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]

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: 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


This article is issued from Wikipedia - version of the Wednesday, January 09, 2013. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.