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Hello, everybody,

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and welcome to early
morning coffee at CERN.

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I'm Steven Goldfarb and we have a really
I would say mind boggling show

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for you today because we're going
to be talking about quantum mechanics.

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And that's a world that boggles I think everybody's mind.

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I think as Richard Feynman said, 
if it doesn't, then you don't get it.

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Right.

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So, so I have here with me, Giulia Negro
from the CMS experiment.

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Giulia, you work, for Purdue University.

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In beautiful Lafayette, Indiana.

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By the way,

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for my French friends, it doesn't mean
that the university has been lost.

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Okay.

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It is actually a beautiful place.

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Lafayette, Indiana.

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And also, with me,
to talk about quantum entanglement
of top quarks

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I have one of my colleagues from the
ATLAS Experiment, Yoav Afik.

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Yoav.

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And he is from

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as you can see from his cup,
the Enrico Fermi Institute,

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at the University of Chicago
in Chicago, Illinois.

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So actually, your institutes
are not far from each other,

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but you guys are both far
from your institutes

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We are both based here at CERN, actually.

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I beat you on that, though,
because I actually work

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for the University of Melbourne
in Australia.

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Okay, so this is a very typical thing,
here at CERN.

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So we're here actually
today we're going to be celebrating

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the International Day of Quantum Science and Technology

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as declared by the United Nations.

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UNESCO sponsors these special events.

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And we'll be talking

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about this really nice measurement
that you guys have made,

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about the quantum entanglement of two top quarks

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in the Large Hadron Collider,
both at ATLAS and at CMS.

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And I have to say, first of all, this is
a measurement that was not previewed.

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We have these these books
when we start these experiments.

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The yellow books, right?

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And I think they were not actually yellow
for the LHC.

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But back in the day they were yellow

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they would they would sort of list
all the different types of physics

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and things that we might discover, things
and measurements, we might make.

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And you guys went beyond that. Right.

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So we're going to talk about that.

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But first I'd like to
to get into quantum mechanics if we can.

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A little bit.

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Maybe you each have
an opinion, but usually when UNESCO

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does something like this, it's
because it's 100 years since something.

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So Giulia,

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What what do you what would you say
happened a hundred years ago

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That launched this?

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Okay.

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Well, 100 years ago,
there were a lot of, discoveries.

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There was, process.

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There were a lot of physicists,

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that had different ideas.

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Yeah.

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For example, Heisenberg
with his matrix mechanics,

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and Schrödinger
with the wave mechanics.

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So that was, what, 1925?

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Yes. It's the centennial this year,

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that's why it's considered the beginning, but,

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yeah, I think it's more of a process

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than a specific year of when this all started.
That makes a lot of sense.

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Yuav, you have an opinion on this?

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Yeah. I see it as a process.

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I think what Giulia mentioned is where let's say
the formalism

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has been designed
for quantum mechanics, but in fact,

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I think it started

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even earlier when Einstein
introduced the photoelectric effect.

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And so he didn't have the exact formalism

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of the quantum mechanics,
of course, as we know it today.

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But he was able to show that light
comes in quanta, which is exactly,

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you know, what is quantum mechanics
is all about - discrete quantities.

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And I think at the time,
I mean, he wasn't always a big fan, right?

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of quantum mechanics, he thought that
there was something strange

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about not being deterministic.

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- I think it was hard for him that
there are many concepts

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that weren't so let's say
intuitive in quantum mechanics.

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I mean, as you mentioned before, right?

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Feynman said, if you think you understand
quantum mechanics means you understood nothing.

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Nothing. Yeah.
And then we understand nothing.

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We're willing to say that as scientists.
It's one of the things you find out

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when you're a scientist, especially
at CERN, is how much you don't know

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Most of the universe
we don't know.

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But we've learned a lot, and we're making
a lot of progress, which is important.

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So our director, Chetna,

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always reminds me
that there's a guy named (Satyendra) Bose

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who was very important
in all of this as well.

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And I think it is interesting
because some of

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the concepts of quantum mechanics

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came about somewhat by mistake.

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I think, you know, you mentioned,

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the photoelectric effect E equals Hv.

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And so there were quanta in,
the energy,

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of a photon, which depends on its frequency.

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So you have to use these exact discreet

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quanta.

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There were also,

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even just before that, that
the equation came from Max Planck, hence

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the Planck constant.

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When he was trying to understand (black body) radiation.

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And he found that using that mathematics,
using

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this idea of these various frequencies,

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you got

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solutions to the problems
that they were looking at.

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So the at the time, they were trying
to measure the different discrete spectra

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of electrons

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orbiting around the proton.

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And, and that's kind of cool,
I think, because we're experimentalists.

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Yeah.

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You know, experiment led and

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they couldn't come up with a solution
using classical mechanics.

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And so we got to this really, really cool
world of quantum mechanics.

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Bose, he also made a mistake
which was in counting, in the classroom.

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And he was talking about
counting different states, we have two particles

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and they can be one spin up and one spin down.

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And you can try to count probabilities.

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And normally you say, okay,
you can have them both up and both down.

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Or there's two different ways
it can be up and down.

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And if you have something like electrons,
where that's the correct way to count

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because you can differentiate
between the two particles.

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But Bose those just said, okay, there's two up,

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two down, and then there's one with one up
and one down.

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So three possibilities.

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It turned out that worked for bosons
like photons.

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And then because they're called bosons right.

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Because of Bose.

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So it was a really good contribution.

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He realised it was a mistake,
but then then he started using it.

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He said, this works.

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And he tried to publish.

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And due to various biases

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around the world, maybe just the bias of
this we have never done before

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or could have been cultural knows,
it wasn't accepted.

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But then he sent it to Einstein.

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and he said it was good,
and it got accepted.

