2014/11/30 by D. Bazeia, F. A. Brito, F. G. Costa +1
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Brane #Classical mechanics #Cosmology and Gravitation Theories #Covariant transformation #Equations of motion #Field equation #Galaxies: Formation, Evolution, Phenomena #Geometry #Gravitation #Mathematical physics #Mathematics #Physics #Scalar (mathematics) #Scalar field #gr-qc #hep-th
paper · pdf · doi:10.1103/physrevd.91.046001
published as Phys. Rev. D 91, 046001 (2015) · Latex, 15 pages, 3 figures; v3: typos corrected
openalex publication_date 2015/02/02 · arxiv created 2015/02/03 · arxiv updated 2015/03/04 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
In this paper we have considered the structure of the nonprojectable Horava-Melby-Thompson 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.