WEBVTT - Smashing Particles for Science

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<v Speaker 1>Brought to you by Toyota. Let's go places. Welcome to

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<v Speaker 1>Forward Thinking, Either and welcome to Forward Thinking, the podcast

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<v Speaker 1>that looks at the future and says he's going for speed.

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<v Speaker 1>I'm Jonathan Strickland. That was a good one. I'm Joe McCormick,

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<v Speaker 1>and Lauren Vogelbaum. Our other host is not with us today,

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<v Speaker 1>but she will be back with us soon. Yeah. So

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<v Speaker 1>we thought we would take this opportunity to talk about, uh,

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<v Speaker 1>you know, some stuff that helps us really get a

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<v Speaker 1>grip on what's really going on out there. Yeah. Um,

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<v Speaker 1>so I saw the movie Transformers for so sorry. Yeah,

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<v Speaker 1>I'm sorry to I'm sorry. I gave those people my money,

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<v Speaker 1>and I'm I'm I'm sorry for the world. Yeah, we're

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<v Speaker 1>we're all victims here. But one thing it got me

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<v Speaker 1>thinking about, since a lot of the movie was taken

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<v Speaker 1>up by things crashing into each other, really big things,

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<v Speaker 1>really big robotic things with laser swords and stuff like that.

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<v Speaker 1>As as you as you do crashing into each other,

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<v Speaker 1>what happens when small things crash into each other, Well,

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<v Speaker 1>then we can get a glimpse of how the universe works. Joe, Yeah, okay,

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<v Speaker 1>So here's a question, And I really do mean this.

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<v Speaker 1>It sounds like I'm being flippant, but here's a real

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<v Speaker 1>question that we are looking for, like answers for this question,

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<v Speaker 1>why do we have stuff? Like? Why is there stuff?

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<v Speaker 1>Why is there matter? And energy? Sure? Why why is

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<v Speaker 1>there stuff? That's a good question. I mean, I don't

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<v Speaker 1>know if it's possible for their not to be stuff,

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<v Speaker 1>but at least there is stuff. See. The reason why

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<v Speaker 1>I ask is that if you look at our theories

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<v Speaker 1>on the the the earliest moments of the universe, keeping

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<v Speaker 1>in mind that if we're we're following the Big Bang

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<v Speaker 1>theory here, the further you get, the closer you get

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<v Speaker 1>to the beginning, the less time matters. Like time, it

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<v Speaker 1>eventually is no longer a thing, and so you can't

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<v Speaker 1>ask what happened before that because there's no time, right,

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<v Speaker 1>So there's no before time. Actually it goes back about

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<v Speaker 1>thirteen point eight billion years, and then you reach the

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<v Speaker 1>boundary of time. Yes, so you can't ask what happened

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<v Speaker 1>before that because that's a meaningless question in the context

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<v Speaker 1>of of the universe, because without time, there's no before. However,

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<v Speaker 1>one of the things we we have hypothesized have theorized

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<v Speaker 1>even is that those early moments there there was matter

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<v Speaker 1>and anti matter, and these two just do not get along. No,

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<v Speaker 1>they tend to completely annihilate one another, don't. Absolutely. If

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<v Speaker 1>matter comes into contact with antimatter, you get total annihilation.

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<v Speaker 1>Assuming you have equal parts. Then you've got nothing left

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<v Speaker 1>of that of that interaction because they will completely annihilate

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<v Speaker 1>one another. But we have matter. So that means something

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<v Speaker 1>happened for some reason, there was more matter than antimatter,

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<v Speaker 1>or something else happened to antimatter, so that for some

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<v Speaker 1>reason we didn't have everything annihilate. And that's why we're

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<v Speaker 1>able to have this podcast. I mean, it's not a

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<v Speaker 1>direct line. It's not a direct line, but we're one

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<v Speaker 1>of the things, you know. So this is one of

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<v Speaker 1>those weird questions about the about the universe. Another one

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<v Speaker 1>would be like, why does the universe exhibit the gravitational

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<v Speaker 1>properties it does? Why does it expand at the rate

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<v Speaker 1>it does? Right, Because here's the thing about expansion. See,

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<v Speaker 1>based upon our understanding of the universe, the universe should

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<v Speaker 1>do one of a couple of things. It should either

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<v Speaker 1>continuously expand if there's not enough matter for the gravitational forces,

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<v Speaker 1>to pull it all back in again, or it should

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<v Speaker 1>expand slow, stop, and then contract because the gravity is

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<v Speaker 1>strong enough pull everything back into the center. Uh. But

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<v Speaker 1>one of the things we noticed is that it is expanding,

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<v Speaker 1>and through the data we've gotten from the Hubble space telescope,

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<v Speaker 1>it's actually expanding at a rate faster than what it

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<v Speaker 1>was billions of years ago. So now that brings in

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<v Speaker 1>a question, why does it do that thing? So now

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<v Speaker 1>we've had all these questions, how are we going to

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<v Speaker 1>solve questions like this? Well, here's the problem, right, I mean,

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<v Speaker 1>these are questions that would most easily be answered if

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<v Speaker 1>we could somehow travel back thirteen point eight billion years.

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<v Speaker 1>I'm gonna stop you right there and say, even if

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<v Speaker 1>we could do that, I'm not sure it would be

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<v Speaker 1>all that easy to answer these questions because how could

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<v Speaker 1>you measure it? No, but it would be it would

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<v Speaker 1>at least we would be there to witness what was

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<v Speaker 1>happening at the very least, if not the moment we

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<v Speaker 1>were dying. Well, let's say that somehow we've managed to exist, uh,

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<v Speaker 1>coexist in parallel to the budding universe. Uh, and we

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<v Speaker 1>were somehow able to measure it. That would be our

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<v Speaker 1>best chance. Of course, we can't do that, right, we don't.

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<v Speaker 1>We don't have a time travel machine, we don't have

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<v Speaker 1>any way of existing in parallel with our own universe.

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<v Speaker 1>So the next best thing I would assume would be

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<v Speaker 1>to somehow create a micro By micro, I mean super micro,

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<v Speaker 1>I'm talking like atomic level re enactment of the conditions

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<v Speaker 1>that were present moments after the Big Bang happened. By

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<v Speaker 1>smashing stuff together, so we see the fundamental uh uh, elements,

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<v Speaker 1>energies that were there before everything kind of coalesced into

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<v Speaker 1>what it actually is now. So you're saying, sort of,

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<v Speaker 1>by simulating or trying to as best as we can

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<v Speaker 1>recreate the initial conditions of the universe, we can get

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<v Speaker 1>a better sense for why the universe looks the way

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<v Speaker 1>it does now exactly. So by that, if we were

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<v Speaker 1>able to do that and then measure it, observe it,

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<v Speaker 1>draw conclusions, we could perhaps start to fill in some

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<v Speaker 1>gaps in our knowledge. But recreating the initial conditions of

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<v Speaker 1>the universe, that sounds crazy. How could you do that? Well,

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<v Speaker 1>if you take it turns out, if you take those small,

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<v Speaker 1>small particles, you know, the small stuff we were talking about,

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<v Speaker 1>the very top of the show, not transformers, but the

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<v Speaker 1>small stuff and then smash them together at at sufficient

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<v Speaker 1>energy we can make them kind of um, well it's

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<v Speaker 1>decomposed of the wrong word, but to to convert into

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<v Speaker 1>their high energy states that they were, uh, that they

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<v Speaker 1>would have been right at moments after the Big Bang,

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<v Speaker 1>before they formed into the particles that we know today.

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<v Speaker 1>And we call these particle colliders. Right, These are the

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<v Speaker 1>machines we use to create these collisions. Uh. And they

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<v Speaker 1>are incredible things. Right, So our topic today is particle colliders.

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<v Speaker 1>We didn't need to bury the lead there that we

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<v Speaker 1>did find transformers in the beginning of the universe, very

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<v Speaker 1>closely related things. Okay, so what is a particle collider

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<v Speaker 1>and how is it different or is it different from

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<v Speaker 1>a particle accelerator. Well, a particle accelerator is something that

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<v Speaker 1>you use in order to get a particle up to

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<v Speaker 1>a certain energy level, certain speed. And it's uh, I

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<v Speaker 1>mean those are components in colliders, but they are also

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<v Speaker 1>used for other things. Yeah, since in one sense there

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<v Speaker 1>sort of is no difference, people often use these terms interchangeably,

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<v Speaker 1>and it's sort of correct to do that because one

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<v Speaker 1>term is basically a more specific term than the other.

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<v Speaker 1>A collider is a specific way of using a particle accelerator,

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<v Speaker 1>or it's sort of a type of particle accelerator, and

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<v Speaker 1>they generally refer to colliding two separate beams of subatomic

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<v Speaker 1>particles or ions. It doesn't have to be subatomic, it

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<v Speaker 1>can be atomic particles. But uh, you know, an accelerator

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<v Speaker 1>doesn't necessarily have to collide it with another beam of

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<v Speaker 1>pro of of particles. It could actually be a fixed target,

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<v Speaker 1>so you could just accelerate stuff out of fixed target

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<v Speaker 1>to find out what happens, or at something where that

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<v Speaker 1>beam of particles might be useful in a piece of technology,

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<v Speaker 1>say the back of a TV screen, or at a

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<v Speaker 1>tumor so. In a technical sense, a particle accelerator is

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<v Speaker 1>a device that uses electromagnetic fields to grab particles, increase

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<v Speaker 1>their speed, and focus them into directed beams. Okay, so

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<v Speaker 1>for one thing, one thing that we have to say

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<v Speaker 1>right away is that if we're using electromagnetic forces, then

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<v Speaker 1>clearly whatever particles we are manipulating need to have some

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<v Speaker 1>form of net charge to them, whether that's positive or negative. Right,

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<v Speaker 1>so you'll see them grabbing like electrons have a negative

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<v Speaker 1>charge or grabbing protons, grabbing ions which are charged those

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<v Speaker 1>atoms that either have more electrons than their natural state

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<v Speaker 1>or fewer electrons, so that they have a net charge

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<v Speaker 1>one way or the other. Yeah. So, one commonly given

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<v Speaker 1>example of a sort of small scale application of the

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<v Speaker 1>same principle behind a particle accelerator is a cathode ray tube.

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<v Speaker 1>That's what the CRT stands or when you talk about

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<v Speaker 1>a CRT monitor or CRT TV, that's the old way

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<v Speaker 1>of creating TV screen, those those larger, bulkier televisions that

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<v Speaker 1>some of our listeners may never have seen. Um So,

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<v Speaker 1>actually Craig Freud and Rich uses this example in his

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<v Speaker 1>house Stuff Works article about atom smashers, which is a

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<v Speaker 1>term will come back to in a minute. So, in

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<v Speaker 1>a cathode ray tube, like on an old TV, you

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<v Speaker 1>use the electrical difference between a cathode which is negatively

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<v Speaker 1>charged and an anode which is positively charged, to pull

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<v Speaker 1>a beam of electrons through an evacuated containers. That's like

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<v Speaker 1>a glass tube where you've sucked all the air out

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<v Speaker 1>of it and it's just a vacuum in side. And remember,

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<v Speaker 1>because like charges repel one another, and opposite charges a track.

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<v Speaker 1>That's why we're getting this ability to move these particles

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<v Speaker 1>where we want them to write, So the positive anode

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<v Speaker 1>wants to pull the electrons from the cathode, and they

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<v Speaker 1>get pulled off in a beam and then shoot through

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<v Speaker 1>that anode toward the TV screen. Of course, you can't

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<v Speaker 1>just you electrons at a TV screen. You've got to

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<v Speaker 1>aim them somehow, right, So that's where electromagnetic coils come in.

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<v Speaker 1>They can focus the beams of electrons and make them

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<v Speaker 1>go where they need to go. And these days particle

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<v Speaker 1>accelerators can be used for all kinds of stuff. We

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<v Speaker 1>don't have so much t c RT technology anymore these days,

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<v Speaker 1>but they can be used for things like treating cancer

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<v Speaker 1>by aiming particle beams at tumors. That's particle therapy. Interesting.

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<v Speaker 1>But most of the time, of course, when people are

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<v Speaker 1>talking about particle accelerators, they're talking about experimental mechanisms like

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<v Speaker 1>the colliders. So a collider is a particular kind of

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<v Speaker 1>particle accelerator that steers beams of accelerated particles into something,

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<v Speaker 1>either into a barrier or into an object, or into

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<v Speaker 1>each other to smash them and study what happens when

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<v Speaker 1>this tiny moment of catastrophe takes place when the when

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<v Speaker 1>the tiny particles go blue. Yeah, that's the technical term. Uh.

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<v Speaker 1>And this is why we wanted to also bring up

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<v Speaker 1>the whole atom smasher thing, because that is another kind

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<v Speaker 1>of nickname for these sort of devices, right, Yeah, not

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<v Speaker 1>to get pedantic, I mean, that's basically it's fine to

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<v Speaker 1>say atom smasher, but that's not technically so much what

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<v Speaker 1>these are anymore, because they're usually not going to be

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<v Speaker 1>grabbing whole atoms. Maybe ions. There's some heavy ion accelerators

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<v Speaker 1>out there, so that would be atomic. But but in

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<v Speaker 1>large part, we're talking about subatomic particles. We're talking. Uh.

