WEBVTT

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Thank you to Displate for supporting PBS. Nothing

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is complicated. By which I mean everything&nbsp;
is complicated because in quantum physics,

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even the nothing of completely empty space has&nbsp;
some pretty crazy properties. One prediction

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that's been around for a while is that under&nbsp;
extreme conditions, the quantum vacuum can

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sort of crystallize. And there's good evidence&nbsp;
that we've observed this for the first time.

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sort of crystallize. And there's good evidence&nbsp;
that we've observed this for the first time.

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you. Links to the merch store in the description.&nbsp;
you, yourselves, your atoms, and ultimately your

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subatomic particles come from excitations in the&nbsp;
quantum fields that fill all of space. But those

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quantum fields exist without you or your subatomic&nbsp;
particles. They exist in empty space. And this

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busy quantum vacuum does stuff. It interacts with&nbsp;
actual particles, subtly changing things like

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magnetic moment or atomic energy levels. Between&nbsp;
the plates of the Casemir experiment, we can coax

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the quantum vacuum into negative energies. And at&nbsp;
extreme positive energies, like at the collision

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point of a particle collider, the empty fields&nbsp;
of the quantum vacuum can be excited to produce

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all sorts of exotic particles. The mathematics&nbsp;
of quantum field theory describes these quantum

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phenomena with incredible precision. But how&nbsp;
far can we really push this? Can we really think

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of the vacuum as this richly structured thing&nbsp;
beyond the microscopic scope of our experiments?

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Well, there is one phenomenon that may reveal&nbsp;
this structure over hundreds or even thousands

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of kilome. An early prediction of quantum field&nbsp;
theory is that an extreme magnetic field may lock

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empty space into a grainy alignment almost like&nbsp;
crystallizing the vacuum itself. A real crystal

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is a solid whose atoms are locked into an ordered&nbsp;
repeating arrangement. But empty space is never

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that. However, the crystal and the magnetized&nbsp;
vacuum do share one exotic property. They

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change how light travels through them, sort of&nbsp;
locking photons into their grainy structure in a

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phenomenon called breringent. We routinely observe&nbsp;
breringents in crystals. Maybe you remember that

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episode we did with Mither from looking glass&nbsp;
universe. She used crystal breringent to do a

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quantum eraser experiment. But to observe vacuum&nbsp;
by refringence, we need magnetic fields billions

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of times stronger than anything we've been&nbsp;
able to create on Earth. Impossible for us,

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but not impossible for the universe. And in a&nbsp;
paper published in Nature this August, scientists

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claim evidence that a magnetar has crystallized&nbsp;
the empty space around it. To understand all of

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this madness, we're going to need to start much&nbsp;
ser much more familiar with good old refractive

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index. Light slows down in glass, in water, in any&nbsp;
transparent medium. The refractive index tells us

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how much this phenomenon is due to the photons's&nbsp;
electromagnetic wave interacting with the electric

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charges, mostly the electrons in the medium. I'll&nbsp;
give you a slightly cartoonish picture. A photon

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in a transparent medium encounters an electron&nbsp;
in an atom. The photon is an electromagnetic

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wave. So it causes the charged particle to wiggle&nbsp;
a bit. We can imagine the photon being momentarily

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absorbed and then remitted by the electron which&nbsp;
slows it down. Now this is an oversimplification

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really. We have a global em field of all the&nbsp;
wiggling electrons inducing phase velocity

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shifts but that's harder to animate. The change&nbsp;
in speed depends on a number of things including

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the wavelength of the light. And this is why&nbsp;
refraction allows us to separate wavelengths of

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light into a spectrum when passed through&nbsp;
a prism. In certain materials, however,

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the refractive index also depends on polarization.&nbsp;
Now, polarization is just the direction that a

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photon's electric field points. That polarization&nbsp;
direction determines the wiggle direction of the

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electrons that the photon encounters. Now, the&nbsp;
more the electron is able to wiggle, the more it

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will slow down or even stop an incoming photon.&nbsp;
In most media, electrons are able to wiggle the

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same in all directions. And so, polarization of&nbsp;
the incoming light doesn't matter. But that's not

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always the case. In a crystal, for example, the&nbsp;
atoms are in a fixed grid. the electrons may have

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more freedom to vibrate in some directions over&nbsp;
others. So if a photon's polarization direction,

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in particular its electric field, happens to be&nbsp;
aligned with the directions where the electrons

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have more wiggle capacity, then there'll be&nbsp;
more of this absorption reission, and that

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will slow the photon down more. So photons with&nbsp;
different polarization directions traveling the

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same direction through a crystal will experience&nbsp;
different refractive indexes and so different

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speeds. This is what breringences. It's pretty&nbsp;
intuitive to see how we get this behavior in

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a crystal because we have real electrons whose&nbsp;
behavior we can talk about admittedly in highly

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simplified ways. But it turns out that even the&nbsp;
vacuum of space can be forced into by refringence.

