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When you pop 10 00:00:29,320 --> 00:00:31,240 Speaker 1: a piece of cheese into your mouth, you're probably not 11 00:00:31,360 --> 00:00:34,280 Speaker 1: thinking about the environmental impact. But the people in the 12 00:00:34,360 --> 00:00:37,680 Speaker 1: dairy industry are. That's why they're working hard every day 13 00:00:37,720 --> 00:00:40,760 Speaker 1: to find new ways to reduce waste, conserve natural resources, 14 00:00:40,800 --> 00:00:44,360 Speaker 1: and drive down greenhouse gas emissions. How is US Dairy 15 00:00:44,400 --> 00:00:48,520 Speaker 1: tackling greenhouse gases? Many farms use anaerobic digesters to turn 16 00:00:48,560 --> 00:00:53,080 Speaker 1: the methane from manure into renewable energy that can power farms, towns, 17 00:00:53,120 --> 00:00:57,240 Speaker 1: and electric cars. Visit us Dairy dot COM's Last Sustainability 18 00:00:57,280 --> 00:00:58,000 Speaker 1: to learn more. 19 00:00:58,960 --> 00:01:02,600 Speaker 2: Here's a little secret. 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So get yourself down a 29 00:01:30,640 --> 00:01:33,360 Speaker 2: street level and learn how to snag the new Samsung 30 00:01:33,400 --> 00:01:36,880 Speaker 2: Galaxy Z flip six on AT and T and maybe 31 00:01:36,880 --> 00:01:39,320 Speaker 2: grab a ladder on the way home. AT and T 32 00:01:39,720 --> 00:01:44,119 Speaker 2: connecting changes everything requires trade in a Galaxy s Note 33 00:01:44,200 --> 00:01:46,960 Speaker 2: or Z series smartphone, limited time offer two hundred and 34 00:01:46,959 --> 00:01:49,880 Speaker 2: fifty six gigabytes for zero dollars. Additional fees, terms and 35 00:01:49,920 --> 00:01:53,360 Speaker 2: restrictions apply. See att dot com, slash Samsung, or visit 36 00:01:53,400 --> 00:01:56,960 Speaker 2: an AT and T store for details. 37 00:02:07,280 --> 00:02:09,280 Speaker 1: Hey, Jorgey, do you have a lot of cousins in 38 00:02:09,320 --> 00:02:09,840 Speaker 1: your family? 39 00:02:10,280 --> 00:02:13,600 Speaker 4: Yeah, I've got a few. I have maybe over thirty 40 00:02:13,639 --> 00:02:15,680 Speaker 4: six cousins, maybe around that number. 41 00:02:16,000 --> 00:02:18,840 Speaker 1: Wow, that's a big family. Well, would you be surprised 42 00:02:18,880 --> 00:02:21,560 Speaker 1: to discover, sort of late in life a brand new 43 00:02:21,639 --> 00:02:23,840 Speaker 1: cousin you'd never even heard of before. 44 00:02:24,200 --> 00:02:26,640 Speaker 4: That would be pretty amazing, kind of weird, I guess, 45 00:02:26,720 --> 00:02:29,680 Speaker 4: but maybe, yeah, I would be surprised, all right. 46 00:02:29,760 --> 00:02:31,720 Speaker 1: And then what if that cousin turns out to be 47 00:02:32,040 --> 00:02:35,400 Speaker 1: exactly like you, like, look like you in every single way. 48 00:02:35,600 --> 00:02:37,720 Speaker 4: Okay, Yeah, that's getting kind of weird. 49 00:02:37,720 --> 00:02:40,720 Speaker 1: All right. And then what if this cousin looks exactly 50 00:02:40,800 --> 00:02:45,240 Speaker 1: like you, except they are two hundred times more. 51 00:02:45,080 --> 00:03:05,840 Speaker 4: Massive Dan Dan do Hi, I'm Jorge. I'm a cartoonist 52 00:03:05,880 --> 00:03:07,800 Speaker 4: and the creator of PhD Comics. 53 00:03:08,000 --> 00:03:11,079 Speaker 1: Hi, I'm Daniel. I'm a particle physicist, and I do 54 00:03:11,200 --> 00:03:12,800 Speaker 1: not have thirty six cousins. 55 00:03:13,400 --> 00:03:17,440 Speaker 4: Welcome to our podcast, Daniel and Jorge Explore Your Family Tree. 56 00:03:17,600 --> 00:03:20,760 Speaker 1: In which we examine all the amazing and fascinating things 57 00:03:20,800 --> 00:03:24,000 Speaker 1: about the universe, about the big things, the small things, 58 00:03:24,040 --> 00:03:26,360 Speaker 1: and about how things are related to each other. 59 00:03:26,880 --> 00:03:29,240 Speaker 4: Yeah, so no, that's not the name of our podcast. 60 00:03:29,280 --> 00:03:32,880 Speaker 4: It's actually Daniel and Jorge Explain the Universe, a production 61 00:03:33,040 --> 00:03:34,800 Speaker 4: of iHeartRadio, in which. 62 00:03:34,639 --> 00:03:37,640 Speaker 1: We do examine crazy things about the universe and we 63 00:03:37,760 --> 00:03:40,120 Speaker 1: try to make them relatable. We try to present them 64 00:03:40,120 --> 00:03:42,000 Speaker 1: in a way that you can understand them. So they 65 00:03:42,000 --> 00:03:43,640 Speaker 1: connect to topics that matter to you. 66 00:03:44,000 --> 00:03:45,680 Speaker 4: Yeah, in a way, we do sort of explore the 67 00:03:45,720 --> 00:03:48,600 Speaker 4: family tree of the universe. You know, how you came 68 00:03:48,640 --> 00:03:53,000 Speaker 4: to be here, what sort of pairings and fusions occurred 69 00:03:53,040 --> 00:03:55,760 Speaker 4: for you to be here in this universe? Appreciating it 70 00:03:55,840 --> 00:03:57,680 Speaker 4: and listening to funny podcasts. 71 00:03:57,760 --> 00:04:00,040 Speaker 1: Yeah, I think one of the reasons people are in 72 00:04:00,120 --> 00:04:02,200 Speaker 1: just did in the origins of the universe and the 73 00:04:02,280 --> 00:04:05,360 Speaker 1: creations of our cosmosis because they want to understand how 74 00:04:05,400 --> 00:04:07,520 Speaker 1: we got here and what it means. In the same 75 00:04:07,560 --> 00:04:10,000 Speaker 1: way people explore their family tree. They want to know 76 00:04:10,240 --> 00:04:12,680 Speaker 1: where did my family come from, what stories are in 77 00:04:12,760 --> 00:04:16,480 Speaker 1: our past, what is my personal context? And also I 78 00:04:16,480 --> 00:04:18,200 Speaker 1: think it's a useful way for us to sort of 79 00:04:18,320 --> 00:04:20,840 Speaker 1: organize our thoughts. You know, when we think about the 80 00:04:21,360 --> 00:04:23,640 Speaker 1: universe in terms of particles, we sometimes think about how 81 00:04:23,640 --> 00:04:27,040 Speaker 1: those particles are related to each other, Like do particles 82 00:04:27,080 --> 00:04:27,760 Speaker 1: have families? 83 00:04:28,160 --> 00:04:30,960 Speaker 4: Yeah? And I think you know, every part of anyone's 84 00:04:31,040 --> 00:04:34,400 Speaker 4: family tree or origin tree kind of tells you a 85 00:04:34,440 --> 00:04:37,000 Speaker 4: little bit of the story of the whole thing, right, 86 00:04:37,120 --> 00:04:40,080 Speaker 4: like how you came to be, how things work and 87 00:04:40,120 --> 00:04:42,200 Speaker 4: how things move about in life. 88 00:04:42,279 --> 00:04:44,400 Speaker 1: And other ways your life could have gone like, if 89 00:04:44,400 --> 00:04:47,640 Speaker 1: you have a very successful cousin that's a gazillionaire, then 90 00:04:47,680 --> 00:04:50,000 Speaker 1: you know you wonder, hmm, could I have made different 91 00:04:50,120 --> 00:04:53,680 Speaker 1: choices and been a gazillionair Or if be people's paths 92 00:04:53,680 --> 00:04:55,039 Speaker 1: in life diverge. 93 00:04:54,680 --> 00:04:57,039 Speaker 4: Yeah, or if you are that bazillion er cousin, then 94 00:04:57,520 --> 00:05:01,400 Speaker 4: good for you. Please these contact as we would love 95 00:05:01,440 --> 00:05:02,440 Speaker 4: to take your donations. 96 00:05:02,680 --> 00:05:04,719 Speaker 1: That's right, it'd be awesome to have at least one 97 00:05:04,760 --> 00:05:08,559 Speaker 1: gazillionaire listener. Who is our richest listener? That's a good question. 98 00:05:08,880 --> 00:05:10,840 Speaker 4: Episode To prove it, you have to send us a check. 99 00:05:12,880 --> 00:05:16,880 Speaker 4: Whoever sends is the biggest check that doesn't bounds. When's 100 00:05:16,960 --> 00:05:19,360 Speaker 4: this little plaque here that I am I'm just now 101 00:05:19,360 --> 00:05:20,000 Speaker 4: putting together? 102 00:05:21,600 --> 00:05:22,520 Speaker 1: It's made of platinum? 103 00:05:22,560 --> 00:05:24,920 Speaker 4: Right, Yeah, well it's going to be once we get 104 00:05:24,920 --> 00:05:25,400 Speaker 4: those checks. 105 00:05:25,480 --> 00:05:28,680 Speaker 1: Yes, you'll get a drawing of a plaque that's made 106 00:05:28,720 --> 00:05:29,200 Speaker 1: of platinum. 107 00:05:29,240 --> 00:05:33,159 Speaker 4: Oh my gosh, even more valuable from a well known 108 00:05:33,200 --> 00:05:34,200 Speaker 4: internet cartoonist. 109 00:05:36,520 --> 00:05:39,640 Speaker 1: Exactly. But we do try to understand the world around us, 110 00:05:39,640 --> 00:05:43,400 Speaker 1: and sometimes that means putting things in context and understanding 111 00:05:43,400 --> 00:05:46,320 Speaker 1: what are the patterns, what are the structures there, and 112 00:05:46,360 --> 00:05:49,080 Speaker 1: what clues do those patterns give? Us about the sort 113 00:05:49,080 --> 00:05:50,880 Speaker 1: of fundamental nature of the universe. 114 00:05:51,040 --> 00:05:53,320 Speaker 4: Yeah. So today on the podcast, we'll be talking about 115 00:05:54,040 --> 00:05:56,640 Speaker 4: a particle in nature that is maybe not the most 116 00:05:56,760 --> 00:06:01,719 Speaker 4: famous one and maybe not the most well known one 117 00:06:01,880 --> 00:06:05,240 Speaker 4: or consequential in your existence, but which does I think 118 00:06:05,640 --> 00:06:08,320 Speaker 4: tell you a little bit about and told humanity a 119 00:06:08,320 --> 00:06:10,560 Speaker 4: little bit about how the universe works. 120 00:06:10,720 --> 00:06:13,919 Speaker 1: Yeah, this is the non gazillionaire cousin. This is the 121 00:06:13,960 --> 00:06:16,480 Speaker 1: cousin that ended up maybe sleeping under the overpass and 122 00:06:16,760 --> 00:06:18,600 Speaker 1: wearing funny clothes to the family reunion. 123 00:06:18,720 --> 00:06:20,159 Speaker 4: Oh, I feel bad for this particle. 124 00:06:20,240 --> 00:06:24,560 Speaker 1: Now, this particle doesn't need your help. It's very massive. 125 00:06:24,800 --> 00:06:32,599 Speaker 4: Yes, In today's episode, we'll be talking about the muon 126 00:06:33,320 --> 00:06:37,159 Speaker 4: Electron's mysterious, lesser known, much more massive cousin. 127 00:06:37,440 --> 00:06:40,320 Speaker 1: And I'm biased, of course, because I'm a particle physicist, 128 00:06:40,400 --> 00:06:43,200 Speaker 1: but I think it's really fascinating to think about how 129 00:06:43,240 --> 00:06:46,640 Speaker 1: we know each particle is there. We talk about the 130 00:06:46,640 --> 00:06:49,560 Speaker 1: standard model of particle physics sometimes, but that's a theoretical 131 00:06:49,600 --> 00:06:53,560 Speaker 1: construct that's like our idea for how these particles might 132 00:06:53,600 --> 00:06:55,640 Speaker 1: relate to each other. And that's fascinating and we'll dig 133 00:06:55,680 --> 00:06:57,760 Speaker 1: into all that. But I think it's also really important 134 00:06:57,800 --> 00:07:00,400 Speaker 1: to remember each of these were discovered. There is a 135 00:07:00,440 --> 00:07:04,240 Speaker 1: story behind each particle. Humanity didn't know it existed and 136 00:07:04,279 --> 00:07:08,320 Speaker 1: then boom, some experiment revealed it. And on the podcast, 137 00:07:08,320 --> 00:07:10,880 Speaker 1: we've talked about the first discovery of the particle, how 138 00:07:10,920 --> 00:07:13,880 Speaker 1: the whole concept of a particle was created, the electron. 