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So we always have to fight
our biases, both from past,

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what we thought was true.

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And we have to draft those.

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But also there's still cultural biases.

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We always get.

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Having a place
like CERN is a great place to battle that.

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Right?

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Because you know,

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when you get when you have lunch,
you know, who knows who will be sitting next to you.

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So, okay, so no one asks the question.

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Quantum mechanics.

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It's a weird world, right?

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It's not like the world that we live in.

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The macroscopic.

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Giulia, tell me:

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What is your favourite effect?

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But of course, it's the quantum entanglement.

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We are speaking about that today.

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And you have

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to have to explain this
because it's really difficult to comprehend.

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And and I suppose
because she said that, you Yoav?

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which one?
She took entanglement from me, 

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so I would 

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say Bell inequality

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or the violation of Bell inequality.


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And I can explain, shortly, what this all means.

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Yeah,
you should explain, because Bell is from CERN.

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So as we spoke before about Einstein.

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So, Einstein, not only Einstein, but


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he had a bit of a problem
with entanglement, right?

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So let me let me try
and explain the concept of entanglement.

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So entanglement tells you ... let's say
that you have two particles.

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You cannot describe them

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within quantum mechanics
independently from each other.

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What does it mean.

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Let's say that we have two particles,
two electrons, for example,

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in two parts of the universe.
These electrons,

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they have a property which is called
spin, which we can measure.

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So it turns out that if we measure,

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if they are coming

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from the same source
which we call as singlet,

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and we measure the spin
of one of the electrons

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on one side of the universe,
we would immediately know the outcome

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on the other one.

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Immediately? So not with time for it to go around the WWW?

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And this is mind blowing, right.

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And it can tell you, for example,
it implies that the information

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travels faster than the speed of light,
which contradicts,

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Einstein's theory of relativity.

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So this is why, in the 30's, Einstein

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together with, with Podolsky and Rosen
came up with the

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famous paper of the EPR paradox,
the Einstein, Podolsky and Rosen paradox,

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which basically claims that quantum
mechanics is an incomplete theory.

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We have a set of hidden variables
within the theory, which tells us

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before the measurement itself, the outcome
of the measurement of one electron and the other one.

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And we need more variables

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in order to describe this theory.

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Okay.

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Now, in the 60's came John Stewart Bell,

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and showed that if these theories exist,

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it means that they have to fulfil

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this, very famous Bell inequality.

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So you can actually exclude these theories

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with additional local hidden variables

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as claimed by Einstein, Podolsky and Rosen.

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by breaking the Bell inequality.


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So it so it's broken then.

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It has been measured to be violated

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many times already. Yes.

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And there was,

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there was a Nobel Prize recently
for that a couple of years ago, yes.

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If I remember somewhere
around here, 2022,

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the winners of the 2022 Nobel Prize
were Aspect, Clauser and Zeilinger

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Exactly, Aspect, Clauser and Zeilinger.

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Very good.

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Yes, exactly. For testing this concept.

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And that's important,
I think, Bell was at CERN actually.

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Yes he was.

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So we have we have some smart people here,

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On occasion, there are some smart people here.

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So as long as we're talking about

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quantum entanglement here,

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you guys both independently
did measurements of quantum entanglement.

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Of course.

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That's why we have different experiments, right?

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You know, and
CMS and Atlas are beautiful experiments.

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They both enormous.

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They both have a lot of people, 
like 5000 or 6000 people on CMS, right?

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5000 or 6000 on ATLAS.

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There's 3000 authors, I think

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Yeah, almost

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You know that
that means that I've written less.

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I've been on ATLAS with you.

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Even before you,

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Yeah, because I think, 
I've been around since 1998

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and I still haven't written
a total of one paper.

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Right.

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Because if you take and divide by 3000,
we have to write more papers, I think.

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So you've independently done this,
I think, the story,

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of how you came up with the idea
of looking

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for quantum entanglement,

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in the LHC, because just like I said,
this is never too far before.

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I think you have the story.
- We came up with the idea.

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So together with, Juan Ramón Muñoz de Nova

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when I was in my Ph.D.,
we were in the same institute.

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He's actually coming from the field
of condensed matter physics.

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So this already tells us something 
about the interdisciplinary nature of this idea.

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And we were friends.

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And we met for coffee breaks at the TECHNION
where I did my PhD.

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And we chatted.

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Also, sometimes about physics, of course.

258
00:12:39,400 --> 00:12:40,000
Yeah, yeah.

259
00:12:40,000 --> 00:12:42,400
Well, more than sometimes. Yeah.

260
00:12:42,400 --> 00:12:44,640
And then he asked me

261
00:12:44,640 --> 00:12:47,640
if I think that we can measure
entanglement at the LHC.

262
00:12:48,000 --> 00:12:51,320
I said, okay,
that's a very interesting question.

263
00:12:52,080 --> 00:12:53,440
And I started to,

264
00:12:54,840 --> 00:12:55,320
to do some

265
00:12:55,320 --> 00:12:58,320
research and to see the possibilities.

266
00:12:58,320 --> 00:13:01,000
Then I saw this,

267
00:13:01,000 --> 00:13:03,040
very unique particle,

268
00:13:03,040 --> 00:13:06,040
which is the top quark,
which I assume we will discuss about soon.

269
00:13:06,200 --> 00:13:06,960
Yeah.

270
00:13:06,960 --> 00:13:09,960
And this seemed to me
also by the previous measurements

272
00:13:10,160 --> 00:13:14,840
that I saw were done
using top quarks as the perfect system.

273
00:13:15,520 --> 00:13:17,840
to try and measure quantum entanglement at the LHC

274
00:13:17,840 --> 00:13:19,600
And that is what we did.

