.240 --> 0:25:50.440
<v Speaker 1>we assume there's a certain amount of mass out there,

0:25:50.720 --> 0:25:53.560
<v Speaker 1>we assume we know how gravity works. We estimate how

0:25:53.600 --> 0:25:56.440
<v Speaker 1>much gravity there should be based on that mass. Right,

0:25:56.440 --> 0:25:58.679
<v Speaker 1>But there are two steps in there. There's figure out

0:25:58.760 --> 0:26:01.600
<v Speaker 1>where the mass is and in calculate how much gravity

0:26:01.640 --> 0:26:05.080
<v Speaker 1>there is from that mass. If that second step is wrong, right,

0:26:05.240 --> 0:26:07.960
<v Speaker 1>if the theory of gravity works differently from what we expected,

0:26:08.160 --> 0:26:11.800
<v Speaker 1>then yeah, that could possibly explain it. Because remember, gravity

0:26:11.920 --> 0:26:14.840
<v Speaker 1>is very very weak, which makes it very very hard

0:26:14.880 --> 0:26:18.199
<v Speaker 1>to test, Like it's difficult to measure the force of

0:26:18.280 --> 0:26:22.000
<v Speaker 1>gravity at the scale of one centimeter between two pebbles

0:26:22.520 --> 0:26:26.280
<v Speaker 1>because there's force there's almost zero, Like you need to

0:26:26.280 --> 0:26:29.880
<v Speaker 1>build a very sensitive instrument to measure the gravitational force

0:26:29.920 --> 0:26:33.440
<v Speaker 1>between anything that's smaller than you know, planets and moons. Yeah,

0:26:33.480 --> 0:26:36.520
<v Speaker 1>because you know, like our current theory of gravity says that,

0:26:36.640 --> 0:26:40.239
<v Speaker 1>you know, gravity changes by one of our squared, Like

0:26:40.280 --> 0:26:43.080
<v Speaker 1>the force of gravity kind of depends on the distance

0:26:43.119 --> 0:26:45.720
<v Speaker 1>between two things squared. And then you put down in

0:26:45.760 --> 0:26:49.120
<v Speaker 1>the denominator and that always seems kind of almost too

0:26:49.119 --> 0:26:51.520
<v Speaker 1>simple to me, Like, what are the chances at the

0:26:51.600 --> 0:26:55.240
<v Speaker 1>universe would pick such a simple little formula to calculate gravity.

0:26:55.320 --> 0:26:58.480
<v Speaker 1>You know, why isn't it like one over our squared

0:26:58.680 --> 0:27:01.639
<v Speaker 1>times are to the zero point seven five? You know,

0:27:01.960 --> 0:27:04.199
<v Speaker 1>I mean, like it seems so simple. Maybe what if

0:27:04.200 --> 0:27:06.040
<v Speaker 1>it's wrong, Like what if gravity isn't one of our

0:27:06.040 --> 0:27:09.240
<v Speaker 1>our square but maybe changes over distances in a way

0:27:09.359 --> 0:27:11.840
<v Speaker 1>that could maybe explain dark matter. Yeah, that's a totally

0:27:11.840 --> 0:27:14.160
<v Speaker 1>realistic thing to think. Although you know, there's a lot

0:27:14.160 --> 0:27:16.440
<v Speaker 1>of these patterns, these one of our our squared patterns

0:27:16.440 --> 0:27:19.280
<v Speaker 1>in physics and enforces and there is a good reason

0:27:19.320 --> 0:27:21.240
<v Speaker 1>for it and a fairly simple way to understand it.

0:27:21.480 --> 0:27:24.520
<v Speaker 1>If you imagine like the surface of a sphere surrounding

0:27:24.560 --> 0:27:27.320
<v Speaker 1>a point. Think about like all the gravitational energy coming

0:27:27.320 --> 0:27:30.040
<v Speaker 1>out of a point, the surface of a sphere surrounding it,

0:27:30.440 --> 0:27:33.640
<v Speaker 1>all the gravitational energy passes through that sphere, and then

0:27:33.800 --> 0:27:36.600
<v Speaker 1>as the radius of that sphere gets larger, what's the

0:27:36.640 --> 0:27:39.480
<v Speaker 1>surface of that sphere? Will it goes like are squared,

0:27:39.920 --> 0:27:42.560
<v Speaker 1>and so the power at any point should go like

0:27:42.680 --> 0:27:46.480
<v Speaker 1>one over our squared. It sort of makes sense geometrically

0:27:46.840 --> 0:27:50.160
<v Speaker 1>but what if geometry is wrong. What if geometry is wrong? Right?

0:27:50.359 --> 0:27:54.879
<v Speaker 1>What is wrong? What if podcasting is wrong? What if

0:27:54.880 --> 0:27:56.920
<v Speaker 1>one plus one is wrong? Well, it kind of, I mean,

0:27:57.119 --> 0:27:59.920
<v Speaker 1>you know, we talk about sometimes about how space is

0:28:00.080 --> 0:28:02.679
<v Speaker 1>not you know, this nice and neat, orderly thing, and

0:28:02.720 --> 0:28:06.560
<v Speaker 1>that sometimes you can even like measure triangles in real

0:28:06.600 --> 0:28:09.560
<v Speaker 1>space that have angles that are bigger than a hundred

0:28:09.600 --> 0:28:13.199
<v Speaker 1>and eighty degrees, could maybe, like space be weird in

0:28:13.280 --> 0:28:16.520
<v Speaker 1>such a way that it's not really one over our squares? Yeah? Absolutely,

0:28:16.520 --> 0:28:18.560
<v Speaker 1>And there are forces that don't go like one of

0:28:18.560 --> 0:28:20.800
<v Speaker 1>our our squared, Like the strong force doesn't go like

0:28:20.800 --> 0:28:23.520
<v Speaker 1>one of our squared at small distances. It gets even

0:28:23.640 --> 0:28:26.560
<v Speaker 1>stronger as you get further away. So you definitely got

0:28:26.560 --> 0:28:29.400
<v Speaker 1>to be open to weirdness. And so around the time

0:28:29.440 --> 0:28:31.480
<v Speaker 1>when dark matter was sort of coming up in the

0:28:31.520 --> 0:28:34.320
<v Speaker 1>world as an idea, when it was based mostly on

