1 00:00:08,440 --> 00:00:11,760 Speaker 1: Hey, Daniel, how much did the last particle accelerator cost? 2 00:00:12,360 --> 00:00:16,800 Speaker 1: The LHC had a price tag of about ten billion dollars? Oh? 3 00:00:16,920 --> 00:00:18,880 Speaker 1: Is that it? And how much will the next one cost? 4 00:00:19,239 --> 00:00:23,639 Speaker 1: Something like fifty to one hundred billion, depending on the design. 5 00:00:23,880 --> 00:00:26,680 Speaker 1: Fifty to one hundred you can narrow it down a 6 00:00:26,720 --> 00:00:29,680 Speaker 1: little bit. It's a fifty billion dollars difference there, and 7 00:00:29,760 --> 00:00:31,760 Speaker 1: we'd be happy with fifty billion, thank you very much. 8 00:00:31,840 --> 00:00:33,519 Speaker 1: I guess who's going to pay for it? We were 9 00:00:33,520 --> 00:00:36,320 Speaker 1: going to send a request to the cartoonists of the world. 10 00:00:36,479 --> 00:00:39,400 Speaker 1: You want cartoonists to pay for physics? You'd be the 11 00:00:39,440 --> 00:00:42,319 Speaker 1: other way around. I feel like I guess we are 12 00:00:42,400 --> 00:00:46,279 Speaker 1: constantly violating the laws of physics in cartoons, so why 13 00:00:46,320 --> 00:00:48,360 Speaker 1: would you pay us? You guys are just rolling in it, 14 00:00:48,400 --> 00:00:51,080 Speaker 1: aren't you? Rolling in? Some But maybe you should scale 15 00:00:51,080 --> 00:00:53,360 Speaker 1: down your ambitions so it's not as expensive. Well, you know, 16 00:00:53,440 --> 00:00:56,040 Speaker 1: we want to solve the deepest mysteries of the universe. 17 00:00:56,040 --> 00:00:58,920 Speaker 1: How do you scale down those ambitions? Isn't that kind 18 00:00:58,920 --> 00:01:02,960 Speaker 1: of your job? Things? Putting things into perspective, shrinking down 19 00:01:02,960 --> 00:01:05,560 Speaker 1: thanks to the quantum level, and I want to scale 20 00:01:05,600 --> 00:01:08,360 Speaker 1: our ten billion dollar budget to one hundred billion dollars 21 00:01:08,560 --> 00:01:13,640 Speaker 1: in quantum coins or what in bitcoins or cue bitcoins. 22 00:01:13,760 --> 00:01:15,920 Speaker 1: There's definitely a lot of uncertainty in whether we'll ever 23 00:01:15,959 --> 00:01:30,959 Speaker 1: get that money, both the scam and legit kind of currency. 24 00:01:34,680 --> 00:01:37,959 Speaker 1: Hi am Jorhemakirtiness and the creator of PhD comics. Hi. 25 00:01:38,080 --> 00:01:40,560 Speaker 1: I'm Daniel. I'm a particle physicist and a professor at 26 00:01:40,640 --> 00:01:43,640 Speaker 1: UC Irvine, and I want all the science projects to 27 00:01:43,640 --> 00:01:46,759 Speaker 1: get more money, really all of them. I'm sure there 28 00:01:46,760 --> 00:01:49,400 Speaker 1: are some science projects you're like, M, I don't know 29 00:01:49,400 --> 00:01:51,280 Speaker 1: if we should do that. As long as they qualify 30 00:01:51,280 --> 00:01:53,520 Speaker 1: as science projects, I think we should invest in them. 31 00:01:53,520 --> 00:01:56,920 Speaker 1: You know, the big government funding agencies. They get inundated 32 00:01:56,960 --> 00:01:59,400 Speaker 1: in proposals every year, and a lot of them are 33 00:01:59,440 --> 00:02:01,920 Speaker 1: really good ideas that they have to say no too 34 00:02:02,320 --> 00:02:05,080 Speaker 1: because they don't have enough money. Yeah, that is pretty sad. 35 00:02:05,080 --> 00:02:07,960 Speaker 1: There should be more money for science, right. Science is 36 00:02:08,040 --> 00:02:11,400 Speaker 1: usually good, usually right, and your also are pretty good 37 00:02:11,400 --> 00:02:13,280 Speaker 1: at doing something good. Yeah, it doesn't matter if you're 38 00:02:13,320 --> 00:02:16,440 Speaker 1: studying the mating patterns of ducks or the formation of 39 00:02:16,480 --> 00:02:19,240 Speaker 1: the Earth or what's inside black hole. You are feeding 40 00:02:19,240 --> 00:02:22,920 Speaker 1: the curiosity of humanity, and history shows us that that 41 00:02:23,040 --> 00:02:26,959 Speaker 1: is a good investment. So sometimes people pitch scientists against 42 00:02:27,040 --> 00:02:29,720 Speaker 1: other scientists, saying like who should get this money? But 43 00:02:29,840 --> 00:02:32,480 Speaker 1: I think we should all get the money, even the cartoonists. 44 00:02:33,680 --> 00:02:36,639 Speaker 1: The science of cartoons. I guess that's a different agency 45 00:02:36,919 --> 00:02:39,720 Speaker 1: in the government. But anyways, welcome to our podcast Daniel 46 00:02:39,760 --> 00:02:43,280 Speaker 1: and Jorge Explain the Universe, a production of iHeartRadio in 47 00:02:43,320 --> 00:02:45,600 Speaker 1: which we use science to try to push back the 48 00:02:45,639 --> 00:02:49,359 Speaker 1: boundaries of human ignorance. We are amazed at this incredible 49 00:02:49,400 --> 00:02:52,680 Speaker 1: and wonderful and beautiful universe that we find ourselves in, 50 00:02:52,720 --> 00:02:54,720 Speaker 1: but we want to do more than just appreciate it. 51 00:02:54,760 --> 00:02:57,880 Speaker 1: We want to understand it. We want to decode its 52 00:02:57,960 --> 00:03:01,120 Speaker 1: mysteries and explain all of them to you. That's right. 53 00:03:01,160 --> 00:03:03,520 Speaker 1: It is a pretty amazing universe. And if you invest 54 00:03:03,600 --> 00:03:05,720 Speaker 1: in our of your time here with us today, we 55 00:03:05,960 --> 00:03:09,280 Speaker 1: hopefully we'll give your returns in terms of you understanding 56 00:03:09,280 --> 00:03:13,400 Speaker 1: how things work and appreciating this amazing and beautiful cosmos 57 00:03:13,520 --> 00:03:15,480 Speaker 1: that we live in. That's right. Although you're welcome to 58 00:03:15,480 --> 00:03:17,359 Speaker 1: invest more than just an hour of your time. Send 59 00:03:17,480 --> 00:03:20,000 Speaker 1: us some cash, no problem. Do you take bitcoins or 60 00:03:20,080 --> 00:03:24,280 Speaker 1: cue bitcoins, Hey, I'll take any donations from my science 61 00:03:24,320 --> 00:03:28,120 Speaker 1: absolutely make out a check just too expressive, Daniel. Have 62 00:03:28,120 --> 00:03:30,560 Speaker 1: you thought of maybe if you reduce your prices, people 63 00:03:30,600 --> 00:03:32,840 Speaker 1: will invest more in it. I would love to make 64 00:03:32,880 --> 00:03:35,800 Speaker 1: science cheaper. You know, something that limits our understanding the 65 00:03:35,880 --> 00:03:39,119 Speaker 1: universe is really just how much money we spend on it. 66 00:03:39,120 --> 00:03:41,800 Speaker 1: It's like we're in the science candy store and we 67 00:03:41,920 --> 00:03:43,960 Speaker 1: just have pennies in our pockets. But if we could 68 00:03:44,000 --> 00:03:46,240 Speaker 1: figure out a way and make it all cheaper than wow, 69 00:03:46,280 --> 00:03:49,240 Speaker 1: we could just buy more secrets of the universe. What 70 00:03:49,360 --> 00:03:51,960 Speaker 1: a day that would be. Yeah, it sounds awesome, although 71 00:03:52,000 --> 00:03:54,640 Speaker 1: they say it all starts with the individuals, Daniel. So 72 00:03:54,960 --> 00:03:57,720 Speaker 1: you know, should we tell your university to cut your 73 00:03:57,720 --> 00:04:04,800 Speaker 1: salary so I should do half as much physics? Well, 74 00:04:05,000 --> 00:04:06,680 Speaker 1: you know you could do twice as much for half 75 00:04:06,720 --> 00:04:11,720 Speaker 1: the price. Yeah, and then I'll eat half as much. Right, Sorry, kids, 76 00:04:11,720 --> 00:04:14,520 Speaker 1: you're not eating today. It's a Tuesday, and it's for science, 77 00:04:14,800 --> 00:04:17,040 Speaker 1: so you could do it too. For Yeah, you could 78 00:04:17,160 --> 00:04:20,560 Speaker 1: do a hunger experiment and also make size cheaper. For 79 00:04:20,880 --> 00:04:24,800 Speaker 1: you know, the mating patterns of certain animals in certain places. 80 00:04:24,960 --> 00:04:27,160 Speaker 1: Sounds like we could learn a lot, but learn we 81 00:04:27,240 --> 00:04:29,839 Speaker 1: do aim to do here on the podcast and so 82 00:04:30,000 --> 00:04:32,840 Speaker 1: there's the rest of humanity in terms of understanding the universe, 83 00:04:32,920 --> 00:04:35,560 Speaker 1: from the immense galaxies out there floating in space to 84 00:04:35,640 --> 00:04:38,240 Speaker 1: the tiny little particles that make up your body and 85 00:04:38,360 --> 00:04:41,040 Speaker 1: everything that you touch on an everyday basis. That's right, 86 00:04:41,080 --> 00:04:43,719 Speaker 1: and we have a few ways of understanding the universe. 87 00:04:44,120 --> 00:04:46,279 Speaker 1: One thing we can do is just look out into 88 00:04:46,320 --> 00:04:49,479 Speaker 1: the universe and find interesting stuff that's happening and try 89 00:04:49,560 --> 00:04:52,560 Speaker 1: to learn from it. That's what astrophysicists have to do, 90 00:04:52,600 --> 00:04:55,200 Speaker 1: because as much as they want to shoot black holes 91 00:04:55,200 --> 00:04:57,799 Speaker 1: at each other, they don't have a black hole collider, 92 00:04:57,960 --> 00:05:00,400 Speaker 1: so they have to wait for nature to set up 93 00:05:00,400 --> 00:05:02,760 Speaker 1: and do it for them. The other approach, of course, 94 00:05:02,920 --> 00:05:04,919 Speaker 1: is to try to create the conditions we want to 95 00:05:04,920 --> 00:05:08,240 Speaker 1: study here on Earth, to set up the experiments that 96 00:05:08,320 --> 00:05:11,360 Speaker 1: might force the universe to reveal one of its secrets 97 00:05:11,360 --> 00:05:13,760 Speaker 1: to us. Yeah, and one of those strategies is to 98 00:05:14,200 --> 00:05:18,440 Speaker 1: basically smash things together, is to collide tiny little particles 99 00:05:18,440 --> 00:05:20,240 Speaker 1: and kind of see how you can break them. I 100 00:05:20,240 --> 00:05:21,680 Speaker 1: guess that's kind of what you're trying to do, right, 101 00:05:21,800 --> 00:05:23,920 Speaker 1: is you're trying to break little particles. Yeah, we are 102 00:05:23,920 --> 00:05:26,560 Speaker 1: trying to break little particles. Essentially, we are trying to 103 00:05:26,600 --> 00:05:29,800 Speaker 1: create new conditions that reveal the laws of physics. You know, 104 00:05:29,839 --> 00:05:32,080 Speaker 1: we have a lot of experience with sort of slow 105 00:05:32,240 --> 00:05:36,280 Speaker 1: moving cold stuff like baseballs flying through the air or 106 00:05:36,320 --> 00:05:39,360 Speaker 1: things swimming through the ocean. Things aren't moving very very fast, 107 00:05:39,560 --> 00:05:41,400 Speaker 1: they don't have a whole lot of energy. So we 108 00:05:41,440 --> 00:05:43,640 Speaker 1: think we understand that kind of physics. But we want 109 00:05:43,680 --> 00:05:46,160 Speaker 1: to understand the physics of the whole universe. We want 110 00:05:46,200 --> 00:05:49,039 Speaker 1: to understand what happens when you push things really really far, 111 00:05:49,160 --> 00:05:51,599 Speaker 1: when you get really really small. And in order to 112 00:05:51,640 --> 00:05:53,920 Speaker 1: do that, we have to create those conditions. So we 113 00:05:53,960 --> 00:05:57,240 Speaker 1: smash tiny particles together to make these really dense little 114 00:05:57,279 --> 00:05:59,720 Speaker 1: blobs of energy that we hope reveal what the sort 115 00:05:59,720 --> 00:06:03,160 Speaker 1: of underlying truths of the universe is. I guess, yeah, 116 00:06:03,200 --> 00:06:05,400 Speaker 1: you're not really trying to break particles. You're trying to 117 00:06:05,440 --> 00:06:08,479 Speaker 1: kind of smush them together and then see what the 118 00:06:08,640 --> 00:06:11,440 Speaker 1: universe does with that smooth the energy. Yeah, when particles 119 00:06:11,480 --> 00:06:14,360 Speaker 1: get really close together, they interact, and that interaction can 120 00:06:14,400 --> 00:06:17,560 Speaker 1: create new kinds of particles. One of the most amazing 121 00:06:17,640 --> 00:06:21,359 Speaker 1: things about particle collisions is that it's not like chemistry. 