Conserved quantities for a charged rotating black holes in 5D Einstein-Maxwell-Chern-Simons theory

Felipe Diaz-Martinez, Rodrigo Olea

Resultado de la investigación: Conference article

Resumen

In this work, we compute the conserved quantities of a charged rotating black hole which appears as the solution of Einstein-Maxwell action in five dimensions coupled to a Chern-Simons term for U(1) field. The addition of the Chern-Simons term will modify the Maxwell equations and the definition of charge but not the Einstein field equations. Upon the addition of suitable boundary terms for the pure gravity sector of the theory, which depend on the extrinsic and intrinsic curvatures (Kounterterms), we obtain the correct conserved quantities of the solution.

Idioma originalEnglish
Número de artículo012022
PublicaciónJournal of Physics: Conference Series
Volumen1043
N.º1
DOI
EstadoPublished - 25 jun 2018
Evento20th Chilean Physics Symposium - Santiago, Chile
Duración: 30 nov 20162 dic 2016

Huella dactilar

Maxwell equation
sectors
curvature
gravitation

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Citar esto

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Conserved quantities for a charged rotating black holes in 5D Einstein-Maxwell-Chern-Simons theory. / Diaz-Martinez, Felipe; Olea, Rodrigo.

En: Journal of Physics: Conference Series, Vol. 1043, N.º 1, 012022, 25.06.2018.

Resultado de la investigación: Conference article

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AB - In this work, we compute the conserved quantities of a charged rotating black hole which appears as the solution of Einstein-Maxwell action in five dimensions coupled to a Chern-Simons term for U(1) field. The addition of the Chern-Simons term will modify the Maxwell equations and the definition of charge but not the Einstein field equations. Upon the addition of suitable boundary terms for the pure gravity sector of the theory, which depend on the extrinsic and intrinsic curvatures (Kounterterms), we obtain the correct conserved quantities of the solution.

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