Bi-scalar tensor vector gravity

Bi-scalar tensor vector gravity theory (BSTV)[1] is an extension of the tensor–vector–scalar gravity theory (TeVeS).[2] TeVeS is a relativistic generalization of Mordehai Milgrom's Modified Newtonian Dynamics MOND paradigm proposed by Jacob Bekenstein.[3] 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.[4]

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

References
  1. Sanders, R.H. (2005-07-01) A tensor-vector-scalar framework for modified dynamics and cosmic dark matter Cornell University Library, retrieved July 11, 2010
  2. Jacob D. Bekenstein (2004), "Relativistic gravitation theory for the modified Newtonian dynamics paradigm", Phys. Rev. D, 70 (8): 083509, arXiv:astro-ph/0403694, Bibcode:2004PhRvD..70h3509B, doi:10.1103/PhysRevD.70.083509
  3. M. Milgrom (1983), "A modification of the Newtonian dynamics as a possible alternative to the hidden mass hypothesis", Astrophys. J., 270: 365–370, Bibcode:1983ApJ...270..365M, doi:10.1086/161130
  4. Zhao, HongSheng; Bacon, David J.; Taylor, Andy N.; Horne, Keith (2005-12-16) Testing Bekenstein's Relativistic MOND gravity with Lensing Data Cornell University Library, retrieved July 11, 2010


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