Bianchi Type I Massive String Magnetized Barotropic Perfect Fluid Cosmological Model in General Relativity

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dc.creatorBali, Raj
dc.creatorPareek, Umesh Kumar
dc.creatorPradhan, Anirudh
dc.date2007-04-05
dc.date2007-06-25
dc.date.accessioned2026-07-07T11:20:10Z
dc.date.available2026-07-07T11:20:10Z
dc.descriptionBianchi type I massive string cosmological model with magnetic field of barotropic perfect fluid distribution through the techniques used by Latelier and Stachel, is investigated. To get the deterministic model of the universe, it is assumed that the universe is filled with barotropic perfect fluid distribution. The magnetic field is due to electric current produced along x-axis with infinite electrical conductivity. The behaviour of the model in presence and absence of magnetic field together with other physical aspects is further discussed.
dc.description10 pages, no figure. Chin. Phys. Lett., Vol. 24, No. 8 (2007), to appear
dc.identifierhttps://arxiv.org/abs/0704.0753
dc.identifierhttp://arxiv.org/abs/0704.0753
dc.identifierChin.Phys.Lett.24:2455-2458,2007
dc.identifierdoi:10.1088/0256-307X/24/8/082
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193877
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBianchi Type I Massive String Magnetized Barotropic Perfect Fluid Cosmological Model in General Relativity
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