WEBVTT

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Okay, let's get into this. We are doing a deep

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dive today into the story of a physicist whose

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work, I mean, it didn't just contribute to science,

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it fundamentally redefined our understanding

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of the universe. And yet her name is often, you

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know, kind of an afterthought when people list

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the greats. Exactly. We're talking about Dr.

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Chen Shengwu. If you look at the real heavy hitters

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in 20th century physics, her name has to be right

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at the top. She had all these powerful nicknames,

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almost like titles. Like what? Things like the

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First Lady of Physics, the Chinese Marie Curie,

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and maybe most importantly, the Queen of Nuclear

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Research. And those aren't just, you know, empty

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praise. They really point to the incredible scope

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of her work. We're talking about everything from

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nuclear fission to quantum entanglement. And

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her work on beta decay was foundational. Absolutely.

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She was, first and foremost, an experimentalist.

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I mean, a master experimentalist. When she got

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a result, it was meticulous, it was rigorous,

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and you just couldn't argue with it. Her precision

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was basically the gold standard for particle

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physics. It was. But her story isn't just about

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scientific genius. Is it? It's also a story of,

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well, profound injustice. And that really brings

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us to the central puzzle of her career. And it's

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really the core of our deep dive today. The Nobel

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Prize. The missing Nobel Prize. Right. If she

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was this master experimentalist, why do we always

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hear about the theorists? Why did Dr. Wu, who

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performed an experiment that some called the

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most important since the one that led to Einstein's

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relativity, why did she not get the 1957 Nobel

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Prize in physics? It's a huge question. The prize

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went to her colleagues, Tung Dao Lee. and Chen

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Ningyang for their theoretical idea. They predicted

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that a fundamental symmetry to the universe might

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be broken. And she's the one who proved it. She

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provided the physical definitive proof. And yet

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she was left out. It was a huge failure by the

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Nobel Committee to follow what was, you know,

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a pretty firm tradition of giving the prize to

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the experimentalists who actually confirm a theory.

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It's a massive oversight. I mean, other Nobel

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winners, like Jack Steinberger, have called it

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the biggest mistake the committee ever made.

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He did, yeah. So our mission for you today is

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to unpack her life, and we're going to do it

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chronologically. We want to focus on three huge

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scientific pillars that make this Nobel omission

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so, so staggering. First, her secret, absolutely

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vital work on the Manhattan Project. Then, her

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incredibly careful work that finally established

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Enrico Fermi's theory of beta decay. And of course,

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the big one. the famous high -stakes Wu experiment

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that shattered a law of nature. We want you to

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understand not just what she proved, but the

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sheer genius it took, experimentally and logistically,

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to actually pull it off. So to get that, we have

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to start at the beginning, in China. To understand

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the precision physicist, we have to go back to

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Luhe, Jiangsu province, in 1912. What's amazing

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right from the start is the environment she grew

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up in. Her father, Wu Zongyi, was just incredibly

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progressive. He really was. I mean, for a girl

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born in rural China in the early 20th century,

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her upbringing was extraordinary. Her father

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was an engineer and he was a social progressive

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who really believed in education for everyone,

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especially for women. And he didn't just believe

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it. He acted on it. That's the key. This wasn't

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just, you know, passive support. He went out

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and founded... The Mingda School for Girls. Yeah.

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That's where Wu got her primary education. He

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surrounded her with books and scientific journals.

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He was actively feeding her curiosity. And that

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encouragement just lit a fire in her. There's

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this incredible anecdote about her ambition when

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she was just 11 years old. Right. Applying for

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secondary school. She chose the Suzu Women's

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Normal School number two. And she picked the

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hardest path. The absolute hardest. The teacher

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training track. Yeah. Her family could have paid

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for an easier school, but she chose this highly

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competitive tuition -free program that would

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guarantee her a job. And to get in, she was ranked

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ninth out of about 10 ,000 applicants. Wow. Ninth

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out of 10 ,000. That kind of drive, that desire

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for rigor, it was there from the very beginning.

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And it wasn't just about books. She had this

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incredible capacity for political conviction,

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even while she was deep in her studies. At National

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Central University, where she started in math

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but switched to physics, she became a student

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leader. And this was during a really tense time

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with Japan. We're not talking about minor campus

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politics here. No, not at all. This was the volatile

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period right before the Sino -Japanese War. For

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a female physics student to get elected as a

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leader then was remarkable. She led these huge

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political protests, even a sit -in at the presidential

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palace in Nanjiang. And she met with Chiang Kai

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-shek. The students did, yes. But here's what's

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so telling about her character. The sources say

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she was incredibly disciplined. She never let

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all that political turmoil distract her from

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her studies. That balancing act, intense scientific

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focus on one hand and deep moral courage on the

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other that really drains her whole life. She

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also had a key female mentor early on, which

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must have been so rare. Her supervisor, Gu Jingwei.

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She was a female professor who had a Ph .D. from

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the University of Michigan. And she's the one

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who really pushed Wu to study abroad. And that

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advice basically set the stage for her move to

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the U .S. in 1936. Yeah, she sailed on the S

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.S. President Hoover, landed in San Francisco.

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The plan was to go to the University of Michigan,

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just like her mentor. But that's not what happened.

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No. That's when she ran into the first big shock

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of American academia. And it changed her entire

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career path. The Berkeley shock? What was that

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about? Well, she was just horrified by the sexism

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at Michigan. It was incredibly conservative back

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then. Women weren't even allowed to use the front

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entrance of the physics building. You're kidding.

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Nope. And that was an immediate deal breaker

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for her. She pivoted and chose the University

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of California, Berkeley instead, which was much

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more liberal and frankly was the place to be

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for physics at that time. Right. Berkeley was

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the epicenter of innovation. It really was. She

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was immediately immersed in the radiation laboratory

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run by Ernest O. Lawrence, you know, the inventor

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of the cyclotron. She met her future husband,

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Luke Yuan, there. It was just a hotbed of cutting

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-edge physics. And her colleagues there, they

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recognized her talent instantly. Oh, immediately.

