Teaching nuclear physics using data rather than models, recovering helium from party balloons
What is the best way to teach nuclear physics? Is the discipline more difficult than particle physics? What does a nuclear physicist make of the film Oppenheimer? These are just three of the questions addressed by David Jenkins in this episode of the Physics World Weekly podcast. A nuclear physicist and author based at the UK’s University of York, Jenkins is in conversation with Physics World’s Matin Durrani.
Also featured in this episode is Dale Keeping, who is helium recovery manager at the UK’s ISIS Neutron and Muon Source. He explains how helium is used at the facility; where the helium supply comes from; and how he and his colleagues manage this non-renewable resource. Keeping also chats about an outreach initiative that involves collecting used party balloons so the helium can be re-used at ISIS.
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1 00:00:08,942 --> 00:00:11,811 Hello and welcome to the physics world weekly 2 00:00:11,811 --> 00:00:12,311 podcast. 3 00:00:12,767 --> 00:00:13,883 I'm Hamish Johnston, 4 00:00:14,520 --> 00:00:17,401 Coming up in this episode, I'm in conversation 5 00:00:17,401 --> 00:00:21,161 with Dale Keeping, who is helium recovery manager 6 00:00:21,456 --> 00:00:22,887 at the Uk's Isis, 7 00:00:23,682 --> 00:00:24,239 Neutron and 8 00:00:24,954 --> 00:00:25,272 Source. 9 00:00:26,162 --> 00:00:29,185 He explains how Helium is used at the 10 00:00:29,185 --> 00:00:29,662 facility, 11 00:00:30,378 --> 00:00:32,367 where the gas comes from. 12 00:00:33,020 --> 00:00:35,899 And how he and his colleagues manage this 13 00:00:35,899 --> 00:00:37,340 non renewable resource. 14 00:00:38,380 --> 00:00:42,155 Dale also chats about an outreach initiative. That 15 00:00:42,155 --> 00:00:45,835 involves collecting used party balloons so that the 16 00:00:45,835 --> 00:00:49,435 helium they contain can be reused at Isis. 17 00:00:50,486 --> 00:00:52,637 Blood first, physics world's mat team 18 00:00:53,514 --> 00:00:54,173 Is in 19 00:00:54,549 --> 00:00:56,484 conversation with David Jenkins. 20 00:00:57,113 --> 00:00:59,359 Who has written a series of textbooks 21 00:00:59,811 --> 00:01:03,460 that take a different approach to teaching nuclear 22 00:01:03,460 --> 00:01:03,856 physics. 23 00:01:04,746 --> 00:01:07,929 Focusing first on how the data lead to 24 00:01:07,929 --> 00:01:08,884 physical models, 25 00:01:09,441 --> 00:01:12,624 rather than beginning with models and theories. 26 00:01:21,468 --> 00:01:22,980 Hello, and I'm delighted to be joined by 27 00:01:23,140 --> 00:01:25,448 David Jenkins, a nuclear physicist at University of 28 00:01:25,528 --> 00:01:27,677 York. Welcome to the podcast, David. Thank you. 29 00:01:27,916 --> 00:01:29,999 I'm happy to be you. Now remember, we 30 00:01:29,999 --> 00:01:31,986 let years ago at an Institute of Physics 31 00:01:31,986 --> 00:01:33,972 awards dinner, and I remember you wrote a 32 00:01:33,972 --> 00:01:36,277 feature for us about nuclear physics and its 33 00:01:36,277 --> 00:01:37,946 role on life on Earth. 34 00:01:38,757 --> 00:01:40,112 But since then you've written a couple of 35 00:01:40,112 --> 00:01:43,299 ebooks for Io about nuclear physics, and it's 36 00:01:43,299 --> 00:01:45,212 given you some insights into how we should 37 00:01:45,212 --> 00:01:46,684 teach. The subject 38 00:01:47,063 --> 00:01:47,622 to students. 39 00:01:48,421 --> 00:01:49,859 But before we come to that, I thought 40 00:01:49,859 --> 00:01:51,617 we'd just start with some the basics. 41 00:01:52,336 --> 00:01:53,865 So what what are the are the big 42 00:01:53,865 --> 00:01:56,565 questions in nuclear physics right now for people 43 00:01:56,565 --> 00:01:58,550 who haven't been keeping an eye on things? 44 00:01:59,185 --> 00:02:01,409 Well, III think there's many. I mean, there's 45 00:02:01,409 --> 00:02:02,520 lots of very technical. 46 00:02:02,853 --> 00:02:04,598 Issues. But I think the issues are are 47 00:02:04,598 --> 00:02:05,574 most interesting, 48 00:02:06,502 --> 00:02:08,645 to to the wider public. Or about the 49 00:02:08,645 --> 00:02:10,811 origin of the chemical elements 50 00:02:11,599 --> 00:02:12,099 And 51 00:02:12,479 --> 00:02:14,419 nuclear physics is is really 52 00:02:14,800 --> 00:02:15,300 underpins 53 00:02:16,000 --> 00:02:18,455 what elements are produced and the import abundant 54 00:02:18,574 --> 00:02:20,574 is in our in our universe, and that's 55 00:02:20,574 --> 00:02:21,715 got very exciting 56 00:02:22,495 --> 00:02:24,094 in the last few years because, 57 00:02:24,974 --> 00:02:27,935 from the discovery of gravitational waves, and then 58 00:02:27,935 --> 00:02:30,906 this light being emitted when when these objects 59 00:02:30,906 --> 00:02:33,165 are colliding id, it's rein, 60 00:02:33,544 --> 00:02:35,542 the whole field of nuclear physics is a 61 00:02:35,542 --> 00:02:37,300 huge number of questions now about. 62 00:02:38,033 --> 00:02:39,230 The origin of the elements. 63 00:02:39,868 --> 00:02:41,544 And that that kinda of tall with your 64 00:02:41,544 --> 00:02:43,698 own particular research interests that I think. Is 65 00:02:43,698 --> 00:02:46,110 that right in saying that? Yeah. So I've 66 00:02:46,269 --> 00:02:48,269 I've I've worked a lot on, they say 67 00:02:48,269 --> 00:02:50,669 everything that's called nuclear astro physics that relates 68 00:02:50,669 --> 00:02:52,590 to the origin of the elements, particularly at 69 00:02:52,590 --> 00:02:54,405 the moment. I've been working on 70 00:02:55,402 --> 00:02:55,902 fusion 71 00:02:56,440 --> 00:02:59,075 in massive stars, what what what what's going 72 00:02:59,075 --> 00:03:01,709 on in in stars that are 8 to 73 00:03:01,709 --> 00:03:03,705 20 times more massive than our son. 74 00:03:04,677 --> 00:03:07,068 But I'm also equally interested in just the 75 00:03:07,068 --> 00:03:09,241 pure aspects of nuclear structure 76 00:03:09,618 --> 00:03:11,610 and the properties of the atomic nucleus. 77 00:03:12,424 --> 00:03:14,102 So I mean, looking back to my undergraduate 78 00:03:14,102 --> 00:03:16,180 days, I actually did a degree in chemical 79 00:03:16,180 --> 00:03:18,338 physics. I don't think there was much nuclear 80 00:03:18,338 --> 00:03:20,895 physics on the syllabus, but what typically do 81 00:03:20,895 --> 00:03:24,202 you physics students that undergraduate level learn about 82 00:03:24,260 --> 00:03:25,717 nuclear physics. How much 83 00:03:26,095 --> 00:03:27,371 is there on the curriculum? 84 00:03:28,407 --> 00:03:30,401 There can be quite quite a lot. I 85 00:03:30,401 --> 00:03:31,014 mean, it 86 00:03:31,767 --> 00:03:32,743 in our university 87 00:03:33,353 --> 00:03:34,145 here at York. 88 00:03:34,858 --> 00:03:36,681 There's quite there's quite a bit on on 89 00:03:36,681 --> 00:03:38,679 the curriculum in there even for the... For 90 00:03:38,679 --> 00:03:40,996 the core program, and the part of the 91 00:03:40,996 --> 00:03:43,953 physics. I you can take options and study, 92 00:03:44,911 --> 00:03:46,842 even in into your third or 4 year 93 00:03:46,842 --> 00:03:48,751 of your degree. But at least in the, 94 00:03:49,228 --> 00:03:50,898 second year of the degree, there's a there's 95 00:03:50,898 --> 00:03:51,296 a lot of, 96 00:03:52,330 --> 00:03:54,500 sang to deal with nuclear physics 97 00:03:55,762 --> 00:03:57,509 probably as much as we discuss particle called 98 00:03:57,588 --> 00:04:00,049 Physics exceptionally. Yeah but that might be because 99 00:04:00,049 --> 00:04:01,899 we've got a lot of near nuclear physicists 100 00:04:01,955 --> 00:04:02,113 year. 101 00:04:02,844 --> 00:04:05,161 And and lots not so many particles ones. 102 00:04:05,721 --> 00:04:07,798 So, I thought we've turned to the new 103 00:04:07,798 --> 00:04:09,476 books that you've been writing. You wanna say 104 00:04:09,476 --> 00:04:12,201 a little bit about them. Yes. So this 105 00:04:12,201 --> 00:04:14,371 is working with Io publishing 106 00:04:14,905 --> 00:04:16,894 for their physics books series. 