0:28:34.440 --> 0:28:37.800
<v Speaker 1>galaxy rotations, people thought, well, how can I tweak gravity

0:28:38.080 --> 0:28:41.240
<v Speaker 1>to explain what I'm seeing without dark matter? What would

0:28:41.240 --> 0:28:42.960
<v Speaker 1>I need to change? How what would you have to

0:28:42.960 --> 0:28:44.880
<v Speaker 1>be like one over our to the third or one

0:28:44.880 --> 0:28:47.360
<v Speaker 1>of our at one point five or whatever in order

0:28:47.360 --> 0:28:51.200
<v Speaker 1>to explain these galaxy rotations without dark matter, and so

0:28:51.240 --> 0:28:54.600
<v Speaker 1>they came up with a different theory. It's called mond

0:28:54.960 --> 0:29:01.760
<v Speaker 1>m O n D for modified Newtonian dynamics. Know, I

0:29:01.760 --> 0:29:04.000
<v Speaker 1>would have just called the dark bath. I wish you

0:29:04.040 --> 0:29:05.760
<v Speaker 1>could get in a time machine and go back and

0:29:05.800 --> 0:29:08.160
<v Speaker 1>tell them because I hate moms. Would that be a

0:29:08.160 --> 0:29:13.520
<v Speaker 1>lot catch here and fun? Dark bath? Well, mon, I

0:29:13.520 --> 0:29:15.920
<v Speaker 1>guess if you're French, then it's like, oh, yeah, it

0:29:15.960 --> 0:29:19.080
<v Speaker 1>means the world. I suppose it's missing the E and

0:29:19.120 --> 0:29:21.959
<v Speaker 1>it commits the terrible acronym crime of taking two letters

0:29:21.960 --> 0:29:26.120
<v Speaker 1>from one of the words, you know, modified. Yeah, all right,

0:29:26.160 --> 0:29:28.840
<v Speaker 1>so there is a kind of a theory in physics.

0:29:28.920 --> 0:29:31.080
<v Speaker 1>It says like maybe we do have gravity wrong, right,

0:29:31.640 --> 0:29:33.920
<v Speaker 1>is like an idea you guys take seriously, like maybe

0:29:34.040 --> 0:29:36.360
<v Speaker 1>there is no dark matter, it's just dark bath. It's

0:29:36.360 --> 0:29:39.120
<v Speaker 1>definitely an idea that physics should take seriously in the

0:29:39.160 --> 0:29:42.320
<v Speaker 1>sense that we should think about alternatives. This one theory

0:29:42.320 --> 0:29:44.920
<v Speaker 1>in particular doesn't have a lot of supporters, and we'll

0:29:44.920 --> 0:29:47.640
<v Speaker 1>get into exactly why, but you know, it's an interesting

0:29:47.680 --> 0:29:52.000
<v Speaker 1>idea and it says like maybe gravity works differently at

0:29:52.160 --> 0:29:55.640
<v Speaker 1>very very large distances, like you know, we've tested gravity

0:29:55.680 --> 0:29:57.880
<v Speaker 1>here on Earth. We know how it works. We've tested

0:29:57.880 --> 0:30:00.560
<v Speaker 1>gravity in the Solar System pretty well. But you know,

0:30:00.640 --> 0:30:03.800
<v Speaker 1>maybe the first time we're looking at gravity on galaxy scales,

0:30:03.880 --> 0:30:07.320
<v Speaker 1>maybe gravity just works differently over like, you know, fifty

0:30:07.400 --> 0:30:10.840
<v Speaker 1>thou light years, right, we haven't done that experiment before.

0:30:10.920 --> 0:30:13.640
<v Speaker 1>Maybe it gets going, like, maybe it gets stronger in

0:30:13.960 --> 0:30:16.880
<v Speaker 1>galaxy size scales. Yeah, And so the idea is actually

0:30:16.920 --> 0:30:20.560
<v Speaker 1>even weirder than that. It says, maybe gravity works differently

0:30:21.280 --> 0:30:25.840
<v Speaker 1>when you have a very very small acceleration, things are

0:30:25.880 --> 0:30:30.720
<v Speaker 1>not being pulled very hard. Maybe gravity works a little

0:30:30.720 --> 0:30:32.600
<v Speaker 1>bit different. Oh my god, you just blew my mind.

0:30:32.600 --> 0:30:35.560
<v Speaker 1>All right, let's let's get into this crazy idea that

0:30:35.600 --> 0:30:39.040
<v Speaker 1>gravity depends on how you're moving maybe, and whether or

0:30:39.080 --> 0:30:55.040
<v Speaker 1>not that could work. But first let's take another quick break, right, Daniel,

0:30:55.080 --> 0:30:58.600
<v Speaker 1>we're talking about dark math to maybe explain dark matter.

0:30:58.920 --> 0:31:01.880
<v Speaker 1>And so there's an idea that maybe our formulation of

0:31:01.880 --> 0:31:04.400
<v Speaker 1>gravity or how we think gravity works could be wrong.

0:31:04.440 --> 0:31:08.080
<v Speaker 1>Maybe and it could maybe act very differently over larger scales,

0:31:08.120 --> 0:31:11.160
<v Speaker 1>like maybe it gets stronger the galaxy scale or when

0:31:11.360 --> 0:31:14.240
<v Speaker 1>you're telling me it's actually when there's lower accelerations. And

0:31:14.240 --> 0:31:16.200
<v Speaker 1>this is just an idea again, right, this is just

0:31:16.240 --> 0:31:18.640
<v Speaker 1>an idea. But hey, everything is just an idea, right,

0:31:18.680 --> 0:31:21.960
<v Speaker 1>even lunch lunch is just an idea. Remember, Oh no, Daniel,

0:31:22.080 --> 0:31:25.080
<v Speaker 1>lunch is very real to me. Well, the idea is,

0:31:25.240 --> 0:31:27.120
<v Speaker 1>you know, somehow you have to get gravity to be

0:31:27.280 --> 0:31:30.840
<v Speaker 1>stronger without breaking things we already know. So what if

0:31:30.960 --> 0:31:33.480
<v Speaker 1>you know affecting things on the edge of the galaxy,

0:31:33.760 --> 0:31:35.920
<v Speaker 1>you could have gravity instead of going like one over

0:31:36.000 --> 0:31:38.640
<v Speaker 1>our squared, which you make it very very weak as

0:31:38.640 --> 0:31:40.760
<v Speaker 1>our gets large, you can make it go like one

0:31:40.800 --> 0:31:43.760
<v Speaker 1>over R. It doesn't fall off as quickly, doesn't get

0:31:43.800 --> 0:31:47.560
<v Speaker 1>weak as quickly with large distances. Interesting, So like the

0:31:47.640 --> 0:31:50.880
<v Speaker 1>gravity I feel with another planet on the other side

0:31:50.880 --> 0:31:54.400
<v Speaker 1>of the Milky Way, maybe it's stronger than I think. Yeah,

0:31:54.480 --> 0:31:56.560
<v Speaker 1>maybe it's not like one over our squares, more like

0:31:56.600 --> 0:31:59.240
<v Speaker 1>one over R and R is still really really large.