139 00:07:14,160 --> 00:07:16,040 Speaker 1: Then we talked about how we know the photon is 140 00:07:16,040 --> 00:07:18,040 Speaker 1: a thing, how we know it's really a particle, the 141 00:07:18,040 --> 00:07:20,200 Speaker 1: photo electric effect, And so now we're going to take 142 00:07:20,240 --> 00:07:22,400 Speaker 1: the next step and talk about the discovery of the muon. 143 00:07:22,680 --> 00:07:25,040 Speaker 4: Yeah, because you know, I think that every particle tells 144 00:07:25,080 --> 00:07:28,360 Speaker 4: a story, you know, and also every story is made 145 00:07:28,400 --> 00:07:30,400 Speaker 4: out of particle. So there's kind of this really weird 146 00:07:30,400 --> 00:07:31,760 Speaker 4: confusing loop there. 147 00:07:33,480 --> 00:07:36,920 Speaker 1: Yeah, this is like the Superhero Origin story particle version. 148 00:07:38,320 --> 00:07:41,520 Speaker 4: Yeah. So the muon is not a name that rolls 149 00:07:41,520 --> 00:07:48,120 Speaker 4: off the tongue. Makes me think of maybe cows muons, maybe. 150 00:07:48,080 --> 00:07:52,800 Speaker 1: Muon muon mew off, muon mew off. I was thinking 151 00:07:52,920 --> 00:07:55,080 Speaker 1: sort of a karate kid thing there. 152 00:07:55,240 --> 00:07:58,000 Speaker 4: Oh, it's back to the eighties references. 153 00:07:58,200 --> 00:08:01,040 Speaker 1: Yeah, back to the eight references. And it's funny actually 154 00:08:01,040 --> 00:08:04,000 Speaker 1: because the name muon is totally inappropriate. We'll dig into 155 00:08:04,000 --> 00:08:06,800 Speaker 1: it later, But they named it before they discovered it 156 00:08:06,840 --> 00:08:09,200 Speaker 1: because they thought it was going to be a different particle, 157 00:08:09,600 --> 00:08:12,680 Speaker 1: and then they sort of changed the name later. It's 158 00:08:12,720 --> 00:08:14,720 Speaker 1: not a great history for naming particles. 159 00:08:14,720 --> 00:08:17,040 Speaker 4: Oh boy, my favorite topic in science. 160 00:08:19,760 --> 00:08:22,360 Speaker 1: Yeah, and so I was wondering, how much do people 161 00:08:22,480 --> 00:08:25,240 Speaker 1: know about Muon's. Is it a famous particle or is 162 00:08:25,280 --> 00:08:27,720 Speaker 1: it sort of the darker cousin of the electron that 163 00:08:27,800 --> 00:08:31,200 Speaker 1: nobody really knows about. Hasn't gotten the same Instagram attention. 164 00:08:31,760 --> 00:08:37,320 Speaker 4: The black sheep, the goateea wearing particle of the family tree. 165 00:08:37,480 --> 00:08:39,640 Speaker 1: Now you're setting it up to be like the grumpy particle. 166 00:08:39,679 --> 00:08:41,480 Speaker 1: It's going to come in with some evil plan to 167 00:08:41,600 --> 00:08:43,720 Speaker 1: finally get its revenge, and it's. 168 00:08:43,559 --> 00:08:45,680 Speaker 4: You already made this particle, the homeless particle that lives 169 00:08:45,720 --> 00:08:46,360 Speaker 4: under a bridge. 170 00:08:46,360 --> 00:08:50,559 Speaker 1: So yeah, that was the sad particle that deserves our 171 00:08:50,679 --> 00:08:53,600 Speaker 1: love and compassion, not the one that's been plotting its 172 00:08:53,679 --> 00:08:55,800 Speaker 1: victorious return to the center of attention. 173 00:08:55,920 --> 00:08:59,079 Speaker 4: Well, you never know what these particles, you know, Physics 174 00:08:59,080 --> 00:08:59,920 Speaker 4: is full of surprises. 175 00:09:02,040 --> 00:09:04,360 Speaker 1: There is a lot of drama. But as usual, I 176 00:09:04,440 --> 00:09:07,439 Speaker 1: walked around and I asked people if they knew what 177 00:09:07,520 --> 00:09:09,680 Speaker 1: the muon was and how we knew it was a thing. 178 00:09:09,840 --> 00:09:11,920 Speaker 4: Yeah, So before you listen to these answers, think about 179 00:09:11,920 --> 00:09:13,880 Speaker 4: it for a second. If someone asks you what a 180 00:09:13,960 --> 00:09:15,960 Speaker 4: muon is, would you know what it is? Have you 181 00:09:16,000 --> 00:09:18,760 Speaker 4: heard it before? Here's what people had to say. 182 00:09:18,960 --> 00:09:20,400 Speaker 1: I'd say, it's a unit of measure. 183 00:09:20,480 --> 00:09:24,120 Speaker 5: It's like one of the fundamental elements or particle of 184 00:09:24,160 --> 00:09:25,120 Speaker 5: what makes up everything. 185 00:09:25,400 --> 00:09:25,959 Speaker 4: A mew on. 186 00:09:26,559 --> 00:09:29,520 Speaker 6: Now, I believe this to be the name of a 187 00:09:29,559 --> 00:09:31,400 Speaker 6: sub atomic particle. 188 00:09:32,840 --> 00:09:38,240 Speaker 4: Luons muon's uh, shoot, I don't remember what classification they 189 00:09:38,320 --> 00:09:42,839 Speaker 4: fall on her as far as the naming conventions. 190 00:09:43,040 --> 00:09:48,040 Speaker 1: Fundamental particle some sort. It's real small sub atomic particles, 191 00:09:49,200 --> 00:09:50,920 Speaker 1: kind of resemed what it does. How do we know 192 00:09:51,040 --> 00:09:57,560 Speaker 1: muons exist? Particles? So what's your opinion of these answers today? 193 00:09:57,640 --> 00:10:00,319 Speaker 4: Pretty good? It sounds like most people have heard it 194 00:10:00,480 --> 00:10:03,719 Speaker 4: or I heard of the word before, you know, very 195 00:10:03,800 --> 00:10:05,640 Speaker 4: only a few people said never heard. 196 00:10:05,440 --> 00:10:08,400 Speaker 1: Of it mm hmmm, or think it was a unit 197 00:10:08,440 --> 00:10:11,080 Speaker 1: of measure, like you know, how much water? Would you like, 198 00:10:11,120 --> 00:10:12,640 Speaker 1: I'll have seven muons of water. 199 00:10:13,520 --> 00:10:15,640 Speaker 4: I wonder that if you pronounced it correctly, maybe they 200 00:10:15,840 --> 00:10:18,880 Speaker 4: knew about it, but just under a different pronunciation. 201 00:10:19,320 --> 00:10:21,439 Speaker 1: You think I'm mispronouncing the name of Muon. 202 00:10:21,480 --> 00:10:23,599 Speaker 4: I don't know. I mean, what's the correct way? Is 203 00:10:23,640 --> 00:10:25,880 Speaker 4: it Muon or Muon? 204 00:10:27,720 --> 00:10:27,800 Speaker 5: Like? 205 00:10:27,920 --> 00:10:30,559 Speaker 1: And you're making it sound like a Disney movie, like, Oh, 206 00:10:30,720 --> 00:10:32,600 Speaker 1: my favorite Disney princess is Mulan. 207 00:10:33,960 --> 00:10:36,360 Speaker 4: My favorite Disney prince is Muon Muan. 208 00:10:38,160 --> 00:10:40,560 Speaker 1: Oh. That is a great way, though, to get more 209 00:10:40,600 --> 00:10:43,200 Speaker 1: attention for particles in the mainstream. We should get Disney 210 00:10:43,200 --> 00:10:46,240 Speaker 1: to name the next Disney princess after a particle. 211 00:10:46,360 --> 00:10:49,400 Speaker 4: Mm why not? Why it could be the next Pixar movie. 212 00:10:49,440 --> 00:10:52,199 Speaker 4: What it's like. What's the emotional roller coaster right of 213 00:10:52,520 --> 00:10:54,760 Speaker 4: being a fundamental particle of nature? 214 00:10:54,960 --> 00:10:57,680 Speaker 1: Yeah? So much to explore there, and I expect that 215 00:10:57,679 --> 00:10:59,640 Speaker 1: we will be getting checks from Pixar when they make 216 00:10:59,640 --> 00:11:02,040 Speaker 1: a billion dollar movie out of it. But I was 217 00:11:02,080 --> 00:11:03,920 Speaker 1: impressed with these answers, though, I want to pick a 218 00:11:03,960 --> 00:11:08,319 Speaker 1: bone about one thing. People say, yes, it's a fundamental particle, 219 00:11:08,480 --> 00:11:11,920 Speaker 1: totally cool. People also say it's a sub atomic particle 220 00:11:12,000 --> 00:11:15,160 Speaker 1: or it's one of the fundamental particles that make up everything. 221 00:11:15,640 --> 00:11:18,079 Speaker 1: And that's really a key idea that I think people 222 00:11:18,080 --> 00:11:20,520 Speaker 1: have not understood about muons, that you can be a 223 00:11:20,559 --> 00:11:23,880 Speaker 1: tiny particle and not be subatomic not be part of 224 00:11:23,920 --> 00:11:24,400 Speaker 1: the atom. 225 00:11:24,720 --> 00:11:27,679 Speaker 4: Oh, I see, sub atomic doesn't just mean it's smaller 226 00:11:27,679 --> 00:11:31,680 Speaker 4: than atom. You're saying that, it means that you're part 227 00:11:31,679 --> 00:11:32,200 Speaker 4: of the atom. 228 00:11:32,400 --> 00:11:36,640 Speaker 1: Remember, fundamental particles have no size there dots, They are 229 00:11:36,720 --> 00:11:40,360 Speaker 1: zero volumes, so they're all smaller than the atom in 230 00:11:40,400 --> 00:11:43,200 Speaker 1: that sense. So being fundamental guarantees you to be smaller 231 00:11:43,280 --> 00:11:45,640 Speaker 1: than the atom. I think to me, sub atomic means 232 00:11:45,679 --> 00:11:47,280 Speaker 1: it's part of the atom, like you break it up 233 00:11:47,320 --> 00:11:49,080 Speaker 1: and you find it inside the atom. 234 00:11:49,200 --> 00:11:52,000 Speaker 4: Okay, so we'll get into that, but let's break it 235 00:11:52,040 --> 00:11:54,520 Speaker 4: down for people. For us, what is a muon and 236 00:11:55,160 --> 00:11:57,960 Speaker 4: why does it sound like an electron? You know it 237 00:11:58,080 --> 00:12:01,400 Speaker 4: ends with on but maybe but it's not the electron. 238 00:12:01,600 --> 00:12:03,959 Speaker 1: Yeah, but it really is related to the electron. It's 239 00:12:03,960 --> 00:12:06,840 Speaker 1: sort of like the electron's cousin. And by that I 240 00:12:06,880 --> 00:12:10,480 Speaker 1: mean that it's identical to the electron in so many ways. 241 00:12:10,800 --> 00:12:13,800 Speaker 1: It has the same electric charge, it has the same 242 00:12:13,880 --> 00:12:17,840 Speaker 1: interactions with matter, like it interacts via the weak force 243 00:12:18,120 --> 00:12:21,320 Speaker 1: and via the electromagnetic force, but it doesn't feel the 244 00:12:21,360 --> 00:12:25,360 Speaker 1: strong force just like the electron. It has a neutrino, 245 00:12:25,679 --> 00:12:28,240 Speaker 1: just like the electron has its neutrino. So in so 246 00:12:28,360 --> 00:12:31,040 Speaker 1: many ways, it's exactly the same as the electron. Sound 247 00:12:31,040 --> 00:12:33,400 Speaker 1: like when you discover a new particle and it's totally different, 248 00:12:33,480 --> 00:12:36,079 Speaker 1: like a quark or a glu on, it's just completely 249 00:12:36,120 --> 00:12:39,080 Speaker 1: different from the electron. This one is very very similar 250 00:12:39,160 --> 00:12:41,760 Speaker 1: to the electron. It's like weirdly similar, but then with 251 00:12:41,880 --> 00:12:43,040 Speaker 1: one important difference. 