Marcelo Samuel Berman
Instituto Albert Einstein, Av. Candido Hartmann, 575, No. 17, 80730–440, Curitiba–PR, Brazil. (msberman@institutoalberteinstein.org).
Received 2007 September 20
Accepted 2008 May 6
RESUMEN
]]> Dando seguimiento a un artículo previo, revisamos los resultados para la energía y momento angular de un hoyo negro de Kerr–Newman, y extendemos el cálculo para el caso de un dilaton en rotación, obtenido a partir del modelo de Garfinkle et al. (1991, 1992). Mostramos que hay, en lo que se refiere solamente a la energía y momento angular, una interacción entre los campos, de forma que, el gravitacional y el electromagnético pueden ser ocultados por la intensidad del campo escalar.
ABSTRACT
Following a prior paper, we review the results for the energy and angular momentum of a Kerr–Newman black hole, and then calculate the same properties for the case of a generalised rotating dilaton of the type derived, without rotation, by Garfinkle et al. (1991, 1992). We show that there is, as far as it refers only to the energy and angular momentum, an interaction among the fields, so that, the gravitational and electromagnetic fields may be obscured by the strength of the scalar field.
Key Words: black hole physics — gravitation — magnetic fields — relativity.
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