107 00:04:18,102 --> 00:04:21,068 We proposed a a series of books on 108 00:04:21,125 --> 00:04:22,022 nuclear structure 109 00:04:22,477 --> 00:04:24,250 and nuclear spectroscopy, 110 00:04:24,625 --> 00:04:25,616 and And 111 00:04:26,227 --> 00:04:28,077 that's been a very, very interesting 112 00:04:28,529 --> 00:04:31,331 evolution actually because of also because of events 113 00:04:31,387 --> 00:04:33,554 because we we signed up to 114 00:04:33,944 --> 00:04:36,181 I'm gonna deliver some of these books just 115 00:04:36,181 --> 00:04:37,160 before the Covid 116 00:04:37,779 --> 00:04:40,175 struck. And then when the Covid arrived, 117 00:04:40,828 --> 00:04:43,127 it we we suddenly had huge amounts of 118 00:04:43,127 --> 00:04:46,299 time to play with to and actually, in 119 00:04:46,299 --> 00:04:47,592 a way it was very therapeutic 120 00:04:47,965 --> 00:04:49,650 because we're able to spend all this time 121 00:04:49,650 --> 00:04:50,846 thinking about writing, 122 00:04:51,722 --> 00:04:54,192 and thinking about how to approach writing the 123 00:04:54,192 --> 00:04:54,431 books. 124 00:04:55,148 --> 00:04:55,786 And, of course, 125 00:04:57,075 --> 00:04:59,724 the Covid also drew it into another perspective 126 00:04:59,861 --> 00:05:02,647 because libraries were closed, You know, you couldn't 127 00:05:02,647 --> 00:05:03,920 go and get a physical book. 128 00:05:05,293 --> 00:05:06,812 You you weren't sure perhaps of that time. 129 00:05:06,971 --> 00:05:08,889 You you'd go to a library ever again. 130 00:05:09,928 --> 00:05:12,586 And so he really opened up the possibilities 131 00:05:12,725 --> 00:05:14,578 of what. Could be done with electronic, 132 00:05:15,137 --> 00:05:18,014 major and electronic rocks for. Because of course 133 00:05:18,014 --> 00:05:20,730 these are, ebooks published fines to your physics, 134 00:05:20,890 --> 00:05:21,390 publishing 135 00:05:22,662 --> 00:05:24,179 so, I mean, who who who would they 136 00:05:24,179 --> 00:05:25,935 be aimed at? Are they mostly aimed at 137 00:05:25,935 --> 00:05:27,372 undergraduate or post grad students? 138 00:05:28,090 --> 00:05:30,405 Yeah. I think they would probably be aimed 139 00:05:30,405 --> 00:05:33,851 at. To the the final year undergraduate students, 140 00:05:34,011 --> 00:05:34,750 but mostly, 141 00:05:36,085 --> 00:05:39,709 postgraduate students doing ph d or or masters 142 00:05:39,767 --> 00:05:41,757 in in in nuclear physics. 143 00:05:42,235 --> 00:05:44,168 So that's the sort of target audience 144 00:05:45,419 --> 00:05:46,350 that we have 145 00:05:46,709 --> 00:05:47,988 And and you... You told me you've kind 146 00:05:47,988 --> 00:05:50,465 of taken a different approach to other nuclear 147 00:05:50,465 --> 00:05:51,664 physics textbook. I mean, what's? 148 00:05:52,703 --> 00:05:54,461 What approach have you taken and how how 149 00:05:54,461 --> 00:05:56,946 does it differ? Would you say? Yeah. I 150 00:05:56,946 --> 00:05:59,642 think this is quite interesting because as I 151 00:05:59,642 --> 00:06:01,069 said, we we spent quite a bit of 152 00:06:01,069 --> 00:06:04,179 time thinking about how to approach. This. So 153 00:06:04,259 --> 00:06:06,896 I I work with my my main collaborator 154 00:06:06,896 --> 00:06:10,092 on these books. Is called John Wood, and 155 00:06:10,092 --> 00:06:12,110 he's a retired professor at Georgia 156 00:06:12,423 --> 00:06:14,252 tech in in the Us and he has, 157 00:06:14,889 --> 00:06:16,956 you know, an enormous number of years of 158 00:06:16,956 --> 00:06:18,944 experience of teaching, and I I've talked for 159 00:06:18,944 --> 00:06:20,296 a lot of years now, 160 00:06:20,870 --> 00:06:23,430 And, of course, you you start getting interested 161 00:06:23,430 --> 00:06:23,930 in 162 00:06:24,230 --> 00:06:25,050 in Pe. 163 00:06:25,350 --> 00:06:26,569 How how to teach 164 00:06:26,949 --> 00:06:28,569 how how to convey 165 00:06:30,003 --> 00:06:31,201 ideas to students, 166 00:06:32,319 --> 00:06:34,953 how how to challenge them how to make 167 00:06:34,953 --> 00:06:36,651 them involved and interested 168 00:06:37,348 --> 00:06:39,126 in in learning and 169 00:06:39,519 --> 00:06:41,353 And as I say, that that that led 170 00:06:41,353 --> 00:06:43,666 us into thinking about how to use books 171 00:06:43,666 --> 00:06:46,298 and so on. So I mean, historically, if 172 00:06:46,298 --> 00:06:48,393 you go back and look at nuclear physics 173 00:06:48,930 --> 00:06:49,582 text books. 174 00:06:51,013 --> 00:06:52,682 They tend to start with models, 175 00:06:53,636 --> 00:06:55,623 and they often tend to start in a 176 00:06:55,623 --> 00:06:56,758 rather kind of 177 00:06:57,547 --> 00:06:59,779 should 1 say biblical kind of way like 178 00:06:59,779 --> 00:07:02,510 a biblical authority, you know, here was the 179 00:07:02,648 --> 00:07:04,742 the model of of the shell model 180 00:07:05,535 --> 00:07:08,334 which is historical model going back to the 181 00:07:08,334 --> 00:07:10,495 the, sort of early 19 fifties. 182 00:07:11,375 --> 00:07:11,875 And 183 00:07:12,254 --> 00:07:14,595 there's nothing wrong with these models, but 184 00:07:14,910 --> 00:07:16,289 it it it's kind of 185 00:07:16,750 --> 00:07:18,509 so us of very old fashioned way of 186 00:07:18,509 --> 00:07:20,189 of of teaching the subject, 187 00:07:20,669 --> 00:07:22,209 and that it can be dry 188 00:07:23,229 --> 00:07:23,949 and boring. 189 00:07:24,444 --> 00:07:26,458 And and sometimes these models 190 00:07:27,153 --> 00:07:29,304 have become less useful as people have got 191 00:07:29,304 --> 00:07:31,217 more data and looked at these models. They 192 00:07:31,217 --> 00:07:33,146 found that there's... Problems with these models, and 193 00:07:33,146 --> 00:07:35,219 that the the the data doesn't really fit 194 00:07:35,219 --> 00:07:35,698 the models. 195 00:07:36,416 --> 00:07:38,250 And then sometimes people have come along and 196 00:07:38,250 --> 00:07:40,404 added a few more parameters of models and 197 00:07:40,404 --> 00:07:43,552 know because you know from your your involvement 198 00:07:43,610 --> 00:07:45,845 science, you can keep adding parameters to models 199 00:07:45,845 --> 00:07:48,160 and fit anything, but then it cease to 200 00:07:48,160 --> 00:07:48,660 be, 201 00:07:49,517 --> 00:07:49,916 physics. 202 00:07:50,886 --> 00:07:53,584 So we're trying to turn the whole thing 203 00:07:53,584 --> 00:07:55,036 around and start with data 204 00:07:55,806 --> 00:07:57,735 in our approach rather than, 205 00:07:58,187 --> 00:07:58,925 with models 206 00:08:00,345 --> 00:08:01,933 So when you say data, what you mean 207 00:08:01,933 --> 00:08:04,395 data that people have got from physics experiments? 208 00:08:04,554 --> 00:08:06,698 And what do you present real data or 209 00:08:06,698 --> 00:08:08,500 you sort of look at the kind of 210 00:08:08,860 --> 00:08:10,220 typical data that 1 would get? 211 00:08:10,939 --> 00:08:13,040 Yes. So so there's there's an enormous, 212 00:08:14,139 --> 00:08:14,639 comp, 213 00:08:15,660 --> 00:08:17,339 and databases of data. 214 00:08:17,753 --> 00:08:20,536 Out there nuclear data. So that's all sorts 215 00:08:20,536 --> 00:08:23,558 of properties of nuclei light. Let's take, for 216 00:08:23,558 --> 00:08:26,182 example, their gross properties. So let the the 217 00:08:26,182 --> 00:08:27,137 massive nuclei. 218 00:08:28,740 --> 00:08:29,534 Their radius. 219 00:08:30,090 --> 00:08:32,630 These are gross properties that people have measured. 220 00:08:33,583 --> 00:08:36,282 We also have excited states of nuclei. 221 00:08:37,332 --> 00:08:39,562 The nucleus is a quantum system, so it 222 00:08:39,562 --> 00:08:42,372 has quantized the excited states of specific, 223 00:08:43,306 --> 00:08:44,777 energy. There are also 224 00:08:45,234 --> 00:08:46,190 transitions between 225 00:08:46,907 --> 00:08:48,102 nuclear excited states. 226 00:08:48,660 --> 00:08:50,891 And because of the energy regime that it's 227 00:08:50,891 --> 00:08:54,570 in, those transitions media by gamma rays, which 228 00:08:54,570 --> 00:08:55,844 are very high energy, 229 00:08:56,800 --> 00:08:57,539 form of 230 00:08:58,074 --> 00:08:58,574 electromagnetic 231 00:08:59,110 --> 00:08:59,747 radiation light. 