275
00:13:19,600 --> 00:13:20,920
Someone had thought about that idea

276
00:13:20,920 --> 00:13:23,440
that you could use the top quark.

277
00:13:23,440 --> 00:13:27,520
So we thought about it together,
you know, Juan and myself together.

278
00:13:27,520 --> 00:13:33,320
And this led to a paper published
about a year after we chatted about it.

279
00:13:33,720 --> 00:13:36,400
This was basically the baseline

280
00:13:36,400 --> 00:13:37,120
for both of the measurements.

281
00:13:37,120 --> 00:13:41,040
And you were a student at the time?
- Yes, I was a PhD student back then.

282
00:13:42,680 --> 00:13:44,320
That's actually our workforce.

283
00:13:45,280 --> 00:13:46,120
People don't realise that.

284
00:13:46,120 --> 00:13:51,280
But like more than a third of the authors
on our experiments are PhD students.

285
00:13:51,440 --> 00:13:54,960
and they're also the people you'll find on
shifts a lot.

286
00:13:54,960 --> 00:13:59,120
Postdocs are also okay,
The rest of us

287
00:13:59,120 --> 00:14:00,320
are kind of useless.

288
00:14:00,320 --> 00:14:03,240
but we have fun anyhow!

289
00:14:03,240 --> 00:14:05,520
So you asked about it.

290
00:14:05,520 --> 00:14:07,800
Maybe Giulia can explain a little bit more

291
00:14:07,800 --> 00:14:10,080
Why is the top quark

292
00:14:10,080 --> 00:14:12,520
something that we can look at

293
00:14:12,520 --> 00:14:14,080
in this case.

294
00:14:14,080 --> 00:14:16,840
So the top quark is very special
because,

295
00:14:16,840 --> 00:14:19,840
a difference
with respect to the other quarks is that

296
00:14:20,200 --> 00:14:23,200
it decays before it can hadronise.

297
00:14:23,760 --> 00:14:26,760
So the information, for example,
the spin information, of the

298
00:14:26,880 --> 00:14:29,880
the top quark is transferred,
to its decay products.

299
00:14:32,720 --> 00:14:35,240
Interesting that you bring up hadronise,
so quarks are very special.

300
00:14:35,240 --> 00:14:37,280
Yes, they are fundamental particles

301
00:14:37,280 --> 00:14:38,240
They're fundamental, 

302
00:14:38,240 --> 00:14:40,440
when we talk about

303
00:14:40,440 --> 00:14:42,080
doing particle physics at CERN,

304
00:14:42,080 --> 00:14:44,200
So we talked about looking
at the elementary

305
00:14:44,200 --> 00:14:47,880
or fundamental particles those things
you can't cut a top quark in half.

306
00:14:48,120 --> 00:14:49,280
Right.

307
00:14:49,280 --> 00:14:52,360
So we have 6 of these quarks.

308
00:14:52,880 --> 00:14:54,760
Two of them are stable
because they're really light.

309
00:14:57,080 --> 00:14:59,320
The up and the down.
The other ones, they appear for short times.

310
00:14:59,320 --> 00:15:02,440
And then I guess the the more massive
they are,

311
00:15:02,960 --> 00:15:06,360
the quicker they decay.
Indeed,


312
00:15:06,720 --> 00:15:10,560
the top quark is the one with the highest mass

313
00:15:10,560 --> 00:15:13,800
it is 40 times, larger than the bottom quark.

314
00:15:13,810 --> 00:15:17,560
It's about 180 times the mass of the proton.

316
00:15:18,400 --> 00:15:19,120
And a proton is made up

317
00:15:19,120 --> 00:15:20,760
of quarks.

318
00:15:20,760 --> 00:15:22,400
Right. So yeah.

319
00:15:22,400 --> 00:15:25,360
The top quark is super massive.

320
00:15:25,360 --> 00:15:28,480
It's the most massive of any of the,
any of the elementary particles.

321
00:15:28,480 --> 00:15:29,680
Even the bosons, like

322
00:15:29,680 --> 00:15:33,200
the W and the Z, even the Higgs
even more massive than the Higgs.

323
00:15:34,240 --> 00:15:36,360
So it doesn't have a chance

324
00:15:36,360 --> 00:15:39,360
like the other quarks
have this wonderful life because

325
00:15:39,840 --> 00:15:44,360
as soon as they're born, they find
a partner or a couple partners, right.

326
00:15:44,760 --> 00:15:46,280
And they hang out with them,

327
00:15:46,280 --> 00:15:49,720
and it takes a huge amount of effort
to pull them apart.

328
00:15:50,080 --> 00:15:52,200
It's the strong nuclear force.

329
00:15:53,480 --> 00:15:56,240
And when you do 
when you finally get these two

330
00:15:56,240 --> 00:16:00,680
quark and antiquark and you pull them apart, 
suddenly out of, out of nowhere

331
00:16:01,880 --> 00:16:04,600
out of the vacuum,
a couple other quarks appear.

333
00:16:05,640 --> 00:16:09,080
they can't get to, they get divorced and
they immediately got new partners.

334
00:16:09,680 --> 00:16:13,040
But the poor top quark is all alone.

335
00:16:13,480 --> 00:16:16,040
and it disintegrates, it transforms

336
00:16:16,040 --> 00:16:16,880
to other

337
00:16:16,880 --> 00:16:18,680
I don't like using decays,

338
00:16:18,680 --> 00:16:20,600
I agree, my wife tells me that more massive you get 

339
00:16:20,600 --> 00:16:22,360
the quicker you'll decay,

340
00:16:22,360 --> 00:16:24,720
And I agree that like,

341
00:16:24,720 --> 00:16:27,000
you know, I don't like this word
because when you think of decays,

342
00:16:27,000 --> 00:16:28,600
you think of the breaking into parts

343
00:16:28,600 --> 00:16:32,480
and the top quark doesn't break into parts,
it transforms into energy.