252 00:12:43,240 --> 00:12:46,920 Speaker 4: Okay, so it's a particle. Let's start down. 253 00:12:48,840 --> 00:12:51,240 Speaker 1: It's not a cow, it's not a Disney princess. 254 00:12:51,840 --> 00:12:54,360 Speaker 4: So it's a particle, meaning like it's a it's one 255 00:12:54,400 --> 00:12:56,520 Speaker 4: of these things that you see in nature in the universe, 256 00:12:56,600 --> 00:12:59,360 Speaker 4: like things that pop up and you can touch them, 257 00:12:59,360 --> 00:13:01,520 Speaker 4: and and it's a thing. 258 00:13:01,760 --> 00:13:04,240 Speaker 1: Yes, muons are a thing. They are a little thing. 259 00:13:04,559 --> 00:13:07,880 Speaker 1: There are particles, and they are little dots of matter. 260 00:13:08,120 --> 00:13:10,760 Speaker 1: They have mass and they have charge and they interact. 261 00:13:10,800 --> 00:13:13,920 Speaker 4: Okay, so it's a particle like the electron. But you're 262 00:13:13,920 --> 00:13:16,600 Speaker 4: saying and you say, it's a cousin of the electron, 263 00:13:16,760 --> 00:13:20,319 Speaker 4: not that they share like not that their parents were siblings, 264 00:13:20,400 --> 00:13:22,840 Speaker 4: but just like in the sense that it's very similar 265 00:13:23,360 --> 00:13:24,400 Speaker 4: to the electron. 266 00:13:24,640 --> 00:13:28,320 Speaker 1: Yeah, when we organize our knowledge, we look for patterns, 267 00:13:28,360 --> 00:13:30,520 Speaker 1: we look for similarities. Right like when we were one 268 00:13:30,600 --> 00:13:32,520 Speaker 1: hundred years ago, when the state of knowledge about the 269 00:13:32,600 --> 00:13:35,040 Speaker 1: universe was the periodic table. We didn't just have like 270 00:13:35,080 --> 00:13:37,439 Speaker 1: a pile of different elements and say here's an element. 271 00:13:37,480 --> 00:13:39,720 Speaker 1: There's an element. We said, oh, look, this one is 272 00:13:39,760 --> 00:13:42,560 Speaker 1: similar to that one. They're both really active, or these 273 00:13:42,600 --> 00:13:45,480 Speaker 1: are really similar because they're both really inactive, or this 274 00:13:45,520 --> 00:13:47,440 Speaker 1: one weighs a tiny bit more than that one. We 275 00:13:47,520 --> 00:13:50,560 Speaker 1: notice patterns. We put those patterns together in the same way. 276 00:13:50,600 --> 00:13:53,720 Speaker 1: We're looking for patterns in the fundamental particles. So we 277 00:13:54,040 --> 00:13:56,360 Speaker 1: try to figure out which ones are related to each other. 278 00:13:56,720 --> 00:13:59,200 Speaker 1: And we have only a few handles on each particle. 279 00:13:59,240 --> 00:14:01,000 Speaker 1: It's only like a few things we can know about 280 00:14:01,000 --> 00:14:02,000 Speaker 1: a particle. 281 00:14:02,440 --> 00:14:04,360 Speaker 4: Right, And so is this a particle that we can 282 00:14:04,480 --> 00:14:07,280 Speaker 4: see in our everyday lives, like is it floating around? 283 00:14:07,400 --> 00:14:12,960 Speaker 4: Does it move around wires and electri electricity like the electron? 284 00:14:13,080 --> 00:14:16,160 Speaker 4: Or is this kind of a weird one of those 285 00:14:16,200 --> 00:14:19,520 Speaker 4: weird particles? And you know you don't ever actually. 286 00:14:19,240 --> 00:14:21,800 Speaker 1: See Yeah, you don't see the muon because it doesn't 287 00:14:21,880 --> 00:14:24,760 Speaker 1: last for very long. It lives for two point two 288 00:14:24,920 --> 00:14:28,560 Speaker 1: microseconds and then it turns into an electron and some neutrinos, 289 00:14:28,720 --> 00:14:32,320 Speaker 1: but they are actually everywhere. There's ten thousand muons going 290 00:14:32,360 --> 00:14:35,240 Speaker 1: through a square meter of Earth every minute, So there's 291 00:14:35,320 --> 00:14:38,240 Speaker 1: lots of muons everywhere, but you just can't really see 292 00:14:38,240 --> 00:14:40,320 Speaker 1: them very easily because they don't last very long. 293 00:14:40,360 --> 00:14:42,360 Speaker 4: Wait wait, I mean, how can they be everywhere but 294 00:14:42,480 --> 00:14:45,920 Speaker 4: also only last two point two microseconds? Does that mean 295 00:14:45,960 --> 00:14:49,920 Speaker 4: that they're constantly coming into existence, lasting for two point 296 00:14:49,920 --> 00:14:54,760 Speaker 4: two microseconds and then disappearing and breaking up or what 297 00:14:54,760 --> 00:14:56,480 Speaker 4: does that mean? How can they be all around is 298 00:14:56,520 --> 00:14:58,320 Speaker 4: but also evaporating at the same time. 299 00:14:58,440 --> 00:15:00,280 Speaker 1: Well, there's two things going on there. One is right, 300 00:15:00,440 --> 00:15:04,360 Speaker 1: they're being created when particles hit the atmosphere. So protons 301 00:15:04,400 --> 00:15:06,600 Speaker 1: hit the atmosphere and they create a shower of particles, 302 00:15:06,640 --> 00:15:09,480 Speaker 1: some of which include muons, and those muons fly along 303 00:15:09,520 --> 00:15:11,440 Speaker 1: a little bit, but they don't last very long, just 304 00:15:11,440 --> 00:15:14,120 Speaker 1: two point two microseconds, and then they turn into electrons. 305 00:15:14,720 --> 00:15:18,120 Speaker 1: But they last for two point two microseconds according to 306 00:15:18,280 --> 00:15:22,200 Speaker 1: their clocks. Because they move really fast, there's a relativistic 307 00:15:22,280 --> 00:15:25,400 Speaker 1: time dilation, so they're according to us that two point 308 00:15:25,440 --> 00:15:29,400 Speaker 1: two microseconds takes longer to click, and so for us 309 00:15:29,440 --> 00:15:32,600 Speaker 1: it can take like seconds or minutes for muons to decay. 310 00:15:33,080 --> 00:15:35,840 Speaker 4: Oh but for them. If you were sitting on top 311 00:15:35,920 --> 00:15:39,200 Speaker 4: of the muon, mm hmm, it would only last You 312 00:15:39,240 --> 00:15:41,320 Speaker 4: would only be alive for two point two microseconds. 313 00:15:41,520 --> 00:15:43,560 Speaker 1: Yeah, that's the half life of a muon. So muon 314 00:15:43,640 --> 00:15:45,600 Speaker 1: is not stable. It's not like an electron. It can 315 00:15:45,640 --> 00:15:48,280 Speaker 1: just sit there for eons and eons and just be itself. 316 00:15:48,520 --> 00:15:50,840 Speaker 1: A muon is a heavy particle, and heavy particles like 317 00:15:50,880 --> 00:15:53,760 Speaker 1: to decay into lighter particles. In this case, the muon 318 00:15:53,840 --> 00:15:57,000 Speaker 1: turns into an electron very quickly according to its clock. 319 00:15:57,120 --> 00:15:58,960 Speaker 4: Oh, I see the ones that we see, the ones 320 00:15:58,960 --> 00:16:02,240 Speaker 4: coming from the Atmosphe are moving fast, so they last longer. 321 00:16:02,280 --> 00:16:04,560 Speaker 4: But if I just created a muon here in front 322 00:16:04,600 --> 00:16:07,080 Speaker 4: of me, it would last only for two point two microseconds, 323 00:16:07,120 --> 00:16:08,360 Speaker 4: and it's not going anywhere. 324 00:16:08,440 --> 00:16:10,640 Speaker 1: Mm hmm. If you could break muons in your oven, 325 00:16:10,920 --> 00:16:12,400 Speaker 1: you take them out of the oven two point two 326 00:16:12,400 --> 00:16:14,440 Speaker 1: microseconds later, boom they turn into election. 327 00:16:14,720 --> 00:16:16,240 Speaker 4: Yeah. Yeah, gotta eat them up real quick. 328 00:16:16,960 --> 00:16:19,320 Speaker 1: Exactly. They're like making fortune cookies or. 329 00:16:19,320 --> 00:16:21,520 Speaker 4: Toss them really fast, have them pop out of toaster 330 00:16:21,640 --> 00:16:23,760 Speaker 4: really fast, in which case it would last longer. 331 00:16:23,960 --> 00:16:28,200 Speaker 1: Technically, right, that's true, Yeah, exactly. Somebody could shoot muons 332 00:16:28,200 --> 00:16:30,240 Speaker 1: into your mouth and it would last long enough to 333 00:16:30,280 --> 00:16:32,440 Speaker 1: get there. I wouldn't recommend that though, that's not a 334 00:16:32,480 --> 00:16:35,320 Speaker 1: suggestion for something somebody should do. And actually two point 335 00:16:35,360 --> 00:16:37,680 Speaker 1: two microseconds is kind of a long time for a 336 00:16:37,720 --> 00:16:40,600 Speaker 1: particle that's this massive to last mm. 337 00:16:40,960 --> 00:16:42,800 Speaker 4: So what does it mean that it disappears or breaks 338 00:16:42,880 --> 00:16:47,160 Speaker 4: up like it's just unstable, like it just it's made 339 00:16:47,200 --> 00:16:49,800 Speaker 4: out of other things and it breaks up, or it 340 00:16:49,840 --> 00:16:52,960 Speaker 4: literally just kind of evaporates into energy and that energy 341 00:16:53,000 --> 00:16:53,960 Speaker 4: turns into something else. 342 00:16:54,200 --> 00:16:56,880 Speaker 1: Yeah, that's a great question. These are fundamental particles, so 343 00:16:56,880 --> 00:16:59,160 Speaker 1: they're not made up of anything else. As far as 344 00:16:59,200 --> 00:17:02,400 Speaker 1: we know. The muon turns into the electron. It's not 345 00:17:02,480 --> 00:17:04,679 Speaker 1: like it has an electron inside of it, and it 346 00:17:04,760 --> 00:17:08,199 Speaker 1: breaks up into an electron and other stuff it converts. 347 00:17:08,600 --> 00:17:11,240 Speaker 1: It goes from a muon, it turns via the weak 348 00:17:11,280 --> 00:17:15,000 Speaker 1: force into a W particle and a neutrino, and then 349 00:17:15,040 --> 00:17:18,120 Speaker 1: the W particle turns into an electron and another neutrino. 350 00:17:18,560 --> 00:17:22,919 Speaker 1: So the muon turns into an electron and two different neutrinos, 351 00:17:23,040 --> 00:17:25,359 Speaker 1: but it didn't have those bits inside of it. Remember, 352 00:17:25,400 --> 00:17:28,280 Speaker 1: particle physics is like alchemy. We can convert one kind 353 00:17:28,320 --> 00:17:30,040 Speaker 1: of matter into another kind of matter. 