122 00:06:21,480 --> 00:06:23,800 Speaker 1: When you're doing chemistry, you combine like H two and 123 00:06:23,920 --> 00:06:26,680 Speaker 1: O two to make water. All the bits that went 124 00:06:26,760 --> 00:06:30,000 Speaker 1: in just get rearranged. Right, Every hydrogen nucleus that was 125 00:06:30,040 --> 00:06:32,840 Speaker 1: there is still there. Every oxygen atom that was there 126 00:06:33,080 --> 00:06:35,680 Speaker 1: is still there. But when we do particle collisions, that's 127 00:06:35,680 --> 00:06:38,160 Speaker 1: not what happens. What comes out of the collisions, it's 128 00:06:38,200 --> 00:06:40,960 Speaker 1: not just like a rearrangement of the bits that went 129 00:06:41,000 --> 00:06:44,160 Speaker 1: in like some big Lego project. Those particles that go 130 00:06:44,200 --> 00:06:48,559 Speaker 1: into the collisions, they get literally annihilated and turned into 131 00:06:48,640 --> 00:06:51,800 Speaker 1: new kinds of matter. So we're not doing chemistry. We're 132 00:06:51,839 --> 00:06:55,400 Speaker 1: doing alchemy. Although that's kind of what you think is happening, right, Like, 133 00:06:55,600 --> 00:06:57,680 Speaker 1: you don't know, you're not quite sure. Maybe inside of 134 00:06:57,720 --> 00:07:00,360 Speaker 1: those little tiny particles are tiny little strength that do 135 00:07:00,480 --> 00:07:03,600 Speaker 1: get kind of rearranged like legos. Isn't that a possibility? Absolutely, 136 00:07:03,600 --> 00:07:05,640 Speaker 1: that's right. There are many layers to our picture of 137 00:07:05,640 --> 00:07:08,320 Speaker 1: the universe. Currently, we think about the particles that are 138 00:07:08,320 --> 00:07:11,200 Speaker 1: interacting those quarks and the electrons as if they are 139 00:07:11,200 --> 00:07:14,680 Speaker 1: fundamental objects. But it certainly might be that they are emerging, 140 00:07:14,760 --> 00:07:17,800 Speaker 1: that there are combinations of even smaller things, and so 141 00:07:17,880 --> 00:07:20,560 Speaker 1: then what it means to annihilate that particle is in fact, 142 00:07:20,600 --> 00:07:23,040 Speaker 1: to break it into its smaller components, which then can 143 00:07:23,240 --> 00:07:25,960 Speaker 1: rearrange themselves. But if we can do that, then we 144 00:07:26,040 --> 00:07:29,840 Speaker 1: hope to smash those components together and maybe annihilate them, 145 00:07:30,000 --> 00:07:32,480 Speaker 1: and eventually we think when you get down to the 146 00:07:32,640 --> 00:07:35,720 Speaker 1: universe and its most basic building block, what you're really 147 00:07:35,760 --> 00:07:40,480 Speaker 1: doing is annihilation of fundamental objects. So you're an annihilist 148 00:07:41,040 --> 00:07:46,320 Speaker 1: at heart, you're an annihilist physicist, I am an annihilist, absolutely, Yeah, 149 00:07:46,520 --> 00:07:49,200 Speaker 1: you subscribe to annihilism. Hey, at least it's an ethos, right, 150 00:07:49,360 --> 00:07:51,000 Speaker 1: you should come up with your own kind of a 151 00:07:51,080 --> 00:07:54,360 Speaker 1: punk rock music for that. But smashing these things together, 152 00:07:54,400 --> 00:07:56,120 Speaker 1: I guess it's one thing that you can learn how 153 00:07:56,160 --> 00:07:59,360 Speaker 1: things work, because I guess when things are that small, 154 00:07:59,520 --> 00:08:02,800 Speaker 1: you can't take a pair of tweezers and pry them open, right, Like, 155 00:08:02,880 --> 00:08:04,760 Speaker 1: That's kind of the only way you can really see 156 00:08:04,760 --> 00:08:08,480 Speaker 1: what's inside of some of these fundamental particles. Yeah, and 157 00:08:08,520 --> 00:08:10,520 Speaker 1: you really put your finger there on what we're trying 158 00:08:10,560 --> 00:08:13,720 Speaker 1: to do. We're trying to see inside these particles. I mean, 159 00:08:13,760 --> 00:08:16,000 Speaker 1: from one perspective, you could say you're annihilating them. From 160 00:08:16,040 --> 00:08:18,880 Speaker 1: another perspective, you could say you're tearing them open. You're 161 00:08:18,920 --> 00:08:21,720 Speaker 1: destroying the arrangement of whatever the smaller bits are, that 162 00:08:21,880 --> 00:08:23,880 Speaker 1: is the electron or the quark. In the end, what 163 00:08:23,880 --> 00:08:26,360 Speaker 1: we're trying to do is pull them apart, and fundamentally, 164 00:08:26,360 --> 00:08:30,080 Speaker 1: it's not that different from using tweezers. What do tweezers do. 165 00:08:30,360 --> 00:08:33,400 Speaker 1: They apply a lot of force in one's very specific 166 00:08:33,480 --> 00:08:36,200 Speaker 1: energy in order to break some bonds, and that's exactly 167 00:08:36,280 --> 00:08:38,439 Speaker 1: what we're trying to do with these particles. We smash 168 00:08:38,520 --> 00:08:41,319 Speaker 1: one proton against the other one, hoping that the high 169 00:08:41,480 --> 00:08:44,720 Speaker 1: energy that the proton has will smash open the other proton, 170 00:08:44,800 --> 00:08:47,880 Speaker 1: revealing what's inside of it, and maybe even the quark 171 00:08:48,000 --> 00:08:51,600 Speaker 1: smashing together will reveal what's inside of them. Well, smashing 172 00:08:51,640 --> 00:08:54,000 Speaker 1: you have been doing at the Large Hadron collider or 173 00:08:54,080 --> 00:08:56,320 Speaker 1: you were right now you have sort of an appointment there, 174 00:08:56,440 --> 00:08:58,880 Speaker 1: that's right. My main research program when I'm not gooving 175 00:08:58,880 --> 00:09:02,760 Speaker 1: off doing podcasts or other projects, is annihilating protons at 176 00:09:02,800 --> 00:09:05,920 Speaker 1: the Large Hadron collider. I'm remember the Atlas experiment, which 177 00:09:05,960 --> 00:09:09,480 Speaker 1: has built a huge electronic device which wraps around the 178 00:09:09,520 --> 00:09:12,000 Speaker 1: point of collisions to take pictures of all the particles 179 00:09:12,000 --> 00:09:14,520 Speaker 1: that fly out and try to learn things about what 180 00:09:14,679 --> 00:09:17,400 Speaker 1: happened in all of those collisions. Yeah, And the whole 181 00:09:17,400 --> 00:09:21,200 Speaker 1: point of the accelerator is to basically accelerate particles. You're 182 00:09:21,200 --> 00:09:25,080 Speaker 1: speeding up the particles from standing still to almost at 183 00:09:25,080 --> 00:09:27,080 Speaker 1: the speed of light, or at least at a very 184 00:09:27,160 --> 00:09:30,000 Speaker 1: high velocity, and then you smash it together to get 185 00:09:30,080 --> 00:09:32,400 Speaker 1: higher and higher energies. But I guess maybe the problem 186 00:09:32,440 --> 00:09:34,600 Speaker 1: is that the LHC is kind of showing its age 187 00:09:34,679 --> 00:09:37,600 Speaker 1: now a little bit. Yeah, that's right. The LHC is big, 188 00:09:37,640 --> 00:09:40,880 Speaker 1: and it's powerful, and it was expensive, but it's also 189 00:09:41,160 --> 00:09:43,760 Speaker 1: limited in its ability. The way we talk about these 190 00:09:43,800 --> 00:09:47,800 Speaker 1: accelerators is basically by quoting their top speed the most 191 00:09:48,080 --> 00:09:50,800 Speaker 1: energy that we can put into the particles that we're 192 00:09:50,800 --> 00:09:54,160 Speaker 1: smashing together. The reason that that's the most interesting number, 193 00:09:54,200 --> 00:09:57,160 Speaker 1: the one that really tells us like the discovery potential 194 00:09:57,280 --> 00:09:59,520 Speaker 1: of this device, is because it limits the kind of 195 00:09:59,520 --> 00:10:02,280 Speaker 1: things that it can create. Like, you take those two particles, 196 00:10:02,360 --> 00:10:04,880 Speaker 1: you smash them together. What else can you make? Well, 197 00:10:04,880 --> 00:10:07,280 Speaker 1: you might be able to have two other electrons come out, 198 00:10:07,360 --> 00:10:09,679 Speaker 1: or two other quarks, or something else we already know about. 199 00:10:10,080 --> 00:10:12,560 Speaker 1: But if you have enough energy, you might be able 200 00:10:12,559 --> 00:10:16,800 Speaker 1: to build something new. Something we haven't seen before because 201 00:10:16,840 --> 00:10:21,280 Speaker 1: it requires more energy density than typically exists in the universe. 202 00:10:21,360 --> 00:10:23,600 Speaker 1: So the more energy you have in your collider, the 203 00:10:23,679 --> 00:10:27,599 Speaker 1: more you have access to like Nature's hidden menu of particles, 204 00:10:27,840 --> 00:10:31,080 Speaker 1: things that can exist in the universe but don't typically 205 00:10:31,280 --> 00:10:34,200 Speaker 1: because there aren't the conditions to make them. So the 206 00:10:34,360 --> 00:10:36,920 Speaker 1: LATEC is big and it's powerful, but it doesn't have 207 00:10:37,080 --> 00:10:39,480 Speaker 1: infinite energy. Yeah. Well, at the time it was built, 208 00:10:39,520 --> 00:10:41,880 Speaker 1: it did sort of break I mean, it definitely broke 209 00:10:41,960 --> 00:10:43,960 Speaker 1: new ground in terms of how much energy you could 210 00:10:43,960 --> 00:10:46,960 Speaker 1: get in an experiment. But I guess you random LAC 211 00:10:47,200 --> 00:10:50,040 Speaker 1: and it found the exploson and all these amazing discoveries, 212 00:10:50,080 --> 00:10:52,280 Speaker 1: and now you're kind of thinking about what's next, how 213 00:10:52,320 --> 00:10:54,840 Speaker 1: can we get more energy? Yeah, we're always thinking about 214 00:10:54,840 --> 00:10:57,240 Speaker 1: what's next. The collider that came just before the LATEC 215 00:10:57,640 --> 00:11:01,000 Speaker 1: was just outside Chicago is the Tevatron about two terra 216 00:11:01,080 --> 00:11:04,720 Speaker 1: electron volts and the Large Hadron Collider has about thirteen 217 00:11:04,960 --> 00:11:08,280 Speaker 1: tera electron volts. And that's a big jump, right, that's 218 00:11:08,320 --> 00:11:11,200 Speaker 1: like almost a factor of seven in terms of the 219 00:11:11,320 --> 00:11:15,360 Speaker 1: territory we could explore and imagine, for example, multiplying the 220 00:11:15,480 --> 00:11:18,000 Speaker 1: territory you've explored by a factor of seven. If you're 221 00:11:18,040 --> 00:11:22,360 Speaker 1: in the field of like geology or planetary astronomy, you've 222 00:11:22,360 --> 00:11:25,240 Speaker 1: only ever looked at Earth, and now you can simultaneously 223 00:11:25,280 --> 00:11:27,839 Speaker 1: land on seven new planets all at the same time 224 00:11:27,840 --> 00:11:30,160 Speaker 1: and see what's there and learn all about it. So 225 00:11:30,200 --> 00:11:32,800 Speaker 1: when we turned on the Large Hadron Collider, it's like 226 00:11:32,840 --> 00:11:35,680 Speaker 1: we multiplied by a factor of seven the sort of 227 00:11:35,840 --> 00:11:39,280 Speaker 1: size of the particle universe that we were able to 228 00:11:39,360 --> 00:11:41,240 Speaker 1: explore and to look at, and we didn't know what 229 00:11:41,400 --> 00:11:43,840 Speaker 1: was there. Every time we do these kinds of explorations, 230 00:11:44,080 --> 00:11:47,120 Speaker 1: there could be huge surprises waiting for us, or sort 231 00:11:47,160 --> 00:11:49,440 Speaker 1: of nothing. And as you say, we found the Higgs boson, 232 00:11:49,679 --> 00:11:51,680 Speaker 1: but we've been running for quite a few years and 233 00:11:51,720 --> 00:11:54,400 Speaker 1: we haven't found anything else since then. Now we're wondering, like, hmm, 234 00:11:54,760 --> 00:11:58,200 Speaker 1: what's around the next corner if we crack open another 235 00:11:58,400 --> 00:12:01,760 Speaker 1: energy range, will there be for easy discoveries waiting for us, 236 00:12:02,280 --> 00:12:05,160 Speaker 1: or just more dust and rubble. Yeah, So the LC 237 00:12:05,320 --> 00:12:07,760 Speaker 1: sort of got you to a certain level, which was amazing, 238 00:12:07,920 --> 00:12:10,640 Speaker 1: But I guess you feel like you've already explored this level. 239 00:12:10,840 --> 00:12:13,440 Speaker 1: You've looked into every corner of this energy level, and 240 00:12:13,640 --> 00:12:18,120 Speaker 1: you're kind of feeling like there's nothing else here. That's 241 00:12:18,160 --> 00:12:21,719 Speaker 1: a very delicate political question as we seek approval for 242 00:12:21,800 --> 00:12:24,400 Speaker 1: running the large changer on cloder for another fifteen years, 243 00:12:24,520 --> 00:12:27,079 Speaker 1: because we're trying to make the science case that running 244 00:12:27,120 --> 00:12:29,520 Speaker 1: it for a lot longer can look for really rare 245 00:12:29,960 --> 00:12:33,000 Speaker 1: particles that maybe we missed in sort of the first scoop. 246 00:12:33,080 --> 00:12:34,920 Speaker 1: So we're sort of going in two directions at once. 247 00:12:35,520 --> 00:12:37,400 Speaker 1: One group of people is like, let's run this thing 248 00:12:37,440 --> 00:12:39,760 Speaker 1: for as long as possible and maybe look for really 249 00:12:39,840 --> 00:12:41,680 Speaker 1: rare stuff we might have missed, and the other group 250 00:12:41,760 --> 00:12:44,439 Speaker 1: is looking towards the future and saying, can we build 251 00:12:44,440 --> 00:12:47,960 Speaker 1: the next one? Can we plan now for the super LHC? 252 00:12:48,440 --> 00:12:52,600 Speaker 1: The super LHC nice sounds like a like a superhero. Well, 253 00:12:52,640 --> 00:12:55,640 Speaker 1: I guess the problem is that the LC was it's big, 254 00:12:55,760 --> 00:12:57,880 Speaker 1: and it was a little expensive. But now if you 255 00:12:57,920 --> 00:13:00,840 Speaker 1: want to get into higher energies, it gets even bigger 256 00:13:00,840 --> 00:13:04,479 Speaker 1: and more expensive, right with the same technology it does. Basically, 257 00:13:04,520 --> 00:13:07,680 Speaker 1: the only thing that limits us from building a bigger accelerator, 258 00:13:07,800 --> 00:13:11,280 Speaker 1: or from having built one instead of the LATEC is money. 259 00:13:11,400 --> 00:13:13,920 Speaker 1: The cost of the accelerator just scales with the size, 260 00:13:14,240 --> 00:13:16,160 Speaker 1: sort of like building a highway. It's like a million 261 00:13:16,240 --> 00:13:19,520 Speaker 1: dollars per mile. More miles means some more millions of dollars. 