John Moffat's STVGravity: Recognition by Physics Community?

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SUMMARY

John Moffat's Scalar-Tensor-Vector Gravity (STVG) presents an alternative to General Relativity (GR) by addressing phenomena such as Galaxy Rotation Curves without invoking dark matter. While STVG has not been universally recognized by the Theoretical Physics Community, it is grounded in established tensor-scalar theories dating back to the 1960s and has been published in peer-reviewed journals. The theory's validity hinges on experimental verification, particularly in scenarios beyond galactic rotation curves, where it may yield different predictions than GR. As of now, no definitive experimental evidence has confirmed STVG's superiority over GR.

PREREQUISITES
  • Understanding of General Relativity (GR)
  • Familiarity with Scalar-Tensor theories
  • Knowledge of Galaxy Rotation Curves
  • Basic principles of experimental physics
NEXT STEPS
  • Research the implications of Moffat's Scalar-Tensor-Vector Gravity on astrophysical phenomena
  • Examine the original Brans-Dicke tensor-scalar theory and its historical context
  • Investigate current experimental tests comparing STVG and General Relativity
  • Explore peer-reviewed articles on STVG available at arXiv.org
USEFUL FOR

Theoretical physicists, astrophysicists, and researchers interested in alternative gravity theories and the ongoing debate surrounding dark matter and galaxy dynamics.

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Is John Moffat's Scalar-Tensor-Vector Gravity an advancement of General Relativity? Is it acknowledged or recognized by the Theoretical Physics Community since it explains certain phenomenon such as Galaxy Rotation Curves and doesn't require directly observed dark matter: http://en.wikipedia.org/wiki/Galaxy_rotation_curve

Here is a list of resources:
http://arxiv.org/PS_cache/gr-qc/pdf/0506/0506021v7.pdf
http://arxiv.org/PS_cache/astro-ph/pdf/0506/0506370v4.pdf
http://en.wikipedia.org/wiki/Scalar–tensor–vector_gravity
 
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According to the (short) Wiki article it explains galactic rotation curves by fitting two adjustable parameters to the data. I don't think it is an advance on GR, but not for that reason alone.
 
Tensor-scalar theories have been around since 1960. "Acknowledged or recognized by the theoretical physics community" is kind of a vague criterion. It's not crank stuff: it was originated by respected relativists, published in peer-reviewed journals, and not found to be logically flawed. Whether the true laws of physics work that way is a question to be decided by experiment. Any such theory has GR as a special case, where some adjustable parameters are set to some specific values. In the case of the original Brans-Dicke tensor-scalar theory, solar-system observations in the 70's showed that those parameters had to be very close to the GR values. The same thing may or may not happen with Moffat's theory. The question for experimentalists to test would be whether, in some area other than galactic rotation curves, it makes predictions that are different from those of GR, and in that situation which theory matches up better with experiment. If Moffat's theory matches experiment and GR doesn't, then Moffat's theory would be an advance over GR. AFAIK no such observations have happened yet.
 

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