dc.contributor.author |
Farakos, K |
en |
dc.contributor.author |
Koutsoumbas, G |
en |
dc.contributor.author |
Pasipoularides, P |
en |
dc.date.accessioned |
2014-03-01T01:26:24Z |
|
dc.date.available |
2014-03-01T01:26:24Z |
|
dc.date.issued |
2007 |
en |
dc.identifier.issn |
1550-7998 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/18066 |
|
dc.subject |
Brane World |
en |
dc.subject |
Einstein Equation |
en |
dc.subject |
General Relativity |
en |
dc.subject |
Parameter Space |
en |
dc.subject |
Scalar Field |
en |
dc.subject |
Spectrum |
en |
dc.subject |
Zero Mode |
en |
dc.subject.classification |
Astronomy & Astrophysics |
en |
dc.subject.classification |
Physics, Particles & Fields |
en |
dc.subject.other |
COSMOLOGICAL CONSTANT PROBLEM |
en |
dc.subject.other |
EXTRA DIMENSION |
en |
dc.subject.other |
STRING ACTION |
en |
dc.subject.other |
DOMAIN-WALL |
en |
dc.subject.other |
WORLD |
en |
dc.subject.other |
MILLIMETER |
en |
dc.subject.other |
HIERARCHY |
en |
dc.title |
Graviton localization and Newton's law for brane models with a nonminimally coupled bulk scalar field |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1103/PhysRevD.76.064025 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1103/PhysRevD.76.064025 |
en |
heal.identifier.secondary |
064025 |
en |
heal.language |
English |
en |
heal.publicationDate |
2007 |
en |
heal.abstract |
Brane world models with a nonminimally coupled bulk scalar field have been studied recently. In this paper we consider metric fluctuations around an arbitrary gravity-scalar background solution, and we show that the corresponding spectrum includes a localized zero mode which strongly depends on the profile of the background scalar field. For a special class of solutions, with a warp factor of the RS form, we solve the linearized Einstein equations, for a pointlike mass source on the brane, by using the brane bending formalism. We see that general relativity on the brane is recovered only if we impose restrictions on the parameter space of the models under consideration. © 2007 The American Physical Society. |
en |
heal.publisher |
AMER PHYSICAL SOC |
en |
heal.journalName |
Physical Review D - Particles, Fields, Gravitation and Cosmology |
en |
dc.identifier.doi |
10.1103/PhysRevD.76.064025 |
en |
dc.identifier.isi |
ISI:000249786900063 |
en |
dc.identifier.volume |
76 |
en |
dc.identifier.issue |
6 |
en |