WEBVTT

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Okay, so welcome to the deep dive everybody.

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Today we are going to be tackling. Sounds fun.

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A really interesting topic that I think a lot

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of people are probably familiar with to some

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degree. But hopefully we'll be able to cover

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it in a new and exciting way today. All right.

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So that is the topic. Of dark matter and dark

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energy. Okay. And for people who aren't already

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aware, this stuff basically makes up. 95 % of

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the universe. Wow. Which is kind of a crazy thing

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to think about. That's a lot we don't know, then.

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It is. So everything that we can see, the stars,

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the planets, the galaxies, all the stuff that

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we're made of, makes up a measly 5%. Really,

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just 5 %? Of the known universe. Wow. So, yeah.

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Kind of crazy. That's more than a little humbling,

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isn't it? It is it is to think everything we've

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ever observed is just a tiny fraction Yeah, and

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it really puts into perspective Just how much

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we still don't know exactly and how much there

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still is out there to learn So I guess you could

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say that we're kind of like explorers going on

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this journey together Okay, like that to make

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sense of these really mind -bending ideas. Yeah,

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let's dive in. We'll do our best to kind of Explain

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them in a way that Hopefully is approachable.

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Yeah and easy to understand but yeah, it's gonna

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be a wild ride I think it's incredible that 95

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% isn't just empty space. It's not like we're

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missing a few puzzle pieces here It's this huge

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unknown presence that's actually shaping the

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universe. Yeah. Yeah, that has a real effect

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Yeah on the things that we can see absolutely

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and that's what makes it so fascinating to study

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exactly So when we talk about dark matter You

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know, we're talking about this really elusive

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thing. You could almost think of it as like the

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universe's shy, introverted cousin. OK. You know,

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it barely interacts with anything. It's like

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the cosmic wallflower. Exactly. You know, it

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doesn't even interact with light. That's why

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it's so hard to even detect. Yeah, that's why

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we can't see it. So let's unpack how we even

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got to the point of knowing that this stuff exists.

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Yeah. How did we figure out something was there

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if we can't see it? Right. So the first clues

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for dark matter actually came from astronomers

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looking at how galaxies spin. Galaxy spin. Yeah.

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So think about our solar system. All right. So

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you have the sun at the center. Right. And then

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the planets orbit around it and the planets further

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away from the sun orbit much slower. That makes

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sense. The sun's gravity is weaker further out.

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Exactly. And that's because the force of gravity

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decreases. with distance. Right, so it's a most

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predictable system. Right, it's like a cosmic

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ballet. Exactly, and so scientists initially

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thought that the same would apply to stars within

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galaxies. Stars closer to the center would be

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zipping around much faster than those further

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out. That makes sense, yeah, because the center

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of the galaxy would have the strongest gravitational

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pull. Right, all that mass concentrated in the

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middle. Right, then they started looking at these...

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distant spiral galaxies. Okay. And they found

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something really weird. What was that? The stars

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at the edges of the galaxies were moving way

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faster than they should have been based on the

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amount of visible matter that was there. So like

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the visible stars and gas weren't enough to explain

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those speeds. Exactly. It was almost as if there

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was way more mass. Holding those galaxies together

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interesting. So like there was some invisible

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source of gravity right then what we could actually

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see that's wild and so this mismatch between

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The observed spees the stars and the amount of

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visible matter was a really strong indication

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That there had to be some kind of invisible matter

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that was providing this extra gravitational pull

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dark matter. Yeah dark matter It's like imagine

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a figure skater spinning really fast. Okay. You

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know, like so fast that their arms should just

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fly off. Yeah. But something invisible is keeping

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them glued on. I like that analogy. It really

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captures the idea. So that invisible force is

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like the dark matter. And it's not just preventing

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galaxies from flying apart. Right. It also played

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a key role in how galaxies formed in the first

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place. Okay, so we know it's there because of

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its effects. Yeah. But the big question is...

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What is it? What is this stuff? So scientists

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have come up with all sorts of different theories.

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about what dark matter could be. And one of the

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most popular ones for a long time has been the

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idea of... Weekly Interacting Massive Particles.

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Weekly Interacting Massive Particles. Which is

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a mouthful. It is, but luckily we have the acronym...

