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298 questions with no upvoted or accepted answers
11 votes
1 answer
458 views

Aren't black holes required to exist forever in our frame of reference instead of evaporating?

I know that for an observer far away, nothing ever crosses a black hole horizon (due to time dilation), while in the frame of reference of a falling observer the horizon is nothing special on its way ...
Stéphane Rollandin's user avatar
7 votes
1 answer
298 views

Charged versus rotating black holes as different kinds of wormholes

I've heard that a maximally extended charged black hole can be a traversable wormhole to the same universe whereas a maximally extended uncharged rotating black hole can only be a wormhole to ...
Timaeus's user avatar
  • 25.7k
6 votes
0 answers
262 views

Why are there multiple universes in the Reissner-Nordström solution?

I am trying to make sense of the Penrose diagram of a non extremal Reissner-Nordström spacetime, that is, the solution with two horizons. The coordinates are $$ v'=\text{exp}\left(\frac{r_+-r_-}{2r_+^...
Lourenco Entrudo's user avatar
5 votes
0 answers
128 views

Is it possible to create a Nil geometry in real spacetime according to general relativity? (What metrics are possible in the real world?)

Background   I've heard that it is possible to construct a Penrose triangle in the 3D geometry Nil. And I wondered: Can we build a Penrose triangle in the real world if spacetime is appropriately ...
Modular Discriminant's user avatar
5 votes
0 answers
260 views

Help understanding the Cartan connection/formalism in General Relativity

I'm trying to understand the Cartan formalism in the context of General Relativity. As I understand it given a pseudo-Riemannian spacetime manifold $M$ we can consider the group of spactime ...
R. Rankin's user avatar
  • 2,847
5 votes
0 answers
761 views

On the embedding of the Schwarzschild metric in six dimensions

At every point of the 4-D space-time, it's metric, being a symmetric 2-tensor, has $\frac{D(D+1)}{2}=10$ independent components. From this we can subtract four degrees of freedom according to the four ...
Spoilt Milk's user avatar
  • 1,349
5 votes
0 answers
782 views

Does any spacetime admit a global foliation in spacelike hypersurfaces?

In the comments of this question the following new questions came up: in general relativity, local coordinates can be found around any point, that single out a time coordinate and a three dimensional ...
doetoe's user avatar
  • 9,304
4 votes
0 answers
92 views

Is the causal structure completely determined by the Weyl tensor alone?

By causal/conformal structure I mean the context of Malament's 1977 theorem. If I understand correctly this means that any two spacetimes which agree about all of the future-directed continuous ...
Daniel Grimmer's user avatar
4 votes
1 answer
112 views

How to relate Riemannian and Lorentzian tetrad fields on the same manifold/spacetime?

Consider Gibbons and Hawkings paper wherein a Riemannian metric $\overset{\mathcal{R}}{g}_{\mu\nu}$ and everywhere well defined normalized line field $l_{\mu}$ on spacetime $M$ may be used to ...
R. Rankin's user avatar
  • 2,847
4 votes
1 answer
122 views

Spacetime metrics extended to negative radius

In the Kerr metric $$ ds^2=\left(1-\frac{2Mr}{\rho^2}\right)dt^2+\frac{4Mar\sin^2\theta}{\rho^2}dtd\varphi-\frac{\rho^2}{\Delta}dr^2-\rho^2d\theta^2-\left(r^2+a^2+\frac{2Ma^2r\sin^2\theta}{\rho^2}\...
john's user avatar
  • 123
4 votes
0 answers
84 views

Conformal Diagram for Astrophysical Black Hole

I have a question about the conformal diagram of an ‘astrophysical’ black hole which forms in finite time (but with no evaporation). Usually I see the conformal diagram presented as something similar ...
Liam Bonds's user avatar
4 votes
0 answers
125 views

How is it possible that a closed null geodesic be incomplete?

In page 190 of "The Large Scale Structure of Spacetime" (Hawking & Ellis), it says: ...there must be a closed null geodesic curve $\gamma$ through $q$. Let $v$ be an affine parameter on ...
黄双林's user avatar
4 votes
0 answers
72 views

Is there an equivalent of Kaluza-Klein for fermionic dimensions?

Taking GR in $D$ dimensions, one can use the process of compactification to turn this into GR in $D-1$ dimensions coupled to a Yang-Mills field. i.e. you start with spin-2 fields and you and up with ...
user avatar
4 votes
0 answers
241 views

A question regarding Leonard Susskind's ER=EPR lecture

https://youtu.be/OBPpRqxY8Uw?t=1315 Right at this instance of the video Susskind starts talking about how space is actually connected by entanglement. (You should watch the video for a accurate ...
user avatar
4 votes
0 answers
217 views

Kerr metric in BMS (Bondi-Metzner-Sachs) coordinates

I am trying to put the Kerr metric into the famous Bondi gauge, which is given for instance by the formula (6.2.10) at page 154 of the following paper: https://arxiv.org/abs/1801.01714. Now, Barnich ...
Nomenomen's user avatar

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