WEBVTT

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Thank you to Displate for supporting PBS. For&nbsp;
a while back there, we thought we might be able&nbsp;&nbsp;

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to avoid the black hole. They'd been lurking as&nbsp;
shadows in our theories of gravity forever. Enough&nbsp;&nbsp;

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mass crammed into a small enough space would&nbsp;
lead to a gravitational field from which not&nbsp;&nbsp;

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even life could escape from the surrounding&nbsp;
surface that we call the event horizon. The&nbsp;&nbsp;

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event horizon generates paradoxes that worry&nbsp;
physicists. And the singularity of infinite&nbsp;&nbsp;

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density within the black hole worries them even&nbsp;
more. And so many brave physicists have fought&nbsp;&nbsp;

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for centuries to prove that these monsters&nbsp;
don't exist. They hoped nature would step&nbsp;&nbsp;

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in to save us from the theoretical horror&nbsp;
of ultimate gravitational collapse. One of&nbsp;&nbsp;

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our final hopes is the plank star, a ball&nbsp;
of energy at the heart of the black hole,&nbsp;&nbsp;

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like frozen shards of the Big Bang. Well,&nbsp;
let's hope they're real for physics's sake.

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it lights up after sun exposure, even in the&nbsp;
depths of space. Now, on to the episode. First,&nbsp;&nbsp;

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there were the dark stars of Mitchell and&nbsp;
Lelass, constructed with only Newtonian gravity.&nbsp;&nbsp;

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These things were gigantic, 500 times the&nbsp;
size of the sun in Mitchell's mind. Happily,&nbsp;&nbsp;

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they aren't possible. Giant clouds of gas fragment&nbsp;
and collapse before a dark star can form. But any&nbsp;&nbsp;

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matter collapsed far enough will have an event&nbsp;
horizon. Those collapsing gas fragments would&nbsp;&nbsp;

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form black holes themselves if they were not&nbsp;
saved by the onset of nuclear fusion as internal&nbsp;&nbsp;

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temperature and pressure spikes. The resulting&nbsp;
outflow of energy counters the gravitational&nbsp;&nbsp;

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crush, birthing a true star, which saves us from&nbsp;
collapse until nuclear fuel runs out. Then the&nbsp;&nbsp;

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collapse must continue. But happily, not to&nbsp;
a black hole. Not yet. At extreme densities,&nbsp;&nbsp;

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think an entire star crammed into the volume of&nbsp;
the Earth, new strange quantum effects come to&nbsp;&nbsp;

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the rescue. The electrons of the stellar core&nbsp;
are crushed until all available quantum states&nbsp;&nbsp;

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are filled and they cannot be forced together&nbsp;
anymore. The resulting electron degeneracy&nbsp;&nbsp;

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pressure halts collapse once again, giving us&nbsp;
a white dwarf. Nature seems to have stepped in&nbsp;&nbsp;

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to halt the absurdity of the black hole. So far so&nbsp;
good for our hero physicists. We have Mitchell and&nbsp;&nbsp;

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Lelass getting us into trouble in the first place&nbsp;
with dark stars. Then Arthur Edington figured out&nbsp;&nbsp;

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that stellar fusion halts collapse and it was&nbsp;
Ralph Fowler applying the brand new field of&nbsp;&nbsp;

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quantum mechanics that gave us white dwarfs.&nbsp;
But then Subramanion Chandra Seca came along&nbsp;&nbsp;

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and at only 19 years old on an ocean voyage from&nbsp;
India to Cambridge to begin working with Fowler,&nbsp;&nbsp;

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he proved that even his new bosses white dwarfs&nbsp;
have a failure point. For any white dwarf 40% more&nbsp;&nbsp;

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massive than the sun, gravitational crush will&nbsp;
always exceed the outward electron degeneracy&nbsp;&nbsp;

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pressure. In fact, by including Einstein's&nbsp;
relativity to the quantum descriptions,&nbsp;&nbsp;

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Chandra found that outward pressure no longer&nbsp;
rises fast enough to resist the rising crush&nbsp;&nbsp;

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as a white dwarf gains mass, leading to runaway&nbsp;
collapse. Edington was famously very annoyed by&nbsp;&nbsp;