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Luis Alvarez, who would go on to win a Nobel

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Prize himself, called her the most talented and

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most beautiful experimental physicist I've ever

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met. Emilio Segre, another giant, compared her

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to Marie Curie. He did. But he added that Wu

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was more worldly, elegant, and witty. Even Lawrence,

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the head of the lab, said she was the most talented

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female experimental physicist he'd ever known.

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But even with all that praise, she still ran

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into prejudice from the institution itself. The

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department head, Raymond Burge, he respected

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her talent enough to let her enroll late, but

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he was on record opposing Asian students getting

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scholarships. So she was in this weird position

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where her talent was undeniable, but the system

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was still pushing back against her. That talent.

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really came to a head with her PhD thesis in

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1940. It was incredible, not just for its content,

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but for its unforeseen historical importance.

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It had two parts, right? Two distinct parts.

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The first was on something called Remstralum.

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Which is what exactly? It's the x -rays that

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are produced when charged particles, in this

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case electrons, slow down really fast as they

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pass by atomic nuclei. She was studying this

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using phosphorus -32, which emits beta particles.

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This was her first really deep dive into beta

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decay, the field that she would just come to

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dominate. And the second part? The second part

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was on radioactive xenon isotopes that are produced

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during nuclear fission. And this is where things

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get really interesting. One of the physicists

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on her thesis committee was J. Robert Oppenheimer.

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The Oppenheimer. The Oppenheimer. And he was

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so blown away by this second part of her thesis

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that he apparently believed she knew everything

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there was to know about something called the

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neutron absorption cross -section of xenon. That

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sounds incredibly specific. It is incredibly

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specific. It's a tiny, esoteric piece of data

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buried in an unpublished PhD thesis. But that

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specific number, that little piece of knowledge,

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would just four years later become the key to

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saving the entire Manhattan Project from a catastrophic

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failure. It's amazing that Oppenheimer was so

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impressed. And yet, after she finishes this incredible

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thesis with recommendations from giants like

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Lawrence and Segre, what happens? Well, this

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is where that institutional genius wasn't enough

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to overcome the institutional barriers. She couldn't

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get a faculty position. Because she was a woman.

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An Asian. It was a combination of both. So she

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stayed at Berkeley for a bit as a postdoc and

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then eventually moved to the East Coast with

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Luke Ewan, who she married in 1942. She took

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a job at Smith College, I read. She did, and

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she found it deeply frustrating. It was a teaching

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-only position, and she had zero opportunity

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for the research that she was so passionate about.

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It got so bad, she had to write to Lawrence and

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ask for letters of recommendation just to get

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out of there. Did Smith try to keep her? They

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did. They upped her salary and made her an associate

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professor. But the lack of research was the real

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problem. So she moved on. She did. She took a

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much better position at Princeton University.

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And she actually made history there as the first

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female faculty member ever in their physics department.

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She was teaching Navy officers because, you know,

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it was wartime. But her very specific, very niche

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expertise was needed somewhere else, somewhere

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much more important. The Manhattan Project. In

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March of 1944, Dr. Wu joined what were called

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the Substitute Alloy Materials Laboratories,

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or SAM Labs, at Columbia. That's a great codename.

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It is. She was initially working on radiation

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detectors, but her role was about to become much,

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much bigger because of a sudden, terrifying crisis

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that was unfolding out in Washington state. This

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is the famous xenon crisis. It's one of those

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amazing stories where... A theoretical disaster

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is completely averted by this one specific piece

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of experimental data that almost no one knew

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existed. That's it. Exactly. In September 1944,

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Colonel Kenneth Nichols gets in touch with Wu

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about a massive problem they're having at the

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brand new B Reactor at the Hanford site. And

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the B Reactor was this was the big one, right?

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The first full scale nuclear reactor in the world.

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The very first. Its whole purpose was to produce

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plutonium 239 for the atomic bomb. It was supposed

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to sustain a controlled nuclear chain reaction.

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And at first it worked. It worked brilliantly.

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The chain reaction started up. It was self -sustaining.

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And then after just a few hours, the reaction

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rate would just plummet to zero. The reactor

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would shut itself down to stop. Then, hours later,

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it would mysteriously start back up on its own,

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only to shut down again a short time later. They

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were caught in this totally useless cycle, and

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nobody could figure out why. The whole project

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is on the line. What did they suspect was happening?

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Well, the top theorists, John Archibald Wheeler

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and the great Enrico Fermi, they suspected a

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specific byproduct of the fission process was

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the culprit, an isotope called xenon -135. Xenon

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-135. They theorized that it was acting as a

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neutron poison. It was just sucking up all the

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free neutrons that were needed to keep the chain

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reaction going. So it was poisoning its own reaction.

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That was the theory. But they needed proof. More

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than that, they needed the exact number. They

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needed to know precisely how likely xenon -135

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was to capture a neutron. That's its neutron

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absorption cross -section. If that number was

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big enough, their theory was right. And how did

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they find that number? This is the crucial part.

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Emilio Segre, who had been on Wu's PhD committee

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back at Berkeley, remembered her thesis. He remembered

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that unpublished second part about radioactive

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xenon isotopes. No way. Yes. Fermi immediately

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contacted Wu. She provided them with her typewritten

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draft. And there it was. Her paper, based on

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work she did years earlier, confirmed it. Xenon

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-135 had an absurdly, catastrophically large

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neutron absorption cross -section, much larger

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than anyone had predicted. So the reactor design

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was just wrong. It didn't account for this super

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poison. It was being poisoned by its own waste

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product. The xenon would build up, kill the reaction,

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then it would decay away over a few hours, which

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allowed the reactor to restart. and then the

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cycle would begin all over again. And Wu's data

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was the key to fixing it. It was everything.

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Her precise number allowed Wheeler to calculate

00:12:20.919 --> 00:12:23.340
exactly how much more uranium fuel they needed,

00:12:23.460 --> 00:12:25.940
and critically, how many extra control rods they

00:12:25.940 --> 00:12:28.120
had to build into the reactor to overcome the

00:12:28.120 --> 00:12:30.100
poisoning effect and keep it running continuously.

00:12:30.419 --> 00:12:33.220
So an unpublished thesis by a young female physicist,

00:12:33.480 --> 00:12:35.860
based on work done years before the project even

00:12:35.860 --> 00:12:38.480
began, literally rescued the most critical part

00:12:38.480 --> 00:12:40.840
of the war effort. That's not an exaggeration.