262 00:13:19,520 --> 00:13:21,360 Speaker 1: So you want more energy, you've got to build a 263 00:13:21,400 --> 00:13:25,280 Speaker 1: bigger collider, which costs more money. And so now people 264 00:13:25,280 --> 00:13:28,360 Speaker 1: are wondering, like, should we just spend ten times as 265 00:13:28,440 --> 00:13:30,880 Speaker 1: much money on a super duper version of this or 266 00:13:31,320 --> 00:13:33,920 Speaker 1: should we figure out a cheaper way to do it? Yeah, 267 00:13:33,960 --> 00:13:36,760 Speaker 1: because I guess, first of all, you'll know that I say, 268 00:13:36,840 --> 00:13:39,320 Speaker 1: with the existing technology, it's going to be a bigger 269 00:13:39,320 --> 00:13:42,360 Speaker 1: and more expensive and also I don't think most scientists 270 00:13:42,360 --> 00:13:45,360 Speaker 1: are going to cut their salary and have it makes 271 00:13:46,160 --> 00:13:48,440 Speaker 1: a cheaper endeavor. So I guess, like you said, we 272 00:13:48,520 --> 00:13:51,800 Speaker 1: have to start looking at maybe new technologies. So today 273 00:13:51,800 --> 00:13:58,920 Speaker 1: on the podcast, we'll be asking the question, is there 274 00:13:58,960 --> 00:14:02,960 Speaker 1: a better way to accelerate particles? I guess that you've 275 00:14:02,960 --> 00:14:05,680 Speaker 1: been using one way to accelerate particles all this time 276 00:14:05,800 --> 00:14:08,640 Speaker 1: or several ways. Right, We've been accelerating particles since about 277 00:14:08,640 --> 00:14:11,800 Speaker 1: the nineteen thirties, and we've had a series of sort 278 00:14:11,800 --> 00:14:14,800 Speaker 1: of technological revolutions. People come up with a new idea 279 00:14:14,880 --> 00:14:16,600 Speaker 1: to make them more powerful, and we get like a 280 00:14:16,640 --> 00:14:19,120 Speaker 1: big jump in energy we're sort of at the end 281 00:14:19,200 --> 00:14:21,080 Speaker 1: of one of those cycles. We've been doing it the 282 00:14:21,120 --> 00:14:23,040 Speaker 1: same way for a few decades now, and we can 283 00:14:23,080 --> 00:14:26,480 Speaker 1: get sort of like little incremental increases without just making 284 00:14:26,520 --> 00:14:29,000 Speaker 1: it bigger, and so it sort of feels like about 285 00:14:29,000 --> 00:14:30,880 Speaker 1: the time that we need to jump to the next 286 00:14:30,920 --> 00:14:34,240 Speaker 1: technology and figure out like a whole new way to 287 00:14:34,320 --> 00:14:36,520 Speaker 1: do this kind of thing. Yeah, like, if maybe the 288 00:14:36,520 --> 00:14:39,480 Speaker 1: engineers figure out a better way to get particles moving, 289 00:14:39,560 --> 00:14:42,080 Speaker 1: you could maybe make accelerators that are at the same 290 00:14:42,200 --> 00:14:44,640 Speaker 1: energy or more but a lot cheaper, right, That's the 291 00:14:44,640 --> 00:14:46,920 Speaker 1: whole point, And maybe eventually you'll just have it on 292 00:14:46,920 --> 00:14:52,240 Speaker 1: your phone. Eventually there's an app for that, perhaps for 293 00:14:52,360 --> 00:14:56,320 Speaker 1: shooting lightspeed particles from your phone. That seems usable. Well, 294 00:14:56,360 --> 00:14:58,360 Speaker 1: you do have a light speed accelerator on your phone 295 00:14:58,440 --> 00:15:01,120 Speaker 1: right now, I mean you have a flashlight literally shoots 296 00:15:01,160 --> 00:15:04,640 Speaker 1: out particles at light speed. Unfortunately not high enough energy 297 00:15:04,680 --> 00:15:07,440 Speaker 1: to do any interesting physics. But yeah, the dream is like, 298 00:15:07,800 --> 00:15:10,600 Speaker 1: instead of having to collaborate with five thousand people from 299 00:15:10,600 --> 00:15:12,800 Speaker 1: all over the world on a ten billion dollar project, 300 00:15:12,880 --> 00:15:15,480 Speaker 1: why can't I just build this thing on a tabletop 301 00:15:15,560 --> 00:15:17,680 Speaker 1: in my own basement or in my lab here at 302 00:15:17,680 --> 00:15:20,360 Speaker 1: you see Irvine for two hundred thousand dollars or something 303 00:15:20,400 --> 00:15:23,200 Speaker 1: and run my own experiments. Why can't everybody have their 304 00:15:23,320 --> 00:15:27,040 Speaker 1: own plank scale particle collider to explore the nature of 305 00:15:27,080 --> 00:15:31,400 Speaker 1: the universe? Well, I can't, and why shouldn't have? But 306 00:15:31,520 --> 00:15:34,800 Speaker 1: that's not the topic today. The topic is can that happen? Like, 307 00:15:34,880 --> 00:15:37,120 Speaker 1: can you imagine a future where you can have a 308 00:15:37,240 --> 00:15:40,760 Speaker 1: particle collider that's as powerful as the LHC, which is huge, 309 00:15:40,760 --> 00:15:44,320 Speaker 1: which is several kilometers along and underground. Can you maybe 310 00:15:44,360 --> 00:15:46,840 Speaker 1: have that in like a little box in your basement. 311 00:15:46,960 --> 00:15:49,040 Speaker 1: It's such a dream. I mean, imagine all of the 312 00:15:49,120 --> 00:15:52,200 Speaker 1: secrets we could learn, those secrets that are just out 313 00:15:52,200 --> 00:15:55,000 Speaker 1: there waiting for us if we only have the technology 314 00:15:55,040 --> 00:15:56,840 Speaker 1: to crack them open. It's like we're in a room 315 00:15:56,880 --> 00:15:59,520 Speaker 1: surrounded by locked boxes and we just don't have the 316 00:15:59,640 --> 00:16:01,880 Speaker 1: key to any of them. You need engineers to save 317 00:16:01,960 --> 00:16:06,320 Speaker 1: users say, we definitely do need the engineers working closely 318 00:16:06,320 --> 00:16:08,640 Speaker 1: with a physicist to figure this all out. Well, it's 319 00:16:08,680 --> 00:16:10,520 Speaker 1: usually we were wondering how many people have thought about 320 00:16:10,560 --> 00:16:13,160 Speaker 1: this question of whether or not there's maybe a better 321 00:16:13,200 --> 00:16:16,560 Speaker 1: way to accelerate particles. So thank you to everybody who 322 00:16:16,640 --> 00:16:19,160 Speaker 1: answers these questions for the podcast to give us a 323 00:16:19,200 --> 00:16:21,760 Speaker 1: sense for what people are thinking and what they already know. 324 00:16:21,960 --> 00:16:24,840 Speaker 1: If you'd like to participate for a future episode, please 325 00:16:24,960 --> 00:16:27,600 Speaker 1: don't be shy. Right to meet two questions at Daniel 326 00:16:27,720 --> 00:16:30,000 Speaker 1: Nhorge dot com. So think about it for a second. 327 00:16:30,040 --> 00:16:32,760 Speaker 1: Do you think there's a better way to accelerate particles. 328 00:16:33,440 --> 00:16:36,400 Speaker 1: Here's what people had to say. My understanding of current 329 00:16:36,400 --> 00:16:41,400 Speaker 1: method is that we apply electromagnetic field to accelerate a particle, 330 00:16:41,600 --> 00:16:47,160 Speaker 1: and then they are propelled in high velocities in a tunnel. 331 00:16:47,680 --> 00:16:49,840 Speaker 1: I'm not sure if there is any other way that 332 00:16:49,880 --> 00:16:52,160 Speaker 1: this could be done. There must be, of course, but 333 00:16:52,360 --> 00:16:54,920 Speaker 1: I don't think it will be that control and this 334 00:16:55,040 --> 00:16:57,280 Speaker 1: might be more physical when I have no clue how 335 00:16:57,320 --> 00:16:59,400 Speaker 1: that can be done well right away, I think about 336 00:16:59,400 --> 00:17:03,200 Speaker 1: the fact that particles go to incredible speeds when they're 337 00:17:03,280 --> 00:17:07,240 Speaker 1: orbiting a black hole in the ucretion disk. So maybe 338 00:17:07,280 --> 00:17:09,720 Speaker 1: gravity would be a better way to accelerate particles. I 339 00:17:09,840 --> 00:17:12,119 Speaker 1: just have no idea how we would go about doing that. 340 00:17:12,680 --> 00:17:16,040 Speaker 1: I think a better way to accelerate particles might be 341 00:17:16,320 --> 00:17:20,960 Speaker 1: to give it more energy or like heat, because if 342 00:17:20,960 --> 00:17:22,639 Speaker 1: you have a lot of energy you're going to be 343 00:17:22,760 --> 00:17:25,280 Speaker 1: moving fast. It also works the same way with heat, 344 00:17:25,280 --> 00:17:26,920 Speaker 1: because like if you're cold, you don't want to move, 345 00:17:26,960 --> 00:17:29,199 Speaker 1: you stay in the same place. I suppose if you 346 00:17:29,200 --> 00:17:33,159 Speaker 1: could get yourself a mini black hole and rip the 347 00:17:33,240 --> 00:17:37,080 Speaker 1: particles around the event horizon, they might speed up pretty good. 348 00:17:37,880 --> 00:17:40,200 Speaker 1: I was wondering when I asked these questions, what if 349 00:17:40,240 --> 00:17:43,240 Speaker 1: somebody actually came up with some super genius way to 350 00:17:43,320 --> 00:17:45,720 Speaker 1: do this, would I end up like collaborating with them, 351 00:17:45,840 --> 00:17:47,800 Speaker 1: or like, would they get the patent for it? I 352 00:17:47,840 --> 00:17:51,119 Speaker 1: mean it could have been Thorny whoa like would you 353 00:17:51,119 --> 00:17:53,040 Speaker 1: have to pay them as some of your salary? That 354 00:17:53,080 --> 00:17:57,520 Speaker 1: would be such a difficult question. I'd hire them on 355 00:17:57,560 --> 00:18:00,560 Speaker 1: the spot. Absolutely. There are some pretty interesting ideas here. 356 00:18:00,640 --> 00:18:03,800 Speaker 1: I think maybe there are, you know, maybe the next 357 00:18:03,880 --> 00:18:06,960 Speaker 1: big idea. It wasn't one of those answers. You think 358 00:18:06,960 --> 00:18:10,639 Speaker 1: the mini black hole is the solution of the problem. Yeah, 359 00:18:10,680 --> 00:18:14,200 Speaker 1: First build a super collider to create mini black holes. 360 00:18:14,240 --> 00:18:17,560 Speaker 1: Then use those mini black holes to accelerate particles. It's 361 00:18:17,600 --> 00:18:20,000 Speaker 1: like a bootstrap. Yeah yeah. Or gravity. That was kind 362 00:18:20,000 --> 00:18:22,080 Speaker 1: of an interesting idea. I mean, we use gravity all 363 00:18:22,080 --> 00:18:26,040 Speaker 1: the time to accelerate spacecraft, right, We definitely do use gravity, absolutely, 364 00:18:26,040 --> 00:18:29,479 Speaker 1: and gravity does accelerate particles like particles fall towards the 365 00:18:29,480 --> 00:18:32,080 Speaker 1: Earth all the time. They're called cosmic rays, and they 366 00:18:32,080 --> 00:18:36,480 Speaker 1: actually do achieve super high energies and create massive collisions 367 00:18:36,560 --> 00:18:39,480 Speaker 1: in the atmosphere that physicists study and used to try 368 00:18:39,520 --> 00:18:42,760 Speaker 1: to understand how particles interact and what it all means. 369 00:18:43,080 --> 00:18:45,679 Speaker 1: But those are a little more difficult to control. All right, Well, 370 00:18:45,680 --> 00:18:49,399 Speaker 1: it's an interesting question. How do we accelerate particles faster, cheaper, 371 00:18:49,480 --> 00:18:52,280 Speaker 1: and better? I guess cheaper, faster better? Isn't that the 372 00:18:52,320 --> 00:18:55,160 Speaker 1: goal of any industry exactly? And then making an app 373 00:18:55,280 --> 00:18:57,840 Speaker 1: how do we do physics cheaper, faster, bet Well, maybe 374 00:18:57,880 --> 00:19:01,080 Speaker 1: a step us through here, how do we currently accelerate particles? 375 00:19:01,080 --> 00:19:04,040 Speaker 1: Like how does the LHC exactly? How does it get 376 00:19:04,080 --> 00:19:05,919 Speaker 1: particles moving so fast? Well, I don't know if that 377 00:19:05,960 --> 00:19:09,040 Speaker 1: pun was intended or not, but we currently use electrical 378 00:19:09,080 --> 00:19:13,240 Speaker 1: currents to accelerate particles. Yes, that was totally on purpose. 