Black hole solutions in braneworlds with induced gravity

Kofinas, G; Papantonopoulos, E; Zamarias, V

dc.contributor.author	Kofinas, G	en
dc.contributor.author	Papantonopoulos, E	en
dc.contributor.author	Zamarias, V	en
dc.date.accessioned	2014-03-01T11:44:33Z
dc.date.available	2014-03-01T11:44:33Z
dc.date.issued	2003	en
dc.identifier.issn	0004-640X	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/37004
dc.subject	Black Hole	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.other	BRANE	en
dc.subject.other	SPACE	en
dc.title	Black hole solutions in braneworlds with induced gravity	en
heal.type	other	en
heal.identifier.primary	10.1023/A:1022584330068	en
heal.identifier.secondary	http://dx.doi.org/10.1023/A:1022584330068	en
heal.language	English	en
heal.publicationDate	2003	en
heal.abstract	An analysis of a spherically symmetric braneworld configuration is performed when the intrinsic curvature scalar is included in the bulk action. In the case when the electric part of the Weyl tensor is zero, all the exterior solutions are found; one of them is of the Schwarzschild-(A)dS(4) form, which is matched to a modified Oppenheimer-Volkoff interior solution. In the case when the electric part of the Weyl tensor is non zero, the exterior Schwarzschild-(A)dS(4) black hole solution is modified receiving corrections from the non-local bulk effects. A non-universal gravitational constant arises, depending on the density of the considered object and the Newton's law is modified for small and large distances; however, the conventional limits are easily obtained.	en
heal.publisher	KLUWER ACADEMIC PUBL	en
heal.journalName	Astrophysics and Space Science	en
dc.identifier.doi	10.1023/A:1022584330068	en
dc.identifier.isi	ISI:000181086600034	en
dc.identifier.volume	283	en
dc.identifier.issue	4	en
dc.identifier.spage	685	en
dc.identifier.epage	690	en