1 00:00:08,520 --> 00:00:10,959 Speaker 1: Hey, Daniel, I have a rude physics question. 2 00:00:11,280 --> 00:00:13,640 Speaker 2: Oh no, not another dark matter poop. 3 00:00:13,480 --> 00:00:15,880 Speaker 1: Jokeer, I hope, I think we did that one already. 4 00:00:16,920 --> 00:00:18,239 Speaker 2: All right then, shoot, all right? 5 00:00:18,360 --> 00:00:21,599 Speaker 1: Is the Higgs boson heavier than expected? 6 00:00:21,880 --> 00:00:24,319 Speaker 2: Are you asking if physicists think the Higgs is like 7 00:00:24,480 --> 00:00:26,560 Speaker 2: too round? That is a bit rude. 8 00:00:27,000 --> 00:00:29,320 Speaker 1: I'm talking about it's mass, not its volume. 9 00:00:31,960 --> 00:00:34,640 Speaker 2: Maybe the Higgs doesn't just give mass to other particles, 10 00:00:34,680 --> 00:00:35,920 Speaker 2: it gives them muscles. 11 00:00:36,200 --> 00:00:39,360 Speaker 1: What like the Higgs is the steroids of the universe? 12 00:00:40,560 --> 00:00:41,160 Speaker 1: Is that legal? 13 00:00:41,600 --> 00:00:43,000 Speaker 2: Lots of physics say yes. 14 00:00:58,600 --> 00:01:00,959 Speaker 1: I am more hamm and cartoonist, the author of Oliver's 15 00:01:01,040 --> 00:01:02,160 Speaker 1: Great Big Universe. 16 00:01:02,240 --> 00:01:05,080 Speaker 2: Hi, I'm Daniel. I'm a particle physicist and a professor 17 00:01:05,120 --> 00:01:08,920 Speaker 2: at UC Irvine, and I feel like my density increases every. 18 00:01:08,800 --> 00:01:13,640 Speaker 1: Year, density of knowledge or density of chocolate eaten, like 19 00:01:13,720 --> 00:01:15,679 Speaker 1: your chocolate cores is getting bigger. 20 00:01:15,720 --> 00:01:18,440 Speaker 2: Well, those two things are tightly correlated, so I'd say 21 00:01:18,480 --> 00:01:18,800 Speaker 2: yes to. 22 00:01:18,800 --> 00:01:23,399 Speaker 1: Be What do you need like chocolate gives you knowledge? 23 00:01:25,480 --> 00:01:28,760 Speaker 2: Well, there's definitely a correlation between Nobel Prizes one and 24 00:01:28,920 --> 00:01:30,440 Speaker 2: chocolate consumed per capita. 25 00:01:30,640 --> 00:01:32,920 Speaker 1: Oh interesting, but which one comes first? 26 00:01:34,400 --> 00:01:37,240 Speaker 2: We don't have to get into correlation versus causation when 27 00:01:37,280 --> 00:01:38,679 Speaker 2: it comes to chocolate. 28 00:01:38,400 --> 00:01:40,360 Speaker 1: I think we do. I mean makes a big difference. 29 00:01:40,680 --> 00:01:42,760 Speaker 1: Like if you have to eat a lot of chocolate 30 00:01:42,800 --> 00:01:44,600 Speaker 1: after you win the Noble Price, and you kind of 31 00:01:44,640 --> 00:01:45,600 Speaker 1: have a lot of work to do. 32 00:01:45,600 --> 00:01:47,120 Speaker 2: All right, let me go get some chocolate and then 33 00:01:47,120 --> 00:01:47,880 Speaker 2: we'll figure this out. 34 00:01:47,960 --> 00:01:50,880 Speaker 1: No, no, no, that's the whole point. You should maybe 35 00:01:50,920 --> 00:01:53,360 Speaker 1: figure out what's the causation here. 36 00:01:53,760 --> 00:01:56,600 Speaker 2: I can't figure anything out without chocolate. It's my superpower. 37 00:01:56,760 --> 00:01:59,400 Speaker 1: Then you're in a paradox. What did you need chocolate 38 00:01:59,480 --> 00:02:01,200 Speaker 1: after you win the Nobel Prize? But you can win 39 00:02:01,240 --> 00:02:03,360 Speaker 1: the Nobel Prize until unless you eat a lot of chocolate. 40 00:02:03,400 --> 00:02:05,600 Speaker 2: What if I opt for a Nobel Price that's not gold, 41 00:02:05,680 --> 00:02:08,320 Speaker 2: it's just gold foil around bad chocolate. 42 00:02:08,919 --> 00:02:12,120 Speaker 1: That doesn't af fix your paradox, though maybe it may 43 00:02:12,240 --> 00:02:15,400 Speaker 1: just means it's impossible. But anyways, Welcome to our podcast, 44 00:02:15,440 --> 00:02:19,480 Speaker 1: Daniel and Jorge Explain the Universe, a production of iHeartRadio. 45 00:02:18,880 --> 00:02:22,359 Speaker 2: In which we dig into the apparent paradox of our universe. 46 00:02:22,480 --> 00:02:27,080 Speaker 2: It is both mysterious and bizarre, and yet somehow also understandable. 47 00:02:27,280 --> 00:02:30,440 Speaker 2: Working carefully at the cold face of knowledge, we can 48 00:02:30,440 --> 00:02:33,359 Speaker 2: hammer away at it and slowly build up an understanding 49 00:02:33,440 --> 00:02:37,040 Speaker 2: of how this universe works from its tiny little quantum 50 00:02:37,080 --> 00:02:40,360 Speaker 2: particles that weave themselves together to give us this reality 51 00:02:40,520 --> 00:02:41,280 Speaker 2: we know and love. 52 00:02:41,400 --> 00:02:44,840 Speaker 1: That's right, the universe is deliciously perplexing. It's dark, and 53 00:02:45,040 --> 00:02:48,359 Speaker 1: it's velvedly smooth, just like chocolate, which means we can't 54 00:02:48,360 --> 00:02:49,079 Speaker 1: get enough of it. 55 00:02:49,160 --> 00:02:53,840 Speaker 2: And it is massive. Not only is it very, very large, 56 00:02:53,880 --> 00:02:57,239 Speaker 2: but it's also filled with a lot of stuff black 57 00:02:57,280 --> 00:03:01,120 Speaker 2: holes and neutron stars and just normal stars and rocky 58 00:03:01,160 --> 00:03:04,520 Speaker 2: planets and maybe squishy little beings crawling on their surface. 59 00:03:04,960 --> 00:03:07,120 Speaker 1: And thank goodness it has squishy little beings like us, 60 00:03:07,160 --> 00:03:09,240 Speaker 1: because we're here to ask questions about it, and we 61 00:03:09,320 --> 00:03:11,359 Speaker 1: do that here on the podcast, where we tackle the 62 00:03:11,400 --> 00:03:14,320 Speaker 1: big unknowns about how this universe works and why it 63 00:03:14,400 --> 00:03:15,120 Speaker 1: is the way it is. 64 00:03:15,240 --> 00:03:17,520 Speaker 2: And often on the podcast we're telling you about the 65 00:03:17,520 --> 00:03:19,799 Speaker 2: things that we have learned in science. But one of 66 00:03:19,880 --> 00:03:22,000 Speaker 2: my favorite kinds of episodes are the ones that dig 67 00:03:22,040 --> 00:03:25,040 Speaker 2: into how we figure it out how we know what 68 00:03:25,120 --> 00:03:27,919 Speaker 2: we know. Rather than just swallowing the numbers as scientists 69 00:03:27,919 --> 00:03:30,160 Speaker 2: give us, we want to unwrap them and figure out 70 00:03:30,320 --> 00:03:33,240 Speaker 2: how exactly they measured this or that to be whatever 71 00:03:33,320 --> 00:03:33,920 Speaker 2: number it is. 72 00:03:34,160 --> 00:03:35,680 Speaker 1: Yeah, because there is a lot to know about the 73 00:03:35,720 --> 00:03:37,560 Speaker 1: universe and a lot that science has figured out, and 74 00:03:37,600 --> 00:03:39,800 Speaker 1: it's interesting to dig into how it is that we 75 00:03:39,880 --> 00:03:43,800 Speaker 1: know these things. Just sometimes the story is maybe even 76 00:03:43,840 --> 00:03:45,480 Speaker 1: better than the facts that you've learned. 77 00:03:45,560 --> 00:03:48,480 Speaker 2: Experimental science is not just go out there and check 78 00:03:48,520 --> 00:03:52,160 Speaker 2: the theoretical predictions. Sometimes the theory doesn't make any predictions, 79 00:03:52,160 --> 00:03:54,400 Speaker 2: and it just says, we don't know how heavy this 80 00:03:54,440 --> 00:03:57,880 Speaker 2: thing is. Go measure it, and measuring it requires inventing 81 00:03:57,960 --> 00:04:01,440 Speaker 2: all sorts of cool and clever tre That's what experimental 82 00:04:01,520 --> 00:04:04,040 Speaker 2: science is all about, and we like to celebrate that 83 00:04:04,080 --> 00:04:06,520 Speaker 2: here in the podcast. We've had fun episodes about all 84 00:04:06,560 --> 00:04:10,040 Speaker 2: of the inventiveness necessary to measure the speed of light, 85 00:04:10,360 --> 00:04:13,000 Speaker 2: or to measure the gravitational constant. 86 00:04:12,760 --> 00:04:15,720 Speaker 1: Or to measure how much chocolate. Physicists can eat safely. 87 00:04:16,440 --> 00:04:18,479 Speaker 2: Data says there is no upper bound. 88 00:04:20,480 --> 00:04:23,880 Speaker 1: Really, that doesn't sound like a scientific statement. I think 89 00:04:23,880 --> 00:04:25,920 Speaker 1: science is pretty clear there is a limit to how 90 00:04:25,960 --> 00:04:27,120 Speaker 1: much chocolate you can eat. 91 00:04:27,200 --> 00:04:29,479 Speaker 2: I don't know. I haven't yet collapsed into a black hole, 92 00:04:29,520 --> 00:04:30,760 Speaker 2: but that may be in my future. 93 00:04:31,200 --> 00:04:33,360 Speaker 1: I guess it's hard to prove a negative or a 94 00:04:33,360 --> 00:04:34,240 Speaker 1: maximum m hm. 95 00:04:34,960 --> 00:04:36,520 Speaker 2: Really the question is if you eat a lot of 96 00:04:36,560 --> 00:04:38,599 Speaker 2: white chocolate, do you turn into a white hole or 97 00:04:38,640 --> 00:04:39,240 Speaker 2: a black hole? 98 00:04:39,520 --> 00:04:41,200 Speaker 1: So to be on the podcast, we'll be asking the 99 00:04:41,320 --> 00:04:49,880 Speaker 1: question how do we measure the Higgs Bosons mass? 100 00:04:50,520 --> 00:04:51,840 Speaker 2: Did you say mass or math? 101 00:04:52,640 --> 00:04:55,760 Speaker 1: I think I said mass, right, So we do. 102 00:04:55,680 --> 00:04:57,360 Speaker 2: Have to use a lot of math to figure out 103 00:04:57,360 --> 00:04:58,599 Speaker 2: the Higgs Boson mass. 104 00:04:58,640 --> 00:05:01,279 Speaker 1: Of course, exposed on have its own math. 105 00:05:01,400 --> 00:05:03,359 Speaker 2: As far as we know, there is just one math. 106 00:05:03,440 --> 00:05:06,880 Speaker 2: There is the math. But everything has its own mass, 107 00:05:07,279 --> 00:05:09,840 Speaker 2: and it's an interesting puzzle to figure out why some 108 00:05:09,880 --> 00:05:12,400 Speaker 2: particles have a lot of it, why some particles don't 109 00:05:12,440 --> 00:05:13,960 Speaker 2: seem to have a lot of it, and to learn 110 00:05:13,960 --> 00:05:17,120 Speaker 2: about exactly how we measure the mass of these tiny 111 00:05:17,279 --> 00:05:19,719 Speaker 2: little particles. You can even just barely see. 112 00:05:19,880 --> 00:05:22,000 Speaker 1: Well, some particles don't have any mass, right. 113 00:05:21,880 --> 00:05:26,320 Speaker 2: Yeah, that's right. Photons have no mass, Gluons have no mass. Gravitons, 114 00:05:26,360 --> 00:05:29,159 Speaker 2: if they exist, probably have no mass as well. Mass 115 00:05:29,200 --> 00:05:31,680 Speaker 2: isn't even a necessary attribute, like you can be a 116 00:05:31,720 --> 00:05:33,760 Speaker 2: thing without having any stuff to you. 117 00:05:34,120 --> 00:05:36,839 Speaker 1: Right, Although, as we've talked about many times on the podcast, 118 00:05:37,200 --> 00:05:39,560 Speaker 1: the question or the idea of mass is kind of 119 00:05:39,560 --> 00:05:41,920 Speaker 1: a tricky one, right, Like there are different kinds of masses, 120 00:05:42,000 --> 00:05:45,120 Speaker 1: and also like what you might call mass is not 121 00:05:45,160 --> 00:05:47,440 Speaker 1: necessarily the stuff that you have about you. 122 00:05:47,680 --> 00:05:51,080 Speaker 2: Yeah, our intuitive understanding of mass is different from the 123 00:05:51,120 --> 00:05:55,560 Speaker 2: sort of mathematical physical description of matter at its most microscopic. 124 00:05:55,760 --> 00:05:58,279 Speaker 1: Well, this is an interesting question because the Higgs boson 125 00:05:58,680 --> 00:06:00,800 Speaker 1: is a pretty big deal in the right. I mean, 126 00:06:00,839 --> 00:06:03,360 Speaker 1: it was discovered a few years ago and people were 127 00:06:03,440 --> 00:06:06,359 Speaker 1: very excited because apparently it is a very important particle 128 00:06:06,400 --> 00:06:09,200 Speaker 1: in the pathion of particles in that it gives mass 129 00:06:09,200 --> 00:06:10,000 Speaker 1: to other particles. 130 00:06:10,080 --> 00:06:12,919 Speaker 2: Yeah, the Higgs boson is a feature of the Higgs field, 131 00:06:13,000 --> 00:06:15,760 Speaker 2: which fills the whole universe. Like other quantum fields, it 132 00:06:15,800 --> 00:06:18,360 Speaker 2: can be excited into making a particle, or it can 133 00:06:18,400 --> 00:06:21,320 Speaker 2: be chill and relaxed down to its lowest state. But 134 00:06:21,320 --> 00:06:24,440 Speaker 2: the Higgs boson, the Higgs particle, the excitation of the 135 00:06:24,560 --> 00:06:28,560 Speaker 2: Higgs field, has all sorts of particle like properties. It moves, 136 00:06:28,640 --> 00:06:30,960 Speaker 2: it has mass, and the value of its mass is 137 00:06:31,040 --> 00:06:35,119 Speaker 2: really important. It's important theoretically and it's important experimentally. 