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1 vote
0 answers
56 views

ADM Formalism for the Effective String Theory

We will consider the following effective action of string theory in leading order of $\alpha'$: $$S=\frac{1}{2\kappa^2_0}\int d^{D}X\sqrt{-G}e^{-2\Phi}\left[R-2\Lambda-\frac{1}{12}H_{\mu\nu\lambda}H^{\...
Daniel Vainshtein's user avatar
0 votes
0 answers
25 views

Do the Komar/ADM mass equations also hold in 2+1D?

All definitions I have come across for the ADM mass require asymptotic flatness, which always is defined for 4 dimensional spacetimes. I was wondering if these formulae in 3+1D hold in 2+1D aswell?
DifferentialgeometryCrusher123's user avatar
1 vote
1 answer
108 views

What is the determinant of the Wheeler-DeWitt metric tensor constructed from spatial metrics in ADM formalism?

The Hamiltonian constraint of General relativity has the following form \begin{align} \frac{(2\kappa)}{\sqrt{h}}\left(h_{ac} h_{bd} - \frac{1}{D-1} h_{ab} h_{cd} \right)p^{ab} p^{cd} - \frac{\sqrt{h}}{...
Faber Bosch's user avatar
0 votes
1 answer
52 views

Solving the Hamiltonian constraint equation in General Relativity

The constraint equation of general relativity reads as follows \begin{align} \frac{(2\kappa)}{\sqrt{h}}\left(h_{ac} h_{bd} - \frac{1}{D-1} h_{ab} h_{cd} \right)p^{ab} p^{cd} - \frac{\sqrt{h}}{(2\...
Faber Bosch's user avatar
2 votes
0 answers
66 views

ADM mass calculation for the BTZ black hole

Considering a non-rotating and non-charged 2+1 dimensional black hole, known as the BTZ black hole which obtained by adding a negative cosmological constant $\Lambda=-\frac{1}{l^2},l\ne0$ to the ...
Daniel Vainshtein's user avatar
2 votes
0 answers
35 views

Partial integration of the Gibbons-Hawking-York boundary term

In https://arxiv.org/abs/1402.6334 on page 16 in their Eq. (5.21), they go from the equation $$S_G+S_\chi\approx\int d^2x\sqrt{-g}XR+\int dt\sqrt{-\gamma}XK$$ to the equation $$=\int d^2x \sqrt{-g}\...
mp62442's user avatar
  • 109
3 votes
2 answers
504 views

Is the mass of curved space, additional mass?

According to Einstein, mass, say in the form of matter, curves space. It is the curvature of space that gives rise to gravity. Now I have heard there is an energy associated with the curvature of ...
John Hobson's user avatar
2 votes
0 answers
67 views

Relation between the Wheeler–DeWitt equation and string theory

Can we derive the Wheeler–DeWitt equations from string theory? Since they are both quantum gravity theory. A simple way seems to be the following logic: The Wheeler–DeWitt equation is the canonically ...
feng lin's user avatar
  • 547
0 votes
0 answers
97 views

Extrinsic curvature, Gauss equation and Christoffel symbol contribution

This question is in the context of geometry of hypersurfaces and ADM formalism. In a $4$-dimensional manifold, we define a $3$-hypersurface with space-like tangent basis $e_a$, $a=1,2,3$, and a normal ...
hyriusen's user avatar
  • 175
2 votes
0 answers
55 views

Lapse and shift choice meaning in asymptotic Minkowski space in ADM formalism

In A Relativist's toolkit by Poisson the defining of the ADM mass starts by introducing an asymptotic Lorenztian frame and in the asymptotic portion of the hypersurface the flow vector becomes: $t^{\...
polology's user avatar
  • 167
1 vote
1 answer
151 views

Star Radius in the Oppenheimer-Snyder metric using ADM formalism

I'm working with gravitational collapse models, in particular with the Oppenheimer-Snyder model. Short list of the assumptions for those unfamiliar with the model, you have a spherical symmetric ...
LolloBoldo's user avatar
  • 1,611
0 votes
0 answers
44 views

How to extract mass from the tt component of the metric

Given an asymptotically flat metric, what is the general recipe in order to obtain the mass from the $tt$ component? In the case of the Schwarzschild metric it is obvious but is there a recipe that ...
Fred's user avatar
  • 31
1 vote
0 answers
44 views

Scalar curvature in ADM Formalism (coordinate to coordinate-free transition)

I am attempting to express the scalar curvature in a coordinate-independent manner. Following the works of Bojowald, Thiemann, we have: $$ {}^{(4)}R= {}^{(3)}R+K_{a b}K^{a b}- (K_a^a)^2 - 2\nabla_a v^...
Powder's user avatar
  • 403
5 votes
1 answer
199 views

BRST structure functions in gravity?

In the classical Hamiltonian BRST formalism, there arise structure functions $\Omega^{\beta_1...\beta_n}_{\alpha_1...\alpha_{n+1}}$ ($n\geq0$) --- see https://inspirehep.net/literature/221897 for ...
dennis's user avatar
  • 742
4 votes
2 answers
127 views

ADM decomposition incompatible with black hole?

In establishing ADM or 3+1 decomposition, one starts with choosing a foliation $\Sigma_t$ where t is a scalar function and $\Sigma_t$ is demanded to be a spacelike slice, i.e. with time-like normal ...
Bowen Zhao's user avatar

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