Self-interactions in linearized gravity

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In summary, the self-interaction term in linearized gravity is of the form h\partial{h}\partial{h}, which is invariant under a gauge transformation. However, the fourth term seems to break this invariance.
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michael879
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self-interactions in "linearized" gravity

This question is really about the gauge invariance seen in linearized gravity. I'm trying to derive the 3-point self-interaction term in the GR lagrangian (in the weak field limit), and the algebra is just a nightmare. I finally gave up and determined that I could find it by just writing down the most general terms, and requiring gauge invariance. By inspecting the Ricci tensor, it is clear that all of these terms are of the form [TEX]h\partial{h}\partial{h}[/TEX]. The most general lagrangian has 10 terms, but under the infinitesimal gauge transformation [TEX]h_{\mu\nu}\rightarrow h_{\mu\nu} + \partial_\mu\alpha_\nu + \partial_\nu\alpha_\mu[/TEX], it can not be made invariant. In fact, even the 4 point term seems to break gauge invariance. Is this gauge invariance purely a feature of the linear terms or am I doing something wrong?

*edit* and if anyone knows this lowest order self-interaction term that would be incredibly helpful.
 
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I'm interested in this question, although I don't have an immediate answer. Isn't gauge invariance an automatic consequence of general covariance?

Expanding on what you said, the first few terms of the Lagrangian must be of the form hμν,στAμνστ + hμν,σhαβ,γBμνσαβγ + hδεhμν,σhαβ,γCδεμνσαβγ + ... where A, B and C are symmetrized products of kronecker deltas.

Is the problem that the gauge transformation is nonlinear? It's not really hμν → ξμ,ν + ξν,μ, it's hμν → hμαξα + hανξα
 
  • #3


For the question of gauge symmetries, it might be helpful to read the 't Hooft and Veltman paper, which you can get free from http://www.numdam.org/numdam-bin/recherche?h=nc&id=AIHPA_1974__20_1_69_0&format=complete

I dug through some old notes and found an expression that I'd worked out years ago for the cubic interaction from the Einstein-Hilbert action. The attached pdf has the expressions before any gauge fixing.
 

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FAQ: Self-interactions in linearized gravity

What is linearized gravity?

Linearized gravity is a simplified mathematical model used to describe the behavior of gravity in weak gravitational fields. It is based on the linear approximation of Einstein's theory of general relativity.

How do self-interactions affect linearized gravity?

Self-interactions in linearized gravity refer to the interactions between the gravitational field and itself. These interactions can cause changes in the shape or strength of the gravitational field, resulting in a non-linear behavior in the otherwise linearized model.

What is the significance of studying self-interactions in linearized gravity?

Studying self-interactions in linearized gravity can help us understand the behavior of gravity in extreme conditions, such as near massive objects or during cosmic events. It can also provide insights into the fundamental nature of gravity and its interactions with other forces.

How are self-interactions in linearized gravity measured or observed?

Self-interactions in linearized gravity can be measured or observed through various methods, such as analyzing the effects of gravitational waves or studying the behavior of particles in strong gravitational fields. These observations can provide evidence of the non-linear behavior of gravity in certain scenarios.

Are there any current research developments in the study of self-interactions in linearized gravity?

Yes, there are ongoing research efforts to better understand self-interactions in linearized gravity and their implications. Some of the current developments include studying the effects of self-interactions on the dynamics of black holes and investigating the role of self-interactions in cosmological models.

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