138 00:06:35,279 --> 00:06:37,320 Speaker 1: As the big question is how do you measure the 139 00:06:37,360 --> 00:06:40,800 Speaker 1: mass of something so important, so crucial to the concept 140 00:06:40,839 --> 00:06:43,400 Speaker 1: of mass itself like the Higgs boson, and so, as 141 00:06:43,480 --> 00:06:45,200 Speaker 1: usually you were wondering how many people out there had 142 00:06:45,200 --> 00:06:47,680 Speaker 1: thought about this question and wondered if they can just 143 00:06:47,720 --> 00:06:49,400 Speaker 1: ask the Higgs boson it's mass. 144 00:06:49,520 --> 00:06:52,840 Speaker 2: How rude, But thank you very much everybody who volunteers 145 00:06:52,880 --> 00:06:54,800 Speaker 2: for this segment of the podcast. If you would like 146 00:06:54,839 --> 00:06:56,800 Speaker 2: to participate, please don't be shy and write to me 147 00:06:57,120 --> 00:07:00,520 Speaker 2: to questions at Danielanjorge dot com. I am waiting for 148 00:07:00,600 --> 00:07:01,200 Speaker 2: your email. 149 00:07:01,520 --> 00:07:03,039 Speaker 1: So think about it for a second. How do you 150 00:07:03,080 --> 00:07:07,320 Speaker 1: think physicists measure the Higgs bosons mass? Here's what people 151 00:07:07,360 --> 00:07:07,800 Speaker 1: had to say. 152 00:07:08,320 --> 00:07:11,680 Speaker 3: I know from the episode on where does the Higgs 153 00:07:11,800 --> 00:07:16,520 Speaker 3: get its mass that you can look at how it 154 00:07:16,600 --> 00:07:20,000 Speaker 3: interacts with the other fields like the top cork and 155 00:07:20,040 --> 00:07:24,240 Speaker 3: the strange cork, and maybe with its interacting with its 156 00:07:24,320 --> 00:07:27,880 Speaker 3: own field. But I have no idea how you measure it. 157 00:07:28,320 --> 00:07:35,120 Speaker 4: I now believe that we can view a boson, and 158 00:07:35,200 --> 00:07:39,240 Speaker 4: so therefore I would imagine you could put it in 159 00:07:40,160 --> 00:07:47,840 Speaker 4: a particle accelerator and throw something at it, and by 160 00:07:47,880 --> 00:07:51,440 Speaker 4: that makes the calculations to measure its mass. 161 00:07:51,680 --> 00:07:54,120 Speaker 5: Measuring the mass of the Higgs is going to be 162 00:07:54,920 --> 00:08:00,160 Speaker 5: exceedingly difficult. Even an optical system would probably be much 163 00:08:00,200 --> 00:08:04,800 Speaker 5: too large to get the mass of the system. I 164 00:08:04,880 --> 00:08:12,560 Speaker 5: one could assume that some interplanetary system telescope might actually 165 00:08:12,640 --> 00:08:16,520 Speaker 5: be a way to go, if we were able to 166 00:08:16,600 --> 00:08:17,560 Speaker 5: figure that out. 167 00:08:17,960 --> 00:08:23,760 Speaker 6: If I remember it right, the Higgs boson was discovered 168 00:08:23,800 --> 00:08:29,320 Speaker 6: when they could detect a pair of photons that were 169 00:08:29,320 --> 00:08:33,720 Speaker 6: emitted in the collider. So maybe its mass would be 170 00:08:33,800 --> 00:08:37,679 Speaker 6: equivalent to the energy of those two photoms. 171 00:08:37,840 --> 00:08:38,720 Speaker 2: I have no idea. 172 00:08:38,800 --> 00:08:41,959 Speaker 5: It could have something to do with its track after 173 00:08:42,160 --> 00:08:43,400 Speaker 5: collision analysis it. 174 00:08:43,520 --> 00:08:46,280 Speaker 1: Turned all right. I am with the last person here 175 00:08:46,280 --> 00:08:50,199 Speaker 1: who said, I have no idea. Sounds like a great title. 176 00:08:49,960 --> 00:08:53,240 Speaker 2: For a book. We should write a book like that. 177 00:08:53,360 --> 00:08:55,800 Speaker 1: Maybe with Tilight we have No Idea and make it 178 00:08:55,840 --> 00:09:01,080 Speaker 1: available for purchase at bookstores and kind of book website. 179 00:09:01,760 --> 00:09:02,680 Speaker 1: That would be a good idea. 180 00:09:03,559 --> 00:09:05,720 Speaker 2: That would be a very good idea. In fact, if 181 00:09:05,720 --> 00:09:07,959 Speaker 2: you went to we have no idea dot com, you 182 00:09:08,040 --> 00:09:09,640 Speaker 2: might even be able to find such a book. 183 00:09:09,760 --> 00:09:12,440 Speaker 1: That's an amazing idea. But yeah, this is an interesting question. 184 00:09:12,600 --> 00:09:14,920 Speaker 1: How do you measure the Higgs bosons mass? If the 185 00:09:14,960 --> 00:09:17,280 Speaker 1: Higgs feel is what gives things mass, it's a bit 186 00:09:17,320 --> 00:09:19,920 Speaker 1: of a conundrum there, So when don't we start at 187 00:09:19,920 --> 00:09:22,840 Speaker 1: the beginning at Daniel? What is the Higgs boson for 188 00:09:22,920 --> 00:09:23,720 Speaker 1: people who don't. 189 00:09:23,559 --> 00:09:25,880 Speaker 2: Know, So, the Higgs boson is an idea that came 190 00:09:25,960 --> 00:09:28,880 Speaker 2: out of the nineteen sixties when people were looking at 191 00:09:28,920 --> 00:09:33,360 Speaker 2: the electromagnetic interaction, which is mediated by the photon, and 192 00:09:33,720 --> 00:09:36,320 Speaker 2: the weak force, which is mediated by the Z and 193 00:09:36,360 --> 00:09:39,440 Speaker 2: the W bosons. So you have these two forces which 194 00:09:39,440 --> 00:09:42,400 Speaker 2: seemed pretty different. The weak force is very weak and 195 00:09:42,400 --> 00:09:45,360 Speaker 2: it has these three weird bosons that mediate it, and 196 00:09:45,400 --> 00:09:47,800 Speaker 2: the electromagnetic force is very strong. It's the one that 197 00:09:47,800 --> 00:09:50,040 Speaker 2: we know, you know, makes lightning and magnets and all 198 00:09:50,040 --> 00:09:52,920 Speaker 2: sorts of stuff and binds together protons electrons into atoms 199 00:09:52,960 --> 00:09:56,000 Speaker 2: and weaves those atoms together into molecules and basically makes 200 00:09:56,040 --> 00:09:58,959 Speaker 2: the structure of everything around us. So it's felt like 201 00:09:59,120 --> 00:10:01,560 Speaker 2: very different forces, but people had an idea that they 202 00:10:01,640 --> 00:10:05,040 Speaker 2: might just click together into one larger idea, which they 203 00:10:05,080 --> 00:10:06,920 Speaker 2: call the electroweak force. 204 00:10:07,120 --> 00:10:09,160 Speaker 1: Now, what do people know about the weak force or 205 00:10:09,160 --> 00:10:11,959 Speaker 1: how do we discover it and what do we think 206 00:10:12,000 --> 00:10:12,360 Speaker 1: it was for? 207 00:10:12,520 --> 00:10:15,000 Speaker 2: Well, the weak force was discovered several decades ago, and 208 00:10:15,160 --> 00:10:18,600 Speaker 2: it was known to be involved in radioactive decay. So, 209 00:10:18,679 --> 00:10:21,880 Speaker 2: for example, when a nucleus decays down to a lighter element, 210 00:10:22,120 --> 00:10:25,880 Speaker 2: it does so using a process called beta decay. Then 211 00:10:25,920 --> 00:10:28,599 Speaker 2: that involves the weak force. So we knew that the 212 00:10:28,600 --> 00:10:30,440 Speaker 2: weak force was a thing, and we knew that it 213 00:10:30,480 --> 00:10:33,880 Speaker 2: did some stuff and it was different from electromagnetism. We 214 00:10:33,920 --> 00:10:36,319 Speaker 2: had postulated the idea that there might be a particle 215 00:10:36,360 --> 00:10:38,840 Speaker 2: out there that only feels the weak force, the neutrino, 216 00:10:39,200 --> 00:10:40,800 Speaker 2: but it hadn't yet been observed. 217 00:10:42,240 --> 00:10:46,040 Speaker 1: Like we knew about radioactive decay, like uranium decays into 218 00:10:46,600 --> 00:10:48,720 Speaker 1: a lower mass uranium. But I guess you needed some 219 00:10:48,800 --> 00:10:50,560 Speaker 1: kind of mechanism for it to do that, and you 220 00:10:50,600 --> 00:10:52,480 Speaker 1: had to sort of invent the force to do that, 221 00:10:52,679 --> 00:10:54,800 Speaker 1: or like it only made sense if you had this 222 00:10:54,880 --> 00:10:55,720 Speaker 1: new kind of force. 223 00:10:56,040 --> 00:11:00,320 Speaker 2: Yeah, you can't explain radioactive decay using just electromagnetism or 224 00:11:00,440 --> 00:11:03,400 Speaker 2: just a strong force. You need a new kind of phenomenon. 225 00:11:03,600 --> 00:11:05,920 Speaker 2: And that's sort of the history of forces, right. We 226 00:11:05,960 --> 00:11:08,320 Speaker 2: see all this stuff out there in the world, and 227 00:11:08,360 --> 00:11:10,080 Speaker 2: we tried to describe it using sort of like the 228 00:11:10,120 --> 00:11:13,520 Speaker 2: shortest possible list of explanations. But sometimes you have to 229 00:11:13,559 --> 00:11:15,920 Speaker 2: add one, you know, like when first time people ever 230 00:11:15,920 --> 00:11:18,280 Speaker 2: saw lightning. They're like, hmm, well, you can't explain that 231 00:11:18,559 --> 00:11:20,920 Speaker 2: with everything we know, So let's add some into the lists. 232 00:11:20,960 --> 00:11:24,360 Speaker 2: Let's say there's a new kind of force electricity, and 233 00:11:24,400 --> 00:11:26,360 Speaker 2: people saw magnets and they're like, ooh wow, this is 234 00:11:26,360 --> 00:11:28,600 Speaker 2: a cool new thing. So then magnets were added to 235 00:11:28,600 --> 00:11:30,960 Speaker 2: the list. Later, we try to shrink that list by 236 00:11:31,000 --> 00:11:33,760 Speaker 2: seeing if we can combine those forces. So electricity and 237 00:11:33,760 --> 00:11:37,440 Speaker 2: magnetism actually two sides of the same force, now just 238 00:11:37,520 --> 00:11:40,960 Speaker 2: one idea electromagnetism. So the weak force was responsible for 239 00:11:41,000 --> 00:11:43,720 Speaker 2: a distinct kind of phenomena that we couldn't explain using 240 00:11:43,760 --> 00:11:46,200 Speaker 2: other forces. But then people were eager to see if 241 00:11:46,200 --> 00:11:48,559 Speaker 2: they could squeeze it together with the other forces. 242 00:11:48,960 --> 00:11:51,280 Speaker 1: What made them think that you could squeeze them together, Like, 243 00:11:51,400 --> 00:11:55,000 Speaker 1: for example, they didn't try to squish together electromagnetism and gravity, 244 00:11:55,080 --> 00:11:55,400 Speaker 1: did they? 245 00:11:55,520 --> 00:11:57,920 Speaker 2: Oh? Yes they did. Einstein spent most of his life 246 00:11:57,960 --> 00:12:01,120 Speaker 2: trying to accomplish that actually and failing, And so theorists 247 00:12:01,160 --> 00:12:03,760 Speaker 2: basically trying to squeeze everything possible together. You know, it's 248 00:12:03,800 --> 00:12:05,320 Speaker 2: like we're looking at a bunch of puzzle pieces on 249 00:12:05,360 --> 00:12:07,440 Speaker 2: the table and we're like, hm, does this fit with that? Nope? 250 00:12:07,520 --> 00:12:10,840 Speaker 2: Does this fit with that? Nope? And electricity and magnetism 251 00:12:11,120 --> 00:12:14,880 Speaker 2: almost fit together just perfectly together with the weak force, 252 00:12:15,240 --> 00:12:18,080 Speaker 2: like they clicked into place, almost perfectly. There was just 253 00:12:18,120 --> 00:12:20,400 Speaker 2: like a little gap missing, and that gap was the 254 00:12:20,480 --> 00:12:21,800 Speaker 2: Higgs boson. Oh. 255 00:12:21,880 --> 00:12:24,920 Speaker 1: Interesting, So the Higgs field and the Higgs boson was 256 00:12:25,040 --> 00:12:26,520 Speaker 1: that missing piece exactly. 257 00:12:26,559 --> 00:12:29,880 Speaker 2: That's why they suspected that it existed, because it seemed 258 00:12:30,000 --> 00:12:32,640 Speaker 2: very likely that these two forces could click together, but 259 00:12:32,720 --> 00:12:36,000 Speaker 2: it didn't quite work. The problem was that photons have 260 00:12:36,160 --> 00:12:38,679 Speaker 2: no mass. Their mass lists right, but the W and 261 00:12:38,800 --> 00:12:41,440 Speaker 2: Z bosons were very, very massive, and that made it 262 00:12:41,520 --> 00:12:44,240 Speaker 2: very very hard to click these two together unless you 263 00:12:44,280 --> 00:12:47,320 Speaker 2: had some special thing out there which could give mass 264 00:12:47,320 --> 00:12:49,240 Speaker 2: to the W and the Z and not give it 265 00:12:49,240 --> 00:12:52,040 Speaker 2: to the photon. And that's what the Higgs does. It 266 00:12:52,120 --> 00:12:55,920 Speaker 2: solves this problem of electroweak symmetry. It's called and noo. 267 00:12:55,920 --> 00:12:58,680 Speaker 2: They tried to bring in the strong force. They just 268 00:12:59,120 --> 00:13:04,120 Speaker 2: decide to the strong force. People basically work on every combination. 269 00:13:04,200 --> 00:13:06,040 Speaker 2: If you could bring the strong force together with the 270 00:13:06,080 --> 00:13:09,960 Speaker 2: electroweak force, then you've achieved a grand unified theory, something 271 00:13:10,040 --> 00:13:11,560 Speaker 2: nobody has been able to make work. 272 00:13:11,600 --> 00:13:13,840 Speaker 1: So far mathematically, would you have to call it like 273 00:13:13,920 --> 00:13:17,520 Speaker 1: the electro met force. It's not weak, it's not strong. 