Cosmological Evolution in a Type0 String Theory

Diamandis, G; Georgalas, B; Mavromatos, N; Papantonopoulos, E; Pappa, I

dc.contributor.author	Diamandis, G	en
dc.contributor.author	Georgalas, B	en
dc.contributor.author	Mavromatos, N	en
dc.contributor.author	Papantonopoulos, E	en
dc.contributor.author	Pappa, I	en
dc.date.accessioned	2014-03-01T01:50:43Z
dc.date.available	2014-03-01T01:50:43Z
dc.date.issued	2001	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/26086
dc.subject	Brane World	en
dc.subject	Extra Dimension	en
dc.subject	Sigma Model	en
dc.subject	String Theory	en
dc.subject	Time Dependent	en
dc.title	Cosmological Evolution in a Type0 String Theory	en
heal.type	journalArticle	en
heal.identifier.primary	10.1142/S0217751X02010534	en
heal.identifier.secondary	http://dx.doi.org/10.1142/S0217751X02010534	en
heal.publicationDate	2001	en
heal.abstract	We study the cosmological evolution of a type-0 string theory by employingnon-criticality, which may be induced by fluctuations of the D3 brane worlds.We check the consistency of the approach to O(alpha ') in the correspondingsigma-model. The ten-dimensional theory is reduced to an effectivefour-dimensional model, with only time dependent fields. We show that thefour-dimensional universe has	en
dc.identifier.doi	10.1142/S0217751X02010534	en