Teaching nuclear physics using data rather than models, recovering helium from party balloons

Physics World Weekly Podcast

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.

2024-06-06 39 min Transcript

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Transcript

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Hello and welcome to the physics world weekly

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podcast.

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I'm Hamish Johnston,

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Coming up in this episode, I'm in conversation

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with Dale Keeping, who is helium recovery manager

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at the Uk's Isis,

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Neutron and

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Source.

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He explains how Helium is used at the

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facility,

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where the gas comes from.

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And how he and his colleagues manage this

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non renewable resource.

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Dale also chats about an outreach initiative. That

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involves collecting used party balloons so that the

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helium they contain can be reused at Isis.

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Blood first, physics world's mat team

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Is in

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conversation with David Jenkins.

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Who has written a series of textbooks

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that take a different approach to teaching nuclear

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physics.

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Focusing first on how the data lead to

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physical models,

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rather than beginning with models and theories.

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Hello, and I'm delighted to be joined by

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David Jenkins, a nuclear physicist at University of

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York. Welcome to the podcast, David. Thank you.

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I'm happy to be you. Now remember, we

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let years ago at an Institute of Physics

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awards dinner, and I remember you wrote a

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feature for us about nuclear physics and its

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role on life on Earth.

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But since then you've written a couple of

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ebooks for Io about nuclear physics, and it's

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given you some insights into how we should

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teach. The subject

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to students.

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But before we come to that, I thought

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we'd just start with some the basics.

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So what what are the are the big

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questions in nuclear physics right now for people

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who haven't been keeping an eye on things?

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Well, III think there's many. I mean, there's

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lots of very technical.

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Issues. But I think the issues are are

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most interesting,

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to to the wider public. Or about the

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origin of the chemical elements

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And

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nuclear physics is is really

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underpins

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what elements are produced and the import abundant

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is in our in our universe, and that's

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got very exciting

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in the last few years because,

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from the discovery of gravitational waves, and then

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this light being emitted when when these objects

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are colliding id, it's rein,

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the whole field of nuclear physics is a

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huge number of questions now about.

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The origin of the elements.

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And that that kinda of tall with your

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own particular research interests that I think. Is

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that right in saying that? Yeah. So I've

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I've I've worked a lot on, they say

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everything that's called nuclear astro physics that relates

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to the origin of the elements, particularly at

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the moment. I've been working on

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fusion

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in massive stars, what what what what's going

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on in in stars that are 8 to

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20 times more massive than our son.

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But I'm also equally interested in just the

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pure aspects of nuclear structure

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and the properties of the atomic nucleus.

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So I mean, looking back to my undergraduate

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days, I actually did a degree in chemical

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physics. I don't think there was much nuclear

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physics on the syllabus, but what typically do

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you physics students that undergraduate level learn about

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nuclear physics. How much

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is there on the curriculum?

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There can be quite quite a lot. I

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mean, it

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in our university

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here at York.

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There's quite there's quite a bit on on

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the curriculum in there even for the... For

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the core program, and the part of the

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physics. I you can take options and study,

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even in into your third or 4 year

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of your degree. But at least in the,

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second year of the degree, there's a there's

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a lot of,

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sang to deal with nuclear physics

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probably as much as we discuss particle called

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Physics exceptionally. Yeah but that might be because

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we've got a lot of near nuclear physicists

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year.

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And and lots not so many particles ones.

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So, I thought we've turned to the new

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books that you've been writing. You wanna say

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a little bit about them. Yes. So this

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is working with Io publishing

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for their physics books series.

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We proposed a a series of books on

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nuclear structure

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and nuclear spectroscopy,

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and And

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that's been a very, very interesting

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evolution actually because of also because of events

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because we we signed up to

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I'm gonna deliver some of these books just

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before the Covid

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struck. And then when the Covid arrived,

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it we we suddenly had huge amounts of

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time to play with to and actually, in

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a way it was very therapeutic

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because we're able to spend all this time

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thinking about writing,

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and thinking about how to approach writing the

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books.

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And, of course,

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the Covid also drew it into another perspective

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because libraries were closed, You know, you couldn't

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go and get a physical book.

