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322 questions with no upvoted or accepted answers
12 votes
0 answers
1k views

Variation of the Einstein-Hilbert action in $D$ dimensions without the Gibbons-Hawking-York (GHY) term

Consider the standard Einstein-Hilbert action in $D \ne 2$ dimensions spacetimes : \begin{equation} S_{EH} = \frac{1}{2 \kappa} \int_{\Omega} R \; \sqrt{- g} \; d^D x, \end{equation} where $\Omega$ is ...
Cham's user avatar
  • 7,592
11 votes
0 answers
664 views

What are Galileons good for?

Lately I've seen many papers (for example "The galileon as a local modification of gravity"; 292 total hits on the arXiv) on types of field theories known as Galileons, and I'm wondering ...
Surgical Commander's user avatar
8 votes
0 answers
383 views

Definition of gravity path integral?

In a non-abelian gauge theory there is a "fundamental" gauge field $A_\mu^a$ with gauge index $a$ often called connection. Although $ A_\mu^a$ is not gauge invariant, gauge invariant quantities can be ...
user47224's user avatar
  • 322
8 votes
0 answers
215 views

Metric transformation, polygons and gravitons

I'm trying to understand the paper by Hitchin called: ''Polygons and gravitons". I'm stuck at page 471. At this point, he does some computations and obtains a metric: $$ \gamma dz d\bar{z}+\gamma^{...
user1201349's user avatar
6 votes
1 answer
451 views

Covariant derivative of the vielbein determinant

The vielbein postulate says that $$\nabla_\mu e_v^{\,a}=\partial_{\mu}e_\nu^{\,a}+\omega_{\mu\,\, b}^{\,\,a}\,e^b_\nu-\Gamma^\sigma_{\mu\nu}\,e^{\,a}_\sigma=0.$$ $\nabla$ is the coordinate covariant ...
gammadragon's user avatar
6 votes
0 answers
290 views

What does black hole formation and evaporation actually look like as viewed from far away?

Many people on Physics SE (myself included) have been confused about what black hole formation and evaporation look like when viewed from far away. For example: Does any particle ever reach any ...
tparker's user avatar
  • 48.4k
5 votes
0 answers
82 views

Bargmann–Wigner equations in NP formalism

Bargmann-Wigner equations describe free particles of arbitrary spin $j$, namely $$(-\gamma^{\mu}\partial_{\mu}+m)_{\alpha_r \alpha_{r’}}\Psi_{\alpha_1,..,\alpha_{r’},...,\alpha_{2j}}=0$$ where we have ...
jacktang1996's user avatar
5 votes
0 answers
605 views

How to find the Hawking temperature for this metric?

I am reading this paper about "Hawking radiation of Kerr-Newman-de Sitter black hole", where the authors find Hawking temperature of this metric The authors state that hawking temperature is given by ...
WhyME's user avatar
  • 265
5 votes
1 answer
319 views

Proportionality Constant in Einstein Field Equations

The Einstein Field Equations: $$G_{ab}~=~8\pi T_{ab}.$$ I am familiar with how to obtain the $8\pi$ proportionality factor through correspondence with Newtonian gravity, but am wondering if this ...
ClassicStyle's user avatar
4 votes
1 answer
169 views

How are objects inside a black hole affected by the gravity of objects outside the black hole?

There are many Q&As about whether something inside a black hole can escape the event horizon if another massive object gets close enough to pull it out. I realize the answer (I think universally ...
Peter Moore's user avatar
4 votes
3 answers
408 views

Confusion over what constitutes a uniform gravitational field in relativity

Suppose we have some observer moving upwards with a constant proper acceleration, by the equivalence principle this is the same as the observer remaining stationary in a gravitational field, like ...
NaiDoeShacks's user avatar
4 votes
0 answers
110 views

Effective field theories in curved spacetime

Loosely speaking, in flat spacetime, one defines the effective Lagrangian by writing down all possible operators compatible with the symmetries and suppressed by some energy scale, and one usually ...
Joel's user avatar
  • 305
4 votes
0 answers
246 views

Gravity's self-energy

Suppose we have a single massive point particle. In the absence of "potentials", the content of the stress-energy tensor would be dictated uniquely by the particle's mass and trajectory (...
Mikael Marcondes's user avatar
4 votes
0 answers
23 views

Effect (if any) of strong(ish) gravity radiation on stars

Two black holes merge, and a good few percent of their total mass is converted into gravitational radiation. Years or decades later, the resulting gravity wave passes through nearby stars. Does it ...
nigel222's user avatar
  • 700
4 votes
0 answers
232 views

The (Newton-Laplace-Ivory-Arnold) shell theorem in general relativity

It is well-known that Birkhoff's theorem and the classification of LTB spacetimes proves one version of Newton's shell theorem in the context of GR. Another statement in Newtonian gravity, often ...
5th decile's user avatar

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