0:31:59.360 --> 0:32:01.880
<v Speaker 1>So you know, those planets don't affect you because the

0:32:01.960 --> 0:32:04.880
<v Speaker 1>gravity from them is still really tiny. But if you're

0:32:04.880 --> 0:32:07.040
<v Speaker 1>adding up lots of planets and you're trying to calculate,

0:32:07.040 --> 0:32:10.040
<v Speaker 1>like how a whole galaxy spins, then it really does

0:32:10.120 --> 0:32:11.960
<v Speaker 1>make a big difference to go like one of our

0:32:11.960 --> 0:32:15.360
<v Speaker 1>are instead of one of are squared. But it seems

0:32:15.400 --> 0:32:18.720
<v Speaker 1>a bit hacky as opposed to dark matter. Dark matter

0:32:18.760 --> 0:32:21.360
<v Speaker 1>doesn't seem hacky. Well, dark matter, you know, you can

0:32:21.440 --> 0:32:24.640
<v Speaker 1>explain a lot of really different things adding just one

0:32:24.760 --> 0:32:27.200
<v Speaker 1>simple idea, like hey, what if there's a new particle

0:32:27.480 --> 0:32:29.800
<v Speaker 1>that's not hacky, Like we don't know why there's a

0:32:29.800 --> 0:32:31.960
<v Speaker 1>certain number of particles in the universe and not more,

0:32:32.120 --> 0:32:34.800
<v Speaker 1>or if there are more, so adding one new particle

0:32:34.800 --> 0:32:37.600
<v Speaker 1>doesn't feel as hacky. Is like let's have gravity have

0:32:37.640 --> 0:32:40.160
<v Speaker 1>a knob on it, or like a distance above which

0:32:40.160 --> 0:32:44.000
<v Speaker 1>it starts behaving different rules, or you know, small accelerations

0:32:44.040 --> 0:32:46.920
<v Speaker 1>below which it starts behaving differently. Really, what why does

0:32:46.920 --> 0:32:49.320
<v Speaker 1>it need to be low accelerations? How does that work? In?

0:32:49.720 --> 0:32:52.000
<v Speaker 1>It doesn't really work as I think I heard you

0:32:52.040 --> 0:32:55.000
<v Speaker 1>react because like the acceleration with respect to what right,

0:32:55.040 --> 0:32:57.600
<v Speaker 1>all of a sudden, that gravity you feel depends on

0:32:57.680 --> 0:33:00.720
<v Speaker 1>your reference frame, and it brings all sorts of symmetries.

0:33:00.960 --> 0:33:04.560
<v Speaker 1>But there is that one idea that accelerations like one

0:33:04.560 --> 0:33:07.280
<v Speaker 1>ten trillions of the gravity on Earth. If you feel

0:33:07.280 --> 0:33:10.080
<v Speaker 1>an acceleration less than that, then the gravity on you

0:33:10.400 --> 0:33:14.160
<v Speaker 1>behaves differently than it does for larger accelerations. Oh, I see.

0:33:14.240 --> 0:33:16.600
<v Speaker 1>It's not you're not saying when you're going at a

0:33:16.680 --> 0:33:19.600
<v Speaker 1>low acceleration, it's just you mean the when the effects

0:33:19.640 --> 0:33:21.760
<v Speaker 1>of gravity are small, maybe it doesn't behave as one

0:33:21.800 --> 0:33:24.000
<v Speaker 1>over our square. Yeah, and the effects of gravity at

0:33:24.120 --> 0:33:27.440
<v Speaker 1>very very far distances are really small. Like what is

0:33:27.520 --> 0:33:30.280
<v Speaker 1>the acceleration on some star at the edge of the

0:33:30.320 --> 0:33:33.560
<v Speaker 1>galaxy due to the black hole the center of the galaxy. Well,

0:33:33.640 --> 0:33:36.600
<v Speaker 1>the distance is fifty thou light years, so the acceleration

0:33:37.160 --> 0:33:40.560
<v Speaker 1>is very small, also because the masses are large, and

0:33:40.600 --> 0:33:42.760
<v Speaker 1>so it's just a way to say, let's have it

0:33:42.800 --> 0:33:46.000
<v Speaker 1>have an effect where we see this weirdness and not

0:33:46.120 --> 0:33:48.400
<v Speaker 1>have an effect anywhere else. Let's try not to break

0:33:48.760 --> 0:33:51.280
<v Speaker 1>what we already know and understand and only have this

0:33:51.400 --> 0:33:54.560
<v Speaker 1>theory turn on in special cases. All right, so that's

0:33:54.560 --> 0:33:56.880
<v Speaker 1>a possibility. But where did this idea come from? Like

0:33:57.000 --> 0:33:59.200
<v Speaker 1>why would we think that maybe gravity is wrong? So

0:33:59.280 --> 0:34:01.080
<v Speaker 1>for a long time there wasn't really a good idea

0:34:01.120 --> 0:34:02.880
<v Speaker 1>that was just like, well, I don't know, but if

0:34:02.920 --> 0:34:05.280
<v Speaker 1>I put in this other formula, I can explain the

0:34:05.280 --> 0:34:09.120
<v Speaker 1>galaxy rotation curves without dark matter. Without dark matter. Yeah,

0:34:09.120 --> 0:34:11.560
<v Speaker 1>So like all right, so either there's missing masks or

0:34:11.600 --> 0:34:15.200
<v Speaker 1>gravity works this other weird way, and then people started thinking, well,

0:34:15.239 --> 0:34:18.080
<v Speaker 1>why would gravity work that way? Is there any reason

0:34:18.200 --> 0:34:20.680
<v Speaker 1>for it? And that's a totally valid line of inquiry, right,

0:34:20.719 --> 0:34:22.760
<v Speaker 1>like what theory do we have to have to explain

0:34:22.800 --> 0:34:25.319
<v Speaker 1>the data? And does that theory make sense? Can we

0:34:25.320 --> 0:34:27.879
<v Speaker 1>come up with a reason why? Maybe that theory is right?