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Soap Knees. Wings. And the name kind of gives

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you some hints about what scientists thought

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these things might be. I break it down for me.

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So massive implies that they have a lot of mass.

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OK, that makes sense. Massive things have a lot

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of mass. Right. And in fact, the source material

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actually mentions that they could have masses

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of several to V. Several to V, that's pretty

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heavy. Yeah. So for anyone who's not a particle

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physicist, which is probably most of us, can

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you put that into perspective? Sure. So a TeV

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is a tera electron volt, which is a unit of energy.

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But in particle physics, we often use it to describe

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mass because of that famous equation, EMCO. Right.

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Energy and mass are basically two sides of the

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same coin. Exactly. So to put that into perspective,

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a proton, which is one of the particles that

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makes up an atom's nucleus, has a mass of about

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one GV or giga electron volt. Okay. So a Tevi

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is a thousand times larger than that. So we're

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talking about particles that are potentially...

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thousands of times more massive than a proton.

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That's right. These are heavy hitters in the

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particle world. Wow. And because they are so

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massive, it's thought that they wouldn't be zipping

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around at the speed of light. OK. Instead, they'd

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be moving much slower, what we call cold dark

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matter. Cold dark matter. Yeah. So their average

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speed would be well below the speed of light.

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And why is that important, the speed? I mean.

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Well, it turns out that the speed of dark matter

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particles would have had a major impact on how

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galaxies formed. Oh, really? Yeah. If they were

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moving too fast, they wouldn't clump together

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gravitationally. OK. And they wouldn't be able

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to provide the scaffolding for galaxies to form.

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Oh, I see. They need to be slow enough to kind

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of hang out in one place and exert their gravitational

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influence. Like the cosmic glue that holds everything

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together. Exactly. OK. So we've got massive.

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Let's talk about the weakly interacting part.

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Right. Because that's the other half of the name.

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Right. So this means that they're predicted to

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only interact with other matter. through the

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weak nuclear force. The weak nuclear force. Okay,

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so that's one of the four fundamental forces

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of nature. Right. But as the name suggests, it's

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very weak. And it only acts over extremely short

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distances. Yeah, it's kind of like the shy introvert

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of the force world. So because of this, the chances

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of a wimp actually interacting with a regular

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particle are incredibly low. Yeah, like astronomically

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low. Which makes them... extremely difficult

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to detect. Is it trying to find a needle in a

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cosmic haystack? Yeah, and WIMP, the source mentions

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that WIMPs are predicted to exist in theories

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like supersymmetry and extra dimensions. Right,

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so those are some pretty mind -bending concepts.

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Yeah, so for those of us who aren't theoretical

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physicists, can you kind of give us a simplified

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explanation of what those are? Sure, so supersymmetry

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is essentially a theory that proposes that. For

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every known particle in the universe, there's

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a corresponding partner particle. OK, like a

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mirror image. Exactly. And some of these hypothetical

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partner particles could have the properties of

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WIMPs. So it's like a whole new set of particles

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that we haven't discovered yet. Right, and extra

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dimensions is the idea that our universe might

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have more than the three spatial dimensions that

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we're familiar with. Right, length, width, and

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height. Exactly. So imagine like a fourth spatial

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dimension. that we can't perceive directly. And

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these extra dimensions could contain particles

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that behave like dark matter? OK, so it's like

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there's this whole hidden realm that we can't

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see. Kind of like a shadow universe. Where dark

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matter might be hanging out. Yeah, it's a fascinating

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idea. It is. So there have been a lot of experiments

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to try and detect WIMPs. One of those famous

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ones was the Large Underground Xenon Detector,

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or LUX. LUX, yeah, I've heard of that one. And

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this thing was built deep underground. Why underground?

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To shield it from all the other radiation. Oh,

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that makes sense. You don't want interference

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from other particles. Right, you want to make

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sure that if you detect something, it's actually

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a wimp, and not just some other random particle.

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Smart. So they ran this experiment for several

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years, but unfortunately, they didn't find...

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any conclusive evidence of wimps. Oh, that's

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a shame. It is. But the search continues with

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even more sensitive experiments being planned.

