WEBVTT - The Matter of Everything, with Suzie Sheehy

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<v Speaker 1>Welcome to Stuff to Blow Your Mind, a production of iHeartRadio.

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<v Speaker 2>Hello, and welcome to the Stuff to Blow Your Mind podcast.

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<v Speaker 2>My name is Joe McCormick. My regular co host, Robert

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<v Speaker 2>Lamb is not with me today, but he'll be joining

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<v Speaker 2>again next time. Today's episode is going to be an interview.

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<v Speaker 2>This is a conversation I had with the accelerator physicist

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<v Speaker 2>and author Susie Sheehy about her recent book The Matter

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<v Speaker 2>of Everything, How Curiosity, Physics and Improbable Experiments Changed the World.

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<v Speaker 2>Susie's publisher sent us a copy of this book for review,

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<v Speaker 2>and I really loved it. So it's a history of

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<v Speaker 2>modern physics experiments from Runken's cathode ray tube and the

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<v Speaker 2>discovery of X rays all the way up to the

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<v Speaker 2>Large Hadron Collider and beyond. And what makes this book

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<v Speaker 2>really special, in my opinion, is that it focuses not

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<v Speaker 2>just on theoretical advancements, but on the labor of designing

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<v Speaker 2>and building experiments to test those new ideas. And because

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<v Speaker 2>it illuminates so much about the experimental apparatus behind the

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<v Speaker 2>progress of science, I think this book has a lot

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<v Speaker 2>of interesting things to say, not just about the history

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<v Speaker 2>of our quest to understand matter and energy, but about

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<v Speaker 2>epistemology and critical thinking and work to read from her

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<v Speaker 2>author bio. Susie Shehe is a physicist, science communicator and

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<v Speaker 2>academic who divides her time between her research groups at

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<v Speaker 2>the University of Oxford and the University of Melbourne. Her

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<v Speaker 2>research addresses both curiosity driven and applied areas, and is

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<v Speaker 2>currently focused on developing new particle accelerators for applications in medicine. Again,

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<v Speaker 2>the book is called The Matter of Everything and I

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<v Speaker 2>guess that does it. For the introduction, Here is my

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<v Speaker 2>interview with Suzie Shehe. Susi Shehey, Welcome to the podcast.

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<v Speaker 3>Thanks Jen, nice to be here.

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<v Speaker 2>So I wanted to start off talking about how I

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<v Speaker 2>think a lot of the histories of physics that I've

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<v Speaker 2>read focus more on the theoretical side, like what led

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<v Speaker 2>to the insights theoretical physicists had, how they dreamed up

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<v Speaker 2>their models, and things like that. I really loved that

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<v Speaker 2>this book was intensely focused on the experimental component of physics,

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<v Speaker 2>and there was a lot of focus on the details

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<v Speaker 2>of the experiments, how they did it, and understanding experiments

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<v Speaker 2>as human projects operating under constraints. What kind of insights

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<v Speaker 2>do you think are revealed by looking at the history

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<v Speaker 2>of particle physics through the experimental lens, in particular, especially

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<v Speaker 2>things that you might miss if you only talk about

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<v Speaker 2>physics as a sort of history of ideas.

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<v Speaker 3>Yeah, you phrased that so beautifully in there by the way,

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<v Speaker 3>the importance of experiments. So I'm an experimental physicist, right.

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<v Speaker 3>So one of the things that I observed when I

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<v Speaker 3>sort of start on the journey of writing this book

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<v Speaker 3>was that almost every other comparable book was written by

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<v Speaker 3>a theoretical physicist, And so you'd get these stories where

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<v Speaker 3>you get this wonderful insight of say, either Einstein or

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<v Speaker 3>one of the key theoretical physicists of the age, And

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<v Speaker 3>it was like it was almost like they came to

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<v Speaker 3>these insights purely from their own personal genius, right. And

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<v Speaker 3>this was the story of physics that I was taught

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<v Speaker 3>pretty much when I did at university as well. But

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<v Speaker 3>it was also the story that comes across in these books.

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<v Speaker 3>And I don't know whether this is just like an egotistical,

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<v Speaker 3>aggrandizing thing that people do. Certainly these people are very

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<v Speaker 3>very smart, right, but they're not islands and I think

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<v Speaker 3>that's one of the key insights that you get from

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<v Speaker 3>taking a different approach to looking at the history and

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<v Speaker 3>looking more at the experiments and more at the wider

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<v Speaker 3>view of how physics progresses. And I think any theoretical

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<v Speaker 3>physicists today would all and hopefully also though is historically,

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<v Speaker 3>would admit that, you know, their work is nothing without

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<v Speaker 3>the work of the experimentalists, because at the end of

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<v Speaker 3>the day, physics is a subject which is trying to

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<v Speaker 3>describe the universe, our actual universe, not just some theoretical

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<v Speaker 3>mathematical universe that doesn't really exist. And so the only

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<v Speaker 3>way to meet those two things in the middle is

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<v Speaker 3>through experiment. You have to actually get out there and

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<v Speaker 3>test nature. But that's where a lot of people, i

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<v Speaker 3>think naively think that we just we know what we're

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<v Speaker 3>doing with that that we just we can go out

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<v Speaker 3>there and build an experiment and test or find this thing,

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<v Speaker 3>and that once the theorist predicts it, that it's a

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<v Speaker 3>straightforward journey. So that's I think the next sort of

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<v Speaker 3>key insight there is that it is not a straightforward

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<v Speaker 3>journey to discover and uncover the nature of our universe,

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<v Speaker 3>especially on these tiny scales. That we're looking at that

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<v Speaker 3>are so much smaller than what we can see with

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<v Speaker 3>our own eyes. And so when you delve into that, then,

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<v Speaker 3>as you say, there's this detailed development of how experiments

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<v Speaker 3>actually work, whether that's electronically, whether that's because they require

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<v Speaker 3>two thousand people with different expertise to actually put them together,

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<v Speaker 3>and also just that co development of technology and instrumentation

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<v Speaker 3>along with the development of ideas and insights about the universe,

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<v Speaker 3>and it really is sort of a synergistic development. So

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<v Speaker 3>there's I think a few things there about throwing out

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<v Speaker 3>the lone genius stereotype, managing to recognize how important it

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<v Speaker 3>is that we actually interact in the real world and

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<v Speaker 3>do experiments, and then just the unpredictable nature of doing

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<v Speaker 3>those experiments at all.

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<v Speaker 2>You mentioned in the book that some people think that

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<v Speaker 2>Diract's equation is the most beautiful equation in all physics.

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<v Speaker 2>I'm sure that people who have a lot of math

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<v Speaker 2>and physics knowledge would consider that subjective, but it made

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<v Speaker 2>me curious about the different ways that instruments within science

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<v Speaker 2>can be perceived not only as useful or accurate, but

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<v Speaker 2>sometimes esthetically beautiful. So I was wondering about the other

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<v Speaker 2>side of that, as an experimentalist, do you have an

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<v Speaker 2>opinion on what is the most beautiful experiment in all

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<v Speaker 2>of physics? Or do you have at least a few candidates?

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<v Speaker 3>Oh, that's nice. Yeah, I think I definitely appreciate the

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<v Speaker 3>beauty of a well designed experiment that can sort of

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<v Speaker 3>cut through all the background noise and find the thing

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<v Speaker 3>that they're looking for. But I'd say I appreciate the

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<v Speaker 3>beauty of an experiment in multiple dimensions though, right, so

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<v Speaker 3>you can. I can appreciate the beauty of an experiment

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<v Speaker 3>which serendipitously found something that it didn't expect, as well

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<v Speaker 3>as appreciating, you know, the sort of really well designed,

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<v Speaker 3>very specific experiment. But now you're putting me on the

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<v Speaker 3>spot if you ask me what my favorite experiment was.

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<v Speaker 3>I mean, in the book, I really focus on twelve

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<v Speaker 3>key experiments that I chose from what could have been thousands, honestly,

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<v Speaker 3>and focused on how those had contributed to our knowledge

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<v Speaker 3>of particle physics over about the last one hundred and

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<v Speaker 3>twenty years. And I think it's easier probably for me

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<v Speaker 3>to choose a favorite from the earlier ones of those

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<v Speaker 3>because they're smaller. It's easier to understand all the different

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<v Speaker 3>parts of the experiment. And so in that sense, in

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<v Speaker 3>a beauty and esthetic appreciation sense, I think I'm going

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<v Speaker 3>to say the cloud chamber. And this was developed in

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<v Speaker 3>the early nineteen hundreds by a physicist named CITR Wilson,

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<v Speaker 3>Charles Wilson, whose first love was actually meteorology, but he

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<v Speaker 3>was working in the Cavender just Labin, Cambridge in the UK,

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<v Speaker 3>alongside all the people doing all the early work in radioactivity,

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<v Speaker 3>so he was very well versed in radioactivity and those ideas.

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<v Speaker 3>But he invented this chamber originally to try and study

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<v Speaker 3>clouds and the interaction of light and electricity in the atmosphere.

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<v Speaker 3>And then he later realized when someone held an X

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<v Speaker 3>ray tube, well, he and a colleague held an X

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<v Speaker 3>ray tube to the side of it, that he could

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<v Speaker 3>see the passage of radiation through this chamber, which had

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<v Speaker 3>a sort of in his case water vapor and nowadays

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<v Speaker 3>we use alcohol vapors, and these little trails would form

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<v Speaker 3>like little tracts of cloud as the radiation went through

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<v Speaker 3>and left a little bit of energy inside the chamber.

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<v Speaker 3>And I find this beautiful because it's really the first

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<v Speaker 3>time as a species that we get to visualize radiation.

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<v Speaker 3>We get to visualize this thing which is otherwise extremely

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<v Speaker 3>abstract and difficult to understand, and now we're seeing its

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<v Speaker 3>effects almost in real time, so you can photograph as

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<v Speaker 3>particles pass through. And then we get and I think

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<v Speaker 3>the beauty comes in because it's this lovely interaction between

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<v Speaker 3>our own capacities as humans and the development of a

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<v Speaker 3>new instrumentation. Because then you can take you can leave

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<v Speaker 3>these chambers up on mountains, so you can take photographs

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<v Speaker 3>of the interactions there, and from that we discover lots

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<v Speaker 3>of new things, including we discover antimatter for the first time.

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<v Speaker 3>So the positron is the opposite version of the electron,

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<v Speaker 3>and when they come together they annihilate. But they can

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<v Speaker 3>also be produced in pairs electron positron pairs. And there

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<v Speaker 3>were positrons detected by a guy called Karl Anderson in

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<v Speaker 3>the US, and he discovered them in his experiments before

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<v Speaker 3>he'd read about Direct's beautiful equation. I'm coming back to

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<v Speaker 3>the equation again now. He actually wasn't aware of Dirac's work,

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<v Speaker 3>which was published in nineteen twenty nine, but in nineteen

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<v Speaker 3>thirty two he'd built this enormous chamber with this huge

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<v Speaker 3>magnet around it and legged it up a mountain and

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<v Speaker 3>discovered this type of anti matter. And I find that

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<v Speaker 3>really beautiful because then he's literally able to use our

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<v Speaker 3>internal sort of track recognition, our pattern finding system, our

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<v Speaker 3>brain to look at the photographs and actually see that

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<v Speaker 3>there's something new there. And there were other particles discovered

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<v Speaker 3>later as well, the new one being a key one,

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<v Speaker 3>which is a heavy version of an electron, and it

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<v Speaker 3>was really the instrument of choice for many many years

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<v Speaker 3>in the field, and it came from a meteorologists. So

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<v Speaker 3>I don't know, there's something in that story for me

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<v Speaker 3>which is just beautiful about how we can use our

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<v Speaker 3>creativity and sort of reuse of ideas in adjacent fields

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<v Speaker 3>to really make amazing discoveries.

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<v Speaker 2>Yeah. I love that example too, And there's a kind

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<v Speaker 2>of beauty and a kind of lightness and elegance to

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<v Speaker 2>it that in a way seems contrasted by other experiments

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<v Speaker 2>you described that are also incredibly important and wonderful stories

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<v Speaker 2>to understand, Like one that stands sort of opposite it

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<v Speaker 2>in my mind is the story of Ernest Lawrence's team

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<v Speaker 2>and their cyclotron and this chapter struck me as interesting

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<v Speaker 2>in part because I think this is the one where

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<v Speaker 2>you illuminate a history of what struck me as interesting.

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<v Speaker 2>Mistakes like you mentioned a faulty reading from an accelerator

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<v Speaker 2>experiment due to I think it was like deuteron coding

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<v Speaker 2>on target elements. Please correct me if I'm getting this wrong.

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<v Speaker 2>And also an incident where they accidentally made the whole

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<v Speaker 2>lab radioactive without realizing it, which interfered with their measurements

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<v Speaker 2>on on a Geiger counter like device. So what is

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<v Speaker 2>the role of error and making a mess in scientific experiments?

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<v Speaker 3>Do you know? I've been thinking about this more since

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<v Speaker 3>writing the book, and I think we don't. I think

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<v Speaker 3>we don't acknowledge the role of error and failure enough

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<v Speaker 3>in science. In fact, we try and cover it up.

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<v Speaker 3>It's a huge there's a huge issue in fact with

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<v Speaker 3>if I failed experiments not being published, and in some fields

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<v Speaker 3>like medicine, that's that's a huge issue. Actually in physics

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<v Speaker 3>it's less of an issue, but it still happens. But

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<v Speaker 3>Ernest Lawrence's example of the cyclotone is a fantastic example

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<v Speaker 3>where by sort of realizing their mistakes and their errors,

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<v Speaker 3>they really made progress in their understanding. So, as you say,

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<v Speaker 3>they developed this particle accelerator, this circular machine, and then

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<v Speaker 3>over time they realized that they're not seeing the results

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<v Speaker 3>that they think they should be seeing because, for example,

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<v Speaker 3>in one situation, basically everything had become radioactive and so

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<v Speaker 3>all of their measurement devices were just picking up all

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<v Speaker 3>the background radiation and not the radiation they were trying

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<v Speaker 3>to look for. But that helped them understand what was

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<v Speaker 3>happening in the machine as it was accelerating, and they

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<v Speaker 3>missed a number of key discoveries that were made by

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<v Speaker 3>other research groups around the world, but they didn't mind

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<v Speaker 3>too much. And Lawrence sort of had this mindset which

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<v Speaker 3>is relevant to the question of errors and failures, which is,

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<v Speaker 3>you know, he sort of would like to say, there's

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<v Speaker 3>research enough for everyone, or there's discovery enough for everyone.

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<v Speaker 3>And so he was this big believer that he was

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<v Speaker 3>quite quite a futurist, I guess because at the start

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<v Speaker 3>of his career he was I think late to in

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<v Speaker 3>his early thirties when he first invented the cyclotron, and

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<v Speaker 3>he invented it because he couldn't see a path of

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<v Speaker 3>the existing technology. To the end of his career even

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<v Speaker 3>you know, he was sort of looking thirty years in

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<v Speaker 3>the future, going, well, these technologies are just they're going

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<v Speaker 3>to be outdated by the time I get to that point,

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<v Speaker 3>so I'm going to have to invent something new to

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<v Speaker 3>give myself, you know, a path of growth through my career.

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<v Speaker 3>And boy did he get it, you know, he really

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<v Speaker 3>The cycloton was an incredible invention and they're still built

0:13:29.360 --> 0:13:33.880
<v Speaker 3>today in hospitals to generate radioisotopes for medical procedures, which

0:13:33.880 --> 0:13:38.200
<v Speaker 3>is very, very useful. But obviously along the way he

0:13:38.280 --> 0:13:41.479
<v Speaker 3>could be perceived at having failed to make key discoveries

0:13:41.880 --> 0:13:45.920
<v Speaker 3>in physics. So I think induced radioactivity was one of

0:13:45.960 --> 0:13:48.520
<v Speaker 3>the ones that he missed actually, and was found by

0:13:48.640 --> 0:13:55.920
<v Speaker 3>Julio and Currie in France. That's Marie Kirey's daughter, arenar Kiri.