274 00:13:17,600 --> 00:13:18,959 Speaker 1: It's just kind of meant. 275 00:13:19,280 --> 00:13:21,320 Speaker 2: Well, you know, there'd be an interesting argument there about 276 00:13:21,360 --> 00:13:23,679 Speaker 2: like which names get kept and which names get dropped. 277 00:13:23,679 --> 00:13:26,400 Speaker 2: I don't know if you noticed, but when electromagnetism got 278 00:13:26,440 --> 00:13:29,480 Speaker 2: merged with the weak force, magnetism got dropped, like the 279 00:13:29,559 --> 00:13:32,080 Speaker 2: least influential partner in a law firm that merged with 280 00:13:32,120 --> 00:13:34,320 Speaker 2: a bigger firm. Right, it's just gone. 281 00:13:35,280 --> 00:13:38,320 Speaker 1: They couldn't just keep phyphonating. I guess I don't know. 282 00:13:38,400 --> 00:13:41,120 Speaker 2: I think they could have. It's a bummer to lose magnetism. 283 00:13:41,120 --> 00:13:43,080 Speaker 2: I like magnets. I don't know what they would call it. 284 00:13:43,120 --> 00:13:46,040 Speaker 2: But the official name right now is the Grand Unified Theory. 285 00:13:46,440 --> 00:13:48,360 Speaker 2: You can bring those together, then you have a grand 286 00:13:48,440 --> 00:13:51,000 Speaker 2: unified theory. And people have been trying all sorts of ways, 287 00:13:51,000 --> 00:13:52,600 Speaker 2: but nobody's been able to make it click. 288 00:13:52,679 --> 00:13:54,679 Speaker 1: All right, So then the Higgs boson and the Higgs 289 00:13:54,679 --> 00:13:57,840 Speaker 1: field made the electromagnetic force and the weak force click together. 290 00:13:58,000 --> 00:13:59,680 Speaker 1: So that's kind of where it came from the idea 291 00:13:59,720 --> 00:14:00,000 Speaker 1: for it. 292 00:14:00,640 --> 00:14:02,600 Speaker 2: That's right, That's why we thought it had to be 293 00:14:02,679 --> 00:14:05,520 Speaker 2: there it or something else which did that job, which 294 00:14:05,520 --> 00:14:07,960 Speaker 2: gave mass to the w Z bosons. And also they 295 00:14:07,960 --> 00:14:09,559 Speaker 2: were able to add a little piece to the Higgs 296 00:14:09,600 --> 00:14:11,520 Speaker 2: force and say, oh, also it interacts with all the 297 00:14:11,559 --> 00:14:14,800 Speaker 2: matter particles and gives them mass as well. So it 298 00:14:14,880 --> 00:14:17,040 Speaker 2: was a very cute little idea, and then we found 299 00:14:17,080 --> 00:14:20,680 Speaker 2: it in twenty twelve, this fantastic triumph of theoretical physics, 300 00:14:20,680 --> 00:14:23,000 Speaker 2: to say, you know, there's a pattern out there that's 301 00:14:23,000 --> 00:14:25,000 Speaker 2: missing a piece. It would make much more sense if 302 00:14:25,040 --> 00:14:27,600 Speaker 2: it existed in the universe, and boom, there it does. 303 00:14:27,680 --> 00:14:30,280 Speaker 2: It makes you feel like, wow, math is not just 304 00:14:30,320 --> 00:14:34,040 Speaker 2: like describing the universe. Maybe it's dictating how the universe works. 305 00:14:34,160 --> 00:14:36,320 Speaker 1: You know, wait, which math? The math are one of 306 00:14:36,360 --> 00:14:36,680 Speaker 1: the math? 307 00:14:38,320 --> 00:14:40,640 Speaker 2: The math, and in this case it's group theory. This 308 00:14:40,840 --> 00:14:43,440 Speaker 2: really weird, abstract kind of math that was invented by 309 00:14:43,440 --> 00:14:45,920 Speaker 2: a bunch of French guys in the eighteen hundreds, not 310 00:14:45,960 --> 00:14:48,560 Speaker 2: because they were interested in particle physics or really physics 311 00:14:48,560 --> 00:14:50,640 Speaker 2: at all. They were just like, huh, look at these 312 00:14:50,640 --> 00:14:53,760 Speaker 2: cool symmetries and patterns. Maybe we can describe them mathematically. 313 00:14:54,080 --> 00:14:57,480 Speaker 2: And then decades later particle physicists were like Ooh, that 314 00:14:57,560 --> 00:15:01,400 Speaker 2: math perfectly described the patterns we're among these particles. Thank 315 00:15:01,440 --> 00:15:03,720 Speaker 2: you very much mathematicians for inventing this tool. 316 00:15:03,920 --> 00:15:06,000 Speaker 1: All right, So, then the Higgs field and the Higgs 317 00:15:06,040 --> 00:15:09,040 Speaker 1: boson is what gives other particles their mass, right, Like, 318 00:15:09,080 --> 00:15:11,760 Speaker 1: if the electron has a certain mass with meaning that 319 00:15:11,800 --> 00:15:14,200 Speaker 1: it's hard to get it moving and it's hard to 320 00:15:14,360 --> 00:15:17,000 Speaker 1: get it to stop, that's inertial mass. That's all due 321 00:15:17,040 --> 00:15:17,960 Speaker 1: to the Higgs field. 322 00:15:18,040 --> 00:15:20,600 Speaker 2: That's right. As the electron moves through the universe, it 323 00:15:20,680 --> 00:15:24,119 Speaker 2: interacts with the Higgs field. That changes how the electron 324 00:15:24,240 --> 00:15:26,720 Speaker 2: moves in a way that to us looks like the 325 00:15:26,760 --> 00:15:29,680 Speaker 2: electron itself has mass. And there's an argument to me 326 00:15:29,720 --> 00:15:31,880 Speaker 2: made to say that the true, the real, the pure 327 00:15:32,040 --> 00:15:35,480 Speaker 2: electron has no mass. But what we see isn't the 328 00:15:35,480 --> 00:15:38,120 Speaker 2: pure electron. We see this like cloud of an electron 329 00:15:38,160 --> 00:15:41,280 Speaker 2: interacting with Higgs bosons, and that's what we call an 330 00:15:41,280 --> 00:15:44,240 Speaker 2: electron because that's what we interact with. We see, we 331 00:15:44,280 --> 00:15:47,200 Speaker 2: measure in our laboratory, and that object, the sort of 332 00:15:47,200 --> 00:15:50,680 Speaker 2: electron interwoven with the Higgs field, that thing has the 333 00:15:50,720 --> 00:15:51,800 Speaker 2: mass of an electron. 334 00:15:52,440 --> 00:15:54,840 Speaker 1: And that's also how you explain how some particles like 335 00:15:54,880 --> 00:15:57,320 Speaker 1: the photon don't have mass. Right, You just figure out 336 00:15:57,320 --> 00:15:59,360 Speaker 1: that in the universe some particles interact with the Higgs 337 00:15:59,360 --> 00:16:02,080 Speaker 1: fields and then some don't, right, Like the photon doesn't 338 00:16:02,080 --> 00:16:03,880 Speaker 1: interact with the Higg fields, and so it doesn't have 339 00:16:03,920 --> 00:16:05,240 Speaker 1: this inertial mass. 340 00:16:05,120 --> 00:16:07,280 Speaker 2: Right exactly. And on one hand, it answers a deep 341 00:16:07,360 --> 00:16:10,640 Speaker 2: question why does the electron have mass? The answer is, oh, 342 00:16:10,640 --> 00:16:12,800 Speaker 2: it interacts with the Higgs field, but it doesn't answer 343 00:16:12,840 --> 00:16:14,720 Speaker 2: a much deeper question, which is like, well, why does 344 00:16:14,760 --> 00:16:17,360 Speaker 2: the muon have more mass? The answer is just, well, 345 00:16:17,360 --> 00:16:19,640 Speaker 2: it interacts more with the Higgs boson, sort of like 346 00:16:19,720 --> 00:16:22,080 Speaker 2: kicks the question down the road to like, well, why 347 00:16:22,120 --> 00:16:24,400 Speaker 2: does the mwon interact with the Higgs boson more than 348 00:16:24,400 --> 00:16:26,920 Speaker 2: the electron? We don't know. That's just like a number 349 00:16:26,960 --> 00:16:27,360 Speaker 2: out there. 350 00:16:27,440 --> 00:16:30,560 Speaker 1: We have to measures, Like, you didn't really answer the question, 351 00:16:30,680 --> 00:16:32,800 Speaker 1: you just changed the name of the thing. 352 00:16:33,880 --> 00:16:36,760 Speaker 2: Well, we answered the question, but it revealed another deeper question. 353 00:16:36,840 --> 00:16:38,680 Speaker 2: It's like we ran the ball down the field another 354 00:16:38,760 --> 00:16:41,440 Speaker 2: ten yards somid some progress, we know a little bit 355 00:16:41,440 --> 00:16:43,760 Speaker 2: more how to focus, But no, we definitely didn't finally 356 00:16:43,800 --> 00:16:44,600 Speaker 2: answer the question. 357 00:16:45,240 --> 00:16:48,200 Speaker 1: And so the Higgs field gives mass to other particles, right, 358 00:16:48,280 --> 00:16:52,760 Speaker 1: like quarks and electrons and its cousins. Even the neutrina 359 00:16:52,800 --> 00:16:54,600 Speaker 1: has a little bit of mass, they think, right, The. 360 00:16:54,640 --> 00:16:56,720 Speaker 2: Neutrinos definitely do have a little bit of mass. We 361 00:16:56,760 --> 00:16:58,840 Speaker 2: don't know exactly how much they have, but we know 362 00:16:58,920 --> 00:17:02,360 Speaker 2: it's very very small. We don't actually know that neutrinos 363 00:17:02,400 --> 00:17:05,000 Speaker 2: get their mass from the Higgs. That's one idea that 364 00:17:05,000 --> 00:17:07,480 Speaker 2: there are neutrinos and anti neutrinos and they do the 365 00:17:07,520 --> 00:17:09,960 Speaker 2: same thing the other particles do and get mass. It's 366 00:17:10,000 --> 00:17:13,119 Speaker 2: also possible the neutrino is even weirder. It might be 367 00:17:13,240 --> 00:17:15,600 Speaker 2: its own anti particle, and so it might get its 368 00:17:15,600 --> 00:17:18,240 Speaker 2: mass in another way. Remember, the Higgs boson is not 369 00:17:18,280 --> 00:17:20,600 Speaker 2: the only way to get mass. You can get mass 370 00:17:20,640 --> 00:17:24,280 Speaker 2: anytime you have any kind of internal stored energy. For example, 371 00:17:24,320 --> 00:17:26,879 Speaker 2: we think dark matter probably doesn't get its mass from 372 00:17:26,920 --> 00:17:30,400 Speaker 2: the Higgs field. So neutrinos might do the same things electrons, 373 00:17:30,480 --> 00:17:32,840 Speaker 2: or they might do something totally different. Mm. 374 00:17:33,000 --> 00:17:36,800 Speaker 1: Interesting. All right, Well, that's the Higgs boson and we 375 00:17:36,920 --> 00:17:39,280 Speaker 1: know that it gives other particles mass. But the question 376 00:17:39,359 --> 00:17:42,919 Speaker 1: now is who gives the Higgs boison its mass? And 377 00:17:42,960 --> 00:17:45,520 Speaker 1: more importantly, for this episode, how do we measure it? 378 00:17:45,720 --> 00:17:48,320 Speaker 1: And so let's dig into those questions. But first let's 379 00:17:48,359 --> 00:18:02,920 Speaker 1: take a quick break. All right, we're talking about the 380 00:18:02,960 --> 00:18:05,840 Speaker 1: Higgs boson. Would you say it's the world's third most 381 00:18:05,880 --> 00:18:07,040 Speaker 1: famous particle. 382 00:18:06,720 --> 00:18:09,040 Speaker 2: Third most famous? It might be the most famous. I 383 00:18:09,080 --> 00:18:10,840 Speaker 2: think it's Michael Jordan of particles. 384 00:18:10,960 --> 00:18:14,280 Speaker 1: Really, you think it's more famous than the electron quarks 385 00:18:14,400 --> 00:18:17,320 Speaker 1: maybe or photons. Photons are really probably up there. So 386 00:18:17,400 --> 00:18:19,840 Speaker 1: I would say it's like photons, electrons, and then maybe 387 00:18:19,880 --> 00:18:20,639 Speaker 1: the Higgs boson. 388 00:18:20,840 --> 00:18:22,920 Speaker 2: I guess I probably have a skewed view of it, 389 00:18:22,960 --> 00:18:26,200 Speaker 2: but I would guess Higgs boson first and then electron. 390 00:18:26,560 --> 00:18:29,360 Speaker 1: I guess it is the most popular particle among physicists 391 00:18:29,359 --> 00:18:32,639 Speaker 1: who study the Higgs boson. That makes sense. 392 00:18:33,160 --> 00:18:34,720 Speaker 2: I would say, I have a massive interest in the 393 00:18:34,760 --> 00:18:35,399 Speaker 2: Higgs boson. 394 00:18:35,480 --> 00:18:39,160 Speaker 1: Yes, you're heavily biased. All right, Well, we were talking 395 00:18:39,200 --> 00:18:41,680 Speaker 1: about how the Higgs field and the Higgs boson gives 396 00:18:41,720 --> 00:18:44,119 Speaker 1: mass to other particles. But then now the question is 397 00:18:44,240 --> 00:18:47,159 Speaker 1: what gives Higgs boson its mass and how do we 398 00:18:47,200 --> 00:18:47,600 Speaker 1: measure it? 399 00:18:47,680 --> 00:18:50,240 Speaker 2: Yeah, the Higgs boson is like the barber who shaves 400 00:18:50,320 --> 00:18:56,040 Speaker 2: himself for herself. The Higgs actually gives mass to itself. Right, 401 00:18:56,040 --> 00:18:59,360 Speaker 2: the Higgs is a really interesting particle because it interacts 402 00:18:59,440 --> 00:19:03,320 Speaker 2: with its That's not true for every particle, like the photon, 403 00:19:03,400 --> 00:19:06,960 Speaker 2: for example, only interacts with particles that have any electric 404 00:19:07,040 --> 00:19:10,760 Speaker 2: charge plus or minus a neutral particle. The photon will 405 00:19:10,800 --> 00:19:14,320 Speaker 2: just fly right by, and the photon is neutral electrically, 406 00:19:14,359 --> 00:19:17,520 Speaker 2: so it doesn't interact with itself. But the Higgs boson 407 00:19:17,760 --> 00:19:20,480 Speaker 2: does interact with itself. Two Higgs bosons coming near each 408 00:19:20,520 --> 00:19:23,800 Speaker 2: other will bounce off each other or attract each other sometimes. 