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That's the spirit of science. Never give up.

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Exactly. So wimps are still a possibility, but

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the jury's still out. Fair enough. So let's move

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on to another popular dark matter candidate.

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OK. And that is axions. Axions, all right. And

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these are very different from wimps. How so?

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Well, for starters, they're predicted to be incredibly

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light. Okay, so instead of massive, we have super

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light. Right. The source mentions that they could

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have masses on the order of microelectron volts.

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Microelectron volts? Wow, that's tiny! Yeah,

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so compared to wimps, they're like feathers.

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So what about their interactions? Are they also

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weakly interacting? Even more so. Axions are

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not predicted to interact through the electromagnetic

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force. Yeah. Or the strong nuclear force. So

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they're practically invisible to us, then. Yeah.

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And not affected by the force that holds atomic

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nuclei together. Right. So they're incredibly

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difficult to detect. So if they're so light and

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barely interact with anything, how could they

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possibly be dark matter? Well, that's a good

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question. And it turns out that they're very

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weak interactions. Yeah. And incredibly light

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mass actually make them very stable. Stable?

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Yeah. They could essentially exist. Yeah. for

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the entire age of the universe. OK, so they're

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like the cosmic Methuselahs of particles. Exactly.

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And that fits in really nicely with the fact

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that we know dark matter has been around for

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billions of years. That makes sense. And despite

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the challenges, there are actually experiments

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trying to detect axions. Oh, wow, really? Yeah,

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like the ADMX experiment. ADMX, what does that

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stand for? It stands for the Axion Dark Matter

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Experiment. Catchy. And there's also the Casper

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experiment. Casper? OK. I don't even want to

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know what that stands for. Yeah, it's a bit of

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a mouthful. But basically, these experiments

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are trying to observe the really subtle effects

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that axions might have on things like electromagnetism

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and the spins of atomic nuclei. So it's like

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they're looking for the faintest whisper against

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the roar of the universe. Exactly. It's a really

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difficult thing to do. I bet. OK, so we've talked

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about massive and weakly interacting particles.

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Limpies. We've talked about. super light, and

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even more weakly interacting particles. Axions.

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So what's next? Well, there's another interesting

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candidate, sterile neutrinos. Sterile neutrinos.

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OK, so we already know that neutrinos exist.

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Right, those tiny little ghosts of the particle

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world. Yeah, they're these incredibly tiny particles

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that interact through the weak nuclear force.

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and they're incredibly difficult to detect. But

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we have managed to detect them, right? We have,

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with these massive underground detectors. Yeah,

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those huge golden chamber detectors that look

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like something out of a sci -fi movie. Right,

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so how are sterile neutrinos different? Well,

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the key difference is that they're theorized

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to interact solely through gravity. Just gravity?

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Yeah, no weak force, no electromagnetic force,

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nothing else. Wow, so they're even more isolated

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than whips. True cosmic loners. Yeah, it's like

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they're practically ghosts. So how could we ever

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hope to find something that only interacts through

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gravity? Ah, that's a great question. And the

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truth is, it would be incredibly difficult. But

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the source does mention a couple of possible

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detection methods. One is by looking for x -ray

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emissions from galaxy clusters, which might be

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produced if sterile neutrinos decay. Interesting.

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And another possibility is to search for subtle

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imprints they might have left. on the cosmic

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microwave background radiation. The CMB. Exactly

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that afterglow of the Big Bang. So it's like,

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we're trying to look for the faintest shadows

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that they might have cast on the universe. Pretty

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much. But as with all these candidates, we haven't

00:12:24.740 --> 00:12:28.440
actually found any direct evidence of their existence.

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So for now, they remain hypothetical. OK, so

00:12:31.600 --> 00:12:33.519
moving on, we have another interesting idea,

00:12:33.639 --> 00:12:37.879
and that is dark photons. Dark photons. So. Are

00:12:37.879 --> 00:12:41.159
these like regular photons? The dark. That's

00:12:41.159 --> 00:12:44.059
a good way to think about it. Ah. But instead

00:12:44.059 --> 00:12:47.200
of carrying the electromagnetic force, they would

00:12:47.200 --> 00:12:50.679
carry a new fundamental force. OK. A dark force,

00:12:50.720 --> 00:12:53.059
if you will. A dark force. That would only interact

00:12:53.059 --> 00:12:55.980
between dark matter particles. OK. It's like

00:12:55.980 --> 00:12:59.570
dark matter has its own. separate communication

00:12:59.570 --> 00:13:01.789
network. You got it. That we're not privy to.