344
00:16:32,480 --> 00:16:33,880
Plus the

345
00:16:35,640 --> 00:16:36,720
W and the bottom quark

346
00:16:36,720 --> 00:16:37,400
Exactly.

347
00:16:37,400 --> 00:16:40,120
So you have these decay
products, you know,

348
00:16:40,120 --> 00:16:43,120
and then you can look at 

349
00:16:44,240 --> 00:16:47,000
their energy, their momentum, their angles

350
00:16:47,000 --> 00:16:49,400
and then you can

351
00:16:49,400 --> 00:16:51,160
figure things out from that?

352
00:16:51,160 --> 00:16:54,640
In our case for the entanglement,

353
00:16:54,680 --> 00:16:58,400
we measured that the angular correlation
between these decay products,

354
00:16:58,400 --> 00:17:01,840
So in this case with the leptons,
that decay from the top quark.

355
00:17:02,560 --> 00:17:03,120
Okay.

356
00:17:03,120 --> 00:17:05,960
So you have you have a couple leptons.

357
00:17:05,960 --> 00:17:08,960
It's complicated when they decay right?

358
00:17:08,960 --> 00:17:13,280
Top quarks have a few possibilities to decay,
we look specifically at,

359
00:17:13,280 --> 00:17:21,640
we need to say that the top quarks are created
in a pair of the top quark and its antimatter
counterpart, the antitop

360
00:17:21,640 --> 00:17:24,640
And between these two,
we actually measured the entanglement

360
00:17:25,040 --> 00:17:27,840
the spin entanglement
between the top of the antitop.

361
00:17:27,840 --> 00:17:28,440
Both of them can decay,

362
00:17:29,400 --> 00:17:30,880
so they can

363
00:17:30,880 --> 00:17:34,120
have a few possibilities
to decay.

364
00:17:34,560 --> 00:17:38,840
One of the possibilities to decay
to final states with charged leptons.

365
00:17:38,840 --> 00:17:41,840
So, for example, electron or positron

366
00:17:42,320 --> 00:17:47,360
or the heavier twin of the electron

367
00:17:48,520 --> 00:17:50,480
not exactly the twin,

368
00:17:50,480 --> 00:17:52,840
the muon or the antimuon

369
00:17:52,840 --> 00:17:53,800
why we do this?

370
00:17:53,800 --> 00:17:57,280
Because the in our detectors,
we measure

371
00:17:58,320 --> 00:18:01,880
the charged leptons in
very good precision.

372
00:18:02,440 --> 00:18:06,640
And we need to have the tracks
being measured very precisely.

373
00:18:07,000 --> 00:18:08,560
Because, as Giulia said before,

374
00:18:08,560 --> 00:18:12,040
in the end, we need to measure
the angular separations between one
charged lepton from one top,

375
00:18:12,040 --> 00:18:15,840
to the other charged lepton
from the antitop.

376
00:18:16,360 --> 00:18:18,920
And this way we can deduce something
about their spin correlations

377
00:18:18,920 --> 00:18:21,920
and about the entanglement
between the top and anti top.

378
00:18:22,160 --> 00:18:24,520
So it tells you
that they are correlated. Yes.

379
00:18:25,960 --> 00:18:26,840
That's interesting.

380
00:18:26,840 --> 00:18:29,840
And you came up with this over coffee,

381
00:18:31,200 --> 00:18:34,200
during a conference in, more or less.

382
00:18:34,920 --> 00:18:40,560
Yeah, a regular coffee break in the office.

383
00:18:41,000 --> 00:18:42,880
Oh, yeah. Okay.

384
00:18:42,880 --> 00:18:44,720
Coffee is very important, by the way.

385
00:18:47,240 --> 00:18:49,240
So Chetna wants to know.

387
00:18:50,560 --> 00:18:51,920
What exactly does it mean?

388
00:18:51,920 --> 00:18:54,880
So under certain circumstances,

389
00:18:54,880 --> 00:18:57,880
they're entangled
you measure that they are entangled

390
00:18:58,360 --> 00:19:03,000
So how are they entangled,
what is the meaning behind this?

391
00:19:03,080 --> 00:19:05,120
So, as Yoav said before, that

392
00:19:05,120 --> 00:19:12,440
means that you cannot describe,
the spin state of one quark independently
from the other

393
00:19:12,480 --> 00:19:13,800
in quantum mechanics,

394
00:19:13,800 --> 00:19:17,160
we use, just for example,
the wave function

395
00:19:17,160 --> 00:19:20,640
to describe the state of a given particle
or a given system.

396
00:19:21,440 --> 00:19:24,960
we can also use what,
what is called the density matrix,

397
00:19:24,960 --> 00:19:27,960
which gives us the density
to be in some specific states.

398
00:19:30,480 --> 00:19:34,560
And the idea behind entanglement
is that if

399
00:19:34,560 --> 00:19:37,960
we have this density matrix which describes
the quantum state of the system,

400
00:19:38,120 --> 00:19:41,120
and we have defined this for 
the top and the antitop.

401
00:19:41,520 --> 00:19:43,680
for the system of the two,

402
00:19:43,680 --> 00:19:46,680
we cannot describe this
just by a combination

403
00:19:46,880 --> 00:19:51,000
of the individual spin density
matrix of each one of the top 

404
00:19:51,520 --> 00:19:52,680
or the antitop.

405
00:19:52,680 --> 00:19:55,200
This tells us
that the state is not separable.

406
00:19:55,200 --> 00:20:00,720
We cannot describe the state of the top and antitop
independently from the other.