0:34:28.320 --> 0:34:32.279
<v Speaker 1>A theory about a theory underpinnings of the theory, right.

0:34:32.440 --> 0:34:35.240
<v Speaker 1>We always in physics want to have a microscopic understanding.

0:34:35.239 --> 0:34:37.279
<v Speaker 1>We don't want to just say gravity just has this

0:34:37.360 --> 0:34:39.120
<v Speaker 1>number on it. We want to know why does it?

0:34:39.120 --> 0:34:41.399
<v Speaker 1>Where does that come from? Why isn't it something else?

0:34:41.440 --> 0:34:43.239
<v Speaker 1>Just like you were saying earlier, why is it one

0:34:43.280 --> 0:34:45.600
<v Speaker 1>of our square not one over our two point one

0:34:45.719 --> 0:34:50.920
<v Speaker 1>or whatever? That's the next version upgraded gravity. And so

0:34:51.040 --> 0:34:54.040
<v Speaker 1>recently there is an idea from a guy in Holland

0:34:54.080 --> 0:34:57.480
<v Speaker 1>to Eric Verlinda, and he has this crazy idea of

0:34:57.520 --> 0:35:01.440
<v Speaker 1>gravity called entropic gravity that i'd be able to explain

0:35:02.000 --> 0:35:06.480
<v Speaker 1>why gravity works differently at these distance scales. I feel

0:35:06.480 --> 0:35:08.719
<v Speaker 1>like maybe he just grabbed two cool sounding things and

0:35:08.719 --> 0:35:14.000
<v Speaker 1>put them together. Tropic answer like dynamic gravity or something.

0:35:14.040 --> 0:35:15.840
<v Speaker 1>But it comes from a cool place. You know, it

0:35:15.880 --> 0:35:21.520
<v Speaker 1>was Stephen Hawking who first connected sort of thermodynamics and gravity.

0:35:21.680 --> 0:35:25.400
<v Speaker 1>He started thinking about the temperature of black holes and thinking,

0:35:25.760 --> 0:35:28.600
<v Speaker 1>you know, if black holes have temperatures, that means they

0:35:28.600 --> 0:35:32.000
<v Speaker 1>should radiate. Oh wait, and that's Hawking radiation. So in

0:35:32.000 --> 0:35:34.160
<v Speaker 1>the last sort of forty years, people have been thinking

0:35:34.200 --> 0:35:37.359
<v Speaker 1>about gravity and through our dynamics as a connection. They're

0:35:37.360 --> 0:35:40.839
<v Speaker 1>trying to understand like, you know, actually, maybe gravity isn't

0:35:40.880 --> 0:35:44.879
<v Speaker 1>a fundamental force, and maybe, you know Einstein's idea that

0:35:44.960 --> 0:35:48.680
<v Speaker 1>gravity is just a curvature spacetime, maybe that's also wrong.

0:35:49.000 --> 0:35:54.080
<v Speaker 1>Maybe instead, gravity is just like an emergent phenomena of thermodynamics.

0:35:54.600 --> 0:35:58.480
<v Speaker 1>Maybe it's just like comes out of the manipulation and

0:35:58.560 --> 0:36:02.000
<v Speaker 1>interaction of some tiny little bits of space in a

0:36:02.040 --> 0:36:05.560
<v Speaker 1>way that feels like gravity to us. That's a little

0:36:05.560 --> 0:36:08.080
<v Speaker 1>bit mind blowing. Yeah, it's a little bit mind blowing.

0:36:08.160 --> 0:36:11.000
<v Speaker 1>This whole idea of emergent phenomena can be hard to

0:36:11.000 --> 0:36:13.239
<v Speaker 1>get your mind around, but it's actually very familiar. You know,

0:36:13.320 --> 0:36:16.480
<v Speaker 1>Like we can talk about wind, right, Wind is an

0:36:16.520 --> 0:36:19.440
<v Speaker 1>emergent phenomena. It's not a fundamental force in the universe.

0:36:19.760 --> 0:36:23.239
<v Speaker 1>You know, two particles interacting don't feel wind. Wind is

0:36:23.280 --> 0:36:25.960
<v Speaker 1>a combination of lots of other things we do understand

0:36:26.000 --> 0:36:30.279
<v Speaker 1>on a microscopical level that has a macroscopic effect, or

0:36:30.400 --> 0:36:33.680
<v Speaker 1>like economics. You know, there are laws of economics that

0:36:33.760 --> 0:36:35.920
<v Speaker 1>come from you know, supply and demand or whatever. It's

0:36:35.960 --> 0:36:38.440
<v Speaker 1>not a fundamental force in the universe, but still you

0:36:38.440 --> 0:36:41.080
<v Speaker 1>could have an understanding of it. And so they think

0:36:41.120 --> 0:36:45.880
<v Speaker 1>maybe gravity is just like a macroscopic effect of something microscopic,

0:36:45.920 --> 0:36:49.840
<v Speaker 1>maybe the thermodynamics of space time. Like there there is

0:36:49.880 --> 0:36:53.279
<v Speaker 1>no gravity, it's just kind of like how space itself

0:36:53.400 --> 0:36:56.560
<v Speaker 1>kind of arranges itself. Yeah, because we know that space

0:36:56.719 --> 0:37:00.640
<v Speaker 1>likes to increase entropy, likes to increase disorder, and so

0:37:00.719 --> 0:37:03.440
<v Speaker 1>we think entropy always increases in the universe, and so

0:37:03.520 --> 0:37:05.960
<v Speaker 1>maybe gravity is just an effect of that. You know.

