dc.creatorLemos JosP.S.
dc.creatorLetelier P.S.
dc.date1991
dc.date2015-06-30T14:09:33Z
dc.date2015-11-26T14:41:45Z
dc.date2015-06-30T14:09:33Z
dc.date2015-11-26T14:41:45Z
dc.date.accessioned2018-03-28T21:48:56Z
dc.date.available2018-03-28T21:48:56Z
dc.identifier
dc.identifierPhysics Letters A. , v. 153, n. 6-7, p. 288 - 290, 1991.
dc.identifier3759601
dc.identifier10.1016/0375-9601(91)90945-5
dc.identifierhttp://www.scopus.com/inward/record.url?eid=2-s2.0-0011352076&partnerID=40&md5=2794ca5fd1ccec344a3a96015678b9b3
dc.identifierhttp://www.repositorio.unicamp.br/handle/REPOSIP/99207
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/99207
dc.identifier2-s2.0-0011352076
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1250987
dc.descriptionA family of solutions of the Einstein equation that represents topological defects with the symmetry of a disk is exhibited. The possibility that this family may be originated from the gravitational collapse of a cloud of particles is considered. © 1991.
dc.description153
dc.description6-7
dc.description288
dc.description290
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dc.languageen
dc.publisher
dc.relationPhysics Letters A
dc.rightsfechado
dc.sourceScopus
dc.titleTopological Defects From Counter Rotating Disks
dc.typeArtículos de revistas


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