232 00:09:00,639 --> 00:09:02,874 So we have all of those databases there 233 00:09:02,874 --> 00:09:04,390 and because, of course, 234 00:09:06,146 --> 00:09:09,100 the nucleus is exploited in various ways like, 235 00:09:09,274 --> 00:09:10,725 for nuclear energy 236 00:09:11,098 --> 00:09:13,636 and for medicine and things like that, it's 237 00:09:13,636 --> 00:09:16,016 very important that people have compiled all this 238 00:09:16,016 --> 00:09:18,336 data over the years So there's a huge 239 00:09:18,336 --> 00:09:19,713 amount of data there, 240 00:09:20,329 --> 00:09:22,800 that that can be touched and then used 241 00:09:22,800 --> 00:09:24,018 more more around 242 00:09:24,793 --> 00:09:25,431 learning from. 243 00:09:26,083 --> 00:09:27,357 So do you think that makes the subject 244 00:09:27,357 --> 00:09:29,745 more accessible it becomes more real and and 245 00:09:29,745 --> 00:09:31,734 less dry as you say because people can 246 00:09:31,734 --> 00:09:32,234 see 247 00:09:32,610 --> 00:09:33,620 real date and kind of 248 00:09:34,456 --> 00:09:36,288 kind of intrigued by it and what that 249 00:09:36,288 --> 00:09:38,359 might tell us. Yes. I think that's what 250 00:09:38,359 --> 00:09:40,191 we tried to do. We tried to say, 251 00:09:40,828 --> 00:09:42,204 let's look at the data. 252 00:09:42,994 --> 00:09:45,388 And let's see if simple patterns emerge from 253 00:09:45,388 --> 00:09:47,861 the data and let's not start with traditional 254 00:09:47,861 --> 00:09:50,230 models like this shell model, which has the 255 00:09:50,269 --> 00:09:52,666 a concept that there are certain magic numbers 256 00:09:52,666 --> 00:09:54,365 of protons and neutrons 257 00:09:54,823 --> 00:09:56,362 for which the system 258 00:09:57,140 --> 00:09:59,854 has closed shells. It's called a bit like 259 00:09:59,854 --> 00:10:01,916 closed shells in a in an atom. So 260 00:10:01,916 --> 00:10:03,105 in an atom, you have the, 261 00:10:03,898 --> 00:10:05,350 you're you have chemical 262 00:10:05,659 --> 00:10:08,052 chemistry background. So we have these things noble 263 00:10:08,052 --> 00:10:09,668 gases that have no chemistry 264 00:10:10,046 --> 00:10:12,518 because they have closed shells of electrons, and 265 00:10:12,518 --> 00:10:15,150 we have certain nuclei that have closed shells 266 00:10:15,150 --> 00:10:17,717 approach tolls and neutrons and they're quite hard 267 00:10:17,717 --> 00:10:20,290 to excite. That's the the the classic 268 00:10:20,827 --> 00:10:21,305 picture of them. 269 00:10:22,342 --> 00:10:24,710 But rather site we're model, 1 can start 270 00:10:24,829 --> 00:10:26,897 looking at all this abundance of data and 271 00:10:26,897 --> 00:10:28,670 actually see naturally how 272 00:10:29,602 --> 00:10:32,557 these features emerge from looking the data. 273 00:10:33,350 --> 00:10:35,728 And then we looked at various aspects of 274 00:10:35,728 --> 00:10:38,448 nuclei. So and nucleus has typically, 275 00:10:39,549 --> 00:10:42,740 a hundred or maybe 200 protons and neutrons 276 00:10:42,740 --> 00:10:45,393 making it up. And the nucleus is fascinating 277 00:10:45,770 --> 00:10:48,403 because many aspects of it are dictated by 278 00:10:48,403 --> 00:10:50,651 the behavior of just 1 of those protons 279 00:10:50,651 --> 00:10:51,368 and neutrons. 280 00:10:52,405 --> 00:10:54,638 And many of the other aspects are dictated 281 00:10:54,638 --> 00:10:57,589 by those hundreds of particles all acting together, 282 00:10:57,908 --> 00:10:58,945 so called collected, 283 00:10:59,756 --> 00:11:02,720 behavior in nuclei, what 1 284 00:11:03,810 --> 00:11:06,615 way that scene is, the the nucleus can 285 00:11:06,672 --> 00:11:09,322 rotate and you can see patterns of rotational 286 00:11:09,322 --> 00:11:12,539 states in nuclei. As you see patterns of 287 00:11:12,598 --> 00:11:15,415 rotational states in molecules in in in chemistry, 288 00:11:15,969 --> 00:11:18,366 That's that's the analogy. And 1 can look 289 00:11:18,366 --> 00:11:21,002 at all this data and see these simple 290 00:11:21,002 --> 00:11:22,041 patterns emerging. 291 00:11:23,013 --> 00:11:24,997 And then we we kind of have chapters 292 00:11:24,997 --> 00:11:26,822 which ask questions, you know, how does the 293 00:11:26,822 --> 00:11:27,139 model... 294 00:11:27,854 --> 00:11:30,552 How does the data support models like rotation? 295 00:11:31,599 --> 00:11:34,087 So rather than starting with a a biblical 296 00:11:34,303 --> 00:11:36,315 authority of a model, we'll let the 297 00:11:36,769 --> 00:11:39,330 the the the data speak. If you like. 298 00:11:40,365 --> 00:11:41,263 And did you 299 00:11:41,719 --> 00:11:43,231 test this with people? Or have you had 300 00:11:43,231 --> 00:11:45,859 any feedback whether that approach is successful and 301 00:11:45,859 --> 00:11:48,105 is what people feel is the right way 302 00:11:48,105 --> 00:11:50,998 to learn. We've had some very nice feedback 303 00:11:51,216 --> 00:11:53,848 from from students and from people around the 304 00:11:53,848 --> 00:11:56,183 world. I mean, it's been interesting. I've had 305 00:11:56,894 --> 00:12:00,029 messages from many different countries, South Africa, 306 00:12:00,886 --> 00:12:01,386 Columbia, 307 00:12:02,163 --> 00:12:04,159 it's clear that people are are using these 308 00:12:04,159 --> 00:12:06,096 books all over the world, which is very 309 00:12:07,287 --> 00:12:07,766 pleasing. 310 00:12:09,044 --> 00:12:09,544 And 311 00:12:10,161 --> 00:12:12,237 I think it's also clear that they've engaged 312 00:12:12,237 --> 00:12:13,456 well with the material 313 00:12:14,233 --> 00:12:15,430 and understood it, 314 00:12:16,163 --> 00:12:18,548 Of course, they've often spotted mistakes, but that's 315 00:12:18,548 --> 00:12:20,535 slide that they then say, why does they 316 00:12:20,535 --> 00:12:22,681 say 82 when it should be 28? 317 00:12:23,238 --> 00:12:25,797 Somebody's type something the wrong way around. But 318 00:12:25,797 --> 00:12:26,297 they've 319 00:12:27,227 --> 00:12:29,452 they've engaged with it, and and they they've 320 00:12:29,452 --> 00:12:31,677 they've found that approach to be useful. I 321 00:12:31,677 --> 00:12:34,061 think that's the feedback, which we're getting. 322 00:12:34,875 --> 00:12:36,714 And I think be the other aspect of 323 00:12:36,714 --> 00:12:38,394 it is that the way that we present 324 00:12:38,394 --> 00:12:39,134 the thing 325 00:12:40,315 --> 00:12:42,929 is very close to research because 326 00:12:43,605 --> 00:12:45,831 we we have exercises in the book. And 327 00:12:45,831 --> 00:12:47,976 we say, well, we looked at this example 328 00:12:47,976 --> 00:12:50,361 in this particular region of the nuclear chart. 329 00:12:50,853 --> 00:12:51,752 This particular 330 00:12:52,128 --> 00:12:54,758 combination of protons and neutrons. Why not have 331 00:12:54,758 --> 00:12:56,591 a look at this region of the nuclear 332 00:12:56,591 --> 00:12:59,636 chart and see what there, go and retrieve 333 00:12:59,636 --> 00:13:01,632 the data and whatever. So we... We're setting 334 00:13:01,632 --> 00:13:03,888 these open ended exercises is that 335 00:13:04,666 --> 00:13:07,300 in a sense, actually generate research questions. 336 00:13:07,952 --> 00:13:10,341 You know, it could turn into AAA 30 337 00:13:10,341 --> 00:13:12,274 year research program to 338 00:13:12,809 --> 00:13:15,038 get the data to to answer that. But 339 00:13:15,197 --> 00:13:15,730 I think 340 00:13:16,490 --> 00:13:18,570 Again, for my experience of teaching, I think 341 00:13:18,570 --> 00:13:21,070 it's it's very useful to show students 342 00:13:22,649 --> 00:13:25,862 where the textbook ends where where research starts, 343 00:13:26,021 --> 00:13:28,168 and I think it's often very difficult for 344 00:13:28,168 --> 00:13:30,020 early career researchers to 345 00:13:30,395 --> 00:13:32,860 make that transition or make that jump ask 346 00:13:32,860 --> 00:13:33,655 those questions. 347 00:13:34,132 --> 00:13:35,428 So we're trying just 348 00:13:36,137 --> 00:13:38,153 to find a way to sort of facilitate 349 00:13:38,291 --> 00:13:39,327 that the half ounce. 350 00:13:40,524 --> 00:13:41,799 So if I was a student, you know, 351 00:13:41,959 --> 00:13:44,032 starting off my Phd into nuclear physics, we 352 00:13:44,032 --> 00:13:46,197 know what would be the The big questions 353 00:13:46,197 --> 00:13:48,107 that, you know, you'd encourage me to go 354 00:13:48,107 --> 00:13:49,618 into what would you go into if you 355 00:13:49,618 --> 00:13:51,209 were spying out again, David. 