0:37:06.000 --> 0:37:08.560
<v Speaker 1>The argument goes something like when things fall into a

0:37:08.600 --> 0:37:12.000
<v Speaker 1>black hole, for example, that increases the entropy of the

0:37:12.040 --> 0:37:14.839
<v Speaker 1>black hole, because otherwise it would violate the second law

0:37:14.880 --> 0:37:18.040
<v Speaker 1>of thermodynamics. Things can't just disappear into the black hole.

0:37:18.520 --> 0:37:21.480
<v Speaker 1>But maybe it's the opposite. Maybe it's not that gravity

0:37:21.520 --> 0:37:24.520
<v Speaker 1>pulls things into the black hole and then increases the entropy.

0:37:24.640 --> 0:37:28.239
<v Speaker 1>Maybe it's entropy that's pushing things into black holes, and

0:37:28.280 --> 0:37:31.239
<v Speaker 1>that's actually what gravity is. That's just like you know,

0:37:31.280 --> 0:37:34.440
<v Speaker 1>the way gas diffuses in a box. You put a

0:37:34.440 --> 0:37:36.480
<v Speaker 1>blob of gas in the corner of a box and

0:37:36.520 --> 0:37:40.439
<v Speaker 1>it spreads out into the box. That's entropy the same way.

0:37:40.480 --> 0:37:44.040
<v Speaker 1>Maybe entropy is stuff falling into itself, like you know,

0:37:44.160 --> 0:37:48.400
<v Speaker 1>having more stuff near itself dense blobs of mass increases

0:37:48.440 --> 0:37:51.839
<v Speaker 1>the temperature, which changes the entropy of the situation. I mean,

0:37:51.920 --> 0:37:55.760
<v Speaker 1>it's a complicated argument involving like quantum entangled space time,

0:37:55.800 --> 0:37:57.799
<v Speaker 1>but I think that's the gist of it, and all

0:37:57.840 --> 0:38:00.680
<v Speaker 1>of that kind of crazy idea is just explain how

0:38:00.800 --> 0:38:03.760
<v Speaker 1>maybe gravity could not be one over our square. Yeah,

0:38:03.800 --> 0:38:06.560
<v Speaker 1>if you have in tropic gravity, so maybe if gravity

0:38:06.719 --> 0:38:09.319
<v Speaker 1>is not a fundamental force in the universe but just

0:38:09.400 --> 0:38:13.000
<v Speaker 1>like an emergent property of quantum space time, and you

0:38:13.040 --> 0:38:17.520
<v Speaker 1>have dark energy, then Virlindis theory predicts that space curs

0:38:17.560 --> 0:38:20.800
<v Speaker 1>in this way, that gravity, the effective force of gravity,

0:38:21.120 --> 0:38:24.480
<v Speaker 1>goes the way mind needs it to explain the galactic

0:38:24.560 --> 0:38:28.279
<v Speaker 1>rotation curves. So that's kind of cool thing. That's an

0:38:28.320 --> 0:38:31.239
<v Speaker 1>alternative to dark matter. Is one alternative to dark matter

0:38:31.320 --> 0:38:35.920
<v Speaker 1>to say we have this weird gravitational thermodynamics idea that

0:38:36.000 --> 0:38:39.239
<v Speaker 1>changes the way gravity works. That explains why we thought

0:38:39.320 --> 0:38:42.200
<v Speaker 1>that was missing stuff. Instead, it's just the gravity works

0:38:42.200 --> 0:38:44.759
<v Speaker 1>differently than we expect it. Interesting alright, So then I

0:38:44.760 --> 0:38:47.719
<v Speaker 1>guess the big question is could that work? Is that

0:38:47.840 --> 0:38:52.560
<v Speaker 1>a valid or plausible theory that maybe explains gravity in

0:38:52.560 --> 0:38:56.040
<v Speaker 1>a different way that then explains dark matter and and

0:38:56.200 --> 0:38:59.080
<v Speaker 1>so that it's not just another particle or kind of stuff.

0:38:59.440 --> 0:39:02.040
<v Speaker 1>Could that war? Well, it's a cool idea, and it

0:39:02.080 --> 0:39:06.320
<v Speaker 1>does explain galaxy rotation curves, and it actually explains galaxy

0:39:06.440 --> 0:39:10.399
<v Speaker 1>rotation curves better than dark matter. There's some galaxies out

0:39:10.400 --> 0:39:12.640
<v Speaker 1>there that we still can't explain using dark matter, Like

0:39:12.760 --> 0:39:15.120
<v Speaker 1>they rotate in weird ways and we don't understand it.

0:39:15.160 --> 0:39:20.719
<v Speaker 1>And you know, but hey, galaxies are weird. They they

0:39:20.719 --> 0:39:26.480
<v Speaker 1>have their own history. No prize, sir. My theory, that's right,

0:39:26.600 --> 0:39:29.240
<v Speaker 1>My theory that the universe is just weird explains everything,

0:39:29.320 --> 0:39:32.880
<v Speaker 1>oh man, the whites and theory of everything, the whites

0:39:32.880 --> 0:39:36.400
<v Speaker 1>and theory of weirdness. But it explains the gaxy rotation

0:39:36.440 --> 0:39:40.120
<v Speaker 1>curves really nicely. But there's a big caveat there, which

0:39:40.120 --> 0:39:43.720
<v Speaker 1>is it was sort of invented to explain those curves,

0:39:43.800 --> 0:39:47.840
<v Speaker 1>like you came up with a theory to fit that data. Really,

0:39:47.960 --> 0:39:50.480
<v Speaker 1>a good test of a theory is does it explain

0:39:50.640 --> 0:39:54.440
<v Speaker 1>other data? Is that a real general principle about the universe,

0:39:54.480 --> 0:39:57.000
<v Speaker 1>something which is really deeply true? Or is it just

0:39:57.080 --> 0:39:59.879
<v Speaker 1>a mathematical tweak to this one plot, this one fig

0:40:00.120 --> 0:40:02.160
<v Speaker 1>or to make. Because if it only works to explain

0:40:02.239 --> 0:40:04.840
<v Speaker 1>one thing, it's it's kind of suspicious, right exactly, And

0:40:04.880 --> 0:40:07.440
<v Speaker 1>if it only works to explain the one thing that

0:40:07.520 --> 0:40:10.160
<v Speaker 1>motivated it, and then probably it's not a deep truth

0:40:10.280 --> 0:40:14.440
<v Speaker 1>of the universe, right a right, So maybe it doesn't work.