0:13:57.640 --> 0:13:59.840
<v Speaker 3>So I've been thinking about this since writing the book,

0:14:00.320 --> 0:14:02.240
<v Speaker 3>and I think I'd like to make the analogy with

0:14:03.679 --> 0:14:06.439
<v Speaker 3>in the arts, right, So, if you have a creative

0:14:06.480 --> 0:14:10.480
<v Speaker 3>practice in the arts, failure is an error. It's just

0:14:10.480 --> 0:14:12.839
<v Speaker 3>an inherent part of it. And it's also very much

0:14:12.880 --> 0:14:16.120
<v Speaker 3>acknowledged that by failing or making an error, you may

0:14:16.280 --> 0:14:18.920
<v Speaker 3>just stumble upon something new, a new way of doing

0:14:18.960 --> 0:14:23.080
<v Speaker 3>something a new invention. I'm even thinking in the culinary world,

0:14:23.120 --> 0:14:26.920
<v Speaker 3>you know. I know of a chef who now runs

0:14:27.120 --> 0:14:30.560
<v Speaker 3>a three Michelin starred restaurant in the UK, and one

0:14:30.600 --> 0:14:33.520
<v Speaker 3>day he accidentally dropped hot coal into a vat of

0:14:33.520 --> 0:14:38.680
<v Speaker 3>cooking oil, and so they later, you know, decided to

0:14:38.680 --> 0:14:40.960
<v Speaker 3>taste it and see how it tasted, and it tastes

0:14:41.000 --> 0:14:43.720
<v Speaker 3>it amazing, and he uses it in his signature dishes

0:14:43.760 --> 0:14:46.840
<v Speaker 3>in a three Michelin starred restaurant now. And I love

0:14:46.920 --> 0:14:50.960
<v Speaker 3>those stories of where errors lead you to new things

0:14:50.960 --> 0:14:53.880
<v Speaker 3>and new ideas. And I do think in science we

0:14:54.280 --> 0:14:56.280
<v Speaker 3>shy away a little bit from that, or we like

0:14:56.320 --> 0:14:58.040
<v Speaker 3>to sort of cover it up and then we publish

0:14:58.040 --> 0:15:00.760
<v Speaker 3>a paper that says the story was a linear one.

0:15:00.760 --> 0:15:04.400
<v Speaker 3>And you know, we made all these discoveries, and in

0:15:04.520 --> 0:15:07.800
<v Speaker 3>digging into the history of these experiments, which were so

0:15:07.920 --> 0:15:12.760
<v Speaker 3>critical in understanding particle physics, I did discover that there

0:15:12.840 --> 0:15:17.040
<v Speaker 3>was probably more failure than even I expected. And as

0:15:17.080 --> 0:15:20.560
<v Speaker 3>an experimentalist myself, I've just come to accept that I

0:15:20.600 --> 0:15:23.160
<v Speaker 3>often don't fully know what I'm doing because no one

0:15:23.200 --> 0:15:26.360
<v Speaker 3>has ever tried to do it before, and that sometimes

0:15:26.400 --> 0:15:28.240
<v Speaker 3>I'm going to try things and they're going to fail.

0:15:28.400 --> 0:15:31.680
<v Speaker 3>And there's a constant process in my lab with my

0:15:31.720 --> 0:15:35.320
<v Speaker 3>students and staff of sort of openly talking about this

0:15:35.640 --> 0:15:37.880
<v Speaker 3>right in it, you know, being candid about it and

0:15:38.160 --> 0:15:40.080
<v Speaker 3>sort of being like that's all right, you know, like

0:15:40.520 --> 0:15:42.880
<v Speaker 3>it's okay that it failed. You didn't know what you

0:15:42.880 --> 0:15:46.360
<v Speaker 3>were doing, because nobody knew what they were doing. But

0:15:46.480 --> 0:15:49.800
<v Speaker 3>for example, you know, you might consider an earlier experiment

0:15:49.840 --> 0:15:52.520
<v Speaker 3>in the book by William Rodkin, who discovered X rays,

0:15:52.960 --> 0:15:56.200
<v Speaker 3>and he discovered them because a sort of painted fluorescent

0:15:56.240 --> 0:16:00.560
<v Speaker 3>screen across his lab was glowing when he had a tube,

0:16:00.920 --> 0:16:04.960
<v Speaker 3>a cathoedray tube in his lab, and he noticed the

0:16:04.960 --> 0:16:07.880
<v Speaker 3>glow and he decided to investigate it. Now, we often

0:16:07.920 --> 0:16:11.960
<v Speaker 3>refer to that as serendipitous, but depending on your perspective,

0:16:12.040 --> 0:16:13.840
<v Speaker 3>you might consider it to be an error. You know,

0:16:13.880 --> 0:16:17.520
<v Speaker 3>you probably shouldn't have had the wrong detector, you know,

0:16:17.800 --> 0:16:21.360
<v Speaker 3>sort of out in the lab at the time. The

0:16:21.400 --> 0:16:23.640
<v Speaker 3>other person that comes to mind is Robert Millican, who

0:16:23.680 --> 0:16:28.280
<v Speaker 3>did twelve years worth of experiments trying to measure what's

0:16:28.320 --> 0:16:31.360
<v Speaker 3>called the photoelectric effect, which is the electrical current that

0:16:31.400 --> 0:16:35.920
<v Speaker 3>flows when you shine light on particular metals. And this

0:16:35.960 --> 0:16:38.760
<v Speaker 3>is an interesting one where along the ways, the early

0:16:38.800 --> 0:16:42.520
<v Speaker 3>phases of quantum mechanics had come around, and Einstein in

0:16:42.560 --> 0:16:45.560
<v Speaker 3>particular had come out with this equation which predicted what

0:16:45.600 --> 0:16:48.680
<v Speaker 3>should happen when you shine this light onto different metals.

0:16:48.920 --> 0:16:54.040
<v Speaker 3>And the upshot of Einstein's theory was really abhorrent to

0:16:54.520 --> 0:16:58.320
<v Speaker 3>the experimentalist. To Robert Millican, he called it the reckless hypothesis.

0:16:58.480 --> 0:17:03.080
<v Speaker 3>And that's because this hype office has implied that light

0:17:03.160 --> 0:17:05.879
<v Speaker 3>would be acting more like a particle than like a

0:17:05.920 --> 0:17:09.199
<v Speaker 3>wave in this experiment. And so he set out to

0:17:09.200 --> 0:17:12.439
<v Speaker 3>prove Einstein wrong, spent twelve years in the lab trying

0:17:12.440 --> 0:17:14.800
<v Speaker 3>to do it, and all he did was pre Einstein

0:17:14.920 --> 0:17:17.840
<v Speaker 3>right to a better precision than anyone had before. So again,

0:17:17.920 --> 0:17:21.080
<v Speaker 3>you might think, and he even thought that he was failing, right.

0:17:21.240 --> 0:17:24.520
<v Speaker 3>He thought he was failing as an experimentalist. He was

0:17:24.560 --> 0:17:26.240
<v Speaker 3>really struggling with He had to build all his own

0:17:26.240 --> 0:17:29.560
<v Speaker 3>equipment from scratch. And then at the end of twelve

0:17:29.640 --> 0:17:32.520
<v Speaker 3>years he sort of comes out with this result, which

0:17:32.560 --> 0:17:36.040
<v Speaker 3>I think even when he published it he still didn't

0:17:36.040 --> 0:17:38.000
<v Speaker 3>fully believe, but he was able to sort of say, well,

0:17:38.040 --> 0:17:42.280
<v Speaker 3>it is consistent with Einstein's prediction. And then later on

0:17:42.480 --> 0:17:45.080
<v Speaker 3>about another ten years later, he was awarded the Nobel

0:17:45.119 --> 0:17:47.960
<v Speaker 3>Prize for that and another famous experiment that he did

0:17:48.000 --> 0:17:52.560
<v Speaker 3>about the charge on the electron, and he changes his tune.

0:17:52.560 --> 0:17:55.400
<v Speaker 3>And I found this fascinating that, you know, this very

0:17:55.440 --> 0:17:59.480
<v Speaker 3>fallible nature of the experimentalist, of sort of thinking one

0:17:59.480 --> 0:18:01.959
<v Speaker 3>thing is going to happen and holding this bias that

0:18:02.080 --> 0:18:05.240
<v Speaker 3>you know, no, nature can't possibly work that way. It's ridiculous.

0:18:05.280 --> 0:18:08.960
<v Speaker 3>It's you know, preposterous that a particle could be a wave.

0:18:09.160 --> 0:18:10.919
<v Speaker 3>You know, sorry, a light could be a wave and

0:18:10.960 --> 0:18:14.320
<v Speaker 3>a particle. And then he gets through his Nobel Prize

0:18:14.680 --> 0:18:18.920
<v Speaker 3>speech or lecture and then he's saying, you know, however,

0:18:18.960 --> 0:18:22.760
<v Speaker 3>many years ago when when I set out to demonstrate

0:18:22.840 --> 0:18:29.320
<v Speaker 3>Einstein's photoelectric theory, so so he's making out like him

0:18:29.400 --> 0:18:32.840
<v Speaker 3>meant to do it all along, and I was I

0:18:32.960 --> 0:18:36.440
<v Speaker 3>was shocked. I was like, did someone transcribe that incorrectly?

0:18:36.600 --> 0:18:41.320
<v Speaker 3>I don't think so. And so so it turns out that,

0:18:41.760 --> 0:18:44.320
<v Speaker 3>you know, I think his bias against it was what

0:18:45.520 --> 0:18:50.080
<v Speaker 3>it gave him this force, this will power to persist

0:18:50.080 --> 0:18:52.399
<v Speaker 3>at his experiment for twelve years because he was just

0:18:52.480 --> 0:18:54.560
<v Speaker 3>like emotionally he was just like, this cannot be right,

0:18:54.600 --> 0:18:58.240
<v Speaker 3>this cannot be right, and you know, you would you

0:18:58.280 --> 0:19:02.240
<v Speaker 3>would say that he if I in that enterprise because

0:19:02.760 --> 0:19:07.399
<v Speaker 3>he was wrong and Enstein was right. But this is

0:19:07.760 --> 0:19:09.679
<v Speaker 3>I think this is how science progresses, and it's an

0:19:09.720 --> 0:19:13.200
<v Speaker 3>important part of how science progresses is that, yes, we're

0:19:13.200 --> 0:19:16.000
<v Speaker 3>all human, we're all you know, we're coming with our biases,

0:19:16.040 --> 0:19:19.360
<v Speaker 3>we're very fallible. But isn't it amazing that we can then,

0:19:20.040 --> 0:19:24.159
<v Speaker 3>you know, use the scientific process and apply, you know,

0:19:24.240 --> 0:19:26.800
<v Speaker 3>as sort of apply things to that process to try

0:19:26.800 --> 0:19:30.800
<v Speaker 3>and UnBias ourselves from the results and come out with

0:19:31.760 --> 0:19:35.359
<v Speaker 3>the knowledge that is, you know, sort of accurate, regardless

0:19:35.359 --> 0:19:37.120
<v Speaker 3>of the fact that you didn't believe it going into

0:19:37.160 --> 0:19:38.960
<v Speaker 3>doing the experiment. I think, I think that's actually a

0:19:39.000 --> 0:19:40.720
<v Speaker 3>pretty amazing thing that we can do.

0:19:41.119 --> 0:19:55.560
<v Speaker 2>And like the culture of experiment is the constraint on that. Yes, yeah, well,

0:19:55.560 --> 0:19:59.639
<v Speaker 2>regarding ideas that are wrong but persistent. One of my

0:19:59.640 --> 0:20:04.160
<v Speaker 2>favorite characters in the book is Ernest Rutherford, And there's

0:20:04.160 --> 0:20:07.679
<v Speaker 2>a part where you quote Ernest Rutherford saying that he

0:20:07.760 --> 0:20:10.080
<v Speaker 2>was originally brought up to think of the atom as

0:20:10.680 --> 0:20:13.480
<v Speaker 2>I think the quote is a nice hard fellow red

0:20:13.560 --> 0:20:17.879
<v Speaker 2>or gray in color according to your taste, and that

0:20:17.960 --> 0:20:20.200
<v Speaker 2>struck me as very funny. But then you also mentioned

0:20:20.240 --> 0:20:25.119
<v Speaker 2>in a footnote that even many physicists, still, despite knowing better,

0:20:25.720 --> 0:20:29.480
<v Speaker 2>think of sub atomic particles and atoms as little balls.

0:20:30.800 --> 0:20:34.359
<v Speaker 2>How do you visualize sub atomic particles or do you

0:20:34.440 --> 0:20:36.879
<v Speaker 2>at all? And is there a better way we should

0:20:36.920 --> 0:20:41.520
<v Speaker 2>try to picture this scale of matter in the mind's

0:20:41.520 --> 0:20:43.359
<v Speaker 2>eye or is it pointless to even try?

0:20:44.680 --> 0:20:48.480
<v Speaker 3>So? I'm going to sheepishly admit that, like all the

0:20:48.520 --> 0:20:51.600
<v Speaker 3>other physicists I've asked, we don't want to admit it.

0:20:51.920 --> 0:20:54.280
<v Speaker 3>But because the first time we were ever introduced to

0:20:54.320 --> 0:20:58.520
<v Speaker 3>the concept of Adams and particles, they were little hard spares.

0:21:00.080 --> 0:21:03.359
<v Speaker 3>When you say protons and neutrons and electrons and the

0:21:03.400 --> 0:21:06.679
<v Speaker 3>atom I have. I have a terrible picture in my

0:21:06.760 --> 0:21:09.960
<v Speaker 3>head that's I know is completely wrong, and yet it persists.

0:21:11.000 --> 0:21:13.320
<v Speaker 3>You know, I have this this, Yeah, I have little

0:21:13.320 --> 0:21:17.080
<v Speaker 3>hard spheres in my mind, just like Rutherford did. And

0:21:17.680 --> 0:21:19.880
<v Speaker 3>I mean this is a This is a huge disservice

0:21:19.920 --> 0:21:23.840
<v Speaker 3>that we do ourselves, I think, by persisting to describe

0:21:23.840 --> 0:21:27.520
<v Speaker 3>in this way. But here's here's a I think a

0:21:27.640 --> 0:21:29.920
<v Speaker 3>key point about the models that we have in our heads.

0:21:29.920 --> 0:21:31.720
<v Speaker 3>And I will answer the question about how better to

0:21:31.800 --> 0:21:35.159
<v Speaker 3>visualize it in a moment. Physics and all the natural

0:21:35.160 --> 0:21:39.520
<v Speaker 3>sciences really are sciences of different scales, and all the

0:21:39.520 --> 0:21:41.199
<v Speaker 3>models that we have and all the theories that we

0:21:41.280 --> 0:21:44.719
<v Speaker 3>have apply on different scales. So if you're a chemist

0:21:44.840 --> 0:21:48.800
<v Speaker 3>or a biologist, it's well, other than some realms of chemistry,

0:21:49.359 --> 0:21:53.159
<v Speaker 3>it's probably okay for you to visualize atoms and particles

0:21:53.200 --> 0:21:57.720
<v Speaker 3>as little hard spheres because the models that predict the

0:21:57.760 --> 0:22:00.280
<v Speaker 3>behavior which you're interested in on the scale that you're

0:22:00.320 --> 0:22:03.280
<v Speaker 3>interested in, which is now more much more macroscopic than microscopic.

0:22:05.000 --> 0:22:07.560
<v Speaker 3>You know, it works perfectly fine, it can sort of

0:22:07.560 --> 0:22:12.760
<v Speaker 3>approximate it. And quantum mechanics, though, is obviously the science.

