Field equations Einstein-Gauss-Bonnet action

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Discussion Overview

The discussion revolves around the Einstein-Gauss-Bonnet (EGB) action in six dimensions, focusing on the formulation of Einstein equations and the calculation of the stress-energy tensor in this context. Participants explore the implications of working in a six-dimensional framework compared to the more familiar four-dimensional case.

Discussion Character

  • Exploratory, Technical explanation, Debate/contested

Main Points Raised

  • One participant presents the EGB action and expresses uncertainty about calculating the stress-energy tensor, indicating a transition from familiar scalar field theories to a six-dimensional context.
  • Another participant suggests that to derive Einstein equations, one typically adds matter action to the gravitational action, referencing a derivation of the four-dimensional Einstein field equations.
  • A later reply emphasizes that in the absence of matter terms in the six-dimensional case, there would be no stress-energy tensor, suggesting that the Einstein equations would involve terms related to spatial curvature set equal to zero.

Areas of Agreement / Disagreement

Participants express differing views on the role of matter terms in the formulation of the Einstein equations in six dimensions, with some uncertainty about how to proceed without them. The discussion remains unresolved regarding the implications of these differences.

Contextual Notes

The discussion highlights limitations related to the assumptions about the presence of matter terms and the specific formulation of the Einstein equations in six dimensions, which may not directly translate from four-dimensional cases.

Nick2014
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Hello everyone!
I have a "great" problem with EGB action. First of all, I'm used to work with potential and scalar field, but now I have the following action
##S=\int\sqrt{-g}\left(2\beta +R+\alpha GB\right)d^6 x##

where GB is the six-dimensional Gauss-Bonnet term, R is the scalar curvature and ##2\beta## is a cosmological constant. ##\alpha## is a coupling parameter. Well, I want to write Einstein equations, but I don't know how to calculate stress-energy tensor ##T##... Thanks in advance
 
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Nick2014 said:
Hello everyone!
I have a "great" problem with EGB action. First of all, I'm used to work with potential and scalar field, but now I have the following action
##S=\int\sqrt{-g}\left(2\beta +R+\alpha GB\right)d^6 x##

where GB is the six-dimensional Gauss-Bonnet term, R is the scalar curvature and ##2\beta## is a cosmological constant. ##\alpha## is a coupling parameter. Well, I want to write Einstein equations, but I don't know how to calculate stress-energy tensor ##T##... Thanks in advance
See the derivation of the four-dimensional einstein field equations:
http://www.science20.com/standup_ph...d_equation_derivation_about_dozen_steps-90263

Basically, you add the matter action to the gravitational action above.
 
Thanks :) but in my case we are in six dim not four... Then, there is no matter terms... My professor says this...
 
Nick2014 said:
Thanks :) but in my case we are in six dim not four... Then, there is no matter terms... My professor says this...
If you're not going to have any matter terms, then you're not going to have a stress-energy tensor. The analog to the Einstein field equations without any matter action would have some terms related to spatial curvature set equal to zero.
 
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very thanks :)
 

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