Astrophysical Constraints on the Bumblebee Model

Published 6 Sep 2014 in astro-ph.SR | (1409.2022v2)

Abstract: In this work the Bumblebee model for spontaneous Lorentz symmetry breaking is considered in the context of spherically symmetric astrophysical bodies. A discussion of the modified equations of motion is presented and constraints on the parameters of the model are perturbatively obtained.

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