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this result and disputed it. He was convinced that&nbsp;
nature must prevent such absurdities as infinite&nbsp;&nbsp;

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collapse. But Chandra was right about the white&nbsp;
dwarf collapse. Maybe Edington will still be right&nbsp;&nbsp;

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about the ultimate infinite collapse. There's&nbsp;
one last resppite for collapsing stellar cores&nbsp;&nbsp;

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when physicists realize that electron capture by&nbsp;
protons could halt collapse as a neutron star. But&nbsp;&nbsp;

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the salvation of the stellar core is limited in&nbsp;
this case. The more mass of the neutron star, the&nbsp;&nbsp;

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more compact it becomes. For neutron stars over&nbsp;
a certain mass, the surface gravity stops light&nbsp;&nbsp;

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from escaping and the dreaded event horizon forms.&nbsp;
And that's it. We've lost our battle to stop black&nbsp;&nbsp;

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holes a long time ago. In fact, they are real.&nbsp;
We've seen them in their extreme gravitational&nbsp;&nbsp;

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effects across the universe and in gravitational&nbsp;
waves and now even in images. They are real. And&nbsp;&nbsp;

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frankly, I think that's awesome. You might like&nbsp;
them, too. I mean, you clicked on this episode.&nbsp;&nbsp;

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So, what's this about physicists wanting to avoid&nbsp;
the event horizon? Well, people were uncomfortable&nbsp;&nbsp;

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with the idea of black holes for good reasons.&nbsp;
And the best reason emerged in the 70s when&nbsp;&nbsp;

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Steven Hawking and others showed that black&nbsp;
holes slowly radiate away their mass, shrink,&nbsp;&nbsp;

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and ultimately vanish. The main problem with this&nbsp;
is that all information of everything swallowed by&nbsp;&nbsp;

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a black hole is deleted in that process. This&nbsp;
violates a core tenet of quantum mechanics,&nbsp;&nbsp;

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information conservation. The other problem with&nbsp;
the formation of an event horizon is that there&nbsp;&nbsp;

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is no known process that can stop matter within it&nbsp;
from collapsing into a point of infinite density&nbsp;&nbsp;

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in the center. This singularity generates plenty&nbsp;
of its own problems. Not least of which is that in&nbsp;&nbsp;

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these conditions, the two theories that we use&nbsp;
to get this far, quantum mechanics and general&nbsp;&nbsp;

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relativity, are so conflicted that they can't&nbsp;
be simultaneously true. Black holes point to&nbsp;&nbsp;

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fundamental flaws in our theories of nature. Okay,&nbsp;
so even if we couldn't prevent the event horizon,&nbsp;&nbsp;

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maybe we can at least stop the formation of the&nbsp;
theorybreaking singularity. New generations of&nbsp;&nbsp;

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physicists took up the ancient battle to save us&nbsp;
from this theoretical catastrophe. Most believed&nbsp;&nbsp;

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that the solution must lie in a union of quantum&nbsp;
mechanics and general relativity. For example,&nbsp;&nbsp;

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string theory proposed fuzz balls in which matter&nbsp;
unravels into its stringy weave filling the region&nbsp;&nbsp;

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beneath the horizon. And we covered that already.&nbsp;
Another possible solution is the plank star. a&nbsp;&nbsp;

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star of near absolute collapse supported in the&nbsp;
last instant only by the grainy structure of&nbsp;&nbsp;

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spacetime itself. This comes from what has been&nbsp;
called the main competitor of string theory loop&nbsp;&nbsp;

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quantum gravity. In LQG, space at the tiniest&nbsp;
scales is blocky. In particular, it's built up&nbsp;&nbsp;

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of quantiz 2D area elements whose interplay looks&nbsp;
like 3D space on larger scales. And here larger&nbsp;&nbsp;

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means anything significantly bigger than the plank&nbsp;
length around 10 theus 35 m. If LQG is right,&nbsp;&nbsp;

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then it should give us the same spacetime as&nbsp;
described by general relativity on larger scales.&nbsp;&nbsp;

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And that needs to be true of any quantum gravity&nbsp;
theory. But none have been completely worked out&nbsp;&nbsp;

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and so there's some guesswork in connecting&nbsp;
the plank scale to the scale of GR. One way to&nbsp;&nbsp;

