Brane structure from a scalar field in general covariant Horava-Lifshitz gravity
arXiv:1411.3979 · doi:10.1103/PhysRevD.91.046001
Abstract
In this paper we have considered the structure of the non-projectable Horava-Melby-Thompson (HMT) gravity to find braneworld scenarios. A relativistic scalar field is considered in the matter sector and we have shown how to reduce the equations of motion to first-order differential equations. In particular, we have studied thick brane solutions of both the dilatonic and Randall-Sundrum types.
arXiv commentLatex, 15 pages, 3 figures; v3: typos corrected
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