407
00:20:02,440 --> 00:20:05,440
You know, if you're listening

408
00:20:06,480 --> 00:20:09,600
and you don't completely get this
it's normal, right?

409
00:20:09,600 --> 00:20:11,880
This is a world that we don't live in.

410
00:20:11,880 --> 00:20:15,120
It's like the electrons
that were mentioned before, right?

411
00:20:15,120 --> 00:20:18,800
Because we know the outcome
of the measurement of

412
00:20:18,800 --> 00:20:21,800
one electron

413
00:20:22,960 --> 00:20:25,400
after we did the measurement
on the other one, it tells us

414
00:20:25,400 --> 00:20:29,120
that basically we cannot describe
the quantum state

415
00:20:29,120 --> 00:20:33,480
of both of the electrons, sorry,
as an independent combination

416
00:20:33,480 --> 00:20:34,880
of the states of both of them,

417
00:20:34,880 --> 00:20:38,560
just because the correlations look so
strong, there's so much affect each other.

418
00:20:39,000 --> 00:20:42,000
And so you have to describe
the system as a whole.

419
00:20:43,800 --> 00:20:44,600
So I understand this

420
00:20:44,600 --> 00:20:48,360
was not simple to do, there were
some hallenges in doing the analysis.

421
00:20:53,640 --> 00:20:55,320
Where to start?

422
00:20:55,320 --> 00:20:58,160
Well, one challenge is that we had to deal

423
00:20:58,160 --> 00:21:00,960
with the modelling of the t-tbar 

424
00:21:00,960 --> 00:21:03,040
production threshold region

425
00:21:03,040 --> 00:21:06,040
So, close to

426
00:21:06,240 --> 00:21:09,040
two times the mass of the top quark

427
00:21:09,040 --> 00:21:09,480
And

428
00:21:09,480 --> 00:21:12,480
this region is not very well modelled yet,

429
00:21:12,880 --> 00:21:15,200
So we had to come up with a

430
00:21:15,200 --> 00:21:18,200
simplified model, and then we introduced this

431
00:21:19,120 --> 00:21:23,040
pseudoscalar resonance,
that is a bound state of a top quark
and a top antiquark,

432
00:21:25,800 --> 00:21:28,200
So this is called toponium.

433
00:21:28,200 --> 00:21:30,040
and then this improves

434
00:21:30,040 --> 00:21:33,040
our modelling of this region.

435
00:21:33,560 --> 00:21:36,560
Including this was not an easy process

436
00:21:37,240 --> 00:21:39,360
and, in our measurements

437
00:21:39,360 --> 00:21:40,800
we managed to do it.

438
00:21:40,800 --> 00:21:45,720
So in ATLAS they came out first
but they didn't include this in the model.

439
00:21:45,760 --> 00:21:50,320
Yeah,
we were able to show that our measurement

440
00:21:51,360 --> 00:21:54,360
is not affected by this effect.

441
00:21:54,640 --> 00:21:57,640
But nevertheless,
this is actually a super interesting point

442
00:21:57,640 --> 00:21:59,920
because this is a very cool effect.

443
00:21:59,920 --> 00:22:02,920
The idea behind this is that

444
00:22:03,040 --> 00:22:07,000
close to the production threshold
where the top and anti-top are slow,

445
00:22:07,840 --> 00:22:10,840
there are some non-relativistic effects that enters

446
00:22:11,680 --> 00:22:14,320
this is the so-called toponium.

447
00:22:14,320 --> 00:22:17,480
It's funny,
this is not included by default

448
00:22:18,040 --> 00:22:20,320
in our Monte Carlo simulations.

449
00:22:20,320 --> 00:22:23,600
It's a non-perturbative effect.

450
00:22:24,640 --> 00:22:27,640
Actually, the tools we used and that were used in CMS,

451
00:22:30,440 --> 00:22:33,800
let's say give a better and better

452
00:22:33,800 --> 00:22:37,120
grasp of this specific effect

453
00:22:37,640 --> 00:22:40,640
and perhaps also the possibility to measure it

454
00:22:41,120 --> 00:22:44,120
and to develop some observables
which are more sensitive to this state

455
00:22:44,680 --> 00:22:48,040
because this state brings an enhancement

456
00:22:48,040 --> 00:22:51,840
of the more entangled events
to a cross section.

457
00:22:51,840 --> 00:22:54,280
So it basically means
that we should see more entangled events than

458
00:22:54,280 --> 00:22:58,360
than expected
from Monte Carlo simulations that we use.

459
00:23:00,640 --> 00:23:02,000
So you mentioned a few things in there.

460
00:23:02,000 --> 00:23:05,000
I'm not sure if
we're going to go into details, but now,

461
00:23:05,600 --> 00:23:09,800
QCD is very complicated.

462
00:23:10,120 --> 00:23:13,120
So you you have these different realms,
right?

463
00:23:13,520 --> 00:23:16,600
the perturbative and the non perturbative,
which has to do

464
00:23:16,600 --> 00:23:19,160
with relativity effects? Yes.

465
00:23:22,320 --> 00:23:29,480
The nice thing is that actually these measurement
of entanglement, beyond being

466
00:23:30,400 --> 00:23:32,680
these measurements of entanglement, beyond

467
00:23:32,680 --> 00:23:35,680
being just, you know, being a very nice

468
00:23:36,880 --> 00:23:39,360
and cool interdisciplinary thing to measure,
they actually brought a lot of benefits

469
00:23:39,360 --> 00:23:42,360
to high-energy physics, 
to measure processes of high-energy physics.


471
00:23:43,000 --> 00:23:46,360
So, so tell me a little bit more about this.
What are the benefits that come from this.

