Q-stars in anti de Sitter spacetime

Prikas, A

dc.contributor.author	Prikas, A	en
dc.date.accessioned	2014-03-01T01:21:16Z
dc.date.available	2014-03-01T01:21:16Z
dc.date.issued	2004	en
dc.identifier.issn	0001-7701	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/16177
dc.subject	Anti de Sitter spacetime	en
dc.subject	non-topological solitons	en
dc.subject	Q stars	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.classification	Physics, Multidisciplinary	en
dc.subject.classification	Physics, Particles & Fields	en
dc.subject.other	Q-BALLS	en
dc.subject.other	BOSON STARS	en
dc.subject.other	EQUATION	en
dc.subject.other	GEON	en
dc.title	Q-stars in anti de Sitter spacetime	en
heal.type	journalArticle	en
heal.identifier.primary	10.1023/B:GERG.0000035955.07614.0d	en
heal.identifier.secondary	http://dx.doi.org/10.1023/B:GERG.0000035955.07614.0d	en
heal.language	English	en
heal.publicationDate	2004	en
heal.abstract	We study q-stars with various symmetries in anti de Sitter spacetime in 3 + 1 dimensions. Comparing with the case of flat spacetime, we find that the value of the field at the center of the soliton is larger when the other parameters show a more complicated behavior. We also investigate their phase space when the symmetry is local and the effect of the charge to its stability.	en
heal.publisher	KLUWER ACADEMIC/PLENUM PUBL	en
heal.journalName	General Relativity and Gravitation	en
dc.identifier.doi	10.1023/B:GERG.0000035955.07614.0d	en
dc.identifier.isi	ISI:000222943800007	en
dc.identifier.volume	36	en
dc.identifier.issue	8	en
dc.identifier.spage	1841	en
dc.identifier.epage	1869	en