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19 votes
3 answers
1k views

Can perfectly stable orbits exist in GR?

Defining "stable orbit" between two bodies as one where, in the absence of other bodies or non-gravitational forces, the distance stays between some value pair $r_{min}>0$ and $r_{max}$. ...
SarcasticSully's user avatar
0 votes
1 answer
85 views

Questions about speed of gravity [duplicate]

If gravity "travels" at $c$, and the sun is travelling "forward", does it mean the planets are actually orbiting various points "behind" the center of the sun? Does it ...
Curious Steve's user avatar
2 votes
3 answers
245 views

Orbit description in Schwarzschild metric

Suppose to have a restricted 2-body system (BH + star with $M_{BH}\gg M_{\mathrm{star}}$) and you want to describe the orbit of the star relative to the BH, i.e. in the Schwarzschild metric. Usually, ...
gravitone123's user avatar
2 votes
1 answer
50 views

How to relate a gravitational plane wave to the GW from a binary system?

I have two different forms of gravitational waves that I am trying to reconcile. A monochromatic GW with angular frequency $\Omega$ propagating in the $\textbf{n}$-direction can be expressed as $$ ...
user1887919's user avatar
  • 1,751
0 votes
1 answer
63 views

Don't Geodesics change due to other geodesics?

So the geodesics that point towards the Earth brings space-time towards the Earth and then back out again, but then the moon has its own geodesics so wouldn't it be kind of like geodesics affecting ...
Roghan Arun's user avatar
  • 1,534
0 votes
0 answers
33 views

Anomalistic periods of Earth and Mercury

Can any one give me a TRUE VALUE for the anomalistic periods of Earth and Mercury? I note the previous question on the following. I more or less implemented the method suggested above using elliptic ...
pwm's user avatar
  • 31
1 vote
1 answer
67 views

GR correction to perihelion precession comparing with newtonian orbit

My professor did the following derivation of the formula for the perihelion precession $\delta \phi = \frac{6\pi G M}{a(1-e^2)}$, but I am missing a factor of 2. I would appreciate if someone can help ...
Damiano Scevola's user avatar
1 vote
1 answer
61 views

Energy of circle orbit in Schwarzschild metric

For Schwarzschild metric we have invariants: \begin{equation} \begin{aligned} & r^2 \frac{d \varphi}{d \tau}=\frac{L}{m} \\ & \left(1-\frac{r_s}{r}\right) \frac{d t}{d \tau}=\frac{E}{m c^2}...
Aslan Monahov's user avatar
0 votes
0 answers
33 views

Circular orbit in a stationary, axially symmetric spacetime

From Poisson's, A Relativists Toolkit, problem 1.12 on page 27: "A particle moving on a circular oribit in a stationary, axially symmetric spacetime is subjected to a dissipative force which ...
Gleeson's user avatar
  • 213
0 votes
1 answer
76 views

What is the expression for strong field Schwarzschild circular orbit perihelion precession?

How can you calculate how large the perihelion shift should be under Schwarzschild conditions in general relativity for minimally disturbed circular orbits in the strong field limit? I think there is ...
Agerhell's user avatar
  • 729
1 vote
0 answers
62 views

Stress-Energy Tensor for a Two Mass System

I just don't understand this tensor and would like to go through an example with you to somehow make sense of it. I consider two spheres with masses $m_1$ and $m_2$, densities $\rho_1$ and $\rho_2$ ...
BinaryBlackHole's user avatar
1 vote
0 answers
81 views

Photon speed for an observer at the photon sphere [closed]

I am asked to compute the orbital period of a photon, in the Scwarzschild spacetime, at the photon sphere for an observer at the same radius, $r^\star=3M$. I have computed the result, $\Delta T=6\pi M$...
Alexandre Zagara's user avatar
1 vote
2 answers
230 views

Can the Schwarzschild orbit equation be solved exactly?

The Schwarzschild orbit is $U'' + U = 1 + \varepsilon \cdot U^2$. I've only seen turning-point analysis that demonstrates shift of perihelion. Is there an exact solution?
LiveProton's user avatar
1 vote
2 answers
173 views

How does the speed (and kinetic energy) necessary to orbit a black hole vary with the radius of orbit?

I understand that closer orbits around Schwarzschild black holes require faster speeds, culminating in a required speed of $c$ at the photon sphere ($r = 3M$ in Schwarzschild coordinates). I'd love to ...
Toby Ord's user avatar
  • 235
0 votes
1 answer
70 views

Can we correctly invoke energy conservation to explain why binary systems do collapse in GR?

I've learned that binary systems emits gravitational waves, so there is energy leaving the system in the form of waves and so the radius of the binary system must decrease as to maintain the ...
Acephalus's user avatar
  • 159

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