354 00:17:30,760 --> 00:17:34,600 Speaker 4: Okay, so it's it doesn't break apart, it's just somehow 355 00:17:34,640 --> 00:17:38,480 Speaker 4: it's very existence. The universe sort of doesn't like it, 356 00:17:38,520 --> 00:17:42,120 Speaker 4: like it it can It just ceazes to exist and 357 00:17:42,160 --> 00:17:45,080 Speaker 4: in favor of other things existing instead of it. 358 00:17:45,200 --> 00:17:47,800 Speaker 1: Yeah, and this is true for every particle that is 359 00:17:47,880 --> 00:17:51,359 Speaker 1: pretty massive. The universe doesn't like massive particles. It's like 360 00:17:51,600 --> 00:17:53,680 Speaker 1: putting a particle on the top of a hill. Eventually 361 00:17:53,720 --> 00:17:56,320 Speaker 1: it's going to roll down. And so the muon is 362 00:17:56,359 --> 00:17:58,040 Speaker 1: like the at the top of the hill, and the 363 00:17:58,040 --> 00:18:00,320 Speaker 1: electron is rolling down to the bottom of the hill. 364 00:18:00,320 --> 00:18:02,800 Speaker 1: Eventually the mion is going to turn into the electron. 365 00:18:03,440 --> 00:18:06,639 Speaker 1: And every particle in nature that can do this does this. 366 00:18:06,760 --> 00:18:08,679 Speaker 1: The only reason the electron doesn't is that there's no 367 00:18:09,040 --> 00:18:10,680 Speaker 1: lighter particle for it to turn into. 368 00:18:11,520 --> 00:18:16,040 Speaker 4: Oh, and that's why we are able to exist, because yes, 369 00:18:16,440 --> 00:18:21,080 Speaker 4: the universe does seem to like electrons and quarks, which 370 00:18:21,200 --> 00:18:23,840 Speaker 4: make us up, and so that's why we're stable. But 371 00:18:23,920 --> 00:18:26,160 Speaker 4: if we were made out of neons, we would disappear 372 00:18:26,200 --> 00:18:26,840 Speaker 4: pretty quickly. 373 00:18:27,040 --> 00:18:29,720 Speaker 1: Yes, exactly. We are made up of the lightest particles 374 00:18:29,760 --> 00:18:31,879 Speaker 1: out there, up quarks and down quarks. Of the lightest 375 00:18:31,920 --> 00:18:34,919 Speaker 1: quarks electrons of the lightest version of that kind of 376 00:18:34,920 --> 00:18:37,639 Speaker 1: particle called e lepton. So the matter that makes us 377 00:18:37,720 --> 00:18:40,000 Speaker 1: up that stable is made out of stuff that can't 378 00:18:40,040 --> 00:18:42,920 Speaker 1: turn into lighter stuff because there is no lighter stuff 379 00:18:42,920 --> 00:18:43,720 Speaker 1: for it to turn into. 380 00:18:44,240 --> 00:18:47,200 Speaker 4: Right, Yeah, there's nothing for it to turn into, so 381 00:18:47,200 --> 00:18:50,600 Speaker 4: we stay where we are. But a meon is heavy 382 00:18:50,640 --> 00:18:52,120 Speaker 4: and could turn into something else. 383 00:18:52,160 --> 00:18:54,800 Speaker 1: So it does precisely. And for those of you wondering, like, well, 384 00:18:54,800 --> 00:18:57,120 Speaker 1: what about a photon, Why can't an electron turn into 385 00:18:57,119 --> 00:18:59,879 Speaker 1: a photon. A photon is massless, Well, remember that there 386 00:18:59,880 --> 00:19:01,879 Speaker 1: are rules about how these things happen, and one of 387 00:19:01,920 --> 00:19:05,719 Speaker 1: those rules is conservation of electric charge. An electron has 388 00:19:05,760 --> 00:19:08,440 Speaker 1: a minus one charge, so it can't turn into a photon, 389 00:19:08,480 --> 00:19:11,560 Speaker 1: which has zero charge, because you'd have to somehow disappear 390 00:19:11,640 --> 00:19:13,639 Speaker 1: that charge. The only way for that to happen is 391 00:19:13,640 --> 00:19:16,919 Speaker 1: for an electron to hit a plus one positron and 392 00:19:16,960 --> 00:19:19,240 Speaker 1: then they can turn into a photon together. But for 393 00:19:19,240 --> 00:19:22,479 Speaker 1: a particle to just spontaneously decay, it has to convert 394 00:19:22,480 --> 00:19:25,080 Speaker 1: to another particle that has all the same sort of 395 00:19:25,359 --> 00:19:26,720 Speaker 1: quantum mechanical numbers. 396 00:19:27,000 --> 00:19:31,159 Speaker 4: Okay, so the meuon is the electron's massive cousin or 397 00:19:31,560 --> 00:19:34,800 Speaker 4: massive sort of like alternate universe version of the electron. 398 00:19:34,920 --> 00:19:37,920 Speaker 1: Right, Yeah, it's two hundred times the mass of the electron. 399 00:19:38,000 --> 00:19:39,360 Speaker 1: It's really really massive. 400 00:19:39,440 --> 00:19:41,640 Speaker 4: That's a lot. It's like two hundred meters crunch into 401 00:19:41,720 --> 00:19:42,240 Speaker 4: the same meat. 402 00:19:42,520 --> 00:19:45,199 Speaker 1: Yes, exactly. It's like if you met another version of you, 403 00:19:45,280 --> 00:19:48,280 Speaker 1: but you weren't bigger, you were denser or something. You're 404 00:19:48,359 --> 00:19:51,080 Speaker 1: two hundred times as much mass, but still fundamental. 405 00:19:51,320 --> 00:19:55,080 Speaker 4: And it doesn't hang around existence very long. It usually 406 00:19:55,720 --> 00:19:58,040 Speaker 4: breaks up into or not breaks up, but it turns 407 00:19:58,040 --> 00:20:02,160 Speaker 4: into lighter particles, so we don't really seed around that much. 408 00:20:02,280 --> 00:20:04,680 Speaker 4: But still it's sort of an important part of the universe, 409 00:20:04,720 --> 00:20:06,879 Speaker 4: and it seems that it's a important part of the 410 00:20:06,960 --> 00:20:10,080 Speaker 4: universe and also tells us a lot about the mysteries 411 00:20:10,160 --> 00:20:11,560 Speaker 4: of how everything is put together. 412 00:20:11,840 --> 00:20:14,359 Speaker 1: Yeah, and it actually lasts a long time for a 413 00:20:14,440 --> 00:20:17,560 Speaker 1: heavy particle. Other particles that are heavy, like the Higgs boson, 414 00:20:17,800 --> 00:20:21,080 Speaker 1: they decay much more quickly. They decay in like ten 415 00:20:21,160 --> 00:20:25,320 Speaker 1: to the minus twenty seconds, whereas this one decays very slowly. 416 00:20:25,320 --> 00:20:28,119 Speaker 1: It's just two point two microseconds. And the reason is 417 00:20:28,160 --> 00:20:30,200 Speaker 1: that it decays via the weak force, which is very 418 00:20:30,240 --> 00:20:32,800 Speaker 1: weak to the weaker the force, the longer it takes 419 00:20:32,800 --> 00:20:33,760 Speaker 1: for that decay to happen. 420 00:20:34,680 --> 00:20:36,280 Speaker 4: All right, let's get into that a little bit more, 421 00:20:36,320 --> 00:20:39,159 Speaker 4: and also how it was discovered and why it is 422 00:20:39,240 --> 00:20:42,919 Speaker 4: such an important particle. But first, let's take a quick break. 423 00:20:47,200 --> 00:20:50,119 Speaker 1: With big wireless providers, what you see is never what 424 00:20:50,240 --> 00:20:52,960 Speaker 1: you get. 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It has to there has to 479 00:23:44,119 --> 00:23:46,679 Speaker 1: be an interaction there. And so what happens is the 480 00:23:46,760 --> 00:23:50,080 Speaker 1: muon turns into a W particle and a neutrino in 481 00:23:50,119 --> 00:23:53,439 Speaker 1: the W particle, remember, is the particle of the weak force. 482 00:23:53,640 --> 00:23:56,639 Speaker 1: It's like the weak force version of the photon. And 483 00:23:56,680 --> 00:23:58,520 Speaker 1: so that's what we mean when we say it uses 484 00:23:58,560 --> 00:24:01,560 Speaker 1: the weak force to decay. It just just spontaneously happened. 485 00:24:01,680 --> 00:24:04,159 Speaker 1: Something has to sort of carry that information, something has 486 00:24:04,200 --> 00:24:06,840 Speaker 1: to make it happen. It's like a reaction, and that 487 00:24:06,880 --> 00:24:09,680 Speaker 1: reaction always includes one of the forces. And in this case, 488 00:24:09,880 --> 00:24:11,240 Speaker 1: it uses the weak force. 489 00:24:11,160 --> 00:24:13,680 Speaker 4: Right, and that weak force came out of just its 490 00:24:13,680 --> 00:24:14,320 Speaker 4: own energy. 491 00:24:14,440 --> 00:24:16,440 Speaker 1: It uses the mass. Right. The muon has a huge 492 00:24:16,440 --> 00:24:18,560 Speaker 1: amount of energy in it because it has so much mass, 493 00:24:18,880 --> 00:24:21,159 Speaker 1: and that mass is turned into the energy of the 494 00:24:21,200 --> 00:24:24,400 Speaker 1: electron and the neutrinos that come out of it. So yeah, 495 00:24:24,400 --> 00:24:27,240 Speaker 1: the weak force turns the mass of the muon into 496 00:24:27,640 --> 00:24:30,239 Speaker 1: very small masses of these other particles and gives them 497 00:24:30,240 --> 00:24:31,320 Speaker 1: a lot of energy. 498 00:24:31,119 --> 00:24:34,120 Speaker 4: Right, and it ends up as an electron and two 499 00:24:34,280 --> 00:24:37,639 Speaker 4: neutrinos precisely. All right, Well, tell us Daniel, how was 500 00:24:37,680 --> 00:24:40,080 Speaker 4: it discovered and why is this an important particle? 501 00:24:40,160 --> 00:24:44,240 Speaker 1: Well, it was discovered initially in cosmic rays. People saw 502 00:24:44,320 --> 00:24:47,320 Speaker 1: these particles just sort of shooting from the sky, and 503 00:24:47,359 --> 00:24:50,320 Speaker 1: they didn't understand what was making them, and they thought, oh, well, 504 00:24:50,480 --> 00:24:52,360 Speaker 1: you know, we found a few particles, so these are 505 00:24:52,359 --> 00:24:55,640 Speaker 1: probably electrons. This is you know, in the early nineteen hundreds, 506 00:24:55,640 --> 00:24:59,159 Speaker 1: we didn't have a really deep understanding of how particles work. 507 00:24:59,240 --> 00:25:01,879 Speaker 1: We didn't have a good bench of particles, and so 508 00:25:02,480 --> 00:25:04,840 Speaker 1: people thought, you know, everything they saw they thought in 509 00:25:04,920 --> 00:25:06,520 Speaker 1: terms of the particles at the time. So they have 510 00:25:06,560 --> 00:25:08,920 Speaker 1: to sort of wind your mind back to what we 511 00:25:09,000 --> 00:25:11,960 Speaker 1: knew at the time. Back then, we knew about protons, 512 00:25:12,040 --> 00:25:14,719 Speaker 1: we knew about neutrons, we knew about electrons, and so 513 00:25:14,760 --> 00:25:17,600 Speaker 1: people saw these particles shooting from the sky. They didn't 514 00:25:17,600 --> 00:25:19,560 Speaker 1: know what made them, but what they saw was that 515 00:25:19,560 --> 00:25:23,800 Speaker 1: they penetrated really far into matter, much more than electrons could. 516 00:25:24,600 --> 00:25:27,840 Speaker 4: We saw the actual muons, the not what it looks 517 00:25:27,920 --> 00:25:31,520 Speaker 4: like after it decays or turns into something else, like 518 00:25:31,560 --> 00:25:34,440 Speaker 4: we actually you can actually see and feel the muons. 519 00:25:34,520 --> 00:25:36,520 Speaker 1: You can't really feel them, but you can make particle 520 00:25:36,560 --> 00:25:38,879 Speaker 1: detectors that can detect them. You can actually do this 521 00:25:38,960 --> 00:25:41,879 Speaker 1: in your garage using something called a cloud chamber. They 522 00:25:41,880 --> 00:25:44,280 Speaker 1: were able to see them using detectors that they put together. 