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dc.contributor.authorSean A. Hayward-
dc.date.accessioned2016-08-28T11:08:45Z-
dc.date.available2016-08-28T11:08:45Z-
dc.date.issued2004-
dc.identifier.issn0556-2821-
dc.identifier.otherOAK-2429-
dc.identifier.urihttps://dspace.ewha.ac.kr/handle/2015.oak/219487-
dc.description.abstractAnalytic solutions are presented which describe the construction of a traversable wormhole from a Schwarzschild black hole, and the enlargement of such a wormhole, in Einstein gravity. The matter model is pure radiation which may have negative-energy density (phantom or ghost radiation) and the idealization of impulsive radiation (infinitesimally thin null shells) is employed.-
dc.languageEnglish-
dc.titleConstruction and enlargement of traversable wormholes from Schwarzschild black holes-
dc.typeArticle-
dc.relation.issue8-
dc.relation.volume70-
dc.relation.indexSCOPUS-
dc.relation.startpage84001-
dc.relation.lastpage1-084001-10-
dc.relation.journaltitlePhysical Review D - Particles, Fields, Gravitation and Cosmology-
dc.identifier.doi10.1103/PhysRevD.70.084001-
dc.identifier.wosidWOS:000224800000054-
dc.identifier.scopusid2-s2.0-19744381713-
dc.author.googleKoyama H.-
dc.author.googleHayward S.A.-
dc.contributor.scopusidSean A. Hayward(7102776215)-
dc.date.modifydate20211210152206-


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