356 00:13:52,179 --> 00:13:54,251 If I was starting out again, I I 357 00:13:54,251 --> 00:13:56,005 wonder if I would do n nucleus physics 358 00:13:56,005 --> 00:13:58,477 6, I do... I might do something different, 359 00:13:58,556 --> 00:13:59,535 but I think 360 00:14:00,882 --> 00:14:02,630 just because I've done it for so many 361 00:14:02,630 --> 00:14:04,536 years, like, you gotta start thinking well, You 362 00:14:04,536 --> 00:14:06,125 know, if I was start they go, I'd 363 00:14:06,125 --> 00:14:08,428 love to know about some other things not 364 00:14:08,428 --> 00:14:10,096 that I find what I'm doing boring. 365 00:14:10,748 --> 00:14:12,980 Because there were so many open questions in 366 00:14:12,980 --> 00:14:14,596 the field and there are so many 367 00:14:15,371 --> 00:14:15,871 important 368 00:14:16,248 --> 00:14:18,973 applications to other fields like fundamental physics and 369 00:14:18,973 --> 00:14:21,306 astro physics and the course all the societal 370 00:14:22,320 --> 00:14:25,029 applications to energy and Medicine to to to 371 00:14:25,029 --> 00:14:26,039 name but a few 372 00:14:26,798 --> 00:14:29,053 But I think I would encourage young people 373 00:14:29,830 --> 00:14:31,905 starting it off in that in the field, 374 00:14:32,783 --> 00:14:35,112 and I'm biased here, but because the the 375 00:14:35,112 --> 00:14:37,026 clue what we've been discussing. But, you know, 376 00:14:37,345 --> 00:14:38,323 I I would 377 00:14:39,577 --> 00:14:42,709 I would encourage them to to challenge authority 378 00:14:42,847 --> 00:14:45,334 around these sorts of things. You know, that 379 00:14:45,334 --> 00:14:47,568 not sort of entered for thinking, you know, 380 00:14:49,083 --> 00:14:52,034 everything's like lay down, all of the foundations 381 00:14:52,034 --> 00:14:54,280 are there the walls of this this structure 382 00:14:54,280 --> 00:14:55,871 this of this topic. 383 00:14:56,587 --> 00:14:59,314 I think I would encourage people to be 384 00:15:00,737 --> 00:15:03,593 more more questioning to to start with the 385 00:15:03,593 --> 00:15:06,370 data. And I think there were other fantastic 386 00:15:06,370 --> 00:15:08,592 things that people could do, and, you know, 387 00:15:09,244 --> 00:15:10,144 I'm a dinosaur 388 00:15:10,842 --> 00:15:12,601 in this sort of thing. But I think 389 00:15:12,601 --> 00:15:14,220 there's a lot that could be done 390 00:15:14,918 --> 00:15:18,115 with techniques like machine learning and so on. 391 00:15:18,689 --> 00:15:21,422 To to look at the data that's available 392 00:15:21,959 --> 00:15:24,193 and let people find patterns in it for 393 00:15:24,193 --> 00:15:24,512 themselves. 394 00:15:25,309 --> 00:15:27,144 Because, you know, I think it's always a 395 00:15:27,144 --> 00:15:29,870 very interesting question in science and physics, you 396 00:15:29,870 --> 00:15:31,884 know, we come to some 397 00:15:32,341 --> 00:15:33,718 understanding the or some model 398 00:15:34,174 --> 00:15:36,326 based on our starting point and the data, 399 00:15:37,059 --> 00:15:39,059 But we're biased. Everything thing we do is 400 00:15:39,059 --> 00:15:41,059 biased and, you know, we have ours and 401 00:15:41,059 --> 00:15:43,299 how we how we decide to do measurements, 402 00:15:43,459 --> 00:15:44,659 how we decide to do things. 403 00:15:45,553 --> 00:15:48,206 May throwing, you know, these more modern 404 00:15:48,903 --> 00:15:52,013 computer techniques that this enormously rich datasets sets 405 00:15:52,013 --> 00:15:55,536 with thousands of data points, you might draw 406 00:15:55,536 --> 00:15:56,673 out a whole different 407 00:15:57,446 --> 00:16:00,072 pattern and things and and it might show 408 00:16:00,072 --> 00:16:01,982 AAA deeper understanding. 409 00:16:03,753 --> 00:16:05,670 Then, you know, what models are there. So 410 00:16:05,830 --> 00:16:07,828 I I just encourage young people always to 411 00:16:07,828 --> 00:16:08,227 question, 412 00:16:09,266 --> 00:16:11,518 but for tip. Maybe that's the long thing 413 00:16:11,518 --> 00:16:13,595 to say, but, you know, that's my feeling 414 00:16:13,595 --> 00:16:15,752 with. I mean, do you ever suffer David 415 00:16:15,752 --> 00:16:18,401 in in physics of kind of people going 416 00:16:18,401 --> 00:16:20,315 into particle physics? That's the sort of sexy 417 00:16:20,315 --> 00:16:20,634 area, 418 00:16:21,193 --> 00:16:23,585 dare I say that and people maybe, you 419 00:16:23,585 --> 00:16:25,739 know, sw you a bit and go and 420 00:16:25,739 --> 00:16:27,095 do they always think of you going into 421 00:16:27,095 --> 00:16:28,866 that feel first of all, you have a 422 00:16:28,866 --> 00:16:30,622 competition with the particle physicists? 423 00:16:31,261 --> 00:16:32,937 They they can be, of course, that sort 424 00:16:32,937 --> 00:16:35,811 of healthy competition between those fields. But I 425 00:16:35,811 --> 00:16:35,890 mean, 426 00:16:37,103 --> 00:16:39,736 they could be quite they are quite different 427 00:16:39,736 --> 00:16:42,928 fields I would say. I mean, particle physics 428 00:16:42,928 --> 00:16:44,500 is... It can be quite 429 00:16:45,097 --> 00:16:47,169 reduction is. You can reduce it down to 430 00:16:47,169 --> 00:16:49,559 sort of finding particles and things like that. 431 00:16:50,436 --> 00:16:53,003 And I think historically a lot people move 432 00:16:53,003 --> 00:16:56,217 from physics 2 particle physics as that field 433 00:16:56,595 --> 00:16:58,591 took off in the fifties and sixties and 434 00:16:58,591 --> 00:16:58,990 so on. 435 00:16:59,709 --> 00:17:01,305 And I think in many ways, 436 00:17:04,350 --> 00:17:06,741 what happened was that nuclear physics turned out 437 00:17:06,741 --> 00:17:07,936 to be too hard. 438 00:17:08,813 --> 00:17:10,899 I know about Don't mean that in a 439 00:17:10,899 --> 00:17:13,687 sort of p way that particle physics is 440 00:17:13,687 --> 00:17:16,156 easy, But I mean that it's hard in 441 00:17:16,156 --> 00:17:18,387 the sense that the the object you're looking 442 00:17:18,387 --> 00:17:18,887 at 443 00:17:19,277 --> 00:17:22,395 is very complicated. It involves hundreds of particles 444 00:17:22,529 --> 00:17:23,029 acting 445 00:17:23,958 --> 00:17:26,655 together. We don't have an overall model as 446 00:17:26,655 --> 00:17:28,653 the nuclear where we would love to help 447 00:17:28,653 --> 00:17:30,239 on various different models, 448 00:17:30,794 --> 00:17:33,673 treating this different aspects of its behavior. But 449 00:17:33,966 --> 00:17:35,021 it's extremely 450 00:17:35,730 --> 00:17:37,350 challenging both to theory 451 00:17:38,529 --> 00:17:40,869 and to experiment. And so that's why 452 00:17:41,809 --> 00:17:44,105 countries are still investing so much in in 453 00:17:44,303 --> 00:17:46,128 facilities to to study that. And, you know, 454 00:17:46,366 --> 00:17:48,112 I think when I when I talk to 455 00:17:48,271 --> 00:17:50,175 Students, I I do make that point, you 456 00:17:50,175 --> 00:17:52,263 know, I think it's important to justify 457 00:17:53,048 --> 00:17:55,376 at the outset. Why is still studying 458 00:17:55,750 --> 00:17:57,896 a field which has bingo over for 100 459 00:17:57,896 --> 00:17:58,214 years. 460 00:17:58,770 --> 00:18:00,122 Not that is it that that is a 461 00:18:00,122 --> 00:18:01,893 good... You know, it goes back to River 462 00:18:03,239 --> 00:18:05,468 initial theory that there was a nucleus of 463 00:18:05,468 --> 00:18:07,617 an anatomy It's about 19 11 I. 464 00:18:08,732 --> 00:18:10,220 And you after then ask you know, after 465 00:18:10,419 --> 00:18:12,416 hundred years don't, you know everything you you 466 00:18:12,416 --> 00:18:14,493 want to know. And, of course, we do 467 00:18:14,493 --> 00:18:16,091 know lots of things. But I think there's 468 00:18:16,091 --> 00:18:18,744 a lot more so, we still don't know. 469 00:18:19,464 --> 00:18:22,265 What's your favorite nucleus dare I ask? Do 470 00:18:22,265 --> 00:18:23,085 you want favorite? 471 00:18:24,265 --> 00:18:26,424 Do you don't want this a favor 1? 