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So empty space is anything but. It's filled with&nbsp;
quantum fields in their lowest energy state. That

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includes the electron field, a ubiquitous layer of&nbsp;
the possibility of electrons everywhere in space.

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And a real electron is a persistent jiggle of&nbsp;
energy in that field. Dump energy into the field

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and you can excite an electron posetron pair. You&nbsp;
could do that with say a gamay photon as long as

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it had enough energy to cover the masses of the&nbsp;
particles via E= MC^². But short of that energy,

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a photon will normally ignore the electron field.&nbsp;
However, there are other ways to get the photon

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and the electron fields to notice each other. One&nbsp;
of those is vacuum by refringence. I'm going to

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describe this in two ways. One more intuitive&nbsp;
but less accurate then a bit more rigorously.

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You may have heard of virtual particles. Even&nbsp;
without sufficient energy to provide the particles

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their mass, we can imagine the quantum vacuum&nbsp;
producing matter antimatter pairs extremely

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briefly with their energy borrowed from the&nbsp;
intrinsic uncertainty of the energy of the

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vacuum. These virtual particles aren't like some&nbsp;
cloud of electrons and posetrons everywhere in

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space. Rather, they're a way of representing the&nbsp;
infinite ways that quantum fields can interact

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with real particles. Virtual particles appear in&nbsp;
the mathematics of quantum field theories, most

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notably in fineman diagrams. But most physicists&nbsp;
consider them a mathematical artifact, albeit a

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very useful one, and useful for intuition, too.&nbsp;
In a strong magnetic field, we can imagine that

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the flickering virtual electron posetron pairs are&nbsp;
no longer randomly oriented. They're generated in

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a preferred direction, and that alignment mimics&nbsp;
the alignment of the real charged particles in

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a crystal. And the result is vacuum polarization&nbsp;
which leads to a polarization dependent refractive

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index and so do vacuum refringence in the passing&nbsp;
photons. A more rigorous but less visually fun

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way to say this is that an extreme magnetic field&nbsp;
produces nonlinear corrections to electromagnetism

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through interaction of the electromagnetic&nbsp;
field with the quantum electron field. These

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corrections alter the propagation of photons&nbsp;
with the size of the effect depending on the

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photon's direction and polarization relative to&nbsp;
the magnetic field. But yeah, it's more fun to say

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that space gets crystallized, even if that's not&nbsp;
strictly true. But the resulting effect is very

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similar to crystals. Interestingly, this vacuum&nbsp;
refractive index doesn't actually slow the wave.

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The photons still travel at full light speed, but&nbsp;
the phase of the wave picks up a lag as though

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it were slowed. Two photons with different&nbsp;
polarizations will keep up with each other,

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but they'll fall out of phase with each other. The&nbsp;
magnetic field strength where vacuum polarization

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gets strong is around 4.4 billion Tesla. This&nbsp;
is called the quantum critical magnetic field.

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And that's not to say that vacuum by referring&nbsp;
can't be seen below that field strength,

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just that the effect drops off very quickly&nbsp;
at lower field strengths. Now, the strongest

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magnetic field that we humans have ever made&nbsp;
is 1,200 Tesla. And by refringence experiments

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are typically way lower than this. The effect is&nbsp;
essentially unobservable in humanmade experiments,

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at least so far. But there are places&nbsp;
in the universe where natural magnetic

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fields don't just approach the critical field&nbsp;
strength, they far exceed it. By far the king

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of magnetic fields is the magnetar. These&nbsp;
are a type of neutron star, the collapsed

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core of a massive star that's not quite massive&nbsp;
enough to become a black hole. In its collapse,

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protons and neutrons are smooshed together to&nbsp;
form neutrons, and the whole thing shrinks into

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a citysized ball with the density of an atomic&nbsp;
nucleus and the mass of a star. In that collapse,

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the magnetic field of the progenitor star is&nbsp;
massively amplified. The shrinking core also

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spins itself up, powering surface dynamos that can&nbsp;
boost the field to up to 100 billion Tesla, which

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is something like 20 times the critical field&nbsp;
strength. So more than enough to crystallize the

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surrounding vacuum and cause vacuum polarization&nbsp;
and breringence. And that's what we may just have

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seen in the recent Nature paper. Rachel Stewart&nbsp;
and collaborators argue that vacuum by referring

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is the best explanation for the extreme X-ray&nbsp;
polarization observed in magnetar IE1547.0-5408.

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The key data comes from the imaging X-ray&nbsp;
polarimetry explorer satellite which was

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launched in 2021 by NASA and the Italian space&nbsp;
agency with the primary purpose of measuring X-ray

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polarization. Now X-ray polarization measurements&nbsp;
are really hard due to the small number of X-ray

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photons and their extreme energies. IXP is&nbsp;
really our first precision X-ray polarimeter.