0:22:12.800 --> 0:22:15.320
<v Speaker 3>When we get down to that very very small level

0:22:16.280 --> 0:22:19.080
<v Speaker 3>and we've realized that it no longer works in the

0:22:19.119 --> 0:22:22.560
<v Speaker 3>same analogous way to say billiard balls on a billiard table,

0:22:23.080 --> 0:22:26.080
<v Speaker 3>and it works in a very different way. Everything is

0:22:26.160 --> 0:22:30.480
<v Speaker 3>much more probabilistic. Nothing is as certain. We can't know

0:22:30.600 --> 0:22:34.000
<v Speaker 3>things like the position and the momentum at the same

0:22:34.040 --> 0:22:39.439
<v Speaker 3>time precisely, so everything becomes a little fuzzier. If I

0:22:39.480 --> 0:22:42.919
<v Speaker 3>were to try and encourage you to properly visualize an atom.

0:22:43.520 --> 0:22:47.359
<v Speaker 3>First of all, you know, the central nucleus of an

0:22:47.400 --> 0:22:51.000
<v Speaker 3>atom is extremely dense and extremely small compared to the

0:22:51.040 --> 0:22:54.439
<v Speaker 3>outer side of the atom. And Rutherford had another beautiful

0:22:54.560 --> 0:22:59.160
<v Speaker 3>analogy for this, which is that if the electrons which

0:22:59.200 --> 0:23:01.960
<v Speaker 3>now you're considering in your head, the electrons to be

0:23:02.040 --> 0:23:04.880
<v Speaker 3>kind of a wave or a sphere or a sort

0:23:04.880 --> 0:23:07.240
<v Speaker 3>of much more, you know, much less like a little

0:23:07.280 --> 0:23:13.920
<v Speaker 3>hard dot and much more like a probability cloud, that

0:23:14.200 --> 0:23:18.439
<v Speaker 3>cloud would be at the walls of a cathedral. And

0:23:18.480 --> 0:23:20.560
<v Speaker 3>if that was the size of a cathedral, then the

0:23:20.680 --> 0:23:22.840
<v Speaker 3>nucleus in the center would be the size of a

0:23:22.880 --> 0:23:26.480
<v Speaker 3>fly or a pee in the middle of the cathedral. So,

0:23:26.640 --> 0:23:29.920
<v Speaker 3>first of all, the scales inside the atom are very

0:23:29.920 --> 0:23:32.800
<v Speaker 3>different to the pictures that we look at when we're

0:23:32.840 --> 0:23:35.880
<v Speaker 3>taught this kind of science, because you just can't fit

0:23:35.920 --> 0:23:38.200
<v Speaker 3>those scales on a page and have them be sensible, right,

0:23:38.240 --> 0:23:41.000
<v Speaker 3>so we condense everything down. So, first of all, for

0:23:41.080 --> 0:23:44.040
<v Speaker 3>most of us, the scales of what things look like

0:23:44.080 --> 0:23:46.800
<v Speaker 3>inside the atom are kind of wrong. And this was

0:23:46.840 --> 0:23:50.040
<v Speaker 3>also something that really blew the minds of even people

0:23:50.080 --> 0:23:54.879
<v Speaker 3>like artists like Vasily Kandinski was really affected by this

0:23:55.000 --> 0:23:58.320
<v Speaker 3>idea that the atom is mostly empty space. It really

0:23:59.520 --> 0:24:02.800
<v Speaker 3>shifted his perception on what nature was made of, because

0:24:02.880 --> 0:24:06.920
<v Speaker 3>suddenly everything around us that seemed solid is made of

0:24:06.960 --> 0:24:10.200
<v Speaker 3>almost nothing. And it's purely the forces between these sort

0:24:10.240 --> 0:24:14.639
<v Speaker 3>of ephemeral objects which are creating our experience of everything

0:24:14.680 --> 0:24:17.639
<v Speaker 3>around us. Which back in twenty eighteen, I give a

0:24:17.720 --> 0:24:19.720
<v Speaker 3>teTeX of new Talk, and people have reflected back to

0:24:19.760 --> 0:24:21.680
<v Speaker 3>me that the moment when they got shivers was when

0:24:21.680 --> 0:24:25.359
<v Speaker 3>I said that you're not even touching the chair beneath you.

0:24:25.359 --> 0:24:28.399
<v Speaker 3>You're hovering ever so slightly above it, and it's just

0:24:28.440 --> 0:24:30.480
<v Speaker 3>the forces between the electrons in the chair and the

0:24:30.520 --> 0:24:33.800
<v Speaker 3>electrons in your body opposing each other that makes you

0:24:33.840 --> 0:24:36.080
<v Speaker 3>feel like you're in contact with the chair, but you're

0:24:36.119 --> 0:24:40.719
<v Speaker 3>never The particles are never actually physically in contact with

0:24:40.800 --> 0:24:44.440
<v Speaker 3>each other. It's just the electromagnetic force and gravity. First

0:24:44.480 --> 0:24:46.600
<v Speaker 3>of all, that is a different way to view it.

0:24:47.240 --> 0:24:49.880
<v Speaker 3>The scale is a different way to view it. And

0:24:49.920 --> 0:24:53.919
<v Speaker 3>then not just the not just the electrons a wave like,

0:24:54.000 --> 0:24:57.640
<v Speaker 3>but also those fundamental particles at the center, the protons

0:24:57.680 --> 0:25:02.199
<v Speaker 3>and neutrons have constituent quarks. And even then, you know,

0:25:02.280 --> 0:25:05.000
<v Speaker 3>we say that there's two types of quarks up and

0:25:05.040 --> 0:25:07.960
<v Speaker 3>down quarks inside the protons and neutrons, but there's really

0:25:08.000 --> 0:25:10.600
<v Speaker 3>a whole lot more so, it's kind of like the

0:25:10.760 --> 0:25:13.359
<v Speaker 3>Nora's box. It's like if you go down further, you

0:25:13.520 --> 0:25:15.119
<v Speaker 3>open it up and you're like, oh, there's all this

0:25:15.160 --> 0:25:17.760
<v Speaker 3>other messa in there as well. And it depends how

0:25:17.760 --> 0:25:20.040
<v Speaker 3>had I look at, what energy scale I look at,

0:25:20.640 --> 0:25:23.120
<v Speaker 3>And it's just you know, so I like to imagine

0:25:23.119 --> 0:25:28.560
<v Speaker 3>the nucleus as sort of as a you know, a

0:25:28.600 --> 0:25:31.320
<v Speaker 3>group of protons and neutrons. But then if I try

0:25:31.359 --> 0:25:33.920
<v Speaker 3>and visualize opening up those protons and neutrons, that's where

0:25:34.040 --> 0:25:36.720
<v Speaker 3>even my brain goes, Nope, nope, I cannot do that.

0:25:37.000 --> 0:25:38.840
<v Speaker 3>That's too complex.

0:25:40.760 --> 0:25:42.960
<v Speaker 2>So you give a bunch of examples in the Book

0:25:43.119 --> 0:25:47.000
<v Speaker 2>of Discoveries in the History of Particle Physics that were

0:25:47.200 --> 0:25:51.359
<v Speaker 2>thought by some to be pure intellectual curiosities with no

0:25:51.520 --> 0:25:56.359
<v Speaker 2>practical use, only to later become very important in broader civilization.

0:25:56.560 --> 0:26:00.119
<v Speaker 2>Maybe they become the backbone of whole new genres of technology,

0:26:01.320 --> 0:26:03.919
<v Speaker 2>or unlock new discoveries, or of unlock new wings in

0:26:03.920 --> 0:26:06.119
<v Speaker 2>the mansion of physics. Do you want to tell the

0:26:06.160 --> 0:26:07.800
<v Speaker 2>story of one or two examples like this?

0:26:08.680 --> 0:26:11.040
<v Speaker 3>Sure, I think let's start right at the start, the

0:26:11.080 --> 0:26:14.439
<v Speaker 3>discovery of the first subatomic particle, the electron, and this

0:26:14.560 --> 0:26:17.439
<v Speaker 3>was done using the same experimental equipment basically as the

0:26:17.560 --> 0:26:21.399
<v Speaker 3>X ray discovery, so a cathoid ray tube. And JJ

0:26:21.480 --> 0:26:24.560
<v Speaker 3>Thompson in England in eighteen ninety seven sort of picked

0:26:24.600 --> 0:26:27.199
<v Speaker 3>up where others had left off and realized that he

0:26:27.200 --> 0:26:30.760
<v Speaker 3>could do a series of experiments bending around the beam

0:26:30.800 --> 0:26:35.159
<v Speaker 3>of so called cathode rays. So that's a glowing, glowing

0:26:35.240 --> 0:26:37.239
<v Speaker 3>green ray down the center of this tube that they

0:26:37.280 --> 0:26:39.199
<v Speaker 3>didn't and they didn't know how it worked at that

0:26:39.280 --> 0:26:41.640
<v Speaker 3>time or what it was made of. So he set

0:26:41.680 --> 0:26:45.440
<v Speaker 3>out to investigate the nature of these cathode rays by

0:26:45.720 --> 0:26:49.400
<v Speaker 3>deflecting them with electric fields and magnetic fields and catching

0:26:49.480 --> 0:26:52.440
<v Speaker 3>the charge and seeing how it moved around. And as

0:26:52.440 --> 0:26:55.040
<v Speaker 3>a result of all of those experiments, which I should

0:26:55.040 --> 0:26:58.440
<v Speaker 3>say he definitely needed help with, even though I say

0:26:58.480 --> 0:27:02.359
<v Speaker 3>it was him, had to have his expert glassblower Ebenezer

0:27:02.400 --> 0:27:06.160
<v Speaker 3>Ever create all the experimental apparatus for him because JJ Thompson,

0:27:06.200 --> 0:27:09.440
<v Speaker 3>despite being like the leading physicist in England at the time,

0:27:10.080 --> 0:27:13.159
<v Speaker 3>was I think I can't remember the exact phrase, but

0:27:13.200 --> 0:27:16.359
<v Speaker 3>it was like exceptionally helpless with his hands is the

0:27:16.359 --> 0:27:21.320
<v Speaker 3>phrase that comes to mind, so that that's a quote

0:27:21.320 --> 0:27:25.320
<v Speaker 3>of someone describing his experimental skills. So somebody else had

0:27:25.320 --> 0:27:27.760
<v Speaker 3>to create all of his apparatus, but anyway, he was

0:27:27.800 --> 0:27:33.919
<v Speaker 3>able to use Ebenezer's apparatus to bend the electrons to

0:27:33.960 --> 0:27:35.960
<v Speaker 3>bend the beam around, and from that he managed to

0:27:36.040 --> 0:27:41.560
<v Speaker 3>establish that not only is the beam made of particles,

0:27:41.600 --> 0:27:45.119
<v Speaker 3>but that those particles were lighter than any atom that

0:27:45.160 --> 0:27:48.040
<v Speaker 3>had ever been observed before, and so he was able

0:27:48.080 --> 0:27:50.280
<v Speaker 3>to establish that this must be some kind of new

0:27:50.320 --> 0:27:54.200
<v Speaker 3>fundamental particle, which we now call the electron, which is

0:27:54.200 --> 0:27:57.240
<v Speaker 3>about two thousand times lighter than the heaviest atom that

0:27:57.240 --> 0:27:59.680
<v Speaker 3>had been seen before. And he was able to tell

0:27:59.720 --> 0:28:04.919
<v Speaker 3>that that was really a fundamental component of matter because

0:28:04.920 --> 0:28:07.760
<v Speaker 3>it didn't matter which cathoid he used. So the cathod

0:28:07.840 --> 0:28:10.119
<v Speaker 3>is the part that the rays jump out of, and

0:28:10.680 --> 0:28:13.480
<v Speaker 3>if it was just an atom, then you would expect

0:28:13.480 --> 0:28:16.000
<v Speaker 3>if you change the cathoid, or have you changed the

0:28:16.040 --> 0:28:19.080
<v Speaker 3>gas inside the tube, that the results would vary, and

0:28:19.119 --> 0:28:22.560
<v Speaker 3>they didn't. So that told him that this electron was

0:28:22.600 --> 0:28:25.320
<v Speaker 3>somehow inside every single type of atom that he was

0:28:25.560 --> 0:28:30.000
<v Speaker 3>working with, so that that was an amazing discovery. And

0:28:30.160 --> 0:28:33.159
<v Speaker 3>they used to be a toast in the Cavendish Lab

0:28:33.240 --> 0:28:35.960
<v Speaker 3>in Cambridge where he made this discovery, and they have

0:28:36.040 --> 0:28:39.720
<v Speaker 3>this annual party where you know, they sort of, I

0:28:39.720 --> 0:28:42.000
<v Speaker 3>don't know, they make up songs and they make up

0:28:42.080 --> 0:28:44.600
<v Speaker 3>poems and they have a fancy dinner, and you know,

0:28:44.760 --> 0:28:48.200
<v Speaker 3>having spent over a decade myself in the UK at Oxford,

0:28:48.200 --> 0:28:50.440
<v Speaker 3>I'm kind of imagining this in a wood paneled room,

0:28:50.560 --> 0:28:54.120
<v Speaker 3>you know, with candlesticks and fancy, fancy food and everyone's

0:28:54.160 --> 0:28:57.360
<v Speaker 3>wearing black tie. And there used to be a toast

0:28:57.360 --> 0:28:59.720
<v Speaker 3>at this annual event where they would toast to the

0:28:59.720 --> 0:29:02.160
<v Speaker 3>electron and they would say, to the electron, may it

0:29:02.200 --> 0:29:07.520
<v Speaker 3>never be of use to anyone, because when he discovered

0:29:07.520 --> 0:29:09.640
<v Speaker 3>it, it really was just him trying to figure out the

0:29:09.640 --> 0:29:14.080
<v Speaker 3>fundamental nature of how these rays happened in this tube

0:29:14.120 --> 0:29:16.880
<v Speaker 3>that numerous scientists had in their labs around the world.

0:29:17.760 --> 0:29:20.240
<v Speaker 3>And in the few years after he discovered the electron,

0:29:20.280 --> 0:29:24.240
<v Speaker 3>he also discovered the process called thermionic emission, which is

0:29:24.480 --> 0:29:26.960
<v Speaker 3>the process by which the electrons actually jump out of

0:29:27.040 --> 0:29:31.320
<v Speaker 3>materials when you heat them up. And this then became

0:29:31.360 --> 0:29:35.520
<v Speaker 3>an incredibly important piece of knowledge which he obviously published

0:29:35.520 --> 0:29:39.040
<v Speaker 3>and you know, wrote all many things about because a

0:29:39.080 --> 0:29:43.920
<v Speaker 3>few years a few years later, an electrical engineer would

0:29:44.200 --> 0:29:47.600
<v Speaker 3>sort of pick up this information and a previous discovery

0:29:47.640 --> 0:29:51.120
<v Speaker 3>that had been made by Thomas Edison when he was

0:29:51.280 --> 0:29:55.200
<v Speaker 3>trying to manufacture reliable light bulbs, and they'd put those

0:29:55.320 --> 0:30:00.000
<v Speaker 3>two ideas together and come up with the first electric vat.

0:30:00.400 --> 0:30:03.200
<v Speaker 3>So that is a device which can control the flow

0:30:03.240 --> 0:30:07.480
<v Speaker 3>of electricity. You apply a small voltage and it either

0:30:07.560 --> 0:30:10.479
<v Speaker 3>lets the current pass or it stops the current. And

0:30:10.520 --> 0:30:15.239
<v Speaker 3>then more and more electronic devices then were invented after this,

0:30:15.720 --> 0:30:17.680
<v Speaker 3>and in order to make those devices, they were one

0:30:17.760 --> 0:30:22.960
<v Speaker 3>hundred percent reliant on JJ. Thompson's materials, on his theories,

0:30:23.200 --> 0:30:24.920
<v Speaker 3>and on the things that he had developed as a

0:30:24.920 --> 0:30:28.680
<v Speaker 3>result of his experiments. And those early tubes were very

0:30:28.680 --> 0:30:32.600
<v Speaker 3>similar in their makeup to the tubes that Thompson was

0:30:32.640 --> 0:30:37.000
<v Speaker 3>working with. Anyway, it's all very similar technology. But one

0:30:37.000 --> 0:30:40.200
<v Speaker 3>thing I find quite interesting is that Thomas Edison just

0:30:40.320 --> 0:30:42.200
<v Speaker 3>you know, he sort of made this discovery, which was

0:30:42.240 --> 0:30:45.800
<v Speaker 3>called the Edison effect, which was kind of about the

0:30:45.800 --> 0:30:48.520
<v Speaker 3>flow of electricity, but he hadn't fully understood it. He

0:30:48.680 --> 0:30:51.200
<v Speaker 3>just if he put an extra electrode inside a light bulb.

