Some new class of Chaplygin Wormholes

dc.creatorRahaman, F.
dc.creatorKalam, M.
dc.creatorRahman, K. A.
dc.date2007-09-20
dc.date.accessioned2026-07-07T11:53:11Z
dc.date.available2026-07-07T11:53:11Z
dc.descriptionSome new class of Chaplygin wormholes are investigated in the framework of a Chaplygin gas with equation of state $ p = - \frac{A}ρ$, $A>0$. Since empty spacetime ($ p = ρ= 0 $) does not follow Chaplygin gas, so the interior Chaplygin wormhole solutions will never asymptotically flat. For this reason, we have to match our interior wormhole solution with an exterior vacuum solution i.e. Schwarzschild solution at some junction interface, say $ r = a $. We also discuss the total amount of matter characterized by Chaplygin gas that supplies fuel to construct a wormhole.
dc.description14 pages, 12 figures, Accepted for publication in Mod.Phys.Lett.A
dc.identifierhttps://arxiv.org/abs/0709.3162
dc.identifierhttp://arxiv.org/abs/0709.3162
dc.identifierMod.Phys.Lett.A23:1199-1211,2008
dc.identifierdoi:10.1142/S0217732308025772
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/204451
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSome new class of Chaplygin Wormholes
dc.typetext

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