523 00:25:44,320 --> 00:25:47,040 Speaker 1: And these detectors were like a cubic piece of film, 524 00:25:47,240 --> 00:25:50,000 Speaker 1: like remember the old way films worked, where like light 525 00:25:50,119 --> 00:25:52,000 Speaker 1: was exposed on the film. You didn't have a digital 526 00:25:52,040 --> 00:25:53,000 Speaker 1: camera or anything. 527 00:25:52,720 --> 00:25:54,920 Speaker 4: And that made some kind of chemical change. You're saying, 528 00:25:54,960 --> 00:25:56,800 Speaker 4: you can make like a solid cube of this. 529 00:25:57,040 --> 00:25:58,960 Speaker 1: Yeah, you just take a solid cube of it, You 530 00:25:59,080 --> 00:26:01,480 Speaker 1: leave it up on a mount and you leave it 531 00:26:01,480 --> 00:26:03,399 Speaker 1: there for like six months, and then you cart it 532 00:26:03,440 --> 00:26:05,679 Speaker 1: back down, or you ask your grad students to do that. 533 00:26:05,840 --> 00:26:08,000 Speaker 1: Then you slice it into pieces and then you can 534 00:26:08,040 --> 00:26:09,800 Speaker 1: develop each of those. And what you do is you 535 00:26:09,840 --> 00:26:12,480 Speaker 1: see all the particles that shot through it in those 536 00:26:12,480 --> 00:26:15,760 Speaker 1: six months, and so they can see and when they 537 00:26:15,760 --> 00:26:19,080 Speaker 1: did this, they saw all these particles shooting through this 538 00:26:19,160 --> 00:26:21,600 Speaker 1: film and they were surprised at how far they were 539 00:26:21,640 --> 00:26:25,199 Speaker 1: going because electrons shouldn't get that far. Electrons penetrate in 540 00:26:25,200 --> 00:26:27,400 Speaker 1: a little bit and then they stop. But these particles 541 00:26:27,400 --> 00:26:28,800 Speaker 1: were shooting all the way through. 542 00:26:29,920 --> 00:26:32,200 Speaker 4: It's kind of like a bull in a china shop, 543 00:26:33,000 --> 00:26:34,840 Speaker 4: you know, versus like a mouse in a china shop. 544 00:26:35,040 --> 00:26:37,239 Speaker 1: Yeah, And they didn't understand that. They thought, well, you know, 545 00:26:37,320 --> 00:26:40,720 Speaker 1: are there two kinds of electrons are there. Sometimes electrons 546 00:26:40,880 --> 00:26:43,359 Speaker 1: can penetrate really far. It was really a puzzle at 547 00:26:43,359 --> 00:26:43,840 Speaker 1: the time. 548 00:26:43,760 --> 00:26:45,919 Speaker 4: What made them think it was an electron. Why couldn't 549 00:26:45,920 --> 00:26:48,879 Speaker 4: it be like a some kind of new atom or something. 550 00:26:48,960 --> 00:26:51,080 Speaker 1: We did know it had negative charge, and so I 551 00:26:51,119 --> 00:26:53,560 Speaker 1: think that's what made people think it was more likely 552 00:26:53,600 --> 00:26:56,400 Speaker 1: to be an electron or something like an electron than 553 00:26:56,440 --> 00:26:59,360 Speaker 1: something positive like inside the nucleus. And remember, at the time, 554 00:26:59,359 --> 00:27:02,760 Speaker 1: we only knew basically about protons, neutrons, and electrons, and 555 00:27:02,840 --> 00:27:05,080 Speaker 1: so everything we saw where like all of a sudden, 556 00:27:05,280 --> 00:27:07,919 Speaker 1: having this imagination that we could explain everything in the 557 00:27:08,000 --> 00:27:10,639 Speaker 1: universe in terms of these particles. And it was a 558 00:27:10,680 --> 00:27:13,000 Speaker 1: great success of the particle model at the time, right, 559 00:27:13,080 --> 00:27:16,040 Speaker 1: like everything could be built out of protons, neutrons, and electrons. 560 00:27:16,040 --> 00:27:18,960 Speaker 1: What a wonderful simplification. And so when we first saw 561 00:27:19,000 --> 00:27:21,399 Speaker 1: these particles that penetrated really far, we thought, well, it 562 00:27:21,480 --> 00:27:24,600 Speaker 1: must be one of those, right, But it was not. 563 00:27:25,040 --> 00:27:28,320 Speaker 1: It was not. And people were able to later produce 564 00:27:28,400 --> 00:27:31,600 Speaker 1: it in the laboratory using collisions and all sorts of 565 00:27:31,600 --> 00:27:34,359 Speaker 1: other stuff, and they discovered that if you put it 566 00:27:34,400 --> 00:27:36,800 Speaker 1: in a magnetic field, it didn't bend as much as 567 00:27:36,800 --> 00:27:39,280 Speaker 1: an electron, and that's when they decided, you know what, 568 00:27:39,359 --> 00:27:41,240 Speaker 1: this must be a different kind of thing. It's like 569 00:27:41,280 --> 00:27:44,520 Speaker 1: a new version of the electron, a different flavor of 570 00:27:44,560 --> 00:27:46,840 Speaker 1: the electron, because it must be more massive, which is 571 00:27:46,880 --> 00:27:49,560 Speaker 1: why it doesn't bend inside the magnetic. 572 00:27:49,240 --> 00:27:51,800 Speaker 4: Field as much, reflected as much because it has so 573 00:27:51,880 --> 00:27:54,800 Speaker 4: much mass. It just has more inertia. 574 00:27:54,840 --> 00:27:57,760 Speaker 1: Precisely, it takes a stronger magnetic field to bend a 575 00:27:57,840 --> 00:28:00,439 Speaker 1: muon than it does for an electron. And this was 576 00:28:00,560 --> 00:28:03,240 Speaker 1: kind of a scandal in particle physics at the time. 577 00:28:03,600 --> 00:28:04,119 Speaker 4: Scandal. 578 00:28:04,320 --> 00:28:07,000 Speaker 1: Yeah, people were upset. They were like, what a muon? 579 00:28:07,200 --> 00:28:10,240 Speaker 1: Who ordered that? Like, we don't need this. We get 580 00:28:10,240 --> 00:28:12,199 Speaker 1: out of here with your ridiculous new particle. We have 581 00:28:12,320 --> 00:28:15,680 Speaker 1: this beautiful description of the universe. We don't want more particles. 582 00:28:16,119 --> 00:28:20,000 Speaker 4: Up until then, everything that you knew about helped make 583 00:28:20,040 --> 00:28:22,480 Speaker 4: the universe. It's kind of what you're saying, like everything 584 00:28:22,600 --> 00:28:24,160 Speaker 4: you knew about had a purpose. 585 00:28:24,280 --> 00:28:26,399 Speaker 1: Yeah, we had taken apart the stuff around us and 586 00:28:26,480 --> 00:28:29,399 Speaker 1: found the basic building blocks, and then we didn't. Some 587 00:28:29,440 --> 00:28:31,320 Speaker 1: people were like, I don't want to hear stories about 588 00:28:31,359 --> 00:28:33,240 Speaker 1: other building blocks that could be out there. It just 589 00:28:33,280 --> 00:28:36,520 Speaker 1: sort of confuses the issue, right, it's a shift in 590 00:28:36,520 --> 00:28:38,600 Speaker 1: the question not just what we made out of, but 591 00:28:38,840 --> 00:28:41,560 Speaker 1: what is the basic organizing principle of the universe. It 592 00:28:41,640 --> 00:28:43,840 Speaker 1: shows you all of a sudden that there's a larger 593 00:28:43,920 --> 00:28:45,720 Speaker 1: question you didn't even think to ask. 594 00:28:46,160 --> 00:28:47,800 Speaker 4: It's like you find something that you don't know what 595 00:28:47,840 --> 00:28:51,040 Speaker 4: to do with it, Like it doesn't help you with 596 00:28:51,120 --> 00:28:53,200 Speaker 4: what you knew about how things work. 597 00:28:53,440 --> 00:28:55,920 Speaker 1: Yeah, you're putting together jigsaw puzzle and all of a sudden, 598 00:28:55,960 --> 00:28:58,080 Speaker 1: somebody hands you like a really big piece that just 599 00:28:58,120 --> 00:29:01,720 Speaker 1: doesn't fit, and you're like, what I didn't ask for, 600 00:29:01,760 --> 00:29:04,880 Speaker 1: that I don't need, That doesn't help me with my problem, Like, well, 601 00:29:04,920 --> 00:29:06,560 Speaker 1: but okay, but this piece is here and it's not 602 00:29:06,640 --> 00:29:07,440 Speaker 1: going away. 603 00:29:07,640 --> 00:29:10,080 Speaker 4: Right, Yeah, And so it makes you think that maybe 604 00:29:10,120 --> 00:29:13,320 Speaker 4: there's another puzzle, or that the puzzle is bigger than 605 00:29:13,360 --> 00:29:13,920 Speaker 4: you think it is. 606 00:29:15,000 --> 00:29:17,000 Speaker 1: Yes, all of a sudden you realize this is a 607 00:29:17,040 --> 00:29:20,400 Speaker 1: three dimensional puzzle and you've been only playing on two dimensions, 608 00:29:20,400 --> 00:29:23,880 Speaker 1: and it just blows your mind. And so that's it's 609 00:29:23,920 --> 00:29:27,400 Speaker 1: sort of an earthquake, an intellectual earthquake through the field 610 00:29:27,400 --> 00:29:29,680 Speaker 1: at the moment. But also it's a great opportunity. Those 611 00:29:29,720 --> 00:29:32,880 Speaker 1: are the kind of discoveries that make you realize, Wow, 612 00:29:32,920 --> 00:29:35,440 Speaker 1: there's a whole larger question to ask, and there's a 613 00:29:35,440 --> 00:29:38,320 Speaker 1: whole world of answers out there. And of course now 614 00:29:38,360 --> 00:29:40,480 Speaker 1: we know there's not just the mew on, this also 615 00:29:40,480 --> 00:29:43,120 Speaker 1: the tao, which is the even heavier version of it, 616 00:29:43,320 --> 00:29:45,920 Speaker 1: and then every particle has these cousins. Yeah. 617 00:29:46,000 --> 00:29:48,240 Speaker 4: I like how this counts as a scandal in physics, 618 00:29:48,800 --> 00:29:50,800 Speaker 4: Like was it on the front page of the Daily 619 00:29:51,240 --> 00:29:59,000 Speaker 4: Physics News or the National Inquiring Inquirer of physics newspapers? 620 00:29:59,360 --> 00:30:01,160 Speaker 1: People have to all the tabloids. 621 00:30:01,240 --> 00:30:05,840 Speaker 4: People had to give testimony about this, and there were. 622 00:30:05,920 --> 00:30:07,880 Speaker 1: You know, physicists are not that exciting, so we just 623 00:30:07,920 --> 00:30:10,520 Speaker 1: got to create drama wherever we can see. There was 624 00:30:10,560 --> 00:30:14,240 Speaker 1: even more drama because some people had predicted the existence 625 00:30:14,240 --> 00:30:16,280 Speaker 1: of a particle sort of similar to this. 626 00:30:17,120 --> 00:30:20,200 Speaker 4: Hmmm, what do you mean predicted like just just guessing. 627 00:30:20,520 --> 00:30:23,360 Speaker 1: Yeah. Well, there was a famous physicist named Yukaba the 628 00:30:23,440 --> 00:30:25,520 Speaker 1: Genius and won a Nobel Prize for all sorts of 629 00:30:25,600 --> 00:30:29,400 Speaker 1: fascinating stuff, and he was trying to understand the strong force. 630 00:30:29,480 --> 00:30:32,080 Speaker 1: He was like, okay, the weak force, we have that one. 631 00:30:32,120 --> 00:30:36,320 Speaker 1: We have the photon for the electromagnetism, but what mediates 632 00:30:36,360 --> 00:30:39,000 Speaker 1: the strong force? And he did some calculations that he thought, hmm, 633 00:30:39,480 --> 00:30:42,400 Speaker 1: I bet there's a particle out there about two hundred 634 00:30:42,480 --> 00:30:45,480 Speaker 1: times the mass of the electron and it mediates the 635 00:30:45,560 --> 00:30:48,480 Speaker 1: strong force, all right, So that's his prediction, right, And 636 00:30:48,520 --> 00:30:50,640 Speaker 1: back in the day, physics would just make predictions like 637 00:30:50,840 --> 00:30:53,120 Speaker 1: here's my idea and here's what I predict. 