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LIGO

LIGO

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Search complete. 290 mentions across 74 episodes found for "LIGO".

Nov 9, 2026

speaker_1NARRATOR
62:40
The most famous such system is the Hulse-Taylor binary pulsar, where pulsar observations have confirmed the existence of gravitational wave energy loss to remarkable precision.
speaker_1NARRATOR
62:51
The detection of gravitational waves by the LIGO observatory from merging neutron stars and black holes has opened a new window on binary evolution, allowing astronomers to observe the final violent moments of stellar theft.
speaker_2ADVERTISER
63:10
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speaker_3ADVERTISER
63:14
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10 MINS LATER

speaker_1NARRATOR
73:04
The final moments before merger are among the most energetic events in the cosmos, with gravitational wave power rivaling the power output of all visible stars in all visible galaxies combined.
speaker_1NARRATOR
73:17
The collision itself produces X-rays and gamma rays, as well as gravitational waves, creating a multi-messenger event that astronomers can observe across the entire electromagnetic spectrum.
speaker_1NARRATOR
73:31
The neutron star merger events detected by LIGO have confirmed theoretical predictions about the creation of heavy elements like gold and platinum, showing that binary star theft and mergers are the furnaces that forge the rarest elements in the periodic table.
speaker_1NARRATOR
73:48
Each detected event carries information about the internal structure of neutron stars, the strength of gravity in the strongest fields, and the universe's expansion history, making binary mergers the most informative events in modern astronomy.
Masha BaryakhtarGUEST
21:53
Let's say you start with a black hole that's born with high spin, say 0.95 dimensionless units, which is close to extremal curve, and some large mass.
Masha BaryakhtarGUEST
22:03
Let's say it was born in the LIGO merger.
Masha BaryakhtarGUEST
22:07
The blue regions here are showing the range of parameters where the super radiance condition is satisfied.
Masha BaryakhtarGUEST
22:13
So that means for particles of angular momentum, L equals 1, 2, and 3.