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<v Speaker 1>For example, one of the ones will be covering a

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<v Speaker 1>lot in this episode the Large Hadron Collider, which, among

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<v Speaker 1>other things, does proton collisions. So you have two different

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<v Speaker 1>beams of protons, which are subatomic particles, right, that's part

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<v Speaker 1>of what makes up an atom. But you can possibly

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<v Speaker 1>charged part yes, and you can also have things like

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<v Speaker 1>electron positron colliders. Now electrons are the negatively charged particles.

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<v Speaker 1>Positrons are their antimatter counterpart essentially. Yeah, So in other words,

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<v Speaker 1>you're using, uh, you're using these things to to move

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<v Speaker 1>very very very tiny particles around. And when I'm saying tiny,

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<v Speaker 1>you might not really get a grip on exactly how

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<v Speaker 1>small we're talking about. Remember the nanoscale. A nanometer is

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<v Speaker 1>one billionth of a meter. The nanoscale is smaller, Like,

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<v Speaker 1>if you're looking at something that's one or two nanometers long,

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<v Speaker 1>you're not looking at it optically because you can't there's

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<v Speaker 1>no way for you to be able to look at

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<v Speaker 1>that optically. Light itself is not going to allow you

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<v Speaker 1>to do that because the wavelengths are too long. But uh,

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<v Speaker 1>the atomic scale is an order of magnitude smaller than that,

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<v Speaker 1>So that's even smaller than a nanometer, right that you

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<v Speaker 1>you essentially can have This is rough because it depends

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<v Speaker 1>upon the atom, but you could have ten atoms side

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<v Speaker 1>by side to make up one nanometer, so they're one

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<v Speaker 1>tenth that size, so they're even smaller. And then we're

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<v Speaker 1>talking sub atomic particles that are even smaller than a

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<v Speaker 1>full atom. So at this point you're talking about things

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<v Speaker 1>that are unimaginably small, and you're talking about directing them

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<v Speaker 1>as precisely as you possibly can so that they collide

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<v Speaker 1>with something like another beam of particles if you if

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<v Speaker 1>you can imagine it, that means that you have to

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<v Speaker 1>focus these beams into insanely tiny, tight packages, or else

0:13:16.960 --> 0:13:18.959
<v Speaker 1>you would never get a collision. It would be like

0:13:19.280 --> 0:13:22.360
<v Speaker 1>if Joe and I were both in uh an enormous

0:13:22.520 --> 0:13:26.360
<v Speaker 1>stadium and blindfolded and set on either end running towards

0:13:26.400 --> 0:13:29.599
<v Speaker 1>each other, and the possibility of us actually colliding that

0:13:29.600 --> 0:13:32.320
<v Speaker 1>would still be far more likely. You know. Yeah, I'd

0:13:32.320 --> 0:13:35.480
<v Speaker 1>say that's actually really generous. It's probably more like if

0:13:35.559 --> 0:13:38.520
<v Speaker 1>I stood on the Moon and you stood on the Earth,

0:13:39.000 --> 0:13:41.440
<v Speaker 1>and we each threw a pencil at each other and

0:13:41.480 --> 0:13:44.920
<v Speaker 1>we somehow were able to escape the various gravitational polls

0:13:46.400 --> 0:13:49.240
<v Speaker 1>saying gravity is negligible in this case, Yes, And the

0:13:49.280 --> 0:13:52.320
<v Speaker 1>idea that those two pencils would meet point to point

0:13:53.120 --> 0:13:55.600
<v Speaker 1>that would be still a level of precision greater than

0:13:55.600 --> 0:13:58.640
<v Speaker 1>what is required, are lesser than what is required, rather

0:13:58.960 --> 0:14:02.440
<v Speaker 1>than these beams of of sub atomic particles meeting is

0:14:03.120 --> 0:14:07.320
<v Speaker 1>an incredible achievement. Yeah, So how do these generally work? Well,

0:14:07.360 --> 0:14:10.640
<v Speaker 1>there's two main setups. You'd see. One is sort of

0:14:10.679 --> 0:14:14.480
<v Speaker 1>the ring shape, the cyclotron, the cyclic Yeah, so that's

0:14:14.480 --> 0:14:17.200
<v Speaker 1>where they would get these particles, like we said, they

0:14:17.240 --> 0:14:21.160
<v Speaker 1>control them with electromagnetic forces within some kind of tube

0:14:21.240 --> 0:14:26.000
<v Speaker 1>and accelerate them around a ring, going faster and faster

0:14:26.080 --> 0:14:28.880
<v Speaker 1>with each turn and increasing well faster and faster to

0:14:28.880 --> 0:14:31.040
<v Speaker 1>a certain point. And then once they get up to

0:14:32.000 --> 0:14:35.000
<v Speaker 1>point something per cent of the speed of light, you're

0:14:35.040 --> 0:14:39.640
<v Speaker 1>just sort of like increasing their relativistic mass, and until

0:14:39.760 --> 0:14:42.960
<v Speaker 1>they finally get to that point where these two uh,

0:14:43.200 --> 0:14:46.080
<v Speaker 1>well one one set would be going clockwise, one would

0:14:46.080 --> 0:14:51.640
<v Speaker 1>be going counterclockwise in the notes, until they finally collide, Yes,

0:14:51.760 --> 0:14:55.040
<v Speaker 1>at specific points around the cyclotron. This would be the

0:14:55.080 --> 0:14:59.360
<v Speaker 1>points where you have some form of scientific instruments that

0:14:59.400 --> 0:15:02.960
<v Speaker 1>are going to be measuring those collisions in various ways. Yeah,

0:15:03.000 --> 0:15:07.040
<v Speaker 1>you've got an instrument sitting where the streams cross and waiting. Yes. Uh.

0:15:07.080 --> 0:15:09.080
<v Speaker 1>And then the other way of doing it instead of

0:15:09.120 --> 0:15:12.080
<v Speaker 1>a ring would be a linear accelerator, Right. That's where

0:15:12.120 --> 0:15:14.800
<v Speaker 1>you just kind of have one big long tube and

0:15:14.880 --> 0:15:17.120
<v Speaker 1>a gun on each side and you aim the bullets

0:15:17.120 --> 0:15:19.840
<v Speaker 1>at each other. Yep, yep, that's that's pretty much it.

0:15:20.000 --> 0:15:23.400
<v Speaker 1>And so the linear one is actually the the uh,

0:15:23.840 --> 0:15:27.680
<v Speaker 1>the earliest type of particle accelerator. The cyclotrons came a

0:15:27.680 --> 0:15:30.440
<v Speaker 1>little later. Yeah, but the linear type may actually figure

0:15:30.520 --> 0:15:34.120
<v Speaker 1>into the future of particle accelerators though the cyclotron is

0:15:34.160 --> 0:15:38.480
<v Speaker 1>what's big today. Yes, literally big today. So yeah, let's

0:15:38.480 --> 0:15:40.800
<v Speaker 1>talk about the history where these things come from. Okay, well,

0:15:40.840 --> 0:15:42.760
<v Speaker 1>if you if you're going to be really technical, you

0:15:42.800 --> 0:15:45.440
<v Speaker 1>have to go all the way back to because that's

0:15:45.440 --> 0:15:48.480
<v Speaker 1>when scientists were at first starting to notice that when

0:15:48.480 --> 0:15:51.800
<v Speaker 1>they were beaming particles at like a sheet of gold,

0:15:51.920 --> 0:15:54.080
<v Speaker 1>some of them were bouncing back, which then began to

0:15:54.720 --> 0:16:00.400
<v Speaker 1>give people a thought of these things have the kind

0:16:00.400 --> 0:16:02.960
<v Speaker 1>of mass and they're behaving in this way. Maybe there's

0:16:02.960 --> 0:16:05.400
<v Speaker 1>a way of smashing these together and kind of seeing

0:16:05.600 --> 0:16:08.960
<v Speaker 1>what makes them tick. Now, it wouldn't be until the

0:16:09.080 --> 0:16:12.040
<v Speaker 1>nineteen thirties that they started to the scientists started to

0:16:12.040 --> 0:16:17.440
<v Speaker 1>build particle accelerators that would actually uh end up colliding

0:16:17.480 --> 0:16:21.520
<v Speaker 1>these particles with something else and um. At that time,

0:16:21.560 --> 0:16:23.520
<v Speaker 1>they were pretty limited. They were usually that they were

0:16:23.520 --> 0:16:27.520
<v Speaker 1>the linear type originally, and they could get it up

0:16:27.560 --> 0:16:31.520
<v Speaker 1>to a few hundred thousand electron volts. So that might

0:16:31.560 --> 0:16:33.400
<v Speaker 1>not mean anything to you. An electron vault is a

0:16:33.480 --> 0:16:37.840
<v Speaker 1>unit of energy. It's equivalent to about one point six

0:16:37.920 --> 0:16:43.000
<v Speaker 1>times ten to the negative nineteen jewels or it's also

0:16:43.000 --> 0:16:45.280
<v Speaker 1>known as the energy gained or lost by the charge

0:16:45.360 --> 0:16:48.960
<v Speaker 1>of a single electron moved across an electric potential difference

0:16:49.040 --> 0:16:51.880
<v Speaker 1>of one vault. Well, that don't mean a lot to me,

0:16:52.400 --> 0:16:55.520
<v Speaker 1>Well at any rate, it's it's it's a very specific,

0:16:55.640 --> 0:17:00.000
<v Speaker 1>very tiny amount of energy. So the the original experiments

0:17:00.000 --> 0:17:02.040
<v Speaker 1>were a few hundred thousand electron volts. Then they kind

0:17:02.040 --> 0:17:05.080
<v Speaker 1>of hit an energy barrier. They were specifically using direct

0:17:05.160 --> 0:17:09.320
<v Speaker 1>voltage to accelerate ions. So those charged atoms uh to

0:17:09.880 --> 0:17:13.040
<v Speaker 1>go and and get into these collisions. But at that

0:17:13.119 --> 0:17:16.840
<v Speaker 1>low energy, you're not getting the collision. The collisions are

0:17:16.880 --> 0:17:19.639
<v Speaker 1>not necessarily as spectacular as what you would need to

0:17:19.720 --> 0:17:22.960
<v Speaker 1>really get an idea of what was going on in

0:17:23.000 --> 0:17:27.760
<v Speaker 1>the earliest moments of the universe. So eventually this this

0:17:27.840 --> 0:17:30.679
<v Speaker 1>approach got up to about a million electron volts. But

0:17:31.240 --> 0:17:35.520
<v Speaker 1>after that, the the problem is that you get voltage breakdown,

0:17:35.600 --> 0:17:38.960
<v Speaker 1>so you could not continue to just try and throw

0:17:39.040 --> 0:17:41.800
<v Speaker 1>more energy at the problem. They couldn't scale it up. Yeah,

0:17:42.000 --> 0:17:45.879
<v Speaker 1>So in the nineteen forties, scientists turned to oscillating radio

0:17:45.920 --> 0:17:51.120
<v Speaker 1>frequency electric fields to resonate with particles through accelerating gaps

0:17:51.600 --> 0:17:53.560
<v Speaker 1>and that's a fancy way of saying they tried something

0:17:53.560 --> 0:17:56.439
<v Speaker 1>else that worked better. It really is. I mean, we

0:17:56.840 --> 0:17:59.080
<v Speaker 1>to go into a lot of detail would require one

0:17:59.119 --> 0:18:02.200
<v Speaker 1>It would require more time and too, frankly, it would

0:18:02.200 --> 0:18:04.240
<v Speaker 1>require a lot more expertise than what I have in

0:18:04.280 --> 0:18:07.440
<v Speaker 1>this field. I've written about particle accelerators in the past,

0:18:07.800 --> 0:18:11.679
<v Speaker 1>and I understand from a very kind of basic approach

0:18:11.800 --> 0:18:15.480
<v Speaker 1>how they work. When you get into fine details, my

0:18:15.640 --> 0:18:19.320
<v Speaker 1>knowledge breaks down pretty rapidly faster than the subotomic particle

0:18:19.359 --> 0:18:23.520
<v Speaker 1>as it turns out. So uh, these accelerators were still linear,

0:18:23.880 --> 0:18:27.520
<v Speaker 1>but then eventually scientists began to experiment a cyclotron designs,

0:18:27.560 --> 0:18:31.440
<v Speaker 1>these big circular designs, and that the purpose was to

0:18:31.480 --> 0:18:34.560
<v Speaker 1>try and continuously accelerate particles. Because you know, you're limited

0:18:34.600 --> 0:18:38.840
<v Speaker 1>by the lengths of whatever linear accelerator you have, and

0:18:38.960 --> 0:18:41.600
<v Speaker 1>that's it, right. You can't you can't loop it back

0:18:41.600 --> 0:18:44.240
<v Speaker 1>and start over. You've got it's essentially a straight path

0:18:44.320 --> 0:18:47.320
<v Speaker 1>to whatever, whether that's two guns facing each other or

0:18:47.359 --> 0:18:50.520
<v Speaker 1>a gun facing a target. But with a circle, you could,

0:18:50.520 --> 0:18:52.840
<v Speaker 1>in theory, just keep moving it around the circle and

0:18:52.840 --> 0:18:55.320
<v Speaker 1>getting it faster and faster and faster until you're ready

0:18:55.320 --> 0:18:58.560
<v Speaker 1>to direct it towards that collision, right, So that's why

0:18:58.640 --> 0:19:01.080
<v Speaker 1>they went with the circular approach. At this point they

0:19:01.080 --> 0:19:04.480
<v Speaker 1>got up to about twenty five million electron volts, and

0:19:04.560 --> 0:19:07.320
<v Speaker 1>by the nineteen fifties they could design elect cyclotrons that

0:19:07.359 --> 0:19:10.960
<v Speaker 1>could push back that energy barrier to two billion electron volts.

