Bianchi Type-I Massive String Magnetized Barotropic Perfect Fluid Cosmological Model in General Relativity
BALI Raj1, PAREEK Umesh Kumar2, PRADHAN Anirudh3
1Department of Mathematics, University of Rajasthan, Jaipur-302 004, India2Department of Mathematics, Jaipur Engineering College and Research Centre, Jaipur-303 905, India3Department of Mathematics, Hindu Post-graduate College, Zamania-232 331, Ghazipur, India
Bianchi Type-I Massive String Magnetized Barotropic Perfect Fluid Cosmological Model in General Relativity
BALI Raj1;PAREEK Umesh Kumar2;PRADHAN Anirudh3
1Department of Mathematics, University of Rajasthan, Jaipur-302 004, India2Department of Mathematics, Jaipur Engineering College and Research Centre, Jaipur-303 905, India3Department of Mathematics, Hindu Post-graduate College, Zamania-232 331, Ghazipur, India
摘要Bianchi 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 obtain 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 the x-axis with infinite electrical conductivity. The behaviour of the model in the presence and absence of magnetic field together with other physical aspects is further discussed.
Abstract：Bianchi 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 obtain 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 the x-axis with infinite electrical conductivity. The behaviour of the model in the presence and absence of magnetic field together with other physical aspects is further discussed.
(Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.))
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2007, Vol. 24 
