Q-stars in 2+1 dimensions

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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 0550-3213 en
dc.identifier.uri http://hdl.handle.net/123456789/16176
dc.subject Analytic Solution en
dc.subject Gravitational Collapse en
dc.subject Scalar Field en
dc.subject Anti De Sitter en
dc.subject.classification Physics, Particles & Fields en
dc.subject.other BOSON STARS en
dc.subject.other Q-BALLS en
dc.subject.other SOLITON STARS en
dc.subject.other EQUILIBRIUM en
dc.subject.other STABILITY en
dc.subject.other DYNAMICS en
dc.subject.other EQUATION en
dc.subject.other GRAVITY en
dc.subject.other GEON en
dc.title Q-stars in 2+1 dimensions en
heal.type journalArticle en
heal.identifier.primary 10.1016/j.nuclphysb.2004.05.005 en
heal.identifier.secondary http://dx.doi.org/10.1016/j.nuclphysb.2004.05.005 en
heal.language English en
heal.publicationDate 2004 en
heal.abstract We study q-stars with one or two scalar fields, non-Abelian, and fermion-scalar q-stars in 2 + 1 dimensions in an anti-de Sitter or flat spacetime. We fully investigate their properties, such as mass, particle number, radius, numerically, and focus on the matter of their stability against decay to free particles and gravitational collapse. We also provide analytical solutions in the case of flat spacetime and other special cases. (C) 2004 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.2004.05.005 en
dc.identifier.isi ISI:000222337700001 en
dc.identifier.volume 690 en
dc.identifier.issue 3 en
dc.identifier.spage 201 en
dc.identifier.epage 229 en

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