638 00:30:52,920 --> 00:30:54,880 Speaker 4: Like we need this for this for what we know 639 00:30:55,160 --> 00:30:56,040 Speaker 4: to make sense. 640 00:30:56,320 --> 00:30:58,680 Speaker 1: Yeah, just like with the Higgs boson, Peter Higgs said, 641 00:30:58,880 --> 00:31:01,360 Speaker 1: this doesn't make sense to me, but if you look 642 00:31:01,360 --> 00:31:03,240 Speaker 1: at the universe in a new way, then it makes 643 00:31:03,240 --> 00:31:05,800 Speaker 1: more sense. And this new way predicts a new particle, 644 00:31:05,840 --> 00:31:07,840 Speaker 1: so you can test my theory. So that was what 645 00:31:07,920 --> 00:31:11,080 Speaker 1: Yukawa did, and he predicted a new particle about two 646 00:31:11,160 --> 00:31:13,920 Speaker 1: hundred times the mass of the electron. Then they found 647 00:31:14,000 --> 00:31:16,800 Speaker 1: this particle and Yukawa was like, whoo, I was right. 648 00:31:17,280 --> 00:31:19,520 Speaker 1: But it turns out this particle has nothing to do 649 00:31:19,560 --> 00:31:21,840 Speaker 1: with this strong force at all. So it's just like 650 00:31:21,880 --> 00:31:25,120 Speaker 1: a coincidence, right, And he still got the Nobel Prize. 651 00:31:25,360 --> 00:31:27,760 Speaker 1: He still got the Nobel Prize, but not for this 652 00:31:28,160 --> 00:31:30,479 Speaker 1: and not for this one. But he's sort of the 653 00:31:30,560 --> 00:31:33,360 Speaker 1: reason why this particle has a strange name. 654 00:31:33,920 --> 00:31:36,680 Speaker 4: Oh really, he was a fan of cows. 655 00:31:37,760 --> 00:31:40,000 Speaker 1: I don't know if he liked Kobe Beef, you know, 656 00:31:40,000 --> 00:31:42,680 Speaker 1: the guy's Japanese or anything, but he you know, we 657 00:31:42,720 --> 00:31:44,800 Speaker 1: had the electron, which is really really light, and we 658 00:31:44,840 --> 00:31:47,760 Speaker 1: had the proton, which is like two thousand times the 659 00:31:47,760 --> 00:31:50,320 Speaker 1: mass of the electron, and he predicted a particle sort 660 00:31:50,320 --> 00:31:53,640 Speaker 1: of at an intermediate mass, and so he wanted it 661 00:31:53,720 --> 00:31:57,360 Speaker 1: called like the you know, the mesotron something where mazo 662 00:31:57,440 --> 00:32:00,720 Speaker 1: means like middle, and so that was the sort of 663 00:32:00,760 --> 00:32:03,880 Speaker 1: the origin of this, like, let's call these particles here, 664 00:32:04,440 --> 00:32:07,560 Speaker 1: you know, in this mass region, we'll call the meso particles. 665 00:32:07,720 --> 00:32:09,360 Speaker 4: Wow, what don't you have to call it the messo 666 00:32:09,520 --> 00:32:14,920 Speaker 4: on or meson on or I feel like, just to 667 00:32:14,960 --> 00:32:15,840 Speaker 4: be consistent here. 668 00:32:17,320 --> 00:32:19,240 Speaker 1: And then later people were like, well, it's not just 669 00:32:19,360 --> 00:32:21,560 Speaker 1: really have anything to do with these other particles that 670 00:32:21,640 --> 00:32:23,640 Speaker 1: we found in the same mass, but we'll just keep 671 00:32:23,680 --> 00:32:25,600 Speaker 1: calling it the muon anyway. 672 00:32:25,280 --> 00:32:27,080 Speaker 4: Right, I bet you wanted to call it the meon. 673 00:32:28,920 --> 00:32:30,520 Speaker 1: Yeah, I'm so smart on. 674 00:32:30,720 --> 00:32:36,400 Speaker 4: Yeah, but this is where like, come on, dude. 675 00:32:36,640 --> 00:32:39,200 Speaker 1: But it's a it's a fascinating moment in physics because. 676 00:32:39,160 --> 00:32:42,560 Speaker 4: Like the or the yuon is themeon, how about we 677 00:32:42,600 --> 00:32:44,520 Speaker 4: call it the miuon done compromise. 678 00:32:46,840 --> 00:32:49,200 Speaker 1: That's exactly how these decisions get made, and that's why 679 00:32:49,520 --> 00:32:51,720 Speaker 1: we have such terrible names for particles. 680 00:32:52,000 --> 00:32:54,120 Speaker 4: Yeah, so, but now it's so it's not a well 681 00:32:54,160 --> 00:32:56,920 Speaker 4: known thing, like everyone knows about muon's. Do they know 682 00:32:56,960 --> 00:32:59,680 Speaker 4: that they're there? And you can study them? You can, 683 00:33:00,160 --> 00:33:03,320 Speaker 4: you can. They're going through our bodies right now at 684 00:33:03,400 --> 00:33:05,120 Speaker 4: ten thousand times per minute. 685 00:33:05,240 --> 00:33:08,400 Speaker 1: Yeah, ten thousand muons per square meter per minute. And 686 00:33:08,440 --> 00:33:10,959 Speaker 1: you're right. At first it was totally exotic and what 687 00:33:11,040 --> 00:33:13,160 Speaker 1: is this weird thing? And now we know it's a 688 00:33:13,200 --> 00:33:17,160 Speaker 1: relative of the electron, but also created another field, which 689 00:33:17,160 --> 00:33:19,880 Speaker 1: is cosmic ray physics. It was the first cosmic ray scene. 690 00:33:20,200 --> 00:33:22,280 Speaker 1: And at first people weren't sure, like where are these 691 00:33:22,320 --> 00:33:24,920 Speaker 1: particles coming from? We know they're coming down from the sky, 692 00:33:25,080 --> 00:33:27,680 Speaker 1: but are they made in the sky or whatever? And 693 00:33:27,760 --> 00:33:30,840 Speaker 1: people did all these crazy experiments, like balloon experiments where 694 00:33:30,840 --> 00:33:34,480 Speaker 1: they shot detectors up into the atmosphere with balloons and 695 00:33:34,560 --> 00:33:37,040 Speaker 1: discovered that the higher up you go, the more muons 696 00:33:37,120 --> 00:33:39,760 Speaker 1: there are, and that tells you that like muons are 697 00:33:39,800 --> 00:33:42,720 Speaker 1: being created in the upper atmosphere, and then they're decaying 698 00:33:42,760 --> 00:33:45,520 Speaker 1: as they sort of come down to Earth. And finally 699 00:33:45,560 --> 00:33:48,440 Speaker 1: people put together this picture that like particles were hitting 700 00:33:48,480 --> 00:33:51,160 Speaker 1: the top of the atmosphere and creating these showers of particles, 701 00:33:51,200 --> 00:33:53,160 Speaker 1: and we were just sort of picking up the little 702 00:33:53,200 --> 00:33:55,480 Speaker 1: last bits of the fireworks as they hit the surface. 703 00:33:55,840 --> 00:33:59,280 Speaker 4: Right. I bet they'd also try to shoot a cout 704 00:33:59,360 --> 00:34:02,360 Speaker 4: to the moon. That's really inspiration. 705 00:34:02,640 --> 00:34:04,480 Speaker 1: Well, you know how the Russians put a dog in 706 00:34:04,480 --> 00:34:07,400 Speaker 1: one of their first attempts to go to space. I 707 00:34:07,440 --> 00:34:10,040 Speaker 1: won't comment as to whether particle physicists ever used a 708 00:34:10,080 --> 00:34:11,359 Speaker 1: weather balloon to launch a cow. 709 00:34:11,560 --> 00:34:14,239 Speaker 4: Yeah, they're like, we gotta up those Russians a dog. 710 00:34:14,920 --> 00:34:19,520 Speaker 4: Anyone can launch a dog into space. Law. 711 00:34:19,840 --> 00:34:22,200 Speaker 1: This is this is well before the space race. This 712 00:34:22,239 --> 00:34:24,319 Speaker 1: is the cow race. But I love thinking about what 713 00:34:24,320 --> 00:34:26,239 Speaker 1: it must have been to be a physicist at that 714 00:34:26,280 --> 00:34:29,000 Speaker 1: time and to it like crack open a whole new 715 00:34:29,120 --> 00:34:33,480 Speaker 1: era of discovery by by you know, putting photographic plates 716 00:34:33,560 --> 00:34:35,879 Speaker 1: up on mountains and just seeing like what's up there. 717 00:34:36,120 --> 00:34:39,000 Speaker 1: There's so many amazing things to discover. Someone like new 718 00:34:39,040 --> 00:34:41,960 Speaker 1: world were opened up. They discover that all this invisible 719 00:34:42,000 --> 00:34:44,799 Speaker 1: stuff is happening around us. That's really wonderful to sort 720 00:34:44,800 --> 00:34:46,960 Speaker 1: of like crack open a new way of looking at 721 00:34:46,960 --> 00:34:47,560 Speaker 1: the universe. 722 00:34:47,760 --> 00:34:50,319 Speaker 4: Yeah, all right, let's get into the last bit here, 723 00:34:50,360 --> 00:34:53,200 Speaker 4: which is what does the muon teaches? What does it 724 00:34:53,280 --> 00:34:56,560 Speaker 4: tell us about how the universe is put together? But first, 725 00:34:56,640 --> 00:34:58,000 Speaker 4: let's take another quick break. 726 00:35:02,560 --> 00:35:04,360 Speaker 1: When you pop a piece of cheese into your mouth, 727 00:35:04,440 --> 00:35:07,600 Speaker 1: or enjoy a rich spoonful of Greek yogurt, you're probably 728 00:35:07,640 --> 00:35:11,720 Speaker 1: not thinking about the environmental impact of each and every bite. 729 00:35:11,719 --> 00:35:14,320 Speaker 1: But the people in the dairy industry are. US dairy 730 00:35:14,360 --> 00:35:18,680 Speaker 1: has set themselves some ambitious sustainability goals, including being greenhouse 731 00:35:18,680 --> 00:35:21,279 Speaker 1: gas neutral by twenty to fifty. That's why they're working 732 00:35:21,280 --> 00:35:23,640 Speaker 1: hard every day to find new ways to reduce waste, 733 00:35:23,719 --> 00:35:27,919 Speaker 1: conserve natural resources, and drive down greenhouse gas emissions. Take water, 734 00:35:27,960 --> 00:35:31,560 Speaker 1: for example, most dairy farms reuse water up to four times. 735 00:35:31,600 --> 00:35:35,000 Speaker 1: The same water cools the milk, cleans equipment, washes the barn, 736 00:35:35,080 --> 00:35:38,800 Speaker 1: and irrigates the crops. How is US dairy tackling greenhouse gases? 737 00:35:38,840 --> 00:35:41,839 Speaker 1: Many farms use anaerobic digestors that turn the methane from 738 00:35:41,840 --> 00:35:45,239 Speaker 1: maneure into renewable energy that can power farms, towns, and 739 00:35:45,280 --> 00:35:47,520 Speaker 1: electric cars. So the next time you grab a slice 740 00:35:47,560 --> 00:35:49,440 Speaker 1: of pizza or lick an ice cream cone, know that 741 00:35:49,520 --> 00:35:52,160 Speaker 1: dairy farmers and processors around the country are using the 742 00:35:52,239 --> 00:35:56,000 Speaker 1: latest practices and innovations to provide the nutrient dense dairy 743 00:35:56,000 --> 00:35:59,040 Speaker 1: products we love with less of an impact. Visit Usdairy 744 00:35:59,080 --> 00:36:01,600 Speaker 1: dot com slash this ability to learn more. 745 00:36:01,520 --> 00:36:05,120 Speaker 6: With the United Explorer Card. 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Navy Federal is ensured by 772 00:37:22,520 --> 00:37:24,520 Speaker 5: NCUA Equal Housing Lender Membership. 