00:12:41.529 --> 00:12:43.990
Her findings were then used across the project

00:12:43.990 --> 00:12:46.570
to build the standard model for producing enriched

00:12:46.570 --> 00:12:49.309
uranium at Oak Ridge and even to design better

00:12:49.309 --> 00:12:51.929
Geiger counters. She was a true pioneer of the

00:12:51.929 --> 00:12:54.750
nuclear age. But she had reservations about it

00:12:54.750 --> 00:12:56.769
later, didn't she? She did. Like a lot of the

00:12:56.769 --> 00:12:59.070
scientists involved, she distanced herself from

00:12:59.070 --> 00:13:01.649
the destructive outcome. She said later she was

00:13:01.649 --> 00:13:04.529
glad her family in China was safe, but she expressed

00:13:04.529 --> 00:13:07.570
a hope that humankind could eventually live in

00:13:07.570 --> 00:13:10.549
peace. Her life's work really turned away from

00:13:10.549 --> 00:13:12.730
bombs and towards understanding the fundamental

00:13:12.730 --> 00:13:16.070
laws of nature. Okay, so the war ends in 1945.

00:13:16.710 --> 00:13:20.269
She accepts a position at Columbia. And in 1952,

00:13:20.309 --> 00:13:22.629
she becomes the first woman to get tenure in

00:13:22.629 --> 00:13:25.210
their physics department. Right. And she immediately

00:13:25.210 --> 00:13:27.269
starts working on these foundational experiments

00:13:27.269 --> 00:13:29.730
that show the same level of genius she brought

00:13:29.730 --> 00:13:32.220
to the xenon problem. For instance, her work

00:13:32.220 --> 00:13:34.740
on quantum entanglement. Yeah, this was in 1949.

00:13:34.779 --> 00:13:37.100
She was the first person to experimentally confirm

00:13:37.100 --> 00:13:40.080
the validity of quantum entanglement, that thing

00:13:40.080 --> 00:13:42.799
Einstein famously called spooky action at a distance.

00:13:43.039 --> 00:13:45.259
The idea that two particles can be linked no

00:13:45.259 --> 00:13:48.100
matter how far apart they are. Exactly. She observed

00:13:48.100 --> 00:13:50.919
the angular correlation of two photons, which

00:13:50.919 --> 00:13:53.299
proved the calculations of a couple of theorists.

00:13:53.340 --> 00:13:56.639
It was a really critical early confirmation of

00:13:56.639 --> 00:13:59.529
this bizarre quantum reality. But the work that

00:13:59.529 --> 00:14:01.789
really set the stage for her biggest breakthrough

00:14:01.789 --> 00:14:05.210
was her complete mastery of beta decay. Right.

00:14:05.330 --> 00:14:08.429
This goes back to Enrico Fermi's famous 1934

00:14:08.429 --> 00:14:12.009
theory that describes how beta decay works. A

00:14:12.009 --> 00:14:14.629
neutron turns into a proton, and it spits out

00:14:14.629 --> 00:14:17.250
an electron and a neutrino. But by the 1940s,

00:14:17.250 --> 00:14:19.230
there were problems. The experimental results

00:14:19.230 --> 00:14:22.049
just weren't quite matching the theory. There

00:14:22.049 --> 00:14:24.490
were these small, frustrating variances. Even

00:14:24.490 --> 00:14:26.429
a brilliant experimentalist like Luis Walter

00:14:26.429 --> 00:14:28.730
Alvarez was getting results that didn't quite

00:14:28.730 --> 00:14:31.169
line up. So Wu set out to figure out what was

00:14:31.169 --> 00:14:33.350
going on. And her conclusion was that the problem

00:14:33.350 --> 00:14:36.389
wasn't with Formy's theory. No. The problem was

00:14:36.389 --> 00:14:38.610
with the experiments themselves. She had this

00:14:38.610 --> 00:14:40.690
hunch that the issue was the way they were preparing

00:14:40.690 --> 00:14:42.750
the radioactive source material. People were

00:14:42.750 --> 00:14:45.149
using a thick, uneven film of something like

00:14:45.149 --> 00:14:47.669
copper sulfate. And why would that matter? Think

00:14:47.669 --> 00:14:50.289
of it like this. If the source is too thick,

00:14:50.730 --> 00:14:53.250
The electrons, the beta particles that are emitted,

00:14:53.470 --> 00:14:56.250
lose some of their energy just trying to escape

00:14:56.250 --> 00:14:58.990
the material itself before they even get to the

00:14:58.990 --> 00:15:02.090
detector. Ah, so that energy loss was distorting

00:15:02.090 --> 00:15:04.090
the measurements. Precisely. It was making the

00:15:04.090 --> 00:15:06.549
results look inconsistent with Fermi's beautiful,

00:15:06.850 --> 00:15:10.090
elegant theory. So what was her solution? This

00:15:10.090 --> 00:15:12.990
seems like a purely practical, experimental genius

00:15:12.990 --> 00:15:15.889
kind of problem. It was. She first took an old

00:15:15.889 --> 00:15:18.919
solenoidal spectrometer. a device that uses a

00:15:18.919 --> 00:15:21.019
magnetic field to measure the energy of electrons,

00:15:21.320 --> 00:15:23.500
and she modified it to be much more precise.

00:15:23.919 --> 00:15:26.519
Then she developed a new method using detergent

00:15:26.519 --> 00:15:29.179
to create an incredibly thin, perfectly even

00:15:29.179 --> 00:15:31.700
film of the radioactive source. So no more energy

00:15:31.700 --> 00:15:34.440
loss. Almost zero. And when she ran the experiment

00:15:34.440 --> 00:15:36.539
with her new, pristine setup... The results were

00:15:36.539 --> 00:15:39.440
perfect. Perfectly consistent with Fermi's model.

00:15:39.720 --> 00:15:42.860
She proved, definitively, that all those other

00:15:42.860 --> 00:15:45.500
discrepancies were just due to experimental error.

