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	2014-03-01T01:17:35Z
dc.date.available	2014-03-01T01:17:35Z
dc.date.issued	2002	en
dc.identifier.issn	0556-2821	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/14574
dc.subject	Closed System	en
dc.subject	Satisfiability	en
dc.subject	Black Hole	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.classification	Physics, Particles & Fields	en
dc.subject.other	INDUCED GRAVITATIONAL CONSTANT	en
dc.subject.other	DARK-MATTER	en
dc.subject.other	BRIGHT SIDE	en
dc.subject.other	BRANE	en
dc.subject.other	BULK	en
dc.subject.other	DIMENSIONS	en
dc.subject.other	COSMOLOGY	en
dc.subject.other	SPACETIME	en
dc.subject.other	BREAKING	en
dc.subject.other	SCALAR	en
dc.title	Black hole solutions in braneworlds with induced gravity	en
heal.type	journalArticle	en
heal.identifier.primary	10.1103/PhysRevD.66.104028	en
heal.identifier.secondary	http://dx.doi.org/10.1103/PhysRevD.66.104028	en
heal.identifier.secondary	104028	en
heal.language	English	en
heal.publicationDate	2002	en
heal.abstract	We extend our previous study on spherically symmetric braneworld solutions with induced gravity, including nonlocal bulk effects. We find the most general static four-dimensional black hole solutions with g(tt)=-g(rr)(-1). They satisfy a closed system of equations on the brane and represent the strong-gravity corrections to the Schwarzschild-(A)dS(4) spacetime. These new solutions have extra terms which give extra attraction relative to the Newtonian-(A)dS(4) force; however, the conventional limits are easily obtained. These terms, when defined asymptotically, behave like AdS(4) in this regime, while when defined at infinitely short distances they predict either an additional attractive Newtonian potential or an attractive potential which scales approximately as rootr. One of the solutions found gives extra deflection of light compared to Newtonian deflection.	en
heal.publisher	AMERICAN PHYSICAL SOC	en
heal.journalName	PHYSICAL REVIEW D	en
dc.identifier.doi	10.1103/PhysRevD.66.104028	en
dc.identifier.isi	ISI:000179679900053	en
dc.identifier.volume	66	en
dc.identifier.issue	10	en