409 00:19:24,040 --> 00:19:27,200 Speaker 1: WHOA Okay, So I guess that is kind of strange 410 00:19:27,200 --> 00:19:29,360 Speaker 1: and different. So the Higgs boson when it's out there 411 00:19:29,359 --> 00:19:32,200 Speaker 1: and it sees another Higgs boson, they can ignore each other. 412 00:19:32,320 --> 00:19:35,800 Speaker 2: They cannot ignore each other exactly. They're like x's that 413 00:19:35,880 --> 00:19:38,640 Speaker 2: are still angry at each other. They always end up entangled. 414 00:19:38,840 --> 00:19:42,119 Speaker 1: Are you saying the whole universe is one big, u 415 00:19:43,400 --> 00:19:44,600 Speaker 1: sad and dramatic story. 416 00:19:44,800 --> 00:19:46,520 Speaker 2: Yeah. And then they go home. They both eat chocolate 417 00:19:46,600 --> 00:19:49,240 Speaker 2: to feel better. Now, the Higgs boson flies through the universe, 418 00:19:49,280 --> 00:19:52,399 Speaker 2: and like other particles, it feels the Higgs field and 419 00:19:52,480 --> 00:19:55,840 Speaker 2: it interacts with the other Higgs bosons. The other manifestations 420 00:19:55,840 --> 00:19:58,800 Speaker 2: of the Higgs field and pigs up mass, and so 421 00:19:58,840 --> 00:20:02,360 Speaker 2: the interaction of the Higgs fiel with itself gives it mass. 422 00:20:02,600 --> 00:20:04,119 Speaker 1: Is that the order you would put it in, like 423 00:20:04,160 --> 00:20:06,520 Speaker 1: you have a Higgs boson which is like a little 424 00:20:06,560 --> 00:20:09,159 Speaker 1: blip in the field, and then that blip interacts with 425 00:20:09,200 --> 00:20:11,160 Speaker 1: the field it's made out of too. 426 00:20:11,119 --> 00:20:13,920 Speaker 2: Exactly in just the same way that an electron interacts 427 00:20:14,000 --> 00:20:16,800 Speaker 2: or the Higgs field. A Higgs boson also interacts or 428 00:20:16,800 --> 00:20:19,159 Speaker 2: the Higgs field, and it has a similar effect on 429 00:20:19,160 --> 00:20:22,159 Speaker 2: the Higgs boson as it does on the electron. What 430 00:20:22,280 --> 00:20:24,920 Speaker 2: we're measuring when we measure the Higgs boson is actually 431 00:20:24,960 --> 00:20:28,560 Speaker 2: this little cloud of a Higgs interacting with other higgses. 432 00:20:29,160 --> 00:20:31,960 Speaker 1: So then that means if the Higgs boson has inertial mass, 433 00:20:31,960 --> 00:20:36,199 Speaker 1: that means the Higgs boson is not dumb, doesn't go 434 00:20:36,240 --> 00:20:36,960 Speaker 1: at the speed of light. 435 00:20:37,119 --> 00:20:39,159 Speaker 2: The Higgs boson does not travel at the speed of 436 00:20:39,200 --> 00:20:42,159 Speaker 2: light exactly because nothing that has mass can go at 437 00:20:42,160 --> 00:20:44,000 Speaker 2: the speed of light. And the Higgs boson mass is 438 00:20:44,040 --> 00:20:46,879 Speaker 2: sort of interesting from like a philosophical perspective, like whoa 439 00:20:46,960 --> 00:20:49,240 Speaker 2: the thing that has mass gives mass itself. It's like 440 00:20:49,560 --> 00:20:52,480 Speaker 2: Santa Claus giving himself a present or something. But it's 441 00:20:52,520 --> 00:20:56,240 Speaker 2: also really fascinating theoretically for other reasons, because the Higgs 442 00:20:56,280 --> 00:20:59,320 Speaker 2: boson doesn't just get mass from its interactions with itself. 443 00:20:59,560 --> 00:21:02,719 Speaker 2: It also who gets mass from interactions with other particles. 444 00:21:02,760 --> 00:21:05,560 Speaker 2: Like we know that the Higgs interacts with electrons, and 445 00:21:05,600 --> 00:21:08,120 Speaker 2: we know that interacts with top quarks, and so those 446 00:21:08,119 --> 00:21:11,080 Speaker 2: interactions give mass to electrons and top quarks, but also 447 00:21:11,240 --> 00:21:14,040 Speaker 2: to the Higgs. So the Higgs gets its mass from 448 00:21:14,040 --> 00:21:17,240 Speaker 2: interacting with itself and from interacting with the other particles. 449 00:21:17,400 --> 00:21:20,159 Speaker 1: Wait, so the mass of the Higgs changes depending on 450 00:21:20,200 --> 00:21:23,000 Speaker 1: who's around it. Like, what if there's no electron or 451 00:21:23,040 --> 00:21:25,840 Speaker 1: meal on around it, would that mean the Eiggs boson 452 00:21:25,960 --> 00:21:26,399 Speaker 1: is lighter? 453 00:21:26,640 --> 00:21:29,320 Speaker 2: Question because I said fields, and those fields are everywhere, 454 00:21:29,400 --> 00:21:31,520 Speaker 2: or there's always an electron field and there's always a 455 00:21:31,560 --> 00:21:34,800 Speaker 2: top quark field. So the Higgs boson interacts with those fields, 456 00:21:34,920 --> 00:21:38,840 Speaker 2: whether or not they're actually electrons or top quarks around, 457 00:21:38,960 --> 00:21:41,720 Speaker 2: whether those fields are excited enough to make real particles, 458 00:21:41,720 --> 00:21:43,520 Speaker 2: it interacts with the fields themselves. 459 00:21:45,080 --> 00:21:46,879 Speaker 1: Well, I guess, just for the record, I think it's 460 00:21:46,920 --> 00:21:50,120 Speaker 1: okay Santa Claus wants to buy himself a gift. I mean, 461 00:21:50,840 --> 00:21:54,159 Speaker 1: the poor guy, I mean allwis only gets one birthday 462 00:21:54,200 --> 00:21:57,600 Speaker 1: present a year from missus Sanna. He can buy himself 463 00:21:57,800 --> 00:21:59,480 Speaker 1: a little some fum. 464 00:22:00,280 --> 00:22:02,560 Speaker 2: Yeah, go ahead, Santa Claus, get yourself some dark chocolate. 465 00:22:03,440 --> 00:22:06,880 Speaker 1: That's right, you do you? Although maybe he likes white chocolate. 466 00:22:07,000 --> 00:22:09,600 Speaker 2: Yeah, maybe he likes peppermint bark. Who knows. Somebody's got 467 00:22:09,720 --> 00:22:11,119 Speaker 2: to like that stuff they keep making it. 468 00:22:11,440 --> 00:22:12,840 Speaker 1: Maybe it's the Santa himself. 469 00:22:14,119 --> 00:22:16,720 Speaker 2: But there's something of a mystery about the Higgs boson mass, 470 00:22:16,760 --> 00:22:19,000 Speaker 2: which is why we're so interested in measuring it, and 471 00:22:19,040 --> 00:22:21,800 Speaker 2: that comes from its interactions with these other particles. It's 472 00:22:21,840 --> 00:22:25,400 Speaker 2: interactions with matter particles like electrons and top quarks that 473 00:22:25,480 --> 00:22:28,160 Speaker 2: makes its mass much much bigger, and when it interacts 474 00:22:28,160 --> 00:22:31,680 Speaker 2: with other bosons like w bosons or gluons or whatever, 475 00:22:31,960 --> 00:22:35,720 Speaker 2: that makes its mass smaller. And the fascinating thing is 476 00:22:35,720 --> 00:22:38,159 Speaker 2: that these two numbers are really really big. They're like 477 00:22:38,240 --> 00:22:41,000 Speaker 2: billions of times bigger than the eventual mass of the 478 00:22:41,080 --> 00:22:44,200 Speaker 2: Higgs boson, which means these two numbers sort of cancel 479 00:22:44,280 --> 00:22:47,400 Speaker 2: each other out almost exactly. It's kind of a mystery 480 00:22:47,440 --> 00:22:48,480 Speaker 2: of modern physics. 481 00:22:48,880 --> 00:22:52,520 Speaker 1: Mm weird. So the Higgs field is that the only 482 00:22:52,560 --> 00:22:54,760 Speaker 1: field that interacts with all the other fields, or do 483 00:22:54,840 --> 00:22:57,480 Speaker 1: all fields interact with each other, or is that unique 484 00:22:57,520 --> 00:22:59,639 Speaker 1: to the Higgs field. It seems like maybe the Higgs 485 00:22:59,640 --> 00:23:01,560 Speaker 1: field is. It's just an everyone's business. 486 00:23:03,240 --> 00:23:06,200 Speaker 2: Every particle we discovered so far feels the weak force, 487 00:23:06,640 --> 00:23:08,760 Speaker 2: So the Higgs feels the weak force, just like the 488 00:23:08,840 --> 00:23:11,520 Speaker 2: neutrinos do, and the W and the C and the quarks. 489 00:23:11,560 --> 00:23:14,359 Speaker 2: Everybody feels the weak force. But the Higgs is neutral, 490 00:23:14,400 --> 00:23:17,600 Speaker 2: so it doesn't interact with photons directly, for example. But 491 00:23:17,640 --> 00:23:19,800 Speaker 2: it's fascinating to me that you do this accounting, Like 492 00:23:19,800 --> 00:23:21,680 Speaker 2: the Higgs boson gets a little bit of mass from 493 00:23:21,720 --> 00:23:24,560 Speaker 2: interacting with itself, we don't know exactly how much. Then 494 00:23:24,560 --> 00:23:27,000 Speaker 2: it gets a huge amount of mass from interacting with 495 00:23:27,040 --> 00:23:29,600 Speaker 2: electrons and nuance and stuff. And then it loses a 496 00:23:29,640 --> 00:23:33,120 Speaker 2: huge amount of mass from interacting with w's and z's, etc. 497 00:23:33,520 --> 00:23:36,400 Speaker 2: And that comes back to almost zero. Like these two 498 00:23:36,480 --> 00:23:39,880 Speaker 2: big numbers, the huge addition and the huge subtraction, don't 499 00:23:39,920 --> 00:23:42,720 Speaker 2: have to be close to each other. They're two enormous numbers, 500 00:23:42,920 --> 00:23:46,280 Speaker 2: and yet they almost balance. Brings the Higgs boson mass 501 00:23:46,359 --> 00:23:49,200 Speaker 2: back down to a reasonable value. In another universe, the 502 00:23:49,280 --> 00:23:52,480 Speaker 2: Higgs boson could have been like a million times heavier 503 00:23:52,520 --> 00:23:54,840 Speaker 2: than it ended up being so heavy we could never 504 00:23:54,920 --> 00:23:55,639 Speaker 2: even discover it. 505 00:23:55,840 --> 00:23:59,280 Speaker 1: Oh, I guess that's a weird concept for a non 506 00:23:59,280 --> 00:24:03,280 Speaker 1: particle to understand, which is like, how do you lose 507 00:24:03,320 --> 00:24:04,600 Speaker 1: mass in an interaction? 508 00:24:04,960 --> 00:24:05,040 Speaker 2: Like? 509 00:24:05,080 --> 00:24:07,800 Speaker 1: What does it mean that, like the Higgs boson loses 510 00:24:07,840 --> 00:24:10,800 Speaker 1: mass when it interacts with certain particles, like it gets 511 00:24:10,880 --> 00:24:13,480 Speaker 1: lighter and moves faster, it's easier to move around. What 512 00:24:13,520 --> 00:24:14,000 Speaker 1: does that mean? 513 00:24:14,080 --> 00:24:15,879 Speaker 2: I think intuitively, the way to think about it is 514 00:24:15,880 --> 00:24:19,159 Speaker 2: that interacting with some of these fields adds to the 515 00:24:19,200 --> 00:24:23,240 Speaker 2: internal stored energy of the effective Higgs boson, and interacting 516 00:24:23,280 --> 00:24:26,840 Speaker 2: with other fields decreases the internal stored energy. Adding to 517 00:24:26,880 --> 00:24:30,520 Speaker 2: the internal stored energy means getting more mass. Losing internal 518 00:24:30,560 --> 00:24:33,639 Speaker 2: stored energy means decreasing your mass. So it's not like 519 00:24:33,760 --> 00:24:36,280 Speaker 2: it gets a kick. It actually like sucks away some 520 00:24:36,320 --> 00:24:39,280 Speaker 2: of the internal stored energy the interaction with some of 521 00:24:39,280 --> 00:24:39,960 Speaker 2: these fields. 522 00:24:41,119 --> 00:24:44,520 Speaker 1: But then that's a whole different mechanism for getting mass, right, 523 00:24:44,600 --> 00:24:48,000 Speaker 1: which is like having stored energy inside that doesn't come 524 00:24:48,000 --> 00:24:49,159 Speaker 1: from the Higgs field, does it? 525 00:24:49,320 --> 00:24:51,560 Speaker 2: In this case, it comes from the interaction between the 526 00:24:51,600 --> 00:24:54,720 Speaker 2: Higgs field and these other particles. So even the Higgs 527 00:24:54,760 --> 00:24:58,199 Speaker 2: field interaction you can think about as internal stored energy. 528 00:24:58,400 --> 00:25:00,479 Speaker 2: Like you think about the electron moving through the universe, 529 00:25:00,520 --> 00:25:02,760 Speaker 2: what is its mass? You could just say it comes 530 00:25:02,760 --> 00:25:05,240 Speaker 2: from the Higgs field, but really what's happening is you're 531 00:25:05,240 --> 00:25:08,000 Speaker 2: creating a new object, which is this electron that interacts 532 00:25:08,000 --> 00:25:10,600 Speaker 2: with the Higgs field, and that thing has energy which 533 00:25:10,760 --> 00:25:13,080 Speaker 2: in the end is coming from the Higgs field, and 534 00:25:13,119 --> 00:25:15,639 Speaker 2: it's storing that energy internally in this new thing. This 535 00:25:15,800 --> 00:25:18,840 Speaker 2: like cloud of electrons and Higgs is sort of interacting together. 