00:15:46.320 --> 00:15:49.179
By fixing the apparatus, she validated Fermi's

00:15:49.179 --> 00:15:51.740
physics, and in the process, she established

00:15:51.740 --> 00:15:54.559
herself as the world's leading authority on beta

00:15:54.559 --> 00:15:57.919
decay. And that mastery was the absolute prerequisite

00:15:57.919 --> 00:15:59.940
for the experiment that was about to change everything.

00:16:00.279 --> 00:16:03.080
This complete mastery of the beta decay really

00:16:03.080 --> 00:16:05.240
does set the stage perfectly for the experiment

00:16:05.240 --> 00:16:08.000
that defines her legacy, shattering the law of

00:16:08.000 --> 00:16:10.620
parity conservation. We're now in the mid -1950s.

00:16:10.639 --> 00:16:12.889
That's right. And two of her colleagues at Columbia,

00:16:13.090 --> 00:16:15.669
the theoretical physicists Sung Dao Lee and Tianning

00:16:15.669 --> 00:16:17.490
Yang, they were wrestling with something called

00:16:17.490 --> 00:16:20.029
the Veda Tau puzzle. OK, before we dive into

00:16:20.029 --> 00:16:21.889
the puzzle, let's make sure we're all clear on

00:16:21.889 --> 00:16:24.389
what parity even is. What did physicists mean

00:16:24.389 --> 00:16:27.169
by conservation of parity and why was it considered

00:16:27.169 --> 00:16:30.169
such a core, unshakable law? Think of that like

00:16:30.169 --> 00:16:32.809
a mirror. Parity conservation means that the

00:16:32.809 --> 00:16:35.370
laws of physics are the same for an event as

00:16:35.370 --> 00:16:38.370
they are for its mirror image. The universe fundamentally

00:16:38.370 --> 00:16:40.899
doesn't distinguish between left and right. So

00:16:40.899 --> 00:16:43.000
if I watch a video of a baseball game and then

00:16:43.000 --> 00:16:45.580
I watch a mirror image of that video, all the

00:16:45.580 --> 00:16:48.200
physics, the way the ball flies, the way the

00:16:48.200 --> 00:16:51.139
bat hits it, all of that should still work. Exactly.

00:16:51.259 --> 00:16:53.919
Physics was assumed to be spatially symmetrical.

00:16:54.639 --> 00:16:57.679
And this wasn't just a minor idea. It was considered

00:16:57.679 --> 00:17:00.360
a fundamental principle that applied to all four

00:17:00.360 --> 00:17:04.099
forces of nature. Gravity, electromagnetism,

00:17:04.240 --> 00:17:06.960
the strong force, and the weak force. It was

00:17:06.960 --> 00:17:09.319
an assumed truth. It was elegant. It was very

00:17:09.319 --> 00:17:11.839
elegant. But these two particles, the theta -misson

00:17:11.839 --> 00:17:14.480
and the tau -misson, were causing a huge problem

00:17:14.480 --> 00:17:16.720
for this elegant idea. The theta -tau puzzle.

00:17:17.019 --> 00:17:19.039
Right. These two particles seemed completely

00:17:19.039 --> 00:17:21.500
identical. They had the same mass, the same lifetime,

00:17:21.640 --> 00:17:25.079
the same charge. But they decayed into completely

00:17:25.079 --> 00:17:27.720
different final states. and those final states

00:17:27.720 --> 00:17:29.779
had different parodies. Okay, that is a puzzle.

00:17:29.920 --> 00:17:32.220
It's like having two identical billiard balls,

00:17:32.460 --> 00:17:34.319
but when you hit them in exactly the same way,

00:17:34.359 --> 00:17:36.119
one shatters and the other one just rolls away.

00:17:36.420 --> 00:17:38.900
That's a great analogy. If parity was conserved,

00:17:39.059 --> 00:17:41.559
as everyone believed, then these had to be two

00:17:41.559 --> 00:17:43.019
different particles. They just happened to look

00:17:43.019 --> 00:17:45.960
identical. But if they were, in fact, the same

00:17:45.960 --> 00:17:49.099
particle, then parity had to be violated. So

00:17:49.099 --> 00:17:53.140
Li and Yang had this radical idea. What if, just

00:17:53.140 --> 00:17:55.890
for the weak interaction, the force governing

00:17:55.890 --> 00:17:59.809
this strange decay, what if parity isn't conserved

00:17:59.809 --> 00:18:02.349
at all? That was their theory, but it was scientific

00:18:02.349 --> 00:18:04.609
heresy. They designed a kind of pencil and paper

00:18:04.609 --> 00:18:07.049
experiment to test it, but they were terrified.

00:18:07.369 --> 00:18:09.710
If the experiment failed, their careers would

00:18:09.710 --> 00:18:11.750
be ruined. So they needed someone to perform

00:18:11.750 --> 00:18:13.890
the experiment whose results would be absolutely

00:18:13.890 --> 00:18:16.410
beyond question. And there was only one person

00:18:16.410 --> 00:18:18.009
in the world with that reputation for that kind

00:18:18.009 --> 00:18:21.569
of work, Dr. Wu. The master of beta decay. Exactly.

00:18:21.950 --> 00:18:24.660
They went to her. and she immediately saw the

00:18:24.660 --> 00:18:27.460
importance of the question. She chose to test

00:18:27.460 --> 00:18:30.619
their theory using radioactive cobalt -60, which

00:18:30.619 --> 00:18:32.740
is a beta particle emitter. It was her specialty.

