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Bi-scalar tensor vector gravity

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Not to be confused with Scalar–tensor–vector gravity or Tensor–vector–scalar gravity.


Bi-scalar tensor vector gravity theory (BSTV)[1] is an extension of the tensor–vector–scalar gravity theory (TeVeS)[2]. TeVeS was proposed by Jacob Bekenstein, BSTV was proposed by R.H.Sanders. BSTV makes TeVeS more flexible by making a non-dynamical scalar field in TeVeS into a dynamical one[3].

References

  1. ^ R.H. Sanders 2005. "A tensor-vector-scalar framework for modified dynamics and cosmic dark matter"[1]
  2. ^ Jacob D. Bekenstein (2004), "Relativistic gravitation theory for the modified Newtonian dynamics paradigm", Phys. Rev. D, 70: 083509, arXiv:astro-ph/0403694, Bibcode:2004PhRvD..70h3509B, doi:10.1103/PhysRevD.70.083509
  3. ^ HongSheng Zhao, David J. Bacon, Andy N. Taylor, Keith Horne (2005). "Testing Bekenstein's Relativistic MOND gravity with Lensing Data"[2]


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