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dc.creatorVasilić, Milovan
dc.creatorVukašinac, Tatjana
dc.date.accessioned2018-03-01T18:52:15Z
dc.date.available2018-03-01T18:52:15Z
dc.date.issued2000
dc.identifier.issn0001-7701
dc.identifier.urihttps://vinar.vin.bg.ac.rs/handle/123456789/2359
dc.description.abstractGeometric sigma-models have been defined as purely geometric theories of scalar fields in interaction with gravity. By construction, these theories possess soliton solutions with topologically nontrivial scalar sectors. We perform a detailed analysis of the stability of the effective scalar field theory far from the soliton core. It is shown that the requirement for the asymptotic stability is consistent with the existence of massive, static, spherically symmetric soliton solutions.en
dc.rightsrestrictedAccessen
dc.sourceGeneral Relativity and Gravitationen
dc.subjecteffective scalar field theoryen
dc.titleAsymptotic stability in geometric sigma-modelsen
dc.typearticleen
dcterms.abstractВасилиц, М; Вукасинац, Т;
dc.citation.volume32
dc.citation.issue5
dc.citation.spage841
dc.citation.epage856
dc.identifier.wos000088084900003
dc.identifier.doi10.1023/A:1001928906663
dc.citation.rankM22
dc.identifier.scopus2-s2.0-0034349265


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