379 00:19:13,720 --> 00:19:15,720 Speaker 1: I wasn't trying to app anything up or anything. I'm 380 00:19:15,720 --> 00:19:19,200 Speaker 1: just trying to be a positive, reinforcing partner on the podcast. Yes, 381 00:19:19,280 --> 00:19:21,640 Speaker 1: I'm just I'm also just trying to you know, kind 382 00:19:21,640 --> 00:19:23,640 Speaker 1: of work the field here. This is why we don't 383 00:19:23,720 --> 00:19:27,320 Speaker 1: charge for this podcast. Let's stop with the electrifinally terrible 384 00:19:27,800 --> 00:19:31,320 Speaker 1: punts here, Let's get down in nuts and bolts. How 385 00:19:31,359 --> 00:19:33,920 Speaker 1: are those nuts and bolts put together? In the LHC 386 00:19:34,200 --> 00:19:37,560 Speaker 1: moving past our magnetic senses of humor. Essentially, we can 387 00:19:37,640 --> 00:19:41,600 Speaker 1: only accelerate charged particles, and the reason is that we 388 00:19:41,800 --> 00:19:44,639 Speaker 1: use electric fields in order to do it. Electric fields 389 00:19:44,680 --> 00:19:48,120 Speaker 1: can tug on charge particles. That's essentially what they are. 390 00:19:48,320 --> 00:19:51,320 Speaker 1: And so the basics is, you want a particle moving fast, 391 00:19:51,400 --> 00:19:54,120 Speaker 1: you put it in an electric field. The voltage there 392 00:19:54,240 --> 00:19:57,800 Speaker 1: will accelerate the particle in one direction. That's like the 393 00:19:57,920 --> 00:20:02,200 Speaker 1: super basic initial version of a particle accelerator. Meaning basically 394 00:20:02,200 --> 00:20:04,600 Speaker 1: you set up like a magnet, right, and then you 395 00:20:04,600 --> 00:20:08,400 Speaker 1: have the magnet attract charge particles, and then that gets 396 00:20:08,400 --> 00:20:11,000 Speaker 1: the moving. Well, we do have magnets, but magnets actually 397 00:20:11,000 --> 00:20:13,960 Speaker 1: cannot accelerate particles. They can only bend them. They can 398 00:20:14,080 --> 00:20:16,760 Speaker 1: change their direction, but they can't speed them up. But 399 00:20:16,800 --> 00:20:20,920 Speaker 1: an electric field can actually accelerate something. And so, for example, 400 00:20:21,119 --> 00:20:24,080 Speaker 1: the old televisions that people used to watch, the ones 401 00:20:24,119 --> 00:20:27,679 Speaker 1: that are not flat screens, had an electron accelerator in 402 00:20:27,760 --> 00:20:29,600 Speaker 1: the back of them. Met a little gun that would 403 00:20:29,640 --> 00:20:32,840 Speaker 1: accelerate electrons across an electric field and shoot it at 404 00:20:32,840 --> 00:20:34,800 Speaker 1: the back of the screen, and that's what actually made 405 00:20:34,840 --> 00:20:37,160 Speaker 1: the images. So everybody used to have their own little 406 00:20:37,200 --> 00:20:41,080 Speaker 1: particle accelerator in their house shooting into their brains extray night, 407 00:20:41,200 --> 00:20:44,160 Speaker 1: and that uses an electric field. It's basically a cathode tube. 408 00:20:44,320 --> 00:20:47,400 Speaker 1: We have a voltage applied and it boils electrons off 409 00:20:47,400 --> 00:20:49,400 Speaker 1: of one of the nodes and towards the other one. 410 00:20:49,840 --> 00:20:52,080 Speaker 1: But I guess what I'm saying, it basically works like 411 00:20:52,080 --> 00:20:55,560 Speaker 1: a magnet, right, cathay tube is basically you're using magnetism 412 00:20:55,600 --> 00:20:59,040 Speaker 1: to move the electrons along. Yeah, I mean you're using 413 00:20:59,080 --> 00:21:02,480 Speaker 1: electromagnetism more generally, using the electric field to accelerate it, 414 00:21:02,520 --> 00:21:04,760 Speaker 1: and then you had a magnet in order to steer 415 00:21:04,880 --> 00:21:08,960 Speaker 1: the electrons. So yeah, absolutely, it's all electromagnetism. And that's why, 416 00:21:09,000 --> 00:21:12,359 Speaker 1: for example, we have proton accelerators and electron accelerators. We 417 00:21:12,400 --> 00:21:17,360 Speaker 1: don't have neutron accelerators or neutral atom accelerators because things 418 00:21:17,480 --> 00:21:19,640 Speaker 1: have to have a charge in order for an electric 419 00:21:19,680 --> 00:21:21,800 Speaker 1: field to push on them. Yeah, I guess just kind 420 00:21:21,840 --> 00:21:24,760 Speaker 1: of generally, that's how things push and pull most of 421 00:21:24,760 --> 00:21:26,600 Speaker 1: the time you're here on Earth, right, Like when I 422 00:21:26,640 --> 00:21:28,960 Speaker 1: pick up a glass of water, or when you push 423 00:21:29,000 --> 00:21:33,200 Speaker 1: on the door, you're really using electromagnetic forces to push 424 00:21:33,200 --> 00:21:36,040 Speaker 1: those things. Yeah, that's absolutely right. A baseball is tugged 425 00:21:36,080 --> 00:21:38,760 Speaker 1: by gravity, but most of the interactions you have are 426 00:21:38,800 --> 00:21:42,040 Speaker 1: really electromagnetic interactions. The electrons that the tip of your 427 00:21:42,119 --> 00:21:45,920 Speaker 1: finger are pushing against the electrons in the wall and resisting. 428 00:21:45,960 --> 00:21:48,720 Speaker 1: That's why things seem to be solid, because the forces 429 00:21:48,880 --> 00:21:52,400 Speaker 1: that fill the space between the tiny little particles, that's 430 00:21:52,400 --> 00:21:57,040 Speaker 1: what gives volume volume, and so that's what constructs our world. Absolutely, 431 00:21:57,240 --> 00:22:00,640 Speaker 1: it would be a very very different world without electromagnetic force. Yeah, 432 00:22:00,720 --> 00:22:02,919 Speaker 1: you just made me realize, like all the neutrons in 433 00:22:02,960 --> 00:22:05,200 Speaker 1: our bodies and the objects around is, we're not really 434 00:22:05,240 --> 00:22:08,440 Speaker 1: pushing them directly, right, Like, it's more like our electrons 435 00:22:08,480 --> 00:22:10,960 Speaker 1: are pushing the electrons and those atoms, and those electrons 436 00:22:10,960 --> 00:22:14,240 Speaker 1: are pushing the protons in the nucleus, and then those 437 00:22:14,280 --> 00:22:16,439 Speaker 1: are the ones that are pushing on the neutrons inside 438 00:22:16,440 --> 00:22:18,840 Speaker 1: of atoms. Yeah, the protons and the neutrons stick together 439 00:22:18,920 --> 00:22:21,960 Speaker 1: using the strong force, and so that's what clumps them together. Yeah, 440 00:22:21,960 --> 00:22:24,080 Speaker 1: it's all a big dance of the forces we've discovered 441 00:22:24,080 --> 00:22:26,360 Speaker 1: to make the world that we know and love. All right, well, 442 00:22:26,359 --> 00:22:29,000 Speaker 1: that's the basic way that hilleriors work right now is 443 00:22:29,080 --> 00:22:31,920 Speaker 1: using electromagnetic fields. Let's get into a little bit more 444 00:22:31,920 --> 00:22:34,960 Speaker 1: detail about that and then also talk about maybe new 445 00:22:34,960 --> 00:22:37,919 Speaker 1: ways that we can get particles going for better and 446 00:22:38,000 --> 00:22:41,200 Speaker 1: more powerful colliders. But first let's take a quick break. 447 00:22:53,680 --> 00:22:57,000 Speaker 1: All right, we're talking about new accelerator technologies here, but 448 00:22:57,119 --> 00:22:59,920 Speaker 1: first we're talking about old accelerator technologies. And you said, 449 00:23:00,080 --> 00:23:03,280 Speaker 1: we've had this old technology sins the fifties, right or 450 00:23:03,280 --> 00:23:06,879 Speaker 1: fifties or thirties. So the very first accelerators were like 451 00:23:06,960 --> 00:23:09,640 Speaker 1: in the thirties and the forties. They got more powerful 452 00:23:09,680 --> 00:23:12,200 Speaker 1: in the fifties, which is what heralded like the era 453 00:23:12,240 --> 00:23:15,440 Speaker 1: of the particle zoo, as people were smashing particles together 454 00:23:15,480 --> 00:23:18,199 Speaker 1: at higher energies and discovering all sorts of stuff. But 455 00:23:18,240 --> 00:23:21,080 Speaker 1: it basically started with just accelerating things over a gap, 456 00:23:21,160 --> 00:23:24,560 Speaker 1: and then people tried to reuse that gap multiple times. 457 00:23:24,600 --> 00:23:26,880 Speaker 1: So like you know, if you go across that gap, 458 00:23:26,920 --> 00:23:28,880 Speaker 1: you speed up. Can we go across that gap more 459 00:23:28,880 --> 00:23:32,560 Speaker 1: than once. So they had accelerators called cyclotrons, where a 460 00:23:32,560 --> 00:23:34,800 Speaker 1: particle would go in a circle and go across the 461 00:23:34,840 --> 00:23:37,960 Speaker 1: gap multiple times. They had singotrons where you got even 462 00:23:38,000 --> 00:23:40,360 Speaker 1: more sophisticated and you would try to like sync up 463 00:23:40,359 --> 00:23:42,399 Speaker 1: the energy in the gap with when the particle was 464 00:23:42,440 --> 00:23:45,080 Speaker 1: going faster and faster. And so I think the basic 465 00:23:45,160 --> 00:23:47,479 Speaker 1: idea is that if you have an electron, First of all, 466 00:23:47,520 --> 00:23:49,439 Speaker 1: you sort of create an electron and you kind of 467 00:23:49,520 --> 00:23:53,040 Speaker 1: put it out there in space in the air by itself, 468 00:23:53,080 --> 00:23:55,879 Speaker 1: and then you basically hold a positive electric charge ahead 469 00:23:55,920 --> 00:23:58,919 Speaker 1: of it basically or a negative charge behind it, and 470 00:23:58,960 --> 00:24:02,320 Speaker 1: then that electro magnetic repulsion or attraction then moves your 471 00:24:02,320 --> 00:24:04,880 Speaker 1: electron forward, and that's how you get it going. Yeah, 472 00:24:04,880 --> 00:24:06,840 Speaker 1: that's basically how you do it. And you can imagine 473 00:24:06,880 --> 00:24:09,360 Speaker 1: doing that with like a battery. For example, a battery 474 00:24:09,400 --> 00:24:12,719 Speaker 1: can create that kind of voltage difference between two plates 475 00:24:12,800 --> 00:24:15,280 Speaker 1: by shuttling the electrons from one side to the other, 476 00:24:15,440 --> 00:24:17,720 Speaker 1: so that if you put an electron in the gap there, 477 00:24:17,880 --> 00:24:20,560 Speaker 1: it will get pushed towards the lower voltage and that's 478 00:24:20,600 --> 00:24:24,160 Speaker 1: what the acceleration is. So essentially you arrange the charges 479 00:24:24,240 --> 00:24:26,280 Speaker 1: to give you an electric field to push on an 480 00:24:26,320 --> 00:24:28,880 Speaker 1: electron and that will accelerate it. Yeah, like you said, 481 00:24:28,920 --> 00:24:31,280 Speaker 1: like in a battery, Like a battery will maybe concentrate 482 00:24:31,320 --> 00:24:34,080 Speaker 1: the electrons and a coil or a wire or plate 483 00:24:34,280 --> 00:24:36,800 Speaker 1: towards the back, and then that will push your single 484 00:24:36,800 --> 00:24:39,760 Speaker 1: electron forward. But there's only kind of so much that 485 00:24:39,920 --> 00:24:42,080 Speaker 1: you can push it, right doing it that way, Yeah, 486 00:24:42,119 --> 00:24:43,800 Speaker 1: there's only so much you can push it. You can 487 00:24:43,840 --> 00:24:47,080 Speaker 1: try to pump a lot of energy into that electric field, 488 00:24:47,119 --> 00:24:49,679 Speaker 1: but eventually things will break down. Like if you have 489 00:24:49,720 --> 00:24:52,240 Speaker 1: two pieces of metal and you put a really strong 490 00:24:52,280 --> 00:24:55,920 Speaker 1: electric field across them, Eventually it will pull the electrons 491 00:24:56,040 --> 00:24:59,399 Speaker 1: out of that metal and break down the electric field. 492 00:24:59,560 --> 00:25:01,840 Speaker 1: And then what you do is once the electron gets going, 493 00:25:01,960 --> 00:25:05,280 Speaker 1: then you use another electric field up ahead to accelerate 494 00:25:05,280 --> 00:25:07,520 Speaker 1: it even more. Yeah. So, because you can't put an 495 00:25:07,560 --> 00:25:10,040 Speaker 1: infinite amount of energy into a single one of these 496 00:25:10,080 --> 00:25:13,440 Speaker 1: sort of like little accelerators, because it'll break down the 497 00:25:13,520 --> 00:25:16,600 Speaker 1: way like lightning is like a breakdown of the voltage 498 00:25:16,600 --> 00:25:19,199 Speaker 1: between the air and the ground. Then you stack them up, 499 00:25:19,240 --> 00:25:20,720 Speaker 1: you say, well, I'm gonna have one and then might 500 00:25:20,760 --> 00:25:22,600 Speaker 1: have another one that might have another one that might 501 00:25:22,640 --> 00:25:24,720 Speaker 1: have another one you just sort of like line these 502 00:25:24,760 --> 00:25:27,040 Speaker 1: things up so that each one gives your electron a 503 00:25:27,080 --> 00:25:29,280 Speaker 1: little bit of a push. Yeah, And I guess initially 504 00:25:29,280 --> 00:25:31,320 Speaker 1: in the fifties they would use they would put these 505 00:25:31,359 --> 00:25:35,000 Speaker 1: in a straight line, right, Like you accelerate an electron 506 00:25:35,040 --> 00:25:37,760 Speaker 1: with one accelerator, and then the next one picks it 507 00:25:37,840 --> 00:25:39,760 Speaker 1: up and accelerate it even more, and you sort of 508 00:25:39,760 --> 00:25:42,040 Speaker 1: like a tunnel or a gun or like the barrel 509 00:25:42,080 --> 00:25:46,800 Speaker 1: of a rifle, and that gets your electrons going even faster. Exactly. 