Wormholes in Einstein-Born-Infeld theory

dc.creatorRicharte, Martín Gustavo
dc.creatorSimeone, Claudio Mauricio
dc.date.accessioned2018-09-26T17:09:26Z
dc.date.available2018-09-26T17:09:26Z
dc.date.created2018-09-26T17:09:26Z
dc.date.issued2009-11
dc.identifierRicharte, Martín Gustavo; Simeone, Claudio Mauricio; Wormholes in Einstein-Born-Infeld theory; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 80; 10; 11-2009; 104033-104040
dc.identifier1550-7998
dc.identifierhttp://hdl.handle.net/11336/60899
dc.identifierCONICET Digital
dc.identifierCONICET
dc.description.abstractSpherically symmetric thin-shell wormholes are studied within the framework of Einstein-Born-Infeld theory. We analyze the exotic matter content, and find that for certain values of the Born-Infeld parameter the amount of exotic matter on the shell can be reduced in relation to the Maxwell case. We also examine the mechanical stability of the wormhole configurations under radial perturbations preserving the spherical symmetry. In addition, in the Appendix the repulsive or attractive character of the wormhole geometries is briefly discussed. © 2009 The American Physical Society.
dc.languageeng
dc.publisherAmerican Physical Society
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://link.aps.org/doi/10.1103/PhysRevD.80.104033
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1103/PhysRevD.80.104033
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectWormholes
dc.subjectBorn-Infeld Theory
dc.subjectStability
dc.titleWormholes in Einstein-Born-Infeld theory
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion


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