0:19:11.280 --> 0:19:13.000
<v Speaker 1>And before the end of the nineteen fifties they got

0:19:13.080 --> 0:19:17.119
<v Speaker 1>up to four hundred billion electron volts. So that energy

0:19:17.160 --> 0:19:20.639
<v Speaker 1>barrier just kept going up and up and up. Um

0:19:20.720 --> 0:19:23.320
<v Speaker 1>and so now these days we're talking about electron volts

0:19:23.320 --> 0:19:25.560
<v Speaker 1>and the trillions, So we should probably just take a

0:19:25.600 --> 0:19:28.600
<v Speaker 1>second to mention why is it so important to get

0:19:28.640 --> 0:19:31.920
<v Speaker 1>the energy so high to increase their speed and increase

0:19:31.960 --> 0:19:36.359
<v Speaker 1>their effective mass. It's really so that those collisions actually

0:19:36.400 --> 0:19:41.560
<v Speaker 1>result in the the primal kind of state that the

0:19:41.640 --> 0:19:44.040
<v Speaker 1>universe was in in those earliest moments. Without it, you

0:19:44.119 --> 0:19:48.000
<v Speaker 1>don't have enough energy to revert back to that. Yeah,

0:19:48.080 --> 0:19:49.880
<v Speaker 1>to get the kind of results you want, you want

0:19:49.880 --> 0:19:54.600
<v Speaker 1>the highest possible energy collision. Although we should say at

0:19:54.640 --> 0:19:58.359
<v Speaker 1>this point the LHC, the large hadron collider again, one

0:19:58.359 --> 0:20:01.800
<v Speaker 1>of the most famous collider is right now um Is

0:20:02.320 --> 0:20:06.119
<v Speaker 1>has been operating, hasn't been operating for the last several months,

0:20:06.119 --> 0:20:09.399
<v Speaker 1>but in its first round it was operating at like

0:20:09.440 --> 0:20:14.560
<v Speaker 1>a third of its capability. Those earliest experiments weren't really

0:20:15.280 --> 0:20:19.600
<v Speaker 1>performed at anywhere near its highest capacity. Although we don't

0:20:19.840 --> 0:20:22.960
<v Speaker 1>expect it ever will run it that now, but it's

0:20:23.000 --> 0:20:26.080
<v Speaker 1>definitely the second round is going to be much higher energy,

0:20:26.200 --> 0:20:28.240
<v Speaker 1>so they're expecting to find some really cool stuff the

0:20:28.280 --> 0:20:30.719
<v Speaker 1>second round through. Well, let's get into the large hat

0:20:30.840 --> 0:20:33.000
<v Speaker 1>round collider. Except first I think we should mention a

0:20:33.000 --> 0:20:36.960
<v Speaker 1>couple of the other notable colliders from recent years. Sure, so, yeah,

0:20:37.000 --> 0:20:40.160
<v Speaker 1>you're talking about like brook Haven's relativistic heavy ion collider

0:20:40.760 --> 0:20:43.680
<v Speaker 1>are Hick that was commissioned back in two thousand. It's

0:20:43.720 --> 0:20:46.120
<v Speaker 1>designed to collide heavy ions, but it's capable of going

0:20:46.160 --> 0:20:48.560
<v Speaker 1>all the way down to protons and size. There is

0:20:48.880 --> 0:20:52.639
<v Speaker 1>Fermi Labs Tiva tron Teva tron Tevatron is what I've

0:20:52.640 --> 0:20:55.440
<v Speaker 1>always said, but it could be Tivatron. Well, yeah, so

0:20:55.680 --> 0:20:59.120
<v Speaker 1>that's one of those proton anti proton colliders that's matter

0:20:59.160 --> 0:21:02.600
<v Speaker 1>and anti matter. Yeah, and uh, it can work as

0:21:02.640 --> 0:21:06.879
<v Speaker 1>both a proton anti proton beam collider or as a

0:21:06.920 --> 0:21:10.359
<v Speaker 1>fixed target collider as well. Um, so it can do

0:21:10.400 --> 0:21:13.520
<v Speaker 1>a couple of different things, and is it I'm to understand.

0:21:13.520 --> 0:21:17.000
<v Speaker 1>I believe it's number two. Yeah. Up until the Large

0:21:17.040 --> 0:21:20.160
<v Speaker 1>Hadron Collider it had become it was the the highest

0:21:20.240 --> 0:21:22.960
<v Speaker 1>energy collider in the world with one point eight trillion

0:21:22.960 --> 0:21:26.840
<v Speaker 1>electron volts, which is pretty significance. But then you've got

0:21:26.840 --> 0:21:30.720
<v Speaker 1>the Large Hadron Collider that's at cern which, uh, you know,

0:21:30.800 --> 0:21:33.399
<v Speaker 1>we we recently got a chance to see the movie

0:21:33.480 --> 0:21:37.080
<v Speaker 1>Particle Fever, which was all about the development of the

0:21:37.119 --> 0:21:39.840
<v Speaker 1>Large Hadron Collider. It's early days of being switched on

0:21:40.280 --> 0:21:43.440
<v Speaker 1>the relationship between theoretical physicists, who are the ones who

0:21:43.480 --> 0:21:45.640
<v Speaker 1>are coming up with the ideas of how the universe

0:21:45.720 --> 0:21:49.520
<v Speaker 1>must work based upon our understanding, and the experimental physicists

0:21:49.560 --> 0:21:51.520
<v Speaker 1>who put those ideas to the test and see if

0:21:51.560 --> 0:21:55.560
<v Speaker 1>they actually hold water. So, yeah, the Large Hadron Collider

0:21:55.640 --> 0:21:59.520
<v Speaker 1>might be the greatest instance of experimental physics in the

0:21:59.560 --> 0:22:02.600
<v Speaker 1>history of humanity. Yeah, depends on how you define greatest,

0:22:02.640 --> 0:22:06.520
<v Speaker 1>I guess, but it's definitely the largest machine ever built

0:22:06.520 --> 0:22:09.159
<v Speaker 1>by humans as far as we know, as long as

0:22:09.200 --> 0:22:11.280
<v Speaker 1>we we don't have that, Like, you know, the Nazis

0:22:11.280 --> 0:22:13.359
<v Speaker 1>built a death star inside of the Earth, kind of

0:22:13.400 --> 0:22:15.639
<v Speaker 1>theory or on the other side of the moon. As

0:22:15.720 --> 0:22:19.520
<v Speaker 1>Iron Sky has taught us, it's a terrible movie. Don't

0:22:19.520 --> 0:22:22.120
<v Speaker 1>watch it. Well, we've already you've already had to endure

0:22:22.160 --> 0:22:25.639
<v Speaker 1>transformers for don't put yourself to more more pain. Uh No,

0:22:26.080 --> 0:22:29.080
<v Speaker 1>there's no serious reason to question. It is the largest

0:22:29.080 --> 0:22:32.000
<v Speaker 1>machine ever built by human beings. So the large hat

0:22:32.040 --> 0:22:34.920
<v Speaker 1>around collider, it's basically just picture this. It is a

0:22:35.000 --> 0:22:41.520
<v Speaker 1>giant underground ring shaped tunnel that's twenty seven kilometers in circumference,

0:22:41.640 --> 0:22:44.199
<v Speaker 1>and that is sixteen point seven miles. They usually just

0:22:44.280 --> 0:22:47.359
<v Speaker 1>call it seventeen miles. Um. If you got in a

0:22:47.400 --> 0:22:50.399
<v Speaker 1>golf cart with an average top speed about twenty miles

0:22:50.400 --> 0:22:53.720
<v Speaker 1>per hour and you drove around this thing, not saying

0:22:53.720 --> 0:22:56.280
<v Speaker 1>there's necessarily room for you to do that, it would

0:22:56.280 --> 0:22:59.760
<v Speaker 1>take you over fifty minutes to make a complete circuit

0:22:59.840 --> 0:23:02.199
<v Speaker 1>inside this tunnel. And this tunnel, by the way, is

0:23:02.200 --> 0:23:05.960
<v Speaker 1>about three thirty feet below the surface of the ground. Yeah, well,

0:23:06.000 --> 0:23:10.800
<v Speaker 1>the depth I think is variable hundreds of feet hundreds

0:23:10.800 --> 0:23:13.520
<v Speaker 1>of feet down under the earth at the border between

0:23:13.520 --> 0:23:18.000
<v Speaker 1>Switzerland and France, pretty close to Geneva. So why was

0:23:18.400 --> 0:23:21.159
<v Speaker 1>this built? Well, it was built for the very reasons

0:23:21.200 --> 0:23:25.280
<v Speaker 1>we've been talking about to create these high energy particle collisions,

0:23:25.720 --> 0:23:28.000
<v Speaker 1>to see what happens, and and to kind of get

0:23:28.040 --> 0:23:29.800
<v Speaker 1>an idea of what was going on at the very

0:23:30.000 --> 0:23:32.760
<v Speaker 1>very earliest moments of them. We're talking like fractions of

0:23:32.760 --> 0:23:35.159
<v Speaker 1>a second when the universe came into existence. Right, So

0:23:35.280 --> 0:23:38.159
<v Speaker 1>we've mentioned it's sort of in general what a particle

0:23:38.160 --> 0:23:41.480
<v Speaker 1>accelerator does. But what does the large had round collider do? Okay, first,

0:23:41.480 --> 0:23:46.240
<v Speaker 1>you've got some feeders that speed up particles first before

0:23:46.280 --> 0:23:50.720
<v Speaker 1>they start with with hydrogen ions the protons just protons,

0:23:50.720 --> 0:23:53.359
<v Speaker 1>So and with those, you've got these uh, think of

0:23:53.400 --> 0:23:56.800
<v Speaker 1>them as kind of like like these are the little

0:23:56.800 --> 0:23:59.680
<v Speaker 1>feeder tubes that get out get those streams of protons

0:23:59.760 --> 0:24:03.080
<v Speaker 1>up to a certain speed before introducing them into the

0:24:03.119 --> 0:24:06.080
<v Speaker 1>collider itself. Well, oh yeah, that's true. Before they enter

0:24:06.160 --> 0:24:09.760
<v Speaker 1>the main ring, they go through several stages of pre acceleration.

0:24:09.920 --> 0:24:12.680
<v Speaker 1>So there are smaller rings they go into first, yes,

0:24:12.800 --> 0:24:14.639
<v Speaker 1>and then it goes into the larger ring where it

0:24:14.640 --> 0:24:20.080
<v Speaker 1>continues to accelerate using super cooled magnets. We're talking like

0:24:20.400 --> 0:24:24.720
<v Speaker 1>we're talking about this whole system. The magnet system is

0:24:24.760 --> 0:24:28.000
<v Speaker 1>cooled down to temperatures that are just above absolute zero.

0:24:28.119 --> 0:24:30.520
<v Speaker 1>But why do they cool them down like that, Jonathan, Well,

0:24:30.560 --> 0:24:34.600
<v Speaker 1>it's mainly to completely cut out all electrical resistance, so

0:24:34.640 --> 0:24:37.120
<v Speaker 1>you make it as efficient as possible. So these are

0:24:37.119 --> 0:24:40.560
<v Speaker 1>super conducting magnets that we're talking about. Not you know,

0:24:40.600 --> 0:24:43.120
<v Speaker 1>when you when you have eliminated resistance, which is generally

0:24:43.160 --> 0:24:46.080
<v Speaker 1>a problem with any kind of electrical system, Right, you

0:24:46.119 --> 0:24:49.359
<v Speaker 1>have some resistance to electron flow, and therefore you lose

0:24:49.400 --> 0:24:52.600
<v Speaker 1>some of that energy as heat. By super cooling it,

0:24:52.720 --> 0:24:55.160
<v Speaker 1>you get rid of that and you make the super

0:24:55.160 --> 0:24:58.639
<v Speaker 1>conduct conducting material where that's no longer a problem, and

0:24:58.720 --> 0:25:01.480
<v Speaker 1>you can make these magne It's incredibly efficient that way

0:25:02.080 --> 0:25:05.480
<v Speaker 1>efficient only after you have used liquid helium to cool

0:25:05.560 --> 0:25:09.520
<v Speaker 1>them down to the just a little bit over absolute zero.