0:30:51.200 --> 0:30:53.920
<v Speaker 3>He noticed that it affected the flow of electricity, and

0:30:54.000 --> 0:30:55.720
<v Speaker 3>he patented it, but he couldn't think of any good

0:30:55.760 --> 0:30:58.400
<v Speaker 3>ideas for it, so he just set it aside and

0:30:58.720 --> 0:31:01.840
<v Speaker 3>ignored it. And if that had been the history, then nothing,

0:31:02.080 --> 0:31:05.360
<v Speaker 3>you know, nothing would have been done about it at all.

0:31:05.400 --> 0:31:08.400
<v Speaker 3>And I'm always amazed that people sort of look at

0:31:08.520 --> 0:31:11.960
<v Speaker 3>Edison and his trial and error approach and they hold

0:31:11.960 --> 0:31:15.600
<v Speaker 3>it up as this example of amazing innovation, and I'm like, well, okay,

0:31:15.600 --> 0:31:18.600
<v Speaker 3>but he ignored possibly the most important thing he ever discovered.

0:31:21.000 --> 0:31:23.040
<v Speaker 3>And it was only because other people picked up the

0:31:23.080 --> 0:31:27.200
<v Speaker 3>ideas and understood it through JJ Thompson's investigations and his theories,

0:31:27.960 --> 0:31:30.680
<v Speaker 3>that then it led to the first electronic devices, the

0:31:30.720 --> 0:31:35.600
<v Speaker 3>first and our ability through vacuum tubes to create things

0:31:35.680 --> 0:31:40.640
<v Speaker 3>like the telecommunications industry to you know, and long distance communications,

0:31:40.840 --> 0:31:44.000
<v Speaker 3>the first computers, all of the early electronics were based

0:31:44.040 --> 0:31:47.240
<v Speaker 3>on these vacuum tubes. And of course that's changed a

0:31:47.280 --> 0:31:50.240
<v Speaker 3>bit now everything's based in silicon and in the future,

0:31:50.280 --> 0:31:53.880
<v Speaker 3>who knows what it will be based on. But if

0:31:53.920 --> 0:31:57.120
<v Speaker 3>that fundamental investigation hadn't happened at the right time and

0:31:57.160 --> 0:32:00.560
<v Speaker 3>that knowledge wasn't there for the electrical engineers to build off.

0:32:01.640 --> 0:32:04.280
<v Speaker 3>I sort of question, perhaps we'd have got there eventually

0:32:04.320 --> 0:32:07.760
<v Speaker 3>with the electronics industry, but the story would have looked very,

0:32:07.840 --> 0:32:12.600
<v Speaker 3>very different. So that's I find that an interesting example

0:32:12.600 --> 0:32:15.680
<v Speaker 3>of the ways in which the sort of curiosity driven research,

0:32:15.880 --> 0:32:18.200
<v Speaker 3>you know, trying to uncover the nature of the universe,

0:32:18.760 --> 0:32:24.200
<v Speaker 3>and our innovation stories and our entrepreneurial stories kind of

0:32:24.720 --> 0:32:27.280
<v Speaker 3>merge all into one, and you start to see it

0:32:27.360 --> 0:32:30.040
<v Speaker 3>not as one is superior to the other, but that

0:32:30.120 --> 0:32:33.760
<v Speaker 3>they are essential to each other, and that we need

0:32:33.800 --> 0:32:38.000
<v Speaker 3>both approaches and we can't just always sort of seed

0:32:38.040 --> 0:32:42.560
<v Speaker 3>fund some entrepreneurial project or support some you know, innovator

0:32:42.600 --> 0:32:45.560
<v Speaker 3>who's full of energy. You actually do need the people

0:32:45.560 --> 0:32:48.560
<v Speaker 3>in the background doing that curiosity driven research in order

0:32:48.600 --> 0:32:50.520
<v Speaker 3>to have new knowledge for those people to build on.

0:32:51.040 --> 0:32:55.480
<v Speaker 2>Well, speaking of the people in the background, another interesting

0:32:55.520 --> 0:32:57.440
<v Speaker 2>thing to me about a lot of the stories you

0:32:57.480 --> 0:33:00.800
<v Speaker 2>tell are that some physics expect eerments that are very

0:33:00.840 --> 0:33:04.800
<v Speaker 2>important in history are surprisingly laborious. Like I think of

0:33:04.880 --> 0:33:09.320
<v Speaker 2>the example of particle counting, These experiments that involve just

0:33:09.360 --> 0:33:12.200
<v Speaker 2>staring at a screen for hours and counting flashes of

0:33:12.280 --> 0:33:15.680
<v Speaker 2>light by hand. Yeah, what are some of the ways

0:33:15.760 --> 0:33:19.880
<v Speaker 2>that crucial physics discoveries depended on types of work that

0:33:20.000 --> 0:33:23.080
<v Speaker 2>people might not think of when they try to imagine

0:33:23.160 --> 0:33:24.560
<v Speaker 2>what scientists are doing.

0:33:26.440 --> 0:33:29.320
<v Speaker 3>Yeah, I think there's a we love them, we love

0:33:29.400 --> 0:33:33.120
<v Speaker 3>the moment of discovery, right, but we're often unwilling to

0:33:33.240 --> 0:33:36.080
<v Speaker 3>figure out exactly what went into that discovery. And I

0:33:36.120 --> 0:33:39.320
<v Speaker 3>have to say it's often it often comes as a

0:33:39.320 --> 0:33:42.000
<v Speaker 3>surprise to people as you say how laborious it was.

0:33:42.080 --> 0:33:44.400
<v Speaker 3>So so that example you're talking about is in those

0:33:44.440 --> 0:33:47.880
<v Speaker 3>early days of nuclear physics where the only detectors we

0:33:47.960 --> 0:33:51.000
<v Speaker 3>had were these fluorescent screens that lit up when high

0:33:51.120 --> 0:33:55.720
<v Speaker 3>energy particles hit them. And so in Cambridge in the

0:33:55.800 --> 0:33:59.240
<v Speaker 3>UK especially, they trained all their students and all their

0:33:59.320 --> 0:34:02.880
<v Speaker 3>staff of how to sit in a dark room and

0:34:03.120 --> 0:34:05.959
<v Speaker 3>look through a microscope at these plates when they were

0:34:06.040 --> 0:34:11.279
<v Speaker 3>radioactive sources present and count each flash of light. But

0:34:11.360 --> 0:34:14.480
<v Speaker 3>of course every human eye and brain is different, and

0:34:14.520 --> 0:34:17.600
<v Speaker 3>so everyone was everyone was trained up and kind of

0:34:17.760 --> 0:34:22.839
<v Speaker 3>measured to see how good they were at this particle counting. Right.

0:34:22.880 --> 0:34:26.080
<v Speaker 3>So there's all these I mean, to get reliable scientific results,

0:34:26.160 --> 0:34:29.560
<v Speaker 3>you need things like calibration, you know, these boring things

0:34:29.600 --> 0:34:31.880
<v Speaker 3>you know, the things that are not sexy or exciting

0:34:31.920 --> 0:34:35.480
<v Speaker 3>about science. Good calibration. You need to know your instruments

0:34:35.600 --> 0:34:39.200
<v Speaker 3>very very very well, and I think any physicist today

0:34:39.200 --> 0:34:43.040
<v Speaker 3>would tell you that until you know your experiment inside out,

0:34:43.239 --> 0:34:45.440
<v Speaker 3>you will not get reliable results from it. And it's

0:34:45.440 --> 0:34:49.560
<v Speaker 3>something that frustrates the heck out of undergraduate students in

0:34:50.080 --> 0:34:52.160
<v Speaker 3>the lab when they're learning physics and they're trying to

0:34:52.160 --> 0:34:55.160
<v Speaker 3>recreate experiments that were done in the past, and even

0:34:55.200 --> 0:34:58.279
<v Speaker 3>though they've got apparatus that someone has prepared for them

0:34:58.320 --> 0:35:02.520
<v Speaker 3>that should be working, driven mad by the intricacies of it.

0:35:03.160 --> 0:35:08.279
<v Speaker 3>And this is the reality, I mean, unfortunately, but you know,

0:35:08.360 --> 0:35:10.719
<v Speaker 3>it's the reality of experimental life, which is that this

0:35:10.760 --> 0:35:12.600
<v Speaker 3>stuff is not easy. And if it was easy, we

0:35:12.640 --> 0:35:16.440
<v Speaker 3>would have done it hundreds of years ago, right, But

0:35:16.560 --> 0:35:20.239
<v Speaker 3>it's difficult. It's often laborious, and often what we're trying

0:35:20.239 --> 0:35:22.600
<v Speaker 3>to do in inventing new technologies and pushing at the

0:35:22.600 --> 0:35:26.880
<v Speaker 3>cutting edge of technologies in experimental science is sometimes to

0:35:26.920 --> 0:35:30.120
<v Speaker 3>get around the laboriousness, or even just to create a

0:35:30.160 --> 0:35:33.840
<v Speaker 3>method to collect enough data that we can actually that

0:35:33.880 --> 0:35:36.560
<v Speaker 3>we can actually use. So obviously, nowadays we don't use

0:35:36.600 --> 0:35:40.279
<v Speaker 3>people sitting in a room particle counting. But there was

0:35:40.320 --> 0:35:44.839
<v Speaker 3>a whole phase of experimental physics where after the technologies

0:35:44.840 --> 0:35:48.759
<v Speaker 3>were invented that allows you to photograph the tracks of particles. Well,

0:35:48.800 --> 0:35:53.239
<v Speaker 3>then who processes the photographic data, right, who maps out

0:35:53.280 --> 0:35:59.120
<v Speaker 3>those tracks and who turns all of that into tables

0:35:59.160 --> 0:36:03.359
<v Speaker 3>that can be analyzed and searched for new physics. And

0:36:03.400 --> 0:36:06.880
<v Speaker 3>the answer that most people probably don't realize is women

0:36:06.960 --> 0:36:10.799
<v Speaker 3>did it. And in the early days these women were

0:36:10.800 --> 0:36:14.000
<v Speaker 3>called there was the computers, So the women who did

0:36:14.480 --> 0:36:18.000
<v Speaker 3>calculations by hand before the computer meant something very different

0:36:18.040 --> 0:36:21.200
<v Speaker 3>to us. And in particle physics even into the forties,

0:36:21.200 --> 0:36:24.680
<v Speaker 3>fifties and sixties, you had the so called scanning girls,

0:36:25.600 --> 0:36:28.480
<v Speaker 3>and these were women who almost all women. There were

0:36:28.520 --> 0:36:30.920
<v Speaker 3>some men who did it should I should say, who

0:36:30.920 --> 0:36:34.840
<v Speaker 3>would sit at these enormous light tables with the copies

0:36:34.880 --> 0:36:38.279
<v Speaker 3>of the photographic images and they would follow a very

0:36:38.320 --> 0:36:43.000
<v Speaker 3>precise sort of protocol in mapping out where the interesting

0:36:43.080 --> 0:36:47.120
<v Speaker 3>things were in those photographs. And there were many, many

0:36:47.160 --> 0:36:50.640
<v Speaker 3>discoveries made this way, something I do find interesting in

0:36:50.840 --> 0:36:53.800
<v Speaker 3>the history. And I'm sure we'll get to the discussion

0:36:53.840 --> 0:36:57.400
<v Speaker 3>of women in physics in a moment. But while some

0:36:57.440 --> 0:37:00.239
<v Speaker 3>of these women were so called scanning girls, it was

0:37:00.280 --> 0:37:04.400
<v Speaker 3>also considered to be a task that all the physicists

0:37:04.440 --> 0:37:07.920
<v Speaker 3>should also know how to do. And this continues to

0:37:07.920 --> 0:37:10.880
<v Speaker 3>this day. Even when you get these big collaborations like

0:37:10.880 --> 0:37:14.680
<v Speaker 3>the large Hadron collider, there's a sort of commitment to

0:37:14.840 --> 0:37:17.480
<v Speaker 3>the experiment that you do some of this grunt work,

0:37:17.520 --> 0:37:19.520
<v Speaker 3>you do some of this laborious work, and today that

0:37:19.600 --> 0:37:23.600
<v Speaker 3>means sitting in a control room and overseeing the running

0:37:23.640 --> 0:37:27.200
<v Speaker 3>of enormous colliders and detectors. But back then it would

0:37:27.200 --> 0:37:30.960
<v Speaker 3>mean that you would do your share of analyzing these images.

0:37:32.120 --> 0:37:36.680
<v Speaker 3>So this, in a way is inseparable work. It's specialized work,

0:37:37.760 --> 0:37:41.319
<v Speaker 3>but it's work where the physicists did as well. And

0:37:41.360 --> 0:37:44.880
<v Speaker 3>there were female physicists at that time who were also

0:37:45.239 --> 0:37:50.520
<v Speaker 3>doing these kinds of analyses. And I almost wonder in

0:37:50.560 --> 0:37:52.840
<v Speaker 3>this time, and this is a it's just an idea

0:37:52.880 --> 0:37:55.880
<v Speaker 3>that has come to me a number of times, I

0:37:55.960 --> 0:37:58.680
<v Speaker 3>almost wonder if the women who were working as physicists

0:37:58.680 --> 0:38:03.000
<v Speaker 3>in those laboratories were somewhat overlooked because the women's work

0:38:03.160 --> 0:38:08.279
<v Speaker 3>at the time was as the scanning girls mostly, you know,

0:38:08.360 --> 0:38:11.839
<v Speaker 3>and so there was this gender divide in roles, and

0:38:12.280 --> 0:38:15.719
<v Speaker 3>even though the women were contributing, and some of them

0:38:15.880 --> 0:38:18.520
<v Speaker 3>were physicists, not you know, they weren't just hired as

0:38:18.520 --> 0:38:23.200
<v Speaker 3>scanning girls, and yet their contributions were overlooked far more

0:38:23.239 --> 0:38:26.319
<v Speaker 3>often than the contributions of their male colleagues. And I

0:38:26.360 --> 0:38:29.480
<v Speaker 3>do wonder how this gender divide in the roles of

0:38:29.520 --> 0:38:34.120
<v Speaker 3>this grunt work actually played into that overlooking at the time.

0:38:35.000 --> 0:38:37.080
<v Speaker 3>But that's just one It's just one aspect of the

0:38:37.239 --> 0:38:40.359
<v Speaker 3>sort of gendered nature of physics as we as we

0:38:40.440 --> 0:38:43.600
<v Speaker 3>now know it, I think. But yeah, the I think

0:38:43.600 --> 0:38:45.319
<v Speaker 3>a lot of people would be really surprised by how

0:38:45.440 --> 0:38:48.160
<v Speaker 3>laborious a lot of the work is. And of course

0:38:48.800 --> 0:38:53.800
<v Speaker 3>that's where automation nowadays and even AI tools just changing

0:38:53.800 --> 0:38:57.440
<v Speaker 3>the game so dramatically, because now that you can automate

0:38:57.680 --> 0:39:00.399
<v Speaker 3>all of these processes and all of our detail as

0:39:00.400 --> 0:39:04.279
<v Speaker 3>a you know, full of electronics instead of photographs, you know,

0:39:04.400 --> 0:39:07.680
<v Speaker 3>the process of actually gathering the data is now much

0:39:07.800 --> 0:39:12.000
<v Speaker 3>much easier, and so people and people can access the

0:39:12.040 --> 0:39:14.719
<v Speaker 3>data around the world, including via the World Wide Web,

0:39:14.719 --> 0:39:19.160
<v Speaker 3>which was invented at soon just for that purpose. And

0:39:19.239 --> 0:39:21.719
<v Speaker 3>so now we can focus on the analysis and we

0:39:21.760 --> 0:39:25.520
<v Speaker 3>can focus on the physics and the contributions to the

0:39:25.560 --> 0:39:29.200
<v Speaker 3>hardware and software become the grunt work and that part

0:39:29.239 --> 0:39:32.520
<v Speaker 3>of the project as the experimentalist. So yeah, it's an

0:39:32.560 --> 0:39:34.279
<v Speaker 3>interesting shift through time.