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do that is using so-called semiclassical gravity&nbsp;
which guesses the pertabbations to the equations&nbsp;&nbsp;

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of general relativity as we approach the plank&nbsp;
scale. And this is how Carlo Revelian co got to&nbsp;&nbsp;

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their first picture of the plank star. It actually&nbsp;
came from an effort to describe what might happen&nbsp;&nbsp;

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if the entire universe collapsed like a reverse&nbsp;
big bang. As densities become extreme enough,&nbsp;&nbsp;

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LQG predicts a semiclassical correction to the&nbsp;
cosmological equations, the Freriedman equations,&nbsp;&nbsp;

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in which an anti-gravity-like effect emerges,&nbsp;
causing the collapse to bounce outwards. This&nbsp;&nbsp;

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loop quantum cosmology is meant to describe an&nbsp;
infinitely expanding and contracting universe with&nbsp;&nbsp;

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loopy bounces between cycles. But in 2014, Ralli&nbsp;
and Franchesco Vidatoto showed how this result&nbsp;&nbsp;

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for a collapsing universe could also be used to&nbsp;
approximate the end result of the collapsing star&nbsp;&nbsp;

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inside a black hole. At a certain point, outward&nbsp;
quantum pressure causes it to bounce. In a way,&nbsp;&nbsp;

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it's analogous to the quantum degeneracy pressures&nbsp;
that stopped our white dwarf and neutron stars&nbsp;&nbsp;

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from collapsing further. In that case, it was&nbsp;
quantum particles unable to occupy the same energy&nbsp;&nbsp;

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levels. But with the plank star, it's the quantum&nbsp;
elements of spaceime itself doing the work. If&nbsp;&nbsp;

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LQG is right, this could handily stop the wicked&nbsp;
singularity from ever forming. For a collapsing&nbsp;&nbsp;

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sun mass star, the resulting object would be&nbsp;
about 1 trillionth of a meter. That's small,&nbsp;&nbsp;

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but it's not pointlike. It's not a singularity. In&nbsp;
fact, it's 23 orders of magnitude larger than the&nbsp;&nbsp;

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plank scale. So, relatively gigantic. This ultra&nbsp;
compressed ball of matter is the plank star that&nbsp;&nbsp;

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we've been teasing. The thing about plank stars&nbsp;
is that they shouldn't last for long, at least in&nbsp;&nbsp;

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this semiclassical description given back in 2014.&nbsp;
The same space-time pressure that stops collapse&nbsp;&nbsp;

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also triggers catastrophic rebound. Now, a similar&nbsp;
thing happens when the core of a massive star is&nbsp;&nbsp;

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halted by the formation of a neutron star. The&nbsp;
rest of the star explodes outwards as a supernova.&nbsp;&nbsp;

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But in the case of the plank star, the resulting&nbsp;
rebound is a white hole. Basically, the opposite&nbsp;&nbsp;

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of a black hole, the time reversal, space and&nbsp;
the energy it contains rushing outwards and an&nbsp;&nbsp;

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event horizon that reverses its direction. All of&nbsp;
this takes place in about the time it takes light&nbsp;&nbsp;

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to cross the size of the plank star, which is a a&nbsp;
tiny fraction of a second. So, it sounds like our&nbsp;&nbsp;

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plank star only exists for an instant after the&nbsp;
black hole formation before exploding outwards.&nbsp;&nbsp;

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But in that case, why do we still see black holes&nbsp;
out there? And why don't we see the flashes of&nbsp;&nbsp;

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extreme energy expected when a white hole forms?&nbsp;
Maybe you've seen the film Interstellar and you&nbsp;&nbsp;

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remember that time close to a black hole event&nbsp;
horizon slows down from the point of view those&nbsp;&nbsp;

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waiting for Matthew McConnA back on Earth. Hours&nbsp;
can translate to years. Well, imagine how strong&nbsp;&nbsp;

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that gravitational time dilation would be from&nbsp;
deep below the event horizon. Strong. A rebounding&nbsp;&nbsp;

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plank star would appear frozen in that state&nbsp;
for billions of years for anyone but the plank&nbsp;&nbsp;

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star. So there you have it. ultimate gravitational&nbsp;
collapse foiled again in a 10 the -12 m wide ball&nbsp;&nbsp;

