Gravitational wave propagation in GR

In summary, "Gravitational wave propagation in General Relativity (GR)" explores how gravitational waves, ripples in spacetime caused by accelerating masses, travel through the universe. The study delves into the mathematical framework of GR, particularly the linearized field equations, which describe how these waves propagate at the speed of light in a vacuum. It highlights the effects of curvature in spacetime and the influence of matter on wave behavior, providing insights into the generation, detection, and implications of gravitational waves for astrophysics and cosmology.
  • #36
Ok, got it :smile:
 
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  • #37
PeterDonis said:
But a single LIGO apparatus has no way of telling which of those two things happened to cause a difference in the round-trip light travel time between the two arms. The only thing LIGO can do is have multiple detectors at widely different locations and look to see if the same signal appears in both of them. That is what would be expected to be the lcase only if the signal is due to a GW: other causes pushing on the reflectors at the ends of the arms would not be expected to cause the same signal in both detectors at widely different locations.
I'm aware of LIGO is actually a distribuited Observatory consisting of two sites in U.S. When you say LIGO has multiple detectors at widely different locations, are you referring to those two different "site locations" or to multiple detectors installed in the same site ?
 
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  • #39
Ah ok, so there is one (Advanced Virgo) here in Italy too :biggrin:
 
  • #40
cianfa72 said:
Ah ok, so there is one (Advanced Virgo) here in Italy too :biggrin:
Yes, and one in Japan, and some others as well.
 

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