0:39:44.480 --> 0:39:46.880
<v Speaker 2>Coming back to the issue of women in the history

0:39:46.920 --> 0:39:49.239
<v Speaker 2>of physics. You mentioned in the book this idea of

0:39:49.400 --> 0:39:53.000
<v Speaker 2>the Matilda fact in physics, and it strikes me that

0:39:53.080 --> 0:39:58.120
<v Speaker 2>there are at least two different ways that the historical

0:39:58.160 --> 0:40:04.080
<v Speaker 2>discrimination against women in physics manifests. There's one where there's

0:40:04.239 --> 0:40:09.000
<v Speaker 2>just direct limitations on their participation, like some researchers having

0:40:09.040 --> 0:40:11.840
<v Speaker 2>projects they considered not suitable for women to work on,

0:40:12.480 --> 0:40:15.120
<v Speaker 2>or the marriage bar where women who had previously been

0:40:15.120 --> 0:40:18.120
<v Speaker 2>involved in research were disallowed from doing so after marriage.

0:40:18.880 --> 0:40:22.719
<v Speaker 2>But there are also cases where women researchers made significant

0:40:22.719 --> 0:40:27.200
<v Speaker 2>contributions to physics discoveries and their role in this work

0:40:27.280 --> 0:40:31.120
<v Speaker 2>was sometimes deliberately censored from public records and recognition. Could

0:40:31.160 --> 0:40:33.120
<v Speaker 2>you talk about a couple of these examples.

0:40:33.520 --> 0:40:37.200
<v Speaker 3>Yeah, sure, I think that's really insightful that there are

0:40:37.239 --> 0:40:41.440
<v Speaker 3>these different ways in which women's involvement in physics was

0:40:42.040 --> 0:40:45.280
<v Speaker 3>a stopped, as you say, you know, sort of prevented,

0:40:45.680 --> 0:40:48.480
<v Speaker 3>but then also that their contributions were diminished, and that

0:40:48.560 --> 0:40:51.399
<v Speaker 3>second one is really where the Matilda effect comes in.

0:40:52.200 --> 0:40:55.360
<v Speaker 3>So one person I'm thinking of here, her name is

0:40:55.400 --> 0:40:59.400
<v Speaker 3>Marietta Blau, and she was a researcher in Austria and

0:40:59.440 --> 0:41:03.120
<v Speaker 3>she invented a new type of particle detector. So I

0:41:03.239 --> 0:41:05.759
<v Speaker 3>talked before about how beautiful I thought the cloud chamber was.

0:41:06.000 --> 0:41:08.239
<v Speaker 3>That's a very active detector. Things have to happen in

0:41:08.239 --> 0:41:10.440
<v Speaker 3>real time. You have to photograph things in real time.

0:41:11.239 --> 0:41:15.640
<v Speaker 3>It's very laborious to look after. And what she invented instead,

0:41:15.640 --> 0:41:18.160
<v Speaker 3>because she had a background both in physics and photography,

0:41:18.800 --> 0:41:23.080
<v Speaker 3>was a photographic plate method of detecting particles. So she

0:41:23.120 --> 0:41:27.320
<v Speaker 3>had this very thick so called emulsions, and they would

0:41:27.600 --> 0:41:31.640
<v Speaker 3>create stacks of these emulsions for high energy charge particles

0:41:31.640 --> 0:41:34.520
<v Speaker 3>to go through. And this now, instead of being looked

0:41:34.560 --> 0:41:37.279
<v Speaker 3>after and photographed it every minute, could just be left

0:41:37.280 --> 0:41:39.439
<v Speaker 3>at the top of a mountain for a month, two

0:41:39.480 --> 0:41:42.960
<v Speaker 3>months and it would just collect data over time and

0:41:43.000 --> 0:41:46.800
<v Speaker 3>then it would be pulled apart and analyzed. And Blau's

0:41:46.840 --> 0:41:49.920
<v Speaker 3>invention led to a whole load of discoveries and she

0:41:49.960 --> 0:41:53.920
<v Speaker 3>herself was actually nominated for the Nobel Prize, but never

0:41:54.200 --> 0:42:00.920
<v Speaker 3>never won it, and her invention led to think at

0:42:01.000 --> 0:42:03.680
<v Speaker 3>least I can think of at least two other Nobel

0:42:03.719 --> 0:42:08.080
<v Speaker 3>prizes that relied on her invention of this photographic emulsion method.

0:42:08.360 --> 0:42:13.000
<v Speaker 3>But she also actually made amazing discoveries with it herself,

0:42:13.719 --> 0:42:16.480
<v Speaker 3>one of which was she called it a star of disintegration,

0:42:16.520 --> 0:42:19.359
<v Speaker 3>which was when a high energy cosmic ray coming from

0:42:19.400 --> 0:42:23.160
<v Speaker 3>space came in and was sort of a direct hit

0:42:23.200 --> 0:42:25.640
<v Speaker 3>on a heavy nucleus, and then that nucleus itself sort

0:42:25.640 --> 0:42:30.000
<v Speaker 3>of exploded and it left this amazing shower like a

0:42:30.160 --> 0:42:34.920
<v Speaker 3>super nova on the photographic emulsions. And this was a

0:42:35.080 --> 0:42:36.920
<v Speaker 3>you know, she published. I'm pretty sure that one was

0:42:36.960 --> 0:42:41.840
<v Speaker 3>published in Nature and her sort of contemporary or not.

0:42:41.920 --> 0:42:44.680
<v Speaker 3>Long after she was working, there was an Indian physicist

0:42:44.760 --> 0:42:47.600
<v Speaker 3>named Biber Chowdery working in India, and she was one

0:42:47.600 --> 0:42:51.520
<v Speaker 3>who was told that her professor didn't have any suitable

0:42:51.520 --> 0:42:53.960
<v Speaker 3>projects for her as a woman, but she persisted anyway,

0:42:54.640 --> 0:42:56.799
<v Speaker 3>and eventually sort of I guess won him over because

0:42:56.840 --> 0:42:59.960
<v Speaker 3>she ended up working with him, and she used similar

0:43:00.040 --> 0:43:04.960
<v Speaker 3>photographic plates, but not of such great quality because she

0:43:05.080 --> 0:43:07.200
<v Speaker 3>didn't have them available to her. It was during World

0:43:07.239 --> 0:43:09.800
<v Speaker 3>War two and she was in India so the supply

0:43:09.920 --> 0:43:15.000
<v Speaker 3>chain wasn't great, but she actually uses photographic plates up

0:43:15.040 --> 0:43:19.160
<v Speaker 3>mountains in India and then she managed to discover the

0:43:19.200 --> 0:43:21.759
<v Speaker 3>two different types of particles, which we would now call

0:43:21.800 --> 0:43:27.200
<v Speaker 3>the muon and the pion, and those were those were

0:43:27.239 --> 0:43:30.200
<v Speaker 3>some of the first observations of those particles, and as

0:43:30.200 --> 0:43:32.520
<v Speaker 3>far as I can tell, it was the first time

0:43:32.600 --> 0:43:35.799
<v Speaker 3>when it had been really recognized that there were two

0:43:35.880 --> 0:43:39.799
<v Speaker 3>different particles. But I think she couldn't quite because of

0:43:39.800 --> 0:43:42.560
<v Speaker 3>the quality of her equipment. She couldn't quite sort of

0:43:42.560 --> 0:43:45.080
<v Speaker 3>say what was what or you know, the difference in

0:43:45.120 --> 0:43:47.760
<v Speaker 3>masses between the two or something like that was missing.

0:43:48.160 --> 0:43:51.239
<v Speaker 3>But this is the first authored paper in Nature, and

0:43:51.280 --> 0:43:53.400
<v Speaker 3>this time I know it was definitely in Nature, you know,

0:43:53.480 --> 0:43:57.359
<v Speaker 3>the top top journal in the world. And then in

0:43:57.400 --> 0:44:00.600
<v Speaker 3>the nineteen fifties, so not long after Cecil Power working

0:44:00.600 --> 0:44:04.560
<v Speaker 3>in England. Are sorry his Nobel prize was nineteen fifty.

0:44:04.600 --> 0:44:07.960
<v Speaker 3>I think his work would have been late forties. He

0:44:08.040 --> 0:44:12.720
<v Speaker 3>used exactly the same technique with superior emulsions to discover

0:44:12.840 --> 0:44:17.680
<v Speaker 3>the pion and in his earlier writing in his it's

0:44:17.719 --> 0:44:20.600
<v Speaker 3>definitely at least one textbook that he writes about, he

0:44:20.640 --> 0:44:24.200
<v Speaker 3>acknowledges Biber Chowdery's earlier work and references her Nature paper.

0:44:24.800 --> 0:44:27.920
<v Speaker 3>And then when he wins the Nobel Prize in nineteen fifty,

0:44:28.080 --> 0:44:31.440
<v Speaker 3>every reference of his that referenced her work are not

0:44:31.640 --> 0:44:34.600
<v Speaker 3>used in the citation for the Nobel Prize. So all

0:44:34.640 --> 0:44:37.920
<v Speaker 3>the papers that are cited of his for the Nobel

0:44:37.960 --> 0:44:41.160
<v Speaker 3>Prize were the ones that didn't recognize the earlier work

0:44:41.200 --> 0:44:45.799
<v Speaker 3>of this woman working in India. And I had never

0:44:45.840 --> 0:44:47.880
<v Speaker 3>heard of her before I wrote this book. I'd never

0:44:47.920 --> 0:44:51.320
<v Speaker 3>come across her story. But I thought that was phenomenal

0:44:51.320 --> 0:44:53.560
<v Speaker 3>because Powell himself was not you know, he wasn't a

0:44:53.560 --> 0:44:56.960
<v Speaker 3>rephensible human. He was a very left leaning liberal person.

0:44:57.040 --> 0:44:59.600
<v Speaker 3>He had an unusually high number of female physicists in

0:44:59.600 --> 0:45:03.239
<v Speaker 3>his labe in Bristol in the UK, and I think

0:45:03.280 --> 0:45:08.080
<v Speaker 3>he himself was I haven't looked into his sort of

0:45:08.160 --> 0:45:10.560
<v Speaker 3>journals and things, whether they exist. I would love to

0:45:10.600 --> 0:45:13.040
<v Speaker 3>know how he felt about the fact that he had

0:45:13.080 --> 0:45:17.040
<v Speaker 3>recognized the President and the Nobel Prize committee had not.

0:45:18.480 --> 0:45:21.400
<v Speaker 3>And so bib Chowdery is someone that even my particle

0:45:21.400 --> 0:45:23.560
<v Speaker 3>physics colleagues have never heard of, even though she made

0:45:23.600 --> 0:45:29.120
<v Speaker 3>this amazing discovery. And so these kinds of behaviors of

0:45:29.320 --> 0:45:33.000
<v Speaker 3>sort of the ignoring of the women's contribution, like people

0:45:33.040 --> 0:45:36.680
<v Speaker 3>will use their contributions but won't acknowledge them properly, and

0:45:36.760 --> 0:45:40.759
<v Speaker 3>so we get this historical track record of you know,

0:45:40.760 --> 0:45:43.680
<v Speaker 3>the Nobel Prize winners who are almost always men other

0:45:43.719 --> 0:45:47.239
<v Speaker 3>than Marie Currey because she was so damn good no

0:45:47.239 --> 0:45:52.040
<v Speaker 3>one could deny it, and you get these contributions of

0:45:52.080 --> 0:45:54.879
<v Speaker 3>these women sort of falling by the wayside. And it's

0:45:54.880 --> 0:45:58.719
<v Speaker 3>called the Matilda effect after Matilda Gage, who was a

0:45:58.719 --> 0:46:03.120
<v Speaker 3>suffragist who first recognized that the contributions of women, and

0:46:03.160 --> 0:46:05.799
<v Speaker 3>back then she was talking about the contributions to technology,

0:46:06.520 --> 0:46:09.759
<v Speaker 3>but she first recognized that these contributions were being overlooked

0:46:10.160 --> 0:46:13.919
<v Speaker 3>or attributed to their male counterparts or peers or even

0:46:13.960 --> 0:46:18.680
<v Speaker 3>their husbands, and not properly attributed to the women who

0:46:18.719 --> 0:46:22.759
<v Speaker 3>made them because of the biases that existed in our society.

0:46:22.920 --> 0:46:27.239
<v Speaker 3>And a historian named Margaret Rossiter sort of coined this

0:46:27.360 --> 0:46:31.400
<v Speaker 3>term the Matilda effect, named after Matilda Gauge, and really

0:46:31.480 --> 0:46:35.680
<v Speaker 3>encouraged all of us to look for those stories when

0:46:35.719 --> 0:46:40.399
<v Speaker 3>we're looking at the history of especially technological fields and

0:46:40.560 --> 0:46:42.839
<v Speaker 3>highly technical fields like physics, where there is a lack

0:46:42.920 --> 0:46:46.759
<v Speaker 3>of women today. First of all, because and even I

0:46:46.840 --> 0:46:49.600
<v Speaker 3>wasn't aware of this that you know, you will probably

0:46:49.640 --> 0:46:51.400
<v Speaker 3>find women that you weren't aware of. And this was

0:46:51.440 --> 0:46:55.200
<v Speaker 3>absolutely my experience in writing this story. But secondly, she

0:46:55.239 --> 0:46:59.400
<v Speaker 3>then encouraged us to write their stories back in because

0:46:59.480 --> 0:47:02.560
<v Speaker 3>you know, there's no other way to correct the record,

0:47:03.160 --> 0:47:07.600
<v Speaker 3>and they have simply been overlooked. And so I mean,

0:47:08.080 --> 0:47:09.719
<v Speaker 3>what could I do other than you know, it was

0:47:09.719 --> 0:47:11.480
<v Speaker 3>sort of a call to arms as far as I

0:47:11.520 --> 0:47:14.760
<v Speaker 3>was concerned, because here was I, you know, a female

0:47:15.040 --> 0:47:18.560
<v Speaker 3>physicist today, having never heard of these women who made

0:47:18.560 --> 0:47:20.480
<v Speaker 3>these amazing discoveries. And I thought, well, if I've never

0:47:20.520 --> 0:47:22.080
<v Speaker 3>heard of them, and I'm writing a book about the

0:47:22.160 --> 0:47:25.520
<v Speaker 3>history of these experiments, then probably no one else has

0:47:25.520 --> 0:47:27.759
<v Speaker 3>ever heard of them. And that turned out to be true.

0:47:28.560 --> 0:47:31.000
<v Speaker 3>And so it was just such a wonderful privilege actually

0:47:31.080 --> 0:47:34.000
<v Speaker 3>to take up Margaret Rossiter's you know, sort of call

0:47:34.040 --> 0:47:36.919
<v Speaker 3>to arms and write their stories back into the main

0:47:37.320 --> 0:47:40.120
<v Speaker 3>stories of the history of these experiments because they're so

0:47:40.120 --> 0:47:44.680
<v Speaker 3>so important, and to me, as a female physicist working today,

0:47:45.480 --> 0:47:49.720
<v Speaker 3>it made me realize, you know, all of the people

0:47:49.760 --> 0:47:53.640
<v Speaker 3>who laid the foundations of my field whom I sort

0:47:53.680 --> 0:47:55.600
<v Speaker 3>of grew up in the field thinking that they were

0:47:55.600 --> 0:47:59.600
<v Speaker 3>pretty much all men other than Marie Currey, that that

0:47:59.760 --> 0:48:02.480
<v Speaker 3>was that was false, and it created for me this

0:48:02.600 --> 0:48:06.319
<v Speaker 3>sense of sort of belonging that I didn't expect to get.