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So this sort of measurement is only recently&nbsp;
possible. The scientists though still needed

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help from NASA's neutron star interior composition&nbsp;
explorer for improving X-ray timing and spectral

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information and from the parks radio telescope&nbsp;
to constrain the magnetic geometry. Together,

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these new observations show extreme polarization&nbsp;
of soft X-rays, which suggests extreme vacuum by

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refringence, at least so the scientists argue.&nbsp;
Let's see how this works by following X-ray

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photons from the surface of the magnetar.&nbsp;
At temperatures of millions of degrees,

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the surface and atmosphere produce huge numbers&nbsp;
of X-rays. Normally, those X-rays would have to

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fight their way through the electrons in the stars&nbsp;
atmosphere. And remember, the electric field of

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photons pushes on charged particles. And electrons&nbsp;
can absorb or scatter light when they're able to

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move in the direction of that push. But these&nbsp;
electrons in the magnetized atmosphere are locked

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to an insanely strong magnetic field. They can&nbsp;
only move relatively easily in the same direction

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of that field. At right angles to the field, the&nbsp;
electrons are locked down, so they can't even

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interact with photons that try to push them in&nbsp;
that direction. X-rays polarized in that direction

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barely see the electrons and so they can escape&nbsp;
from deep within that thick blocking atmosphere.

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But this by itself isn't enough to give us&nbsp;
strongly polarized X-rays seen from Earth. The

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polarization directions of escaping light varies&nbsp;
across the magnetar surface. So from this distance

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all of those different directions should mix&nbsp;
together and partly cancel out. And this is where

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vacuum by refringence comes in. The polarized&nbsp;
X-rays escaping from the atmosphere still have

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to travel through hundreds or even thousands of&nbsp;
kilometers of intensely magnetized empty space.

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Vacuum by refringence makes different polarization&nbsp;
components of those X-rays accumulate phases at

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different rates which keeps each X-ray locked to a&nbsp;
preferred polarization direction set by the local

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magnetic field. As the magnetic field gradually&nbsp;
shifts into a large scale order dipole field,

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the polarizations of all X-rays follow and end up&nbsp;
pointing in the same direction. And that's roughly

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what saw in the 2 to 3 kilo electron volt X-ray&nbsp;
band. The polarization fraction reached as high

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as around 80% during certain parts of the stars&nbsp;
rotation. And that polarization fraction changed

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as the magnetar spun, which makes sense. At each&nbsp;
point in the rotation, we're seeing a different

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orientation of the stars magnetic field and a&nbsp;
somewhat different view of the X-ray emmitting

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region. The result is exciting enough to warrant&nbsp;
the Nature paper, but it's not a definitive

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detection of vacuum by refringence. Another study&nbsp;
published earlier this year argues that most of

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the X-rays could come from a single small hot spot&nbsp;
on the surface of the star. Under the geometry

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favored by that analysis, the photons start out&nbsp;
with fairly similar polarization directions. So,

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we don't need the surrounding magnetic field&nbsp;
to organize them nearly as much. But the latest

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study has an important counterargument. The new&nbsp;
parks radio observations suggest that we are

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looking almost straight down the rotational axis&nbsp;
of the magnetar with its magnetic axis also nearly

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aligned with that axis. And when the authors&nbsp;
model the X-ray emission using that geometry,

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a hotspot alone has a much harder time reproducing&nbsp;
what EXP sees. But if the models allow the

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polarization to keep following the magnetic&nbsp;
field through vacuum by refringence, then the

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observations are reproduced much more naturally.&nbsp;
There's still some tension here. The geometry

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inferred from the X-rays alone is only consistent&nbsp;
with the radiived geometry at around the 2.5 sigma

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level and the X-ray data allows a much wider&nbsp;
range of possibilities. So even the authors stop

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short of claiming a detection. Still remember that&nbsp;
vacuum by refringence isn't some speculative new

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phenomenon invented just to explain these data.&nbsp;
It's a firm prediction of quantum electronamics

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and magnetars have magnetic fields easily strong&nbsp;
enough for the effect to actually matter. So this

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observation is worth taking seriously as perhaps&nbsp;
our clearest glimpse of vacuum by refringence. The

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universe is weird and normally we need to build&nbsp;
incredibly precise and/or gigantic experiments to

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explore its weirdest properties. But the universe&nbsp;
is also awesome and sometimes it generously

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provides us with dead stars crushed to near black&nbsp;
hole densities with magnetic fields so strong that

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they grip the quantum vacuum itself. Perfect&nbsp;
for checking if we were right all along about

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magnetically crystallized spacetime. Thank you&nbsp;
to Displate for supporting PBS. Displate posters