510 00:25:46,960 --> 00:25:49,000 Speaker 1: There's a little bit of a wrinkle there though, because 511 00:25:49,119 --> 00:25:51,880 Speaker 1: what happens when your electron passes a sort of negative 512 00:25:51,880 --> 00:25:54,720 Speaker 1: potential plate of the first one, is it wants to 513 00:25:54,760 --> 00:25:57,520 Speaker 1: slow down. If you imagine like a bunch of positive 514 00:25:57,600 --> 00:26:00,520 Speaker 1: charges there that are pulling the electron towards that first plate, 515 00:26:00,720 --> 00:26:03,399 Speaker 1: what happens when it passes it, Now those positive charges 516 00:26:03,440 --> 00:26:06,560 Speaker 1: are pulling it back. And so people develop these really 517 00:26:06,600 --> 00:26:11,040 Speaker 1: fancy techniques to oscillate the voltage across those plates so 518 00:26:11,040 --> 00:26:13,760 Speaker 1: that when the particles moving towards it pulling it towards it, 519 00:26:13,800 --> 00:26:16,320 Speaker 1: and then just as it passes it flips the charges 520 00:26:16,320 --> 00:26:19,440 Speaker 1: and pushes it away. So we have these like RF 521 00:26:19,480 --> 00:26:22,520 Speaker 1: cavities they're called. With these oscillating fields, there are time 522 00:26:22,600 --> 00:26:25,400 Speaker 1: perfectly to speed the particles up and then avoid slowing 523 00:26:25,400 --> 00:26:28,200 Speaker 1: them down. And as you say, the strategy to making 524 00:26:28,240 --> 00:26:31,439 Speaker 1: them bigger and longer and faster is just to stack 525 00:26:31,480 --> 00:26:33,760 Speaker 1: them up to make a big tunnel and put a 526 00:26:33,800 --> 00:26:35,879 Speaker 1: bunch of these in there. Yeah, that's how they did 527 00:26:35,920 --> 00:26:37,760 Speaker 1: it initially. But then at some point they figured out 528 00:26:37,760 --> 00:26:40,639 Speaker 1: that you can get even more acceleration by having the 529 00:26:40,680 --> 00:26:44,400 Speaker 1: particles going a circle and basically go through this accelerating 530 00:26:44,440 --> 00:26:47,040 Speaker 1: part multiple times, and then they can go faster and 531 00:26:47,040 --> 00:26:49,639 Speaker 1: faster and faster each time. Yeah. So the one design 532 00:26:49,680 --> 00:26:52,560 Speaker 1: of the accelerator is called a linear accelerator. There's one 533 00:26:52,600 --> 00:26:54,880 Speaker 1: like that at Stanford, there's one like that in Germany. 534 00:26:54,960 --> 00:26:57,080 Speaker 1: We just shoot them down a tunnel. It's a one go. 535 00:26:57,240 --> 00:26:59,040 Speaker 1: You speed them up, you get them to as fast 536 00:26:59,080 --> 00:27:00,879 Speaker 1: as you can, and then them at the end. But 537 00:27:00,960 --> 00:27:03,879 Speaker 1: another strategy is to reuse the tunnel by having a 538 00:27:03,960 --> 00:27:05,959 Speaker 1: go in a circle. And so as you say, you 539 00:27:06,000 --> 00:27:07,880 Speaker 1: have like something that gives it a kick, and then 540 00:27:07,880 --> 00:27:09,480 Speaker 1: you have something that bends it, and you have something 541 00:27:09,520 --> 00:27:10,880 Speaker 1: it gives it a kick, and then you have something 542 00:27:10,880 --> 00:27:13,480 Speaker 1: that bends it, and so the large hadron colliders like that. 543 00:27:13,560 --> 00:27:15,960 Speaker 1: It's a big circle and the particles move around a 544 00:27:15,960 --> 00:27:18,920 Speaker 1: tunnel and there's segments that push it and then segments 545 00:27:18,920 --> 00:27:22,320 Speaker 1: that bend it using very powerful magnets bend it, you mean, 546 00:27:22,400 --> 00:27:25,600 Speaker 1: like as in they make the particles kind of go 547 00:27:25,720 --> 00:27:27,439 Speaker 1: right a little bit and then then makes them go 548 00:27:27,480 --> 00:27:30,320 Speaker 1: in a circle. Yeah. So the particles move not actually 549 00:27:30,359 --> 00:27:33,040 Speaker 1: in a perfect circle, because they move in straight lines 550 00:27:33,040 --> 00:27:36,000 Speaker 1: through the little mini accelerator segments and then they bend 551 00:27:36,280 --> 00:27:38,960 Speaker 1: through the magnets. So it's more like a really big 552 00:27:39,040 --> 00:27:41,840 Speaker 1: polygon with a bunch of straight sides. Yeah, I guess 553 00:27:41,880 --> 00:27:44,520 Speaker 1: the difference it's sort of like the between a sling shot, 554 00:27:44,960 --> 00:27:46,760 Speaker 1: like you pull back and then you let go and 555 00:27:46,880 --> 00:27:50,120 Speaker 1: the rover bands throw the rock forward or whatever you're 556 00:27:50,119 --> 00:27:52,600 Speaker 1: trying to shoot and using a sling where you like 557 00:27:52,600 --> 00:27:54,680 Speaker 1: put the rock in a little sling and then you 558 00:27:55,119 --> 00:27:56,800 Speaker 1: spin and spin and spin, and each time you spin 559 00:27:56,840 --> 00:27:58,399 Speaker 1: it you make it go faster and then at some 560 00:27:58,480 --> 00:28:00,199 Speaker 1: point you let it go, you know. Or if going 561 00:28:00,240 --> 00:28:02,399 Speaker 1: to use like kid analogies, it's like the difference between 562 00:28:02,400 --> 00:28:04,359 Speaker 1: a slide. You start at the top and you go 563 00:28:04,440 --> 00:28:06,200 Speaker 1: fast and you hit the bottom or a merry go 564 00:28:06,320 --> 00:28:08,800 Speaker 1: round where your friend can keep pushing it faster and 565 00:28:08,840 --> 00:28:11,399 Speaker 1: faster and faster, and you're going around faster and faster 566 00:28:11,760 --> 00:28:13,960 Speaker 1: until you both throw up. And that's really what particle 567 00:28:13,960 --> 00:28:16,159 Speaker 1: physics is all about, right, throwing up what's inside of 568 00:28:16,200 --> 00:28:19,359 Speaker 1: the fundamental particles. Yeah, we're exploring the vomit frontier in 569 00:28:19,400 --> 00:28:23,919 Speaker 1: the end, it's right, your vomit physicists, nihilist vomiting physics. 570 00:28:23,960 --> 00:28:26,600 Speaker 1: And that's basically the technology. The large hadron collider is 571 00:28:26,600 --> 00:28:29,159 Speaker 1: pushing bend, pushing bend, push in bend. And what limits 572 00:28:29,160 --> 00:28:32,320 Speaker 1: the large hadron collider is essentially the size of the tunnel. 573 00:28:32,480 --> 00:28:34,159 Speaker 1: Building that kind of tunnel and filling it with all 574 00:28:34,200 --> 00:28:37,800 Speaker 1: that technology is expensive. But in order to get fast, 575 00:28:37,960 --> 00:28:40,320 Speaker 1: you gotta go big. Well, maybe to talk a little 576 00:28:40,320 --> 00:28:42,800 Speaker 1: bit about why it needs to be bigger, it's because 577 00:28:42,800 --> 00:28:46,360 Speaker 1: of the limitations in the magnets that bend the path 578 00:28:46,440 --> 00:28:49,880 Speaker 1: of the particles. Right, Like, if you can get stronger 579 00:28:50,480 --> 00:28:53,480 Speaker 1: magnets are a better way to kind of curve the 580 00:28:53,520 --> 00:28:56,120 Speaker 1: path of these particles, then you could have the same 581 00:28:56,160 --> 00:28:58,960 Speaker 1: circle but just have the particles go faster in it. Yeah, 582 00:28:58,960 --> 00:29:00,959 Speaker 1: if you had stronger magnet that could bend them more 583 00:29:01,000 --> 00:29:03,600 Speaker 1: effectively at the same speed. Then, yeah, you could have 584 00:29:03,640 --> 00:29:06,840 Speaker 1: a smaller circle, which means you could reuse the same 585 00:29:06,960 --> 00:29:10,640 Speaker 1: linear accelerating segments at the same magnets more times. Right, 586 00:29:10,680 --> 00:29:12,560 Speaker 1: So it would go around more times to get to 587 00:29:12,600 --> 00:29:14,880 Speaker 1: the same speed. But you could build a smaller device 588 00:29:15,120 --> 00:29:19,120 Speaker 1: instead of time to be like tens of kilometers around. Right, 589 00:29:19,400 --> 00:29:21,600 Speaker 1: this tunnel, the large change on collider is filled with 590 00:29:21,680 --> 00:29:24,640 Speaker 1: tens of kilometers of these things. Right, it's not a 591 00:29:24,720 --> 00:29:27,640 Speaker 1: small device. But if the magnets were more powerful and 592 00:29:27,680 --> 00:29:29,760 Speaker 1: you could bend it, then you could basically shrink the 593 00:29:29,800 --> 00:29:31,800 Speaker 1: size of that circle and the whole thing would be 594 00:29:31,840 --> 00:29:34,440 Speaker 1: smaller and cheaper, right, Because I guess the problem is 595 00:29:34,480 --> 00:29:37,560 Speaker 1: that the faster the particles go, the harder it is 596 00:29:37,560 --> 00:29:39,400 Speaker 1: to get them to go in a circle. Right, Because 597 00:29:39,400 --> 00:29:41,760 Speaker 1: the fasters are going the kind of more I guess 598 00:29:41,880 --> 00:29:44,080 Speaker 1: entrifical the force you need to kind of keep them 599 00:29:44,080 --> 00:29:46,240 Speaker 1: in a circle. Yeah, you need strong magnets to move 600 00:29:46,360 --> 00:29:49,800 Speaker 1: very high speed particles and a circle. It's a centripetal 601 00:29:49,880 --> 00:29:52,840 Speaker 1: force towards the center that keeps something moving in a circle, 602 00:29:53,120 --> 00:29:56,000 Speaker 1: the same way the Earth moves around the Sun because 603 00:29:56,080 --> 00:29:58,840 Speaker 1: of the force of gravity pulling it towards the Sun. 604 00:29:59,320 --> 00:30:01,920 Speaker 1: So we can make these particles kind of like orbit 605 00:30:02,040 --> 00:30:05,040 Speaker 1: the center of the collider using these magnets to bend 606 00:30:05,040 --> 00:30:08,000 Speaker 1: their path to provide that same kind of force, And 607 00:30:08,040 --> 00:30:10,080 Speaker 1: if we could provide a stronger force, we could bend 608 00:30:10,120 --> 00:30:12,920 Speaker 1: them in a tighter circle. Yeah. So like right now, 609 00:30:12,960 --> 00:30:16,160 Speaker 1: you probably could accelerate the particles faster, like you can't 610 00:30:16,160 --> 00:30:18,120 Speaker 1: make them go faster, but you wouldn't be able to 611 00:30:18,360 --> 00:30:21,280 Speaker 1: basically control them. Like if you accelerated them any faster, 612 00:30:21,480 --> 00:30:24,080 Speaker 1: they would basically go off the rails kind of right, 613 00:30:24,160 --> 00:30:26,120 Speaker 1: Like they would start hitting the walls of your collider 614 00:30:26,160 --> 00:30:28,760 Speaker 1: and that would burn them up, and then you'd poke 615 00:30:28,800 --> 00:30:30,680 Speaker 1: a hole in your tup tunnel and then the whole 616 00:30:30,720 --> 00:30:33,560 Speaker 1: thing goes That's right. We're limited either by the magnet 617 00:30:33,600 --> 00:30:36,080 Speaker 1: technology or by the size of the tunnel. Like we 618 00:30:36,120 --> 00:30:38,960 Speaker 1: can make the tunnel bigger with the same magnets and 619 00:30:39,000 --> 00:30:41,680 Speaker 1: then we could get the higher energy, or we could 620 00:30:41,680 --> 00:30:44,680 Speaker 1: make the tunnel smaller with stronger magnets to get to 621 00:30:44,760 --> 00:30:47,360 Speaker 1: the same energy. But if we had the same tunnel 622 00:30:47,480 --> 00:30:49,760 Speaker 1: and we just whizzed them around more and kept pushing 623 00:30:49,760 --> 00:30:51,880 Speaker 1: on them. Then eventually we would not be able to 624 00:30:51,920 --> 00:30:54,440 Speaker 1: contain them using our magnets. It would just slam into 625 00:30:54,480 --> 00:30:56,520 Speaker 1: the wall. So if you increase the energy, do you 626 00:30:56,520 --> 00:30:59,120 Speaker 1: have someone down there at the basement going she kind 627 00:30:59,120 --> 00:31:05,920 Speaker 1: of take any more cut? Yeah, that's a specific job, absolutely, 628 00:31:06,240 --> 00:31:09,000 Speaker 1: and you have to hire a scotchman from your collaboration 629 00:31:09,080 --> 00:31:11,280 Speaker 1: to do that one. No, we prefer Panamanians to do 630 00:31:11,280 --> 00:31:13,720 Speaker 1: a Scottish accent. Actually, oh yeah, that's just as good. 631 00:31:15,400 --> 00:31:21,400 Speaker 1: No comment for our Scottish listeners. But our magnet technology 632 00:31:21,480 --> 00:31:24,400 Speaker 1: is pretty awesome. I mean, we have super conducting magnets 633 00:31:24,440 --> 00:31:27,480 Speaker 1: down there. We're really pushing the limits of what magnets 634 00:31:27,520 --> 00:31:30,760 Speaker 1: can do. And so one way we could improve particle 635 00:31:30,800 --> 00:31:34,360 Speaker 1: colliders is to make some breakthrough in magnet technology to 636 00:31:34,440 --> 00:31:38,360 Speaker 1: make these things more powerful and smaller or cheaper. What's 637 00:31:38,360 --> 00:31:40,880 Speaker 1: the limitation, I guess is it just that the magnets. 638 00:31:41,000 --> 00:31:43,680 Speaker 1: You're already running as much current as you can through 639 00:31:43,720 --> 00:31:46,160 Speaker 1: these magnets or what, Yeah, we're running as much current 640 00:31:46,160 --> 00:31:49,280 Speaker 1: as we can without them breaking down. They're already cooled 641 00:31:49,320 --> 00:31:51,840 Speaker 1: down to a few degrees Calvin. So we can take 642 00:31:51,880 --> 00:31:54,320 Speaker 1: advantage of their super conducting nature, which means if we 643 00:31:54,360 --> 00:31:57,240 Speaker 1: get super duper strong magnets out of our current and 644 00:31:57,320 --> 00:31:59,840 Speaker 1: they don't like heat up and distort. Maybe you remember that, 645 00:32:00,000 --> 00:32:01,880 Speaker 1: and we turned on the large hende On collider. There 646 00:32:01,920 --> 00:32:04,120 Speaker 1: was a disaster in two thousand and nine, just a 647 00:32:04,200 --> 00:32:06,720 Speaker 1: few months in, and some of the liquid helium that 648 00:32:06,800 --> 00:32:09,280 Speaker 1: was keeping this thing cool sprayed out everywhere and the 649 00:32:09,280 --> 00:32:11,240 Speaker 1: whole thing warmed up, and it was a big disaster. 