WEBVTT

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Thank you to Incogni for supporting PBS.

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We spent the last decade listening to the&nbsp;
vanishingly faint vibrations in the fabric of

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spacetime from black holes colliding across the&nbsp;
universe. Now, hundreds of detections later, we

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finally thought we understood the story they were&nbsp;
telling. But then we spotted something that should

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be impossible. A black hole smaller than known&nbsp;
stellar astrophysics allows. A black hole that may

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have formed in the Big Bang itself. It may tell&nbsp;
us something incredible about our universe—but

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also equally importantly about what this young&nbsp;
field&nbsp;of gravitational wave astronomy has become.

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much as it's inspired us, check it out at the&nbsp;
Space Time merch store. Now on to the episode.

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Ten years ago, LIGO detected gravitational&nbsp;
waves for the first time. It was one of

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those discoveries that immediately felt like&nbsp;
the beginning of something much bigger. Yes,

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we’d proved Einstein right. Again. But we'd&nbsp;
also gained an entirely new way of observing

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the universe. What else would that lead to?&nbsp;
Entirely new types of collapsed object? Dancing

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cosmic strings? Echoes from the Big Bang? Even&nbsp;
cracks in the deeper depths of Einstein’s theory?

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Revolutionary observations are exciting because&nbsp;
we don’t know what the new field might evolve

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into. Now fast-forward ten years. We're finally&nbsp;
far enough away from that first detection to ask

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what gravitational-wave astronomy actually has&nbsp;
become. Has it lived up to those expectations?

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Has it changed astrophysics? Or has it mostly&nbsp;
confirmed what we already thought we knew?

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That question has been on my mind because&nbsp;
LIGO, Virgo and KAGRA released their latest

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gravitational-wave catalog—now nearly&nbsp;
400 detections of gravitational monsters

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colliding across the cosmos. But just as we&nbsp;
started to think we understood what we were

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seeing—building and refining our theories of&nbsp;
how they must have come to be… something new

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appeared. It's only a candidate for now, but&nbsp;
if it survives further analysis, it may contain

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a black hole that’s lighter than anyone thought&nbsp;
possible. A black hole that could NOT have formed

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from a star. It’s not confirmed, but people&nbsp;
are paying attention. We'll come back to it.

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Now, the first gravitational-wave detection was&nbsp;
a huge headline, and shortly thereafter a Nobel

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prize. Fair enough. The Laser Interferometer&nbsp;
Gravitational Wave Observatory and its cousins

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are, after all, are miracles of human ingenuity&nbsp;
and chutzpah. The kilometer-scale vacuum systems;

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the mirrors isolated from vibrations&nbsp;
smaller than the width of an atomic nucleus;

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sensitivity improving one observing run at a&nbsp;
time until esoteric tricks of quantum optics

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pushed the fundamental limits of measurement.&nbsp;
Thousands of scientists and engineers working

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together for decades to measure distortions&nbsp;
of spacetime of only about one part in 10²¹.

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Virgo and then KAGRA joined the two LIGO&nbsp;
detectors to improve our ability to localize

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sources on the sky. An ecosystem of fast-response&nbsp;
"traditional" observatories made ready to follow

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up gravitational wave hits. So much work by so&nbsp;
many people, even before the first detection—of

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black holes colliding a billion light years away.
But then something more interesting happened.

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LIGO and its partners got to work. We’ve since&nbsp;
watched spacetime wobbles many hundreds of times

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and how have nearly confirmed 400 mergers of black&nbsp;
holes, with a few neutron stars in the mix. We

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quietly built something far more powerful than any&nbsp;
one measurement of black hole mergers. We built a

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catalog. And in that catalog lies a pattern.&nbsp;
And in that pattern we can infer a universe.

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An interesting thing about every successful&nbsp;
observatory is that it eventually fades away.

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And I mean that nobody asks anymore whether&nbsp;
the James Webb Space&nbsp;Telescope can see distant

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galaxies—we shifted to wondering at the galaxies&nbsp;
themselves—and then wondering what this tells us

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about structure formation in our universe.&nbsp;
We marveled that the Large Hadron Collider

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could make Higgs Bosons— but then we dug into&nbsp;
measuring the particle's properties—then asked

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what its existence tells us about the quantum&nbsp;
structure of reality. The instrument disappears

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and the universe takes center stage.
The same thing has happened with

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gravitational-wave astronomy. Signals&nbsp;
that once would have been buried in the

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noise became routine detections. The catalog&nbsp;
grew—10 mergers, 50, 100—eventually there were

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too many to think about one at a time. And&nbsp;
I think that's the moment this field really

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crossed a threshold. The “discoveries” were&nbsp;
no longer individual events; the discovery

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was the population of events. And it’s in&nbsp;
this catalog that the real science happens.