0:48:06.360 --> 0:48:08.239
<v Speaker 3>Out of the process of writing this book, I sort

0:48:08.239 --> 0:48:11.160
<v Speaker 3>of thought, Wow, women like me have always been that.

0:48:11.280 --> 0:48:14.160
<v Speaker 3>Women who've been curious about the universe, women who've wanted

0:48:14.160 --> 0:48:17.000
<v Speaker 3>to be in the lab and using their technical skills

0:48:17.040 --> 0:48:20.320
<v Speaker 3>and making these contributions to society and to our knowledge

0:48:20.680 --> 0:48:23.239
<v Speaker 3>have always been there. This isn't a weird thing that

0:48:23.320 --> 0:48:26.719
<v Speaker 3>I'm doing. I'm not unusual to want to do this.

0:48:27.960 --> 0:48:31.239
<v Speaker 3>And yeah, I've since had that sentiment reflected back by

0:48:32.160 --> 0:48:34.239
<v Speaker 3>women young and old. Actually, you know, sort of young

0:48:34.280 --> 0:48:36.640
<v Speaker 3>women starting out thinking of whether physics is for them.

0:48:37.000 --> 0:48:40.319
<v Speaker 3>I've had some lovely feedback that they you know, sort

0:48:40.320 --> 0:48:43.160
<v Speaker 3>of read the book. They read about these women who fought,

0:48:43.280 --> 0:48:45.360
<v Speaker 3>you know, I mean it was so hard to achieve

0:48:45.360 --> 0:48:47.600
<v Speaker 3>that as well, because often these women were denied formal

0:48:47.719 --> 0:48:50.480
<v Speaker 3>education in physics, that weren't even allowed in the lecture theaters.

0:48:50.680 --> 0:48:52.520
<v Speaker 3>So to realize that they were there and the things

0:48:52.520 --> 0:48:56.120
<v Speaker 3>that they achieved, just you know, it was a very

0:48:56.239 --> 0:48:59.520
<v Speaker 3>very encouraging and positive thing for me, even though in

0:48:59.560 --> 0:49:02.920
<v Speaker 3>their own life it was obviously a very negative experience sometimes.

0:49:02.960 --> 0:49:06.359
<v Speaker 3>But to me today these stories writing them back in

0:49:06.960 --> 0:49:10.520
<v Speaker 3>brings I think, a new perspective on who gets to

0:49:10.560 --> 0:49:11.239
<v Speaker 3>do physics.

0:49:11.840 --> 0:49:15.960
<v Speaker 2>It's definitely a powerful thing learning these stories. So I

0:49:16.000 --> 0:49:17.359
<v Speaker 2>want to come to the part of the book where

0:49:17.400 --> 0:49:22.879
<v Speaker 2>you talk about particle accelerators. Clearly you have a love

0:49:22.960 --> 0:49:27.600
<v Speaker 2>for accelerators. That's your field. Imagine somebody who is generally

0:49:27.640 --> 0:49:32.400
<v Speaker 2>positive about science, but views particle accelerators, especially the big projects,

0:49:32.400 --> 0:49:36.799
<v Speaker 2>the big colliders, as maybe too big and complicated to

0:49:36.840 --> 0:49:41.120
<v Speaker 2>be charismatic, as like objects of the imagination, and maybe

0:49:41.200 --> 0:49:44.399
<v Speaker 2>views their findings as too abstract to digest. What would

0:49:44.440 --> 0:49:47.960
<v Speaker 2>you tell this person to give them particle accelerator fever, like,

0:49:48.120 --> 0:49:49.520
<v Speaker 2>how would you make them fall in love?

0:49:50.160 --> 0:49:52.719
<v Speaker 3>Oh? That's real, that's really interesting. So I think we

0:49:52.840 --> 0:49:56.239
<v Speaker 3>live in an interesting time in terms of particle accelerators

0:49:56.800 --> 0:49:59.680
<v Speaker 3>because you know, obviously they're very well developed now and

0:49:59.680 --> 0:50:03.400
<v Speaker 3>we have these enormous machines. So the large hydron collidor

0:50:03.440 --> 0:50:07.120
<v Speaker 3>in Switzerland is twenty seven kilometers in circumference one hundred

0:50:07.120 --> 0:50:11.120
<v Speaker 3>meters underground. Right, it's fricking enormous and it's very difficult

0:50:11.160 --> 0:50:13.560
<v Speaker 3>to wrap your head around. First of all, I would

0:50:13.560 --> 0:50:16.800
<v Speaker 3>say to anybody who doesn't find that kind of experiment

0:50:16.960 --> 0:50:20.560
<v Speaker 3>charismatic on paper, I implore you to go and visit.

0:50:21.239 --> 0:50:25.360
<v Speaker 3>It will blow your mind. Honestly. It is just such

0:50:25.440 --> 0:50:30.160
<v Speaker 3>an enormous feat of human ingenuity. And today, in order

0:50:30.200 --> 0:50:34.359
<v Speaker 3>to achieve these enormous experiments, we all have to work

0:50:34.400 --> 0:50:37.640
<v Speaker 3>together and collaborate, and CERN is an amazing example of that,

0:50:37.800 --> 0:50:41.160
<v Speaker 3>and the big national labs in the US have also

0:50:41.880 --> 0:50:44.960
<v Speaker 3>been great examples of that, where you're bringing together experts

0:50:45.000 --> 0:50:48.640
<v Speaker 3>from so many different areas because these projects are things

0:50:48.680 --> 0:50:51.960
<v Speaker 3>that we cannot achieve alone. Now, SERN is a wonderful

0:50:52.000 --> 0:50:55.000
<v Speaker 3>example because it was created post World War two somewhat

0:50:55.000 --> 0:50:58.600
<v Speaker 3>as a peace building project, so in its remit or

0:50:58.640 --> 0:51:01.680
<v Speaker 3>in its constitution is science for peace. So they are

0:51:01.719 --> 0:51:04.319
<v Speaker 3>not allowed to work on any defense related projects, are

0:51:04.360 --> 0:51:07.480
<v Speaker 3>not allowed to work on anything with weapon ability. Is

0:51:07.520 --> 0:51:10.319
<v Speaker 3>it's probably the word that I should use. They're not

0:51:10.360 --> 0:51:12.040
<v Speaker 3>even allowed to turn a profit, not even in the

0:51:12.080 --> 0:51:15.960
<v Speaker 3>gift shop, which took some people by surprise. And I've

0:51:15.960 --> 0:51:17.719
<v Speaker 3>had a few people comment on that but I noted

0:51:17.800 --> 0:51:19.640
<v Speaker 3>that in the book, But to me it was obvious

0:51:19.680 --> 0:51:23.040
<v Speaker 3>because it's CERN, and they exist, you know, to seek

0:51:23.040 --> 0:51:25.480
<v Speaker 3>new knowledge in physics, and they exist sort of for

0:51:25.719 --> 0:51:29.600
<v Speaker 3>the betterment of humanity in a sort of grand sense.

0:51:30.280 --> 0:51:33.760
<v Speaker 3>And so after nineteen fifty six, you've got people working

0:51:33.840 --> 0:51:38.560
<v Speaker 3>at cerne across borders from countries who were at war

0:51:38.719 --> 0:51:41.560
<v Speaker 3>just a few years earlier. And this continues today. You know,

0:51:41.600 --> 0:51:44.560
<v Speaker 3>there are both Russian and Ukrainian scientists working at CERN

0:51:44.800 --> 0:51:51.600
<v Speaker 3>alongside each other. And so CERN really is this amazing

0:51:52.680 --> 0:51:56.040
<v Speaker 3>human project where we've learned to collaborate with thousands of

0:51:56.080 --> 0:51:59.799
<v Speaker 3>people to achieve things that certainly one lab can't do,

0:51:59.800 --> 0:52:03.160
<v Speaker 3>a lot one nation can't do alone. These are truly

0:52:03.400 --> 0:52:07.560
<v Speaker 3>global projects, so much so that sort of successful collaboration

0:52:07.719 --> 0:52:10.080
<v Speaker 3>that even the UN has come to people at CERN,

0:52:10.880 --> 0:52:14.120
<v Speaker 3>have come to people at CERN and tried to work

0:52:14.120 --> 0:52:17.279
<v Speaker 3>together on Okay, how come STERN is so successful in

0:52:17.320 --> 0:52:19.839
<v Speaker 3>its collaboration, right? What can the rest of us learn

0:52:19.920 --> 0:52:24.200
<v Speaker 3>from the way that CERN collaborates that could benefit the

0:52:24.239 --> 0:52:27.359
<v Speaker 3>rest of the world. And so, even if the technology

0:52:27.680 --> 0:52:31.760
<v Speaker 3>doesn't float your boat, I think the human collaboration aspect

0:52:31.840 --> 0:52:36.279
<v Speaker 3>of it is something which most people find quite inspiring.

0:52:37.600 --> 0:52:40.960
<v Speaker 3>The other side of that is actually around the technology itself.

0:52:40.960 --> 0:52:43.359
<v Speaker 3>And as you say, I'm a total nerd for particle accelerators.

0:52:43.400 --> 0:52:47.000
<v Speaker 3>It is my professional day job. I design particle accelerators.

0:52:47.040 --> 0:52:50.480
<v Speaker 3>I love it. They're great machines. And one of the

0:52:50.480 --> 0:52:52.719
<v Speaker 3>reasons I love it, and the reason I chose it

0:52:53.120 --> 0:52:56.400
<v Speaker 3>back when I chose my PhD topic, was because someone

0:52:57.400 --> 0:52:59.959
<v Speaker 3>who turned out to be my PhD supervisor he called.

0:53:00.200 --> 0:53:01.799
<v Speaker 3>He was like, so this isn't what you applied for,

0:53:01.880 --> 0:53:05.920
<v Speaker 3>because originally I applied to do particle physics with Higgs

0:53:05.920 --> 0:53:08.960
<v Speaker 3>Boson type stuff. And he said, okay, hear me out,

0:53:09.000 --> 0:53:11.879
<v Speaker 3>hear me out. I want to design a new type

0:53:11.880 --> 0:53:15.360
<v Speaker 3>of particle accelerator to treat cancer. And I was just like,

0:53:16.000 --> 0:53:20.520
<v Speaker 3>what what do you mean? Why are you find beings

0:53:20.560 --> 0:53:24.200
<v Speaker 3>at people? And it turned out I was just I

0:53:24.280 --> 0:53:26.440
<v Speaker 3>just was a bit naive. I didn't realize that you

0:53:26.480 --> 0:53:31.320
<v Speaker 3>could use these technologies at smaller scales for all sorts

0:53:31.360 --> 0:53:35.640
<v Speaker 3>of societal applications. So about half of all cancer treatments

0:53:35.640 --> 0:53:41.240
<v Speaker 3>are actually done using small particle accelerators. For what's called radiotherapy,

0:53:41.320 --> 0:53:43.920
<v Speaker 3>which is one of the most successful forms of cancer

0:53:43.920 --> 0:53:47.800
<v Speaker 3>treatment that we've ever had, and it's a small electronic accelerator.

0:53:47.800 --> 0:53:50.240
<v Speaker 3>It generates X rays and then you shape those two

0:53:50.920 --> 0:53:53.760
<v Speaker 3>the tumor inside the body, and the whole accelerator actually

0:53:53.920 --> 0:53:56.600
<v Speaker 3>rotates around the patient to be able to deliver beams

0:53:56.600 --> 0:53:59.799
<v Speaker 3>from different angles. And nowadays we have more advanced forms

0:53:59.840 --> 0:54:03.360
<v Speaker 3>of cancer treatment using heavier particles like protons and carbon

0:54:03.440 --> 0:54:06.080
<v Speaker 3>ions that are more precise in the way that they

0:54:06.120 --> 0:54:10.120
<v Speaker 3>deposit the dose. And that was the area that I

0:54:10.160 --> 0:54:13.080
<v Speaker 3>did my PhD on and even today I run a

0:54:13.080 --> 0:54:18.000
<v Speaker 3>research group about accelerators for medical applications. And so when

0:54:18.040 --> 0:54:21.600
<v Speaker 3>you look at it, there's about fifty thousand particle accelerators

0:54:21.600 --> 0:54:24.280
<v Speaker 3>in the world, and only a fraction of a percent

0:54:24.360 --> 0:54:28.440
<v Speaker 3>are actually used for particle physics. And so what has

0:54:28.480 --> 0:54:31.920
<v Speaker 3>happened since we first invented accelerators in the nineteen twenties

0:54:31.960 --> 0:54:35.440
<v Speaker 3>and thirties is that as we invent these new technologies

0:54:36.200 --> 0:54:40.160
<v Speaker 3>and the knowledge of how to accelerate beams of fundamental

0:54:40.200 --> 0:54:44.880
<v Speaker 3>particles and control them, more and more applications have emerged,

0:54:44.920 --> 0:54:48.680
<v Speaker 3>so not just in cancer treatment, but also in industries.

0:54:48.840 --> 0:54:52.400
<v Speaker 3>So you can use particle accelerators to change the color

0:54:52.440 --> 0:54:57.440
<v Speaker 3>of a gemstone by bombarding diamonds, you know, diamond companies

0:54:57.480 --> 0:55:01.400
<v Speaker 3>to conchange the color of a gemstone, often from clear

0:55:01.440 --> 0:55:05.080
<v Speaker 3>to pink. Now that's you know, that's quite capitalistic because

0:55:05.120 --> 0:55:06.799
<v Speaker 3>note you're just trying to gain a bit more money.

0:55:06.920 --> 0:55:09.840
<v Speaker 3>That's not really a very very very useful thing. But actually,

0:55:09.880 --> 0:55:15.080
<v Speaker 3>all the devices that we use today rely on electronic chips,

0:55:15.400 --> 0:55:17.279
<v Speaker 3>and today those are so small that you have to

0:55:17.280 --> 0:55:20.320
<v Speaker 3>implant ions one by one. You can't do that using chemistry.

0:55:20.520 --> 0:55:24.560
<v Speaker 3>You have to do it using effectively a small particle accelerator.

0:55:24.920 --> 0:55:28.440
<v Speaker 3>And so almost everywhere you look, in every aspect of society,

0:55:28.960 --> 0:55:32.040
<v Speaker 3>you will find somewhere in there a story about how

0:55:32.160 --> 0:55:37.279
<v Speaker 3>we use this really advanced technologies to create sort of

0:55:37.280 --> 0:55:40.200
<v Speaker 3>the modern world around us. And yet we almost always

0:55:40.239 --> 0:55:42.759
<v Speaker 3>don't know don't know that it's there. And some of

0:55:42.800 --> 0:55:46.480
<v Speaker 3>the most I think inspiring work that happens there is

0:55:46.520 --> 0:55:50.600
<v Speaker 3>when we're looking at things like you know, in the

0:55:50.880 --> 0:55:53.560
<v Speaker 3>environment or in cultural heritage. So we're able to do

0:55:54.000 --> 0:55:58.600
<v Speaker 3>really advanced dating techniques putting together you know, the deep

0:55:59.160 --> 0:56:03.680
<v Speaker 3>prehistoric story of our Earth and our species and other

0:56:03.719 --> 0:56:08.200
<v Speaker 3>species across large tracts of time because we have these

0:56:08.239 --> 0:56:12.200
<v Speaker 3>techniques that come from fundamental physics. And so this is

0:56:12.239 --> 0:56:14.320
<v Speaker 3>where I get really excited, is because I'm like, Okay,

0:56:14.360 --> 0:56:16.520
<v Speaker 3>so I can sit in the lab every day, I

0:56:16.560 --> 0:56:19.359
<v Speaker 3>can design these machines, I can test them, and they

0:56:19.360 --> 0:56:24.719
<v Speaker 3>can be used for everything from you know, looking at

0:56:24.760 --> 0:56:29.120
<v Speaker 3>an artwork to discover whether it's real or fake, to

0:56:30.719 --> 0:56:33.760
<v Speaker 3>shrinking the shrink wrap that goes around a Christmas turkey.

