Galaxy Rotation Curves in Covariant Horava-Lifshitz Gravity
High Energy Physics - Theory
2013-12-19 v2 General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
Abstract
Using the multiplicity of solutions for the projectable case of the covariant extension of Horava-Lifshitz Gravity, we show that an appropriate choice for the auxiliary field allows for an effective description of galaxy rotation curves. This description is based on static and spherically symmetric solutions of covariant Horava-Lifshitz Gravity and does not require Dark Matter.
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Cite
@article{arxiv.1303.1394,
title = {Galaxy Rotation Curves in Covariant Horava-Lifshitz Gravity},
author = {Jean Alexandre and Martyna Kostacinska},
journal= {arXiv preprint arXiv:1303.1394},
year = {2013}
}
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