0:25:09.560 --> 0:25:14.359
<v Speaker 1>It's actually technically colder than empty space, because even empty

0:25:14.359 --> 0:25:17.200
<v Speaker 1>space still has a bit of a temperature. It's because

0:25:17.280 --> 0:25:19.120
<v Speaker 1>remember absolutely zeros when you get to a point where

0:25:19.160 --> 0:25:22.520
<v Speaker 1>there's no molecular movement. Sorry, I'm just trying to think

0:25:22.560 --> 0:25:24.520
<v Speaker 1>what is the temperature of empty space? I would seem

0:25:24.560 --> 0:25:26.159
<v Speaker 1>to depend on whether you're in the shade or in

0:25:26.200 --> 0:25:29.080
<v Speaker 1>the lining fire from the sun. Right, Well, you know,

0:25:29.320 --> 0:25:33.800
<v Speaker 1>it's sure, it's it's five kelvin, but it feels like

0:25:33.880 --> 0:25:38.560
<v Speaker 1>nine kelvin. Um, No, it's it's but no, it really

0:25:38.640 --> 0:25:42.280
<v Speaker 1>is true. It's really cooling things down. It's reducing molecular

0:25:42.359 --> 0:25:44.919
<v Speaker 1>movement to a level below that which you would find

0:25:45.000 --> 0:25:49.320
<v Speaker 1>in your you know, any given empty space sector. So

0:25:49.600 --> 0:25:53.520
<v Speaker 1>so these magnets become extremely powerful and they're acting upon

0:25:53.600 --> 0:25:59.240
<v Speaker 1>these tiny, tiny particles. So it's they're they're pretty compelling, yes, uh.

0:25:59.280 --> 0:26:01.840
<v Speaker 1>And they have the ability to get these things going

0:26:02.000 --> 0:26:06.720
<v Speaker 1>extremely fast practically just just a well, it's hard to

0:26:06.720 --> 0:26:11.760
<v Speaker 1>say practical, right, but at the speed of light, it's

0:26:11.800 --> 0:26:16.239
<v Speaker 1>an incredible speed. And you've got uh and by the way,

0:26:16.280 --> 0:26:23.520
<v Speaker 1>that nine seven that was just me kind of extremely fast.

0:26:24.240 --> 0:26:27.240
<v Speaker 1>You have one beam, like we said, going clockwise, one

0:26:27.280 --> 0:26:30.520
<v Speaker 1>being going counterclockwise, and you do this until they've reached

0:26:30.520 --> 0:26:34.359
<v Speaker 1>the proper speeds and relativistic mass, and then those beams

0:26:34.400 --> 0:26:39.919
<v Speaker 1>get focused by specific magnets to collide at very particular

0:26:40.000 --> 0:26:43.320
<v Speaker 1>points along the circumference of the LHC. Now, at each

0:26:43.359 --> 0:26:46.119
<v Speaker 1>of these points, as we mentioned before, where the collision

0:26:46.240 --> 0:26:49.640
<v Speaker 1>is is ready to happen, there are instruments waiting. Yeah,

0:26:49.640 --> 0:26:53.119
<v Speaker 1>we're saying instruments. That sounds like there's like a little

0:26:53.520 --> 0:26:59.320
<v Speaker 1>sensor or something. No, we're talking like multi story scientific facilities.

0:26:59.320 --> 0:27:01.359
<v Speaker 1>We're talking like like some of them were five stories

0:27:01.440 --> 0:27:05.560
<v Speaker 1>or seven stories tall, seventy feet tall. This is an

0:27:05.800 --> 0:27:12.280
<v Speaker 1>enormous facility that has tons of microelectronics in it, literally

0:27:12.320 --> 0:27:16.040
<v Speaker 1>tons of micro electronics in it, all in an effort

0:27:16.080 --> 0:27:18.840
<v Speaker 1>to capture snapshots of what is going on in the

0:27:19.119 --> 0:27:23.000
<v Speaker 1>those fractions of a second when these collisions happen. Because

0:27:23.400 --> 0:27:25.840
<v Speaker 1>this stuff is you know, blink and it's over, blink

0:27:25.960 --> 0:27:28.480
<v Speaker 1>and and fourteen billion of them are over. I mean,

0:27:28.520 --> 0:27:33.600
<v Speaker 1>it's incredibly fast. You know, we're talking about uh so

0:27:33.680 --> 0:27:36.600
<v Speaker 1>fast that again, to try and imagine an interval of

0:27:36.680 --> 0:27:41.120
<v Speaker 1>time that short is impossible, at least for me. Maybe

0:27:41.160 --> 0:27:44.880
<v Speaker 1>other people are capable of doing it, but it's it's

0:27:44.920 --> 0:27:47.159
<v Speaker 1>how fast I wanted to run out of the theater.

0:27:47.320 --> 0:27:53.240
<v Speaker 1>And yeah, instantaneous is pretty much it, right, right, Okay,

0:27:53.320 --> 0:27:56.080
<v Speaker 1>So I do want to get into what they discover

0:27:56.200 --> 0:27:58.159
<v Speaker 1>with these experiments. But one more thing I think we

0:27:58.160 --> 0:28:01.439
<v Speaker 1>should uh talk about first and is how they built

0:28:01.480 --> 0:28:07.040
<v Speaker 1>this thing. I mean, what a seventeen mile tunnel for

0:28:07.119 --> 0:28:09.320
<v Speaker 1>one thing? For one thing? They didn't have to to

0:28:09.440 --> 0:28:12.200
<v Speaker 1>dig the tunnel for the LHC, right, that's true. Yeah,

0:28:12.200 --> 0:28:14.840
<v Speaker 1>the tunnel already existed, so that was smarter them to

0:28:14.960 --> 0:28:18.040
<v Speaker 1>use this. It was already from a previous experiment called

0:28:18.040 --> 0:28:22.960
<v Speaker 1>the l EP, the Large Electron Positron Collider, which was

0:28:23.280 --> 0:28:27.480
<v Speaker 1>decommissioned in the late eighties to make way for the LHC.

0:28:27.840 --> 0:28:31.359
<v Speaker 1>So the LHC has been in development for for years

0:28:31.359 --> 0:28:32.800
<v Speaker 1>and years and years. In fact, it was one of

0:28:32.800 --> 0:28:36.200
<v Speaker 1>those things where it became huge news as it got

0:28:36.240 --> 0:28:38.880
<v Speaker 1>closer and closer to coming online. But the funny thing

0:28:38.960 --> 0:28:41.920
<v Speaker 1>is it had been around in some form or another

0:28:42.120 --> 0:28:45.280
<v Speaker 1>at least in the building process for a decade, for

0:28:45.440 --> 0:28:49.360
<v Speaker 1>more actually more than a decade, almost two decades. So

0:28:49.480 --> 0:28:52.120
<v Speaker 1>it was pretty incredible that to me when I was

0:28:52.200 --> 0:28:54.160
<v Speaker 1>learning more about it, like, why haven't we heard about

0:28:54.280 --> 0:28:55.720
<v Speaker 1>a lot about this before? And part of that is

0:28:55.800 --> 0:28:59.200
<v Speaker 1>just um that at the time when the LHC was

0:28:59.240 --> 0:29:02.200
<v Speaker 1>being built, there were other possible colliders that were in

0:29:02.280 --> 0:29:04.720
<v Speaker 1>consideration to be built in other parts of the world,

0:29:05.080 --> 0:29:08.080
<v Speaker 1>including in the United States, that ended up not panning out.

0:29:08.600 --> 0:29:10.840
<v Speaker 1>We don't need no science now. We could do a

0:29:10.960 --> 0:29:14.600
<v Speaker 1>full episode about that story, but we are going to

0:29:14.640 --> 0:29:19.120
<v Speaker 1>focus on the optimistic, not the sad. So at any rate,

0:29:19.320 --> 0:29:23.560
<v Speaker 1>the Large Electron Positron Collider was the largest electron posit

0:29:23.760 --> 0:29:27.600
<v Speaker 1>positron collider ever built. It had five thousand, one hundred

0:29:27.720 --> 0:29:31.480
<v Speaker 1>seventy six magnets and one hundred twenty eight accelerating cavities,

0:29:32.040 --> 0:29:33.880
<v Speaker 1>and it did what you would think it would do.

0:29:33.920 --> 0:29:38.680
<v Speaker 1>It collides electrons or did collide electrons with positrons, and uh,

0:29:39.000 --> 0:29:43.080
<v Speaker 1>they would again try to. When they meet, they annihilate

0:29:43.080 --> 0:29:47.720
<v Speaker 1>one another and produce high energies, which almost instantly rematerializes

0:29:47.800 --> 0:29:49.880
<v Speaker 1>streams of particles. But again, that was one of those

0:29:49.880 --> 0:29:52.680
<v Speaker 1>things of let's see what happens in these high energy

0:29:52.720 --> 0:29:55.320
<v Speaker 1>particle collisions and learn more about the nature of the

0:29:55.400 --> 0:29:58.120
<v Speaker 1>universe itself. Yeah, so this is a great place to

0:29:58.200 --> 0:30:03.040
<v Speaker 1>build the LHC, especially because being so deep underground, this

0:30:03.040 --> 0:30:06.520
<v Speaker 1>tunnel provides good protection. And it's two way protection, right.

0:30:06.880 --> 0:30:10.920
<v Speaker 1>It helps protect the surface from radiation from the experiments,

0:30:10.960 --> 0:30:14.000
<v Speaker 1>but also, maybe even more than that, helps protect the

0:30:14.080 --> 0:30:17.520
<v Speaker 1>experiments from radiation from the outside exactly. Yeah, you want

0:30:17.520 --> 0:30:20.760
<v Speaker 1>to have that shielding material there to try and keep

0:30:20.800 --> 0:30:23.600
<v Speaker 1>the experiment as pure as possible, so that you don't

0:30:23.600 --> 0:30:26.600
<v Speaker 1>have to worry about some sort of outside factor interfering

0:30:26.600 --> 0:30:28.760
<v Speaker 1>with it. Now, that doesn't mean that an outside factor

0:30:28.800 --> 0:30:33.240
<v Speaker 1>couldn't interfere with it. A bird with a baguette might um,

0:30:33.280 --> 0:30:35.560
<v Speaker 1>But that's you know. You may have heard back when

0:30:35.560 --> 0:30:40.960
<v Speaker 1>the LHC was was getting toward doing its first actual

0:30:41.000 --> 0:30:45.200
<v Speaker 1>experiment with with UH, an actual collision, things were delayed

0:30:45.240 --> 0:30:46.960
<v Speaker 1>when a what was it actually had there was some

0:30:47.040 --> 0:30:50.560
<v Speaker 1>kind of coolant failure. Well, first there was a coolant failure. First,

0:30:50.600 --> 0:30:53.520
<v Speaker 1>there was the liquid helium leak which was happening on

0:30:53.560 --> 0:30:58.240
<v Speaker 1>the shortly after they first tested the beams, which that

0:30:58.560 --> 0:31:01.280
<v Speaker 1>in that case they weren't even trying to collide anything.

0:31:01.280 --> 0:31:02.959
<v Speaker 1>They were just making sure that they could move a

0:31:03.000 --> 0:31:08.720
<v Speaker 1>beam through clockwise and counterclockwise before ever planning out a collision.

0:31:09.440 --> 0:31:12.440
<v Speaker 1>And then the UH Not too long after that there

0:31:12.480 --> 0:31:15.640
<v Speaker 1>was a helium leak, which set everything back by several months.

0:31:16.600 --> 0:31:19.480
<v Speaker 1>Once they got that fixed, the next problem was that

0:31:20.480 --> 0:31:23.960
<v Speaker 1>there was a there was some sort of of malfunction

0:31:24.600 --> 0:31:29.720
<v Speaker 1>sometimes attributed to particles that got into a ventilation duct

0:31:29.800 --> 0:31:34.240
<v Speaker 1>that may have been caused by a bird carrying something

0:31:34.440 --> 0:31:36.680
<v Speaker 1>and dropping it in there. So it ends up always

0:31:36.680 --> 0:31:40.640
<v Speaker 1>being described as a bird carrying a baguette and dropping

0:31:40.640 --> 0:31:44.880
<v Speaker 1>the food where it landed on this in an incredible coincidence,

0:31:44.960 --> 0:31:50.080
<v Speaker 1>landed down this ventilation shaft and mucked up some important electronics,

0:31:50.080 --> 0:31:53.400
<v Speaker 1>which thus caused some some short circuiting and some other issues.

