Spherically symmetric braneworld solutions with an(4)R term in the bulk

Kofinas, G; Papantonopoulos, E; Pappa, I

dc.contributor.author	Kofinas, G	en
dc.contributor.author	Papantonopoulos, E	en
dc.contributor.author	Pappa, I	en
dc.date.accessioned	2014-03-01T01:18:21Z
dc.date.available	2014-03-01T01:18:21Z
dc.date.issued	2002	en
dc.identifier.issn	0556-2821	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/14954
dc.subject	Boundary Condition	en
dc.subject	Solar System	en
dc.subject	Upper Bound	en
dc.subject	Vanishing of	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.classification	Physics, Particles & Fields	en
dc.subject.other	INDUCED GRAVITATIONAL CONSTANT	en
dc.subject.other	CONFORMAL WEYL GRAVITY	en
dc.subject.other	WORLD BLACK-HOLES	en
dc.subject.other	DE-SITTER SPACE	en
dc.subject.other	3-BRANE WORLD	en
dc.subject.other	DOMAIN-WALLS	en
dc.subject.other	FIELD THEORY	en
dc.subject.other	BRIGHT SIDE	en
dc.subject.other	DARK-MATTER	en
dc.subject.other	COMPACTIFICATION	en
dc.title	Spherically symmetric braneworld solutions with an(4)R term in the bulk	en
heal.type	journalArticle	en
heal.identifier.primary	10.1103/PhysRevD.66.104014	en
heal.identifier.secondary	104014	en
heal.identifier.secondary	http://dx.doi.org/10.1103/PhysRevD.66.104014	en
heal.language	English	en
heal.publicationDate	2002	en
heal.abstract	An analysis of a spherically symmetric braneworld configuration is performed when the intrinsic curvature scalar is included in the bulk action; the vanishing of the electric part of the Weyl tensor is used as the boundary condition for the embedding of the brane in the bulk. All the solutions outside a static localized matter distribution are found; some of them are of the Schwarzschild-(A)dS4 form. Two modified Oppenheimer-Volkoff interior solutions are also found; one is matched to a Schwarzschild-(A)dS4 exterior, while the other is not. A nonuniversal gravitational constant arises, depending on the density of the considered object; however, the conventional limits of Newton's constant are recovered. An upper bound of the order of TeV for the energy string scale is extracted from the known solar system measurements (experiments). On the contrary, in the usual brane dynamics, this string scale is calculated to be larger than TeV. © 2002 The American Physical Society.	en
heal.publisher	AMERICAN PHYSICAL SOC	en
heal.journalName	Physical Review D	en
dc.identifier.doi	10.1103/PhysRevD.66.104014	en
dc.identifier.isi	ISI:000179679900039	en
dc.identifier.volume	66	en
dc.identifier.issue	10	en