650 00:32:11,640 --> 00:32:14,040 Speaker 1: So these things are not easy to operate and to 651 00:32:14,200 --> 00:32:17,040 Speaker 1: keep functional. One of the many ways that the beam 652 00:32:17,080 --> 00:32:19,320 Speaker 1: can go wrong is something we call a quench, when 653 00:32:19,360 --> 00:32:21,680 Speaker 1: one of the magnets basically fails and the beam just 654 00:32:21,760 --> 00:32:24,600 Speaker 1: like gets dumped into the rock. And so we're really 655 00:32:24,640 --> 00:32:28,200 Speaker 1: operating at the limit of magnet technology. All right, Well, 656 00:32:28,240 --> 00:32:30,239 Speaker 1: then I guess the idea is that is there like 657 00:32:30,280 --> 00:32:34,080 Speaker 1: a revolutionary new technology or a totally different way of 658 00:32:34,120 --> 00:32:37,160 Speaker 1: doing the whole particle accelerating thing that could maybe like 659 00:32:37,480 --> 00:32:40,640 Speaker 1: let you get away with faster velocities without having these 660 00:32:40,760 --> 00:32:44,520 Speaker 1: gigantic tunnels and these superconducting magnets. Oh there is, and 661 00:32:44,640 --> 00:32:47,680 Speaker 1: I'm dying to talk about it. Well, steps through this, Danuel. 662 00:32:47,880 --> 00:32:50,920 Speaker 1: What is this amazing technology called and how does it work? 663 00:32:51,040 --> 00:32:53,960 Speaker 1: So the idea is, instead of making the magnet stronger, 664 00:32:54,200 --> 00:32:57,560 Speaker 1: can we make the accelerator part much more powerful? Can 665 00:32:57,600 --> 00:33:01,480 Speaker 1: we accelerate particles to much higher energies over a shorter distance. 666 00:33:01,560 --> 00:33:04,600 Speaker 1: I remember before the limitation was that we couldn't have 667 00:33:04,720 --> 00:33:08,360 Speaker 1: strong enough electric fields across two metal plates because it 668 00:33:08,400 --> 00:33:11,800 Speaker 1: would like make a breakdown between those plates. Remember that 669 00:33:11,880 --> 00:33:14,560 Speaker 1: right now, in our colliders, these particles are accelerated through 670 00:33:14,560 --> 00:33:17,040 Speaker 1: a vacuum. So between those plates, it's not like air, 671 00:33:17,360 --> 00:33:19,480 Speaker 1: So you're not getting like ionization of the air the 672 00:33:19,520 --> 00:33:22,080 Speaker 1: way you do when you have like static electricity or 673 00:33:22,160 --> 00:33:25,120 Speaker 1: lightning jumping from the ground to the earth. It's really 674 00:33:25,160 --> 00:33:27,920 Speaker 1: a pure breakdown of the metal, right You're like pulling 675 00:33:27,920 --> 00:33:30,600 Speaker 1: the electrons off of the metal. And so in order 676 00:33:30,640 --> 00:33:33,240 Speaker 1: to avoid this breakdown, people are thinking, well, maybe we 677 00:33:33,280 --> 00:33:35,840 Speaker 1: shouldn't have a vacuum, Maybe we should fill that with 678 00:33:35,920 --> 00:33:38,800 Speaker 1: something in order to avoid a breakdown. And so one 679 00:33:38,880 --> 00:33:42,280 Speaker 1: idea is to use a plasma instead of having a vacuum. 680 00:33:42,400 --> 00:33:43,760 Speaker 1: So let me see if I get this straight. It's 681 00:33:43,800 --> 00:33:46,560 Speaker 1: sort of like the same technology where you have plates, 682 00:33:46,640 --> 00:33:49,680 Speaker 1: like metal plates, and in these plates you basically like 683 00:33:49,880 --> 00:33:52,320 Speaker 1: run a current through them, so that you kind of 684 00:33:52,320 --> 00:33:54,440 Speaker 1: make a magnet basically, but now the twist is and 685 00:33:54,560 --> 00:33:56,680 Speaker 1: instead of having it in a vacuum, you put it 686 00:33:56,720 --> 00:33:59,120 Speaker 1: inside of a plasma. That's right, We use a plasma 687 00:33:59,120 --> 00:34:01,560 Speaker 1: instead of having a vacuum. But now we don't have 688 00:34:01,640 --> 00:34:05,760 Speaker 1: the external electric field provided by some plates. Now we 689 00:34:05,840 --> 00:34:10,200 Speaker 1: use the plasma itself to generate the electric fields internally. 690 00:34:10,360 --> 00:34:12,840 Speaker 1: So wait, there's no plates, there's no plates at all. No, 691 00:34:13,160 --> 00:34:15,960 Speaker 1: but we think that it's possible to generate much stronger 692 00:34:16,000 --> 00:34:19,680 Speaker 1: electric fields within the plasma than it is between two 693 00:34:19,719 --> 00:34:22,040 Speaker 1: metal plates and a vacuum. Okay, so you use the 694 00:34:22,080 --> 00:34:25,440 Speaker 1: plasma as the plate kind of m exactly. And so 695 00:34:25,480 --> 00:34:27,880 Speaker 1: you take this plasma and you like zap it with 696 00:34:27,960 --> 00:34:32,000 Speaker 1: a laser, which rearranges all the charges within the plasma 697 00:34:32,080 --> 00:34:35,000 Speaker 1: in such a way to create very strong electric fields 698 00:34:35,040 --> 00:34:38,840 Speaker 1: inside the plasma that can then be used to accelerate particles. 699 00:34:39,040 --> 00:34:41,520 Speaker 1: That's the basic idea. So what would this look like 700 00:34:41,600 --> 00:34:44,640 Speaker 1: A like a tube basically kind of or a tunnel 701 00:34:44,719 --> 00:34:48,120 Speaker 1: filled with plasma, and then you're shooting lasers into this 702 00:34:48,360 --> 00:34:52,400 Speaker 1: to create kind of like variations in the electric fields 703 00:34:52,440 --> 00:34:55,440 Speaker 1: inside of the plasma. Exactly. Remember that a plasma is 704 00:34:55,480 --> 00:34:58,680 Speaker 1: just really hot gas. Like you take hydrogen hydrogen as 705 00:34:58,680 --> 00:35:01,560 Speaker 1: a proton and electron. The electron is happily orbiting of 706 00:35:01,560 --> 00:35:03,880 Speaker 1: the nucleus the proton, and if you give that electron 707 00:35:03,920 --> 00:35:06,239 Speaker 1: more energy, it goes up an energy level sort of 708 00:35:06,360 --> 00:35:09,200 Speaker 1: larger orbital radius, and you keep doing that, eventually the 709 00:35:09,239 --> 00:35:11,680 Speaker 1: electron goes free. And so that's what a plasma is. 710 00:35:11,840 --> 00:35:14,960 Speaker 1: The electrons have so much energy that they're not bound 711 00:35:14,960 --> 00:35:18,560 Speaker 1: anymore to the protons. So it's a charged gas, right. 712 00:35:18,600 --> 00:35:21,719 Speaker 1: It has positive and negative charges all flowing around in it, 713 00:35:22,080 --> 00:35:25,280 Speaker 1: unlike neutral hydrogen, which is you know, protons and electrons 714 00:35:25,320 --> 00:35:28,480 Speaker 1: bound tightly together, so they're effectively neutral. So this plasma 715 00:35:28,600 --> 00:35:33,280 Speaker 1: is like microscopically charged, but typically it's like macroscopically neutral. 716 00:35:33,520 --> 00:35:35,160 Speaker 1: You take like a big chunk of it as the 717 00:35:35,200 --> 00:35:39,400 Speaker 1: same number of electrons and protons, but you can induce 718 00:35:39,480 --> 00:35:41,560 Speaker 1: waves in it. You can like pull on the electrons 719 00:35:41,640 --> 00:35:43,759 Speaker 1: or zap all the electrons, get them to move in 720 00:35:43,800 --> 00:35:47,839 Speaker 1: one direction, which will create an electric field within the plasma, 721 00:35:47,960 --> 00:35:50,800 Speaker 1: like you create you're creating a current of electrons inside 722 00:35:50,800 --> 00:35:52,360 Speaker 1: of the plasma. Is that what you mean? What you 723 00:35:52,400 --> 00:35:55,399 Speaker 1: actually do is create like a wake field inside of it, 724 00:35:55,719 --> 00:35:57,920 Speaker 1: so it's not literally a current, but yeah, you're creating 725 00:35:57,960 --> 00:36:01,440 Speaker 1: like these waves of electrons through the plasma. They're like 726 00:36:01,480 --> 00:36:04,480 Speaker 1: density waves where the electrons are like wiggling, and that 727 00:36:04,520 --> 00:36:08,680 Speaker 1: creates electromagnetic fields which you can then use to accelerate particles. 728 00:36:08,760 --> 00:36:10,799 Speaker 1: So you have this tube, as you said, of plasma, 729 00:36:10,880 --> 00:36:12,839 Speaker 1: and you use zap it with the laser and you 730 00:36:12,920 --> 00:36:17,319 Speaker 1: choose the laser frequency just right to excite oscillations in 731 00:36:17,360 --> 00:36:20,680 Speaker 1: the electrons in the plasma to create this wake field, 732 00:36:21,040 --> 00:36:22,800 Speaker 1: and then you dump your particle into it and it 733 00:36:22,880 --> 00:36:25,759 Speaker 1: sort of like surfs along this electromagnetic field that you've 734 00:36:25,760 --> 00:36:28,520 Speaker 1: created with your laser, and it gets shot at the end, 735 00:36:28,719 --> 00:36:32,399 Speaker 1: going much much faster. Interesting, all right, well, maybe take 736 00:36:32,400 --> 00:36:34,120 Speaker 1: a step a little bit of a step back here. 737 00:36:34,400 --> 00:36:38,600 Speaker 1: How does the laser cause the electrons to form into waves? 738 00:36:39,840 --> 00:36:42,520 Speaker 1: Like do electrons interact with photons? Is that the idea 739 00:36:42,600 --> 00:36:45,640 Speaker 1: electrons do interact with photons, and so lasers are just 740 00:36:45,680 --> 00:36:48,600 Speaker 1: like a great way to dump energy into the plasma. 741 00:36:48,680 --> 00:36:50,799 Speaker 1: And typically you can think about a plasma as like 742 00:36:50,840 --> 00:36:53,360 Speaker 1: a bunch of individual particles. You know, you have protons, 743 00:36:53,400 --> 00:36:55,920 Speaker 1: you have electrons that have charges, so they can interact 744 00:36:55,920 --> 00:36:57,960 Speaker 1: with photons and fields and all this stuff. But that's 745 00:36:57,960 --> 00:37:00,359 Speaker 1: a little bit of a nightmare because there're so many 746 00:37:00,400 --> 00:37:03,040 Speaker 1: of them. It just seems like a buzzing chaos. But 747 00:37:03,120 --> 00:37:05,360 Speaker 1: you can also think about the plasma sort of like 748 00:37:05,480 --> 00:37:09,319 Speaker 1: collectively and think about the collective motion of the electrons. 749 00:37:09,719 --> 00:37:12,839 Speaker 1: So plasmas have like tiny, little local behavior, but they 750 00:37:12,880 --> 00:37:16,799 Speaker 1: also have sort of like long distance collective behavior. You 751 00:37:16,840 --> 00:37:19,840 Speaker 1: can get plasmas to do things like have waves moving 752 00:37:19,880 --> 00:37:22,440 Speaker 1: through them, And so if you dump a laser beam 753 00:37:22,440 --> 00:37:24,799 Speaker 1: into it with the right frequency and you can sort 754 00:37:24,800 --> 00:37:26,799 Speaker 1: of excite it to do these waves the same way 755 00:37:26,840 --> 00:37:29,040 Speaker 1: you can if you like slap your hand against the 756 00:37:29,080 --> 00:37:31,200 Speaker 1: surface of a lake and do it at the right frequency, 757 00:37:31,400 --> 00:37:34,840 Speaker 1: you can get the lake to produce these waves. But 758 00:37:34,960 --> 00:37:37,160 Speaker 1: I guess the main mechanism is that it's interacting with 759 00:37:37,160 --> 00:37:40,239 Speaker 1: the electrons, because I guess light doesn't interact with the protons. 760 00:37:40,600 --> 00:37:42,799 Speaker 1: The light does interact with the protons as well, right, 761 00:37:42,840 --> 00:37:45,600 Speaker 1: protons are also charged, but remember protons are much more 762 00:37:45,640 --> 00:37:49,839 Speaker 1: massive than electrons, and so the same energy doesn't accelerate 763 00:37:49,960 --> 00:37:52,719 Speaker 1: those protons to move as much. So this whole thing 764 00:37:52,719 --> 00:37:56,040 Speaker 1: happens really really fast. Basically before the protons can sort 765 00:37:56,040 --> 00:37:58,080 Speaker 1: of get out of bed. The electrons have this big 766 00:37:58,120 --> 00:37:59,960 Speaker 1: wave that passes through them, and the protons are like 767 00:38:00,160 --> 00:38:02,399 Speaker 1: what sort of like me? And in this podcast right now? 768 00:38:02,760 --> 00:38:06,000 Speaker 1: All right, well, let's let's react to that laser a 769 00:38:06,000 --> 00:38:08,239 Speaker 1: bit of knowledge there, and let's dig a little bit 770 00:38:08,280 --> 00:38:10,319 Speaker 1: more into this effect than how you can use it 771 00:38:10,360 --> 00:38:13,880 Speaker 1: to axillary particles, maybe faster than the Large Hadron collider. 772 00:38:14,560 --> 00:38:29,160 Speaker 1: But first let's take another quick break. All right, we're 773 00:38:29,160 --> 00:38:32,120 Speaker 1: talking about a new way to killary particles that is 774 00:38:32,160 --> 00:38:36,440 Speaker 1: maybe faster and cheaper and better than the current technology 775 00:38:36,560 --> 00:38:39,600 Speaker 1: which is at the Large Hadron Collider. And so this 776 00:38:39,760 --> 00:38:43,640 Speaker 1: technology involves using a plasma. So you have a plasma, 777 00:38:43,920 --> 00:38:47,200 Speaker 1: which is like a gas where all of the atoms 778 00:38:47,200 --> 00:38:50,960 Speaker 1: have been broken down into single electrons and maybe protons 779 00:38:51,080 --> 00:38:53,359 Speaker 1: or at least clumps of protons, and so you have 780 00:38:53,400 --> 00:38:55,799 Speaker 1: the soup of all this stuff floating around that has 781 00:38:55,960 --> 00:38:58,359 Speaker 1: a charge, and then you shoot a laser into it. 782 00:38:58,400 --> 00:39:02,480 Speaker 1: And somehow that laser cites things, or maybe it causes 783 00:39:02,520 --> 00:39:06,200 Speaker 1: electrons to clump or to scatter. What exactly is happening there. 