Dynamics of curved gravitating walls

dc.creatorBonjour, F
dc.creatorCharmousis, C
dc.creatorGregory, R
dc.date2000
dc.dateOCT 15
dc.date2014-12-02T16:31:12Z
dc.date2015-11-26T16:46:05Z
dc.date2014-12-02T16:31:12Z
dc.date2015-11-26T16:46:05Z
dc.date.accessioned2018-03-28T23:31:50Z
dc.date.available2018-03-28T23:31:50Z
dc.identifierPhysical Review D. American Physical Soc, v. 62, n. 8, 2000.
dc.identifier0556-2821
dc.identifierWOS:000089977200012
dc.identifier10.1103/PhysRevD.62.083504
dc.identifierhttp://www.repositorio.unicamp.br/jspui/handle/REPOSIP/63612
dc.identifierhttp://www.repositorio.unicamp.br/handle/REPOSIP/63612
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/63612
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1274423
dc.descriptionWe examine the dynamics of a self-gravitating domain wall using the lambda Phi (4) model as a specific example. We find that the Nambu motion of the wall is quite generic and dominates the wall motion even in the presence of gravity. We calculate the corrections to this leading order motion, and estimate the effect of the inclusion of gravity on the dynamics of the wall. We then treat the case of a spherical gravitating thick wall as a particular example, solving the field equations and calculating che corrections to the Nambu motion analytically for this specific case. We find that the presence of gravity retards collapse in this case.
dc.description62
dc.description8
dc.languageen
dc.publisherAmerican Physical Soc
dc.publisherCollege Pk
dc.publisherEUA
dc.relationPhysical Review D
dc.relationPhys. Rev. D
dc.rightsaberto
dc.sourceWeb of Science
dc.subjectCosmic Structure Formation
dc.subjectRelativistic Domain-walls
dc.subjectCurvature Corrections
dc.subjectGeneral-relativity
dc.subjectExtra Dimension
dc.subjectStrings
dc.subjectBubbles
dc.subjectWaves
dc.titleDynamics of curved gravitating walls
dc.typeArtículos de revistas


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