00:13:02.309 --> 00:13:05.429
Exactly. Interesting. So if dark matter is made

00:13:05.429 --> 00:13:07.909
up of particles that can talk to each other through

00:13:07.909 --> 00:13:10.850
this dark force, it could potentially explain

00:13:10.850 --> 00:13:13.710
some of the things we observe about its distribution

00:13:13.710 --> 00:13:16.350
in the universe. Like what? Well for example,

00:13:16.809 --> 00:13:19.389
the distribution of dark matter in dwarf galaxies

00:13:19.389 --> 00:13:22.669
doesn't quite match. what our simulations predict.

00:13:23.470 --> 00:13:25.470
If dark matter particles were only interacting

00:13:25.470 --> 00:13:28.169
through gravity, we'd expect to see a much denser

00:13:28.169 --> 00:13:30.309
concentration of dark matter in the centers of

00:13:30.309 --> 00:13:32.590
these galaxies. But that's not what we observe.

00:13:32.649 --> 00:13:35.250
So the dark force could smooth things out a bit.

00:13:35.789 --> 00:13:38.330
Exactly. If these particles can interact with

00:13:38.330 --> 00:13:40.549
each other through this dark force, it could

00:13:40.549 --> 00:13:43.289
lead to a more even distribution of dark matter.

00:13:43.590 --> 00:13:46.649
And the source mentions that. These dark photons

00:13:46.649 --> 00:13:50.629
might even be able to mix. with regular photons.

00:13:50.789 --> 00:13:54.129
Mix. Yeah. It's a theoretical possibility. And

00:13:54.129 --> 00:13:56.629
if it happens, it could lead to some really subtle

00:13:56.629 --> 00:13:59.549
signals that we might be able to detect. OK,

00:13:59.549 --> 00:14:01.289
so that would be a way of indirectly detecting

00:14:01.289 --> 00:14:04.690
them. Exactly. But so far, no such luck. OK,

00:14:04.690 --> 00:14:07.429
so no evidence yet. Not yet, but the search continues.

00:14:07.669 --> 00:14:10.529
So we've gone through this whole list of potential

00:14:10.529 --> 00:14:14.309
dark matter particles. But what if dark matter

00:14:14.309 --> 00:14:16.509
isn't a particle at all? Now you're talking.

00:14:16.590 --> 00:14:20.019
Yeah. And that brings us to the idea of emergent

00:14:20.019 --> 00:14:22.080
gravity. Emergent gravity, that sounds pretty

00:14:22.080 --> 00:14:24.659
radical. It is. It's a completely different way

00:14:24.659 --> 00:14:27.259
of thinking about dark matter. All right. I'm

00:14:27.259 --> 00:14:29.360
intrigued. Lay it on me. So instead of saying

00:14:29.360 --> 00:14:34.039
that there's this new type of particle that we

00:14:34.039 --> 00:14:37.100
haven't discovered yet, emergent gravity proposes.

00:14:37.940 --> 00:14:40.840
That gravity itself isn't what we think it is.

00:14:40.980 --> 00:14:43.279
Whoa, hold on. You're saying gravity isn't fundamental.

00:14:43.580 --> 00:14:46.100
Well. Not in the way we currently understand

00:14:46.100 --> 00:14:48.039
it. Emergent gravity suggests that. Gravity might

00:14:48.039 --> 00:14:50.620
actually emerge from a more fundamental phenomenon.

00:14:50.659 --> 00:14:53.440
And what phenomenon would that be? Quantum entanglement.

