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Bi-scalar tensor vector gravity : ウィキペディア英語版 | Bi-scalar tensor vector gravity
Bi-scalar tensor vector gravity theory (BSTV)〔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〕 is an extension of the ''tensor–vector–scalar gravity'' theory (TeVeS). TeVeS is a relativistic generalization of Mordehai Milgrom's Modified Newtonian Dynamics MOND paradigm 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.〔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〕 ==References==
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