472 00:18:27,713 --> 00:18:27,872 Well, 473 00:18:29,383 --> 00:18:30,679 there's a there's a funny 474 00:18:31,054 --> 00:18:33,542 funny story with with nuclei because 475 00:18:34,253 --> 00:18:34,971 you always say, 476 00:18:36,887 --> 00:18:39,441 study nuclei that have an even number of 477 00:18:39,441 --> 00:18:42,075 protons and an even number of neutrons because 478 00:18:42,075 --> 00:18:44,809 there's structure and their properties is is simple. 479 00:18:45,529 --> 00:18:47,130 And if you study ones that have an 480 00:18:47,130 --> 00:18:48,970 odd number of protons and a odd number 481 00:18:48,970 --> 00:18:51,954 of neutrons, Their structure is extremely complicated. 482 00:18:52,566 --> 00:18:54,791 So that's the kind of general rule, but 483 00:18:54,791 --> 00:18:57,255 that there are some special ones that are 484 00:18:57,255 --> 00:18:58,819 so called n equals zed 485 00:18:59,178 --> 00:19:01,724 nuclei have the same number of protons and 486 00:19:01,724 --> 00:19:02,043 neutrons. 487 00:19:02,600 --> 00:19:04,988 And in those systems, even the odd adult 488 00:19:04,988 --> 00:19:06,283 nuclei have a beautiful 489 00:19:07,151 --> 00:19:10,094 simple symmetry that you can look at and 490 00:19:10,094 --> 00:19:10,594 grasp 491 00:19:10,969 --> 00:19:12,719 and get something nice out of it. So 492 00:19:12,799 --> 00:19:14,089 III 493 00:19:14,089 --> 00:19:16,409 studied some years ago, 1 of these odd, 494 00:19:17,049 --> 00:19:19,690 n equals that nuclear was bromine 70. So 495 00:19:19,849 --> 00:19:21,804 I think that would be my favorite. 1 496 00:19:22,583 --> 00:19:24,341 you thought people were said to you your 497 00:19:24,341 --> 00:19:25,779 math to study this, it would be very 498 00:19:25,779 --> 00:19:26,898 complicated breaks it's talk. 499 00:19:27,857 --> 00:19:29,935 For various reasons of cemetery so. 500 00:19:30,746 --> 00:19:32,734 Absolutely nice. Yeah. I'll all that 1. Go 501 00:19:32,734 --> 00:19:34,722 through that 1 there. Yeah. Yeah. Yeah. And 502 00:19:34,722 --> 00:19:36,869 thanks, David. Before we go... I'm. Haven't actually 503 00:19:36,869 --> 00:19:37,903 asked you what the name the book were. 504 00:19:38,221 --> 00:19:40,623 Book were you've written. You want to name 505 00:19:40,623 --> 00:19:43,965 check them? Yes. So the... There is actually 506 00:19:43,965 --> 00:19:46,591 gonna be free books in the end. The 507 00:19:46,591 --> 00:19:48,279 only 2 of them are published so far. 508 00:19:48,440 --> 00:19:50,200 And the other 1 is in sort of 509 00:19:50,200 --> 00:19:50,700 final 510 00:19:51,240 --> 00:19:54,220 stages of the preparation. So the first book 511 00:19:54,359 --> 00:19:56,700 is called nuclear data, a primer 512 00:19:57,253 --> 00:19:59,646 and that 1 focuses on things like these 513 00:19:59,646 --> 00:20:02,677 gross properties, mass and radius, of the nucleus 514 00:20:02,677 --> 00:20:03,735 and some simple 515 00:20:04,112 --> 00:20:06,106 aspects of the structure of the nucleus. 516 00:20:06,839 --> 00:20:09,393 Then the second book is called nuclear data, 517 00:20:09,553 --> 00:20:12,745 a collective motion view. So that focuses is 518 00:20:12,745 --> 00:20:15,060 on collected properties of nuclei, 519 00:20:15,712 --> 00:20:16,212 particularly 520 00:20:16,827 --> 00:20:19,694 rotation of nuclei and vibration of nuclei. 521 00:20:20,252 --> 00:20:22,322 And the final 1 that John and I 522 00:20:22,322 --> 00:20:23,857 just completely at the moment 523 00:20:24,168 --> 00:20:27,977 is called nuclear data, an independent particle called 524 00:20:27,977 --> 00:20:30,460 motion view. So that's looking at the other 525 00:20:30,516 --> 00:20:31,016 extreme 526 00:20:31,564 --> 00:20:34,118 where all the properties of this nucleus are 527 00:20:34,118 --> 00:20:36,513 dictated by just 1 of the protons or 528 00:20:36,513 --> 00:20:38,668 neutrons that makes it up. So we've got 529 00:20:38,668 --> 00:20:40,046 a sort of general book 530 00:20:40,837 --> 00:20:44,289 1 our collective behavior at 1 about, an 531 00:20:44,427 --> 00:20:45,862 independent particle behavior. 532 00:20:46,341 --> 00:20:48,335 And I think we're we kinda love to 533 00:20:48,335 --> 00:20:50,111 write more, but we probably. 534 00:20:51,613 --> 00:20:54,154 Enough for now. Said 2 the intelligence books. 535 00:20:54,868 --> 00:20:56,615 Lovely, David. Before we go, 1 last question 536 00:20:56,694 --> 00:20:58,679 I was thinking, nuclear physics in in sort 537 00:20:58,679 --> 00:21:01,000 of the public mind, they associate that with 538 00:21:01,000 --> 00:21:03,704 nuclear weapons. And the Oppenheimer film, did you 539 00:21:03,704 --> 00:21:04,977 watch it? Did what did you make of 540 00:21:04,977 --> 00:21:05,136 it? 541 00:21:05,932 --> 00:21:07,940 Alright. I thought that film is very good. 542 00:21:08,180 --> 00:21:10,116 Yeah. I... Because I I'd I 543 00:21:10,573 --> 00:21:12,727 I, you know, I I often get worried, 544 00:21:12,887 --> 00:21:14,578 but when I see the films a very 545 00:21:14,578 --> 00:21:14,897 long. 546 00:21:15,695 --> 00:21:17,931 3 hours. It was 3 hours wasn't it. 547 00:21:18,090 --> 00:21:18,889 And I found... 548 00:21:19,767 --> 00:21:21,284 I think I watched that film when I 549 00:21:21,284 --> 00:21:22,901 watched the June 2 film, 550 00:21:23,772 --> 00:21:26,157 and both those films were very long, but 551 00:21:26,157 --> 00:21:27,350 then they came to the end that I 552 00:21:27,350 --> 00:21:28,940 didn't notice that they were long. Now, it's 553 00:21:28,940 --> 00:21:30,530 kinda like, 3 hours went by. I said, 554 00:21:30,689 --> 00:21:32,200 in my mind, that's a good film. My 555 00:21:32,279 --> 00:21:34,384 I bought it. I thought he was very 556 00:21:34,838 --> 00:21:36,826 well done. It was very well active Wasn't 557 00:21:36,826 --> 00:21:39,131 it. And Killing and Murphy was... I fought 558 00:21:39,131 --> 00:21:39,631 very 559 00:21:40,085 --> 00:21:41,754 very, very good as open oppenheimer, but and 560 00:21:41,834 --> 00:21:43,382 I think it at the 561 00:21:44,075 --> 00:21:46,062 the sense of the time and how those 562 00:21:46,062 --> 00:21:48,073 people work. And it felt kind of 563 00:21:48,526 --> 00:21:50,037 it could felt kind of real to me. 564 00:21:50,196 --> 00:21:52,527 I I could see those scientists like, 565 00:21:53,246 --> 00:21:55,084 who are acted as there's sort of real 566 00:21:55,084 --> 00:21:56,362 peak, and I don't know what you felt. 567 00:21:56,522 --> 00:21:57,960 But IIII 568 00:21:57,960 --> 00:22:00,449 like to. Yeah. III only looked to my 569 00:22:00,449 --> 00:22:02,204 watch once during the film, which I think 570 00:22:02,204 --> 00:22:03,640 is a really good sign and, you know, 571 00:22:03,799 --> 00:22:05,236 often I get quite bored with films. 572 00:22:05,887 --> 00:22:08,029 And that 1, I didn't. There was only 573 00:22:08,029 --> 00:22:09,377 once I looked at my watch. And, yeah, 574 00:22:09,457 --> 00:22:11,440 it was 3 hours. It was quite remarkable. 575 00:22:11,836 --> 00:22:11,995 Yeah. 576 00:22:12,884 --> 00:22:14,403 Did it lead to a ups surge of 577 00:22:14,403 --> 00:22:16,880 interest in physics or not had any impact 578 00:22:16,880 --> 00:22:18,558 you think? Would do people not make the 579 00:22:18,558 --> 00:22:20,476 link between bombs and the kind of research 580 00:22:20,476 --> 00:22:20,876 you're doing? 581 00:22:22,882 --> 00:22:24,256 Well, I hope they don't make 582 00:22:24,710 --> 00:22:27,887 They do negative to what. IIII 583 00:22:27,887 --> 00:22:30,111 don't know really. I only got people talking. 584 00:22:30,349 --> 00:22:32,352 I mean, it's always got the. Got got 585 00:22:32,352 --> 00:22:34,662 the, you know, and it has got people 586 00:22:34,662 --> 00:22:36,733 talking and people who asked me about it 587 00:22:36,733 --> 00:22:39,043 and things like that. But but I... I'm 588 00:22:39,043 --> 00:22:40,817 not sure it's directly affected 589 00:22:41,845 --> 00:22:44,153 students interested in, like, joining the field or 590 00:22:44,153 --> 00:22:46,621 something like that. And not not to my 591 00:22:46,621 --> 00:22:48,474 knowledge, but It'd I'd be interesting to 592 00:22:49,105 --> 00:22:51,105 to know. I mean, obviously, that that that 593 00:22:51,105 --> 00:22:52,565 film's got a lot of, 594 00:22:53,424 --> 00:22:55,605 you know, very very sad historical 595 00:22:57,439 --> 00:22:59,037 features to it. And, you know, it means, 596 00:22:59,277 --> 00:23:01,674 it's a true story It's history. I I'd 597 00:23:01,674 --> 00:23:02,973 be interesting to know, 598 00:23:03,832 --> 00:23:06,444 how it's changed people's views of that about 599 00:23:06,564 --> 00:23:08,240 the area of science. 