0:40:14.680 --> 0:40:16.440
<v Speaker 1>Can it explain some of the other things that we

0:40:16.480 --> 0:40:19.880
<v Speaker 1>know about dark matter, like the lensing and the cosmic

0:40:20.040 --> 0:40:24.200
<v Speaker 1>microwave background and the structure of the universe? A tweak

0:40:24.239 --> 0:40:26.800
<v Speaker 1>to our theory of gravity also explain all of these things?

0:40:26.880 --> 0:40:31.040
<v Speaker 1>In a word, No, it just doesn't work. No, galax

0:40:31.080 --> 0:40:33.360
<v Speaker 1>is are just weird. No galax is just weird. No,

0:40:33.480 --> 0:40:36.160
<v Speaker 1>it does not explain the cosmic microwave background, Like, it's

0:40:36.360 --> 0:40:40.520
<v Speaker 1>very difficult to explain that using anything else other than

0:40:40.840 --> 0:40:43.920
<v Speaker 1>some new kind of particle or promodial black hole or

0:40:43.960 --> 0:40:47.080
<v Speaker 1>something some new kind of stuff. You just can't explain

0:40:47.160 --> 0:40:49.160
<v Speaker 1>it using deviation and gravity because it was on a

0:40:49.200 --> 0:40:51.759
<v Speaker 1>really small scale. This is like, you know, things were

0:40:51.840 --> 0:40:55.799
<v Speaker 1>near by each other. This wasn't galactic distances interesting, And

0:40:55.840 --> 0:40:58.360
<v Speaker 1>it's very difficult to explain the structure of the universe.

0:40:58.520 --> 0:41:01.080
<v Speaker 1>And then there is one really awesome example of dark

0:41:01.120 --> 0:41:03.799
<v Speaker 1>matter that's sort of like a smoking gun that makes

0:41:03.800 --> 0:41:07.319
<v Speaker 1>it almost impossible to explain using anything but some new

0:41:07.400 --> 0:41:10.040
<v Speaker 1>kind of matter stuff, some new kind of stuff. Yeah,

0:41:10.280 --> 0:41:14.200
<v Speaker 1>and that's this Bullet cluster. There was this collision millions

0:41:14.200 --> 0:41:17.399
<v Speaker 1>and millions of years ago, far far away between two

0:41:17.480 --> 0:41:20.560
<v Speaker 1>clusters of galaxy that passed through each other. And we

0:41:20.600 --> 0:41:23.479
<v Speaker 1>thought that those clusters of galaxies they had normal matter

0:41:23.640 --> 0:41:26.480
<v Speaker 1>like stars and planets, etcetera, and then also clumps of

0:41:26.560 --> 0:41:29.799
<v Speaker 1>dark matter. So what happened is they passed through each other,

0:41:30.320 --> 0:41:33.280
<v Speaker 1>and the gas and the dust it all collided amid

0:41:33.320 --> 0:41:36.000
<v Speaker 1>big collisions and slowed down and all that stuff. But

0:41:36.080 --> 0:41:38.479
<v Speaker 1>the dark matter, it doesn't interact with the normal matter,

0:41:38.480 --> 0:41:40.520
<v Speaker 1>and it doesn't interact with itself very much at all

0:41:40.600 --> 0:41:43.479
<v Speaker 1>either because gravity is so weak, so the dark matter

0:41:43.520 --> 0:41:45.920
<v Speaker 1>is sort of passed through. So what we see when

0:41:45.920 --> 0:41:47.560
<v Speaker 1>we look up in the skies, we see like a

0:41:47.600 --> 0:41:50.880
<v Speaker 1>big blob in the center while the gas and dust interacted,

0:41:51.120 --> 0:41:53.799
<v Speaker 1>and then on either side we see the dark matter

0:41:53.840 --> 0:41:56.239
<v Speaker 1>that passed through, and we can see that because of

0:41:56.280 --> 0:41:58.640
<v Speaker 1>the gravitational lensing. Right, But doesn't it all I know,

0:41:58.719 --> 0:42:00.960
<v Speaker 1>we talked about the bullet cluster it before, but doesn't

0:42:01.000 --> 0:42:05.279
<v Speaker 1>it still just come down to gravitational lensing, Like what

0:42:05.400 --> 0:42:09.160
<v Speaker 1>if gravity can explain gravitational lensing, could that also explain

0:42:09.600 --> 0:42:12.200
<v Speaker 1>the bullet cluster that we see. It's very difficult to

0:42:12.239 --> 0:42:14.120
<v Speaker 1>explain the bullet cluster in any other way because you

0:42:14.160 --> 0:42:17.360
<v Speaker 1>need to have gravitational lensing in exactly those right spots

0:42:17.640 --> 0:42:21.920
<v Speaker 1>on opposite sides of this very obvious collision. So it's

0:42:21.920 --> 0:42:24.640
<v Speaker 1>a very nice explanation to think, oh, there's some invisible

0:42:24.640 --> 0:42:27.799
<v Speaker 1>matter that passed through and it's now sitting there distorting

0:42:27.800 --> 0:42:30.720
<v Speaker 1>the background galaxy. See, the bullet cluster is like proved

0:42:30.760 --> 0:42:34.920
<v Speaker 1>that whatever it's causing these gravitational things is mobile, like

0:42:35.120 --> 0:42:37.839
<v Speaker 1>it can move like stuff. But if it was just

0:42:37.880 --> 0:42:41.719
<v Speaker 1>a gravitational theory tweak, that wouldn't like keep going or

0:42:41.800 --> 0:42:44.319
<v Speaker 1>move or change from here to there exactly, and it

0:42:44.360 --> 0:42:46.920
<v Speaker 1>can be separated from the normal matter. It's not just

0:42:47.000 --> 0:42:49.760
<v Speaker 1>a gravitational tweak from the normal matter, right, the normal

0:42:49.760 --> 0:42:52.760
<v Speaker 1>matter was left behind in the middle. It's its own

0:42:52.880 --> 0:42:55.799
<v Speaker 1>kind of stuff. It has its own gravity. And so

0:42:55.880 --> 0:42:58.279
<v Speaker 1>that's sort of like a bullet in the brain of

0:42:58.320 --> 0:43:01.720
<v Speaker 1>the you know, non dark matter theories. The bullet cluster