00:14:53.639 --> 00:14:55.779
Quantum entanglement, you mean that spoopy action

00:14:55.779 --> 00:14:58.120
at a distance? The one and only. So as you know,

00:14:58.620 --> 00:15:01.960
quantum entanglement is this really strange connection

00:15:01.960 --> 00:15:05.539
where two particles become linked no matter how

00:15:05.539 --> 00:15:07.179
far apart they are. Right, it's like they're

00:15:07.179 --> 00:15:10.059
communicating instantaneously even across vast

00:15:10.059 --> 00:15:13.860
distances. And so the idea with emergent gravity

00:15:14.220 --> 00:15:18.139
is that the effects that we attribute to dark

00:15:18.139 --> 00:15:20.799
matter, like the faster than expected rotation

00:15:20.799 --> 00:15:24.470
of galaxies, might actually be caused by... this

00:15:24.470 --> 00:15:28.490
intricate web of quantum entanglement that permeates

00:15:28.490 --> 00:15:30.750
the universe. So it's like gravity is an emergent

00:15:30.750 --> 00:15:33.590
property of this underlying quantum entanglement.

00:15:33.789 --> 00:15:36.450
Exactly. It's a really mind -blowing concept.

00:15:36.730 --> 00:15:38.629
It really challenges our understanding of what

00:15:38.629 --> 00:15:40.750
gravity is. Yeah, and it's important to point

00:15:40.750 --> 00:15:44.230
out that this is still a very theoretical idea.

00:15:44.509 --> 00:15:47.559
There's no direct experimental evidence. to support

00:15:47.559 --> 00:15:49.919
it yet but it's a fascinating possibility it

00:15:49.919 --> 00:15:51.980
is okay so we've covered a lot of ground we have

00:15:51.980 --> 00:15:54.039
on dark matter now let's shift gears okay talk

00:15:54.039 --> 00:15:57.139
about the other big mysterious component hmm

00:15:57.139 --> 00:16:01.200
of the universe dark energy dark energy the cosmic

00:16:01.200 --> 00:16:04.580
accelerator yeah so this is the force that's

00:16:04.580 --> 00:16:07.159
thought to be responsible for the accelerating

00:16:07.159 --> 00:16:09.740
expansion of the universe. Right. So for billions

00:16:09.740 --> 00:16:11.840
of years, the universe has been expanding. Since

00:16:11.840 --> 00:16:14.120
the Big Bang. Exactly. Right. And if gravity

00:16:14.120 --> 00:16:16.919
was the only force at play, we'd expect that

00:16:16.919 --> 00:16:19.440
expansion to slow down. Right. Because gravity

00:16:19.440 --> 00:16:23.379
pulls things together. But in the late 1990s,

00:16:23.799 --> 00:16:26.059
astronomers made a shocking discovery. What was

00:16:26.059 --> 00:16:28.279
that? The expansion of the universe wasn't slowing

00:16:28.279 --> 00:16:30.879
down. It was speeding up. Speeding up. Yeah,

00:16:30.879 --> 00:16:32.879
like someone had stepped on the cosmic gas pedal.

00:16:33.179 --> 00:16:35.960
OK, so what could possibly be causing that? Well,

00:16:35.960 --> 00:16:38.480
that's the million dollar question. And the leading

00:16:38.480 --> 00:16:41.620
explanation is dark energy. Dark energy. It's

00:16:41.620 --> 00:16:44.600
mysterious force that's pushing everything apart.

00:16:44.720 --> 00:16:46.820
And it's not just pushing things apart. It's

00:16:46.820 --> 00:16:49.659
pushing them apart at an accelerating rate. Right.

00:16:49.679 --> 00:16:51.700
So the expansion is getting faster and faster.

00:16:51.940 --> 00:16:55.659
OK. So what are some of the leading theories

00:16:55.659 --> 00:16:59.360
about what dark energy could be? All right. Well,

00:16:59.399 --> 00:17:02.779
one of the simplest explanations. is the cosmological

00:17:02.779 --> 00:17:06.519
constant. And this idea actually goes all the

00:17:06.519 --> 00:17:09.380
way back to Einstein. Oh, wow. Yeah, he originally

00:17:09.380 --> 00:17:12.240
introduced it as a way to keep the universe static.

