Modified gravitation ; how to make it relativistic ?

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Discussion Overview

The discussion revolves around the modification of Newton's law of gravitation and the implications of such modifications for a relativistic framework. Participants explore how to adapt gravitational potential in the context of the Schwarzschild metric, questioning the adequacy of simple substitutions and the need for a more rigorous approach.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Rudi proposes modifying the Schwarzschild metric by replacing terms with a function of gravitational potential, questioning if this is too simplistic.
  • Jim suggests that while the proposed modification might be a good first approximation, it is likely too simplistic.
  • Another participant agrees that the approach is likely too simplistic and emphasizes the need for more specific details regarding the proposed modification.
  • Rudi references a specific modification from literature and questions the rationale behind the perceived simplicity of his approach.
  • Garth inquires about the action that generates Rudi's metric, highlighting the need for a foundational framework.
  • Rudi clarifies that he currently only has a potential and questions the limitations of his proposed substitution.
  • One participant notes that the weak field limit should yield a specific form for the metric, suggesting that the form of the potential is crucial for the validity of the substitution.
  • Another participant points out that modifying GR based on issues with Newtonian gravity raises conceptual questions about the relationship between the two theories.

Areas of Agreement / Disagreement

Participants generally agree that the proposed modification is likely too simplistic, but there is no consensus on the correct approach to make it relativistic. Multiple competing views on the relationship between Newtonian gravity and general relativity remain unresolved.

Contextual Notes

Participants express uncertainty regarding the implications of modifying the gravitational potential and the necessary conditions for such modifications to be valid within a relativistic framework. The discussion highlights the dependence on the specific form of the potential and the need for a rigorous theoretical foundation.

notknowing
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Suppose one is not happy with Newton's law of gravitation and finds that it should be modified and that one has an equation describing the gravitational potential
[tex]\phi[/tex] in function of radius. If one then want to obtain a relativistic description, would it be sufficient to replace in the Schwarzschild metric the term(s)

[tex] \left(\ 1 - \frac {2 G M} {c^2 r} \right)[/tex]

by

[tex] \left(\ 1 + \frac {2 \phi} {c^2 } \right)[/tex]

or would that be to simplistic?

Rudi Van Nieuwenhove
 
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"would that be too simplistic?"
Probably (almost certainly) yes, but it would likely be a good first approximation.

Jim Graber
 
Too simplistic, in all likelihood. If you want more detail I think you'll have to be more specific concerning the modification you have in mind. Providing some rationale for your proposed nonrelativistic correction would probably also be appropriate!
 
Chris Hillman said:
Too simplistic, in all likelihood. If you want more detail I think you'll have to be more specific concerning the modification you have in mind. Providing some rationale for your proposed nonrelativistic correction would probably also be appropriate!

The modification I had in mind is described in : http://arxiv.org/abs/0712.1110
I expected that it was too simplistic, but I don't exactly understand why. If I look for instance in the book Gravity, An Introduction to Einstein's general relativity by James B. Hartle, I find that the derivation of the metric for the static weak field metric (eq. 6.20 on page 126) would have exactly the same form if [tex]\phi[/tex] would have a different radial dependence, or am I wrong? And if it is too simplistic, what would be the correct way to make it relativistic? Or what objection could be made to the simple replacement of [tex]\phi[/tex] with a different radial dependence in the Schwarzschild metric? What physical principles would it violate?
 
Rudi,

What action do you have that generates your metric?

Garth
 
Garth said:
Rudi,

What action do you have that generates your metric?

Garth

For the moment I have neither a metric nor an action. The only thing I have is a simple potential. What would prevent me from using the replacement described in my earlier post?

Rudi Van Nieuwenhove
 
Certainly, the weak field limit should produce [tex]g_{00} = 1+2\phi(r)[/tex], so in that sense it seems reasonable as a first approximation (as others have echoed already). I think it depends on the form of the potential, and how it depends on the radial coordinate. If you consider the extra-dimensional Schwarzschild metric, it follows the pattern you suggest, e.g.:

[tex]g_{00} = 1-\left(\frac{r_H}{r}\right)^{n+1}[/tex]

which we know is an exact solution (derived from the action) and basically boils down to substituting the [tex]n+1[/tex]-dimensional potential. I would think that as long as the potential follows a power-law behavior, you're good to go (but in that case you're not proposing something radically different).

That being said, I think you've raised an interesting question, because it's not one that I've seen explained with any high degree of satisfaction.
 
Last edited:
Rudi,
you start by proposing that if Newtonian gravity is not satisfactory and should be modified, that we should modify GR. Metrics are not part of Newtonian gravity so you are proposing modifying GR ( ?) because N. gravity is no good. Your question does not make sense to me.

As has been pointed out, Newtonian gravity emerges as a weak field solution in GR. But GR and Newtonian gravity are separate and different theories.
 

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