Artículo
Smooth null hypersurfaces near the horizon in the presence of tails
Fecha de publicación:
04/2013
Editorial:
Amer Physical Soc
Revista:
Physical Review D
ISSN:
1550-7998
Idioma:
Inglés
Tipo de recurso:
Artículo publicado
Clasificación temática:
Resumen
We show that the power-law decay modes found in linear perturbations of Schwarzschild black holes, generally called tails, do not produce caustics on a naturally defined family of null surfaces in the neighbourhood of i+ of a black hole horizon. This null congruence thus yields a well behaved coordinate system both near the event horizon and at null infinity.
Palabras clave:
Black Hole
,
Tails
,
Caustics
Archivos asociados
Licencia
Identificadores
Colecciones
Articulos(IFEG)
Articulos de INST.DE FISICA ENRIQUE GAVIOLA
Articulos de INST.DE FISICA ENRIQUE GAVIOLA
Citación
Kozameh, Carlos Nicolas; Moreschi, Osvaldo Mario; Perez, Alejandro Jose; Smooth null hypersurfaces near the horizon in the presence of tails; Amer Physical Soc; Physical Review D; 87; 4-2013; 1-5;
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