5 MINS LATER

Masha BaryakhtarGUEST
27:38
I'm bored? OK.
Masha BaryakhtarGUEST
27:40
So the other very cool and possibly non-intuitive thing is that you have this huge energy density in the cloud.
Masha BaryakhtarGUEST
27:48
And that can actually source gravitational wave radiation, which is observable at LIGO.
Masha BaryakhtarGUEST
27:54
And I'll talk about that in a few slides.
Adrian Price-WhelanGUEST
1:41
So we're finding large numbers of binary stars using the radial velocity method throughout a huge portion of the Milky Way.
Adrian Price-WhelanGUEST
1:48
We found some interesting things like compact object companion candidates that are non-interacting, and we're starting to think about how to use those to understand the sort of progenitors to what are now the LIGO events.
Adrian Price-WhelanGUEST
2:00
I also gave a talk in the fall at one of the lunch talks about the work that I'm doing related to galactic accretion, so on some discoveries we've had related to stars that are forming in the Magellanic Stream as the large and small Magellanic Cloud are merging with the Milky Way.
Adrian Price-WhelanGUEST
2:15
But today I'm really going to focus on this sort of third topic about dark matter, about galactic archaeology, and try to give you the big picture view of where I see research going in the next 10 years or so.
Neil deGrasse TysonHOST
16:16
Book in there somewhere, isn't there? Somewhere, man.
Neil deGrasse TysonHOST
16:18
So Jana, your book, The Black Hole Blues, it explored LIGO, just the quest, not so much LIGO, but the quest to measure gravity waves and what effort that would take.
Neil deGrasse TysonHOST
16:33
So could you describe to me what's going on when two black holes collide? and how they're gonna give us a gravity wave.
Neil deGrasse TysonHOST
16:39
Why don't they give us gravity waves all the time?
Janna LevinGUEST
18:28
So it's like mallets on a drum.
Janna LevinGUEST
18:30
When they get closer and closer, they're getting louder and louder, and it's like this crescendo.
Janna LevinGUEST
18:34
So when LIGO made its first detection, it was the last one fifth of a second of the orbits of two black holes, each one about 30 times the mass of the sun, a couple hundred kilometers across.
Janna LevinGUEST
18:44
They're going very nearly the speed of light, and they're executing a few orbits in the final one fifth of a second, and boom, it's finally loud enough.
Chuck NiceHOST
29:50
He says this.
Chuck NiceHOST
29:51
LIGO has used light waves to detect the shrinking and expanding of space caused by passing gravitational waves.
Chuck NiceHOST
29:58
But wouldn't the waves be in and out of the material of space? If space expands, don't your light waves stretch along with it? Uh...
Chuck NiceHOST
30:11
and any other measuring rod, as Einstein would say, and cancel out the change.
Chuck NiceHOST
31:45
That's right.
Chuck NiceHOST
31:46
So now watch.
Neil deGrasse TysonHOST
31:47
It's because of that fact that LIGO, Laser Interferometer Gravitational Wave Observatory, has two lasers at right angles to each other.
Neil deGrasse TysonHOST
32:02
So if one of them stretched, moving that way, it's not stretching the other one.
Neil deGrasse TysonHOST
41:49
Well, let me lead off, and then, Kim, you pick up the baton here.
Neil deGrasse TysonHOST
41:52
So a new telescope that came online within the last six years is LIGO, the Laser Interferometer Gravitational Wave Observatory.
Neil deGrasse TysonHOST
42:03
It's discovering gravitational waves from colliding black holes that have been moving through the universe for billions of years.
Neil deGrasse TysonHOST
42:12
And so, Kim, that sounds like a natural to turn that into sound.
Dave FarinaHOST
26:42
The same can be the case for any other area of physics, and we must remember that some developments elude experimental verification for decades because new technologies must first be developed in order for such experiments to occur.
Dave FarinaHOST
26:56
To find gravitational waves, Physicists had to invent and build LIGO, and they eventually succeeded.
Dave FarinaHOST
27:03
Sometimes it's not even about technology.
Dave FarinaHOST
27:05
When Mendel established the field of genetics, for almost a hundred years, nobody could figure out the mechanism of heredity.
Giorgio GrattaGUEST
8:43
This is 10 to the minus 25.
Giorgio GrattaGUEST
8:45
LIGO, which with its many kilometer arms, doesn't get that far down.
Giorgio GrattaGUEST
8:52
So it is, I think, generally very interesting to look at those things.
Giorgio GrattaGUEST
8:57
All right, so how does the experiment work? Well, actually, you do the usual undergraduate lab, Musbauer spectroscopy experiment, where you look at the resonant absorptions of photons that are emitted with a narrow line.
Frans PretoriusGUEST
1:25
And so like, do they really exist? Is this just theorist fantasy, or do black holes actually exist? And the answer, science can't prove things like that definitively, especially with astronomical objects, but over the last few decades, the evidence has been growing and growing, and I'd say it's almost incontrovertible now that black holes really do exist.
Frans PretoriusGUEST
1:48
And what's particularly exciting in the last few years, as Andy mentioned, is four years ago LIGO started observing gravitational waves from black hole collisions.
Frans PretoriusGUEST
1:58
And this is now a whole new level of direct evidence that tells us black holes exist.
Frans PretoriusGUEST
2:03
So I'll explain a little bit about gravitational waves, and then I'll show you what aspects of the signals, or why do we say that the signals that LIGO has shown us actually is coming from the collisions of black holes? What is this evidence that these very strange and fascinating objects actually exist, as described by Einstein's theory of general relativity? Okay, so let's sort of begin with Newton's theory of gravity, which is now well over 300 years old.
Frans PretoriusGUEST
2:40
In 1687, Newton came up with his universal law of gravitation, sort of consistent with his Newtonian mechanics framework, where gravity was one of the forces that could exist in nature.
Frans PretoriusGUEST
2:54
And it's a very particular force, and he came up with a very elegant description for this, the so-called universal law of gravitation.

25 MINS LATER

Frans PretoriusGUEST
28:04
And there really are no convincing ones.
Frans PretoriusGUEST
28:06
So that's perhaps a decent argument for it being black holes, but in some sense, they're such extraordinary objects, paraphrasing Carl Sagan, we need extraordinary evidence to say that we're really getting black holes as predicted by relativity.
MashaGUEST
13:08
And so what we did is we provided values for what the beyond-GR modifications to these quasi-normal modes look like.
MashaGUEST
13:18
And this is useful, for example, for LIGO data analysis where people perform tests of general relativity by looking at the post-merger spectrum in gravitational waves and compare it to, let's say, results from what you would get if you were to do perturbations of a Kerr spacetime.
MashaGUEST
13:38
And what I'm thinking about right now is inspiraling systems.
MashaGUEST
13:43
So specifically, something like GW150914, which is the first LIGO detection.
MashaGUEST
13:50
And thinking about, okay, well, if we think about what this system looks like beyond general relativity, and we ask ourselves, okay, how are the inspiral merger and ring down modified? we can produce sort of preliminary results where, similarly to the paper that I talked about earlier, we can provide sort of details on how the quasi-normal mode spectrum is modified, and moreover, we can provide, let's say, modifications to the merger phase.
MashaGUEST
14:22
And so all of this is useful for gravitational wave data analysis because currently analyses are performed using kind of general relativity as your original model.

9 MINS LATER

Chiara MingarelliGUEST
23:08
So I'm really interested in supermassive black holes, in particular, supermassive black hole binaries that are emitting gravitational waves.
Chiara MingarelliGUEST
23:16
So not only am I interested in the individual supermassive black hole binary systems, but also in the cosmic merger history of these supermassive black holes that generates a low frequency gravitational wave background.

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