773 00:37:24,560 --> 00:37:26,000 Speaker 1: Required terms and conditions apply. 774 00:37:26,120 --> 00:37:28,719 Speaker 5: Loan subject to approval. Call one eight eight eight four 775 00:37:28,719 --> 00:37:31,080 Speaker 5: two sixty three two waight for details about credit costs. 776 00:37:39,680 --> 00:37:42,600 Speaker 4: All right, Danio, So the muon is a thing. It's there. 777 00:37:43,560 --> 00:37:47,160 Speaker 4: It's super massive. It looks just like the electron. We 778 00:37:47,239 --> 00:37:50,239 Speaker 4: can feel it. It's going through us right now. Why 779 00:37:50,320 --> 00:37:52,960 Speaker 4: is it there? That's the question that maybe a lot 780 00:37:53,000 --> 00:37:55,000 Speaker 4: of people have. I mean, we don't need the muon 781 00:37:55,120 --> 00:37:59,040 Speaker 4: to make iPhones or pizzash, So why is it there? 782 00:37:59,200 --> 00:38:01,640 Speaker 1: Is that the standard upon which we judge things. Now, 783 00:38:02,080 --> 00:38:04,040 Speaker 1: if you don't need you for iPhones or pizzas, you 784 00:38:04,080 --> 00:38:05,000 Speaker 1: don't need to exist. 785 00:38:05,360 --> 00:38:06,560 Speaker 4: What else is there? Daniel? 786 00:38:08,800 --> 00:38:15,799 Speaker 1: That's my whole life basic. I just keeps No. It's 787 00:38:15,800 --> 00:38:17,920 Speaker 1: a good question. It's a question i'd like to know 788 00:38:17,960 --> 00:38:20,960 Speaker 1: the answer to. Why does the muon exist? The short 789 00:38:21,040 --> 00:38:22,680 Speaker 1: version of the answer is the title of a great 790 00:38:22,680 --> 00:38:25,240 Speaker 1: book I read last year. It's called we have No Idea? 791 00:38:25,719 --> 00:38:28,440 Speaker 1: Because we really do have no idea Why the muon 792 00:38:28,520 --> 00:38:28,839 Speaker 1: is there? 793 00:38:29,080 --> 00:38:32,239 Speaker 4: Doesn't seem to be used for anything, is what you're saying. 794 00:38:32,320 --> 00:38:35,000 Speaker 4: Like the trinos, I think, also are there, but we 795 00:38:35,040 --> 00:38:36,640 Speaker 4: don't know why why they're there? Right? 796 00:38:36,760 --> 00:38:39,560 Speaker 1: Yeah, neutrinos and muons and many of the other particles 797 00:38:39,680 --> 00:38:42,279 Speaker 1: are not part of the atom. You know, build them. 798 00:38:42,360 --> 00:38:43,960 Speaker 1: You don't use them to build up the stuff that 799 00:38:44,000 --> 00:38:46,640 Speaker 1: we're familiar with, but they sort of can exist. They're 800 00:38:46,680 --> 00:38:49,479 Speaker 1: on nature's menu. You might ask the same question about 801 00:38:49,520 --> 00:38:51,920 Speaker 1: like some of the really heavy elements, like why is 802 00:38:51,920 --> 00:38:56,240 Speaker 1: plutonium a thing? Well, it turns out you can assemble 803 00:38:56,320 --> 00:38:59,080 Speaker 1: protons and neutrons and electrons in this way that's stable 804 00:38:59,120 --> 00:39:00,600 Speaker 1: and hangs out and it does this is funny thing. 805 00:39:00,600 --> 00:39:03,680 Speaker 4: We call it plutonium, and plutonium also decays, right, it 806 00:39:03,800 --> 00:39:07,120 Speaker 4: like breaks up. This one actually breaks up into other things. 807 00:39:07,160 --> 00:39:10,120 Speaker 4: But it's also kind of ephemeral, like it's only there 808 00:39:11,000 --> 00:39:13,359 Speaker 4: for so long before it becomes something else. 809 00:39:13,560 --> 00:39:17,400 Speaker 1: Precisely, and in the same way, we organize our list 810 00:39:17,480 --> 00:39:19,760 Speaker 1: of particles, and we wonder, like, why are these there? 811 00:39:19,960 --> 00:39:23,680 Speaker 1: What does this tell us about? Maybe one deeper layer 812 00:39:23,719 --> 00:39:26,759 Speaker 1: of reality, Like maybe the muons and the electrons are 813 00:39:26,760 --> 00:39:29,880 Speaker 1: made out of smaller particles, and these are just like 814 00:39:29,960 --> 00:39:34,239 Speaker 1: different ways to assemble those little internal bits, right, And 815 00:39:34,280 --> 00:39:36,160 Speaker 1: there's a few ways to assemble them, the way that 816 00:39:36,320 --> 00:39:38,520 Speaker 1: there's a few ways to assemble protons and neutrons to 817 00:39:38,560 --> 00:39:41,200 Speaker 1: get different elements. Maybe there's a few ways to assemble 818 00:39:41,239 --> 00:39:44,000 Speaker 1: these little tinyons. One way is to get an electron, 819 00:39:44,040 --> 00:39:45,840 Speaker 1: and other ways to get a muon, other ways to 820 00:39:45,840 --> 00:39:48,200 Speaker 1: get a tao, which is the third member of that family. 821 00:39:48,600 --> 00:39:50,920 Speaker 1: We just don't know. We know it's a clue though, right, 822 00:39:50,960 --> 00:39:54,080 Speaker 1: It's a tantalizing clue that there's something going on here. 823 00:39:54,080 --> 00:39:55,280 Speaker 1: We just don't know what it means. 824 00:39:55,640 --> 00:39:58,879 Speaker 4: It's a clue as to some sort of a hint 825 00:39:58,920 --> 00:40:01,760 Speaker 4: that there's some sort of rule for how electrons exist, 826 00:40:01,880 --> 00:40:04,480 Speaker 4: Like if you can make an electron that's heavier, maybe 827 00:40:04,480 --> 00:40:09,160 Speaker 4: that tells you something about what makes an electron an electron. 828 00:40:08,840 --> 00:40:11,040 Speaker 1: Precisely, and why there are three of them tells you 829 00:40:11,080 --> 00:40:13,520 Speaker 1: something about how that rule has to play out. Because 830 00:40:13,760 --> 00:40:16,480 Speaker 1: there's three electrons, the electron, the muon, and the towel. 831 00:40:16,680 --> 00:40:21,640 Speaker 1: There's three neutrinos. There's also three upquarks. There's three down quarks. 832 00:40:22,120 --> 00:40:24,680 Speaker 1: Like there's something really fundamental going on there we just 833 00:40:24,719 --> 00:40:27,920 Speaker 1: don't understand. But it seems like an obvious clue. You know. 834 00:40:28,040 --> 00:40:30,239 Speaker 1: It's like you're doing your jigsaw puzzle and then you 835 00:40:30,280 --> 00:40:31,960 Speaker 1: find this other weird piece. It turns out, oh, that 836 00:40:31,960 --> 00:40:34,520 Speaker 1: piece fits into a different jigsaw puzzle you didn't even 837 00:40:34,600 --> 00:40:36,880 Speaker 1: know about. And you know, it's as you start to 838 00:40:36,880 --> 00:40:38,359 Speaker 1: get this larger picture. 839 00:40:38,160 --> 00:40:40,280 Speaker 4: Right, or you find it like all of your pieces 840 00:40:40,320 --> 00:40:44,000 Speaker 4: have three sides to them, then you start thinking, you know, 841 00:40:44,080 --> 00:40:46,800 Speaker 4: whoever made this puzzle, if it was made by somebody 842 00:40:47,239 --> 00:40:48,720 Speaker 4: had a thing for threes. 843 00:40:49,239 --> 00:40:52,160 Speaker 1: Yeah, the universe has a thing for threes, and we 844 00:40:52,239 --> 00:40:54,520 Speaker 1: don't know why that is. The muon was our first 845 00:40:54,560 --> 00:40:58,160 Speaker 1: clue that particles have copies at all. And now it 846 00:40:58,160 --> 00:41:01,640 Speaker 1: turns out every particle has three copies, and so that's 847 00:41:01,680 --> 00:41:04,319 Speaker 1: a huge open question. Is a kind of question people 848 00:41:04,320 --> 00:41:06,080 Speaker 1: are going to look back in one hundred years and 849 00:41:06,120 --> 00:41:09,319 Speaker 1: be like, man, that was so obvious. Why couldn't they 850 00:41:09,360 --> 00:41:11,840 Speaker 1: figure it out? If I was a physicist in twenty nineteen, 851 00:41:11,960 --> 00:41:14,680 Speaker 1: I would totally figured it out. But it's not so 852 00:41:14,760 --> 00:41:16,719 Speaker 1: easy when you don't know the answer when you have 853 00:41:16,760 --> 00:41:18,680 Speaker 1: to come up with it. But it's important for people 854 00:41:18,680 --> 00:41:21,240 Speaker 1: to understand. You know, it's not part of the stuff 855 00:41:21,280 --> 00:41:23,640 Speaker 1: that we are made of, but it does answer this 856 00:41:23,760 --> 00:41:27,520 Speaker 1: larger questions like what is the sort of context of everything. 857 00:41:27,560 --> 00:41:29,520 Speaker 1: That's why we're trying to figure out like what are 858 00:41:29,560 --> 00:41:32,239 Speaker 1: all the particles? Because the more particles you put into 859 00:41:32,239 --> 00:41:34,680 Speaker 1: this table, the more clues we get as to what 860 00:41:34,719 --> 00:41:36,959 Speaker 1: the rules are for making this table. And then maybe 861 00:41:36,960 --> 00:41:39,600 Speaker 1: we can peel back a layer and show how this 862 00:41:39,680 --> 00:41:41,360 Speaker 1: table is put together, right. 863 00:41:41,280 --> 00:41:43,120 Speaker 4: Or I guess maybe a question I would have is 864 00:41:43,160 --> 00:41:45,040 Speaker 4: how do you even know it's a separate thing? Like 865 00:41:45,200 --> 00:41:47,680 Speaker 4: why isn't it just called the heavy electron? Could it 866 00:41:47,760 --> 00:41:49,880 Speaker 4: just be an electron that just gets a lot of 867 00:41:49,920 --> 00:41:52,840 Speaker 4: mass added on to it somehow through energy or something. 868 00:41:53,040 --> 00:41:54,719 Speaker 1: That's a deep question and goes sort of to like 869 00:41:54,800 --> 00:41:57,280 Speaker 1: what do we call a particle. Part of the identity 870 00:41:57,320 --> 00:41:59,360 Speaker 1: of the particle is its mass. Like that's how we 871 00:41:59,400 --> 00:42:02,040 Speaker 1: identify what particle we're talking about. We measure the mass 872 00:42:02,040 --> 00:42:03,319 Speaker 1: and we say, well, if it has this mass, it's 873 00:42:03,320 --> 00:42:06,440 Speaker 1: an electron. It's sort of semantics, but it's it's what 874 00:42:06,480 --> 00:42:09,239 Speaker 1: we mean by an electron. We mean quantum dot in 875 00:42:09,280 --> 00:42:11,520 Speaker 1: space that has these properties, and one of those is 876 00:42:11,560 --> 00:42:13,759 Speaker 1: the mass. Oh I see, and there are only a few. 877 00:42:13,800 --> 00:42:15,719 Speaker 1: It's not like this. It's there's a knob. You can't 878 00:42:15,719 --> 00:42:17,840 Speaker 1: have halfway between an electron and muon this like the 879 00:42:17,880 --> 00:42:20,400 Speaker 1: electron mass, the muon mass, the tau mass. There's some 880 00:42:20,520 --> 00:42:21,440 Speaker 1: notches there. 881 00:42:21,560 --> 00:42:24,000 Speaker 4: Right, And so this was the first particle that kind 882 00:42:24,000 --> 00:42:27,080 Speaker 4: of we found outside of the ones that make up atoms. 883 00:42:27,120 --> 00:42:29,160 Speaker 4: Is that what you're saying that this was the first 884 00:42:29,160 --> 00:42:30,080 Speaker 4: one that was weird? 