Bianchi Type-I Massive String Magnetized Barotropic Perfect Fluid Cosmological Model in General Relativity
-
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.
Article Text
-
-
-
About This Article
Cite this article:
BALI Raj, PAREEK Umesh Kumar, PRADHAN Anirudh. Bianchi Type-I Massive String Magnetized Barotropic Perfect Fluid Cosmological Model in General Relativity[J]. Chin. Phys. Lett., 2007, 24(8): 2455-2458.
BALI Raj, PAREEK Umesh Kumar, PRADHAN Anirudh. Bianchi Type-I Massive String Magnetized Barotropic Perfect Fluid Cosmological Model in General Relativity[J]. Chin. Phys. Lett., 2007, 24(8): 2455-2458.
|
BALI Raj, PAREEK Umesh Kumar, PRADHAN Anirudh. Bianchi Type-I Massive String Magnetized Barotropic Perfect Fluid Cosmological Model in General Relativity[J]. Chin. Phys. Lett., 2007, 24(8): 2455-2458.
BALI Raj, PAREEK Umesh Kumar, PRADHAN Anirudh. Bianchi Type-I Massive String Magnetized Barotropic Perfect Fluid Cosmological Model in General Relativity[J]. Chin. Phys. Lett., 2007, 24(8): 2455-2458.
|