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There's actually a name for the transition that&nbsp;
gravitational wave astronomy is going through. The

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philosopher of science Thomas Kuhn argued that&nbsp;
scientific revolutions eventually settle into

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what he called normal science. It’s a slightly&nbsp;
unfortunate name, because the most exciting

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science happens in the “normal” phase. In the&nbsp;
case of a revolutionary observational technique,

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Kuhnian normality is the moment a new instrument&nbsp;
becomes dependable enough that scientists stop

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asking whether it works, and start using&nbsp;
it to answer questions they couldn't even

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ask before. That's where gravitational-wave&nbsp;
astronomy is today. With a single detection,

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we can say that gravitational waves are real&nbsp;
and that black holes sometimes merge. And we

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can measure things about the masses and&nbsp;
the spins and their distance and whatnot.

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But with a catalog of detections we can&nbsp;
infer a huge hidden population of black

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hole pairs out there that spend billions&nbsp;
of years orbiting one another in complete

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darkness. And from the spacetime ripples&nbsp;
that wobble though the Earth from the

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last fraction of a second of their inspiral,&nbsp;
we can learn the properties of that whole

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hidden population. We learned that many&nbsp;
of these black holes are much heavier than

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we thought likely. That taught us that&nbsp;
there are unexpected growth mechanisms

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after black holes initial formation for&nbsp;
the collapse of massive stellar cores.

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From the black hole spins we inferred some really

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surprising things about the&nbsp;
way these merging black holes

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find each other.

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A little while ago, when we were talking about&nbsp;
the Dark Energy Survey, I said that reality

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often hides in the relationships between&nbsp;
data. That's what's happening here. The

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universe isn't revealing itself one merger&nbsp;
at a time. It's revealing itself through

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the patterns those mergers form together.
The inference chain is pretty incredible

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if you think about it. Remember that LIGO and co&nbsp;
never measure any of the stuff we figure out. No

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ancient binary progenitor stars for example,&nbsp;
not even the binary black holes themselves.

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We measure a miniscule ripple in spacetime&nbsp;
lasting a fraction of a second. We get to binary

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black holes by asking “what sort of phenomenon&nbsp;
could have produced this?” And once we build the

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catalog—once we know the population properties—we&nbsp;
ask a different question: “What sort of universe

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could have given rise to such a population?”&nbsp;
The ripple remembers the merger and the merger

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remembers the parent stars. And with many ripples&nbsp;
we can infer all the way back to the universe that

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produced the stars that produced the merging black&nbsp;
holes and the faint signal that LIGO catches.

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All of astronomy works this way. It’s a&nbsp;
particularly awesome example of “reverse

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inference”, where we’re only given the&nbsp;
after-the-fact traces and need to infer

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the processes that led to them. Like a detective&nbsp;
figuring out a crime from a room full of subtle

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clues. And astronomy is especially dependent on&nbsp;
reverse inference because there’s no re-running

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the experiment. Other fields have the luxury&nbsp;
of regrowing the culture in a petri dish or

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re-smashing protons in the collider. Astronomy&nbsp;
gets a handful of ancient photons, neutrinos,

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gravitational waves, and has to figure out&nbsp;
the universe that created them. But before

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we can do that, we need this intermediate&nbsp;
step of the catalog. Of the population. Of

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what our universe normally makes. The work&nbsp;
then of normal science is to understand what

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is normal. So maybe it’s a good name after all.
And the reason we care so much about the ordinary

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is that it allows us to prove ourselves wrong.&nbsp;
Attempting to falsify our models—to disprove

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our ideas about the universe is the highest&nbsp;
priority of science. And so a hallmark of a

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mature field of science is that it’s no longer&nbsp;
trying to construct the basic explanations—it’s

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trying to break them. Instead of asking “can I&nbsp;
explain this?”, a mature science asks "Does my

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explanation still survive the next observation?"
Let’s take the example of the correlations between

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the spins of merging black holes. If we&nbsp;
assume that all merging black holes come

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from massive binary stars that formed from&nbsp;
the same cloud of interstellar dust then we

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have a prediction. The spins of those black&nbsp;
holes should both carry the signature of the

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original rotation of the birth cloud. The binary&nbsp;
black holes should have correlated spin. But when

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we look at hundreds of black hole mergers, we&nbsp;
find that indeed many have correlated spin,

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indicating formation by the expected process.&nbsp;
But there’s a second population in which the

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spins of the merging pair are uncorrelated with&nbsp;
each other—pointing in random directions. That

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falsifies the hypothesis that all mergers&nbsp;
come from binary stars. We now have a second

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population of black hole pairs that came together&nbsp;
after their progenitor stars died. In that case,

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they probably found each other after falling&nbsp;
towards the centers of dense star clusters.

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No individual merger points confidently to&nbsp;
one formation scenario or the other, but

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every detection nudges the weight of evidence in&nbsp;
a different direction. After hundreds of events,

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we start to be more confident that, across&nbsp;
the universe and back through its history,

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both of these processes played out. And that we&nbsp;
live in a universe in which both are possible.