536 00:25:19,240 --> 00:25:21,760 Speaker 2: So it's really all the same kind of mechanism. The 537 00:25:21,840 --> 00:25:24,119 Speaker 2: Higgs is like an example of how you can have 538 00:25:24,240 --> 00:25:27,080 Speaker 2: internal stored energy, but you're right, it's not the only one. 539 00:25:27,200 --> 00:25:29,960 Speaker 2: Like other forces can give you internal stored energy, like 540 00:25:30,000 --> 00:25:32,840 Speaker 2: the gluons inside the proton give you internal. 541 00:25:32,440 --> 00:25:34,800 Speaker 1: Stored energy, and then when those get a lot of 542 00:25:34,840 --> 00:25:38,720 Speaker 1: internal stored energy like in the proton, it feels heavier. 543 00:25:39,000 --> 00:25:40,680 Speaker 1: Is that also due to the Higgs field or is 544 00:25:40,720 --> 00:25:43,760 Speaker 1: that just due to some other unknown mechanism in the universe. 545 00:25:43,800 --> 00:25:46,120 Speaker 2: That's just the fundamental nature of mass that we don't 546 00:25:46,119 --> 00:25:49,560 Speaker 2: really understand. That internal stored energy has inertia, and you know, 547 00:25:49,640 --> 00:25:53,199 Speaker 2: you can change the relationship between those gluons, increasing or 548 00:25:53,240 --> 00:25:56,240 Speaker 2: decreasing mass. Right, so if those gluons interact with something 549 00:25:56,280 --> 00:25:59,240 Speaker 2: else outside and change their relative energy levels, that can 550 00:25:59,359 --> 00:26:01,080 Speaker 2: change the mass of the particle. 551 00:26:01,119 --> 00:26:03,560 Speaker 1: Well, I guess the other question I had was, you know, 552 00:26:03,600 --> 00:26:05,960 Speaker 1: you said that the Higgs boson doesn't move at the 553 00:26:05,960 --> 00:26:07,879 Speaker 1: speed of light, but at the same time it's a 554 00:26:07,880 --> 00:26:10,679 Speaker 1: particle that gives other particles mass. Does that mean that 555 00:26:10,800 --> 00:26:13,960 Speaker 1: mass is not instantaneous or that there's some kind of 556 00:26:14,040 --> 00:26:17,240 Speaker 1: delay in how the universe or how you feel mass 557 00:26:17,280 --> 00:26:18,520 Speaker 1: in some particles. 558 00:26:18,320 --> 00:26:21,720 Speaker 2: Like if you change the mass of a particle, would 559 00:26:21,720 --> 00:26:24,160 Speaker 2: that ripple out at less than the speed of light? 560 00:26:24,520 --> 00:26:28,280 Speaker 1: Or like if an electron moves, you know, the inertia 561 00:26:28,320 --> 00:26:31,280 Speaker 1: you would feel is somehow delayed because it has to 562 00:26:31,280 --> 00:26:32,879 Speaker 1: get it from the Higgs field, which doesn't move at 563 00:26:32,920 --> 00:26:33,520 Speaker 1: the speed of light. 564 00:26:33,640 --> 00:26:36,520 Speaker 2: Information about any motion is always delayed, even if it 565 00:26:36,560 --> 00:26:39,879 Speaker 2: travels at the speed of light. Right, Even like gravitational waves, 566 00:26:39,880 --> 00:26:42,359 Speaker 2: which travel at the speed of light are not instantaneous. 567 00:26:42,880 --> 00:26:44,520 Speaker 2: So whether or not you travel at the speed of 568 00:26:44,560 --> 00:26:47,960 Speaker 2: light or not, you're still not propagating information instantaneously. 569 00:26:48,080 --> 00:26:50,919 Speaker 1: M so I guess I mean more of a delay, 570 00:26:51,920 --> 00:26:54,359 Speaker 1: like you could see something happen before you feel its mass. 571 00:26:54,520 --> 00:26:56,040 Speaker 2: I think we had to pull apart a little bit 572 00:26:56,040 --> 00:27:00,320 Speaker 2: here the gravitational and the inertial situation, because this see 573 00:27:00,320 --> 00:27:04,359 Speaker 2: something's mass really means to observe it moving. Right. Mass 574 00:27:04,400 --> 00:27:07,000 Speaker 2: is all about like what is your inertia? How do 575 00:27:07,000 --> 00:27:09,760 Speaker 2: you move through the universe? How do you respond to forces? 576 00:27:09,960 --> 00:27:13,000 Speaker 2: And we're not talking about like how your existence changes, 577 00:27:13,080 --> 00:27:16,719 Speaker 2: like the curvature of space time and ripples from your acceleration. Right, 578 00:27:16,720 --> 00:27:18,960 Speaker 2: we're not talking about gravitational waves. We're just talking about 579 00:27:19,000 --> 00:27:19,720 Speaker 2: inertial mass. 580 00:27:20,280 --> 00:27:22,239 Speaker 1: Well, I guess that the question is the same. You know, 581 00:27:22,280 --> 00:27:24,720 Speaker 1: do you feel inertial mass at a later time that 582 00:27:24,760 --> 00:27:27,440 Speaker 1: you would like if a photon bounced off of an electron. 583 00:27:27,520 --> 00:27:29,359 Speaker 2: It's a great question. I haven't thought about it before, 584 00:27:29,600 --> 00:27:31,919 Speaker 2: but I think that probably what's going on is that 585 00:27:32,000 --> 00:27:35,119 Speaker 2: this is all internal to the object we call the electron, 586 00:27:35,600 --> 00:27:37,359 Speaker 2: and we don't have enough energy to like break the 587 00:27:37,400 --> 00:27:40,720 Speaker 2: electron open and see the Higgs is inside propagating. We 588 00:27:40,880 --> 00:27:43,119 Speaker 2: just like wrap that whole thing up into an object 589 00:27:43,200 --> 00:27:45,399 Speaker 2: we call the electron. And what we're talking about here 590 00:27:45,400 --> 00:27:48,280 Speaker 2: is something that's really going on inside the electron. You'd 591 00:27:48,280 --> 00:27:49,960 Speaker 2: be worried about, like how long it takes a Higgs 592 00:27:49,960 --> 00:27:52,119 Speaker 2: boson to move from one side of the electron to 593 00:27:52,200 --> 00:27:54,280 Speaker 2: the other. But from our point of view on the outside, 594 00:27:54,280 --> 00:27:57,240 Speaker 2: the electron is effectively a point particle, so it's not 595 00:27:57,320 --> 00:27:59,840 Speaker 2: really an issue like whether the Higgs can get from 596 00:27:59,840 --> 00:28:02,080 Speaker 2: one inside of the electron to the other to make 597 00:28:02,080 --> 00:28:04,920 Speaker 2: it like a consistent object with a single kind of mass. 598 00:28:05,400 --> 00:28:09,040 Speaker 1: It just seems like it's like a force that has 599 00:28:09,080 --> 00:28:11,480 Speaker 1: a certain delay to it, you know, like a slower 600 00:28:11,520 --> 00:28:15,200 Speaker 1: force than say the electro magnetic force, which communicates with photons, 601 00:28:15,240 --> 00:28:17,040 Speaker 1: which are going at the speed of light. 602 00:28:17,160 --> 00:28:19,400 Speaker 2: Yeah, that's right. Photons do travel at speed of light, 603 00:28:19,440 --> 00:28:22,920 Speaker 2: and ripples in the Higgs field travels slower. There are 604 00:28:23,040 --> 00:28:27,159 Speaker 2: some particles whose mass changes. Remember, neutrinos don't have a 605 00:28:27,240 --> 00:28:30,600 Speaker 2: definite mass when they are created. They are a mixture 606 00:28:30,720 --> 00:28:34,560 Speaker 2: of various mass states, so that kind of inertial mass 607 00:28:34,600 --> 00:28:37,000 Speaker 2: information might propagate it less than the speed of light. 608 00:28:37,280 --> 00:28:39,080 Speaker 1: All right, Well, let's get to the main question of 609 00:28:39,080 --> 00:28:41,800 Speaker 1: the episode, which is how do you measure the mass 610 00:28:41,840 --> 00:28:44,080 Speaker 1: of the Higgs boson. That was kind of a part 611 00:28:44,080 --> 00:28:46,680 Speaker 1: of what the big discovery was in twenty twelve, right, 612 00:28:46,840 --> 00:28:48,720 Speaker 1: Like you kind of had to guess what its mass 613 00:28:48,840 --> 00:28:49,960 Speaker 1: was to know where to look for it. 614 00:28:50,040 --> 00:28:52,800 Speaker 2: Yeah, it's a really interesting bit of scientific history because 615 00:28:53,080 --> 00:28:56,320 Speaker 2: when Higgs came up with this idea, his theory work 616 00:28:56,480 --> 00:28:58,680 Speaker 2: no matter what the mass to the Higgs was, Like 617 00:28:58,720 --> 00:29:02,000 Speaker 2: the Higgs could be very very or super duper honk 618 00:29:02,040 --> 00:29:05,600 Speaker 2: and heavy and his theory would still work. And that's cool. 619 00:29:05,640 --> 00:29:08,120 Speaker 2: It makes a very powerful theory, but it's also sort 620 00:29:08,120 --> 00:29:10,440 Speaker 2: of frustrating from an experimental point of view because he 621 00:29:10,480 --> 00:29:13,800 Speaker 2: didn't predict the Higgs mass. If his theory only worked 622 00:29:13,840 --> 00:29:15,800 Speaker 2: for one value of the Higgs mass, then he could 623 00:29:15,800 --> 00:29:17,920 Speaker 2: have said, go out there, look for it. It has 624 00:29:18,000 --> 00:29:20,440 Speaker 2: this value, I predict it, you know, like baby Ruth 625 00:29:20,520 --> 00:29:22,920 Speaker 2: calling his shot. But instead he said, well it might 626 00:29:22,960 --> 00:29:25,360 Speaker 2: exist and it might have any value. So you got 627 00:29:25,360 --> 00:29:27,480 Speaker 2: to look for in all sorts of different ways. 628 00:29:27,440 --> 00:29:29,920 Speaker 1: Meaning like the mass would work no matter what the 629 00:29:30,280 --> 00:29:32,760 Speaker 1: mass of the Higgs boson is, or would you have 630 00:29:32,880 --> 00:29:36,600 Speaker 1: like very different universes if it did have different masses, if. 631 00:29:36,520 --> 00:29:37,960 Speaker 2: You know all the particles that are out there in 632 00:29:38,000 --> 00:29:41,000 Speaker 2: the universe interacting with the Higgs boson, then you know 633 00:29:41,040 --> 00:29:44,080 Speaker 2: what its mass is because its mass comes from interacting 634 00:29:44,080 --> 00:29:47,200 Speaker 2: with itself and interacting with all those other particles. If 635 00:29:47,200 --> 00:29:49,400 Speaker 2: you don't know the other particles out there in the universe, 636 00:29:49,440 --> 00:29:51,880 Speaker 2: you don't know everything that's contributing to the Higgs mass. 637 00:29:52,400 --> 00:29:54,000 Speaker 2: And so we didn't know. We didn't know what all 638 00:29:54,000 --> 00:29:55,760 Speaker 2: the particles were. We still don't know what all the 639 00:29:55,760 --> 00:29:58,480 Speaker 2: particles are. If you measure all the other particles very 640 00:29:58,560 --> 00:30:01,320 Speaker 2: very precisely, then you can predict what the Higgs mass 641 00:30:01,320 --> 00:30:03,480 Speaker 2: could be. But that's only if you know all the 642 00:30:03,520 --> 00:30:06,200 Speaker 2: particles in the universe, and we're pretty sure we don't. 643 00:30:06,360 --> 00:30:08,840 Speaker 1: So I guess he just didn't know what the mass 644 00:30:08,840 --> 00:30:11,040 Speaker 1: of the Higgs boson was supposed to be, just because 645 00:30:11,120 --> 00:30:13,280 Speaker 1: you didn't have all the information about what else is 646 00:30:13,280 --> 00:30:14,680 Speaker 1: out there in the universe exactly. 647 00:30:14,720 --> 00:30:17,200 Speaker 2: And that's another reason why knowing the mass is exciting, 648 00:30:17,560 --> 00:30:19,200 Speaker 2: because it gives you a way to tell, like, is 649 00:30:19,240 --> 00:30:21,240 Speaker 2: there something out there we don't know about, something else 650 00:30:21,520 --> 00:30:23,760 Speaker 2: interacting with the Higgs field and making it heavier or 651 00:30:23,840 --> 00:30:25,800 Speaker 2: making it lighter. What we can do is predict the 652 00:30:25,880 --> 00:30:27,640 Speaker 2: value the Higgs field based on all the particles that 653 00:30:27,680 --> 00:30:29,600 Speaker 2: we do think are out there. Then we can go 654 00:30:29,640 --> 00:30:31,480 Speaker 2: out there and measure the Higgs and say does it 655 00:30:31,560 --> 00:30:32,760 Speaker 2: agree with our prediction? 656 00:30:33,080 --> 00:30:35,480 Speaker 1: All right, So then we discovered the Higgs boson, and 657 00:30:35,560 --> 00:30:37,720 Speaker 1: so what is its mass? And how do we know 658 00:30:37,760 --> 00:30:38,600 Speaker 1: what its mass was? 659 00:30:38,840 --> 00:30:41,040 Speaker 2: So we measure the mass of particles in a weird unit. 660 00:30:41,040 --> 00:30:46,440 Speaker 2: It's called the GeV giggle electron volts one billion electron bolts. 