600 00:23:09,198 --> 00:23:11,113 Alright. Well, I hope your books get more 601 00:23:11,113 --> 00:23:12,549 students into the field. So thanks so much, 602 00:23:12,709 --> 00:23:14,359 David would been brilliant to talk to you 603 00:23:14,720 --> 00:23:15,220 and 604 00:23:15,519 --> 00:23:16,640 thanks for your time on the podcast. 605 00:23:17,119 --> 00:23:17,920 Thank you very much. 606 00:23:25,762 --> 00:23:28,404 Helium is an inner gas that is relatively 607 00:23:28,619 --> 00:23:30,365 rare and earth's atmosphere. 608 00:23:31,000 --> 00:23:31,476 However, 609 00:23:31,809 --> 00:23:35,008 it plays crucial roles in science and technology. 610 00:23:35,857 --> 00:23:39,112 Had, it's also used to float party balloons. 611 00:23:40,161 --> 00:23:43,526 It's an expensive commodity at a non renewable 612 00:23:43,742 --> 00:23:46,527 resource, which is why many users try to 613 00:23:46,527 --> 00:23:49,584 recover and reuse as much of the element 614 00:23:49,799 --> 00:23:50,673 as possible. 615 00:23:51,467 --> 00:23:52,817 At the Uk's Isis, 616 00:23:53,532 --> 00:23:54,350 neutron and 617 00:23:54,723 --> 00:23:54,961 source, 618 00:23:55,770 --> 00:23:58,942 That process is the responsibility of dale keeping, 619 00:23:59,656 --> 00:24:00,869 who is the facility's 620 00:24:01,242 --> 00:24:02,907 helium recovery manager. 621 00:24:03,796 --> 00:24:06,046 He joins me down the line from Har 622 00:24:06,341 --> 00:24:07,080 in Oxford. 623 00:24:07,852 --> 00:24:10,023 Hi, Dale. Welcome to the podcast. 624 00:24:10,557 --> 00:24:10,875 Hiya. 625 00:24:12,083 --> 00:24:15,103 So so, Dale, how is helium used in 626 00:24:15,103 --> 00:24:16,772 science and technology at Isis? 627 00:24:17,567 --> 00:24:19,180 We mainly helium 628 00:24:19,569 --> 00:24:21,977 to call samples down in a Cryo. 629 00:24:22,909 --> 00:24:23,647 The helium 630 00:24:24,260 --> 00:24:25,635 supplies heat exchanger, 631 00:24:26,089 --> 00:24:28,975 which is connected to the sample space 632 00:24:30,083 --> 00:24:32,656 The helium is supplied to the heat exchanger 633 00:24:32,794 --> 00:24:35,187 and then is pumped across it to cool 634 00:24:35,187 --> 00:24:36,724 the sample down via 635 00:24:37,181 --> 00:24:39,390 evaporation to 1.6 k 636 00:24:40,309 --> 00:24:43,286 Right. And so is that is that liquid 637 00:24:43,346 --> 00:24:46,382 helium that you're using then? Yeah. So we 638 00:24:46,382 --> 00:24:49,352 use liquid helium within the main bar? Of 639 00:24:49,352 --> 00:24:52,368 the price that. Yeah. You're cooling samples. Is 640 00:24:52,368 --> 00:24:54,352 that what you're cooling to to get them 641 00:24:54,352 --> 00:24:56,653 down to to a very low temperature so 642 00:24:56,653 --> 00:24:57,740 that people can make 643 00:24:58,337 --> 00:25:01,205 make measurements at low temperatures? Is that is 644 00:25:01,205 --> 00:25:04,153 that mostly what you're doing? Or are are 645 00:25:04,153 --> 00:25:07,181 you cooling magnets and and and and other 646 00:25:07,181 --> 00:25:09,830 things? Yeah. We we we do have super 647 00:25:09,830 --> 00:25:10,628 conducting magnets. 648 00:25:11,107 --> 00:25:11,586 And, 649 00:25:12,944 --> 00:25:13,423 mainly, 650 00:25:13,902 --> 00:25:15,738 what we find the samples eye, it could 651 00:25:15,738 --> 00:25:18,169 be mainly a crystal or or powder 652 00:25:18,705 --> 00:25:20,618 or something like that. Yeah. We we do 653 00:25:20,618 --> 00:25:22,291 our other patients as well, 654 00:25:23,168 --> 00:25:24,864 where we use maybe Cc. 655 00:25:25,813 --> 00:25:28,680 Or which is close like refrigerators or flow 656 00:25:28,680 --> 00:25:30,750 price stats and and things like that that 657 00:25:30,750 --> 00:25:32,741 we we can use as well. And where 658 00:25:32,741 --> 00:25:33,958 does our helium 659 00:25:34,589 --> 00:25:37,066 supply come from at the moment. I mean, 660 00:25:37,306 --> 00:25:39,543 I'm I'm guessing that you would get a 661 00:25:39,543 --> 00:25:41,994 delivery from a from a specialist 662 00:25:42,674 --> 00:25:43,893 supplier. But 663 00:25:44,352 --> 00:25:46,430 where do they get the helium from? 664 00:25:47,309 --> 00:25:47,809 Helium 665 00:25:48,268 --> 00:25:51,465 is trapped in yes crust by imp role? 666 00:25:52,039 --> 00:25:55,874 And is extracted as a product of the 667 00:25:55,874 --> 00:25:57,472 liquid natural gas industry. 668 00:25:58,591 --> 00:26:01,402 Therefore, it's only really found in a few 669 00:26:01,402 --> 00:26:04,519 places around the world. For example, the Us, 670 00:26:05,158 --> 00:26:05,558 Algeria, 671 00:26:06,037 --> 00:26:09,246 Our he supply actually comes from Qatar. I 672 00:26:09,246 --> 00:26:11,553 see. And it's... I'm I mean, I think 673 00:26:11,712 --> 00:26:14,280 I'm right in saying that it's it's created 674 00:26:14,336 --> 00:26:15,950 by the... Is it the radioactive 675 00:26:16,564 --> 00:26:16,802 decay? 676 00:26:17,611 --> 00:26:21,259 Of uranium, I think underground. Yeah. Produces the 677 00:26:21,259 --> 00:26:24,273 helium, and then it somehow gets trapped in 678 00:26:24,273 --> 00:26:24,773 with 679 00:26:25,398 --> 00:26:27,941 with the natural gas and and and sort 680 00:26:27,941 --> 00:26:28,838 of extracted 681 00:26:29,212 --> 00:26:31,857 that way. Yeah. I think it's extracted from 682 00:26:32,470 --> 00:26:33,446 fractional dis. 683 00:26:34,154 --> 00:26:35,588 I mean, I'm guessing that... You know, there's 684 00:26:35,588 --> 00:26:36,486 lots of radioactive 685 00:26:36,942 --> 00:26:39,890 decay going on in the earth, but that's 686 00:26:39,890 --> 00:26:43,497 a that's a fairly slow process. So 687 00:26:43,888 --> 00:26:46,271 it it it is in limited supply, isn't 688 00:26:46,271 --> 00:26:48,257 it? I mean, new new 689 00:26:48,733 --> 00:26:51,355 supply, areas open up. I mean, you mentioned 690 00:26:51,593 --> 00:26:53,474 Qatar, which I think is a fairly new 691 00:26:54,473 --> 00:26:57,750 producer of helium. But how secure is is 692 00:26:57,750 --> 00:27:00,627 the supply? If we don't use it responsibly? 693 00:27:00,867 --> 00:27:02,305 Will it run out eventually? 694 00:27:03,119 --> 00:27:06,480 Yeah. So people have predicted that Helium will 695 00:27:06,480 --> 00:27:07,539 run out in, 696 00:27:08,080 --> 00:27:09,359 a few hundred years time, 697 00:27:10,240 --> 00:27:12,000 depending on the usage levels. 698 00:27:13,527 --> 00:27:15,594 Things that, I, you know, I think do 699 00:27:15,594 --> 00:27:18,775 affect the supply are maintenance of the gas 700 00:27:18,775 --> 00:27:19,832 company's plant 701 00:27:20,286 --> 00:27:21,581 weather conflict 702 00:27:23,403 --> 00:27:25,312 you know, this is why we having a 703 00:27:25,312 --> 00:27:27,937 system in place to capture as much helium 704 00:27:27,937 --> 00:27:28,993 as we possibly. 705 00:27:29,622 --> 00:27:32,986 Cam is is crucial to ensure a continuous 706 00:27:33,042 --> 00:27:34,099 source for 707 00:27:34,633 --> 00:27:35,133 scientific 708 00:27:35,588 --> 00:27:35,986 experiments. 709 00:27:36,956 --> 00:27:38,310 And and so how do you do that? 710 00:27:38,549 --> 00:27:40,721 How do you how do you capture Helium 711 00:27:41,415 --> 00:27:44,282 at the moment? Helium itself. It's it's a 712 00:27:44,282 --> 00:27:44,782 tiny 713 00:27:45,253 --> 00:27:47,163 Adam isn't it that can sort of sneak 714 00:27:47,163 --> 00:27:48,379 out of your pipes 715 00:27:48,913 --> 00:27:51,460 very easily. How how how do you how 716 00:27:51,460 --> 00:27:53,609 do you recycle it and and capture it? 717 00:27:54,166 --> 00:27:56,747 Is 1 of 1 of our biggest challenges 718 00:27:56,804 --> 00:27:58,631 is is trying to keep all of the 719 00:27:58,631 --> 00:27:59,585 helium leak tight. 