Black hole and thin-shell wormhole solutions in Einstein-Hoffman-Born-Infeld theory

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dc.contributor.authorMazharimousavi, S. Habib
dc.contributor.authorHalilsoy, Mustafa
dc.contributor.authorAmirabi, Zahra
dc.date.accessioned2016-01-20T11:42:40Z
dc.date.available2016-01-20T11:42:40Z
dc.date.issued2009
dc.descriptionThe file in this item is the post-print version of the article (author’s copy; author’s final manuscript, accepted for publication after peer-review process). Due to copyright restrictions, the access to the publisher version (published version) of this article is only available via subscription. You may click URI (with DOI: 10.1016/j.physleta.2011.08.036) and have access to the Publisher Version of this article through the publisher web site or online databases, if your Library or institution has subscription to the related journal or publication.en_US
dc.description.abstractWe employ an old field theory model, formulated and discussed by Born, Infeld, Hoffman and Rosen during 1930s. Our method of cutting-gluing of spacetimes resolves the double-valuedness in the displacement vector D(E), pointed out by these authors. A characteristic feature of their model is to contain a logarithmic term, and by bringing forth such a Lagrangian anew, we aim to attract the interest of field theorists to such a Lagrangian. We adopt the Hoffman-Born-Infeld (HBI) Lagrangian in general relativity to construct black holes and investigate the possibility of viable thin-shell wormholes. In particular, the stability of thin-shell wormholes supported by normal matter in 5-dimensional Einstein-HBI-Gauss-Bonnet gravity is highlighted.en_US
dc.description.versionPost-Print Author Version (Final Author Manuscript, accepted for publication, after peer-review process).
dc.identifier.citationS. Habib Mazharimousavi, Mustafa Halilsoy and Zahra Amirabi, Phys. Lett. A 375 (2011) 3649: "Black hole and thin-shell wormhole solutions in Einstein-Hoffman-Born-Infeld theory."en_US
dc.identifier.doi10.1016/j.physleta.2011.08.036
dc.identifier.issn0375-9601
dc.identifier.otherDOI: 10.1016/j.physleta.2011.08.036
dc.identifier.scopus2-s2.0-80052967107
dc.identifier.scopusqualityQ2
dc.identifier.urihttp://dx.doi.org/10.1016/j.physleta.2011.08.036
dc.identifier.urihttps://hdl.handle.net/11129/2019
dc.identifier.wosWOS:000296043200001
dc.identifier.wosqualityQ2
dc.indekslendigikaynakScopus
dc.indekslendigikaynakWeb of Science
dc.language.isoen
dc.publisherPhysics Letters A, Elsevieren_US
dc.relation.ispartofseriesElsevier;Physics A375:3649-3654,2011
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.subjectwormholesen_US
dc.subjectgeneral relativityen_US
dc.subjectthin-shellsen_US
dc.titleBlack hole and thin-shell wormhole solutions in Einstein-Hoffman-Born-Infeld theoryen_US
dc.typeArticle

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