0:31:53.480 --> 0:31:56.480
<v Speaker 1>I've read a rather cryptic statement from them saying that

0:31:56.800 --> 0:31:59.400
<v Speaker 1>they like wanted to clarify, we don't know a bird

0:31:59.480 --> 0:32:02.000
<v Speaker 1>dropped of a get on one of our one of

0:32:02.040 --> 0:32:05.600
<v Speaker 1>our facilities components. We just what did they say? It

0:32:05.680 --> 0:32:08.920
<v Speaker 1>was something like there were bread crumbs and feathers found

0:32:09.000 --> 0:32:12.480
<v Speaker 1>at the sea. It could have been that someone was

0:32:12.520 --> 0:32:14.800
<v Speaker 1>plucking a bird and eating a bag at and then

0:32:14.840 --> 0:32:18.080
<v Speaker 1>sabotaged it. Who knows. But that also led a lot

0:32:18.120 --> 0:32:20.280
<v Speaker 1>of I don't know, a lot of it was tongue

0:32:20.320 --> 0:32:23.120
<v Speaker 1>in cheek, but a lot of people saying that perhaps

0:32:23.200 --> 0:32:28.120
<v Speaker 1>the the Large Hadron Collider was sabotaging itself, or that

0:32:28.320 --> 0:32:30.960
<v Speaker 1>someone from the future had come back to sabotage the

0:32:31.120 --> 0:32:33.600
<v Speaker 1>LHC to prevent it from destroying the world. Oh yeah,

0:32:33.680 --> 0:32:35.880
<v Speaker 1>we should talk about it destroying the world, which it

0:32:35.960 --> 0:32:39.520
<v Speaker 1>totally is going to do. It's it totally has not happened.

0:32:39.520 --> 0:32:41.920
<v Speaker 1>Have you noticed, like that. Do you over all those

0:32:41.920 --> 0:32:43.920
<v Speaker 1>people who thought that was gonna happen, do you remember what?

0:32:44.080 --> 0:32:46.240
<v Speaker 1>Have you seen the website? I think it's has the

0:32:46.400 --> 0:32:48.680
<v Speaker 1>LHC destroyed the world dot Com? Something like that. No,

0:32:48.920 --> 0:32:53.440
<v Speaker 1>just it just says no, which is great. But okay,

0:32:53.480 --> 0:32:57.160
<v Speaker 1>So anyway, the LHC took the place of the l

0:32:57.160 --> 0:33:00.000
<v Speaker 1>e P it was, of course, has its own magnet.

0:33:00.000 --> 0:33:02.960
<v Speaker 1>It's one thousand, two thirty two dipole magnets that are

0:33:03.000 --> 0:33:06.600
<v Speaker 1>fifteen meters in length. Those guide the beams of protons.

0:33:06.680 --> 0:33:10.440
<v Speaker 1>And then you have the three quadruple magnets, which are

0:33:10.440 --> 0:33:13.880
<v Speaker 1>between five and seven ms long, that focus those beams

0:33:13.880 --> 0:33:17.280
<v Speaker 1>that get them into those very precise parameters for the

0:33:17.280 --> 0:33:21.000
<v Speaker 1>collisions to happen. Okay, so we've got it all set up.

0:33:21.360 --> 0:33:24.080
<v Speaker 1>We've got protons going one way, we got protons going

0:33:24.120 --> 0:33:27.240
<v Speaker 1>another way. They're ready to collide. The instruments are waiting.

0:33:27.720 --> 0:33:31.440
<v Speaker 1>What do we discover? So? Uh well, I mean, how

0:33:31.480 --> 0:33:35.640
<v Speaker 1>about the particle that helps tied together the standard model

0:33:35.680 --> 0:33:38.840
<v Speaker 1>of physics. That sounds pretty good. That's pretty good. It's

0:33:39.160 --> 0:33:42.080
<v Speaker 1>you might have heard of it, Higgs boson, the Higgs boson.

0:33:42.360 --> 0:33:45.280
<v Speaker 1>That's right. So at the LHC. They did not come

0:33:45.360 --> 0:33:47.320
<v Speaker 1>up with the idea of the Higgs boson. This is

0:33:47.360 --> 0:33:50.240
<v Speaker 1>a this has been a hypothetical particle that we've known

0:33:50.280 --> 0:33:54.000
<v Speaker 1>about for a long time. We've just never seen it again.

0:33:54.080 --> 0:33:56.880
<v Speaker 1>This is where we get the theoretical physicists, right. The

0:33:56.880 --> 0:33:59.680
<v Speaker 1>theoretical physicists are the ones who look at the universe

0:33:59.800 --> 0:34:02.520
<v Speaker 1>as we understand it, and then they start looking at

0:34:02.640 --> 0:34:05.680
<v Speaker 1>gaps and our understanding and they start trying to theorize

0:34:06.000 --> 0:34:10.160
<v Speaker 1>what could possibly fill those gaps. The Higgs boson was

0:34:10.400 --> 0:34:15.040
<v Speaker 1>this hypothetical particle that that kind of filled in this

0:34:15.120 --> 0:34:18.480
<v Speaker 1>gap of of information we had. So the standard model

0:34:18.640 --> 0:34:20.960
<v Speaker 1>is really complicated. We're not going to go into everything

0:34:21.000 --> 0:34:23.120
<v Speaker 1>about it, but and we could not if we tried. No,

0:34:23.280 --> 0:34:25.520
<v Speaker 1>if we tried, we would just completely muck it up.

0:34:26.120 --> 0:34:29.520
<v Speaker 1>Uh So, just complete honesty there. But the Higgs boson

0:34:29.760 --> 0:34:33.240
<v Speaker 1>sort of like the rug in the big Lebowski, tied

0:34:33.320 --> 0:34:36.960
<v Speaker 1>the whole room together. It's true, it's um. It's often

0:34:37.000 --> 0:34:41.759
<v Speaker 1>explained as the particle that gives other particles their mass,

0:34:41.600 --> 0:34:45.000
<v Speaker 1>that it doesn't exactly give them their mass, but it

0:34:45.040 --> 0:34:49.360
<v Speaker 1>helps us understand the mechanism of mass. Yeah, it was

0:34:49.520 --> 0:34:52.439
<v Speaker 1>one of those things where in order to understand why

0:34:52.520 --> 0:34:55.480
<v Speaker 1>matter has mass, we had to have this hypothetical particle

0:34:55.960 --> 0:34:58.680
<v Speaker 1>to uh to help with our understanding, right, And if

0:34:58.719 --> 0:35:01.520
<v Speaker 1>it didn't exist, if it turned out that we did

0:35:01.560 --> 0:35:04.719
<v Speaker 1>experiments and found no evidence of this particle, would mean

0:35:04.800 --> 0:35:09.200
<v Speaker 1>that something about our fundamental understanding of the universe is wrong. Yeah,

0:35:09.200 --> 0:35:11.720
<v Speaker 1>it would mean the thing we called the standard model

0:35:11.840 --> 0:35:15.600
<v Speaker 1>needs a major revamp. There's something completely wrong with it.

0:35:15.680 --> 0:35:17.839
<v Speaker 1>And in fact, I know that there were there were

0:35:17.880 --> 0:35:20.640
<v Speaker 1>theoretical physicists who were really kind of hoping for that,

0:35:20.719 --> 0:35:23.360
<v Speaker 1>because it would mean that there'd be a whole new

0:35:23.440 --> 0:35:27.640
<v Speaker 1>world to have to understand in the world of theoretical physics. Right.

0:35:27.640 --> 0:35:31.000
<v Speaker 1>It would mean that the assumptions we had made were faulty,

0:35:31.080 --> 0:35:33.560
<v Speaker 1>and therefore we had to really we would have to

0:35:33.680 --> 0:35:37.320
<v Speaker 1>look at them again, reassess them, and figure out new

0:35:37.360 --> 0:35:42.040
<v Speaker 1>assumptions to make. However, they start, Yeah, they started smashing

0:35:42.080 --> 0:35:46.640
<v Speaker 1>protons together looking for a Higgs boson. Did they find one? Yeah?

0:35:46.680 --> 0:35:49.320
<v Speaker 1>In fact, at first it was one of those very

0:35:49.440 --> 0:35:54.239
<v Speaker 1>very appropriate scientific announcements. First of all, they may have

0:35:54.360 --> 0:35:56.719
<v Speaker 1>been found. Yeah, And not only that, but the experiments

0:35:56.760 --> 0:36:00.800
<v Speaker 1>had happened well before the announcement. Right that we're talking

0:36:01.239 --> 0:36:03.239
<v Speaker 1>months and months and months and months and months had

0:36:03.239 --> 0:36:06.560
<v Speaker 1>passed before there was ever an announcement of what had

0:36:06.600 --> 0:36:09.040
<v Speaker 1>been found. Like you'll you'll hear, oh my gosh, in

0:36:09.080 --> 0:36:11.719
<v Speaker 1>two thousand twelve, the Higgs boson was discovered and then

0:36:11.719 --> 0:36:13.920
<v Speaker 1>you read Wait a minute, this experiment was done in

0:36:13.920 --> 0:36:16.880
<v Speaker 1>a full year earlier. It took them that long to

0:36:17.120 --> 0:36:20.120
<v Speaker 1>understand the data, to make sure that they knew what

0:36:20.160 --> 0:36:23.000
<v Speaker 1>they were looking at, to confirm it with other people

0:36:23.000 --> 0:36:25.640
<v Speaker 1>who knew what they were talking about, right, to establish

0:36:25.880 --> 0:36:28.560
<v Speaker 1>at what level of certainty could they say that this

0:36:28.600 --> 0:36:31.960
<v Speaker 1>was the Higgs boson and uh, And they were very

0:36:32.000 --> 0:36:36.520
<v Speaker 1>cautious about it appropriately, so I would say, but at

0:36:36.520 --> 0:36:40.520
<v Speaker 1>this point, we feel like certain it was the Higgs boson.

0:36:41.000 --> 0:36:43.160
<v Speaker 1>That's what they found, and in fact it showed that

0:36:43.200 --> 0:36:47.680
<v Speaker 1>this standard model was UH as we understood it correct

0:36:47.719 --> 0:36:51.160
<v Speaker 1>like it it filled in that gap. So how exactly

0:36:51.200 --> 0:36:53.480
<v Speaker 1>does it fill in the gap? Again, that's not something

0:36:53.520 --> 0:36:56.160
<v Speaker 1>we're really qualified to discuss, but it's sort of the

0:36:56.239 --> 0:36:59.920
<v Speaker 1>top level. The question is how can a single particle

0:37:00.000 --> 0:37:03.879
<v Speaker 1>will affect everything? From how we understand how these tiny thing,

0:37:04.080 --> 0:37:07.360
<v Speaker 1>how these tiny particles relate to each other too. Cosmology

0:37:07.520 --> 0:37:11.480
<v Speaker 1>like our entire idea of how the universe is structure. Well,

0:37:11.520 --> 0:37:14.200
<v Speaker 1>it also has to do with something called the Higgs field,

0:37:14.600 --> 0:37:18.760
<v Speaker 1>which occupies the whole universe. So we're good there, thank goodness, um,

0:37:18.800 --> 0:37:22.240
<v Speaker 1>and that the Higgs boson is the thing about mass

0:37:22.400 --> 0:37:26.160
<v Speaker 1>which when a particle is passed through the Higgs field,

0:37:26.560 --> 0:37:28.680
<v Speaker 1>the Higgs boson is what determines whether or not that

0:37:28.719 --> 0:37:32.240
<v Speaker 1>particle has mass or does not have mass. So it's

0:37:33.000 --> 0:37:35.799
<v Speaker 1>it's again, it's it gets to a point where it's

0:37:35.800 --> 0:37:39.240
<v Speaker 1>beyond my understanding and beyond beyond that high level description.

0:37:39.400 --> 0:37:41.600
<v Speaker 1>I can't explain it. Well, one thing we do know

0:37:42.080 --> 0:37:44.520
<v Speaker 1>that the physicists who are working on this reported and

0:37:44.600 --> 0:37:46.400
<v Speaker 1>this is the thing that was highlighted really well in

0:37:46.400 --> 0:37:49.200
<v Speaker 1>that documentary we watched called Particle Fever again and yeah,

0:37:49.239 --> 0:37:50.759
<v Speaker 1>you should check it out if you get a chance.

0:37:51.280 --> 0:37:54.040
<v Speaker 1>It's available on iTunes, I believe. Yeah. One of the

0:37:54.080 --> 0:37:56.680
<v Speaker 1>things they talked about, how was how the mass of

0:37:56.719 --> 0:38:02.120
<v Speaker 1>the Higgs boson would, depending on what that value was,

0:38:02.600 --> 0:38:06.799
<v Speaker 1>would lend support to totally different views of cosmology of

0:38:07.160 --> 0:38:10.760
<v Speaker 1>what the universe fundamentally looks like. So if you measure

0:38:10.800 --> 0:38:13.640
<v Speaker 1>the mass of the Higgs boson, and it's one number

0:38:14.080 --> 0:38:16.680
<v Speaker 1>that looks like really good evidence that fits with a

0:38:16.719 --> 0:38:21.000
<v Speaker 1>theory called supersymmetry, which is a theory, a theory, or

0:38:21.000 --> 0:38:23.440
<v Speaker 1>a hypothesis you might want to call it. It's um

0:38:23.440 --> 0:38:27.480
<v Speaker 1>a very interesting idea about how uh space and matter

0:38:27.640 --> 0:38:31.360
<v Speaker 1>are fundamentally formed. Another idea would be the multiverse, the

0:38:31.400 --> 0:38:34.040
<v Speaker 1>idea that our local universe, all the things we can

0:38:34.120 --> 0:38:36.680
<v Speaker 1>see going back to the Big Bang, are not all

0:38:36.719 --> 0:38:39.960
<v Speaker 1>there is, but they're just one of many universes in

0:38:40.000 --> 0:38:44.200
<v Speaker 1>a greater multiverse. How could we ever have evidence for that? Well,

0:38:44.680 --> 0:38:48.280
<v Speaker 1>if the value of the Higgs boson were a certain number,

0:38:48.440 --> 0:38:51.520
<v Speaker 1>that would also seem to indicate the theoretical physicists that

0:38:51.560 --> 0:38:54.960
<v Speaker 1>the idea of the multiverses maybe more well evidenced, and

0:38:55.000 --> 0:38:57.759
<v Speaker 1>this would be incredible. It would also kind of be

0:38:57.840 --> 0:39:00.640
<v Speaker 1>sad because as far as we know, there's no way

0:39:00.680 --> 0:39:04.040
<v Speaker 1>we could ever observe any other universe other than our own.

