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0 votes
1 answer
125 views

Event horizon in stationary spacetime

In the case of non-stationary spacetimes finding the event horizon is no easy task. The stationary case should somehow be less involved or so it is in some well known cases, such as the Kerr spacetime....
Mr. Feynman's user avatar
  • 1,989
1 vote
1 answer
85 views

Metric of Einstein static universe (ESU) black hole

The Einstein static universe (ESU) has metric $$ g = - dt^2 + d\chi^2 + \sin^2 \chi d\Omega^2 $$ With $$ t \in \mathbb{R}, \chi \in (0,\pi) .$$ Is there a metric that describes an eternal black hole ...
Octavius's user avatar
  • 743
2 votes
1 answer
320 views

Why cant a repulsive event horizon of negative mass be theoretically constructed?

An event horizon appears in the Schwarzschild metric when considering a positive point mass in General Relativity. But for a negative point mass in the negative mass Schwarzschild metric, which ...
Manuel's user avatar
  • 476
3 votes
2 answers
297 views

Time in the negative mass Schwarzschild solution

I have read that for the Schwarzschild metric solution with $M<0$, something odd happens with the time coordinate. For the constants of motion, $dt/d\tau=e(1 - 2GM/r)^{-1}$ with $M<0$ and $e$ a ...
Manuel's user avatar
  • 476
3 votes
1 answer
90 views

Kruskal Diagram: 2D projection?

Is a Kruskal diagram a 2D flat space projection of Schwarzschild space-time diagram? If not, isn't it true that one could not draw one accurately on a paper? BTW, I am not referring to Penrose ...
Nayeem1's user avatar
  • 1,161
3 votes
2 answers
158 views

About the temporal coordinate $t_*$ in Eddinton-Finkelstein coordinate

For the Schwarzschild solution $ds^2=-(1-\frac{2GM}{r})dt^2+(1-\frac{2GM}{r})^{-1}dr^2+r^2(d\theta^2+sin^2\theta d\phi^2)$, if we set $dr^2_*=(1-\frac{2GM}{r})^{-2}dr^2$(in other words, $r_*=r+2GMlog{|...
Lagrange629's user avatar
2 votes
0 answers
568 views

How to derive the Kerr killing vector?

The Kerr metric have two killing vectors: $$t^{\mu} \equiv (k_{t})^{\mu} = (1,0,0,0)\hspace{5mm} \mathrm{and}\hspace{5mm} \phi^{\mu} \equiv (k_{\phi})^{\mu} = (0,0,0,1). \tag{1}$$ In general, it is ...
M.N.Raia's user avatar
  • 3,085
1 vote
1 answer
187 views

Schwarzschild geometry

In the text "Exploring Black Holes" by Taylor ,Wheeler I came across the following thought experiment "We consider two imaginary concentric spherical shells and suppose we measure the &...
the_passionate_one's user avatar
0 votes
1 answer
147 views

Schwarzschild with cosmic strings: How can I visualize the string?

Geometrically, you can talk about a cosmic string in Schwarzschild black hole with this metric $[1]$: $$ds^{2} = -\Big(1- \frac{r_{s}}{r}\Big) dt^{2} + \frac{1}{\Big(1- \frac{r_{s}}{r}\Big)}dr^{2} + ...
M.N.Raia's user avatar
  • 3,085
2 votes
2 answers
262 views

How do I deal with the radius-coordinate of the schwarzschild-metric in this numerical problem?

It is well known that if a black hole fulfills certain conditions, it's tidal forces will rip incoming objects apart even before they cross the event horizon. So at some point, the curvature of space ...
MegAmaNeo1's user avatar
1 vote
1 answer
123 views

Visualization of time curvature of spacetime

The Flamm's paraboloid is a slice of the Schwarzschild metric by two spatial dimensions. This shows the space dilation, but without the time component doesn't really give much insight into the ...
Jan Hudec's user avatar
  • 1,601
2 votes
1 answer
567 views

A doubt on the Topology of Einstein-Rosen Bridges (or Schwarzschild/Kruskal Wormholes)

Well, one of the "mantras" of General Relativity is: Einstein Field Equations concerns about the local geometrical structure of spacetime (the metric tensor) and tell you nothing about the ...
M.N.Raia's user avatar
  • 3,085
4 votes
1 answer
394 views

Penrose diagram for two black holes

There are well-known Penrose diagrams for black holes: And for collapsing star: Diagram for collapsing star is obtained by joining two Penrose diagrams: Is it possible to join diagrams for two ...
Nikita's user avatar
  • 5,707
0 votes
2 answers
59 views

Replacing the $M$ coefficient in Schwarzschild metric with a distribution $M(r)$

Consider the Schwarzschild metric $$ds^2 = -f(r)dt^2 + \frac{1}{f(r)}dr^2+r^2 d\Omega^2,$$ where $f(r)=1-\frac{2M}{r}$. I take it that $M$, although not really the mass of a black hole, is the ...
jboy's user avatar
  • 595
0 votes
1 answer
102 views

Existence of parallel vector field

Is there any known parallel vector field in a Schwarzschild spacetime? Or any method to identify parallel vector fields in any spacetime, given the metric $g$?
Avik De's user avatar

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