784 00:39:06,280 --> 00:39:08,759 Speaker 1: It causes the electrons to wiggle, It creates like a 785 00:39:08,840 --> 00:39:12,399 Speaker 1: wave of the electrons moving through the plasma, and again 786 00:39:12,440 --> 00:39:15,840 Speaker 1: you choose it very specifically the laser pulsed length to 787 00:39:15,920 --> 00:39:19,040 Speaker 1: be resonant with the modes of the plasma. Everything that 788 00:39:19,080 --> 00:39:21,480 Speaker 1: can wiggle, everything we can describe in terms of like 789 00:39:21,680 --> 00:39:25,319 Speaker 1: wave physics has resonant frequencies, the way, for example, your 790 00:39:25,320 --> 00:39:28,759 Speaker 1: shower is really good and amplifying certain frequencies when you're 791 00:39:28,800 --> 00:39:32,360 Speaker 1: singing and not others, or guitar strings like to oscillate 792 00:39:32,360 --> 00:39:36,040 Speaker 1: at certain frequencies and not others. They're resonant frequencies in 793 00:39:36,080 --> 00:39:37,920 Speaker 1: the same way that like a laser is made use 794 00:39:37,960 --> 00:39:41,320 Speaker 1: a resonant cavity. And so the equations of the motion 795 00:39:41,400 --> 00:39:45,280 Speaker 1: of the electrons who the plasma allow for certain frequencies 796 00:39:45,560 --> 00:39:48,680 Speaker 1: of collective motion where the electrons will like slash back 797 00:39:48,719 --> 00:39:51,600 Speaker 1: and forth all together. Instead of getting like a bunch 798 00:39:51,600 --> 00:39:53,799 Speaker 1: of individual electrons doing their own thing, you get this 799 00:39:53,880 --> 00:39:57,239 Speaker 1: like collective behavior of all the electrons if you push 800 00:39:57,239 --> 00:39:58,920 Speaker 1: it the right way, sort of like pushing your kid 801 00:39:58,960 --> 00:40:01,640 Speaker 1: on a swing right shit the right frequency, and your 802 00:40:01,719 --> 00:40:03,880 Speaker 1: kids can get going really really fast. You push it 803 00:40:04,000 --> 00:40:06,360 Speaker 1: like random times, then you're going to get like chaotic 804 00:40:06,400 --> 00:40:08,239 Speaker 1: motion in the swing. And I guess that's what the 805 00:40:08,320 --> 00:40:11,440 Speaker 1: light is doing. Like the full time will hit electrons 806 00:40:11,440 --> 00:40:15,040 Speaker 1: in a certain way, and because of the frequency, does 807 00:40:15,040 --> 00:40:17,560 Speaker 1: it in different ways in different locations. And that's how 808 00:40:17,640 --> 00:40:20,040 Speaker 1: you create the wave inside of the plasma exactly. And 809 00:40:20,080 --> 00:40:22,480 Speaker 1: so in order to do this you need laser pulses. 810 00:40:22,680 --> 00:40:24,879 Speaker 1: You're not just like shining a bright laser beam into 811 00:40:24,920 --> 00:40:27,439 Speaker 1: this thing and heating up all the electrons. You're doing 812 00:40:27,520 --> 00:40:30,600 Speaker 1: laser pulses so that you have like laser pulses at 813 00:40:30,640 --> 00:40:34,080 Speaker 1: different locations through the plasma at the same time. So 814 00:40:34,120 --> 00:40:37,279 Speaker 1: those pulse lengths and the pulse timings have to be 815 00:40:37,440 --> 00:40:40,440 Speaker 1: just right to excite this motion in the plasma, like 816 00:40:40,520 --> 00:40:43,480 Speaker 1: push on the right electrons at the right moment across 817 00:40:43,520 --> 00:40:45,839 Speaker 1: the plasma to get this thing going. I guess it's 818 00:40:45,840 --> 00:40:47,680 Speaker 1: sort of like you said, it's like having a pool 819 00:40:48,040 --> 00:40:50,400 Speaker 1: and then you have kind of like a wave maker 820 00:40:50,440 --> 00:40:52,560 Speaker 1: in the backack, like one of those pool and those 821 00:40:52,880 --> 00:40:55,680 Speaker 1: water parks. Right, You're like you're using the laser to 822 00:40:55,719 --> 00:40:57,759 Speaker 1: create waves in the pool, and then you're sort of 823 00:40:57,840 --> 00:41:00,239 Speaker 1: dropping like a little kid in the life preserver. Hey, 824 00:41:00,280 --> 00:41:02,719 Speaker 1: we'll get pushed by the waves to the shallow end. 825 00:41:02,760 --> 00:41:04,880 Speaker 1: That's kind of the idea, right, that's the idea. And 826 00:41:04,920 --> 00:41:07,920 Speaker 1: the reason this works better than the previous approach of 827 00:41:08,040 --> 00:41:10,680 Speaker 1: just having like two metal plates and an electric field 828 00:41:10,680 --> 00:41:13,319 Speaker 1: across them is because you can have much much stronger 829 00:41:13,360 --> 00:41:17,520 Speaker 1: electric fields in a plasma without anything breaking down. Basically, 830 00:41:17,520 --> 00:41:20,319 Speaker 1: the plasma is already broken down, right, there's nothing else 831 00:41:20,440 --> 00:41:22,960 Speaker 1: to break down, so, like there's no limit to how 832 00:41:23,040 --> 00:41:26,480 Speaker 1: much you can bunch electrons together or something within a 833 00:41:26,520 --> 00:41:29,200 Speaker 1: plasma or there maybe the kind is right is in there, 834 00:41:29,520 --> 00:41:33,200 Speaker 1: Like you can't bunch electrons infinitely. You can't bunch it infinitely, 835 00:41:33,200 --> 00:41:36,200 Speaker 1: but you can dump a lot of energy into this plasma. 836 00:41:36,239 --> 00:41:38,040 Speaker 1: And the cool thing is your laser beam doesn't have 837 00:41:38,120 --> 00:41:40,520 Speaker 1: to have as much energy sort of per photon. You 838 00:41:40,520 --> 00:41:42,759 Speaker 1: can just do a lot of photons to end up 839 00:41:42,880 --> 00:41:44,719 Speaker 1: with a lot of energy. So you don't need to 840 00:41:44,760 --> 00:41:48,160 Speaker 1: already have a super high energy laser to create a 841 00:41:48,200 --> 00:41:51,480 Speaker 1: super high energy particle beam. You can use a high 842 00:41:51,560 --> 00:41:54,480 Speaker 1: intensity laser to dump a lot of energy into the 843 00:41:54,520 --> 00:41:58,080 Speaker 1: plasma which creates these fields, and then accelerate the particles 844 00:41:58,280 --> 00:42:02,120 Speaker 1: to very high energy. Now, which particles are you accelerating 845 00:42:02,160 --> 00:42:04,880 Speaker 1: then the electrons in the plasma or the protons in 846 00:42:04,920 --> 00:42:08,279 Speaker 1: the plasma or are you trying to accelerate something else? Neither, right, 847 00:42:08,320 --> 00:42:10,000 Speaker 1: So then you dump in a particle bunch that you're 848 00:42:10,040 --> 00:42:13,839 Speaker 1: trying to accelerate, and they move through the plasma following 849 00:42:13,880 --> 00:42:17,040 Speaker 1: this wake, following the wake of these electrons, and they're 850 00:42:17,040 --> 00:42:20,040 Speaker 1: sort of like the surfers. Wouldn't you be accelerating protons too? 851 00:42:20,160 --> 00:42:22,600 Speaker 1: Aren't protonons part of the soup? Like how do you 852 00:42:22,600 --> 00:42:24,520 Speaker 1: you know, like if you have a soup with a wave, 853 00:42:24,600 --> 00:42:26,360 Speaker 1: they sort of like in our pool analogy, or you 854 00:42:26,400 --> 00:42:28,080 Speaker 1: have a WaveMaker in the back and you're trying to 855 00:42:28,560 --> 00:42:31,520 Speaker 1: accelerate a drop of water you dump into it. So 856 00:42:31,560 --> 00:42:34,920 Speaker 1: the protons in the plasma don't get accelerated because they 857 00:42:34,920 --> 00:42:37,040 Speaker 1: don't respond on this time scale. The whole thing happens 858 00:42:37,080 --> 00:42:39,239 Speaker 1: like too fast for them to even get moving. The 859 00:42:39,320 --> 00:42:41,719 Speaker 1: electrons in the plasma they do get excited, and you 860 00:42:41,760 --> 00:42:44,239 Speaker 1: do get this wave through the plasma, and then you 861 00:42:44,320 --> 00:42:47,640 Speaker 1: have a third bunch which sort of rides that electric wave. 862 00:42:47,719 --> 00:42:51,120 Speaker 1: The wake of that electron wave is a very high 863 00:42:51,239 --> 00:42:54,479 Speaker 1: gradient electric field which you will accelerate a particle that's 864 00:42:54,480 --> 00:42:57,680 Speaker 1: put in just the right location and velocity the same 865 00:42:57,719 --> 00:43:00,480 Speaker 1: way as surfer needs to catch a wave to ride it, 866 00:43:00,520 --> 00:43:02,960 Speaker 1: they need to be in the right spot and already 867 00:43:03,040 --> 00:43:06,319 Speaker 1: going at the right speed. That's why the surfer rides 868 00:43:06,360 --> 00:43:09,160 Speaker 1: the wave. But the other things are left behind. And 869 00:43:09,200 --> 00:43:11,919 Speaker 1: so you have this like third group which rides that wake, 870 00:43:12,280 --> 00:43:14,839 Speaker 1: sort of like the surfer on the wave right, right, 871 00:43:14,880 --> 00:43:17,839 Speaker 1: but except that the surfer is made out of water too. Yes, 872 00:43:18,000 --> 00:43:20,440 Speaker 1: in this case, the surfer is made out of matter. 873 00:43:20,719 --> 00:43:22,960 Speaker 1: The waves are made out of matter, right. It's just 874 00:43:23,000 --> 00:43:25,719 Speaker 1: a question of where you are and how fast you're 875 00:43:25,760 --> 00:43:28,120 Speaker 1: already going. And so if you're in the right location, 876 00:43:28,120 --> 00:43:31,359 Speaker 1: if it's timed just right, then you're riding that wave 877 00:43:31,400 --> 00:43:34,680 Speaker 1: and you're constantly getting accelerated, whereas electrons in these waves 878 00:43:34,680 --> 00:43:36,919 Speaker 1: are sort of slashing back and forth. I guess maybe 879 00:43:36,960 --> 00:43:38,799 Speaker 1: what's confusing me is that I feel like if you 880 00:43:39,160 --> 00:43:41,760 Speaker 1: drop a bunch of electrons into an electron soup, they'll 881 00:43:41,800 --> 00:43:44,840 Speaker 1: just get, you know, absorbed by the soup. You know. 882 00:43:45,440 --> 00:43:47,360 Speaker 1: But maybe the right way to think about it is 883 00:43:47,400 --> 00:43:50,040 Speaker 1: more like you have this wave pool. You're making the waves, 884 00:43:50,600 --> 00:43:54,360 Speaker 1: and then you shoot. There's a jet of water in 885 00:43:54,360 --> 00:43:57,279 Speaker 1: the back that's shooting it towards the shallow end, and 886 00:43:57,400 --> 00:44:00,839 Speaker 1: somehow it kind of gets an extra busive speed by 887 00:44:00,880 --> 00:44:03,960 Speaker 1: the waves. If you just dropped electrons into any random 888 00:44:04,040 --> 00:44:06,920 Speaker 1: spot in the plasma, they would become part of the plasma. 889 00:44:07,040 --> 00:44:09,640 Speaker 1: But if you set up this wave and then inject 890 00:44:09,680 --> 00:44:13,279 Speaker 1: particles at the right place with the right speed, they 891 00:44:13,360 --> 00:44:16,320 Speaker 1: can ride the wave generated by the plasma without becoming 892 00:44:16,520 --> 00:44:19,839 Speaker 1: part of the plasma. All right, that's the technology. It's 893 00:44:19,920 --> 00:44:23,360 Speaker 1: using plasma. But plasma is kind of tricky, right, Plasma 894 00:44:23,480 --> 00:44:25,920 Speaker 1: is super duper hot and it's really hard to contain, 895 00:44:25,960 --> 00:44:28,879 Speaker 1: and you also need maggots to contain plasma. So how 896 00:44:28,880 --> 00:44:31,439 Speaker 1: well does this technology work? Well, it works really really 897 00:44:31,480 --> 00:44:34,800 Speaker 1: well so far. It's taken decades. Like the original ideas 898 00:44:35,080 --> 00:44:37,280 Speaker 1: are from like the fifties, and then in the seventies 899 00:44:37,320 --> 00:44:39,640 Speaker 1: people started working in the first prototypes. It was actually 900 00:44:39,840 --> 00:44:41,719 Speaker 1: here at you see Irvine and a guy named Norm 901 00:44:41,800 --> 00:44:45,960 Speaker 1: Rustoker who pioneered this technology together with his grand student 902 00:44:46,120 --> 00:44:49,560 Speaker 1: Toshiki Tajima. But they were limited by the laser technology. 903 00:44:49,560 --> 00:44:52,560 Speaker 1: You need like really really fast pulses. And then in 904 00:44:52,600 --> 00:44:56,680 Speaker 1: the nineties people developed like super ultra fast sync lasers 905 00:44:56,800 --> 00:44:59,759 Speaker 1: and that's when the first demonstration was performed. But by 906 00:44:59,800 --> 00:45:01,760 Speaker 1: now people have been doing it all over the world, 907 00:45:01,800 --> 00:45:04,960 Speaker 1: and they've been able to create these little accelerators that 908 00:45:05,000 --> 00:45:09,120 Speaker 1: can accelerate particles to very high speeds over short distances. 909 00:45:09,200 --> 00:45:11,319 Speaker 1: And we typically measure this in terms of like how 910 00:45:11,400 --> 00:45:15,359 Speaker 1: much energy can you dump into a particle per centimeter, right, 911 00:45:15,360 --> 00:45:17,279 Speaker 1: because you want to accelerate a particle and you don't 912 00:45:17,320 --> 00:45:19,400 Speaker 1: want to have to take a mile or two miles 913 00:45:19,400 --> 00:45:22,360 Speaker 1: to do it. And so these little plasma accelerators have 914 00:45:22,400 --> 00:45:25,239 Speaker 1: been able to accelerate particles too much higher energies per 915 00:45:25,320 --> 00:45:28,680 Speaker 1: centimeter than the traditional approach, by a factor of a 916 00:45:28,840 --> 00:45:32,960 Speaker 1: hundred or a thousand. Cool. But I guess you know, 917 00:45:33,000 --> 00:45:35,600 Speaker 1: how are they overcoming the difficulties in the problem? Right? 