0:39:04.239 --> 0:39:06.440
<v Speaker 1>And keep in mind that those other universes would have

0:39:07.320 --> 0:39:10.399
<v Speaker 1>very different laws of physics than ours do. Yeah, that's

0:39:10.440 --> 0:39:12.920
<v Speaker 1>part of the theory, right, Yeah, yeah, that that if

0:39:13.280 --> 0:39:16.480
<v Speaker 1>it's not like it's not necessarily the parallel universe theory

0:39:16.920 --> 0:39:20.760
<v Speaker 1>where we could do a Slider's like leap into another

0:39:21.000 --> 0:39:24.560
<v Speaker 1>another universe and be perfectly fine. Yeah, or you might

0:39:24.600 --> 0:39:27.200
<v Speaker 1>just you know, end up becoming pure thought, you know,

0:39:27.480 --> 0:39:31.120
<v Speaker 1>or pure energy, just like the the guys in MST

0:39:31.239 --> 0:39:33.960
<v Speaker 1>three K and that last episode did and on Comedy

0:39:34.000 --> 0:39:37.319
<v Speaker 1>Central before they coalesced back into People and Robots and

0:39:37.440 --> 0:39:40.760
<v Speaker 1>Sci Fi Channel. Anyway, Well, we should take a brief

0:39:41.000 --> 0:39:44.360
<v Speaker 1>diversion to talk about how the media interacted with the

0:39:44.400 --> 0:39:46.719
<v Speaker 1>Higgs Boson. Well, first of all, have you heard about

0:39:46.719 --> 0:39:49.080
<v Speaker 1>the god particle? Yeah, this is what they called it.

0:39:49.120 --> 0:39:51.040
<v Speaker 1>I don't know where this name got started. I could

0:39:51.040 --> 0:39:52.880
<v Speaker 1>probably find out if I wanted to look it up,

0:39:52.920 --> 0:39:54.839
<v Speaker 1>but I don't. I don't want to look it up.

0:39:55.280 --> 0:39:59.800
<v Speaker 1>The name. It's a frustrating nickname because it made for

0:40:00.040 --> 0:40:04.840
<v Speaker 1>some awesomely stupid media coverage and reaction among the general public.

0:40:05.640 --> 0:40:09.120
<v Speaker 1>People called it the god particle. But this particle has

0:40:09.120 --> 0:40:14.239
<v Speaker 1>nothing to do with theology or with religion. I saw

0:40:14.400 --> 0:40:16.680
<v Speaker 1>people were reacting. I actually saw a thing just a

0:40:16.680 --> 0:40:19.960
<v Speaker 1>few minutes ago. Is a collection of Twitter reactions people

0:40:19.960 --> 0:40:23.000
<v Speaker 1>had because the Higgs Boson was announced, simply because of

0:40:23.040 --> 0:40:25.759
<v Speaker 1>that nomenclature. But the fact that someone called it a

0:40:25.840 --> 0:40:28.600
<v Speaker 1>God particle, and then people began to assume that that

0:40:28.600 --> 0:40:31.840
<v Speaker 1>meant it either was a particle that would prove or

0:40:31.960 --> 0:40:35.480
<v Speaker 1>somehow disprove the existence of God. Yeah. Of course, this

0:40:35.520 --> 0:40:38.879
<v Speaker 1>particle doesn't do anything close to either of those, has

0:40:38.920 --> 0:40:41.880
<v Speaker 1>nothing to do with it. Yeah. Yeah, but people, I

0:40:41.920 --> 0:40:43.719
<v Speaker 1>don't know, I guess that's what they were interested in

0:40:43.760 --> 0:40:47.680
<v Speaker 1>talking about. So let's also be fair. Okay, people will

0:40:47.719 --> 0:40:51.040
<v Speaker 1>read the headline and no further. Sometimes I am also

0:40:51.120 --> 0:40:53.319
<v Speaker 1>guilty of this. By the way, I'm not saying that.

0:40:53.560 --> 0:40:56.239
<v Speaker 1>I'm not saying people as in those people of their

0:40:56.320 --> 0:40:58.400
<v Speaker 1>never bothered to read the full article. But this is

0:40:58.440 --> 0:41:01.440
<v Speaker 1>one case when you didn't do it. Yeah, okay, right,

0:41:01.480 --> 0:41:03.640
<v Speaker 1>in this case, I did read the full article and

0:41:03.680 --> 0:41:07.120
<v Speaker 1>I wrote one as well, But yeah I didn't. You know,

0:41:07.160 --> 0:41:09.200
<v Speaker 1>there are times where I'm just as guilty of that.

0:41:09.239 --> 0:41:11.560
<v Speaker 1>So I don't mean to say that, you know, somehow

0:41:11.600 --> 0:41:14.040
<v Speaker 1>I'm better than those people. I am those people, just

0:41:14.080 --> 0:41:16.279
<v Speaker 1>not in this one case. Okay. So the discovery the

0:41:16.360 --> 0:41:19.640
<v Speaker 1>Higgs boson, we discovered it, we looked at it's it's mass,

0:41:19.719 --> 0:41:22.720
<v Speaker 1>and we were like, here it is. Did it settle

0:41:22.800 --> 0:41:27.920
<v Speaker 1>all these questions? About the multiverse, about the about the supersymmetry,

0:41:28.000 --> 0:41:31.799
<v Speaker 1>all these other questions. No, not really, but it did

0:41:31.840 --> 0:41:34.320
<v Speaker 1>still give us a really interesting piece of the puzzle

0:41:34.560 --> 0:41:36.840
<v Speaker 1>that will give us something new to work with going

0:41:36.920 --> 0:41:39.680
<v Speaker 1>forward in new theoretical physics, because now we know a

0:41:39.680 --> 0:41:42.200
<v Speaker 1>few things. Number One, we have a better idea that

0:41:42.239 --> 0:41:45.759
<v Speaker 1>the standard model of physics is on track like it's

0:41:45.480 --> 0:41:49.080
<v Speaker 1>It hasn't been disproved, so we So it's not like

0:41:49.160 --> 0:41:52.560
<v Speaker 1>we suddenly have to completely refocus our efforts in some

0:41:52.640 --> 0:41:55.080
<v Speaker 1>new direction. What we need to do is kind of

0:41:55.080 --> 0:41:57.759
<v Speaker 1>refine what we're looking for and how we're looking for it.

0:41:57.840 --> 0:41:59.839
<v Speaker 1>So we've sort of seen like a mile marker along

0:41:59.840 --> 0:42:02.040
<v Speaker 1>the race. It's like, Okay, we're sort of sort of

0:42:02.080 --> 0:42:04.600
<v Speaker 1>going in the right direction. Good to know that we've

0:42:04.600 --> 0:42:07.600
<v Speaker 1>also got a value that we can work with plugging

0:42:07.600 --> 0:42:10.960
<v Speaker 1>into new theoretical physics and moving forward. But I have

0:42:11.080 --> 0:42:15.560
<v Speaker 1>the question, what's next? Is there anything left for the

0:42:15.640 --> 0:42:18.600
<v Speaker 1>large head round collider to discover? Or now that we've

0:42:18.600 --> 0:42:22.120
<v Speaker 1>got the Higgs boson, is that it so much? There's

0:42:22.200 --> 0:42:25.359
<v Speaker 1>so much? Yeah, So the Higgs boson is easily the

0:42:25.360 --> 0:42:28.360
<v Speaker 1>thing that most media outlets have focused on when it

0:42:28.400 --> 0:42:31.080
<v Speaker 1>comes to what the LHC is doing. But that is

0:42:31.120 --> 0:42:34.719
<v Speaker 1>just one part of all the different experiments going on.

0:42:34.840 --> 0:42:38.399
<v Speaker 1>That's just one thing. It's very important part, but it's

0:42:38.440 --> 0:42:42.399
<v Speaker 1>not the only part. So we have questions about matter

0:42:42.440 --> 0:42:44.200
<v Speaker 1>and antimatter. Like I said at the top of the show,

0:42:44.680 --> 0:42:47.600
<v Speaker 1>why was it that at the Big Bang there was

0:42:47.640 --> 0:42:51.920
<v Speaker 1>more matter than antimatter? Or why wasn't Why didn't equal

0:42:51.960 --> 0:42:55.640
<v Speaker 1>parts annihilate each other? What was it about that event

0:42:56.160 --> 0:42:58.960
<v Speaker 1>that created the universe as we know it? Why did

0:42:59.000 --> 0:43:01.000
<v Speaker 1>it happen that way? We need to answer those questions

0:43:01.000 --> 0:43:02.759
<v Speaker 1>if we want to have a true understanding of how

0:43:02.760 --> 0:43:06.880
<v Speaker 1>our universe works. Uh. Also, you've heard about dark energy,

0:43:07.000 --> 0:43:09.680
<v Speaker 1>dark matter, that stuff. Yeah, dark matter is a thing

0:43:09.800 --> 0:43:13.080
<v Speaker 1>that helps us explain why the universe looks like it does.

0:43:14.000 --> 0:43:17.959
<v Speaker 1>So the universe displays certain gravitational properties that don't seem

0:43:18.040 --> 0:43:20.640
<v Speaker 1>to make sense given how much matter we think is

0:43:20.640 --> 0:43:23.239
<v Speaker 1>in the universe. Yeah, we look around, we see all

0:43:23.239 --> 0:43:25.640
<v Speaker 1>this matter. We see it behaving in a way that's

0:43:25.680 --> 0:43:28.640
<v Speaker 1>not completely consistent with how we understand the universe to

0:43:28.680 --> 0:43:31.719
<v Speaker 1>work based upon the amount of matter we're able to see.

0:43:32.160 --> 0:43:36.360
<v Speaker 1>So what that has caused people to theorize or hypothesize

0:43:36.880 --> 0:43:38.919
<v Speaker 1>is that there's some stuff out there that we are

0:43:39.120 --> 0:43:42.959
<v Speaker 1>incapable of observing, that are that is in some way

0:43:43.080 --> 0:43:46.440
<v Speaker 1>acting upon the rest of the stuff in the universe,

0:43:46.960 --> 0:43:50.160
<v Speaker 1>and it's only because we are incapable of perceiving it

0:43:50.520 --> 0:43:53.600
<v Speaker 1>that it's a mystery to us that it's totally there.

0:43:53.719 --> 0:43:55.680
<v Speaker 1>And if we had a way of perceiving it, we could,

0:43:55.760 --> 0:43:59.120
<v Speaker 1>it would just fit neatly into our our our vision

0:43:59.120 --> 0:44:03.280
<v Speaker 1>of how the universe works. Um, I mean, if it doesn't, again,

0:44:03.440 --> 0:44:07.399
<v Speaker 1>our fundamental understanding of how things work is off. So

0:44:08.239 --> 0:44:10.560
<v Speaker 1>this dark energy and dark matter would make up the

0:44:10.640 --> 0:44:15.000
<v Speaker 1>majority of energy and matter in the universe, that the

0:44:15.040 --> 0:44:17.080
<v Speaker 1>stuff that we can actually observe would be just a

0:44:17.120 --> 0:44:21.480
<v Speaker 1>tiny little fraction of the overall picture, which is pretty phenomenal.

0:44:21.560 --> 0:44:24.520
<v Speaker 1>But again, we can't observe it. So one of the

0:44:24.560 --> 0:44:27.280
<v Speaker 1>things that we can, we can observe the effects of it. Yeah,

0:44:27.440 --> 0:44:30.960
<v Speaker 1>and so there there's and there's some you know, hypotheses

0:44:31.000 --> 0:44:35.359
<v Speaker 1>about what it could ultimately actually be, whether it's uh

0:44:35.560 --> 0:44:39.680
<v Speaker 1>whimps or MACHOs or other fun terms. But at any rate,

0:44:39.760 --> 0:44:41.320
<v Speaker 1>a lot of the experiments at the l h C

0:44:41.680 --> 0:44:44.800
<v Speaker 1>are dedicated to looking for evidence of dark energy and

0:44:44.880 --> 0:44:51.520
<v Speaker 1>dark matter. Cosmic rays. Yeah, so cosmic rays again something

0:44:51.520 --> 0:44:53.560
<v Speaker 1>that happens in the universe all the time, right, You

0:44:53.600 --> 0:44:56.680
<v Speaker 1>get these these charged particles that are moving at high energy.