720 00:28:00,856 --> 00:28:03,579 You know, we have maybe 2 kilometers of 721 00:28:03,579 --> 00:28:06,231 pipe work and hundreds of o to, 722 00:28:06,688 --> 00:28:08,283 you know, try and keep on top of 723 00:28:08,283 --> 00:28:10,537 which can be quite a challenge 724 00:28:11,009 --> 00:28:11,650 for the team. 725 00:28:12,849 --> 00:28:14,710 But... Yeah. We we try and recycle 726 00:28:15,490 --> 00:28:17,570 all of the helium that's used out in 727 00:28:17,570 --> 00:28:18,390 the experiments 728 00:28:18,703 --> 00:28:21,826 So when the helium leaves the experiments at 729 00:28:21,883 --> 00:28:24,903 atmospheric pressure is collected via a pipeline, 730 00:28:25,459 --> 00:28:28,098 which then makes its way back to the 731 00:28:28,098 --> 00:28:31,786 helium recovery building. The helium expands into 732 00:28:32,402 --> 00:28:33,460 a very large 733 00:28:33,916 --> 00:28:37,595 collection balloon, which is 22 meters cubes in 734 00:28:37,595 --> 00:28:37,993 volume. 735 00:28:39,108 --> 00:28:42,374 The helium is then compressed up to a 736 00:28:42,374 --> 00:28:44,467 maximum of a hundred and 95 bar 737 00:28:46,460 --> 00:28:49,019 gas then makes its way through series of 738 00:28:49,019 --> 00:28:49,500 filters. 739 00:28:52,073 --> 00:28:54,401 And then it will go into a man 740 00:28:55,093 --> 00:28:56,944 depending on its purity 741 00:28:57,477 --> 00:29:00,100 would depend upon what Mc bank it will 742 00:29:00,100 --> 00:29:01,647 be put in. So 743 00:29:02,099 --> 00:29:04,163 if it's less than 98 percent, 744 00:29:04,797 --> 00:29:07,019 it go into what we call as our 745 00:29:07,019 --> 00:29:07,971 sort of dirty bank. 746 00:29:09,733 --> 00:29:12,751 If it's better than 98 percent efficient, it 747 00:29:12,751 --> 00:29:14,602 will go into our clean 748 00:29:15,293 --> 00:29:15,928 sort storage. 749 00:29:16,579 --> 00:29:18,747 And then from there, when we want to 750 00:29:18,883 --> 00:29:19,383 produce 751 00:29:21,108 --> 00:29:23,674 liquid helium, we can then run 752 00:29:24,064 --> 00:29:24,883 it's gas 753 00:29:26,140 --> 00:29:26,640 through 754 00:29:27,018 --> 00:29:29,652 a line dryer, which is essentially another filter, 755 00:29:30,211 --> 00:29:32,366 and then it will make its way into, 756 00:29:33,339 --> 00:29:35,099 delete viral or cold box. 757 00:29:36,059 --> 00:29:36,559 And 758 00:29:37,500 --> 00:29:39,599 first of all, it will enter a purifier 759 00:29:40,059 --> 00:29:42,549 where it will remove all of its impurities, 760 00:29:43,027 --> 00:29:45,359 and then it will go into the l 761 00:29:45,416 --> 00:29:47,726 side of things to be cooled down, 762 00:29:49,240 --> 00:29:49,797 use liquid. 763 00:29:50,689 --> 00:29:53,242 And then from there, it will go into 764 00:29:53,242 --> 00:29:53,960 a very large, 765 00:29:55,955 --> 00:29:56,673 mother vessel, 766 00:29:58,123 --> 00:30:00,191 which what we have... We have a 2000 767 00:30:00,191 --> 00:30:00,691 liter 768 00:30:01,146 --> 00:30:01,646 mother. 769 00:30:02,180 --> 00:30:04,248 And then from there, we can d cam 770 00:30:04,248 --> 00:30:06,157 into smaller mobile vessels. 771 00:30:07,048 --> 00:30:08,506 And that's where we can 772 00:30:09,283 --> 00:30:11,518 take these jira out into the into the 773 00:30:11,518 --> 00:30:12,737 halls within Isis 774 00:30:13,194 --> 00:30:15,682 to be used again for experiments. So It's 775 00:30:15,682 --> 00:30:16,818 just a continuous 776 00:30:17,589 --> 00:30:18,065 cycle. 777 00:30:18,780 --> 00:30:20,527 So could can you give us an idea 778 00:30:20,527 --> 00:30:23,148 of of how much liquid helium you would 779 00:30:23,148 --> 00:30:23,648 be 780 00:30:24,278 --> 00:30:24,778 producing 781 00:30:25,156 --> 00:30:25,975 or using 782 00:30:26,512 --> 00:30:28,666 at Isis in a... I don't know in 783 00:30:28,666 --> 00:30:30,182 a week or a month? Is it a? 784 00:30:30,581 --> 00:30:32,909 Is it is it a huge amount or 785 00:30:32,989 --> 00:30:36,359 I suppose that's re relatively speaking? Yeah. So 786 00:30:36,418 --> 00:30:38,092 so when we we we tend to use 787 00:30:38,092 --> 00:30:40,006 a lot more helium when when we're in 788 00:30:40,006 --> 00:30:40,405 cycle. 789 00:30:41,459 --> 00:30:43,556 So our l fire produces 790 00:30:44,255 --> 00:30:45,613 20 liquid is an hour. 791 00:30:46,412 --> 00:30:46,912 And 792 00:30:48,824 --> 00:30:49,780 when we're in cycle, 793 00:30:50,179 --> 00:30:52,252 we we can almost guarantee that the l 794 00:30:52,252 --> 00:30:54,564 fire will be running throughout throughout the cycle. 795 00:30:54,803 --> 00:30:56,956 So it's it's it's quite a lot we 796 00:30:56,956 --> 00:30:57,410 get 797 00:30:58,088 --> 00:31:00,003 So in in cycle, does that mean when 798 00:31:00,003 --> 00:31:03,036 the when when you're producing neutrons and ons 799 00:31:03,036 --> 00:31:05,430 when people are doing experiments. Yeah. Right. Yeah. 800 00:31:06,321 --> 00:31:08,149 Okay. So so it sounds to me that, 801 00:31:08,228 --> 00:31:09,897 you know, you you you have to put 802 00:31:09,897 --> 00:31:12,599 quite a bit of effort into into keeping 803 00:31:12,599 --> 00:31:14,799 your helium in the pipes, and then 804 00:31:15,318 --> 00:31:18,667 recycling it. Are are there alternatives to to 805 00:31:18,667 --> 00:31:21,400 using helium for some cryo 806 00:31:22,017 --> 00:31:22,814 applications at Isis? 807 00:31:23,452 --> 00:31:25,719 Yeah. So So we can use 808 00:31:26,491 --> 00:31:27,945 close like refrigerators 809 00:31:28,478 --> 00:31:29,932 to to call our samples, 810 00:31:30,942 --> 00:31:33,748 such as pulse shoots. However, you know, they 811 00:31:33,748 --> 00:31:36,245 are slower to reach low temperatures, 812 00:31:37,024 --> 00:31:39,581 and they won't go below 4.5 k. 813 00:31:41,035 --> 00:31:43,434 That there is also the argument that this 814 00:31:43,434 --> 00:31:45,134 uses a lot of electricity 815 00:31:45,434 --> 00:31:48,234 as opposed to use helium that has already 816 00:31:48,234 --> 00:31:49,009 been recycled 817 00:31:49,768 --> 00:31:52,162 Oh, I see. Oh, that's interesting because I 818 00:31:52,162 --> 00:31:53,757 mean, I would have thought that, you know, 819 00:31:53,917 --> 00:31:54,816 sort of re 820 00:31:55,912 --> 00:31:58,560 helium would that that that would have a 821 00:31:58,560 --> 00:32:01,194 certain energy cost to it. But but you're 822 00:32:01,194 --> 00:32:03,769 saying that that that is more efficient than 823 00:32:03,907 --> 00:32:04,865 than using these... 824 00:32:07,033 --> 00:32:07,990 Mechanical coolers. 825 00:32:08,628 --> 00:32:11,122 Yeah. Yeah. Because because we're we're l 826 00:32:12,537 --> 00:32:14,313 virtually all the time. Is 827 00:32:15,023 --> 00:32:17,406 it sort of offset the electrical side of 828 00:32:17,406 --> 00:32:19,789 using a Cc. And As was as I 829 00:32:19,789 --> 00:32:22,649 mentioned in the intro, Helium is also used 830 00:32:22,649 --> 00:32:25,443 in in party balloons And I think a, 831 00:32:25,522 --> 00:32:26,578 you know, a lot of 832 00:32:27,029 --> 00:32:27,529 physicists, 833 00:32:28,140 --> 00:32:30,623 particularly those who work in cryo. 834 00:32:31,964 --> 00:32:33,798 Are, you know, a a gassed guest by 835 00:32:33,798 --> 00:32:36,351 this that, you know, they they see party 836 00:32:36,351 --> 00:32:38,605 balloons as a as a as wasting 837 00:32:39,461 --> 00:32:41,557 a a finite and very valuable 838 00:32:42,345 --> 00:32:42,663 resource. 839 00:32:43,695 --> 00:32:46,315 But you're you're involved in a program to 840 00:32:46,315 --> 00:32:48,958 to try to recover some of that helium 841 00:32:49,014 --> 00:32:51,333 that's used for balloons. Can you Can you 842 00:32:51,333 --> 00:32:52,450 tell us a bit about that? 843 00:32:53,407 --> 00:32:55,422 Yeah. So so I presented 844 00:32:56,597 --> 00:32:59,389 a local school to talk about the importance 845 00:32:59,389 --> 00:33:00,527 of recycling 846 00:33:01,638 --> 00:33:04,515 tied this into how we can recycle helium 847 00:33:04,515 --> 00:33:05,154 at Isis. 848 00:33:06,432 --> 00:33:07,971 So the school children 849 00:33:08,364 --> 00:33:11,229 and now recycle their helium balloons that would 850 00:33:11,229 --> 00:33:12,980 have otherwise being discarded. 851 00:33:14,174 --> 00:33:15,868 The this this helium 852 00:33:16,895 --> 00:33:18,805 that they're recycling. And it it will be 853 00:33:18,805 --> 00:33:20,499 used in experiments. 854 00:33:20,874 --> 00:33:21,374 And, 855 00:33:21,909 --> 00:33:23,443 you know, it's nice the children 856 00:33:23,833 --> 00:33:25,602 can have a direct impact 857 00:33:25,975 --> 00:33:28,275 on the science that is taking place Isis. 858 00:33:29,465 --> 00:33:31,706 I I think they should feel very proud 859 00:33:31,706 --> 00:33:32,664 that's what they're doing. 