Gauge Vectors-Tensor Gravity

preprint2014arXivOpen access

Abstract

We review and extend the Gauge Vectors-Tensor gravity: a covariant theory of gravity composed of a metric and gauge fields, leading to simple second order partial differential equations of motion, whose Newtonian and strong limits coincide to those of the Einsten-Hilbert action but the physics of its very weak fields should be identified through observation. We show that GVT is at least as dynamically stable as the Einstein-Hilbert gravity. It accommodates the MOND paradigm. We study its gravitational light deflection. We show that the post Newtonian parameter of γγ vanishes in the MOND regime of GVT gravity. Since ΛΛCDM assumes that γ=1γ=1, this suggests to observationally measure the γγ parameter in the weak regime of gravity as either a test for ΛΛCDM or GVT models

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