Weinberg's gauge-fixed quantum gravity

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Discussion Overview

The discussion revolves around Weinberg's 1965 paper on a gauge-fixed quantum field theory of gravitation, specifically focusing on the Coulomb-like gauge approach to the graviton. Participants explore the implications of this approach, its nonlocal Hamiltonian, and its relation to Einstein's equations, as well as its reception and further development in the literature.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants note that Weinberg's approach involves a noncovariant field dynamics requiring a nonlocal "Newtonian" term to restore covariance, leading to a linear form of Einstein's equations.
  • There is mention of DeWitt's work as a continuation of Weinberg's ideas, although some participants express a specific interest in the Coulomb-gauge approach rather than DeWitt's contributions.
  • One participant suggests that the gravitational Coulomb gauge might be more prevalent in classical gravitational wave literature, drawing parallels to the Transverse Traceless (TT) gauge.
  • Concerns are raised about the gradient terms in the graviton propagator and their potential contributions to physical amplitudes, with some participants questioning whether these have been addressed in existing literature.
  • Another participant discusses the implications of moving nonlinear terms in the Einstein Equation to the right-hand side, suggesting it leads to a noncovariantly-conserved form for the total energy-momentum pseudotensor.

Areas of Agreement / Disagreement

Participants express varying levels of familiarity with the topic, and while there is some agreement on the significance of Weinberg's work, multiple competing views and uncertainties remain regarding the implications and applications of the Coulomb gauge approach.

Contextual Notes

Some participants highlight the lack of resolution regarding the conjectured nonlocality of the Hamiltonian and the gradient terms in the propagator, indicating that these aspects may not have been fully explored or proven in the literature.

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TL;DR
Anyone completed the derivation of Einstein's Equation?
In this 1965 paper by Weinberg, https://journals.aps.org/pr/abstract/10.1103/PhysRev.138.B988, he describes a quantum field theory of the graviton in a Coulomb-like fixed gauge, where the free graviton has only space-space components and is traceless. This of course makes the field dynamics non-covariant; he then shows that to get back covariance, you need to add a nonlocal "Newtonian" term to the Hamiltonian and also have the graviton couple to a conserved tensor. After a long calculation he gets back the linear form of Einstein's equations, and argues that the tensor on the right-hand side will include a gravitational energy term that is equivalent to the nonlinear parts of the left-hand side in Einstein's equations. But he does not prove this. He also does not prove that certain noncovariant "gradient terms" in his graviton propagator will not contribute to physical amplitudes; he conjectures that this requirement will in fact fix the form of the gravitational energy term.

Has this approach been taken up by others? Have these conjectures ever been proven?
 
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Demystifier said:
Hey, good to see you're still around! I've been away from PF for a while, but when I come back I get my first response from an old friend!

DeWitt's work is certainly very central and powerful, but I'm specifically interested in the "Coulomb-gauge" approach developed by Weinberg in that paper. I like it because it gives the field operators a fully explicit interpretation, in terms of creating and annihilating (on-shell) gravitons. OTOH the explicitly nonlocal Hamiltonian is a bit of a steep price... though maybe not for a Bohmian like you!
 
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Not an expert, but perhaps the gravitational Coulomb gauge is studied more in classical gravitational wave literature.
 
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Demystifier said:
Not an expert, but perhaps the gravitational Coulomb gauge is studied more in classical gravitational wave literature.
It is actually quite similar to the standard Transverse Traceless (TT) gauge. It might even be identical; I'm not sure about that. Kind of ironic that Weinberg calls his gauge "too ugly to deserve a name"! Was TT gauge in use for gravitational waves, back in 1965?

Anyhow, none of the classical GR literature will address the the issue of the gradient terms in the propagator. They also are unlikely to have used Weinberg's Hamiltonian much, because of the nonlocality. But it would be interesting if someone did a detailed comparison between this Hamiltonian and the ADM version.

As for the gravitational energy pseudotensor, it's obvious that moving the nonlinear terms in ##G_{\mu\nu}## to the RHS of the Einstein Equation does give a noncovariantly-conserved (and symmetric) form for the total SEM pseudotensor - assuming Einstein's Equation holds. The interesting question is finding some set of assumptions that make this form unique, beyond the also-obvious point that it serves as the source for the linear part of ##G_{\mu\nu}##. (Linear here means first-order in ##h_{\mu\nu} = g_{\mu\nu}-\eta_{\mu\nu}##)
 
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