THE BIANCHI TYPE V MAGNETIZED STRING DUST COSMOLOGICAL MODEL IN GENERAL RELATIVITY
2007 ◽
Vol 16
(11)
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pp. 1769-1781
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Keyword(s):
Type V
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The Bianchi type V magnetized string dust cosmological model for perfect fluid distribution is investigated. We assume that the magnetic field is along the x direction, so F23 is the only nonvanishing component of Fij. We also find that F14 = 0 = F24 = F34 due to the assumption of infinite electrical conductivity. The behavior of the model in the presence and the absence of a magnetic field is also discussed.
2007 ◽
Vol 5
(1)
◽
pp. 79-84
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1985 ◽
Vol 108
(1)
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pp. 195-201
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Keyword(s):