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Questions tagged [gravitational-waves]

For questions about the propagation of waves carried by space-time, for instance as described by general relativity. Not to be confused with gravity waves, such as ocean surface waves.

21 votes
2 answers
1k views

The phase difference at the beam splitter of a LIGO-like interferometer is given by $$ \Delta \phi \simeq \frac{4\pi}{\lambda} h L\ , $$ where $h$ is the gravitational wave strain (assuming a ...
ProfRob's user avatar
  • 145k
0 votes
1 answer
82 views

This question was prompted by Bucher et al. published in Nature last month: Bucher T. et al. “Superluminal correlations in ensembles of optical phase singularities.” Nature, Vol. 651, pp. 920–926, ...
MutantMoose's user avatar
2 votes
0 answers
49 views

I am busy studying Gravitational waves and have come across two definition which I am not entirely certain off how they are derived and what they mathematically represent. The first is the energy ...
John's user avatar
  • 43
1 vote
1 answer
112 views

How do gravitational waves propagate through spacetime without a medium? I'm trying to understand gravitational waves at an introductory level, and I'm confused about how they propagate. My confusion: ...
z3itra's user avatar
  • 21
0 votes
0 answers
36 views

can you suggest any resources that explain gravitational waves easily?
4 votes
1 answer
253 views

I'm currently in my second bachelor of mathematics (with extra physics). I want to make mp3-files or wav-files from real observations of gravitational waves for a personal little project. (In the best ...
6 votes
0 answers
81 views

Solitons are an unusual type of waves which don’t disperse due to nonlinear effects. Since general relativity is nonlinear, we can expect the existence of soliton gravitational waves or EM waves. ...
哲煜黄's user avatar
  • 2,867
5 votes
1 answer
186 views

I am trying to derive equation (3.13) from this article on 1st Order Cosmic Phase transition and GWs. First, they are calculating the transition rate $\langle q_0| e^{-i H (t_f-t_i)}| q_0\rangle$ in ...
Alex's user avatar
  • 147
0 votes
0 answers
71 views

Half a century ago Nathan Rosen questioned existence of gravitational waves claiming they should emit 1/2-1/2 retarded-advanced waves: https://link.springer.com/article/10.1007/BF00759493 In 1991 Huw ...
Jarek Duda's user avatar
  • 1,248
0 votes
0 answers
127 views

Does anybody know what factors influence the stability of a Kerr black hole when small perturbations are applied? While I know the Kerr–Newman solution is generally considered to be linearly stable, I ...
Алина Адилканова's user avatar
0 votes
1 answer
76 views

In the context of linearized General Relativity, if a monochromatic, plane-fronted gravitational wave in the transverse-traceless (TT) gauge is described by the metric perturbation: $ h_{ij}^{\mathrm{...
seaofpotential's user avatar
1 vote
0 answers
61 views

Most of perturbation theory in GR is done by perturbing the metric, i.e. writing $g = g_B + \alpha h$, where $\alpha$ is our expansion parameter and $h$ is our perturbation, and then developing either ...
Moguntius's user avatar
  • 486
5 votes
3 answers
467 views

I am studying linearized gravity and the construction of the transverse–traceless (TT) gauge starting from the Lorenz gauge, pages 149/150 of Sean Carroll’s GR notes, linked below. After imposing the ...
Shaashaank's user avatar
0 votes
1 answer
89 views

In the context of the linearized Einstein equations and gravitational waves, Wald defines an effective "stress-energy tensor of the gravitational field" which is constructed from quadratic ...
Tob Ernack's user avatar
2 votes
0 answers
143 views

When we perform a gauge transformation in GR, is it just a coordinate transformation? Or is it something deeper? Because in the derivation of gravitational waves, we first went to Lorenz gauge and ...
Shaashaank's user avatar

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