Type 0 brane inflation from mirage cosmology

Papantonopoulos, E; Pappa, I

dc.contributor.author	Papantonopoulos, E	en
dc.contributor.author	Pappa, I	en
dc.date.accessioned	2014-03-01T01:15:57Z
dc.date.available	2014-03-01T01:15:57Z
dc.date.issued	2000	en
dc.identifier.issn	0217-7323	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/13847
dc.subject	Three Dimensional	en
dc.subject.classification	Physics, Nuclear	en
dc.subject.classification	Physics, Particles & Fields	en
dc.subject.classification	Physics, Mathematical	en
dc.subject.other	3-BRANE UNIVERSE	en
dc.subject.other	DIMENSIONS	en
dc.subject.other	TACHYON	en
dc.subject.other	MILLIMETER	en
dc.subject.other	GRAVITY	en
dc.subject.other	TEV	en
dc.title	Type 0 brane inflation from mirage cosmology	en
heal.type	journalArticle	en
heal.identifier.primary	10.1142/S0217732300002784	en
heal.identifier.secondary	http://dx.doi.org/10.1142/S0217732300002784	en
heal.language	English	en
heal.publicationDate	2000	en
heal.abstract	We consider a three-dimensional brane-universe moving in a type 0 string background. The motion induces on the brans a cosmological evolution which, for some range of the parameters, exhibits an inflationary phase.	en
heal.publisher	WORLD SCIENTIFIC PUBL CO PTE LTD	en
heal.journalName	MODERN PHYSICS LETTERS A	en
dc.identifier.doi	10.1142/S0217732300002784	en
dc.identifier.isi	ISI:000166509500003	en
dc.identifier.volume	15	en
dc.identifier.issue	35	en
dc.identifier.spage	2145	en
dc.identifier.epage	2152	en