HEAL DSpace

Induced cosmology on a regularized brane in six-dimensional flux compactification

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dc.contributor.author Papantonopoulos, E en
dc.contributor.author Papazoglou, A en
dc.contributor.author Zamarias, V en
dc.date.accessioned 2014-03-01T01:28:41Z
dc.date.available 2014-03-01T01:28:41Z
dc.date.issued 2008 en
dc.identifier.issn 0550-3213 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/18912
dc.subject Cosmology with extra dimensions en
dc.subject Extra dimensions en
dc.subject.classification Physics, Particles & Fields en
dc.subject.other CONSTANT PROBLEM en
dc.subject.other 6 DIMENSIONS en
dc.subject.other SUPERGRAVITY en
dc.subject.other VACUUM en
dc.subject.other MILLIMETER en
dc.subject.other UNIVERSE en
dc.title Induced cosmology on a regularized brane in six-dimensional flux compactification en
heal.type journalArticle en
heal.identifier.primary 10.1016/j.nuclphysb.2007.12.031 en
heal.identifier.secondary http://dx.doi.org/10.1016/j.nuclphysb.2007.12.031 en
heal.language English en
heal.publicationDate 2008 en
heal.abstract We consider a six-dimensional Einstein-Maxwell system compactified in an axisymmetric two-dimensional space with one capped regularized conical brane of codimension one. We study the cosmological evolution which is induced on the regularized brane as it moves in between known static bulk and cap solutions. Looking at the resulting Friedmann equation, we see that the brane cosmology at high energies is dominated by a five-dimensional rho(2) energy density term. At low energies, we obtain a Friedmann equation with a term linear to the energy density with, however, negative coefficient in the small four-brane radius limit (i.e., with negative effective Newton's constant). We discuss ways out of this problem. (C) 2008 Elsevier B.V. All rights reserved. en
heal.publisher ELSEVIER SCIENCE BV en
heal.journalName Nuclear Physics B en
dc.identifier.doi 10.1016/j.nuclphysb.2007.12.031 en
dc.identifier.isi ISI:000255556200006 en
dc.identifier.volume 797 en
dc.identifier.issue 3 en
dc.identifier.spage 520 en
dc.identifier.epage 536 en


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