885 00:42:30,320 --> 00:42:33,400 Speaker 1: Yeah, precisely, it's weird and cute. I'm glad you're finally 886 00:42:33,400 --> 00:42:35,960 Speaker 1: putting positive attributes on the on the muon, you know, 887 00:42:36,080 --> 00:42:36,560 Speaker 1: trying to make it. 888 00:42:36,719 --> 00:42:40,880 Speaker 4: I said weird. I didn't say cue. I think somebody 889 00:42:40,920 --> 00:42:43,680 Speaker 4: has a particle fetish, and it's not the cartoonist. 890 00:42:43,800 --> 00:42:46,960 Speaker 1: Yes, well, maybe the particle physicist has a particle fetish. 891 00:42:47,000 --> 00:42:50,520 Speaker 1: I will totally own up to that. I love you particles. 892 00:42:52,800 --> 00:42:56,239 Speaker 4: I think we all love particles by necessity. We can't 893 00:42:56,239 --> 00:42:56,560 Speaker 4: live with that. 894 00:42:56,760 --> 00:42:59,000 Speaker 1: You just like particles when they make up pizza and iPhones, 895 00:42:59,040 --> 00:43:01,800 Speaker 1: though otherwise you don't care about them. You objectify particles 896 00:43:01,840 --> 00:43:04,560 Speaker 1: and cartoonists cartoonists. 897 00:43:04,880 --> 00:43:07,239 Speaker 4: Well, I think this particle is interesting in that it 898 00:43:07,440 --> 00:43:11,080 Speaker 4: also kind of hints, you know, the universe is full, 899 00:43:11,200 --> 00:43:14,319 Speaker 4: is full of these small little details that people can 900 00:43:14,440 --> 00:43:18,120 Speaker 4: explain right now and then maybe tell us a little 901 00:43:18,160 --> 00:43:23,160 Speaker 4: bit about that there are other mysteries yet to discover. 902 00:43:23,440 --> 00:43:25,560 Speaker 1: Yeah, and you know, the story of how the muon 903 00:43:25,719 --> 00:43:28,879 Speaker 1: was discovered is also motivational. Right, People saw this weird 904 00:43:28,880 --> 00:43:30,680 Speaker 1: stuff in these pictures, and they could have just shrugged 905 00:43:30,680 --> 00:43:32,040 Speaker 1: it off. They could have been like, I don't know, 906 00:43:32,239 --> 00:43:35,120 Speaker 1: electrons are doing some weird that day, whatever, But instead 907 00:43:35,120 --> 00:43:38,120 Speaker 1: of cracked open this whole other mystery. And we're still 908 00:43:38,160 --> 00:43:41,839 Speaker 1: doing that. We still don't totally understand the muon. One 909 00:43:41,840 --> 00:43:44,360 Speaker 1: thing we'd like to understand is the muon's magnetic field. 910 00:43:44,560 --> 00:43:47,399 Speaker 4: Oh, it's odd. It has a weird magnetic field. 911 00:43:47,560 --> 00:43:50,279 Speaker 1: Yeah, these particles, remember, have quantum spin, so they're doing 912 00:43:50,360 --> 00:43:53,520 Speaker 1: something we like spinning. That's giving them each a little 913 00:43:53,600 --> 00:43:56,800 Speaker 1: magnetic field because they have electric charge and spinning charges 914 00:43:56,840 --> 00:44:00,279 Speaker 1: get magnetic fields. But when we predict the magnetic field 915 00:44:00,480 --> 00:44:02,000 Speaker 1: of the muon from what we know about it, and 916 00:44:02,040 --> 00:44:04,120 Speaker 1: then we go when we measure the magnetic field, it's 917 00:44:04,120 --> 00:44:07,560 Speaker 1: a little bit different. It's not exactly right, and that 918 00:44:07,640 --> 00:44:10,160 Speaker 1: little difference we could say, Hmm, I don't know, shrug 919 00:44:10,239 --> 00:44:12,480 Speaker 1: it off. Maybe meuon is doing some weird that day, 920 00:44:12,640 --> 00:44:14,799 Speaker 1: or it could be a clue. It could be that 921 00:44:14,800 --> 00:44:18,000 Speaker 1: the muon is like interacting with new weird heavy particles 922 00:44:18,040 --> 00:44:20,520 Speaker 1: we haven't even seen before. It could be the first 923 00:44:20,640 --> 00:44:22,800 Speaker 1: evidence that there are more particles out there that we 924 00:44:22,840 --> 00:44:27,200 Speaker 1: haven't yet discovered. And also they help us unravel ancient mysteries, 925 00:44:27,600 --> 00:44:29,759 Speaker 1: like maybe you heard about how muons are used to 926 00:44:29,760 --> 00:44:32,319 Speaker 1: take a picture of the inside of pyramids. 927 00:44:32,520 --> 00:44:34,600 Speaker 4: What do you mean, like we can make a neon 928 00:44:34,760 --> 00:44:37,680 Speaker 4: viewer like like meon glasses. 929 00:44:37,800 --> 00:44:40,719 Speaker 1: No, we can use muons to like X ray a pyramid. 930 00:44:41,120 --> 00:44:44,440 Speaker 1: Because what happens is muons, the sizillian muons shooting from 931 00:44:44,480 --> 00:44:47,600 Speaker 1: the sky through everything. And if you take a muon 932 00:44:47,680 --> 00:44:50,000 Speaker 1: detector and you put it on the other side of something, 933 00:44:50,440 --> 00:44:52,879 Speaker 1: you can tell sort of the density of that thing, 934 00:44:53,239 --> 00:44:57,160 Speaker 1: because muons will penetrate air differently than they'll penetrate rock, 935 00:44:57,239 --> 00:45:00,000 Speaker 1: for example. And so you take a lot of muan 936 00:45:00,280 --> 00:45:02,960 Speaker 1: you shoot them through something, you can tell whether that 937 00:45:03,000 --> 00:45:06,120 Speaker 1: thing is fill, is hollow or not hollow. And so 938 00:45:06,160 --> 00:45:08,520 Speaker 1: they did this recently by looking at muons that went 939 00:45:08,520 --> 00:45:11,480 Speaker 1: through the Great Pyramids, because we're curious, like what's inside 940 00:45:11,480 --> 00:45:13,440 Speaker 1: the Great Pyramid, but you don't want to take it apart, 941 00:45:13,960 --> 00:45:16,200 Speaker 1: and so they use it basically to X ray the 942 00:45:16,200 --> 00:45:17,480 Speaker 1: Great Pyramids. 943 00:45:17,000 --> 00:45:20,799 Speaker 4: Like you put a detector underneath the pyramid or or what. 944 00:45:21,040 --> 00:45:23,440 Speaker 1: Yeah, you take the detectors as far underneath the pyramids 945 00:45:23,440 --> 00:45:25,480 Speaker 1: as you can in some of those rooms that do exist. 946 00:45:26,080 --> 00:45:28,600 Speaker 1: And you know, you can't build an X ray gun 947 00:45:28,640 --> 00:45:31,400 Speaker 1: the size of the pyramids. But the sky is a 948 00:45:31,480 --> 00:45:34,319 Speaker 1: muon gun, right, The sky is shooting muons at us 949 00:45:34,360 --> 00:45:34,919 Speaker 1: all the time. 950 00:45:35,080 --> 00:45:37,080 Speaker 4: The sky is a muon gun. 951 00:45:37,560 --> 00:45:41,600 Speaker 1: Oh my god, yeah, yeah, put on your tin hats, folks, 952 00:45:41,600 --> 00:45:43,960 Speaker 1: because the sky really is shooting particles. 953 00:45:43,960 --> 00:45:46,640 Speaker 4: That sounds like I need like a lead titanium hed 954 00:45:46,719 --> 00:45:47,439 Speaker 4: not a tin head. 955 00:45:48,239 --> 00:45:50,000 Speaker 1: Maybe you know, maybe the Pharaohs had the right idea. 956 00:45:50,040 --> 00:45:52,239 Speaker 1: Maybe that's why they have those really weird headdresses. 957 00:45:52,320 --> 00:45:54,520 Speaker 4: Hmmm. Well, that's what I was going to ask, is 958 00:45:55,080 --> 00:45:59,000 Speaker 4: how do you know what neons look like after they 959 00:45:59,080 --> 00:46:01,680 Speaker 4: go through Aliens? There are alies inside the pyramid you 960 00:46:01,719 --> 00:46:02,200 Speaker 4: wouldn't know. 961 00:46:04,760 --> 00:46:06,880 Speaker 1: Wow. I was so ready with an answer to that 962 00:46:06,960 --> 00:46:09,320 Speaker 1: question until you went to Aliens, and now I'm totally 963 00:46:09,400 --> 00:46:09,880 Speaker 1: at a lost. 964 00:46:11,640 --> 00:46:14,040 Speaker 4: That's why I'm here, Daniel, to ask the tough questions 965 00:46:14,719 --> 00:46:16,280 Speaker 4: that are on everyone's minds. 966 00:46:16,719 --> 00:46:20,440 Speaker 1: Joking aside, they did find something inside the pyramids. They 967 00:46:20,440 --> 00:46:23,000 Speaker 1: think they may have found a new empty room inside 968 00:46:23,000 --> 00:46:25,759 Speaker 1: the pyramids that they didn't know about before, because the 969 00:46:25,800 --> 00:46:29,600 Speaker 1: way the Muon's full of cows before the cows are 970 00:46:29,600 --> 00:46:31,520 Speaker 1: the Aliens actually to wrap it all up. 971 00:46:32,320 --> 00:46:36,200 Speaker 4: Then we're in deep trouble when their overlord's coming and 972 00:46:36,280 --> 00:46:38,160 Speaker 4: they're like, what are you guys doing. 973 00:46:39,280 --> 00:46:42,560 Speaker 1: And they say, welcome to our our leader, King Muon 974 00:46:44,520 --> 00:46:47,839 Speaker 1: the first, the first first of his name. No, they 975 00:46:47,960 --> 00:46:50,520 Speaker 1: found that inside the Great Pyramid there may be a 976 00:46:50,560 --> 00:46:53,200 Speaker 1: new hollow section that nobody knew about before, and it's 977 00:46:53,200 --> 00:46:56,000 Speaker 1: only thanks to muons that we were able to muon 978 00:46:56,320 --> 00:46:57,920 Speaker 1: x ray the Pyramids. 979 00:46:57,600 --> 00:47:02,120 Speaker 4: M a new on chamber they phone. 980 00:47:02,560 --> 00:47:06,120 Speaker 1: Thanks thanks to me on Yes. So it may not 981 00:47:06,200 --> 00:47:08,400 Speaker 1: be inside your iPhone and it may not be inside 982 00:47:08,440 --> 00:47:12,240 Speaker 1: your pizza, but it does help unravel ancient mysteries about 983 00:47:12,239 --> 00:47:13,360 Speaker 1: ancient civilizations. 984 00:47:14,080 --> 00:47:16,440 Speaker 4: All right, Well, with that, we will wrap it up 985 00:47:16,480 --> 00:47:19,000 Speaker 4: and we hope you enjoyed that little discussion about this 986 00:47:19,400 --> 00:47:24,160 Speaker 4: unknown but super massive and mysterious part of the universe. 987 00:47:23,960 --> 00:47:27,560 Speaker 1: Part of our family of cousins, particles, big, small, massive 988 00:47:27,640 --> 00:47:29,840 Speaker 1: or not. We love you all, at least I do. 989 00:47:30,040 --> 00:47:32,000 Speaker 4: Thanks for tuning in. See you next time. 990 00:47:39,800 --> 00:47:42,160 Speaker 1: Before you still have a question after listening to all 991 00:47:42,160 --> 00:47:45,400 Speaker 1: these explanations, please drop us a line. We'd love to 992 00:47:45,400 --> 00:47:47,880 Speaker 1: hear from you. You can find us on Facebook, Twitter, 993 00:47:47,920 --> 00:47:51,600 Speaker 1: and Instagram at Daniel and Jorge That's one word, or 994 00:47:51,719 --> 00:47:56,040 Speaker 1: email us at Feedback at Danielandjorge dot com. Thanks for 995 00:47:56,080 --> 00:47:59,000 Speaker 1: listening and remember that Daniel and Jorge Explain the Universe 996 00:47:59,120 --> 00:48:03,480 Speaker 1: is a production of iHeartRadio. For more podcasts from iHeartRadio, 997 00:48:03,600 --> 00:48:07,760 Speaker 1: visit the iHeartRadio app, Apple Podcasts, or wherever you listen 998 00:48:07,840 --> 00:48:19,160 Speaker 1: to your favorite shows. 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