661 00:30:46,720 --> 00:30:49,600 Speaker 2: It's actually a pretty convenient unit because the proton weighs 662 00:30:49,600 --> 00:30:52,640 Speaker 2: about one GeV. Our electrons are much much lighter than that. 663 00:30:52,680 --> 00:30:55,480 Speaker 2: For example, they're like half of an MeV half of 664 00:30:55,480 --> 00:30:59,120 Speaker 2: a million electron bolts, and the Higgs boson is about 665 00:30:59,120 --> 00:31:01,760 Speaker 2: one hundred and twenty five of these things. It's one 666 00:31:01,840 --> 00:31:05,000 Speaker 2: hundred and twenty five point three five plus or minus 667 00:31:05,200 --> 00:31:07,240 Speaker 2: point one five GeV. 668 00:31:07,760 --> 00:31:10,040 Speaker 1: Wait, the mass of the Higgs boson is one hundred 669 00:31:10,040 --> 00:31:13,080 Speaker 1: and twenty five times greater than the mass of a proton. 670 00:31:13,400 --> 00:31:16,760 Speaker 2: Yeah, exactly, it's the second heaviest particle we know. It's 671 00:31:16,840 --> 00:31:19,040 Speaker 2: lighter only than the top quark, which is about one 672 00:31:19,120 --> 00:31:21,160 Speaker 2: hundred and seventy three GeV. 673 00:31:21,520 --> 00:31:23,239 Speaker 1: Well, it's kind of weird to think about, right, Like 674 00:31:23,320 --> 00:31:26,600 Speaker 1: the electron is thousands of times slighter and yet when 675 00:31:26,600 --> 00:31:30,560 Speaker 1: it interacts with the Higgs boson, the Higgs boson is heavier. 676 00:31:30,840 --> 00:31:33,959 Speaker 2: Yeah, exactly. The top quark interacts with the higgs boson 677 00:31:34,160 --> 00:31:37,000 Speaker 2: like crazy. Those two guys have a party every time 678 00:31:37,080 --> 00:31:39,200 Speaker 2: they meet. And that's why the top quark is super 679 00:31:39,280 --> 00:31:39,920 Speaker 2: duper heavy. 680 00:31:40,160 --> 00:31:43,800 Speaker 1: That's why it's the top because it's it's a fun particle. 681 00:31:44,720 --> 00:31:48,760 Speaker 1: It's thet I don't know it likes to party. 682 00:31:50,200 --> 00:31:53,000 Speaker 2: But we know the higgs Boson mass very very precisely. 683 00:31:53,040 --> 00:31:55,360 Speaker 2: We know it more precisely than the top quark. Even 684 00:31:55,400 --> 00:31:57,720 Speaker 2: the top quark we discovered in the nineties and we've 685 00:31:57,720 --> 00:32:00,040 Speaker 2: been working to measure it's mass ever since. Then. With 686 00:32:00,040 --> 00:32:02,800 Speaker 2: the Higgs boson, we know a precision of one part 687 00:32:02,880 --> 00:32:03,240 Speaker 2: in one. 688 00:32:03,160 --> 00:32:05,600 Speaker 1: Thousand, all right, So then how do we know the mass? 689 00:32:05,640 --> 00:32:07,360 Speaker 1: How do you measure the mass of any particle? You 690 00:32:07,360 --> 00:32:09,320 Speaker 1: can't just put it on a scale, right, and you 691 00:32:09,360 --> 00:32:11,400 Speaker 1: can't just like drop it from a building to see 692 00:32:11,480 --> 00:32:14,480 Speaker 1: how fast it accelerates, exactly. 693 00:32:14,520 --> 00:32:16,160 Speaker 2: We can't do any of those kinds of things that 694 00:32:16,200 --> 00:32:19,400 Speaker 2: you usually do because these particles last for only a 695 00:32:19,440 --> 00:32:21,520 Speaker 2: few moments. You know, we're talking like ten to the 696 00:32:21,560 --> 00:32:24,720 Speaker 2: negative twenty three seconds, which means it. Technically, we don't 697 00:32:24,720 --> 00:32:28,560 Speaker 2: even see these particles. Nobody's ever seen a Higgs boson. 698 00:32:28,840 --> 00:32:31,320 Speaker 2: They never even seen a track of a Higgs boson 699 00:32:31,440 --> 00:32:33,960 Speaker 2: left in one of our detectors, because they just don't 700 00:32:34,000 --> 00:32:36,760 Speaker 2: last for long enough already, and then it decays into 701 00:32:36,760 --> 00:32:39,320 Speaker 2: other stuff. We know the Higgs exists because of patterns 702 00:32:39,360 --> 00:32:42,360 Speaker 2: in those particle decays that are consistent with the Higgs 703 00:32:42,440 --> 00:32:45,160 Speaker 2: being there and inconsistent with the Higgs not being there. 704 00:32:45,600 --> 00:32:47,520 Speaker 2: So then to measure its mass, we have to look 705 00:32:47,560 --> 00:32:49,920 Speaker 2: at the patterns of those particles and try to extract 706 00:32:50,000 --> 00:32:53,360 Speaker 2: that information the streak that those particles left after the 707 00:32:53,440 --> 00:32:56,240 Speaker 2: Higgs boson turned into them. Mmm. Yeah. 708 00:32:56,280 --> 00:32:59,920 Speaker 1: We often use the analogy of like studying an accidency. 709 00:33:00,240 --> 00:33:02,680 Speaker 1: After the accident, you sort of study the debris and 710 00:33:02,760 --> 00:33:05,960 Speaker 1: you kind of figure out, like, oh, this car crash 711 00:33:06,000 --> 00:33:07,600 Speaker 1: into that car is here at this point, and they 712 00:33:07,680 --> 00:33:10,840 Speaker 1: crash in the corner back corner, and because the fenders 713 00:33:11,480 --> 00:33:13,400 Speaker 1: over here, we know how fast they were going. You're 714 00:33:13,400 --> 00:33:17,000 Speaker 1: saying like, somewhere between the crash and finding the debris, 715 00:33:17,200 --> 00:33:20,040 Speaker 1: like a Higgs boson popped up into the universe and 716 00:33:20,080 --> 00:33:21,200 Speaker 1: then it disappeared again. 717 00:33:21,360 --> 00:33:23,400 Speaker 2: Yeah, and the car crash analogy is helpful, but it's 718 00:33:23,400 --> 00:33:26,360 Speaker 2: also misleading an important way, because when you're looking at 719 00:33:26,400 --> 00:33:29,440 Speaker 2: a car crash, you're looking at pieces of the car, right, 720 00:33:29,480 --> 00:33:31,920 Speaker 2: the fender is here and the windshield wipers over there. 721 00:33:32,080 --> 00:33:34,200 Speaker 2: When you're looking at the results of a particle collision, 722 00:33:34,240 --> 00:33:36,440 Speaker 2: you're not looking at like pieces of the Higgs boson. 723 00:33:36,640 --> 00:33:39,360 Speaker 2: The Higgs boson doesn't like break in half and you 724 00:33:39,400 --> 00:33:41,280 Speaker 2: find bits of it here and bits of it there. 725 00:33:41,480 --> 00:33:44,800 Speaker 2: It converts from a Higgs boson into totally different kinds 726 00:33:44,800 --> 00:33:47,440 Speaker 2: of matter. So, for example, a Higgs boson can decay 727 00:33:47,760 --> 00:33:50,479 Speaker 2: into two bottom quarks, and that doesn't mean that there 728 00:33:50,480 --> 00:33:53,160 Speaker 2: are two bottom quarks inside a Higgs boson. It means 729 00:33:53,160 --> 00:33:55,040 Speaker 2: that the energy that used to be in the Higgs 730 00:33:55,040 --> 00:33:57,640 Speaker 2: field is now in the bottom quark field. The Higgs 731 00:33:57,720 --> 00:33:59,840 Speaker 2: is gone. It's not like it's bits are rearranged into 732 00:33:59,840 --> 00:34:02,400 Speaker 2: something else. It's gone and that energy is now in 733 00:34:02,480 --> 00:34:03,400 Speaker 2: a different field. 734 00:34:03,760 --> 00:34:05,960 Speaker 1: Right. Yeah, things trend into energy, but sort of the 735 00:34:06,000 --> 00:34:08,120 Speaker 1: analogy is still the same, right, Like all the parts 736 00:34:08,120 --> 00:34:10,360 Speaker 1: still have to fit together at the end, Like you 737 00:34:10,400 --> 00:34:13,279 Speaker 1: can't just invent energy out of nowhere, like you have 738 00:34:13,320 --> 00:34:15,880 Speaker 1: to do some accounting to make sure that all the 739 00:34:15,880 --> 00:34:18,080 Speaker 1: bits that you got at the end were part of 740 00:34:18,080 --> 00:34:21,200 Speaker 1: the same thing at the beginning, and that is actually 741 00:34:21,280 --> 00:34:23,200 Speaker 1: how you find the mass, right like you do the 742 00:34:23,320 --> 00:34:24,480 Speaker 1: through accounting. 743 00:34:24,160 --> 00:34:28,200 Speaker 2: Exactly through accounting basically a quantum information and energy. Quantum 744 00:34:28,239 --> 00:34:30,960 Speaker 2: information is sort of amazing. We talked about the podcast 745 00:34:30,960 --> 00:34:33,040 Speaker 2: a few times, and the idea is that quantum information 746 00:34:33,320 --> 00:34:36,600 Speaker 2: is not destroyed in the universe, which means that every 747 00:34:36,760 --> 00:34:40,319 Speaker 2: past moment in the universe creates a unique present because 748 00:34:40,360 --> 00:34:42,120 Speaker 2: as a unique connection, as where there was a one 749 00:34:42,200 --> 00:34:44,200 Speaker 2: to one mapping, you can reverse it. You can say, 750 00:34:44,400 --> 00:34:46,680 Speaker 2: I'm going to take the present, I'm going to rewind 751 00:34:46,680 --> 00:34:48,400 Speaker 2: it figure out what was going on in the past. 752 00:34:48,960 --> 00:34:50,920 Speaker 2: And so you can take the particles that the Higgs 753 00:34:50,960 --> 00:34:53,880 Speaker 2: boson decayed into, maybe like two bottom quarks that we 754 00:34:53,920 --> 00:34:55,800 Speaker 2: see in our detector. You can figure out what the 755 00:34:55,880 --> 00:34:58,839 Speaker 2: Higgs boson was doing. Most specifically, you can figure out 756 00:34:58,880 --> 00:35:02,319 Speaker 2: its momentum and you can figure out its energy, and 757 00:35:02,400 --> 00:35:05,600 Speaker 2: from those two pieces of information you can measure its mass. 758 00:35:05,840 --> 00:35:08,080 Speaker 1: I guess, so that means you sort of infer its mass, 759 00:35:08,120 --> 00:35:10,879 Speaker 1: right or you deduce its mass from what it's doing 760 00:35:11,280 --> 00:35:13,120 Speaker 1: or what do you see its progeny doing. 761 00:35:13,239 --> 00:35:15,200 Speaker 2: Yeah, and that makes it sound a little bit indirect, 762 00:35:15,560 --> 00:35:18,080 Speaker 2: and the end all measurements are indirect, are all inferences 763 00:35:18,120 --> 00:35:20,960 Speaker 2: based on observation. That's when we feel pretty confident in 764 00:35:21,040 --> 00:35:24,000 Speaker 2: But yeah, we're measuring the energy of the two particles. 765 00:35:24,160 --> 00:35:26,120 Speaker 2: And you know, one of the listeners actually came very 766 00:35:26,120 --> 00:35:29,320 Speaker 2: close to answering it. He said, the Higgs was discovered 767 00:35:29,320 --> 00:35:31,719 Speaker 2: when they saw a pair of photons, and maybe the 768 00:35:31,760 --> 00:35:34,480 Speaker 2: mass is equivalent to the energy of those photons. And 769 00:35:34,480 --> 00:35:38,080 Speaker 2: that's almost exactly right. The energy of those photons tells 770 00:35:38,080 --> 00:35:41,000 Speaker 2: you a lot, and also their direction and their momentum 771 00:35:41,080 --> 00:35:43,360 Speaker 2: tells you the momentum of the Higgs, and with that 772 00:35:43,480 --> 00:35:46,200 Speaker 2: information together you can get the mass. Because remember of 773 00:35:46,320 --> 00:35:48,600 Speaker 2: energy we're talking about like energy of motion, which is 774 00:35:48,600 --> 00:35:50,680 Speaker 2: the momentum, and then energy of mass. And so if 775 00:35:50,719 --> 00:35:53,319 Speaker 2: you have the total energy and you know the momentum, 776 00:35:53,440 --> 00:35:55,640 Speaker 2: the last little bit has to be the mass. 777 00:35:56,880 --> 00:35:58,800 Speaker 1: Sounds like that listener was very enlightened. 778 00:36:00,200 --> 00:36:01,560 Speaker 2: Brilliant, brilliant comment. 779 00:36:01,960 --> 00:36:04,680 Speaker 1: And so let's shed more light into this measurement of 780 00:36:04,680 --> 00:36:08,000 Speaker 1: the Higgs bosons mass. What's hard about that and what 781 00:36:08,120 --> 00:36:10,680 Speaker 1: does it mean about our picture of the universe? So 782 00:36:10,760 --> 00:36:13,000 Speaker 1: let's stick in to that. But first let's take another 783 00:36:13,080 --> 00:36:28,080 Speaker 1: quick break. All right, we're talking about the Higgs bosons. 784 00:36:28,440 --> 00:36:30,600 Speaker 1: Higgs boson researchers favorite particle. 785 00:36:31,000 --> 00:36:33,360 Speaker 2: Yeah, that's right, or maybe the most famous particle and 786 00:36:33,400 --> 00:36:36,279 Speaker 2: maybe our favorite particle because it's the last one we discovered. 787 00:36:36,520 --> 00:36:38,879 Speaker 2: And it's not very often that you discover a new 788 00:36:38,880 --> 00:36:41,320 Speaker 2: particle from the top quark in the nineties and the 789 00:36:41,360 --> 00:36:45,200 Speaker 2: Higgs boson in the early twenty tens and nothing ever since. 790 00:36:45,400 --> 00:36:47,319 Speaker 2: So you spent a lot of time studying each one 791 00:36:47,360 --> 00:36:48,360 Speaker 2: because they're precious. 