Bi-scalar tensor vector gravity

{{Distinguish|Scalar–tensor–vector gravity|Tensor–vector–scalar gravity}}

Bi-scalar tensor vector gravity theory (BSTV)Sanders, R.H. (2005-07-01) [https://arxiv.org/abs/astro-ph/0502222v2 A tensor-vector-scalar framework for modified dynamics and cosmic dark matter] Cornell University Library, retrieved July 11, 2010 is an extension of the tensor–vector–scalar gravity theory (TeVeS).{{Citation |arxiv=astro-ph/0403694 |title=Relativistic gravitation theory for the modified Newtonian dynamics paradigm |year=2004 |author=Jacob D. Bekenstein |journal=Phys. Rev. D |volume=70 |issue=8 |pages=083509 |doi=10.1103/PhysRevD.70.083509 |bibcode=2004PhRvD..70h3509B}} TeVeS is a relativistic generalization of Mordehai Milgrom's Modified Newtonian Dynamics MOND paradigm proposed by Jacob Bekenstein.{{Citation |bibcode=1983ApJ...270..365M |title=A modification of the Newtonian dynamics as a possible alternative to the hidden mass hypothesis |year=1983 |author=M. Milgrom |journal=Astrophys. J. |volume=270 |pages=365–370 |doi=10.1086/161130|doi-access=free }} 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.Zhao, HongSheng; Bacon, David J.; Taylor, Andy N.; Horne, Keith (2005-12-16) [https://arxiv.org/abs/astro-ph/0509590 Testing Bekenstein's Relativistic MOND gravity with Lensing Data] Cornell University Library, retrieved July 11, 2010