0:44:57.120 --> 0:44:58.880
<v Speaker 1>You know. The kind of cool thing about what the

0:44:59.000 --> 0:45:02.120
<v Speaker 1>LHC does is it sort of create something like a

0:45:02.120 --> 0:45:05.560
<v Speaker 1>cosmic ray. Yeah. Actually, I mean really does create cosmic rays.

0:45:05.600 --> 0:45:07.759
<v Speaker 1>It's just it's doing it in lab conditions, so it's

0:45:07.800 --> 0:45:12.880
<v Speaker 1>under controlled conditions ray. Then again, it's a highly charged particle.

0:45:12.960 --> 0:45:16.080
<v Speaker 1>It tends to be um something that would if we

0:45:16.160 --> 0:45:19.120
<v Speaker 1>came into contact with it would really mess us up

0:45:19.120 --> 0:45:22.960
<v Speaker 1>big time. But luckily the Earth has a couple of layers. Yeah,

0:45:23.000 --> 0:45:24.520
<v Speaker 1>there a couple of layers of protection that we have

0:45:24.600 --> 0:45:27.640
<v Speaker 1>here on Earth. The atmosphere and the magnetosphere in particular

0:45:27.920 --> 0:45:30.600
<v Speaker 1>are helping us out a lot, so we don't have

0:45:30.640 --> 0:45:33.080
<v Speaker 1>to worry about it so much. Uh. And there's some

0:45:33.080 --> 0:45:35.280
<v Speaker 1>people who are worried about cosmic rays at the LHC,

0:45:35.560 --> 0:45:38.680
<v Speaker 1>but again, this is under controlled conditions. This is the

0:45:38.680 --> 0:45:41.000
<v Speaker 1>way you want to see it happen. Um. There are

0:45:41.000 --> 0:45:42.960
<v Speaker 1>some people who are worried that that might lead to

0:45:43.120 --> 0:45:45.640
<v Speaker 1>a catastrophic event. But if you just point out the

0:45:45.640 --> 0:45:48.000
<v Speaker 1>fact that cosmic rays are colliding with stuff all the

0:45:48.040 --> 0:45:50.439
<v Speaker 1>time throughout the universe, and our universe is still here.

0:45:50.920 --> 0:45:55.480
<v Speaker 1>That's pretty good evidence that we're in safe territory, right

0:45:55.600 --> 0:45:57.719
<v Speaker 1>that that we're not going to rip a hole through

0:45:57.760 --> 0:46:02.360
<v Speaker 1>the spacetime continuum and get uh hold into Doctor Who's universe. Okay,

0:46:02.400 --> 0:46:06.480
<v Speaker 1>So I have a question. Yeah, we've talked about black holes.

0:46:07.000 --> 0:46:10.680
<v Speaker 1>Number one, could it? Could the LHC teach us anything

0:46:10.719 --> 0:46:13.439
<v Speaker 1>new about black holes? And number two? Could it? As

0:46:13.480 --> 0:46:16.759
<v Speaker 1>I hope we've already suggested, it could not create a

0:46:16.760 --> 0:46:19.920
<v Speaker 1>black hole that will kill everyone. I'm so glad you

0:46:19.960 --> 0:46:22.360
<v Speaker 1>said we'll kill everyone, because that's the part that I

0:46:22.400 --> 0:46:25.040
<v Speaker 1>can say. No, it might create a black hole, but

0:46:25.040 --> 0:46:28.040
<v Speaker 1>we're talking like a micro black hole that would last

0:46:28.080 --> 0:46:30.360
<v Speaker 1>for a fraction of a second before collapsing in on itself.

0:46:30.719 --> 0:46:33.080
<v Speaker 1>So when I say micro black hole, i'm talking about

0:46:33.560 --> 0:46:35.960
<v Speaker 1>you know the black holes we think of in cosmology.

0:46:36.239 --> 0:46:38.440
<v Speaker 1>Those are the former stars. Yeah, it's a result of

0:46:38.440 --> 0:46:41.160
<v Speaker 1>a of a collapse star. Right, stars having to be

0:46:41.200 --> 0:46:43.480
<v Speaker 1>pretty big. I don't know if you've noticed. In fact,

0:46:43.520 --> 0:46:46.920
<v Speaker 1>some stars aren't big enough to become black holes. Like

0:46:46.960 --> 0:46:49.960
<v Speaker 1>our star doesn't have enough mass to become a black hole.

0:46:50.160 --> 0:46:52.600
<v Speaker 1>So you have to be an enormous star to become

0:46:52.640 --> 0:46:55.400
<v Speaker 1>one of these incredibly powerful black holes that start gulping

0:46:55.440 --> 0:46:57.120
<v Speaker 1>everything up and nothing can escape it, and then you

0:46:57.120 --> 0:46:59.640
<v Speaker 1>have the spighettification and all that kind of fun stuff. Right.

0:47:00.640 --> 0:47:03.000
<v Speaker 1>I don't know if you know this, but a sub

0:47:03.040 --> 0:47:07.279
<v Speaker 1>atomic particle is slightly smaller than your average star, let

0:47:07.320 --> 0:47:09.160
<v Speaker 1>alone a star large enough to make a black hole.

0:47:09.960 --> 0:47:13.239
<v Speaker 1>And by slightly smaller, I mean is the other end

0:47:13.239 --> 0:47:15.200
<v Speaker 1>of the scale. I mean it's you know, you talk

0:47:15.239 --> 0:47:18.080
<v Speaker 1>about something that's so large you can't imagine exactly how

0:47:18.320 --> 0:47:21.160
<v Speaker 1>big it is, to something so small you can't imagine

0:47:21.160 --> 0:47:24.040
<v Speaker 1>how small it is. So first of all, you're talking

0:47:24.040 --> 0:47:26.680
<v Speaker 1>about a black hole that has has less energy than

0:47:27.080 --> 0:47:32.160
<v Speaker 1>a mosquito flapping its wings, so no energy really at all. Second,

0:47:32.239 --> 0:47:35.520
<v Speaker 1>it collapses within a split second. It does not have

0:47:35.640 --> 0:47:39.040
<v Speaker 1>the energy needed to become any kind of macroscopic effect

0:47:39.160 --> 0:47:41.279
<v Speaker 1>on the world around us, so that is not going

0:47:41.320 --> 0:47:44.960
<v Speaker 1>to happen. However, being able to create these teeny tiny

0:47:44.960 --> 0:47:47.600
<v Speaker 1>black holes means that on a very tiny scale, we

0:47:47.680 --> 0:47:51.359
<v Speaker 1>might learn more about how they how they work, So

0:47:51.520 --> 0:47:54.919
<v Speaker 1>we could learn more about black holes through these experiments.

0:47:55.440 --> 0:47:58.920
<v Speaker 1>But there's no chance that this is going to create

0:47:58.960 --> 0:48:01.440
<v Speaker 1>a black hole that's going to destroy the Earth. I mean,

0:48:01.440 --> 0:48:03.080
<v Speaker 1>it's the same sort of things before when I talked

0:48:03.080 --> 0:48:06.440
<v Speaker 1>about cosmic rays hitting the Earth all the time. The

0:48:06.480 --> 0:48:11.200
<v Speaker 1>collisions that happened within the LHC are recreations of things

0:48:11.239 --> 0:48:14.680
<v Speaker 1>that happen in nature. Okay, these things happen out in

0:48:14.719 --> 0:48:18.840
<v Speaker 1>the universe a lot. Because the universe is is so huge,

0:48:19.280 --> 0:48:21.880
<v Speaker 1>it's not like these are are super common events in

0:48:21.920 --> 0:48:25.680
<v Speaker 1>our particular solar system. But if you take the entire universe,

0:48:26.000 --> 0:48:28.840
<v Speaker 1>these things happen all the time, and the universe is

0:48:28.920 --> 0:48:32.200
<v Speaker 1>still there. So what's what we're seeing now is this

0:48:32.400 --> 0:48:36.799
<v Speaker 1>controlled experiment within a laboratory where again the safety has

0:48:36.800 --> 0:48:40.800
<v Speaker 1>already been established because we're here. If it weren't safe,

0:48:40.840 --> 0:48:43.960
<v Speaker 1>we never would have made it because things would have

0:48:44.040 --> 0:48:47.160
<v Speaker 1>destroyed themselves already before the Earth could have even formed.

0:48:47.680 --> 0:48:50.319
<v Speaker 1>So that's the way to look at it, saying like, look,

0:48:51.000 --> 0:48:54.040
<v Speaker 1>did you eat a sandwich today. Guess what, here's the

0:48:54.080 --> 0:48:56.719
<v Speaker 1>really super cool thing that we might discover. You're going

0:48:56.760 --> 0:48:59.480
<v Speaker 1>to tell me about another discovery. Yeah, here's the coolest one.

0:49:00.160 --> 0:49:03.120
<v Speaker 1>We don't know. We could we could discover something that

0:49:03.239 --> 0:49:07.399
<v Speaker 1>we have yet to hypothesize about, or something that completely

0:49:07.520 --> 0:49:12.520
<v Speaker 1>and fundamentally changes some aspect of how we understand the

0:49:12.560 --> 0:49:14.880
<v Speaker 1>universe to work. Yeah, and in fact, these are the

0:49:14.920 --> 0:49:19.600
<v Speaker 1>coolest types of discoveries. These are the disruptive discoveries, the

0:49:19.680 --> 0:49:23.600
<v Speaker 1>things that force us to go way back and say, Okay,

0:49:23.719 --> 0:49:26.040
<v Speaker 1>we were getting a lot of stuff wrong, or we

0:49:26.120 --> 0:49:29.400
<v Speaker 1>had no idea that there was this whole other world

0:49:29.719 --> 0:49:34.520
<v Speaker 1>of of rules and and facts and interacting objects to discover. Right.

0:49:34.640 --> 0:49:37.960
<v Speaker 1>And when you get into stuff like that, it brings

0:49:38.040 --> 0:49:42.000
<v Speaker 1>up the obvious response to all these people, uh that

0:49:42.400 --> 0:49:45.520
<v Speaker 1>are opposed to projects like this, because they're like, what

0:49:45.560 --> 0:49:48.000
<v Speaker 1>does it actually do? You know? Yeah, how is this

0:49:48.040 --> 0:49:50.160
<v Speaker 1>going to help us build a better mousetrap? Right? The

0:49:50.160 --> 0:49:52.799
<v Speaker 1>ones who wants some form of practical application, Well, first

0:49:52.800 --> 0:49:56.239
<v Speaker 1>of all, uh, on the face of it, if you

0:49:56.280 --> 0:49:58.480
<v Speaker 1>were to and this is in that movie that we

0:49:58.480 --> 0:50:03.359
<v Speaker 1>were talking about, they're American politicians railing against creating this

0:50:03.560 --> 0:50:06.480
<v Speaker 1>the super collider in the United States. And the response

0:50:06.520 --> 0:50:09.600
<v Speaker 1>of the theoretical physicist David Kaplan is that, you know,

0:50:09.680 --> 0:50:13.000
<v Speaker 1>I can't I can't tell you what this is for.

0:50:13.080 --> 0:50:16.320
<v Speaker 1>It may not ever have any practical purpose The reason

0:50:16.400 --> 0:50:18.360
<v Speaker 1>for it is for us to understand the nature of

0:50:18.400 --> 0:50:22.719
<v Speaker 1>the universe. It's to increase our understanding, which has its

0:50:22.760 --> 0:50:27.160
<v Speaker 1>own value outside of just a practical application of making

0:50:27.200 --> 0:50:29.839
<v Speaker 1>some technology that makes our lives better. Of course, if

0:50:29.880 --> 0:50:33.279
<v Speaker 1>you do want to appease this, this call for practical application,

0:50:33.600 --> 0:50:37.040
<v Speaker 1>you can make a pretty good case because all of

0:50:37.080 --> 0:50:41.440
<v Speaker 1>the technology we have today came out of non technological

0:50:41.560 --> 0:50:45.600
<v Speaker 1>scientific discovery, stuff that people were figuring out about how

0:50:45.640 --> 0:50:48.160
<v Speaker 1>the world worked. I've heard this example used a lot.

0:50:48.200 --> 0:50:51.360
<v Speaker 1>I can't remember, uh if he used it specifically in

0:50:51.400 --> 0:50:52.880
<v Speaker 1>the film, but there have been a lot of scientists

0:50:52.920 --> 0:50:58.800
<v Speaker 1>who bring this up. Radio waves. Yeah, okay, electromagnetic radiation.

0:50:58.840 --> 0:51:02.000
<v Speaker 1>I mean, that's totally true. That's a scientific discovery about

0:51:02.000 --> 0:51:05.719
<v Speaker 1>the nature of physics and reality. But guess what now

0:51:05.800 --> 0:51:09.800
<v Speaker 1>we've got GPS and satellites and microwave, overn's, cell phones,

0:51:10.040 --> 0:51:13.959
<v Speaker 1>radio stations, set, I mean everything. Yeah. The point he makes,

0:51:14.000 --> 0:51:17.360
<v Speaker 1>he said, think of radio waves. When radio waves were discovered,

0:51:17.400 --> 0:51:20.080
<v Speaker 1>they weren't called radio waves because we didn't have radios

0:51:20.160 --> 0:51:24.839
<v Speaker 1>yet we built radios in order to this, right. So

0:51:24.880 --> 0:51:27.120
<v Speaker 1>that's the thing is that you cannot predict what sort

0:51:27.120 --> 0:51:30.520
<v Speaker 1>of practical application may come out of this exploratory science.