0:56:33.880 --> 0:56:37.440
<v Speaker 3>That's a real application polem. A cross linking is the

0:56:37.520 --> 0:56:41.560
<v Speaker 3>technical term, but you know, you know, to uncovering the

0:56:41.640 --> 0:56:44.279
<v Speaker 3>Higgs boson in the secrets of the universe. And to me,

0:56:44.840 --> 0:56:47.920
<v Speaker 3>the fact that it's the same physics and the same

0:56:48.160 --> 0:56:50.680
<v Speaker 3>area of research that I can do that that contributes

0:56:50.680 --> 0:56:53.399
<v Speaker 3>to all of these different areas of our society. That

0:56:53.440 --> 0:56:56.400
<v Speaker 3>gets me really excited because I'm never bored. I can

0:56:56.440 --> 0:56:59.640
<v Speaker 3>always choose a new application. I can always choose a

0:56:59.680 --> 0:57:04.560
<v Speaker 3>new type of machine to work on. And we're always

0:57:04.600 --> 0:57:08.400
<v Speaker 3>trying to make improvements in the energy efficiency, you know,

0:57:08.440 --> 0:57:12.040
<v Speaker 3>trying to make things smaller and better and cheaper, and

0:57:12.320 --> 0:57:15.919
<v Speaker 3>just trying to push forward the frontiers of these technologies

0:57:16.440 --> 0:57:21.200
<v Speaker 3>using our knowledge of fundamental physics in order to do

0:57:21.320 --> 0:57:23.840
<v Speaker 3>some good in the world, you know, to actually make

0:57:23.880 --> 0:57:26.919
<v Speaker 3>a difference to people's lives, and that's why I show

0:57:27.000 --> 0:57:28.920
<v Speaker 3>up in the lab every day. And I've had a

0:57:28.960 --> 0:57:30.880
<v Speaker 3>lot of people say, well, I had no idea that

0:57:30.920 --> 0:57:34.160
<v Speaker 3>you could do that with physics. That's amazing. And so

0:57:34.200 --> 0:57:35.960
<v Speaker 3>I've been told on a number of occasions that my

0:57:36.080 --> 0:57:40.280
<v Speaker 3>job today is kind of the current equivalent of being

0:57:40.280 --> 0:57:43.280
<v Speaker 3>a rocket scientist. You know, I'm sort of working on

0:57:43.280 --> 0:57:45.960
<v Speaker 3>this cutting edge of technology which is taking us to

0:57:46.040 --> 0:57:50.960
<v Speaker 3>new frontiers of knowledge and exploration. And while it's not

0:57:51.040 --> 0:57:52.880
<v Speaker 3>quite as dramatic as a rocket, when you start up

0:57:52.880 --> 0:57:56.560
<v Speaker 3>one of these machines, it is to me incredibly inspiring.

0:57:56.600 --> 0:58:00.600
<v Speaker 3>And every approach that we take, whether it's collaborating, you know,

0:58:00.640 --> 0:58:03.800
<v Speaker 3>in a multidisciplinary sense I collaborate very strongly with cancer

0:58:03.840 --> 0:58:08.920
<v Speaker 3>researchers nowadays, or collaborating across different nations and different technical skills,

0:58:09.760 --> 0:58:14.240
<v Speaker 3>I think really this type of research is sort of

0:58:15.000 --> 0:58:18.520
<v Speaker 3>unique in a way, but it's also representative of the

0:58:18.560 --> 0:58:24.160
<v Speaker 3>approach that I think has led us to so many successes, both,

0:58:24.800 --> 0:58:27.880
<v Speaker 3>you know, both in science but also in terms of

0:58:27.960 --> 0:58:30.960
<v Speaker 3>improving our lives as people.

0:58:40.360 --> 0:58:44.160
<v Speaker 2>I have a question about how you approach experiments in

0:58:44.200 --> 0:58:49.920
<v Speaker 2>physics when you're doing an experiment and you're getting results

0:58:50.000 --> 0:58:52.040
<v Speaker 2>that are not at all what you expect to see.

0:58:53.640 --> 0:58:57.600
<v Speaker 2>How do you prioritize exploring the options that what you

0:58:57.680 --> 0:59:01.040
<v Speaker 2>expect to see is wrong versus there is something wrong

0:59:01.040 --> 0:59:01.720
<v Speaker 2>with your method.

0:59:03.600 --> 0:59:06.240
<v Speaker 3>I always err on the side of assuming I'm an idiot,

0:59:07.120 --> 0:59:13.240
<v Speaker 3>So maybe just imposters in drome, But no, okay, this

0:59:13.440 --> 0:59:16.560
<v Speaker 3>is kind of what I mean about ensuring you one

0:59:16.600 --> 0:59:19.880
<v Speaker 3>hundred percent understand your apparatus. So typically when you start

0:59:19.880 --> 0:59:22.080
<v Speaker 3>out an experiment and I'm thinking here of just a

0:59:22.120 --> 0:59:26.400
<v Speaker 3>small experiment that I built in the UK, and when

0:59:26.400 --> 0:59:28.280
<v Speaker 3>we first started using it, we'd get all these like

0:59:28.320 --> 0:59:33.440
<v Speaker 3>electrical signals that we just didn't understand, and so my

0:59:33.480 --> 0:59:36.360
<v Speaker 3>assumption there was not that the fundamental thing that I

0:59:36.440 --> 0:59:40.760
<v Speaker 3>was trying to study was wrong. My assumption almost always

0:59:40.920 --> 0:59:43.600
<v Speaker 3>is to assume that I don't understand my experiment well enough,

0:59:44.240 --> 0:59:47.600
<v Speaker 3>and to devise little tests and little questions and little

0:59:47.640 --> 0:59:51.680
<v Speaker 3>experiments to test my understanding of the equipment and to

0:59:51.800 --> 0:59:55.520
<v Speaker 3>test you know, I'll always pull it back to a

0:59:55.560 --> 0:59:57.840
<v Speaker 3>test case where I'm like, okay, I should one hundred

0:59:57.840 --> 1:00:01.160
<v Speaker 3>percent know the outcome of doing this test, So then

1:00:01.160 --> 1:00:04.080
<v Speaker 3>I run that test and if that one is still failing.

1:00:04.840 --> 1:00:07.400
<v Speaker 3>Then I'm like, Okay, there's something wrong with the equipment,

1:00:07.840 --> 1:00:10.400
<v Speaker 3>and maybe there's something wrong or maybe I've dialed it

1:00:10.440 --> 1:00:12.840
<v Speaker 3>in wrong, or I've got the wrong impedance matching, or

1:00:12.880 --> 1:00:16.560
<v Speaker 3>I've got you know, like something, something that I've failed

1:00:16.600 --> 1:00:20.520
<v Speaker 3>to recognize is important in the experiment doing what I

1:00:20.560 --> 1:00:22.480
<v Speaker 3>wanted to do. And I think that would be a

1:00:22.480 --> 1:00:25.800
<v Speaker 3>familiar experience to almost every experiment, which is to go

1:00:25.880 --> 1:00:29.320
<v Speaker 3>in with this overabundance of optimism that everything's going to

1:00:29.360 --> 1:00:32.520
<v Speaker 3>work first time, and then slowly work your way through

1:00:32.760 --> 1:00:35.040
<v Speaker 3>the many, many, many ways in which you were wrong

1:00:36.280 --> 1:00:40.320
<v Speaker 3>until you really fully understand everything that's happening. And then

1:00:41.000 --> 1:00:44.640
<v Speaker 3>then if you're testing your theory, or maybe there isn't

1:00:44.640 --> 1:00:46.560
<v Speaker 3>a theory, maybe you're just testing something that doesn't have

1:00:46.560 --> 1:00:49.280
<v Speaker 3>a theory yet, and if then it's coming back and

1:00:49.320 --> 1:00:52.360
<v Speaker 3>giving you a result that you don't expect, then you

1:00:52.440 --> 1:00:55.200
<v Speaker 3>start to get those little you know, I'm getting shivers

1:00:55.240 --> 1:00:57.200
<v Speaker 3>just saying it. It's ridiculous, isn't it. But like those

1:00:57.240 --> 1:00:59.520
<v Speaker 3>little shivers which say, oh, this is something new, this

1:00:59.600 --> 1:01:04.480
<v Speaker 3>isn't all. This is a potential to discover something that

1:01:04.480 --> 1:01:09.320
<v Speaker 3>no one's ever seen before, and it's in that mode

1:01:09.360 --> 1:01:13.920
<v Speaker 3>where you're both confident in your experiment that you can

1:01:14.040 --> 1:01:18.320
<v Speaker 3>really ask the questions about the nature of reality. And

1:01:18.760 --> 1:01:21.400
<v Speaker 3>in that moment, I think more often than not, you

1:01:21.560 --> 1:01:25.280
<v Speaker 3>want to be wrong, right. You want nature to be

1:01:26.760 --> 1:01:29.080
<v Speaker 3>throwing a caveball at you, You want it to be

1:01:29.120 --> 1:01:33.280
<v Speaker 3>something surprising, and those are I think those are the

1:01:33.280 --> 1:01:38.640
<v Speaker 3>moments in which would be the closest that I think

1:01:38.680 --> 1:01:41.200
<v Speaker 3>you would get to having sort of a Eureka moment

1:01:41.320 --> 1:01:44.440
<v Speaker 3>or that moment of I've seen something new for the

1:01:44.520 --> 1:01:48.120
<v Speaker 3>very first time. And it's only by working your way

1:01:48.160 --> 1:01:50.280
<v Speaker 3>through those smaller steps that you can get to that

1:01:50.400 --> 1:01:52.880
<v Speaker 3>level of confidence. And I think a lot of people

1:01:54.240 --> 1:01:58.040
<v Speaker 3>don't realize that that is very much the day to

1:01:58.120 --> 1:02:02.040
<v Speaker 3>day role of an experiment or is working your way

1:02:02.120 --> 1:02:05.960
<v Speaker 3>through these annoying things, and you have to learn to

1:02:06.040 --> 1:02:09.800
<v Speaker 3>love that process, right, You have to learn to love

1:02:09.960 --> 1:02:12.520
<v Speaker 3>the small bits of understanding and the small discoveries that

1:02:12.560 --> 1:02:15.200
<v Speaker 3>come along the way. You know, maybe you've discovered a

1:02:15.240 --> 1:02:19.520
<v Speaker 3>new way of arranging your apparatus that happens to give you,

1:02:19.520 --> 1:02:21.800
<v Speaker 3>you know, ten times more signal than you had before,

1:02:21.840 --> 1:02:25.760
<v Speaker 3>and that's really satisfying. And so I think experimental science.

1:02:25.920 --> 1:02:29.640
<v Speaker 3>For that reason, it sort of appeals to people who

1:02:29.720 --> 1:02:33.440
<v Speaker 3>like to tinker. It appeals to the detail orientated mind.

1:02:33.880 --> 1:02:36.840
<v Speaker 3>At the same time it has to appeal to people

1:02:36.880 --> 1:02:39.800
<v Speaker 3>who have that bigger vision, you know, who have that

1:02:40.960 --> 1:02:43.800
<v Speaker 3>longer term time frame, because if you expect to go

1:02:43.800 --> 1:02:46.040
<v Speaker 3>into the lab every day and make one discovery every day,

1:02:46.040 --> 1:02:49.280
<v Speaker 3>you're going to be solely disappointed. But if you can

1:02:49.360 --> 1:02:52.960
<v Speaker 3>keep in mind the big picture and work toward that

1:02:53.120 --> 1:02:56.280
<v Speaker 3>over and often it is years, you know, and keep

1:02:56.440 --> 1:03:00.440
<v Speaker 3>that enthusiasm and keep that wonder that have in the

1:03:00.520 --> 1:03:03.720
<v Speaker 3>lab every day, I think that's the sort of personality

1:03:03.840 --> 1:03:07.440
<v Speaker 3>type that fits experimental science very very well.

1:03:08.040 --> 1:03:10.040
<v Speaker 2>There's a point about your book that I really love

1:03:10.080 --> 1:03:13.720
<v Speaker 2>you in talking about how big projects like the large

1:03:13.760 --> 1:03:16.080
<v Speaker 2>hadron collider you've talked about this today as well, are

1:03:16.520 --> 1:03:22.400
<v Speaker 2>illustrative of deeper points about human collaboration. And I wonder if,

1:03:23.160 --> 1:03:24.880
<v Speaker 2>in a way you even alluded to this earlier when

1:03:24.880 --> 1:03:27.320
<v Speaker 2>you were talking about what types of experiments are easier

1:03:27.360 --> 1:03:30.600
<v Speaker 2>to talk about in the setting like our conversation today.

1:03:31.160 --> 1:03:34.160
<v Speaker 2>I wonder if these big collaborative stories like the large

1:03:34.160 --> 1:03:37.720
<v Speaker 2>Hadron collider are more difficult to fit in the shape

1:03:37.760 --> 1:03:41.080
<v Speaker 2>of a compelling and memorable narrative than stories with a

1:03:41.120 --> 1:03:44.920
<v Speaker 2>single protagonist. Obviously, a lot of the most inspiring and

1:03:44.960 --> 1:03:48.320
<v Speaker 2>amazing stories in your book are about these huge megaprojects

1:03:48.320 --> 1:03:52.240
<v Speaker 2>with these unthinkable amounts of coordination and collaboration. Are there

1:03:52.280 --> 1:03:56.320
<v Speaker 2>tricks to telling those stories in a way that makes

1:03:56.360 --> 1:03:59.440
<v Speaker 2>them work as stories? But it's still true to the reality.

1:04:01.520 --> 1:04:05.240
<v Speaker 3>It was very difficult. Yes, So I will definitely acknowledge

1:04:05.240 --> 1:04:08.400
<v Speaker 3>it is so much harder to write about enormous collaborations

1:04:08.440 --> 1:04:12.120
<v Speaker 3>than it is to write about a few individuals. And

1:04:12.200 --> 1:04:15.960
<v Speaker 3>I think in terms of the story, you know, the

1:04:16.000 --> 1:04:20.920
<v Speaker 3>story arc or the narrative creation process. I had to

1:04:20.960 --> 1:04:26.440
<v Speaker 3>find my own route through that, and so I was

1:04:26.480 --> 1:04:30.880
<v Speaker 3>looking for things like, Okay, well, you know, if i'm

1:04:31.040 --> 1:04:34.040
<v Speaker 3>if I'm creating a sort of story arc, so you know,

1:04:34.080 --> 1:04:36.560
<v Speaker 3>what would my crisis moment be, What would you know,

1:04:36.640 --> 1:04:40.200
<v Speaker 3>what would a sort of pinnacle moment be? What is

1:04:40.240 --> 1:04:44.200
<v Speaker 3>my like sort of inciting idea that sort of sets

1:04:44.560 --> 1:04:48.000
<v Speaker 3>sets that story off on a journey. And you can

1:04:48.200 --> 1:04:52.600
<v Speaker 3>find those things within the stories of the big experiments.

1:04:52.960 --> 1:04:57.200
<v Speaker 3>It does make it harder to focus on individual but

1:04:57.320 --> 1:05:00.760
<v Speaker 3>I actually, in the end, especially for the large Hadron Collider.

