Rotating black holes in a Randall-Sundrum brane with a cosmological constant
Contribuinte(s) |
UNIVERSIDADE DE SÃO PAULO |
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Data(s) |
29/10/2013
29/10/2013
2012
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Resumo |
In this work we have constructed axially symmetric vacuum solutions of the gravitational field equations in a Randall-Sundrum brane. A non-null effective cosmological constant is considered, and asymptotically de Sitter and anti-de Sitter spacetimes are obtained. The solutions describe rotating black holes in a four-dimensional brane. Optical features of the solutions are treated, emphasizing the rotation of the polarization vector along null congruences. DOI: 10.1103/PhysRevD.86.124047 Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq) e Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior (CAPES) Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq) e Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior (CAPES) Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP), Brazil Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP), Brazil |
Identificador |
PHYSICAL REVIEW D, COLLEGE PK, v. 86, n. 12, supl. 1, Part 4, pp. 92-108, DEC 26, 2012 1550-7998 http://www.producao.usp.br/handle/BDPI/36265 10.1103/PhysRevD.86.124047 |
Idioma(s) |
eng |
Publicador |
AMER PHYSICAL SOC COLLEGE PK |
Relação |
PHYSICAL REVIEW D |
Direitos |
openAccess Copyright AMER PHYSICAL SOC |
Palavras-Chave | #3-BRANE WORLD #FIELD #THERMODYNAMICS #DIMENSIONS #HIERARCHY #RADIATION #EQUATIONS #METRICS #PHYSICS #MASS #ASTRONOMY & ASTROPHYSICS #PHYSICS, PARTICLES & FIELDS |
Tipo |
article original article publishedVersion |