The Effect of Sources on the Inner Horizon of Black Holes

dc.contributor.author	Gürtuğ, Özay
dc.contributor.author	Halilsoy, Mustafa
dc.date.accessioned	2016-01-26T09:07:53Z
dc.date.available	2016-01-26T09:07:53Z
dc.date.issued	2001
dc.identifier.citation	Ozay Gurtug and Mustafa Halilsoy, “Effect of Sources on the Inner Horizon of Black Holes.” Physical Review D . Vol: 64 , 084023, (2001).	en_US
dc.identifier.issn	1550-2368 (online)
dc.identifier.issn	1550-7998 (print)
dc.identifier.other	DOI: 10.1103/PhysRevD.64.084023
dc.identifier.uri	http://hdl.handle.net/11129/2050
dc.description	The file in this item is the publisher version (published version) of the article.	en_US
dc.description.abstract	A single pulse of null dust and colliding null dust both transform a regular horizon into a spacelike singularity in the space of colliding waves. The local isometry between such space-times and black holes extrapolates these results to the realm of black holes. However, the inclusion of particular scalar fields instead of null dust creates null singularities rather than spacelike ones on the inner horizons of black holes.	en_US
dc.language.iso	en_US	en_US
dc.publisher	Physical Review D, American Physical Society (APS)	en_US
dc.relation.ispartofseries	;Phys.Rev. D64 (2001) 084023
dc.subject	gravity	en_US
dc.subject	general relativity	en_US
dc.subject	Black Holes	en_US
dc.title	The Effect of Sources on the Inner Horizon of Black Holes	en_US
dc.type	Article	en_US
dc.description.version	Publisher Version (Published Version).