1:05:00.800 --> 1:05:03.760
<v Speaker 3>I used myself as an example of a tiny, tiny

1:05:03.760 --> 1:05:07.280
<v Speaker 3>individual within this enormous collaboration, and that worked for me

1:05:07.360 --> 1:05:10.520
<v Speaker 3>partly because I actually didn't go on to continue in

1:05:10.560 --> 1:05:13.280
<v Speaker 3>that collaboration. I worked in it. As a student. I

1:05:13.320 --> 1:05:17.880
<v Speaker 3>did this very very small project which people love to

1:05:17.320 --> 1:05:21.160
<v Speaker 3>h to recite the name of the project that I did,

1:05:21.200 --> 1:05:25.680
<v Speaker 3>which was it was the design of a no, hang on,

1:05:26.480 --> 1:05:27.840
<v Speaker 3>I'm going to get it, I'm going to get it wrong.

1:05:27.840 --> 1:05:30.600
<v Speaker 3>But it was the design of a monitoring system for

1:05:30.680 --> 1:05:33.760
<v Speaker 3>the heating for that sorry, for the heaters of the

1:05:33.800 --> 1:05:37.240
<v Speaker 3>cooling system, of the inner detector of the atlast.

1:05:36.800 --> 1:05:41.600
<v Speaker 2>Experiment cooling system.

1:05:41.920 --> 1:05:44.560
<v Speaker 3>Now the monitoring system. Yes, the monitoring system for the

1:05:44.560 --> 1:05:48.600
<v Speaker 3>heaters of the cooling system. Okay, if you have a

1:05:48.600 --> 1:05:52.560
<v Speaker 3>cooling system and you don't want it to all like

1:05:52.760 --> 1:05:56.360
<v Speaker 3>clog up with condensation, right, so sometimes you need heaters

1:05:56.400 --> 1:05:58.920
<v Speaker 3>on there to bring the temperature back up and stabilize it,

1:05:58.960 --> 1:06:00.520
<v Speaker 3>like you need to be able to move temperature in

1:06:00.520 --> 1:06:05.120
<v Speaker 3>two directions anyway. So that was my crazy, you know,

1:06:05.200 --> 1:06:07.440
<v Speaker 3>tidy little project that I did for three months when

1:06:07.480 --> 1:06:10.360
<v Speaker 3>I was a summer student as an undergraduate working at CERN.

1:06:10.960 --> 1:06:16.680
<v Speaker 3>And it was illustrative though, of this idea that you know,

1:06:16.920 --> 1:06:20.600
<v Speaker 3>I was this sort of tiny cog in this enormous machine.

1:06:21.000 --> 1:06:24.880
<v Speaker 3>And I think the way I used that story was

1:06:24.960 --> 1:06:28.800
<v Speaker 3>also to sort of say I doubted that this machine

1:06:28.840 --> 1:06:32.880
<v Speaker 3>could ever work, because if I was making this contribution

1:06:33.080 --> 1:06:35.720
<v Speaker 3>and deep within my code was the ability to switch

1:06:35.760 --> 1:06:38.880
<v Speaker 3>the whole machine off, then surely, you know, statistically, this

1:06:38.880 --> 1:06:41.840
<v Speaker 3>thing was never never going to work, and so I

1:06:41.880 --> 1:06:45.760
<v Speaker 3>was as surprised as everybody else. Well, I don't think

1:06:45.280 --> 1:06:48.320
<v Speaker 3>the actual rest of the collaboration would have been surprised

1:06:48.320 --> 1:06:52.360
<v Speaker 3>when it worked, but I was surprised from my experience

1:06:52.840 --> 1:06:55.000
<v Speaker 3>when it worked as well as it did when they

1:06:55.000 --> 1:06:59.240
<v Speaker 3>started the machine up. Of course, people who remember back

1:06:59.240 --> 1:07:01.120
<v Speaker 3>in two thousand and eight will remember that it worked

1:07:01.160 --> 1:07:04.000
<v Speaker 3>for about seven days before it blew itself up, and

1:07:04.040 --> 1:07:05.919
<v Speaker 3>then they spent a year fixing it before it came

1:07:05.960 --> 1:07:08.880
<v Speaker 3>back online. And I was I was at an event

1:07:08.920 --> 1:07:11.080
<v Speaker 3>the other day where someone referred to the startup of

1:07:11.120 --> 1:07:14.160
<v Speaker 3>the large Hudron collider, in which they said, about two

1:07:14.200 --> 1:07:17.200
<v Speaker 3>thousand and eight, with a shake of the hand, you know,

1:07:17.600 --> 1:07:20.560
<v Speaker 3>this is sort of you know, this Italian style like

1:07:21.440 --> 1:07:25.040
<v Speaker 3>wobble of the hand that means roughly they did that.

1:07:25.200 --> 1:07:27.240
<v Speaker 3>They said it started laughing about two thousand and eight,

1:07:27.320 --> 1:07:31.040
<v Speaker 3>and it was all about that hand wobble of like, oh,

1:07:31.080 --> 1:07:33.360
<v Speaker 3>that means the machine blew itself up and it had

1:07:33.400 --> 1:07:35.960
<v Speaker 3>to be fixed for a year. But anyway, so I'm

1:07:35.960 --> 1:07:38.360
<v Speaker 3>getting off the track onto the large Hudron collider. But

1:07:38.400 --> 1:07:40.800
<v Speaker 3>I think, I think, yes, it is much more difficult

1:07:41.920 --> 1:07:45.880
<v Speaker 3>to write narratives about enormous collaborations. But I think that

1:07:46.000 --> 1:07:49.720
<v Speaker 3>speaks to something a little deepant is something which has

1:07:49.760 --> 1:07:53.040
<v Speaker 3>come out of conversations with people now that we're studying

1:07:53.200 --> 1:07:58.320
<v Speaker 3>even larger colliders. So the next one potential next iteration

1:07:58.480 --> 1:08:01.920
<v Speaker 3>is one hundred kilometers in succumb and will take about

1:08:02.000 --> 1:08:06.920
<v Speaker 3>forty years to build, to design and build. That's getting

1:08:06.960 --> 1:08:10.120
<v Speaker 3>to the same lengths as or longer than a lot

1:08:10.120 --> 1:08:15.560
<v Speaker 3>of careers in the field. And so I think we

1:08:15.720 --> 1:08:17.840
<v Speaker 3>are running into and it's something that I've been talking

1:08:17.840 --> 1:08:21.679
<v Speaker 3>to people about, a sort of two big, too long,

1:08:21.960 --> 1:08:26.840
<v Speaker 3>too complex problem with these collaborations. And even though they

1:08:27.640 --> 1:08:30.639
<v Speaker 3>I find them more inspiring in what they have been

1:08:30.680 --> 1:08:35.360
<v Speaker 3>able to achieve. If I was given the choice again,

1:08:35.720 --> 1:08:39.640
<v Speaker 3>now you know, I'm a student, I'm raring to go

1:08:39.680 --> 1:08:44.200
<v Speaker 3>in this field. I'm really interested, what would I choose

1:08:44.240 --> 1:08:47.519
<v Speaker 3>to work on, for saying, my PhD now at the

1:08:47.560 --> 1:08:51.360
<v Speaker 3>age of early twenties, embarking on a PhD, which can

1:08:51.400 --> 1:08:54.720
<v Speaker 3>be anywhere between about three and however many years, you know,

1:08:54.800 --> 1:08:58.040
<v Speaker 3>seven eight years for some people, it's a huge commitment

1:08:58.120 --> 1:09:00.000
<v Speaker 3>and a huge chunk of your life at that age.

1:09:00.760 --> 1:09:05.400
<v Speaker 3>And totally I hear stories of professors who are struggling

1:09:05.439 --> 1:09:09.880
<v Speaker 3>to recruit students to projects for the sort of next

1:09:09.920 --> 1:09:12.640
<v Speaker 3>mega colliders because they're like, well, there's not going to

1:09:12.640 --> 1:09:15.400
<v Speaker 3>be any data to work with for forty years. Like

1:09:15.880 --> 1:09:17.680
<v Speaker 3>how am I going to have a career in this

1:09:17.800 --> 1:09:19.960
<v Speaker 3>Why would I commit three to seven years to something

1:09:19.960 --> 1:09:24.679
<v Speaker 3>that might not even be built? And so I don't

1:09:24.680 --> 1:09:26.360
<v Speaker 3>want to make out like there's a crisis or a

1:09:26.439 --> 1:09:28.519
<v Speaker 3>lack of people who are interested and very committed to

1:09:28.520 --> 1:09:33.519
<v Speaker 3>this field. But I just hear inklings of dissatisfaction or

1:09:33.720 --> 1:09:40.160
<v Speaker 3>sort of little little inklings of trouble, and I'm I'm

1:09:40.240 --> 1:09:43.559
<v Speaker 3>curious about that, and I'm curious about how we're going

1:09:43.600 --> 1:09:46.960
<v Speaker 3>to resolve that. And I guess there's two parts. Either

1:09:46.960 --> 1:09:48.840
<v Speaker 3>we find a way to resolve that through the career

1:09:48.880 --> 1:09:53.280
<v Speaker 3>structure and through having shorter projects alongside these big, long

1:09:53.360 --> 1:09:57.880
<v Speaker 3>ones that you know, keep people motivated and keep everyone working,

1:09:58.240 --> 1:10:00.679
<v Speaker 3>or we really have to think about are these projects

1:10:00.680 --> 1:10:06.040
<v Speaker 3>too big? Should we really be focusing all our energy

1:10:06.160 --> 1:10:11.040
<v Speaker 3>on technologies which can shrink down the size of future

1:10:11.280 --> 1:10:14.800
<v Speaker 3>collided projects, which is very very difficult although they are

1:10:14.840 --> 1:10:22.160
<v Speaker 3>in progress. And also just refocus back down on the

1:10:22.200 --> 1:10:26.160
<v Speaker 3>sort of structure in which these collaborations work, because realistically,

1:10:26.400 --> 1:10:29.240
<v Speaker 3>you've got groups of about ten to twenty people in

1:10:29.280 --> 1:10:32.919
<v Speaker 3>a research group in a university. Those work on specific

1:10:32.960 --> 1:10:35.280
<v Speaker 3>sub areas of the experiment, and then they all join

1:10:35.360 --> 1:10:37.920
<v Speaker 3>together and eventually you get you know, two thousand people.

1:10:39.080 --> 1:10:41.880
<v Speaker 3>And so it's not that two thousand people are sort

1:10:41.880 --> 1:10:46.000
<v Speaker 3>of a negalitarian, you know, flat structure who all somehow

1:10:46.040 --> 1:10:49.040
<v Speaker 3>know each other and communicate. That would be absolutely wild.

1:10:49.640 --> 1:10:54.599
<v Speaker 3>There is a substructure, and so I'm interested in how

1:10:54.640 --> 1:10:58.200
<v Speaker 3>we can use that substructure that works very well in small,

1:10:58.320 --> 1:11:01.280
<v Speaker 3>close knit groups who then go out and work with

1:11:01.320 --> 1:11:03.760
<v Speaker 3>other groups around the world. Perhaps there's a way we

1:11:03.760 --> 1:11:07.439
<v Speaker 3>can do that in the time domain as well. Right, so,

1:11:07.520 --> 1:11:11.200
<v Speaker 3>perhaps there's a way of having more contained sections of projects,

1:11:12.000 --> 1:11:15.080
<v Speaker 3>perhaps with applications, you know, that sort of keep people

1:11:15.640 --> 1:11:18.760
<v Speaker 3>interested on that sort of you know, few year timescale

1:11:19.600 --> 1:11:21.920
<v Speaker 3>that can drive things along. So maybe instead of in

1:11:21.960 --> 1:11:24.120
<v Speaker 3>the future, instead of contributing to hardware or sitting in

1:11:24.200 --> 1:11:28.000
<v Speaker 3>a control room, maybe you're contributing to the societal applications

1:11:28.080 --> 1:11:31.120
<v Speaker 3>of the spin offs of the work that you're doing

1:11:31.200 --> 1:11:37.680
<v Speaker 3>alongside developing the longer term curiosity driven parts. That's just

1:11:37.760 --> 1:11:41.960
<v Speaker 3>my idea. It's very much an unsolved thing. But I

1:11:41.960 --> 1:11:44.599
<v Speaker 3>think if I was given the chance again, I would

1:11:44.640 --> 1:11:47.280
<v Speaker 3>struggle to commit to a project that wasn't going to

1:11:47.360 --> 1:11:50.479
<v Speaker 3>have data for forty years. So I do want to

1:11:50.479 --> 1:11:52.639
<v Speaker 3>acknowledge that it's a very interesting time for young people

1:11:52.720 --> 1:11:55.200
<v Speaker 3>to be entering the field in that sense.

1:11:56.320 --> 1:11:58.040
<v Speaker 2>Right at the end of the book, you offer a

1:11:58.080 --> 1:11:59.840
<v Speaker 2>couple of big lessons that you think we need to

1:12:00.080 --> 1:12:03.439
<v Speaker 2>brace for the future of physics and collaborative research projects.

1:12:03.520 --> 1:12:05.360
<v Speaker 2>Do you want to mention those before we sign off?

1:12:06.160 --> 1:12:07.840
<v Speaker 3>Yes. So, I think some of the things that I've

1:12:07.920 --> 1:12:11.240
<v Speaker 3>learned through writing the book around collaboration and this curiosity

1:12:11.400 --> 1:12:15.040
<v Speaker 3>driven research is that it is so important that we

1:12:15.439 --> 1:12:18.160
<v Speaker 3>value it, that we value its impact in society, and

1:12:18.240 --> 1:12:21.479
<v Speaker 3>that we create space for people to do this kind

1:12:21.520 --> 1:12:25.320
<v Speaker 3>of research, not just space, but also it requires funding.

1:12:25.360 --> 1:12:27.040
<v Speaker 3>And I know it sounds a little daddy to mix

1:12:27.120 --> 1:12:31.000
<v Speaker 3>curiosity driven research and money, but in our society those

1:12:31.040 --> 1:12:33.080
<v Speaker 3>two things are going to have to go hand in hand.

1:12:33.160 --> 1:12:35.720
<v Speaker 3>So you know, even the future, we want to be

1:12:35.760 --> 1:12:39.439
<v Speaker 3>able to create collaborations so we can really get the

1:12:39.479 --> 1:12:43.960
<v Speaker 3>best out of specialized skills that people have to the

1:12:44.000 --> 1:12:48.040
<v Speaker 3>betterment of society. We need to really think about how

1:12:48.080 --> 1:12:51.479
<v Speaker 3>we value things that don't set out with a goal

1:12:51.520 --> 1:12:54.280
<v Speaker 3>in mind, and I think we need to center those

1:12:54.600 --> 1:12:58.240
<v Speaker 3>and we need to really value the fact that somebody

1:12:58.240 --> 1:13:02.200
<v Speaker 3>would commit their life and career to something where they

1:13:02.240 --> 1:13:05.240
<v Speaker 3>don't even know what the outcome is going to look like.

1:13:05.479 --> 1:13:07.840
<v Speaker 3>We need to protect that with everything that we have,

1:13:08.000 --> 1:13:11.680
<v Speaker 3>because that is such a generative force in our society

1:13:11.680 --> 1:13:12.120
<v Speaker 3>for good.

1:13:12.680 --> 1:13:15.240
<v Speaker 2>Susi Shi, thank you so much for talking today. It

1:13:15.240 --> 1:13:17.680
<v Speaker 2>has been a privilege and a pleasure lovely to be here.

1:13:17.720 --> 1:13:18.080
<v Speaker 3>Thanks Ja.

1:13:19.040 --> 1:13:21.720
<v Speaker 2>All right, well that's it for today. Thanks again to

1:13:21.720 --> 1:13:24.639
<v Speaker 2>Susie Sheihi for being so generous with her time. If

1:13:24.640 --> 1:13:26.280
<v Speaker 2>you want to pick up a copy of the book,

1:13:26.560 --> 1:13:30.519
<v Speaker 2>it is called The Matter of Everything, The Matter of Everything,

1:13:30.680 --> 1:13:33.720
<v Speaker 2>and it's out in hardback in ebook form and as

1:13:33.720 --> 1:13:37.320
<v Speaker 2>an audiobook narrated by Susie herself. Stuff to Blow Your

1:13:37.320 --> 1:13:39.920
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