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You you weren't sure perhaps of that time.

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You you'd go to a library ever again.

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And so he really opened up the possibilities

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of what. Could be done with electronic,

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major and electronic rocks for. Because of course

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these are, ebooks published fines to your physics,

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publishing

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so, I mean, who who who would they

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be aimed at? Are they mostly aimed at

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undergraduate or post grad students?

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Yeah. I think they would probably be aimed

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at. To the the final year undergraduate students,

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but mostly,

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postgraduate students doing ph d or or masters

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in in in nuclear physics.

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So that's the sort of target audience

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that we have

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And and you... You told me you've kind

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of taken a different approach to other nuclear

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physics textbook. I mean, what's?

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What approach have you taken and how how

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does it differ? Would you say? Yeah. I

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think this is quite interesting because as I

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said, we we spent quite a bit of

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time thinking about how to approach. This. So

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I I work with my my main collaborator

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on these books. Is called John Wood, and

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he's a retired professor at Georgia

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tech in in the Us and he has,

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you know, an enormous number of years of

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experience of teaching, and I I've talked for

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a lot of years now,

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And, of course, you you start getting interested

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in

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in Pe.

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How how to teach

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how how to convey

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ideas to students,

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how how to challenge them how to make

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them involved and interested

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in in learning and

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And as I say, that that that led

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us into thinking about how to use books

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and so on. So I mean, historically, if

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you go back and look at nuclear physics

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text books.

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They tend to start with models,

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and they often tend to start in a

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rather kind of

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should 1 say biblical kind of way like

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a biblical authority, you know, here was the

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the model of of the shell model

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which is historical model going back to the

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the, sort of early 19 fifties.

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And

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there's nothing wrong with these models, but

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it it it's kind of

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so us of very old fashioned way of

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of of teaching the subject,

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and that it can be dry

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and boring.

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And and sometimes these models

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have become less useful as people have got

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more data and looked at these models. They

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found that there's... Problems with these models, and

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that the the the data doesn't really fit

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the models.

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And then sometimes people have come along and

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added a few more parameters of models and

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know because you know from your your involvement

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science, you can keep adding parameters to models

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and fit anything, but then it cease to

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be,

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physics.

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So we're trying to turn the whole thing

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around and start with data

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in our approach rather than,

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with models

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So when you say data, what you mean

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data that people have got from physics experiments?

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And what do you present real data or

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you sort of look at the kind of

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typical data that 1 would get?

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Yes. So so there's there's an enormous,

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comp,

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and databases of data.

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Out there nuclear data. So that's all sorts

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of properties of nuclei light. Let's take, for

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example, their gross properties. So let the the

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massive nuclei.

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Their radius.

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These are gross properties that people have measured.

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We also have excited states of nuclei.

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The nucleus is a quantum system, so it

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has quantized the excited states of specific,

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energy. There are also

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transitions between

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nuclear excited states.

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And because of the energy regime that it's

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in, those transitions media by gamma rays, which

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are very high energy,

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form of

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electromagnetic

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radiation light.

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So we have all of those databases there

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and because, of course,

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the nucleus is exploited in various ways like,

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for nuclear energy

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and for medicine and things like that, it's

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very important that people have compiled all this

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data over the years So there's a huge

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amount of data there,

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that that can be touched and then used

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more more around

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learning from.

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So do you think that makes the subject

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more accessible it becomes more real and and

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less dry as you say because people can

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see

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real date and kind of

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kind of intrigued by it and what that

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might tell us. Yes. I think that's what

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we tried to do. We tried to say,

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let's look at the data.

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And let's see if simple patterns emerge from

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the data and let's not start with traditional

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models like this shell model, which has the

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a concept that there are certain magic numbers

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of protons and neutrons

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for which the system

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has closed shells. It's called a bit like

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closed shells in a in an atom. So

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in an atom, you have the,

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you're you have chemical

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chemistry background. So we have these things noble

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gases that have no chemistry

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because they have closed shells of electrons, and

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we have certain nuclei that have closed shells

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approach tolls and neutrons and they're quite hard

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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,

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