0:51:31.040 --> 0:51:34.040
<v Speaker 1>Just know that if stuff does happen, it's going to

0:51:34.120 --> 0:51:37.879
<v Speaker 1>be pretty amazing. So it's it's it's one of those

0:51:37.920 --> 0:51:40.359
<v Speaker 1>that's really it's a hard sell for people who are

0:51:40.400 --> 0:51:44.160
<v Speaker 1>paying the bills, right, It's a hard sell to say, Look,

0:51:45.200 --> 0:51:48.520
<v Speaker 1>we may never have any sort of practical application for

0:51:48.560 --> 0:51:51.840
<v Speaker 1>this technology, but we will understand more about how the

0:51:51.920 --> 0:51:55.680
<v Speaker 1>universe works. And understanding more is a good thing, and

0:51:55.719 --> 0:51:59.560
<v Speaker 1>it may lead to incredible practical applications. Who knows, the

0:51:59.600 --> 0:52:01.840
<v Speaker 1>information sation that we get from these kind of experiments

0:52:01.880 --> 0:52:05.880
<v Speaker 1>could lead to developments and things like interstellar space travel

0:52:05.960 --> 0:52:09.640
<v Speaker 1>down the road in ways we cannot anticipate, maybe even

0:52:09.840 --> 0:52:16.080
<v Speaker 1>time travel. You can go eat a bighette in two thousand,

0:52:16.320 --> 0:52:19.480
<v Speaker 1>whatever year it was nine, I don't know. I'm telling you.

0:52:19.480 --> 0:52:21.640
<v Speaker 1>There were theories that it was actually a time travel

0:52:21.680 --> 0:52:24.320
<v Speaker 1>paradox thing. But anyway, Okay, so I have a question

0:52:25.120 --> 0:52:28.640
<v Speaker 1>here we are, what's the next big step in particle physics.

0:52:28.680 --> 0:52:30.600
<v Speaker 1>What's the next thing we're going to do. Obviously, I

0:52:30.640 --> 0:52:33.240
<v Speaker 1>know there have been some upgrades planned for the LHC

0:52:33.360 --> 0:52:36.640
<v Speaker 1>itself and it's next round of experiments will be done

0:52:36.640 --> 0:52:38.960
<v Speaker 1>at higher energy levels than the first round, right, that

0:52:39.000 --> 0:52:42.799
<v Speaker 1>will begin sometime in that alone is really cool. But

0:52:43.320 --> 0:52:47.239
<v Speaker 1>what what's the next thing we could build after the LHC. Well,

0:52:47.760 --> 0:52:51.439
<v Speaker 1>remember linear particle accelerators, Yeah, way back in the day. Yeah,

0:52:51.440 --> 0:52:53.560
<v Speaker 1>back in the nineteen thirties I mentioned they might be

0:52:53.600 --> 0:52:56.439
<v Speaker 1>in the future of particle accelerators. Yeah. Yeah. So here

0:52:56.480 --> 0:52:58.680
<v Speaker 1>here's why you might say, well, why would we go

0:52:58.760 --> 0:53:02.000
<v Speaker 1>back to a technology after we had moved on to

0:53:02.160 --> 0:53:05.880
<v Speaker 1>a different format. And the reason is that part of

0:53:05.880 --> 0:53:08.920
<v Speaker 1>the problem with the cyclotron approach is that you have

0:53:09.000 --> 0:53:11.400
<v Speaker 1>to expend a lot of energy to move those particles

0:53:11.400 --> 0:53:13.719
<v Speaker 1>in an arc. You know, to move them in an arc,

0:53:13.760 --> 0:53:17.440
<v Speaker 1>you have to uh to exert energy on them, and

0:53:17.560 --> 0:53:23.359
<v Speaker 1>you can cause sub atomic particles to to change and

0:53:23.440 --> 0:53:27.960
<v Speaker 1>not have reached their ideal relativistic masses. That because you

0:53:28.040 --> 0:53:31.200
<v Speaker 1>have to continuously exert this extra pressure in order to

0:53:31.239 --> 0:53:33.319
<v Speaker 1>make them arc. If you can move them in a

0:53:33.360 --> 0:53:36.640
<v Speaker 1>straight line, you wouldn't have to do that, right you wouldn't.

0:53:36.680 --> 0:53:39.160
<v Speaker 1>You just have a straight pathway and you're just really

0:53:39.239 --> 0:53:41.520
<v Speaker 1>accelerating them and making sure that they stay in the

0:53:42.360 --> 0:53:45.279
<v Speaker 1>within the parameters of that pathway. You don't. But you

0:53:45.320 --> 0:53:47.000
<v Speaker 1>don't have to bend them, you don't have to move

0:53:47.040 --> 0:53:50.040
<v Speaker 1>them in an arc, and you can you can increase

0:53:50.080 --> 0:53:52.399
<v Speaker 1>the whole energy level in that sense, or at least

0:53:52.400 --> 0:53:57.239
<v Speaker 1>the relativistic mass in that sense. And so, uh, that's

0:53:57.280 --> 0:54:01.040
<v Speaker 1>why we're looking at the possibility of some innier particle

0:54:01.120 --> 0:54:05.000
<v Speaker 1>accelerators and colliders in the future. So just one big

0:54:05.080 --> 0:54:08.640
<v Speaker 1>long tunnel, well really long. I mean, if we're talking

0:54:08.640 --> 0:54:11.560
<v Speaker 1>about the International Linear Collider, you're talking about thirty one

0:54:11.640 --> 0:54:15.799
<v Speaker 1>kilometer long particle accelerator. Yeah, that's so that's a proposed

0:54:15.880 --> 0:54:19.279
<v Speaker 1>collider that uh, it's not being built yet, it's just

0:54:19.320 --> 0:54:21.440
<v Speaker 1>in the proposal stage, but a lot of the particle

0:54:21.480 --> 0:54:24.399
<v Speaker 1>physics community are talking about it now. It's not even

0:54:24.440 --> 0:54:26.080
<v Speaker 1>clear where it would be built, but I've read that

0:54:26.200 --> 0:54:29.680
<v Speaker 1>Japan has expressed interest in hosting it. Yeah, finding finding

0:54:29.719 --> 0:54:33.400
<v Speaker 1>thirty one kilometers that you can use to build not

0:54:33.520 --> 0:54:36.640
<v Speaker 1>just the accelerator, but then all the scientific installations that

0:54:36.719 --> 0:54:39.560
<v Speaker 1>you need in order to actually study the collisions. That's

0:54:39.640 --> 0:54:41.839
<v Speaker 1>I mean, that's a lot of that's a lot of space. Yeah,

0:54:41.920 --> 0:54:45.239
<v Speaker 1>So what would the International Linear Collider do well? In

0:54:45.280 --> 0:54:49.280
<v Speaker 1>this case, we're talking about another electron positron collider. Okay,

0:54:49.400 --> 0:54:53.319
<v Speaker 1>so annihilating electrons and positrons and incredibly high energies to

0:54:53.440 --> 0:54:57.680
<v Speaker 1>really see what happens once again at these high energy

0:54:57.719 --> 0:55:02.920
<v Speaker 1>particle collisions, and it's it's more to say more of

0:55:02.920 --> 0:55:05.680
<v Speaker 1>the same as a as a disservice, but it's really

0:55:05.680 --> 0:55:07.759
<v Speaker 1>to get a slightly different like think of it as

0:55:07.800 --> 0:55:11.600
<v Speaker 1>a different angle view on what is happening at the

0:55:11.640 --> 0:55:15.239
<v Speaker 1>earliest moments of the universe. I hate that science and

0:55:15.280 --> 0:55:18.600
<v Speaker 1>politics have to mix, because it would be wonderful if

0:55:18.600 --> 0:55:21.440
<v Speaker 1>we lived in a world where we could pursue scientific

0:55:21.560 --> 0:55:24.839
<v Speaker 1>endeavors without having to worry about where the funding comes from.

0:55:24.840 --> 0:55:27.080
<v Speaker 1>But that's not the world we live in, right and

0:55:27.080 --> 0:55:30.080
<v Speaker 1>and because we need to make those considerations, they are important.

0:55:30.120 --> 0:55:35.120
<v Speaker 1>I don't want to suggest that a country that decides

0:55:35.200 --> 0:55:38.319
<v Speaker 1>not to fund some sort of scientific endeavor is doing

0:55:38.400 --> 0:55:41.799
<v Speaker 1>so for the wrong reasons. There may be very compelling

0:55:41.880 --> 0:55:44.840
<v Speaker 1>reasons why that money needs to go somewhere else. I

0:55:44.920 --> 0:55:47.400
<v Speaker 1>don't wish to make this that kind of black and white,

0:55:47.440 --> 0:55:49.960
<v Speaker 1>simplistic view of how the world works. The world is

0:55:50.000 --> 0:55:54.560
<v Speaker 1>insanely complicated. So I just wish that we lived in

0:55:54.600 --> 0:55:57.080
<v Speaker 1>this world where we didn't have to worry about that. Well,

0:55:57.120 --> 0:56:00.239
<v Speaker 1>I mean, in in either case, I am also very

0:56:00.280 --> 0:56:02.600
<v Speaker 1>sympathetic to the idea that, yeah, we we've got a

0:56:02.600 --> 0:56:05.160
<v Speaker 1>lot of things that need funding. Yeah, there's a lot

0:56:05.200 --> 0:56:07.920
<v Speaker 1>of competition for that. But at the same time, scientific

0:56:07.960 --> 0:56:11.359
<v Speaker 1>research like this is funding the future. That sounds kind

0:56:11.360 --> 0:56:14.200
<v Speaker 1>of like a cliche. I'm sorry, but it is. It's

0:56:14.239 --> 0:56:17.080
<v Speaker 1>just it's how you invest in what's happening to your

0:56:17.160 --> 0:56:20.160
<v Speaker 1>children and in their world. Sure, it's just a really

0:56:20.200 --> 0:56:23.120
<v Speaker 1>hard sell in the short term, right you can you

0:56:23.160 --> 0:56:26.600
<v Speaker 1>can demonstrate how long term gains are are one of

0:56:26.640 --> 0:56:29.160
<v Speaker 1>the things that go hand in hand with funding science.

0:56:29.640 --> 0:56:32.759
<v Speaker 1>But for people who are are you know, kind of

0:56:33.000 --> 0:56:37.640
<v Speaker 1>concerned about a short election cycle that comes around every

0:56:37.640 --> 0:56:40.120
<v Speaker 1>four to six years or so, or two to six

0:56:40.200 --> 0:56:42.600
<v Speaker 1>years or so, however long, depending upon where you are

0:56:42.600 --> 0:56:45.839
<v Speaker 1>and what position you hold, then saying oh, I want

0:56:45.880 --> 0:56:49.200
<v Speaker 1>to vote for this incredibly expensive endeavor that's going to

0:56:49.239 --> 0:56:52.560
<v Speaker 1>pay off possibly twenty five years down the road is

0:56:52.680 --> 0:56:55.320
<v Speaker 1>a really tough sell. It's a cell that needs to happen,

0:56:55.840 --> 0:56:58.759
<v Speaker 1>but it's a tough one. So anyway, this was fun

0:56:58.800 --> 0:57:00.919
<v Speaker 1>to talk about particle excel raiders and the fact that

0:57:00.920 --> 0:57:03.120
<v Speaker 1>that you know, there's this is stuff that's happening right

0:57:03.160 --> 0:57:07.239
<v Speaker 1>now that's already incredibly exciting, and who knows what could

0:57:07.239 --> 0:57:10.319
<v Speaker 1>be right around the corner or around the bend. I

0:57:10.360 --> 0:57:12.440
<v Speaker 1>guess we should say with in the case of cyclotrons,

0:57:12.920 --> 0:57:15.680
<v Speaker 1>so because you can't have a corner with circles. Uh.

0:57:15.719 --> 0:57:18.160
<v Speaker 1>But if you guys out there have any suggestions for

0:57:18.160 --> 0:57:21.080
<v Speaker 1>a future topics, something that you are really exciting about

0:57:21.160 --> 0:57:23.240
<v Speaker 1>that you want to know more about, let us know.

0:57:23.720 --> 0:57:27.160
<v Speaker 1>Drops the line on Facebook, on Twitter, on Google Plus.

0:57:27.280 --> 0:57:29.400
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0:57:29.400 --> 0:57:32.439
<v Speaker 1>to hearing from you. You hear from us really soon.

0:57:36.640 --> 0:57:39.080
<v Speaker 1>For more on this topic in the future of technology,

0:57:39.400 --> 0:57:52.120
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0:57:52.600 --> 0:57:53.560
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