00:18:33.259 --> 00:18:36.440
But the experiment itself, it was almost impossible

00:18:36.440 --> 00:18:39.319
with the technology of the 1950s. A logistical

00:18:39.319 --> 00:18:41.740
and technical nightmare, I've heard. A complete

00:18:41.740 --> 00:18:44.519
nightmare. She needed to achieve two extreme

00:18:44.519 --> 00:18:46.799
conditions at the same time, and she spent a

00:18:46.799 --> 00:18:49.079
whole year on this, putting all her other research

00:18:49.079 --> 00:18:51.240
on hold. Okay, let's break it down. Condition

00:18:51.240 --> 00:18:55.220
one. Cryogenics. She needed to get the Cobalt

00:18:55.220 --> 00:18:59.000
-60 sample incredibly cold. Why? She had to get

00:18:59.000 --> 00:19:01.740
the atoms to stop wiggling around? At normal

00:19:01.740 --> 00:19:03.779
temperatures, the nuclei in the cobalt are all

00:19:03.779 --> 00:19:06.220
spinning in random directions. If you're trying

00:19:06.220 --> 00:19:08.599
to measure a directional preference, all that

00:19:08.599 --> 00:19:11.079
randomness just averages out to zero. So you

00:19:11.079 --> 00:19:12.779
wouldn't see anything even if the effect was

00:19:12.779 --> 00:19:15.259
there. Correct. So she had to cool the sample

00:19:15.259 --> 00:19:17.819
down to just fractions of a degree above absolute

00:19:17.819 --> 00:19:22.400
zero, about 0 .003 Kelvin. She used these specialized

00:19:22.400 --> 00:19:25.160
liquid helium refrigerators to basically freeze

00:19:25.160 --> 00:19:27.960
the atoms in place. Once they were frozen, she

00:19:27.960 --> 00:19:30.450
could move on to condition two. Magnetic alignment.

00:19:30.730 --> 00:19:32.269
How did she get them all to spin in the same

00:19:32.269 --> 00:19:35.250
direction? She used a powerful, uniform magnetic

00:19:35.250 --> 00:19:37.970
field. She put the sample inside a solenoid magnet,

00:19:38.210 --> 00:19:40.490
which acted like a giant compass for the atomic

00:19:40.490 --> 00:19:43.170
nuclei, lining up all their spin axes in the

00:19:43.170 --> 00:19:44.809
same direction. And then the detectors were set

00:19:44.809 --> 00:19:47.170
up to measure... What? They were set up to count

00:19:47.170 --> 00:19:49.450
the beta particles that were emitted along the

00:19:49.450 --> 00:19:52.480
direction of the spin. And the particles... emitted

00:19:52.480 --> 00:19:55.440
against the direction of the spin. If the numbers

00:19:55.440 --> 00:19:58.240
were the same, symmetry holds. If the numbers

00:19:58.240 --> 00:20:01.160
were different, symmetry is broken. And she couldn't

00:20:01.160 --> 00:20:02.839
do this at Columbia. She had to go somewhere

00:20:02.839 --> 00:20:05.420
else. Right. She had to travel to the National

00:20:05.420 --> 00:20:08.299
Bureau of Standards in Maryland, which had the

00:20:08.299 --> 00:20:11.859
specialized cryogenic equipment she needed. This

00:20:11.859 --> 00:20:14.720
adds a layer of drama because she's now physically

00:20:14.720 --> 00:20:17.440
separated from Li and Yang during the most critical

00:20:17.440 --> 00:20:20.069
part of the experiment. So Li and Yang's prediction

00:20:20.069 --> 00:20:22.390
was that the emission would be asymmetrical.

00:20:22.769 --> 00:20:26.029
Yes. They predicted that more beta particles

00:20:26.029 --> 00:20:28.829
would be ejected in one direction, say, opposite

00:20:28.829 --> 00:20:31.069
to the nuclear spin, than in the other. And when

00:20:31.069 --> 00:20:33.109
she finally ran the experiment, what did the

00:20:33.109 --> 00:20:35.829
detector show? The result was immediate, and

00:20:35.829 --> 00:20:38.460
it was dramatic. The asymmetry was there beyond

00:20:38.460 --> 00:20:41.779
any possible statistical doubt. A far, far greater

00:20:41.779 --> 00:20:44.400
number of electrons were emitted in the direction

00:20:44.400 --> 00:20:46.660
opposite to the spin of the nucleus. Parity was

00:20:46.660 --> 00:20:49.640
violated. Parity was not conserved under the

00:20:49.640 --> 00:20:53.420
weak nuclear force. This beautiful, elegant principle

00:20:53.420 --> 00:20:57.359
that everyone had assumed was true was not. The

00:20:57.359 --> 00:20:59.559
universe at this fundamental level actually does

00:20:59.559 --> 00:21:02.059
have a preference. It prefers left over right.

00:21:02.240 --> 00:21:05.039
She called Lee immediately. She did. And he asked

00:21:05.039 --> 00:21:07.220
her, are you sure? Because the implications were

00:21:07.220 --> 00:21:09.660
just so massive. This wasn't just a small correction.

00:21:09.920 --> 00:21:12.500
This was shattering a core belief of physics.

00:21:12.759 --> 00:21:15.710
And the impact was huge. It meant the theta and

00:21:15.710 --> 00:21:18.009
tau mesons were, in fact, the same particle.

00:21:18.210 --> 00:21:21.250
Which we now call the kion, yes. And her results

00:21:21.250 --> 00:21:23.970
were so clean, so definitive, they were confirmed

00:21:23.970 --> 00:21:26.849
by other labs almost instantly and published

00:21:26.849 --> 00:21:29.230
right alongside Li and Yang's theoretical paper

00:21:29.230 --> 00:21:31.490
in the same issue of the journal. The physics

00:21:31.490 --> 00:21:34.349
community was just stunned. Completely stunned.

00:21:34.650 --> 00:21:36.650
Otto Frisch said that physicists at Princeton

00:21:36.650 --> 00:21:38.069
thought it was the most impactful experiment

00:21:38.069 --> 00:21:40.769
since the Michelson -Morley experiment. The experiment

00:21:40.769 --> 00:21:43.329
that inspired Einstein's theory of relativity.

00:21:43.569 --> 00:21:46.390
That's an incredible comparison. It is, because

00:21:46.390 --> 00:21:49.190
this discovery really did set the stage for all

00:21:49.190 --> 00:21:52.009
of modern particle physics. It showed that fundamental

00:21:52.009 --> 00:21:55.650
symmetries could be broken, and that idea is

00:21:55.650 --> 00:21:58.029
the absolute foundation of the Standard Model.