472
00:23:47,360 --> 00:23:48,680
So besides the

473
00:23:48,680 --> 00:23:51,680
possibility to have a better grasp of toponym,

474
00:23:52,640 --> 00:23:54,520
mentioned before by Giulia,

475
00:23:54,520 --> 00:23:57,520
So for example,
if you look at the measurement by CMS,

476
00:23:57,600 --> 00:24:01,680
you can see that the data agrees better
with the existence of this toponium.

477
00:24:02,320 --> 00:24:05,840
Which is quite nice, because if we look at our

478
00:24:06,800 --> 00:24:11,080
resolution in the detector
to reconstruct the invariant mass

479
00:24:11,520 --> 00:24:13,680
of the top and the anti top,

480
00:24:13,680 --> 00:24:15,680
We can never see this because it's

481
00:24:15,680 --> 00:24:18,880
a lot more narrow than our t-tbar resolution.

482
00:24:18,880 --> 00:24:21,880
But with the spin correlation effects and
entanglement observables,

483
00:24:22,880 --> 00:24:25,880
it's possible to see some signs of this,

484
00:24:25,900 --> 00:24:31,920
It also gave a push to theorists,
to investigate a bit more.

485
00:24:31,920 --> 00:24:35,000
And this also came up in a few
other measurements

486
00:24:35,640 --> 00:24:38,640
by CMS, these effects,

487
00:24:40,440 --> 00:24:43,320
In addition, I have to say that

488
00:24:43,320 --> 00:24:47,760
there are many new techniques to search for physics

489
00:24:47,760 --> 00:24:51,480
beyond the Standard Model that has been developed
based on the quantum observables

490
00:24:52,000 --> 00:24:56,280
that we thought about and
that we looked at in our measurements.

491
00:24:57,520 --> 00:24:58,840
Physics beyond the Standard Model

492
00:24:58,840 --> 00:25:03,040
is something we all want because
this is what makes our careers here

493
00:25:04,000 --> 00:25:06,840
as experimentalists is forever

494
00:25:06,840 --> 00:25:09,840
trying to find out
what's wrong with theory.

495
00:25:10,640 --> 00:25:12,480
We love theorists. We love theorists.

496
00:25:12,480 --> 00:25:16,360
But they only explain
5% of the universe.

497
00:25:16,520 --> 00:25:19,160
Or less, we don't even know gravity.

498
00:25:19,160 --> 00:25:22,480
Okay, so there are a lot of things,
a lot of big questions out there.

499
00:25:22,800 --> 00:25:26,120
And so we're always looking to see
where the model can break.

500
00:25:26,760 --> 00:25:27,840
And that gives us hints.

501
00:25:27,840 --> 00:25:30,840
And so to see this
it gives us some more tools.

502
00:25:31,480 --> 00:25:36,200
I should mention
toponium is only one of the oniums right?

503
00:25:36,400 --> 00:25:38,600
There are others that have been measured

504
00:25:38,600 --> 00:25:41,720
bottomonium, charmonium,

505
00:25:42,040 --> 00:25:44,960
meaning that you have a charm quark and an anti charm,

506
00:25:44,960 --> 00:25:50,200
bottom, or anti bottom,
but these we can measure more directly.

507
00:25:51,360 --> 00:25:52,320
Yes, but

508
00:25:52,320 --> 00:25:55,720
with the top it's not so easy.

509
00:25:55,720 --> 00:25:57,320
Also,

510
00:25:57,320 --> 00:26:01,000
it's not exactly the same thing
because the tops really decay before

511
00:26:01,000 --> 00:26:04,600
they can form like a particle
a bound state, a meson,

512
00:26:04,840 --> 00:26:08,360
So maybe toponium is a bit
of a misleading name.

513
00:26:08,480 --> 00:26:10,040
So they haven't really formed,

514
00:26:10,040 --> 00:26:13,040
They exchange a few gluons
before they decay.

515
00:26:13,880 --> 00:26:17,360
Gluons being the carriers
of the strong nuclear force,

516
00:26:18,160 --> 00:26:21,160
like photons,
we have photons coming through us right now.

517
00:26:21,920 --> 00:26:24,920
That's what's inside these protons.

518
00:26:25,960 --> 00:26:27,200
The gluons, great name.

519
00:26:27,200 --> 00:26:29,440
Keeps it all glued.

520
00:26:29,440 --> 00:26:32,360
So my next question for you is,
what's next?

521
00:26:32,360 --> 00:26:35,600
I mean, if you you guys learn off
from each other, this is very common

522
00:26:36,360 --> 00:26:41,440
for experiments. We go to conferences
or we have discussions or seminars.

523
00:26:41,440 --> 00:26:44,080
That's when we share information.

524
00:26:45,560 --> 00:26:47,160
Of course, you know,

525
00:26:47,160 --> 00:26:50,160
some information gets shared during coffee breaks,

526
00:26:50,960 --> 00:26:53,560
As we've learned,

527
00:26:53,560 --> 00:26:54,960
But now, I mean,

528
00:26:54,960 --> 00:26:58,000
will ATLAS, for example,
do a measurement with toponium

529
00:26:59,200 --> 00:27:02,200
included, or,

530
00:27:02,480 --> 00:27:05,480
you found that it's an effect that doesn't
we don't know.

531
00:27:05,640 --> 00:27:06,960
Can't say.

532
00:27:06,960 --> 00:27:07,720
Oh, yeah.

533
00:27:07,720 --> 00:27:10,720
We can't always say these things.

534
00:27:14,600 --> 00:27:18,600
In general, how do you see us going forward with
these measurements?

535
00:27:19,560 --> 00:27:22,560
Well there is not only quantum entanglement
that we can measure,

536
00:27:22,800 --> 00:27:26,320
there are also lots of other quantum correlations,
537
00:27:26,640 --> 00:27:30,480
like Bell's inequality, as we mentioned before.

