Refining the MOND Interpolating Function and TeVeS Lagrangian

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Refining MOND interpolating function and TeVeS Lagrangian

The phenomena customly called Dark Matter or Modified Newtonian Dynamics (MOND) have been argued by Bekenstein (2004) to be the consequences of a covariant scalar field, controlled by a free function (related to the MOND interpolating function μ̃(g/a0)) in its Lagrangian density. In the context of this relativistic MOND theory (TeVeS), we examine critically the interpolating function in the tran...

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evaluation of new mond interpolating function with rotation curves of galaxies

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A Primer to Relativistic Mond Theory

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ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 2006

ISSN: 0004-637X,1538-4357

DOI: 10.1086/500805