Hasn't Gravitational Lensing Already Proved Einstein? (LIGO)

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SUMMARY

The recent achievements of LIGO represent a significant experimental validation of Einstein's General Theory of Relativity, particularly through the direct detection of gravitational waves. While gravitational lensing and the Hulse–Taylor binary pulsar observations have provided substantial evidence for general relativity, LIGO's findings introduce a new dimension to astrophysics, akin to the advancements brought by radio and x-ray astronomy. The observed gravitational waveforms align closely with predictions from general relativity, reinforcing its validity in extreme gravitational environments. This breakthrough not only strengthens existing theories but also raises questions about the nature of black holes and the potential discovery of new forms of matter.

PREREQUISITES
  • Understanding of General Relativity principles
  • Familiarity with gravitational wave detection technology
  • Knowledge of binary pulsar systems, specifically the Hulse–Taylor binary pulsar
  • Concepts of black hole physics and the no-hair theorem
NEXT STEPS
  • Explore the implications of LIGO's gravitational wave observations on astrophysics
  • Research the Hulse–Taylor binary pulsar and its significance in gravitational wave studies
  • Investigate the no-hair theorem and its relevance to black hole characterization
  • Learn about neutron-star mergers and their potential to inform nuclear physics
USEFUL FOR

Astronomers, physicists, and researchers interested in gravitational wave astronomy, general relativity, and the fundamental nature of black holes and matter.

dlivingston
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The news out of LIGO is being heralded as one of the most important experimental verifications of physics in decades, as it provides experimental support to the General Theory.

The news makes it seem as though it were like the Higgs Boson was; theoretically concrete, but up in the air until this research confirmed it.

But hasn't the well known gravitational lensing effect already provided nearly as strong experimental evidence?
 
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You are right. We have much experimental evidence in favour of general relativity, and the binary pulsar observations of Taylor and Hulse showed that gravitational waves exist.

LIGOs achievement is
1) technological, allowing an amazing direct detection of a gravitational wave;
2) hopefully will allow a new type of astronomy, just like radiowaves and x-rays allow us to see more of what is out there than visible light allows.
 
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dlivingston said:
But hasn't the well known gravitational lensing effect already provided nearly as strong experimental evidence?

Sure, as has the observations on the Hulse–Taylor binary pulsar along with plenty of other tests. However this is akin to detecting the oscillation of a radio signal for the first time ever. It's a very, very strong piece of evidence in favor of general relativity, and it potentially puts great constraints on any present or future competing theories.
 
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In addition to the points that others have made above, the waveform that was observed agrees well with GR-based calculations for the merger of black holes. That is a unique test of general relativity in the regime of very strong gravitational fields.
 
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bcrowell said:
That is a unique test of general relativity in the regime of very strong gravitational fields.

Do they get any stronger than that?!
 
Drakkith said:
Do they get any stronger than that?!

I do still want to see the gravitational wave signal from two supermassive black holes colliding :-)
 
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Are you sure it's more energetic? The masses are larger, but they are moving slower and are farther away from each other. Does the gravitational radiation power increase monotonically with mass? There's also this issue that the wavelength will be much longer - ten million miles.
 
Oohh, great insights folks. I've learned something and am 200 feet deep in a Wikipedia rabbit hole that started with the Hulse–Taylor binary pulsar. Appreciate it. :)
 
bcrowell said:
I do still want to see the gravitational wave signal from two supermassive black holes colliding :-)

As a nuclear physicist I'd be even more eager to see (transient) gravitational waves from neutron-star mergers, because this could help to restrict the equation of state of nuclear (neutron-rich) matter.

Black holes are quite boring due to the no-hair theorem: It's just some object with a mass, a spin, and an electric charge. This brings up another question, I always ask myself, when I listen to talks about black holes (including Sagittarius in our own galaxy): The only argument we have that these very massive objects are truly black holes is that they have very large masses, ruling out any so far thinkable kind of matter composition (like e.g., neutron or quark stars), but maybe they could be just "stars" of a today unknown kind of matter. So is it possible with a very accurate observation of gravitational waves to falsify the assumption that these objects are just black holes or can one perhaps learn something about possible yet unknown forms of matter?
 
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vanhees71 said:
So is it possible with a very accurate observation of gravitational waves to falsify the assumption that these objects are just black holes or can one perhaps learn something about possible yet unknown forms of matter?

A good question. I'd also like to find a new kind of matter that can withstand the force of 4 million solar masses compressed into an area of space less than 50 million km across.
 
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vanhees71 said:
As a nuclear physicist I'd be even more eager to see (transient) gravitational waves from neutron-star mergers, because this could help to restrict the equation of state of nuclear (neutron-rich) matter.

Black holes are quite boring due to the no-hair theorem: It's just some object with a mass, a spin, and an electric charge. This brings up another question, I always ask myself, when I listen to talks about black holes (including Sagittarius in our own galaxy): The only argument we have that these very massive objects are truly black holes is that they have very large masses, ruling out any so far thinkable kind of matter composition (like e.g., neutron or quark stars), but maybe they could be just "stars" of a today unknown kind of matter. So is it possible with a very accurate observation of gravitational waves to falsify the assumption that these objects are just black holes or can one perhaps learn something about possible yet unknown forms of matter?
There are a growing set of observations to the effect that BH candidates have no surface, consistent horizon rather than exotic body.
 

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