538
00:27:30,920 --> 00:27:33,480
So for sure, one of the next

539
00:27:33,480 --> 00:27:35,120
point will be to also discover

540
00:27:36,840 --> 00:27:38,560
these new quantum effects.

541
00:27:38,560 --> 00:27:40,840
I want to give maybe a number.

542
00:27:40,840 --> 00:27:41,920
Just to give you an idea.

543
00:27:41,920 --> 00:27:43,920
Why is it interesting to do these measurements

544
00:27:43,920 --> 00:27:47,080
So we mentioned before the Nobel Prize
in physics.

545
00:27:47,520 --> 00:27:48,120
Right.

546
00:27:48,120 --> 00:27:51,120
And it was done by testing

547
00:27:51,960 --> 00:27:54,200
the entanglement and the Bell inequality with photons.

548
00:27:54,200 --> 00:27:56,640
What we do here at the LHC,
the measurement

549
00:27:56,640 --> 00:27:57,720
that both CMS and ATLAS did

550
00:27:57,720 --> 00:28:02,840
with top quarks, is about
12 orders of magnitude higher in energy than

551
00:28:03,000 --> 00:28:07,120
all of these extremely important
laboratory experiments.

552
00:28:07,840 --> 00:28:10,360
So when you go so much
higher in the scale,

553
00:28:10,360 --> 00:28:13,880
there is already
a fundamental interest of why we do this.

554
00:28:14,520 --> 00:28:17,400
And what CMS and ATLAS did,

555
00:28:17,400 --> 00:28:19,920
at least to me, is a proof of concept

556
00:28:19,920 --> 00:28:24,560
that we can actually perform
such measurements using collider physics,

557
00:28:25,240 --> 00:28:28,000
using collider experiments,

558
00:28:28,000 --> 00:28:30,800
and there is so much room for doing more.
So many other proposals,

559
00:28:30,800 --> 00:28:31,920
to measure many other things.

560
00:28:33,480 --> 00:28:36,040
A lot has come up

561
00:28:36,040 --> 00:28:36,640
since then.

562
00:28:36,640 --> 00:28:40,080
And we think we can say
both in CMS and ATLAS we are 

563
00:28:40,720 --> 00:28:45,400
now working on performing these other measurements
in some other parts of phase space with top quarks, 

564
00:28:45,440 --> 00:28:49,040
or, for example, with the Higgs boson decay.

565
00:28:49,640 --> 00:28:53,320
And so there is a lot to do.

566
00:28:53,720 --> 00:28:56,640
This is the first time this is being done
in collider research.

567
00:28:56,640 --> 00:28:59,840
It was the measurement with the highest
energy ever performed.

568
00:29:00,840 --> 00:29:03,160
At the LHC it was the first time.

569
00:29:03,160 --> 00:29:06,160
It was done before

570
00:29:06,200 --> 00:29:09,480
in colliders with mesons

571
00:29:10,320 --> 00:29:14,440
at lower energies, 
in particular with B mesons,

572
00:29:15,240 --> 00:29:19,400
but it's a different type of entanglement.

573
00:29:20,080 --> 00:29:25,320
It's more flavour entanglement
it's related to other properties of particles.

574
00:29:26,040 --> 00:29:28,440
But never at the LHC,

575
00:29:28,440 --> 00:29:30,880
never with quarks

576
00:29:30,880 --> 00:29:33,240
which are fundamental particles,

577
00:29:33,240 --> 00:29:37,520
It's pure quantum entanglement
because it's a fundamental particle

578
00:29:38,680 --> 00:29:41,360
Remember the example that I gave with

579
00:29:41,360 --> 00:29:44,360
both of the electrons at other parts of the Universe.

580
00:29:44,480 --> 00:29:47,240
Yeah. This was never done actually.

582
00:29:48,040 --> 00:29:48,200
Yeah.

583
00:29:48,200 --> 00:29:50,840
That would take some effort to go 
to different parts of the universe.

584
00:29:50,840 --> 00:29:51,760
Well yes.

585
00:29:51,760 --> 00:29:54,760
But in general between two what
we call free electrons.

586
00:29:54,880 --> 00:29:55,440
Yeah.

587
00:29:55,440 --> 00:29:58,680
I mean it was done with a bit
more complicated systems.

588
00:29:58,680 --> 00:30:04,440
Here, we actually measured the entanglement
between two quarks which are 

589
00:30:04,440 --> 00:30:07,440
let's say quasi-free particles.

590
00:30:09,480 --> 00:30:11,400
So, you have theorists

591
00:30:11,400 --> 00:30:15,280
coming to you, saying,
I got some ideas now, right?

592
00:30:15,280 --> 00:30:18,280
I guess you have both been approached by theorists

593
00:30:18,280 --> 00:30:20,760
and different things in quantum mechanics that
can be measured.

594
00:30:20,760 --> 00:30:25,160
Also though, what we have coming up in a few years,

595
00:30:26,040 --> 00:30:28,640
we're going to tear our experiments apart

596
00:30:28,640 --> 00:30:31,560
and we're going to go
to a High-Luminosity LHC.

597
00:30:31,560 --> 00:30:34,080
So actually, we have,
a year and a half or so

598
00:30:34,080 --> 00:30:37,840
of running
and then nothing for 3 and a half to 4 years.

599
00:30:37,840 --> 00:30:41,520
And then we start up with brand new
beautiful detectors

600
00:30:42,360 --> 00:30:45,360
made to be able to go at a much higher rate,
so we'll have much higher statistics,

601
00:30:46,200 --> 00:30:46,800
will that help?

602
00:30:47,320 --> 00:30:48,880
Will that be of use to you?