918 00:45:35,640 --> 00:45:37,480 Speaker 1: Like how do you first of all maintain a plasma 919 00:45:37,520 --> 00:45:40,680 Speaker 1: that's pretty hard, and then how do you shoot electrons 920 00:45:40,680 --> 00:45:41,800 Speaker 1: into it? And how do you get them out of 921 00:45:41,840 --> 00:45:44,880 Speaker 1: the plasma. So maintaining a plasma is not always that hard, right, 922 00:45:45,120 --> 00:45:47,600 Speaker 1: Like you have plasma in the fluorescent lights that are 923 00:45:47,680 --> 00:45:50,400 Speaker 1: above you, or it's just very dilute and so it 924 00:45:50,440 --> 00:45:54,080 Speaker 1: doesn't like destroy the glass. And you typically think about 925 00:45:54,080 --> 00:45:56,279 Speaker 1: plasmas being really hard to contain in the case of 926 00:45:56,280 --> 00:45:59,359 Speaker 1: like fusion experiments, when you need a certain density also 927 00:45:59,400 --> 00:46:01,960 Speaker 1: in order to act fusion. We don't want fusion happening 928 00:46:01,960 --> 00:46:04,120 Speaker 1: in these plasmas, so they don't have to be actually 929 00:46:04,120 --> 00:46:07,200 Speaker 1: that dense. So the containment is not nearly as challenging 930 00:46:07,480 --> 00:46:09,799 Speaker 1: as it is in the case of fusion experiments. You 931 00:46:09,840 --> 00:46:12,160 Speaker 1: can just basically have a can of the plasma and 932 00:46:12,200 --> 00:46:14,719 Speaker 1: it's all right, and that's enough to get particles going. 933 00:46:14,920 --> 00:46:17,400 Speaker 1: That's enough to get particles going. The main challenge was 934 00:46:17,480 --> 00:46:20,560 Speaker 1: really the lasers, and now they've solved that, and so 935 00:46:20,600 --> 00:46:23,200 Speaker 1: now they've really demonstrated this. They have these devices that 936 00:46:23,200 --> 00:46:27,359 Speaker 1: it can actually accelerate particles to tens of GeV over 937 00:46:27,480 --> 00:46:31,319 Speaker 1: centimeters or tens of centimeters, which is very exciting. It's 938 00:46:31,320 --> 00:46:34,680 Speaker 1: exciting because it's a small amount. But you're also you're 939 00:46:34,719 --> 00:46:36,680 Speaker 1: thinking ahead and you're thinking, we're going to stack these 940 00:46:36,760 --> 00:46:39,680 Speaker 1: up to get like a thousand of these to get 941 00:46:39,719 --> 00:46:43,000 Speaker 1: a terra electronvol exactly. So now the question is can 942 00:46:43,040 --> 00:46:45,319 Speaker 1: they scale Where they've done it is they've proven the 943 00:46:45,320 --> 00:46:49,680 Speaker 1: principle that you can accelerate particles more effectively over short distances. 944 00:46:49,760 --> 00:46:52,640 Speaker 1: But we're not that interested in tiny little accelerators. We 945 00:46:52,680 --> 00:46:54,399 Speaker 1: still want them kind of big so we can get 946 00:46:54,400 --> 00:46:56,960 Speaker 1: to really high energies. And so the question is can 947 00:46:57,040 --> 00:46:59,960 Speaker 1: you stack these things up? And that's where the technology 948 00:47:00,200 --> 00:47:02,400 Speaker 1: struggle is right now, because what you need to do 949 00:47:02,520 --> 00:47:04,560 Speaker 1: is like match these things up. You need to keep 950 00:47:04,600 --> 00:47:06,400 Speaker 1: these things in sync. When you have the particles that 951 00:47:06,440 --> 00:47:09,200 Speaker 1: you're accelerating come out of one stage of a plasma 952 00:47:09,239 --> 00:47:11,840 Speaker 1: accelerator and you want to send them into the next one, 953 00:47:11,960 --> 00:47:14,319 Speaker 1: then you have to like time the laser pulses in 954 00:47:14,360 --> 00:47:18,080 Speaker 1: that next plasma accelerator perfectly, so like your little bunch 955 00:47:18,120 --> 00:47:20,919 Speaker 1: of accelerating particles hit just the right part of the wave, 956 00:47:21,239 --> 00:47:23,879 Speaker 1: otherwise everything's lost. And in order to get that all 957 00:47:23,920 --> 00:47:27,440 Speaker 1: that timing just perfectly in sync is very very challenging. 958 00:47:27,560 --> 00:47:29,279 Speaker 1: So what they've been able to do is match a 959 00:47:29,320 --> 00:47:33,200 Speaker 1: couple of stages, maybe up to like five stages, but 960 00:47:33,360 --> 00:47:35,400 Speaker 1: nobody's confident that they can do it for like a 961 00:47:35,560 --> 00:47:37,839 Speaker 1: hundred or a thousand, which is the kind of thing 962 00:47:37,840 --> 00:47:40,040 Speaker 1: you would need to do to really get to like 963 00:47:40,560 --> 00:47:43,800 Speaker 1: physics level accelerators where we can start answering deep questions 964 00:47:43,800 --> 00:47:46,640 Speaker 1: about the universe. So we're maybe still kind of far 965 00:47:46,719 --> 00:47:49,879 Speaker 1: away because you would need to be able to sink 966 00:47:49,960 --> 00:47:53,360 Speaker 1: and stack you're like, you're saying hundreds of these in 967 00:47:53,400 --> 00:47:55,480 Speaker 1: a row or maybe one in a circle. Is the 968 00:47:55,520 --> 00:47:57,080 Speaker 1: idea to put them all in a row and for 969 00:47:57,160 --> 00:48:00,920 Speaker 1: a straight accelerator or to maybe replace its lerators at 970 00:48:00,920 --> 00:48:03,400 Speaker 1: the LC. It depends on what you want to accelerate. 971 00:48:03,680 --> 00:48:06,200 Speaker 1: For electrons, you can't really accelerate them in the circle 972 00:48:06,440 --> 00:48:09,720 Speaker 1: because when you bend electrons in a circle, they radiate 973 00:48:09,719 --> 00:48:13,680 Speaker 1: away photons and they'll lose their energy really really fast. Protons, however, 974 00:48:13,760 --> 00:48:15,600 Speaker 1: you can accelerate them in a circle, and because they 975 00:48:15,640 --> 00:48:18,000 Speaker 1: have more masks, they tend to radiate less. So that's 976 00:48:18,000 --> 00:48:21,480 Speaker 1: why protons accelerators tend to be circles and electron accelerators 977 00:48:21,560 --> 00:48:24,120 Speaker 1: tend to be straight lines. So people want to do both. 978 00:48:24,200 --> 00:48:26,319 Speaker 1: They want to do straight electron accelerators and then want 979 00:48:26,320 --> 00:48:29,960 Speaker 1: to occur protons into circles to smash them together. Protons 980 00:48:29,960 --> 00:48:31,880 Speaker 1: we can tend to get to higher energies because of 981 00:48:31,920 --> 00:48:34,480 Speaker 1: these circular colliders. I think this technology has come a 982 00:48:34,520 --> 00:48:37,000 Speaker 1: long way in the last few decades. It's definitely not 983 00:48:37,120 --> 00:48:40,520 Speaker 1: ready for prime time. Nobody's like proposing, let's build one 984 00:48:40,560 --> 00:48:42,480 Speaker 1: of these things in five years or in ten years. 985 00:48:42,520 --> 00:48:46,840 Speaker 1: But there are like larger and larger demonstration experiments being 986 00:48:46,880 --> 00:48:49,879 Speaker 1: built and that are working, and lots of different ideas 987 00:48:49,920 --> 00:48:52,239 Speaker 1: that people are using to develop these things, not just 988 00:48:52,400 --> 00:48:54,600 Speaker 1: laser pulses, is ones where you drive it with a 989 00:48:54,640 --> 00:48:57,319 Speaker 1: proton beam, and all sorts of other variations. It's a 990 00:48:57,400 --> 00:49:00,640 Speaker 1: very exciting area and it might be in like you know, 991 00:49:00,680 --> 00:49:03,320 Speaker 1: a couple of decades that we're ready to talk about, 992 00:49:03,360 --> 00:49:07,760 Speaker 1: like building a LHC size or super LT size particle 993 00:49:07,800 --> 00:49:11,680 Speaker 1: accelerator that's significantly smaller than the other plans we have. 994 00:49:11,880 --> 00:49:14,960 Speaker 1: So this technology will also accilerate protons. It can also 995 00:49:15,000 --> 00:49:17,560 Speaker 1: accelerate protons, yes, but then I guess you'll run into 996 00:49:17,600 --> 00:49:19,560 Speaker 1: the same problem that you haven't in the LHC, Like 997 00:49:19,640 --> 00:49:22,040 Speaker 1: if you can make them go faster, but then you 998 00:49:22,080 --> 00:49:24,480 Speaker 1: still need to man to bend them into a circle 999 00:49:24,640 --> 00:49:26,600 Speaker 1: or you need to build a bigger circle. Yeah, you'll 1000 00:49:26,600 --> 00:49:28,399 Speaker 1: still have that problem if you want to bend into 1001 00:49:28,400 --> 00:49:31,040 Speaker 1: a circle. But if you have a super duper plasma accelerator, 1002 00:49:31,080 --> 00:49:33,000 Speaker 1: maybe you just get them up to super high speeds 1003 00:49:33,000 --> 00:49:35,480 Speaker 1: in a straight line, which could also work for protons. 1004 00:49:35,520 --> 00:49:38,120 Speaker 1: I mean, if it's powerful enough, then you don't need 1005 00:49:38,160 --> 00:49:41,160 Speaker 1: to go around many many times interesting. Well, there's a 1006 00:49:41,160 --> 00:49:43,560 Speaker 1: lot of promise there. It sounds like it's definitely something 1007 00:49:43,560 --> 00:49:46,160 Speaker 1: people are hoping is around the corner, and that might 1008 00:49:46,200 --> 00:49:49,160 Speaker 1: revolutionize the way we're doing particle physics, because the way 1009 00:49:49,160 --> 00:49:52,640 Speaker 1: we're doing it right now definitely doesn't seem sustainable. I mean, 1010 00:49:52,719 --> 00:49:55,880 Speaker 1: particle physicists are talking about the next generation of colliders 1011 00:49:55,880 --> 00:49:57,680 Speaker 1: and how it's going to cost one hundred billion dollars 1012 00:49:57,680 --> 00:50:00,239 Speaker 1: and I'm all for it, you know, of course, but 1013 00:50:00,280 --> 00:50:02,839 Speaker 1: I'm pretty skeptical that governments are going to pony up 1014 00:50:02,920 --> 00:50:05,720 Speaker 1: that much money for another experiment. And so I'm looking 1015 00:50:05,719 --> 00:50:08,840 Speaker 1: forward to, you know, the revolution that makes particle physics cheaper, 1016 00:50:08,920 --> 00:50:11,239 Speaker 1: faster better. Did I tell you every once went to 1017 00:50:11,280 --> 00:50:13,759 Speaker 1: a conference for this technology? No you didn't. Did it 1018 00:50:13,800 --> 00:50:17,279 Speaker 1: accelerate your mind? Yeah? I got smashed. My brain got 1019 00:50:17,320 --> 00:50:22,000 Speaker 1: smashed a thousand tiny bits. All right. Well, there's a 1020 00:50:22,000 --> 00:50:24,640 Speaker 1: lot of promise in this new way of accelerating things, 1021 00:50:24,760 --> 00:50:27,280 Speaker 1: but it also sounds like there's a ton of challenges 1022 00:50:27,320 --> 00:50:29,200 Speaker 1: because you still have to scale these up, and you 1023 00:50:29,280 --> 00:50:32,280 Speaker 1: still have to maybe potentially bend them into a circle. 1024 00:50:32,480 --> 00:50:35,160 Speaker 1: Which city should we build the next giant particle collider 1025 00:50:35,200 --> 00:50:39,320 Speaker 1: on the Pasadena. Oh good, good, not South Pasadena exactly, 1026 00:50:39,400 --> 00:50:42,400 Speaker 1: always your neighbors. All right, Well, hopefully that made you 1027 00:50:42,440 --> 00:50:44,839 Speaker 1: think a little bit about how scientists are out there 1028 00:50:44,960 --> 00:50:48,080 Speaker 1: trying to break things apart and trying to uncover what's 1029 00:50:48,120 --> 00:50:52,920 Speaker 1: inside of the fundamental particles that make up nature and 1030 00:50:53,480 --> 00:50:56,560 Speaker 1: matter itself. That's right, because to answer the deepest questions 1031 00:50:56,560 --> 00:50:59,480 Speaker 1: in the universe, we need to develop more and more technology. 1032 00:50:59,520 --> 00:51:02,799 Speaker 1: We need better, inc more clever engineers to give us 1033 00:51:02,800 --> 00:51:05,360 Speaker 1: the tools we can use to ask these questions. And 1034 00:51:05,360 --> 00:51:07,839 Speaker 1: maybe it's gonna be plasma technology, or maybe it's gonna 1035 00:51:07,840 --> 00:51:11,440 Speaker 1: be something totally different that somebody else out there sinks up. 1036 00:51:11,560 --> 00:51:14,560 Speaker 1: We need more money or cheaper physicists, one of the two, 1037 00:51:14,880 --> 00:51:17,680 Speaker 1: but the skip fund the engineers. All right, Well, we 1038 00:51:17,719 --> 00:51:20,560 Speaker 1: hope you enjoyed that. Thanks for joining us, See you 1039 00:51:20,600 --> 00:51:30,880 Speaker 1: next time. Thanks for listening, and remember that Daniel and 1040 00:51:30,960 --> 00:51:34,560 Speaker 1: Jorge Explain the Universe is a production of iHeartRadio. For 1041 00:51:34,760 --> 00:51:39,680 Speaker 1: more podcasts from iHeartRadio, visit the iHeartRadio app, Apple Podcasts, 1042 00:51:39,800 --> 00:51:42,160 Speaker 1: or wherever you listen to your favorite shows.