Thin Domain Walls in Lyra Geometry

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dc.creatorRahaman, F.
dc.creatorKalam, M.
dc.creatorMondal, R.
dc.date2006-05-08
dc.date2007-03-07
dc.date.accessioned2026-07-07T10:40:52Z
dc.date.available2026-07-07T10:40:52Z
dc.descriptionThis paper studies thin domain walls within the frame work of Lyra Geometry. We have considered two models. First one is the thin domain wall with negligible pressures perpendicular and transverse direction to the wall and secondly, we take a particular type of thin domain wall where the pressure in the perpendicular direction is negligible but transverse pressures are existed. It is shown that the thin domain walls have no particle horizon and the gravitational force due to them is attractive.
dc.description8 pages, typos are corrected, published Astrophysics and Space Sciences 305, 337 (2006)
dc.identifierhttps://arxiv.org/abs/gr-qc/0605042
dc.identifierhttp://arxiv.org/abs/gr-qc/0605042
dc.identifierAstrophys.SpaceSci.305:337-340,2006
dc.identifierdoi:10.1007/s10509-006-9063-6
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181460
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThin Domain Walls in Lyra Geometry
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