603
00:30:48,880 --> 00:30:52,360
We will have more data so 
we can get measurements more precisely.

604
00:30:53,760 --> 00:30:57,800
So, for example,
I mean, as was mentioned before by Giulia,

605
00:30:57,800 --> 00:31:02,440
we have a lot more concepts of
quantum correlations that we can measure.

606
00:31:02,920 --> 00:31:06,280
If you look, for example at Bell state,
or Bell inequality,

607
00:31:07,680 --> 00:31:09,680
if we look at the measurement,

608
00:31:09,680 --> 00:31:12,960
in t-tbar,
we have to go to a lot more extreme

609
00:31:12,960 --> 00:31:16,200
parts of phase space,
to perform these measurements.

610
00:31:16,680 --> 00:31:19,680
And if we have more data
in order to do it,

611
00:31:20,000 --> 00:31:24,240
it means that we have more events
and more statistics to actually be able to

612
00:31:25,280 --> 00:31:27,640
do these measurements because,

613
00:31:27,640 --> 00:31:30,280
of course,
we need statistics to make

614
00:31:30,280 --> 00:31:34,200
precise measurements
So extreme parts of phase space.

615
00:31:34,200 --> 00:31:35,400
Sounds like a great place to go.

616
00:31:36,760 --> 00:31:37,080
But it is

617
00:31:37,080 --> 00:31:40,080
sort of those things 
which are rare.

618
00:31:40,160 --> 00:31:43,480
It's rare to find something 
that has this momentum,

619
00:31:43,480 --> 00:31:44,320
this energy,

620
00:31:44,320 --> 00:31:47,320
this mass, whatever.

621
00:31:47,400 --> 00:31:48,840
Those are what we consider phase space.

622
00:31:48,840 --> 00:31:51,560
And yeah, with more statistics.

623
00:31:51,560 --> 00:31:54,320
Even if we're not going to increase energy,
because the LHC won't increase 

624
00:31:54,320 --> 00:31:55,800
much more,

625
00:31:55,800 --> 00:31:58,080
we are about as high as we can go,

626
00:31:58,080 --> 00:32:02,240
having much more data
is a way of also going up in energy

627
00:32:02,240 --> 00:32:05,240
because we can produce those things
the more rare things you will see there.

628
00:32:08,240 --> 00:32:08,640
Okay.

629
00:32:08,640 --> 00:32:11,400
Well,
I'm looking forward to seeing new results.

630
00:32:11,400 --> 00:32:13,760
I think it's going to be a lot of fun.
I think especially because

631
00:32:13,760 --> 00:32:16,960
you've gone into an area
that we haven't been in before.

632
00:32:17,000 --> 00:32:20,000
So congratulations on doing that.

633
00:32:20,560 --> 00:32:21,920
So thank you.

634
00:32:21,920 --> 00:32:24,280
I want you to thank Giulia Negro

635
00:32:24,280 --> 00:32:28,360
From Purdue University,
in the CMS experiment.

636
00:32:28,800 --> 00:32:33,480
And also Yoav Afik from the ATLAS experiment
and from  

637
00:32:33,840 --> 00:32:37,440
Enrico Fermi Institute,
as shown on his cup

638
00:32:37,880 --> 00:32:39,360
and you have your beautiful CMS cup here.

639
00:32:39,360 --> 00:32:41,080
And I celebrate outreach.

640
00:32:41,080 --> 00:32:43,200
with my IPPOG cup here.

641
00:32:43,200 --> 00:32:46,840
This has been early morning coffee
at CERN.

642
00:32:47,360 --> 00:32:50,360
It's a podcast by the scientists of CERN

643
00:32:50,440 --> 00:32:53,360
about the science of CERN.

644
00:32:53,360 --> 00:32:56,760
You can find all of our episodes
on CERN's YouTube channel.

645
00:32:57,040 --> 00:33:00,240
And if you don't want to look at our
lovely faces, you can also listen to us

646
00:33:00,240 --> 00:33:03,440
anywhere where you get a podcast
Early Morning Coffee at CERN.

647
00:33:04,240 --> 00:33:05,400
Anywhere.

648
00:33:05,400 --> 00:33:08,400
Our editor and producer is Chetna Krishna.

649
00:33:08,400 --> 00:33:11,640
Our executive producer is Jacques Fichet
Studio.

650
00:33:11,640 --> 00:33:14,080
Ron Suykerbuyk is our technical lead.

651
00:33:14,080 --> 00:33:18,680
Our studio manager is Max Brice,
sound engineer by Piotr Traczyk.

652
00:33:18,920 --> 00:33:21,760
Our original theme comes from 
the Canettes Blues Band

653
00:33:21,760 --> 00:33:24,960
with piano by Wojt "Play it in any key" Krajewski.

654
00:33:25,040 --> 00:33:29,760
Many thanks to Paola Catapano, Matthew Chalmers
and Arnaud Marsollier

655
00:33:30,000 --> 00:33:33,120
for all of their great advice
and strategic planning, and a big

656
00:33:33,120 --> 00:33:37,120
thanks to the entire
ECO team (that's not the Ecological team, by the way)

657
00:33:38,040 --> 00:33:42,840
Rather, the Education, Communication and Outreach
team at CERN for providing us with access

658
00:33:42,840 --> 00:33:47,240
to Wire Chamber Studio and
all the help that comes along with it.

659
00:33:47,760 --> 00:33:52,440
Opinions expressed here are our own
and do not necessarily reflect

660
00:33:52,440 --> 00:33:56,440
those of CERN or our colleagues,
even though we think they ought to.

661
00:33:57,040 --> 00:34:00,400
My name is Steven Goldfarb, and this
has been Early Morning Coffee at CERN.

662
00:34:00,440 --> 00:34:01,800
We'll see you again next month.