0:43:01.840 --> 0:43:05.880
<v Speaker 1>is a bullet suspicious. People really took Moms sort of

0:43:05.960 --> 0:43:09.240
<v Speaker 1>seriously until then. And then when the bullet cluster was discovered,

0:43:09.280 --> 0:43:12.200
<v Speaker 1>people are like, oh, well, that's it. Dark matter is real,

0:43:12.640 --> 0:43:16.640
<v Speaker 1>and Mond is dead and never Mond. And at that

0:43:16.680 --> 0:43:20.040
<v Speaker 1>point people really didn't take months seriously. So since then,

0:43:20.480 --> 0:43:23.399
<v Speaker 1>Mond has been much more of a fringe theory. I mean,

0:43:23.680 --> 0:43:26.160
<v Speaker 1>Virlin's idea is more recent, and it's quote of cool,

0:43:26.480 --> 0:43:28.960
<v Speaker 1>but it sort of explains something that nobody really takes

0:43:29.000 --> 0:43:32.239
<v Speaker 1>seriously anymore. So it's very fringe in a way. The

0:43:32.280 --> 0:43:35.359
<v Speaker 1>bullet cluster shows you that dark matter or whatever it's

0:43:35.400 --> 0:43:39.640
<v Speaker 1>causing these gravitational distortions and footprints, is mobile like it's

0:43:39.760 --> 0:43:41.880
<v Speaker 1>it can move like stuff. It moves like a stuff

0:43:41.920 --> 0:43:45.880
<v Speaker 1>can move. Yeah, And so again it's unsatisfying because we

0:43:45.920 --> 0:43:48.360
<v Speaker 1>don't know what it is and and we've been looking

0:43:48.360 --> 0:43:50.480
<v Speaker 1>for for a while it's not like we're just like, oh,

0:43:50.520 --> 0:43:54.320
<v Speaker 1>it's some invisible stuff, let's move on. We've built dedicated

0:43:54.360 --> 0:43:57.239
<v Speaker 1>experiments to look for it. We thought several times that

0:43:57.360 --> 0:43:59.839
<v Speaker 1>we would definitely find it and then haven't seen it.

0:44:00.200 --> 0:44:02.359
<v Speaker 1>So there's definitely some tension there. It's not like dark

0:44:02.400 --> 0:44:04.839
<v Speaker 1>matter is a beautiful theory that's all wrapped up, like

0:44:05.160 --> 0:44:08.120
<v Speaker 1>we don't understand why we haven't been able to find

0:44:08.160 --> 0:44:11.680
<v Speaker 1>the dark matter yet. There's definitely something weird going on there,

0:44:11.840 --> 0:44:14.279
<v Speaker 1>and it's very healthy to think about new ideas, but

0:44:14.480 --> 0:44:18.000
<v Speaker 1>mond doesn't quite work. There is no other idea out

0:44:18.080 --> 0:44:21.440
<v Speaker 1>there that explains what we see nearly as well as

0:44:21.520 --> 0:44:24.480
<v Speaker 1>some new cold particles. I have an idea is it's

0:44:24.480 --> 0:44:27.840
<v Speaker 1>snack based. It's called Hey, maybe dark matter is weird.

0:44:29.880 --> 0:44:32.640
<v Speaker 1>It's weird, yeah, And that's why people are sort of

0:44:32.680 --> 0:44:35.200
<v Speaker 1>digging further and further into the barrel of ideas for

0:44:35.280 --> 0:44:37.520
<v Speaker 1>dark matter. People thought for a long time, Okay, dark

0:44:37.560 --> 0:44:41.319
<v Speaker 1>matter must just be some weakly interacting massive particle, some

0:44:41.400 --> 0:44:44.360
<v Speaker 1>new lava stuff, but we haven't seen it, and so

0:44:44.400 --> 0:44:47.000
<v Speaker 1>then people are well, maybe it's axions, or maybe it's

0:44:47.080 --> 0:44:49.919
<v Speaker 1>primordial black holes, or and there are some other even

0:44:50.080 --> 0:44:55.440
<v Speaker 1>crazier ideas like squirmyons, what like they're uncomfortable and social situations.

0:44:55.520 --> 0:45:00.239
<v Speaker 1>What do you mean introvertons? Yeah, no, squirmy on are

0:45:00.280 --> 0:45:03.279
<v Speaker 1>this crazy idea that you know how particles are like

0:45:03.440 --> 0:45:06.800
<v Speaker 1>excitations of quantum fields are like little bundles of energy

0:45:06.800 --> 0:45:09.960
<v Speaker 1>in a quantum field. People think, well, maybe not all

0:45:10.120 --> 0:45:12.480
<v Speaker 1>energy and quantum fields are particles. Maybe some of them

0:45:12.520 --> 0:45:15.760
<v Speaker 1>are like more distributed or spread out in weird ways.

0:45:15.760 --> 0:45:18.640
<v Speaker 1>And they found that you can like tangle up quantum

0:45:18.680 --> 0:45:21.520
<v Speaker 1>fields in these weird ways, like make nots of them,

0:45:21.800 --> 0:45:24.439
<v Speaker 1>and that's what they call squirmyons. And it's not could

0:45:24.480 --> 0:45:27.880
<v Speaker 1>like it could create gravity. Yeah, because any energy density

0:45:27.920 --> 0:45:32.040
<v Speaker 1>creates gravity. Well, we'll have to dig into that for

0:45:32.120 --> 0:45:36.680
<v Speaker 1>another episode. Sounds pretty for sure. So there's lots of

0:45:36.680 --> 0:45:38.799
<v Speaker 1>ideas the whole spectrum, right, dark matter is not just

0:45:38.960 --> 0:45:42.799
<v Speaker 1>one idea, the sort of spectrum of ideas all satisfied

0:45:42.840 --> 0:45:45.920
<v Speaker 1>the condition that it's some new kind of cold object.

