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Large Scale Structure in Bekenstein's theory of relativistic Modified Newtonian Dynamics

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arxiv astro-ph/0505519 v2 pith:53DOOR3E submitted 2005-05-26 astro-ph gr-qchep-th

C. Skordis , D. F. Mota , P. G. Ferreira , C. Boehm This is my paper · ORCID
classification astro-phgr-qchep-th
keywords theorybekensteinevolutionfieldgravitymodifiedbackgroundcosmic
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A relativistic theory of modified gravity has been recently proposed by Bekenstein. The tensor field in Einstein's theory of gravity is replaced by a scalar, a vector, and a tensor field which interact in such a way to give Modified Newtonian Dynamics (MOND) in the weak-field non-relativistic limit. We study the evolution of the universe in such a theory, identifying its key properties and comparing it with the standard cosmology obtained in Einstein gravity. The evolution of the scalar field is akin to that of tracker quintessence fields. We expand the theory to linear order to find the evolution of perturbations on large scales. The impact on galaxy distributions and the cosmic microwave background is calculated in detail. We show that it may be possible to reproduce observations of the cosmic microwave background and galaxy distributions with Bekenstein's theory of MOND.

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    Static spherically symmetric vacuum solutions of AeST include two classes of stealth Reissner-Nordstrom black holes with nontrivial secondary scalar and vector hair.

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