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The growing catalog also hints that many black&nbsp;
holes are a bit too massive and spinning a bit

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too rapidly for either of the above scenarios,&nbsp;
allowing us to motivate another formation

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scenario. Some black holes probably sink&nbsp;
into the dense gas disks surrounding active

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supermassive black holes in galaxy centers.&nbsp;
There, the gas can shepherd them together,

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allowing repeated mergers that naturally produce&nbsp;
unusually massive, rapidly rotating black holes.

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This is still just a hypothesis—but one&nbsp;
that's increasingly consistent with the

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growing population of LIGO detections.&nbsp;
But again, the evidence is only in the

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population, not in any one observation.
This is why gravitational wave astronomy

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is rapidly evolving into a mature science, The&nbsp;
individual discoveries are less important than the

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broader, statistical picture. The universe leaves&nbsp;
the most telling traces of its past in statistics,

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not in objects. A mature science interrogates&nbsp;
those statistics to interrogate its models

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of the universe that might explain them. And to&nbsp;
eliminate the models that fail. A mature science

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is in the business of eliminating explanations&nbsp;
until, gradually, the picture that remains starts

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looking less like one possible universe and&nbsp;
more like the universe we actually live in.

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Which brings us back to that one curious signal of&nbsp;
the impossibly light black hole. We don't directly

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measure the masses of each black hole—instead&nbsp;
we measure a particular combination of the two

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masses—the chirp mass. So on November 12th last&nbsp;
year, both LIGO detectors and Virgo quivered under

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an exceptionally faint spacetime ripple that&nbsp;
suggests an extraordinarily low chirp mass.

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If confirmed, it’s very likely that at least one&nbsp;
of the objects has less than the mass of the Sun.

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Such objects should be impossible by the&nbsp;
established modes of black hole formation.

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A dense stellar core of one solar mass does not&nbsp;
collapse into a black hole—it forms a white dwarf.

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But above the Chandrasekhar mass of 1.4&nbsp;
solar masses it becomes a neutron star,

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and only above 3 or so times the sun’s mass&nbsp;
can a dead stellar core collapse into a black

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hole. Now white dwarfs just aren’t compact&nbsp;
enough to produce a LIGO signal on merger,

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but neutron stars and black holes simply&nbsp;
can’t form at such a low mass—at least not

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via stellar evolution. But why did the field&nbsp;
have to be mature in order to spot this thing?

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Well imagine that the very first LIGO signal&nbsp;
had&nbsp;&nbsp;indicated a sub-solar mass black hole merger.

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What would we have concluded? Well probably that&nbsp;
our instrument or our analysis method was flawed.

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We would have spent months or years tweaking&nbsp;
and recalibrating and hoping to catch another.

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Instead, this apparently-tiny black hole&nbsp;
merger came a decade in, when we know that

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LIGO reliably finds and measures appropriately&nbsp;
large masses for its black hole mergers.

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We know the instrument and analysis works.&nbsp;
So now, rather than stressing that we messed

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up somehow, we get to move forward with science.&nbsp;
LIGO has told us what is ordinary—and black

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hole pairs of 3 to 50 solar masses are routine.&nbsp;
Those are consistent with black holes formed in

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the collapse of the dead cores of massive stars.
But a sub-solar mass black hole is NOT consistent

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with this picture. If confirmed, it will falsify&nbsp;
the hypothesis that all merging black holes come

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from stars. We’d need yet another formation&nbsp;
channel. If this thing is real, the best

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explanation seems to be that those black holes are&nbsp;
primordial. That they formed in the unimaginably

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dense conditions of the early universe, before&nbsp;
the first stars had even begun to shine. Finding

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primordial black holes with LIGO would allow&nbsp;
us to extend our reverse inference process all

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the way back to the moments after the Big Bang.
That's an extraordinary possibility, and so also

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requires extraordinary evidence. More detailed&nbsp;
analysis is needed to ensure it isn’t a fluke of

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detector noise and that the inferred masses are&nbsp;
correct. This candidate may still disappear or

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never rise to the level of a confident detection.&nbsp;
That sounds disappointing, but it means the

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process of this now-mature science is working.
Of course, if the sub-solar masses prove to

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be real then we have another mini-scientific&nbsp;
revolution. It starts with one detection—the

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first primordial black hole. Then we find another,&nbsp;
and another, and build the catalog and measure the

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population. From things like the number density&nbsp;
and the mass distribution we’ll learn how and when

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these PBHs formed, just as we did with the regular&nbsp;
black hole mergers. In the case of PBHs, we’d

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learn whether these things can explain dark matter&nbsp;
and derive powerful constraints on the conditions

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of the extremely early universe. Finding multiple&nbsp;
primordial black holes with LIGO would allow us to

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extend our reverse inference process all the&nbsp;
way back to the moments after the Big Bang,

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and PBH detection would become normal science..
Gravitational wave astronomy is right now

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transitioning into a mature field, at least&nbsp;
with respect to “normal” black hole mergers.

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Be excited when it uncovers extraordinary new&nbsp;
things, like this possible PBH. But be satisfied

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when it doesn’t, because this meticulous&nbsp;
mapping of the normal is the real work,

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and the key to an iteratively better&nbsp;
understanding of the whole of space time.
