Thin shell wormhole due to dyadosphere of a charged black hole

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dc.creatorRahaman, F.
dc.creatorKalam, M.
dc.creatorRahman, K A
dc.date2008-06-09
dc.date.accessioned2026-07-07T12:39:06Z
dc.date.available2026-07-07T12:39:06Z
dc.descriptionTo explain Gamma Ray Bursts, Ruffini argued that the event horizon of a charged black hole is surrounded by a special region called, the Dyadosphere where electric field exceeds the critical value for $e^+$ $e^-$ pair production. In the present work, we construct a thin shell wormhole by performing a thought surgery between two dadospheres. Several physical properties of this thin shell wormhole have been analyzed.
dc.description10 pages, 2 figures. Accepted in Mod.Phys.Lett.A
dc.identifierhttps://arxiv.org/abs/0806.1391
dc.identifierhttp://arxiv.org/abs/0806.1391
dc.identifierMod.Phys.Lett.A24:53-61,2009
dc.identifierdoi:10.1142/S0217732309027406
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/218990
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThin shell wormhole due to dyadosphere of a charged black hole
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