LIGO
ProjectWikipedia
290
MENTIONS
74
EPISODES
41
PODCASTS
Search complete. 290 mentions across 74 episodes found for "LIGO".
Nov 9, 2026
When Stars Steal From Each Other: The Strange Lives of Stellar Pairs
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62:40speaker_1NARRATOR
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.
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62:51speaker_1NARRATOR
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.
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63:10speaker_2ADVERTISER
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63:14speaker_3ADVERTISER
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10 MINS LATER
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73:04speaker_1NARRATOR
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.
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73:17speaker_1NARRATOR
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.
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73:31speaker_1NARRATOR
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.
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73:48speaker_1NARRATOR
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 Baryakhtar - Searching for New Particles with Black Holes and Grav Waves (February 27, 2020)
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21:53Masha BaryakhtarGUEST
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.
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22:03Masha BaryakhtarGUEST
Let's say it was born in the LIGO merger.
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22:07Masha BaryakhtarGUEST
The blue regions here are showing the range of parameters where the super radiance condition is satisfied.
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22:13Masha BaryakhtarGUEST
So that means for particles of angular momentum, L equals 1, 2, and 3.
5 MINS LATER
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27:38Masha BaryakhtarGUEST
I'm bored? OK.
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27:40Masha BaryakhtarGUEST
So the other very cool and possibly non-intuitive thing is that you have this huge energy density in the cloud.
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27:48Masha BaryakhtarGUEST
And that can actually source gravitational wave radiation, which is observable at LIGO.
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27:54Masha BaryakhtarGUEST
And I'll talk about that in a few slides.
Adrian Price-Whelan - Mapping dark matter with stellar streams (February 25, 2020)
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1:41Adrian Price-WhelanGUEST
So we're finding large numbers of binary stars using the radial velocity method throughout a huge portion of the Milky Way.
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1:48Adrian Price-WhelanGUEST
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.
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2:00Adrian Price-WhelanGUEST
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.
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2:15Adrian Price-WhelanGUEST
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.
StarTalk Podcast_ Celebrating Einstein_ with Neil deGrasse Tyson
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16:16Neil deGrasse TysonHOST
Book in there somewhere, isn't there? Somewhere, man.
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16:18Neil deGrasse TysonHOST
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.
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16:33Neil deGrasse TysonHOST
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.
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16:39Neil deGrasse TysonHOST
Why don't they give us gravity waves all the time?
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18:28Janna LevinGUEST
So it's like mallets on a drum.
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18:30Janna LevinGUEST
When they get closer and closer, they're getting louder and louder, and it's like this crescendo.
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18:34Janna LevinGUEST
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.
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18:44Janna LevinGUEST
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.
Scientific Martyrs_ Life Beyond Our Planet _ More_ _ Cosmic Queries _106
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29:50Chuck NiceHOST
He says this.
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29:51Chuck NiceHOST
LIGO has used light waves to detect the shrinking and expanding of space caused by passing gravitational waves.
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29:58Chuck NiceHOST
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...
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30:11Chuck NiceHOST
and any other measuring rod, as Einstein would say, and cancel out the change.
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31:45Chuck NiceHOST
That's right.
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31:46Chuck NiceHOST
So now watch.
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31:47Neil deGrasse TysonHOST
It's because of that fact that LIGO, Laser Interferometer Gravitational Wave Observatory, has two lasers at right angles to each other.
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32:02Neil deGrasse TysonHOST
So if one of them stretched, moving that way, it's not stretching the other one.
Sounds of the Universe with Neil deGrasse Tyson _ Kimberly Arcand – Cosmic Queries
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41:49Neil deGrasse TysonHOST
Well, let me lead off, and then, Kim, you pick up the baton here.
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41:52Neil deGrasse TysonHOST
So a new telescope that came online within the last six years is LIGO, the Laser Interferometer Gravitational Wave Observatory.
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42:03Neil deGrasse TysonHOST
It's discovering gravitational waves from colliding black holes that have been moving through the universe for billions of years.
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42:12Neil deGrasse TysonHOST
And so, Kim, that sounds like a natural to turn that into sound.
The Problem With Sabine Hossenfelder
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26:42Dave FarinaHOST
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.
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26:56Dave FarinaHOST
To find gravitational waves, Physicists had to invent and build LIGO, and they eventually succeeded.
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27:03Dave FarinaHOST
Sometimes it's not even about technology.
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27:05Dave FarinaHOST
When Mendel established the field of genetics, for almost a hundred years, nobody could figure out the mechanism of heredity.
Giorgio Gratta - A new look at Mossbauer spectroscopy for fundamental physics...(September 4, 2025)
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8:43Giorgio GrattaGUEST
This is 10 to the minus 25.
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8:45Giorgio GrattaGUEST
LIGO, which with its many kilometer arms, doesn't get that far down.
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8:52Giorgio GrattaGUEST
So it is, I think, generally very interesting to look at those things.
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8:57Giorgio GrattaGUEST
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 Pretorius - Black Hole Collisions: The Extreme Side of Gravity (September 25, 2019)
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1:25Frans PretoriusGUEST
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.
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1:48Frans PretoriusGUEST
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.
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1:58Frans PretoriusGUEST
And this is now a whole new level of direct evidence that tells us black holes exist.
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2:03Frans PretoriusGUEST
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.
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2:40Frans PretoriusGUEST
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.
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2:54Frans PretoriusGUEST
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
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28:04Frans PretoriusGUEST
And there really are no convincing ones.
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28:06Frans PretoriusGUEST
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.
Gotham Fest Session 2 - Bigger Than Smallest (September 6, 2019)
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13:08MashaGUEST
And so what we did is we provided values for what the beyond-GR modifications to these quasi-normal modes look like.
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13:18MashaGUEST
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.
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13:38MashaGUEST
And what I'm thinking about right now is inspiraling systems.
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13:43MashaGUEST
So specifically, something like GW150914, which is the first LIGO detection.
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13:50MashaGUEST
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.
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14:22MashaGUEST
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
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23:08Chiara MingarelliGUEST
So I'm really interested in supermassive black holes, in particular, supermassive black hole binaries that are emitting gravitational waves.
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23:16Chiara MingarelliGUEST
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.
64 more episodes mention LIGO.
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