0:45:46.400 --> 0:45:48.680
<v Speaker 1>But what that object is. It could be one particle,

0:45:48.719 --> 0:45:51.880
<v Speaker 1>could be many kinds of particles. It could be black holes,

0:45:51.960 --> 0:45:54.279
<v Speaker 1>it could be squirmyons, it could be something else we

0:45:54.320 --> 0:45:57.240
<v Speaker 1>haven't even thought of yet. Whatever, it is. We're pretty

0:45:57.280 --> 0:46:00.160
<v Speaker 1>sure it's stuff. It's something that has gravity stuff when

0:46:00.160 --> 0:46:02.400
<v Speaker 1>it's there, that's right. But I mean it's really interesting

0:46:02.440 --> 0:46:04.440
<v Speaker 1>because I feel like we've known dark matters is there

0:46:04.480 --> 0:46:06.279
<v Speaker 1>for a while now, and we just can't seem to

0:46:06.280 --> 0:46:08.200
<v Speaker 1>crack it. We can't seem to find it keeps um

0:46:08.200 --> 0:46:11.160
<v Speaker 1>eluding us, you know, like it just keeps on hiding

0:46:11.200 --> 0:46:13.799
<v Speaker 1>there and not letting us know what it is. That's right,

0:46:13.840 --> 0:46:15.440
<v Speaker 1>But we don't know how long the story is. You know,

0:46:15.480 --> 0:46:17.880
<v Speaker 1>we were looking for the Higgs boson for fifty years

0:46:18.000 --> 0:46:20.319
<v Speaker 1>and then we found it. We were looking for the

0:46:20.360 --> 0:46:23.040
<v Speaker 1>top cork for twenty years before we found it. A

0:46:23.040 --> 0:46:25.000
<v Speaker 1>lot of those things. People thought, oh, we'll find this

0:46:25.040 --> 0:46:27.400
<v Speaker 1>in the next year two and then they were confused

0:46:27.400 --> 0:46:29.680
<v Speaker 1>and disappointed to not discover it soon. But you know,

0:46:29.760 --> 0:46:32.239
<v Speaker 1>eventually we got there and we we figured it out.

0:46:32.280 --> 0:46:35.359
<v Speaker 1>So maybe we're just five years away from discovering dark matter,

0:46:35.440 --> 0:46:37.400
<v Speaker 1>or maybe it's going to be another hundred. Maybe we

0:46:37.440 --> 0:46:40.000
<v Speaker 1>need a new crazy idea for what dark matter is.

0:46:40.040 --> 0:46:43.359
<v Speaker 1>But dark matter, I'm pretty sure is so all those

0:46:43.400 --> 0:46:47.800
<v Speaker 1>physicists squirming around relax. Maybe dark matter is in our future.

0:46:47.880 --> 0:46:50.239
<v Speaker 1>That's right. I certainly hope it is. It would be fascinating.

0:46:50.280 --> 0:46:52.879
<v Speaker 1>And remember that it's most of the stuff out there

0:46:52.880 --> 0:46:56.319
<v Speaker 1>in the universe. Like, what a crazy opportunity to learn

0:46:56.360 --> 0:46:59.040
<v Speaker 1>about the way the universe works, you know, to know

0:46:59.120 --> 0:47:01.359
<v Speaker 1>that of the stuff out there in the universe has

0:47:01.400 --> 0:47:03.840
<v Speaker 1>been hidden from us. The day we crack that open

0:47:03.920 --> 0:47:05.759
<v Speaker 1>and get to learn about it, like, it could have

0:47:05.800 --> 0:47:09.719
<v Speaker 1>incredibly complex structure, it could have interactions and biology and

0:47:09.800 --> 0:47:12.600
<v Speaker 1>chemistry and all sorts of crazy stuff. Movest of the

0:47:12.600 --> 0:47:14.960
<v Speaker 1>stuff out there in the universe we haven't yet gotten

0:47:14.960 --> 0:47:17.640
<v Speaker 1>to play with, and so we're eager, we're desperate to

0:47:17.680 --> 0:47:19.600
<v Speaker 1>figure out what this stuff is. Yeah, because if you're

0:47:19.600 --> 0:47:22.200
<v Speaker 1>the scientist that discovers what dark matter is, I mean,

0:47:22.320 --> 0:47:25.399
<v Speaker 1>that's like a lot of three cred you know. It's

0:47:25.440 --> 0:47:29.360
<v Speaker 1>like you could say that you discovered eight eight percent

0:47:29.440 --> 0:47:31.440
<v Speaker 1>of everything in the universe. I think they would have

0:47:31.480 --> 0:47:33.719
<v Speaker 1>to give you five Nobel Prizes, you know, just for

0:47:33.719 --> 0:47:35.840
<v Speaker 1>that one discovery. They have to give you eighty percent

0:47:35.880 --> 0:47:38.600
<v Speaker 1>of all the Nobel prizes. I think, Yeah, yeah, there

0:47:38.600 --> 0:47:40.719
<v Speaker 1>you go. You get all the Nobel Prizes for the

0:47:40.719 --> 0:47:43.560
<v Speaker 1>next four hundred years, just to balance it out. Yeah,

0:47:43.640 --> 0:47:45.560
<v Speaker 1>So it's a big question, and who knows, maybe one

0:47:45.600 --> 0:47:48.279
<v Speaker 1>of our listeners will be the one who discovers it.

0:47:48.360 --> 0:47:49.879
<v Speaker 1>That's right, It could be you out there, it could

0:47:49.880 --> 0:47:51.960
<v Speaker 1>be your kids out there. What we definitely need to

0:47:51.960 --> 0:47:53.759
<v Speaker 1>do or keep our minds open and come up with

0:47:53.800 --> 0:47:57.000
<v Speaker 1>new ideas for what dark matter is really cool? All right, Well,

0:47:57.320 --> 0:48:00.440
<v Speaker 1>we hope you enjoyed that view into this story is

0:48:00.520 --> 0:48:02.520
<v Speaker 1>dark matter and how we know it's there and how

0:48:02.680 --> 0:48:06.640
<v Speaker 1>we know it's not just a weird fluke of gravitational equations.

0:48:06.800 --> 0:48:17.200
<v Speaker 1>Thanks for tuning in, See you next time. Thanks for listening,

0:48:17.280 --> 0:48:20.000
<v Speaker 1>and remember that Daniel and Jorge Explain the Universe is

0:48:20.000 --> 0:48:23.440
<v Speaker 1>a production of I Heart Radio. For more podcast For

0:48:23.520 --> 0:48:27.279
<v Speaker 1>my heart Radio, visit the i heart Radio app, Apple Podcasts,

0:48:27.400 --> 0:48:29.760
<v Speaker 1>or wherever you listen to your favorite shows.