00:21:58.410 --> 00:22:00.089
OK, let's connect the dots here to something

00:22:00.089 --> 00:22:03.130
even bigger. You mentioned this discovery led

00:22:03.130 --> 00:22:05.109
to understanding something called CP violation

00:22:05.109 --> 00:22:07.869
and that this helps explain why the universe

00:22:07.869 --> 00:22:11.349
even exists. That's a huge leap. How do we get

00:22:11.349 --> 00:22:14.529
from wiggling cobalt atoms to the Big Bang? It

00:22:14.529 --> 00:22:16.950
is hugely, but it follows directly from Wu's

00:22:16.950 --> 00:22:19.789
result. You see, once physicists realized that

00:22:19.789 --> 00:22:22.460
parity. The P and CP could be violated. They

00:22:22.460 --> 00:22:24.539
started looking at other symmetries. They looked

00:22:24.539 --> 00:22:26.660
at the combined symmetry of charge conjugation,

00:22:26.759 --> 00:22:29.559
C, which is swapping a particle for its antiparticle,

00:22:29.660 --> 00:22:32.279
and parity P. So CT symmetry. Right. And the

00:22:32.279 --> 00:22:35.019
theory was, if CP symmetry was perfectly conserved,

00:22:35.160 --> 00:22:37.140
the Big Bang should have created equal amounts

00:22:37.140 --> 00:22:39.500
of matter and antimatter. And if that happened,

00:22:39.619 --> 00:22:41.579
they would have all met and annihilated each

00:22:41.579 --> 00:22:44.000
other, leaving a universe of just energy. No

00:22:44.000 --> 00:22:47.289
planets, no stars, no us. Precisely. The fact

00:22:47.289 --> 00:22:49.890
that we are here in a universe full of matter

00:22:49.890 --> 00:22:52.970
means that symmetry must have been broken. There

00:22:52.970 --> 00:22:55.309
must have been a tiny violation of CP symmetry

00:22:55.309 --> 00:22:57.430
in the early universe that allowed a little bit

00:22:57.430 --> 00:23:00.289
more matter to survive than antimatter. And the

00:23:00.289 --> 00:23:03.210
idea that a fundamental symmetry could be broken

00:23:03.210 --> 00:23:06.410
at all started with Wu's experiment. Her experiment

00:23:06.410 --> 00:23:09.289
opened that door. It quite literally provides

00:23:09.289 --> 00:23:11.789
the foundation for explaining why we have a universe

00:23:11.789 --> 00:23:14.089
of structure instead of just a void of light.

00:23:14.430 --> 00:23:16.150
Which brings us back to the great controversy.

00:23:16.569 --> 00:23:20.230
Li and Yang get the Nobel Prize in 1957 for the

00:23:20.230 --> 00:23:23.410
theory. Wu, who did the incredibly difficult

00:23:23.410 --> 00:23:27.210
experiment that proved it, gets nothing. It's

00:23:27.210 --> 00:23:29.539
just indefensible. As you said, Jack Steinberger

00:23:29.539 --> 00:23:31.619
called it the Nobel Committee's biggest mistake.

00:23:31.880 --> 00:23:34.779
Even Wolfgang Polly, who had famously wagered

00:23:34.779 --> 00:23:37.039
against parity violation, he was shaken by what

00:23:37.039 --> 00:23:39.259
he called the sudden death of parity, and he

00:23:39.259 --> 00:23:41.359
couldn't believe Wu was denied the prize. The

00:23:41.359 --> 00:23:43.740
decision was also made incredibly fast, wasn't

00:23:43.740 --> 00:23:46.500
it? The confirmation was in late 1956, and the

00:23:46.500 --> 00:23:48.799
prize was awarded less than a year later. It

00:23:48.799 --> 00:23:51.660
was very rushed. It's very likely the committee

00:23:51.660 --> 00:23:54.039
didn't fully appreciate the immense technical

00:23:54.039 --> 00:23:56.819
difficulty of what she had accomplished. But

00:23:56.819 --> 00:23:59.660
we know her peers did. We know now that she received

00:23:59.660 --> 00:24:03.099
20 different Nobel nominations between 1958 and

00:24:03.099 --> 00:24:06.079
1973. She did eventually get major international

00:24:06.079 --> 00:24:09.180
recognition, though. Yes. In 1978, she was awarded

00:24:09.180 --> 00:24:11.680
the very first Wolf Prize in physics, which is

00:24:11.680 --> 00:24:13.619
often seen as an award for people who deserved

00:24:13.619 --> 00:24:16.190
a Nobel but never got one. The parity experiment

00:24:16.190 --> 00:24:18.990
was her most famous, but her work was far from

00:24:18.990 --> 00:24:21.309
over. Not at all. In fact, shattering parity

00:24:21.309 --> 00:24:23.630
just opened up a whole new set of questions about

00:24:23.630 --> 00:24:26.029
the weak interaction. Which brings us to the

00:24:26.029 --> 00:24:29.069
conserved vector current, or CVC, hypothesis.

00:24:29.609 --> 00:24:32.130
That sounds a bit technical. What were Richard

00:24:32.130 --> 00:24:33.990
Feynman and Murray Gell -Mann trying to do with

00:24:33.990 --> 00:24:36.309
that? They were trying to build a universal framework.

00:24:36.950 --> 00:24:39.670
After parity was broken, everyone realized that

00:24:39.670 --> 00:24:41.990
Fermi's original theory of beta decay needed

00:24:41.990 --> 00:24:45.440
an upgrade. CDC was basically Feynman and Gell

00:24:45.440 --> 00:24:47.240
-Mann's attempt to show that the rules for beta

00:24:47.240 --> 00:24:50.279
decay weren't some random isolated thing. They

00:24:50.279 --> 00:24:53.140
followed a predictable, conserved pattern. Sort

00:24:53.140 --> 00:24:55.900
of like how electric charge is conserved. A universal

00:24:55.900 --> 00:24:58.200
law for the weak force. That's what they were

00:24:58.200 --> 00:25:00.440
after. And once again, to prove their theory,

00:25:00.640 --> 00:25:04.180
they needed an experimentalist with unparalleled

00:25:04.180 --> 00:25:07.839
precision. They needed Dr. Wu. Of course. There's

00:25:07.839 --> 00:25:10.220
a story that Gell -Mann went up to her and asked,

00:25:10.279 --> 00:25:13.180
sort of jokingly, how long did Yang and Li pursue

00:25:13.180 --> 00:25:17.059
you to follow up on their work? It was this universal

00:25:17.059 --> 00:25:19.299
acknowledgement that if you had a foundational

00:25:19.299 --> 00:25:22.019
theory about the weak force, you had to go to

00:25:22.019 --> 00:25:24.079
her to prove it. So she took on the challenge.