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of energy that looks like the universe as it was&nbsp;
essentially at the big bang but at least it's not&nbsp;&nbsp;

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pointlike or even actually plank scale but we're&nbsp;
not quite safe yet the description I just gave you&nbsp;&nbsp;

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of the plank star is over a decade old it involves&nbsp;
some serious approximations the quantum gravity&nbsp;&nbsp;

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effects were approximated as a modification to&nbsp;
the standard equations of general relativity and&nbsp;&nbsp;

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the collapsing star was approx approximated as&nbsp;
a collapsing universe, which really means that&nbsp;&nbsp;

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its matter was smooth and infinitely extended.&nbsp;
Not really what a collapsing star looks like.&nbsp;&nbsp;

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Nonetheless, yet again, we have a mechanism&nbsp;
by which the collapse is halted, reaching the&nbsp;&nbsp;

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theoretical unpleasantness of the singularity. And&nbsp;
in 2024, Ralli and Vidati updated the picture to&nbsp;&nbsp;

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describe what the plank star eventually evolves&nbsp;
into. Let's zoom back out to the event horizon&nbsp;&nbsp;

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again. With the interior plank star frozen by time&nbsp;
dilation, the event horizon itself slowly shrinks&nbsp;&nbsp;

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as it leaks Hawking radiation. Remember that this&nbsp;
is a problem if it causes the black hole to vanish&nbsp;&nbsp;

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and take its precious quantum information with&nbsp;
it. Now, just as loop quantum gravity arrests the&nbsp;&nbsp;

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plank star collapse, it also stops the final stage&nbsp;
of evaporation of the event horizon. In essence,&nbsp;&nbsp;

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the surface area of the horizon becomes&nbsp;
quantized and can't decay any further. That&nbsp;&nbsp;

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leaves us with a plank relic, a plank length&nbsp;
event horizon that's stuck that way forever.&nbsp;&nbsp;

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And these are actually a possible prediction&nbsp;
of quantum gravity in general. And of course,&nbsp;&nbsp;

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we've talked about them before. But what about the&nbsp;
frozen plank star within that plank relic event&nbsp;&nbsp;

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horizon? Now remember that the internal plank star&nbsp;
was much bigger than a plank length. So trillions&nbsp;&nbsp;

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of times bigger than the plank relic that's&nbsp;
supposed to contain it. But this is actually&nbsp;&nbsp;

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what happens. Just as time dilation freezes the&nbsp;
plank star rebound, the enormous stretching of&nbsp;&nbsp;

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space within that near pointlike event horizon&nbsp;
holds a plank star a trillion times larger. But&nbsp;&nbsp;

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the weirdness doesn't end there. As the shrinking&nbsp;
event horizon approaches the plank scale,&nbsp;&nbsp;

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it is subject to strong quantum effects. And one&nbsp;
of those is the possibility of quantum tunneling&nbsp;&nbsp;

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from the black hole state into the white hole&nbsp;
state. That same white hole can also transition&nbsp;&nbsp;

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back into a black hole and the cycle can repeat&nbsp;
indefinitely, leaving our plank relic and the star&nbsp;&nbsp;

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it contains in a quantum superposition of black&nbsp;
hole and white hole simultaneously. Okay, we've&nbsp;&nbsp;

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come a long way since the gigantic dark stars of&nbsp;
centuries ago. Now, nature seems pretty intent&nbsp;&nbsp;

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on forming event horizons. But maybe we could&nbsp;
narrowly avoid the singularity if we follow the&nbsp;&nbsp;

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path of loop quantum gravity, the final stage of&nbsp;
collapse may be simultaneously near point like a&nbsp;&nbsp;

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knot, flickering eternally between being about to&nbsp;
explode and about to collapse. As an added bonus,&nbsp;&nbsp;

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quantum information is preserved in the relatively&nbsp;
gigantic pocket within that infinite decimal spec.&nbsp;&nbsp;

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Oh, and these things might explain dark matter,&nbsp;
too, but that would require a terrifyingly large&nbsp;&nbsp;

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number of these balls of big bang energy locked&nbsp;
like genies in moes of frozen spacetime. Thank&nbsp;&nbsp;
