Q-stars in anti de Sitter spacetime

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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 http://hdl.handle.net/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.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

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