00:25:24.299 --> 00:25:26.299
She did. She worked with her team at Columbia,

00:25:26.460 --> 00:25:31.000
and in December of 1962, she confirmed the CVC

00:25:31.000 --> 00:25:34.200
hypothesis. This was another huge piece of the

00:25:34.200 --> 00:25:36.440
puzzle for the standard model. It provided a

00:25:36.440 --> 00:25:38.599
complete solid foundation for Fermi's theory

00:25:38.599 --> 00:25:41.259
and also supported the theory of the two -component

00:25:41.259 --> 00:25:43.539
neutrino, which her parity experiment had actually

00:25:43.539 --> 00:25:45.519
established in the first place. Feynman must

00:25:45.519 --> 00:25:48.359
have been thrilled. He was ecstatic. He called

00:25:48.359 --> 00:25:50.559
the confirmed CVC theory one of his greatest

00:25:50.559 --> 00:25:52.779
scientific achievements, which shows you how

00:25:52.779 --> 00:25:55.460
much he valued her experimental proof. And during

00:25:55.460 --> 00:25:57.359
all this, her work ethic was just legendary.

00:25:57.980 --> 00:26:00.500
It was. She was made a full professor in 1958

00:26:00.500 --> 00:26:04.299
and got an endowed chair in 1973. She worked

00:26:04.299 --> 00:26:06.859
from 8 in the morning until 7 or 8 at night most

00:26:06.859 --> 00:26:09.559
days. Her students called her the Dragon Lady.

00:26:09.819 --> 00:26:12.920
That sounds intimidating. She was definitely

00:26:12.920 --> 00:26:14.900
demanding. But you have to understand, in her

00:26:14.900 --> 00:26:17.819
field, one tiny flaw in preparing a radioactive

00:26:17.819 --> 00:26:21.000
source could completely invalidate months of

00:26:21.000 --> 00:26:23.940
work. She knew that better than anyone. But the

00:26:23.940 --> 00:26:25.980
sources also say she treated her students like

00:26:25.980 --> 00:26:27.900
family. She'd have lunch with them every day,

00:26:27.980 --> 00:26:30.319
talk through their problems, personal and professional.

00:26:30.599 --> 00:26:33.099
It was a balance of extreme rigor and genuine

00:26:33.099 --> 00:26:36.279
care. And her scientific curiosity went way beyond

00:26:36.279 --> 00:26:39.140
just particle physics. Oh, absolutely. She co

00:26:39.140 --> 00:26:41.220
-wrote the definitive textbook on beta decay

00:26:41.220 --> 00:26:43.539
in 1966, which is still a standard reference

00:26:43.539 --> 00:26:46.039
today. And she even ventured into biology. She

00:26:46.039 --> 00:26:48.059
did. She used a technique called must -power

00:26:48.059 --> 00:26:50.839
spectroscopy to study the molecular changes in

00:26:50.839 --> 00:26:53.240
hemoglobin that cause sickle cell disease. And

00:26:53.240 --> 00:26:54.799
she did these incredibly detailed experiments

00:26:54.799 --> 00:26:57.400
on a rare poropsis called double beta decay,

00:26:57.700 --> 00:27:00.079
working 2 ,000 feet underground in a salt mine

00:27:00.079 --> 00:27:03.099
to shield her detectors from cosmic rays. All

00:27:03.099 --> 00:27:05.160
this work kept her in the U .S., though, far

00:27:05.160 --> 00:27:08.200
from her family in China, which was going through

00:27:08.200 --> 00:27:11.140
immense turmoil. That's one of the tragic parts

00:27:11.140 --> 00:27:13.599
of her story. Because of travel restrictions,

00:27:13.960 --> 00:27:16.579
she couldn't go back to mainland China until

00:27:16.579 --> 00:27:20.220
1973 after Nixon's visit started to open things

00:27:20.220 --> 00:27:22.740
up. And it was a difficult return. Heartbreaking.

00:27:22.960 --> 00:27:25.019
She learned that her uncle and her brother had

00:27:25.019 --> 00:27:27.559
died during the Cultural Revolution and her parents'

00:27:27.680 --> 00:27:30.500
tombs had been destroyed. It's a measure of her

00:27:30.500 --> 00:27:34.039
global stature, though, that the premier, Zhou

00:27:34.039 --> 00:27:37.460
Enlai, personally apologized to her for the destruction.

00:27:37.740 --> 00:27:40.759
As her career went on, she became much more outspoken,

00:27:40.759 --> 00:27:43.059
not just about science, but about social issues.

00:27:43.359 --> 00:27:45.299
She really started to leverage her scientific

00:27:45.299 --> 00:27:48.539
authority for advocacy. She successfully protested

00:27:48.539 --> 00:27:50.440
for the human rights of journalists and academics

00:27:50.440 --> 00:27:53.079
imprisoned in Taiwan, using her international

00:27:53.079 --> 00:27:55.400
reputation to pressure the government. And she

00:27:55.400 --> 00:27:57.579
spoke out forcefully against gender discrimination.

00:27:57.980 --> 00:28:00.140
Her most famous quote on that came at an MIT

00:28:00.140 --> 00:28:03.019
symposium in 1964. She just asked the audience,

00:28:03.160 --> 00:28:06.519
I wonder whether the tiny atoms and nuclei or

00:28:06.519 --> 00:28:08.680
the mathematical symbols or the DNA molecules

00:28:08.680 --> 00:28:11.880
have any preference for either masculine or feminine

00:28:11.880 --> 00:28:14.099
treatment. I read that it got huge applause.

00:28:14.420 --> 00:28:16.799
It did. It just perfectly captured the absurdity

00:28:16.799 --> 00:28:18.940
of gender bias in a field that's supposed to

00:28:18.940 --> 00:28:21.599
be purely about merit and intellect. She also

00:28:21.599 --> 00:28:24.500
insisted on being called Professor Wu, not Professor

00:28:24.500 --> 00:28:27.440
Yuan, her husband's name. She was very particular

00:28:27.440 --> 00:28:30.019
about that professional respect. And in 1975,

00:28:30.319 --> 00:28:33.500
the chairman of her department at Columbia realized

00:28:33.500 --> 00:28:36.339
she was being paid less than her male colleagues

00:28:36.339 --> 00:28:38.740
of the same rank, and he immediately fixed it.