00:17:12.480 --> 00:17:15.269
Static? Because back then, people thought the

00:17:15.269 --> 00:17:17.309
universe was eternal and unchanging. Right, the

00:17:17.309 --> 00:17:19.769
steady state model. But later when it was discovered

00:17:19.769 --> 00:17:22.190
that the universe was actually expanding, he

00:17:22.190 --> 00:17:24.670
abandoned the cosmological constant, calling

00:17:24.670 --> 00:17:26.930
it his biggest blunder. Oh, the irony. Right.

00:17:27.150 --> 00:17:29.309
But now the cosmological constant is back. And

00:17:29.309 --> 00:17:32.390
it's being used to explain the accelerating expansion.

00:17:32.549 --> 00:17:35.269
Exactly. So what is it exactly? It's basically

00:17:35.269 --> 00:17:39.369
the idea that empty space itself has energy.

00:17:39.480 --> 00:17:42.119
Empty space having energy, that's pretty mind

00:17:42.119 --> 00:17:45.220
-blowing. Yeah, and this energy is thought to

00:17:45.220 --> 00:17:47.140
have a negative pressure. Negative pressure.

00:17:47.140 --> 00:17:50.720
What does that mean? Well, it means that instead

00:17:50.720 --> 00:17:53.380
of pulling things together, like gravity does,

00:17:53.700 --> 00:17:56.799
it pushes them apart. Oh, I see. And so this

00:17:56.799 --> 00:18:00.019
energy of empty space is what's thought to be

00:18:00.019 --> 00:18:02.720
driving the accelerating expansion. OK, but where

00:18:02.720 --> 00:18:06.240
does this energy come from? Well, that's where

00:18:06.240 --> 00:18:07.940
things get a little tricky. One way to think

00:18:07.940 --> 00:18:10.599
about it. Is in terms of quantum fluctuations

00:18:10.599 --> 00:18:13.539
quantum fluctuations. So in the quantum world

00:18:13.539 --> 00:18:16.279
Empty space. It's actually empty. It's full of

00:18:16.279 --> 00:18:20.279
these Virtual particles that are constantly popping

00:18:20.279 --> 00:18:23.140
into and out of existence So like a constant

00:18:23.140 --> 00:18:25.759
sea of particles being created and destroyed

00:18:25.759 --> 00:18:28.640
exactly and these particles Have energy. Okay,

00:18:28.640 --> 00:18:30.299
so that's the source of the energy. Yeah, and

00:18:30.299 --> 00:18:32.859
so the energy associated with these quantum fluctuations

00:18:32.859 --> 00:18:37.609
Is what's thought to contribute? To the cosmological

00:18:37.609 --> 00:18:39.849
constant that makes sense, but there's a problem

00:18:39.849 --> 00:18:43.329
a problem. What is it a big one? Oh when physicists

00:18:43.329 --> 00:18:46.710
try to calculate The value of the cosmological

00:18:46.710 --> 00:18:49.569
constant based on quantum field theory they get

00:18:49.569 --> 00:18:52.009
an answer. That's way too big way too big How

00:18:52.009 --> 00:18:54.369
big are you talking? We're talking 120 orders

00:18:54.369 --> 00:18:57.109
of magnitude 120 orders magnitude. That's a one

00:18:57.109 --> 00:18:59.890
with 120 zeros after it Yeah, so it's like trying

00:18:59.890 --> 00:19:03.490
to measure the distance to the moon and being

00:19:03.490 --> 00:19:07.089
off by the size of the entire solar system. Wow,

00:19:07.130 --> 00:19:09.170
that's not just a little off that's astronomically

00:19:09.170 --> 00:19:11.829
off. It is. And so this is a huge problem for

00:19:11.829 --> 00:19:14.410
the cosmological constant idea. Yeah, it's a

00:19:14.410 --> 00:19:18.109
major discrepancy. Because it suggests that there's

00:19:18.109 --> 00:19:20.650
something fundamental that we're missing. About

00:19:20.650 --> 00:19:23.009
how quantum mechanics and gravity work together.

00:19:23.190 --> 00:19:26.289
Exactly. So while the cosmological constant is

00:19:26.289 --> 00:19:29.390
the simplest explanation for dark energy, it

00:19:29.390 --> 00:19:31.809
also comes with this huge baggage. Yeah, a lot

00:19:31.809 --> 00:19:33.130
of unanswered questions.