860 00:33:33,780 --> 00:33:35,455 And and how does that work? Do you... 861 00:33:36,333 --> 00:33:38,189 Do do you have, like, a big balloon 862 00:33:38,406 --> 00:33:40,661 that you you sort of d can't 863 00:33:40,973 --> 00:33:43,358 the helium from the small balloons into and 864 00:33:43,358 --> 00:33:45,902 then take that big balloon back to Isis. 865 00:33:46,061 --> 00:33:48,288 Is that how it works. We're we're able 866 00:33:48,288 --> 00:33:50,116 to receive the balloons from the school. 867 00:33:52,122 --> 00:33:54,374 Get get delivered to isis. So 868 00:33:54,750 --> 00:33:57,139 we simply just take the balloons and and 869 00:33:57,139 --> 00:33:58,971 run it through a small vacuum pump. 870 00:33:59,864 --> 00:34:01,862 At low pressure, which would just go back 871 00:34:01,862 --> 00:34:04,999 to our back to our large helium balloon 872 00:34:05,298 --> 00:34:06,357 bag. So 873 00:34:06,736 --> 00:34:09,545 yeah. It's very very quick. Very easy. Do 874 00:34:09,545 --> 00:34:11,778 do you think that's that's something that could 875 00:34:11,778 --> 00:34:13,851 be done on a larger scale. 876 00:34:14,968 --> 00:34:17,121 I mean, III have no idea, you know, 877 00:34:17,360 --> 00:34:19,471 but how how much Helium is used 878 00:34:20,248 --> 00:34:21,765 in the Uk, for example, 879 00:34:22,403 --> 00:34:25,357 you know, to to to inflate balloons. But 880 00:34:25,516 --> 00:34:27,368 I mean, could could this be something that 881 00:34:27,368 --> 00:34:29,046 could be done on a on a wider 882 00:34:29,046 --> 00:34:31,282 scale, do you think? For mine for my 883 00:34:31,282 --> 00:34:33,061 understanding. And this is sort of the first 884 00:34:33,120 --> 00:34:35,842 this this been really done around this. So, 885 00:34:36,239 --> 00:34:38,149 you know, it'd be great if if people 886 00:34:38,149 --> 00:34:38,786 could do that. 887 00:34:41,028 --> 00:34:42,778 Some from my understanding, there's only... 888 00:34:43,335 --> 00:34:44,869 I think there's only around 20 889 00:34:45,641 --> 00:34:46,755 helium recovery plants, 890 00:34:48,124 --> 00:34:50,441 in the in in in England. So 891 00:34:51,000 --> 00:34:52,699 I think it would be quite a challenge 892 00:34:52,758 --> 00:34:53,258 to 893 00:34:54,436 --> 00:34:55,335 implement something 894 00:34:56,444 --> 00:34:58,512 on a big scale. So... Lily, 895 00:34:59,547 --> 00:35:01,694 Good stuff. And and finally Dale, 896 00:35:02,331 --> 00:35:06,266 you your background, your training is in auto 897 00:35:06,402 --> 00:35:06,902 mechanics 898 00:35:07,436 --> 00:35:07,936 and 899 00:35:08,471 --> 00:35:09,186 and plumbing. 900 00:35:09,840 --> 00:35:10,579 Can you 901 00:35:11,280 --> 00:35:14,480 maybe tell our listeners how you became interested 902 00:35:14,480 --> 00:35:15,140 in working 903 00:35:15,599 --> 00:35:17,219 at Isis? And 904 00:35:17,774 --> 00:35:19,048 you know, you know, how how you got 905 00:35:19,048 --> 00:35:20,903 this job as Helium 906 00:35:21,359 --> 00:35:21,859 recovery 907 00:35:22,634 --> 00:35:24,760 manager. Yeah. I started off as 908 00:35:25,358 --> 00:35:26,018 a vehicle 909 00:35:26,874 --> 00:35:27,773 technician where 910 00:35:29,189 --> 00:35:30,247 where I was a teenager, 911 00:35:32,301 --> 00:35:34,145 you know. Play him with things in the 912 00:35:34,145 --> 00:35:34,463 garage. 913 00:35:35,972 --> 00:35:37,322 Yeah. And then it went from there. I 914 00:35:37,322 --> 00:35:39,545 got got got qualified as a vehicle technician 915 00:35:39,545 --> 00:35:41,710 and wanting to carry on learn in, so 916 00:35:41,869 --> 00:35:43,309 I don't I done some plumbing in and 917 00:35:43,309 --> 00:35:45,949 then moved on to some gas work. Yeah. 918 00:35:46,109 --> 00:35:47,550 So we're a job that was advertised at 919 00:35:47,710 --> 00:35:48,929 Isis, and 920 00:35:50,520 --> 00:35:52,588 we're gonna the cryo gen team. So so, 921 00:35:52,667 --> 00:35:53,462 yeah. I applied. 922 00:35:54,098 --> 00:35:55,450 And, yeah. I was fortunate to get it. 923 00:35:55,530 --> 00:35:58,154 So, yeah, I just always wanted to continue 924 00:35:58,154 --> 00:35:59,719 my learning and and 925 00:36:00,399 --> 00:36:00,798 you know, 926 00:36:01,518 --> 00:36:02,317 he can prove him. 927 00:36:03,915 --> 00:36:05,135 And with Cryo, 928 00:36:06,712 --> 00:36:08,550 you know, for for me every day is 929 00:36:08,550 --> 00:36:09,190 a school day, 930 00:36:09,924 --> 00:36:12,102 I'll always be learning with cryo. 931 00:36:12,481 --> 00:36:12,981 So 932 00:36:14,079 --> 00:36:16,635 yeah. Really really really fascinating to me really. 933 00:36:17,449 --> 00:36:19,210 And and what sort of advice would you 934 00:36:19,210 --> 00:36:20,829 give to somebody who has, 935 00:36:21,289 --> 00:36:22,809 you know, the technical skills, 936 00:36:23,609 --> 00:36:26,010 and wants to, you know, work in a 937 00:36:26,010 --> 00:36:26,829 in a scientific 938 00:36:27,302 --> 00:36:29,290 facility like Isis. What... 939 00:36:30,244 --> 00:36:32,630 Did you have any career advice for them? 940 00:36:33,186 --> 00:36:34,776 How how should they pursue that? 941 00:36:35,509 --> 00:36:36,628 Yeah. I'd I'd just say, 942 00:36:37,827 --> 00:36:40,463 you know, just just just keep keep learning. 943 00:36:41,582 --> 00:36:43,340 I didn't know what I wanted to do. 944 00:36:43,912 --> 00:36:46,319 Until I was in in my twenties. So, 945 00:36:46,455 --> 00:36:48,442 you know, there's there's there's plenty of time 946 00:36:48,442 --> 00:36:51,780 to, you know, find find the right route 947 00:36:51,780 --> 00:36:55,062 for you. I was very hesitant about applying 948 00:36:55,062 --> 00:36:57,773 for the job because I didn't have a 949 00:36:57,773 --> 00:36:58,273 certain 950 00:36:58,810 --> 00:36:59,310 qualifications 951 00:37:00,326 --> 00:37:00,826 around, 952 00:37:01,522 --> 00:37:02,022 Cryo 953 00:37:03,293 --> 00:37:05,930 but, yeah, gave a go, and yeah, I 954 00:37:05,930 --> 00:37:08,486 was lucky enough to, be accepted. So, yeah, 955 00:37:08,646 --> 00:37:10,658 I'd just say, you know, get get give 956 00:37:10,658 --> 00:37:12,414 it a go, You know? This is something 957 00:37:12,414 --> 00:37:14,410 you're interested in, You know, but go for 958 00:37:14,410 --> 00:37:17,124 it. Well, that's great. Thanks. Thanks for talking 959 00:37:17,124 --> 00:37:20,974 about Helium Recovery dell. That's that's 1 of 960 00:37:20,974 --> 00:37:23,375 my favorite subjects, so smell problems. 961 00:37:31,541 --> 00:37:33,217 I'm afraid that's all the time we have 962 00:37:33,217 --> 00:37:36,351 for this week's podcast. Thanks to dale keeping 963 00:37:36,743 --> 00:37:38,414 David Jenkins and Mat team 964 00:37:39,210 --> 00:37:42,075 For joining me today and a special thanks 965 00:37:42,075 --> 00:37:43,826 to our producer Fred Isles. 966 00:37:44,479 --> 00:37:46,735 I hope you've been enjoying the new music 967 00:37:46,954 --> 00:37:47,853 in the podcast. 968 00:37:48,311 --> 00:37:50,487 It's called 137 969 00:37:50,546 --> 00:37:53,441 and was composed and performed by the physicist 970 00:37:53,914 --> 00:37:54,813 Philip Lori. 971 00:37:55,588 --> 00:37:58,240 He talks about the significance of that number 972 00:37:58,298 --> 00:38:01,327 and the creative process involved in making the 973 00:38:01,327 --> 00:38:01,827 music 974 00:38:02,218 --> 00:38:04,940 over on the Physics World stories podcast. 975 00:38:05,552 --> 00:38:07,377 And you can listen to that on the 976 00:38:07,536 --> 00:38:11,304 Physics World website or at your favorite podcast 977 00:38:11,518 --> 00:38:11,914 provider. 978 00:38:12,549 --> 00:38:13,739 Just look for the headline, 979 00:38:14,294 --> 00:38:17,570 swift earthquakes and new podcast music 980 00:38:18,278 --> 00:38:20,670 inspired by the fine structure constant. 981 00:38:21,706 --> 00:38:24,656 And you heard right, the podcast also looks 982 00:38:24,656 --> 00:38:26,511 at the seismic activity 983 00:38:26,984 --> 00:38:29,405 associated with Taylor Swift concerts 984 00:38:29,864 --> 00:38:30,764 with the si 985 00:38:31,704 --> 00:38:32,204 Jacqueline 986 00:38:32,824 --> 00:38:33,964 Kaplan Hour,