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dc.creatorVasilic, M
dc.creatorVukasinac, T
dc.date.accessioned2018-03-01T18:14:22Z
dc.date.available2018-03-01T18:14:22Z
dc.date.issued1996
dc.identifier.issn0264-9381 (print)
dc.identifier.urihttp://vinar.vin.bg.ac.rs/handle/123456789/1999
dc.description.abstractThe properties of gravitational kinks are studied within some simple models of two-dimensional gravity. In spacetimes of cylindrical topology we prove the existence of kinks of constant curvature with arbitrary kink numbers. In R(1) x R(1) spacetimes m = 1 kink solutions of the equation R = 0 are found, whereas \m\ GT 1 flat kinks are proved not to exist. We give a detailed analysis of the behaviour of gravitational kinks under coordinate transformations. Viewed as nonsingular black holes \m\ GT 1 kink solutions are found within a simple dilaton gravity theory. The general form of the potential function is determined from the demand that the theory possesses an arbitrary number of inequivalent kink configurations.en
dc.rightsrestrictedAccessen
dc.sourceClassical and Quantum Gravityen
dc.titleGravitational kinks in two spacetime dimensionsen
dc.typearticleen
dcterms.abstractВасилиц, М; Вукасинац, Т;
dc.citation.volume13
dc.citation.issue7
dc.citation.spage1995
dc.citation.epage2005
dc.identifier.wosA1996UZ31500024
dc.identifier.doi10.1088/0264-9381/13/7/024
dc.identifier.scopus2-s2.0-21344434521


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