00:28:38.819 --> 00:28:40.900
Her advocacy even reached the White House. It

00:28:40.900 --> 00:28:43.990
did. 1975, she became the first female president

00:28:43.990 --> 00:28:46.390
of the American Physical Society. And in that

00:28:46.390 --> 00:28:48.630
role, she formally asked President Gerald Ford

00:28:48.630 --> 00:28:51.430
to create a permanent scientific advisory body

00:28:51.430 --> 00:28:54.849
for the president. And he did it. He did. Ford

00:28:54.849 --> 00:28:57.269
signed a law creating the Office of Science and

00:28:57.269 --> 00:29:01.250
Technology Policy, the OSTP, which institutionalized

00:29:01.250 --> 00:29:03.490
scientific advice at the highest level of government.

00:29:03.930 --> 00:29:06.410
That's a direct result of her leadership. She

00:29:06.410 --> 00:29:09.549
retired in 1981, but her influence didn't wane.

00:29:10.000 --> 00:29:12.960
Her name was synonymous with quality. The director

00:29:12.960 --> 00:29:15.559
general of CERN said that if Wu didn't experiment,

00:29:15.940 --> 00:29:18.119
everyone in physics just believed it must be

00:29:18.119 --> 00:29:21.779
correct. Her reputation was truth. Maurice Goldhaber

00:29:21.779 --> 00:29:23.859
had that great quote about her. Oh, it's the

00:29:23.859 --> 00:29:27.079
best. He quipped that people avoid doing experiments

00:29:27.079 --> 00:29:29.880
in beta decay simply because they know that Wu

00:29:29.880 --> 00:29:31.900
Qiancheng will do a better job than anybody.

00:29:32.400 --> 00:29:34.339
That's the ultimate sign of respect from your

00:29:34.339 --> 00:29:37.200
peers. The honors she received are just incredible.

00:29:37.500 --> 00:29:39.839
First woman to get an honorary doctorate from

00:29:39.839 --> 00:29:41.980
Princeton, the National Medal of Science, induction

00:29:41.980 --> 00:29:44.440
into the National Women's Hall of Fame. And in

00:29:44.440 --> 00:29:47.319
2020, Time magazine finally named her Woman of

00:29:47.319 --> 00:29:50.039
the Year for 1945. For her role in the Manhattan

00:29:50.039 --> 00:29:52.619
Project, a long overdue recognition. And in the

00:29:52.619 --> 00:29:55.319
end, her story came full circle. It did. Her

00:29:55.319 --> 00:29:57.980
ashes were interred at the Mingda School in China,

00:29:58.220 --> 00:30:01.039
the very school her father founded for girls,

00:30:01.160 --> 00:30:03.920
where her whole journey began. So after this

00:30:03.920 --> 00:30:06.200
deep dive, What does it all mean? What's the

00:30:06.200 --> 00:30:09.359
big takeaway from her life and work? I think

00:30:09.359 --> 00:30:11.380
the sources show us she wasn't just a scientist.

00:30:11.440 --> 00:30:15.259
She was this force of nature, a triple threat.

00:30:15.599 --> 00:30:18.619
How so? Well, first, she was a scientific genius

00:30:18.619 --> 00:30:20.880
who dragged physics from the comfortable, elegant

00:30:20.880 --> 00:30:23.960
world of perfect symmetry into the more complex,

00:30:24.079 --> 00:30:26.140
more interesting reality of the standard model.

00:30:26.460 --> 00:30:29.160
Second. She was a pioneer who literally rescued

00:30:29.160 --> 00:30:31.579
a critical part of the war effort. with knowledge

00:30:31.579 --> 00:30:35.200
from her unpublished PhD thesis. And third, she

00:30:35.200 --> 00:30:37.380
was a fearless advocate who used the authority

00:30:37.380 --> 00:30:39.700
she earned in the lab to fight for human rights

00:30:39.700 --> 00:30:42.799
and for gender equality. Her entire legacy is

00:30:42.799 --> 00:30:45.940
this blend of unwavering precision and deep moral

00:30:45.940 --> 00:30:48.000
conviction. She looked at something everyone

00:30:48.000 --> 00:30:50.720
just assumed was a fundamental truth, the conservation

00:30:50.720 --> 00:30:53.140
of parity, and she had the courage and the skill

00:30:53.140 --> 00:30:55.119
to prove that the universe was actually more

00:30:55.119 --> 00:30:57.900
complicated and, frankly, more interesting than

00:30:57.900 --> 00:31:00.029
we had ever imagined. Which leaves us with a

00:31:00.029 --> 00:31:02.470
final, really provocative thought for you to

00:31:02.470 --> 00:31:05.170
consider. The discovery of parity violation meant

00:31:05.170 --> 00:31:07.650
that on a fundamental level, the universe literally

00:31:07.650 --> 00:31:10.789
distinguishes between left and right. That tiny

00:31:10.789 --> 00:31:13.230
asymmetry, that small preference, is the reason

00:31:13.230 --> 00:31:16.509
we exist. So, if the most fundamental rules that

00:31:16.509 --> 00:31:18.549
govern the smallest particles can be broken,

00:31:18.750 --> 00:31:21.529
what does that imply about all the other rules

00:31:21.529 --> 00:31:24.009
and assumed symmetries that govern our own reality?

00:31:24.670 --> 00:31:27.109
What other impossible symmetries, in physics,

00:31:27.269 --> 00:31:29.190
in biology, maybe even in our social structures,

00:31:29.369 --> 00:31:32.089
are just waiting out there for another meticulous,

00:31:32.089 --> 00:31:34.250
dedicated, and courageous experimentalist like

00:31:34.250 --> 00:31:36.589
Jianxiong Wu to come along and shatter them?

00:31:36.970 --> 00:31:39.630
It's a compelling thought to mull over as we

00:31:39.630 --> 00:31:41.589
move through a universe that, it turns out, just

00:31:41.589 --> 00:31:42.730
might have a preferred hand.
