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dc.creatorVasilic, M
dc.creatorVukasinac, T
dc.date.accessioned2018-03-03T15:12:18Z
dc.date.available2018-03-03T15:12:18Z
dc.date.issued1997
dc.identifier.issn0550-3213 (print)
dc.identifier.urihttp://vinar.vin.bg.ac.rs/handle/123456789/7236
dc.description.abstractThe exsistence of gravitational kinks in 2d dilaton gravity, for topologically trivial spacetimes, is analysed. Hamiltonian analysis shows that such configurations are allowed, at least in a finite interval of time, provided some appropriate initial conditions are chosen. Investigation of the stationary case gives the conditions which the potential of the dilaton field has to satisfy in order that the theory admits gravitational kink solutions. As a special example, flat gravitational kinks are considered.en
dc.rightsrestrictedAccessen
dc.sourceNuclear Physics Ben
dc.titleGravitational kinks in 2d dilaton gravityen
dc.typearticleen
dcterms.abstractВасилиц, М; Вукасинац, Т;
dc.citation.spage334
dc.citation.epage337
dc.identifier.wosA1997XN29400059
dc.identifier.doi10.1016/S0920-5632(97)00375-7
dc.citation.otherSuppl: 57B
dc.description.other2nd Meeting on Constrained Dynamics and Quantum Gravity (QG96), Sep 17-21, 1996, Santa Margherita, Italyen


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