Bianchi Type-V Magnetized String Cosmological Model with Variable Magnetic Permeability for Viscous Fluid distribution

2010 ◽  
Vol 27 (8) ◽  
pp. 089801
Author(s):  
Atul Tyagi ◽  
Keerti Sharma
Keyword(s):  
Cosmological Model ◽  
Viscous Fluid ◽  
Magnetic Permeability ◽  
Bianchi Type ◽  
Fluid Distribution ◽  
String Cosmological Model ◽  
Type V ◽  
Bianchi Type V ◽  
Variable Magnetic Permeability

THE BIANCHI TYPE V MAGNETIZED STRING DUST COSMOLOGICAL MODEL IN GENERAL RELATIVITY

2007 ◽  
Vol 16 (11) ◽  
pp. 1769-1781 ◽  
Author(s):  
RAJ BALI ◽  
SHILPI JAIN
Keyword(s):  
Magnetic Field ◽  
Electrical Conductivity ◽  
General Relativity ◽  
Cosmological Model ◽  
Bianchi Type ◽  
Fluid Distribution ◽  
Type V ◽  
The Magnetic Field ◽  
Bianchi Type V ◽  
Nonvanishing Component

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.

Bianchi type-V bulk viscous string cosmological model in f(R,T) gravity

2013 ◽  
Vol 348 (1) ◽  
pp. 247-252 ◽  
Author(s):  
R. L. Naidu ◽  
D. R. K. Reddy ◽  
T. Ramprasad ◽  
K. V. Ramana
Keyword(s):  
Cosmological Model ◽  
Bianchi Type ◽  
String Cosmological Model ◽  
Bulk Viscous ◽  
Type V ◽  
Bianchi Type V
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