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Graviton localization and Newton law for a dS4 brane in a 5D bulk

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dc.contributor.author Kehagias, A en
dc.contributor.author Tamvakis, K en
dc.date.accessioned 2014-03-01T01:17:56Z
dc.date.available 2014-03-01T01:17:56Z
dc.date.issued 2002 en
dc.identifier.issn 0264-9381 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/14716
dc.subject.classification Astronomy & Astrophysics en
dc.subject.classification Physics, Multidisciplinary en
dc.subject.classification Physics, Particles & Fields en
dc.subject.other PERTURBATIVE QUANTUM-GRAVITY en
dc.subject.other VACUUM DOMAIN-WALLS en
dc.subject.other COSMOLOGICAL CONSTANT en
dc.subject.other EXTRA DIMENSION en
dc.subject.other HIERARCHY en
dc.subject.other COMPACTIFICATION en
dc.subject.other MILLIMETER en
dc.subject.other SPACETIME en
dc.subject.other INFLATION en
dc.subject.other FIELD en
dc.title Graviton localization and Newton law for a dS4 brane in a 5D bulk en
heal.type journalArticle en
heal.identifier.primary 10.1088/0264-9381/19/18/101 en
heal.identifier.secondary http://dx.doi.org/10.1088/0264-9381/19/18/101 en
heal.language English en
heal.publicationDate 2002 en
heal.abstract We consider a dS(4) brane embedded in a five-dimensional bulk with a positive, vanishing or negative bulk cosmological constant and derive the localized graviton spectrum that consists of a normalizable zero mode separated by a gap from a continuum of massive states. We estimate the massive sector contribution to the static potential at short distances and find that only in the case of a negative bulk cosmological constant is there a range, determined by the effective four-dimensional and bulk cosmological constants, where the conventional Newton law is valid. en
heal.publisher IOP PUBLISHING LTD en
heal.journalName Classical and Quantum Gravity en
dc.identifier.doi 10.1088/0264-9381/19/18/101 en
dc.identifier.isi ISI:000178687100001 en
dc.identifier.volume 19 en
dc.identifier.issue 18 en
dc.identifier.spage L185 en
dc.identifier.epage L192 en


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