792 00:36:49,280 --> 00:36:51,000 Speaker 1: So if you discover a new particle, that'll be your 793 00:36:51,040 --> 00:36:54,719 Speaker 1: new favorite. I see how fickly your a physicists are. 794 00:36:54,920 --> 00:36:57,280 Speaker 2: That's right, The young one is always the baby particle 795 00:36:57,320 --> 00:36:59,680 Speaker 2: of the family, and you know you gotta love the baby. 796 00:36:59,480 --> 00:37:03,080 Speaker 1: Just fall in the latest trend, the latest hit particle. Well, 797 00:37:03,239 --> 00:37:05,680 Speaker 1: we're asking the question of how you measure the mass 798 00:37:05,680 --> 00:37:07,799 Speaker 1: of the Higgs boson, and it seems like you do 799 00:37:07,840 --> 00:37:10,399 Speaker 1: it at the Large Hadron Collider and any collider can 800 00:37:10,400 --> 00:37:12,839 Speaker 1: any collider study the mass of the Higgs or right now, 801 00:37:13,000 --> 00:37:15,520 Speaker 1: is the Large Hadron Collider at the only collider that 802 00:37:15,560 --> 00:37:15,920 Speaker 1: can do that? 803 00:37:16,200 --> 00:37:18,719 Speaker 2: Well, the LAHC doesn't have a monopoly on a per se. 804 00:37:18,840 --> 00:37:20,640 Speaker 2: It's just that it's the only one that has enough 805 00:37:20,719 --> 00:37:23,600 Speaker 2: energy to make the Higgs boson, and so it's the 806 00:37:23,600 --> 00:37:25,960 Speaker 2: only place that it can be studied. So far, we're 807 00:37:25,960 --> 00:37:28,840 Speaker 2: working on plans for other colliders, including maybe even a 808 00:37:28,920 --> 00:37:32,280 Speaker 2: Muon collider that can make like huge numbers of Higgs bosons, 809 00:37:32,480 --> 00:37:34,239 Speaker 2: but you have to make it in order to study it. 810 00:37:34,560 --> 00:37:36,800 Speaker 1: And so we were talking about how you collide things 811 00:37:36,840 --> 00:37:39,320 Speaker 1: and then you look at the debris, and then you 812 00:37:39,360 --> 00:37:42,440 Speaker 1: figure out that in some crashes, like the evidence you 813 00:37:42,440 --> 00:37:45,520 Speaker 1: see can only be explained by the Higgs boson, and 814 00:37:46,200 --> 00:37:49,520 Speaker 1: from the debris can also sort of infer what its 815 00:37:49,600 --> 00:37:51,959 Speaker 1: mass is. And so we got that down pretty good. 816 00:37:52,000 --> 00:37:53,680 Speaker 2: We have that down pretty good. There's been a lot 817 00:37:53,680 --> 00:37:56,640 Speaker 2: of really really careful studies, and this is not an 818 00:37:56,680 --> 00:37:59,160 Speaker 2: easy thing to do. I mean, we're saying the Higgs 819 00:37:59,200 --> 00:38:02,200 Speaker 2: boson turns to two photons or two bottom quarks or 820 00:38:02,239 --> 00:38:05,200 Speaker 2: sometimes two w bosons, and we're just saying, oh, you 821 00:38:05,239 --> 00:38:08,760 Speaker 2: measure those particles, masses and energies. But that's not trivial. 822 00:38:08,840 --> 00:38:12,799 Speaker 2: You know, that involves building and calibrating complicated detectors in 823 00:38:12,960 --> 00:38:15,800 Speaker 2: order to measure those streaks and extract that information. 824 00:38:16,040 --> 00:38:18,759 Speaker 1: Yeah, and also like that it doesn't happen every time 825 00:38:18,760 --> 00:38:21,560 Speaker 1: you crash some particles, right, Like, you have to collide 826 00:38:21,840 --> 00:38:25,040 Speaker 1: trillions of particles to sort of get one where maybe 827 00:38:25,080 --> 00:38:26,759 Speaker 1: a Higgs boson can be seen. 828 00:38:26,840 --> 00:38:29,560 Speaker 2: Oh yeah, great point. The Higgs boson is really really rare. 829 00:38:29,960 --> 00:38:33,320 Speaker 2: That's why we collide particles so often, millions and millions 830 00:38:33,360 --> 00:38:35,680 Speaker 2: of times per second, hoping that maybe like one of 831 00:38:35,719 --> 00:38:38,160 Speaker 2: those collisions will give us a Higgs boson. So first 832 00:38:38,200 --> 00:38:40,319 Speaker 2: we have to smash in the particles together to get 833 00:38:40,320 --> 00:38:42,040 Speaker 2: a sample that's going to have a bunch of Higgs 834 00:38:42,080 --> 00:38:44,400 Speaker 2: bosons in them. Then we have to try to isolate 835 00:38:44,440 --> 00:38:47,400 Speaker 2: the collisions that we think probably come from the Higgs boson, 836 00:38:47,719 --> 00:38:50,239 Speaker 2: but that's not totally possible. Some of those collisions will 837 00:38:50,280 --> 00:38:53,360 Speaker 2: always be due to other stuff that just happens to Also, 838 00:38:53,480 --> 00:38:56,600 Speaker 2: give two photons that look kind of like a Higgs boson, 839 00:38:57,040 --> 00:38:59,560 Speaker 2: or give two w bosons that look kind of like 840 00:38:59,560 --> 00:39:02,120 Speaker 2: a Higgs photon. So you can never say this collision 841 00:39:02,160 --> 00:39:03,960 Speaker 2: has a Higgs in it or that collision has a 842 00:39:04,000 --> 00:39:06,400 Speaker 2: Higgs in it. It's always statistical. You have a set 843 00:39:06,400 --> 00:39:08,800 Speaker 2: of collisions you say, we think there's like ten percent 844 00:39:08,840 --> 00:39:11,399 Speaker 2: Higgs in here, or there's fourteen percent Higgs in here. 845 00:39:11,520 --> 00:39:14,680 Speaker 1: But I guess since the Higgs boson gives all particles 846 00:39:14,760 --> 00:39:18,399 Speaker 1: their mass, isn't technically the Higgs boson in all collisions too. 847 00:39:18,640 --> 00:39:20,440 Speaker 2: It is, but sort of in a virtual sense. Like 848 00:39:20,480 --> 00:39:22,920 Speaker 2: the Higgs field is everywhere, and the Higgs field is 849 00:39:22,920 --> 00:39:26,040 Speaker 2: involved in everything, even low energy collisions. But if you 850 00:39:26,080 --> 00:39:27,680 Speaker 2: want to study its mass, you have to make a 851 00:39:27,719 --> 00:39:30,279 Speaker 2: real Higgs boson. You have to excite the field enough 852 00:39:30,560 --> 00:39:33,239 Speaker 2: so that it pops out an actual Higgs boson, a 853 00:39:33,280 --> 00:39:34,920 Speaker 2: real one, not a virtual one. 854 00:39:35,400 --> 00:39:36,240 Speaker 1: What's the difference? 855 00:39:36,520 --> 00:39:39,840 Speaker 2: Virtual particles really just saying another ripple in the fields, 856 00:39:39,880 --> 00:39:42,759 Speaker 2: like information wiggling through the field. But that information can 857 00:39:42,800 --> 00:39:45,600 Speaker 2: propagate in all sorts of ways that particles don't propagate. 858 00:39:45,880 --> 00:39:48,239 Speaker 2: You know, particles, for example, have a specific mass, or 859 00:39:48,280 --> 00:39:50,960 Speaker 2: real Higgs boson moving through the Higgs field has a 860 00:39:51,080 --> 00:39:54,040 Speaker 2: very specific mass. Virtual particles don't have to follow those rules. 861 00:39:54,080 --> 00:39:56,360 Speaker 2: They can have all sorts of weird masses, including like 862 00:39:56,480 --> 00:40:01,000 Speaker 2: zero or negative masses. Virtual particles are not really particles, 863 00:40:01,040 --> 00:40:03,799 Speaker 2: they're just ripples in the Higgs field. You can sometimes 864 00:40:03,960 --> 00:40:06,560 Speaker 2: kind of describe using particle like words. 865 00:40:07,560 --> 00:40:09,600 Speaker 1: But I guess, if the Higgs boson is so rare, 866 00:40:09,920 --> 00:40:12,960 Speaker 1: is it really what's giving mass to the other particles then, 867 00:40:13,120 --> 00:40:15,600 Speaker 1: because I feel like you're saying it's rare and virtual 868 00:40:16,040 --> 00:40:18,080 Speaker 1: and you rarely ever see it, but at the same time, 869 00:40:18,160 --> 00:40:20,240 Speaker 1: it's affecting us all the time everywhere. 870 00:40:20,440 --> 00:40:22,759 Speaker 2: Yeah, because the Higgs field is everywhere. Even if there 871 00:40:22,760 --> 00:40:25,960 Speaker 2: are no real Higgs bosons around, the Higgs field fills 872 00:40:25,960 --> 00:40:29,520 Speaker 2: the whole universe, and it's constantly interacting with your electrons 873 00:40:29,520 --> 00:40:31,920 Speaker 2: and your top quarks. So maybe what you're getting at 874 00:40:31,960 --> 00:40:34,400 Speaker 2: is it is possible to detect the Higgs field and 875 00:40:34,440 --> 00:40:38,799 Speaker 2: to deduce things about it from its interactions with those particles, right, Like, 876 00:40:38,840 --> 00:40:41,239 Speaker 2: by measuring the top quark very precisely and measuring the 877 00:40:41,400 --> 00:40:43,840 Speaker 2: w boson very very precisely, we can learn a lot 878 00:40:43,880 --> 00:40:45,719 Speaker 2: about the Higgs field, and that's how they make those 879 00:40:45,760 --> 00:40:48,040 Speaker 2: predictions of what the Higgs mass sort of has to 880 00:40:48,080 --> 00:40:50,719 Speaker 2: be like. Before we found the Higgs boson mass, we 881 00:40:50,800 --> 00:40:53,360 Speaker 2: had ideas for what its mass might be based on 882 00:40:53,400 --> 00:40:56,920 Speaker 2: these sort of indirect measurements observations of how it's affecting 883 00:40:56,960 --> 00:40:57,960 Speaker 2: the other particles. 884 00:40:58,239 --> 00:41:00,439 Speaker 1: All right, Well, let's get to what we know about 885 00:41:00,480 --> 00:41:02,440 Speaker 1: the mass of the Higgs field. So you said, we 886 00:41:02,520 --> 00:41:04,759 Speaker 1: know that it's one hundred and twenty five zero point 887 00:41:04,800 --> 00:41:08,560 Speaker 1: thirty five GEVs plus or minus zero point one percent. 888 00:41:08,760 --> 00:41:11,360 Speaker 1: What does that mean? Is that more than what we expected? 889 00:41:11,440 --> 00:41:13,760 Speaker 1: It seems like it's a lot, because it's one hundred 890 00:41:13,960 --> 00:41:16,120 Speaker 1: times more than the mass of the proton. But is 891 00:41:16,160 --> 00:41:19,279 Speaker 1: that surprising or is that expected? Is it interesting that 892 00:41:19,320 --> 00:41:21,319 Speaker 1: it weighs that much or could it have been any 893 00:41:21,320 --> 00:41:21,920 Speaker 1: other mass? 894 00:41:21,920 --> 00:41:24,640 Speaker 2: Well, first of all, it's very impressive that it's measured 895 00:41:24,800 --> 00:41:27,799 Speaker 2: so precisely. Like, this is really hard. I guess it's 896 00:41:27,840 --> 00:41:29,200 Speaker 2: kind of my job so. 897 00:41:29,360 --> 00:41:33,360 Speaker 1: This horn, But like this is not hard, Yes, according 898 00:41:33,360 --> 00:41:38,800 Speaker 1: to people who had to do it. 899 00:41:36,600 --> 00:41:38,600 Speaker 2: It is really hard. You know, like a Higgs boson 900 00:41:38,640 --> 00:41:41,120 Speaker 2: decays the two photons. You got to measure those photons 901 00:41:41,160 --> 00:41:42,839 Speaker 2: really precisely. You got to come up with all sorts 902 00:41:42,840 --> 00:41:45,239 Speaker 2: of clever ways to know, like how can you tell 903 00:41:45,239 --> 00:41:47,600 Speaker 2: the difference between photon and dis energy and that energy 904 00:41:47,640 --> 00:41:50,240 Speaker 2: and how do you know for sure? Like people spend 905 00:41:50,320 --> 00:41:54,440 Speaker 2: weeks and weeks sweating over the details, the tiny little 906 00:41:54,440 --> 00:41:57,759 Speaker 2: problems it might crop up in your photon calibration which 907 00:41:57,800 --> 00:42:01,160 Speaker 2: gets propagated to your Higgs Boson calibration. And it's all 908 00:42:01,239 --> 00:42:04,600 Speaker 2: because this number means a lot, as you were saying earlier, 909 00:42:04,600 --> 00:42:06,719 Speaker 2: like the Higgs bison could have been heavier, it could 910 00:42:06,719 --> 00:42:08,640 Speaker 2: have been lighter. It was a little bit of a 911 00:42:08,680 --> 00:42:12,160 Speaker 2: surprise to some people that it was so light, because remember, 912 00:42:12,360 --> 00:42:15,320 Speaker 2: those two numbers have to somehow balance each other out, 913 00:42:15,560 --> 00:42:18,080 Speaker 2: like a huge, big random positive number and a huge, 914 00:42:18,120 --> 00:42:21,759 Speaker 2: big random negative number somehow almost cancel out to give 915 00:42:21,800 --> 00:42:24,840 Speaker 2: this slightly positive number. And there's some folks out there 916 00:42:24,920 --> 00:42:26,840 Speaker 2: who were thinking that those numbers are never going to 917 00:42:26,920 --> 00:42:28,840 Speaker 2: cancel out, that they were going to give us a 918 00:42:29,000 --> 00:42:31,919 Speaker 2: huge number, like something so big we would never see 919 00:42:31,920 --> 00:42:33,240 Speaker 2: it in the large Hadron colliner. 920 00:42:33,600 --> 00:42:36,480 Speaker 1: So it was lighter than people expected. They thought it 921 00:42:36,520 --> 00:42:38,440 Speaker 1: was going to be even more huge. 922 00:42:38,640 --> 00:42:40,480 Speaker 2: Yeah, some people thought it was going to be really huge. 923 00:42:40,520 --> 00:42:43,560 Speaker 2: Other people have ideas to explain that sort of apparent coincidence. 