Can GR be formulated as background dependent?

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Discussion Overview

The discussion centers on the possibility of formulating General Relativity (GR) as a background-dependent theory, exploring whether such a formulation can reproduce key results of GR while allowing for a fixed spacetime metric. The scope includes theoretical implications, conceptual clarifications, and references to existing literature.

Discussion Character

  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants propose that GR could be viewed as a field acting over a spacetime metric rather than encoding it within the metric itself, potentially allowing for time-varying phenomena.
  • Others argue against this view, stating that a fixed metric would lead to different causal orderings, as causality in GR is determined by the dynamically determined metric.
  • A participant references Kip Thorne's work, suggesting a formulation of GR where spacetime remains flat and matter deforms measurement devices, which could be considered background dependent.
  • Another participant notes a formulation in Thorne's book that requires harmonic coordinates, indicating that the approach may depend on specific assumptions about spacetime.
  • One participant asserts that a background-dependent formulation is consistent, provided certain caveats are acknowledged, and discusses the challenges related to global nontrivial topologies and the need for multiple coordinate charts.
  • It is mentioned that using a vielbein introduces a background-dependent perspective within GR, highlighting the existence of alternative formulations that deviate from pure linearized gravity.

Areas of Agreement / Disagreement

Participants express differing views on the feasibility and implications of a background-dependent formulation of GR, with no consensus reached on the validity of such an approach.

Contextual Notes

Limitations include the dependence on specific assumptions regarding spacetime and the potential for unresolved mathematical steps related to the formulation of GR in different contexts.

ensabah6
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as a field acting over a spacetime metric (rather than encoding it in the metric) but still reproduce key GR results including time-varying phenomena?
 
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No, because events would have a different causal ordering in the two cases.
The causal order is determined by the metric---which defines the lightcones and therefore which events can influence which---who is in the causal past of whom.

In the real GR there is the one dynamically determined metric g, and that decides causality.

In the fake case you have a fixed metric h and on top of that a small field k so that the combined result is supposed to reproduce the real GR case and give g = h + k.

The difference is that in the fake case causality is determined by the fixed h.
 
Kip Thorne's book "Black holes and time warps: Einstein's outrageous legacy" mentions a formulation of GR in which spacetime is flat, and instead of curving spacetime, matter deforms "measurement devices" to get the same predictions about the results of experiments as standard GR. That sounds like a formulation that we might want to call "background dependent".
 
I tried to find the formulation that Thorne refers to, but the closest I could find is Section 4.3 "Einstein's equations in relaxed form", which requires that one can set up harmonic coordinates "Equation 62 is exact, and depends only on the assumption that spacetime can be covered by harmonic coordinates." http://relativity.livingreviews.org/Articles/lrr-2006-3/

There is apparently a different approach to GR using geometric algebra in which spacetime is flat: http://arxiv.org/abs/gr-qc/0405033
 
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My answer would be yes it is completely consistent, modulo the caveats found in MTW chapter 18 or in Weinbergs book. Starting from linearized gravity, you have to bootstrap your way up to the full nonlinear equations, but that works fine and there is no problem with causality.

There is a small technical issue for global nontrivial topologies which means in practise that you have to be careful and glue together several coordinate charts, but again that has been done and there isn't much of a problem.

The bigger problem is what if you want the local chart to be something other than a connected Euclidean topology. We know of no physical example where that would not be the case, but if you insist on being completely general (perhaps more general than nature herself) then you would have a case.

Anyway, more generally there are other perfectly valid formulations of GR other than 'pure' linearized gravity, where you do need to break the diffeomorphism group and specify coordinates from the onset. For instance, everytime you use a vielbien you are explicitly providing a background dependent picture of GR (in terms of frame fields)
 

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