924 00:42:43,600 --> 00:42:46,000 Speaker 2: They say, well, maybe there is a connection between all 925 00:42:46,000 --> 00:42:48,200 Speaker 2: the particles that are making the Higgs heavier and all 926 00:42:48,239 --> 00:42:50,560 Speaker 2: the particles that are making the Higgs lighter. Maybe there's 927 00:42:50,560 --> 00:42:53,080 Speaker 2: like a balance in the universe, a symmetry that says 928 00:42:53,320 --> 00:42:55,719 Speaker 2: for every particle that's making the Higgs heavier, there has 929 00:42:55,840 --> 00:42:58,359 Speaker 2: to be one making the Higgs lighter, and that's why 930 00:42:58,400 --> 00:43:00,719 Speaker 2: these two things cancel each other out. Maybe there are 931 00:43:00,760 --> 00:43:03,000 Speaker 2: a whole bunch of other particles out there and then 932 00:43:03,080 --> 00:43:06,080 Speaker 2: just sort of like magically balancing everything that we have seen. 933 00:43:06,560 --> 00:43:09,319 Speaker 2: And that's a theory called supersymmetry. It says to make 934 00:43:09,360 --> 00:43:12,160 Speaker 2: those two different contributions balance and keep the Higgs field 935 00:43:12,360 --> 00:43:14,960 Speaker 2: very very light. So for some people when we saw 936 00:43:15,000 --> 00:43:17,400 Speaker 2: the Higgs boson mass, was you think it's kind of heavy. 937 00:43:17,400 --> 00:43:19,960 Speaker 2: Some people think it's kind of light. Actually, they thought 938 00:43:20,000 --> 00:43:22,760 Speaker 2: maybe this is a hint that there are these super 939 00:43:22,760 --> 00:43:24,040 Speaker 2: symmetric fields out there. 940 00:43:24,200 --> 00:43:26,960 Speaker 1: Could the Higgs boson have had zero mass? Was that 941 00:43:27,000 --> 00:43:29,680 Speaker 1: a possibility when you went into it, or did the 942 00:43:29,719 --> 00:43:32,560 Speaker 1: Peter Higgs theory say it had to have some mass. 943 00:43:32,600 --> 00:43:34,520 Speaker 2: It could have had zero mass. That is a possibility, 944 00:43:34,880 --> 00:43:36,560 Speaker 2: But you know, then it would have been pretty easy 945 00:43:36,600 --> 00:43:39,640 Speaker 2: to find because it would have been very easy to create, 946 00:43:40,040 --> 00:43:42,640 Speaker 2: and early searches for the Higgs bosons in the seventies, 947 00:43:42,640 --> 00:43:45,239 Speaker 2: for example, ruled that out pretty quickly. So by the 948 00:43:45,320 --> 00:43:47,680 Speaker 2: time we turned on the Large Hadron collider, we already 949 00:43:47,719 --> 00:43:49,640 Speaker 2: knew the Higgs Boson had to be heavier than like 950 00:43:49,719 --> 00:43:53,440 Speaker 2: one hundred and fifteen or so gv because remember, there 951 00:43:53,480 --> 00:43:55,759 Speaker 2: was another collider in the nineties which ran into the 952 00:43:55,800 --> 00:44:00,920 Speaker 2: early two thousands called the LP Large Electron possit Tron Collider, 953 00:44:01,080 --> 00:44:03,440 Speaker 2: and that one would have found the Higgs boson if 954 00:44:03,440 --> 00:44:05,760 Speaker 2: it was up to about one hundred and fourteen GeV. 955 00:44:06,440 --> 00:44:08,080 Speaker 1: All right, well, then what does it mean that it 956 00:44:08,120 --> 00:44:10,120 Speaker 1: has the mass that it has. What does it mean 957 00:44:10,120 --> 00:44:12,279 Speaker 1: for the future, I guess, or our understanding of the 958 00:44:13,120 --> 00:44:14,480 Speaker 1: models of the universe. 959 00:44:14,320 --> 00:44:16,520 Speaker 2: Right now, it means that there's no specific evidence for 960 00:44:16,680 --> 00:44:19,200 Speaker 2: other particles out there. Like if the Higgs boson had 961 00:44:19,239 --> 00:44:22,040 Speaker 2: had some very crazy heavy mass, it would mean, oh, 962 00:44:22,040 --> 00:44:25,160 Speaker 2: it's getting influenced by another particle out there that's making 963 00:44:25,200 --> 00:44:27,680 Speaker 2: it heavier, a particle we haven't seen yet. So in 964 00:44:27,719 --> 00:44:29,719 Speaker 2: that way, like making a very precise measurement at the 965 00:44:29,760 --> 00:44:32,840 Speaker 2: Higgs Boson mass is a great way to test our understanding, 966 00:44:32,920 --> 00:44:35,160 Speaker 2: you know, because these things are all connected. You might 967 00:44:35,160 --> 00:44:37,120 Speaker 2: remember that there was a very precise measurement at the 968 00:44:37,280 --> 00:44:40,360 Speaker 2: w Boson mass last year. They gave a very weird result, 969 00:44:40,480 --> 00:44:42,959 Speaker 2: a result that didn't agree with all of our calculations, 970 00:44:43,239 --> 00:44:45,520 Speaker 2: and these are all tightly coupled, the W the top 971 00:44:45,600 --> 00:44:47,560 Speaker 2: the Higgs. If you change one of them, it changes 972 00:44:47,640 --> 00:44:50,040 Speaker 2: all the other ones. So getting a weird value for 973 00:44:50,080 --> 00:44:52,759 Speaker 2: the W mass means maybe there's something else going on 974 00:44:52,880 --> 00:44:55,200 Speaker 2: out there. So that's why it's important to get a 975 00:44:55,280 --> 00:44:58,320 Speaker 2: very precise measurement. It's like without creating those new particles, 976 00:44:58,320 --> 00:45:00,800 Speaker 2: you can be sensitive to their existence, which is a 977 00:45:00,800 --> 00:45:04,520 Speaker 2: pretty cool way to explore the universe indirectly. It's also 978 00:45:04,560 --> 00:45:07,920 Speaker 2: relevant to the question of whether the Higgs field is stable. 979 00:45:08,520 --> 00:45:12,200 Speaker 2: How the Higgs interacts with itself changes how stable the 980 00:45:12,239 --> 00:45:15,200 Speaker 2: Higgs field is, and that's connected to the Higgs mass, 981 00:45:15,239 --> 00:45:17,920 Speaker 2: But the Higgs boson also, because it couples to itself, 982 00:45:18,400 --> 00:45:21,640 Speaker 2: its mass effects whether might collapse, and if Higgs field 983 00:45:21,640 --> 00:45:24,840 Speaker 2: collapses it changes the whole structure of the universe and 984 00:45:24,880 --> 00:45:28,800 Speaker 2: our whole experience. So measuring the Higgs boson mass tells 985 00:45:28,920 --> 00:45:30,920 Speaker 2: us whether or not the Higgs field is likely to 986 00:45:30,960 --> 00:45:32,480 Speaker 2: be stable or unstable. 987 00:45:32,680 --> 00:45:35,600 Speaker 1: M you say that, it also tells you whether there 988 00:45:35,640 --> 00:45:37,840 Speaker 1: are more particles out there. So if you have this 989 00:45:37,960 --> 00:45:40,680 Speaker 1: measurement down pretty good, does that mean that you don't 990 00:45:40,680 --> 00:45:43,040 Speaker 1: think there are other particles out there yet to discover. 991 00:45:43,239 --> 00:45:44,839 Speaker 1: You think we've maybe discovered them all. 992 00:45:45,120 --> 00:45:47,120 Speaker 2: Well, if you can where this recent measurement of the 993 00:45:47,200 --> 00:45:49,640 Speaker 2: W mass by CDF, the one that says that everything 994 00:45:49,680 --> 00:45:52,359 Speaker 2: is out of whack and the things don't agree, then 995 00:45:52,440 --> 00:45:54,960 Speaker 2: everything agrees pretty nicely. At the top, the W, and 996 00:45:54,960 --> 00:45:57,120 Speaker 2: the Higgs are all consistent with each other, and that 997 00:45:57,160 --> 00:45:59,680 Speaker 2: means that there isn't evidence for anything new out there yet. 998 00:46:00,000 --> 00:46:03,400 Speaker 2: Other hand, it leaves this question unanswered of why the 999 00:46:03,440 --> 00:46:05,160 Speaker 2: top and the W and all that stuff add up 1000 00:46:05,160 --> 00:46:07,279 Speaker 2: to give a Higgs that's so light, Like I said, 1001 00:46:07,360 --> 00:46:09,920 Speaker 2: just a coincidence. The masses of these particles are tuned 1002 00:46:10,160 --> 00:46:12,600 Speaker 2: to one part in ten to the ten, so that 1003 00:46:12,640 --> 00:46:14,680 Speaker 2: the Higgs boson just happens to come out to be 1004 00:46:14,760 --> 00:46:17,480 Speaker 2: this very small number. It seems like too big a coincidence, 1005 00:46:17,880 --> 00:46:20,840 Speaker 2: and so we're looking for another explanation. And another explanation 1006 00:46:21,000 --> 00:46:24,200 Speaker 2: might be other particles out there that like help balance 1007 00:46:24,200 --> 00:46:26,600 Speaker 2: the Higgs boson mass, but we just don't know so far. 1008 00:46:27,400 --> 00:46:29,960 Speaker 1: All right, Well, I guess stay tuned. You have the 1009 00:46:30,040 --> 00:46:32,880 Speaker 1: large Headron collider. You just upgraded it, right, you're running 1010 00:46:32,880 --> 00:46:35,440 Speaker 1: that maybe faster than it had been before. 1011 00:46:35,600 --> 00:46:38,239 Speaker 2: Yeah, that's right. We're getting more and more collisions every time, 1012 00:46:38,320 --> 00:46:41,120 Speaker 2: and more protons in every collision, and we're going to 1013 00:46:41,239 --> 00:46:43,120 Speaker 2: run it for another ten issue, and we're going to 1014 00:46:43,200 --> 00:46:46,279 Speaker 2: run it for decades longer and collect huge piles of 1015 00:46:46,320 --> 00:46:48,840 Speaker 2: events and sift through them for evidence to see if 1016 00:46:48,840 --> 00:46:51,200 Speaker 2: the Higgs is doing something weird, because we can measure 1017 00:46:51,200 --> 00:46:53,360 Speaker 2: the higgs boson mass in all sorts of different ways 1018 00:46:53,560 --> 00:46:55,640 Speaker 2: when it decaysed to photons, or in it decays to 1019 00:46:55,680 --> 00:46:58,080 Speaker 2: bottom quarks or in the case to w bosons, and 1020 00:46:58,120 --> 00:47:00,640 Speaker 2: we can also compare those against each other. Does the 1021 00:47:00,680 --> 00:47:02,960 Speaker 2: Higgs look heavier when it turns into a photon or 1022 00:47:03,000 --> 00:47:05,360 Speaker 2: when it turns into quarks, or when it turns into w's. 1023 00:47:05,640 --> 00:47:08,560 Speaker 2: If there's any disagreement there, that's another hint that something 1024 00:47:08,600 --> 00:47:09,440 Speaker 2: new is going on. 1025 00:47:09,920 --> 00:47:11,320 Speaker 1: Wait, the mask can change. 1026 00:47:11,760 --> 00:47:13,640 Speaker 2: The mass should be the same no matter how you 1027 00:47:13,680 --> 00:47:15,879 Speaker 2: measure it. It should be the same if it turns 1028 00:47:15,880 --> 00:47:17,719 Speaker 2: into photons, or if it turns into b's orf it 1029 00:47:17,760 --> 00:47:20,480 Speaker 2: turns into w's. But if there's something else going on, 1030 00:47:20,520 --> 00:47:22,480 Speaker 2: if it's not the Higgs that we thought it was, 1031 00:47:22,680 --> 00:47:24,120 Speaker 2: or if there's more than one higgs, or if there 1032 00:47:24,160 --> 00:47:27,480 Speaker 2: are other particles getting involved. Then you might measure different 1033 00:47:27,480 --> 00:47:29,680 Speaker 2: masses in those different decay modes, and that would be 1034 00:47:29,680 --> 00:47:32,120 Speaker 2: a signed this something else going on you don't understand. 1035 00:47:32,280 --> 00:47:34,160 Speaker 1: Could be that the Higgs boson is actually made out 1036 00:47:34,160 --> 00:47:36,000 Speaker 1: of white chocolate, not dark travel. 1037 00:47:37,719 --> 00:47:40,360 Speaker 2: It's been Santus present to himself all this time. 1038 00:47:40,280 --> 00:47:45,400 Speaker 1: All this time. That's right, it's the clos hypothesis. Should 1039 00:47:45,440 --> 00:47:48,759 Speaker 1: have been the clouds field. Yeah, the Clawson, there you go, 1040 00:47:49,080 --> 00:47:53,760 Speaker 1: the Sandton. All right. Well, a lot of interesting questions 1041 00:47:53,880 --> 00:47:56,880 Speaker 1: talking about and thinking about in this fundamental particle of 1042 00:47:56,920 --> 00:47:58,960 Speaker 1: the universe. I guess the next time you step on 1043 00:47:58,960 --> 00:48:01,480 Speaker 1: a scale, think about you're measuring what your mass is, 1044 00:48:01,840 --> 00:48:05,160 Speaker 1: and think about how many virtual or real Higgs Bosons 1045 00:48:05,239 --> 00:48:07,600 Speaker 1: are flying all around you and inside of you. 1046 00:48:07,719 --> 00:48:10,480 Speaker 2: And how this is just one step in our understanding 1047 00:48:10,600 --> 00:48:13,279 Speaker 2: of the universe. We have this crazy model we put 1048 00:48:13,320 --> 00:48:15,359 Speaker 2: together on our heads and it makes predictions and it 1049 00:48:15,400 --> 00:48:17,600 Speaker 2: has blank spaces in it. Then me go out and 1050 00:48:17,680 --> 00:48:20,440 Speaker 2: confront the actual universe and see if we can get 1051 00:48:20,480 --> 00:48:23,520 Speaker 2: this model to describe everything that we experience. 1052 00:48:23,760 --> 00:48:26,600 Speaker 1: So thanks for joining us, see you next time. 1053 00:48:34,520 --> 00:48:37,320 Speaker 2: Thanks for listening, and remember that Daniel and Jorge explain 1054 00:48:37,400 --> 00:48:41,399 Speaker 2: the universe is a production of iHeartRadio. For more podcasts 1055 00:48:41,400 --> 00:48:46,040 Speaker 2: from iHeartRadio, visit the iHeartRadio app, Apple Podcasts, or wherever 1056 00:48:46,120 --> 00:48:47,840 Speaker 2: you listen to your favorite shows.