Bianchi type V and VI0 cosmological models in Lyra geometry

1991 ◽  
Vol 182 (2) ◽  
pp. 189-200 ◽  
Author(s):  
T. Singh ◽  
G. P. Singh
Keyword(s):  
Bianchi Type ◽  
Lyra Geometry ◽  
Cosmological Models ◽  
Type V ◽  
Bianchi Type V

scholarly journals Tilted cosmological models of Bianchi type V

2006 ◽  
Vol 73 (4) ◽  
Author(s):  
Michael Bradley ◽  
Daniel Eriksson
Keyword(s):  
Bianchi Type ◽  
Cosmological Models ◽  
Type V ◽  
Bianchi Type V

scholarly journals Bianchi type-V string cosmological models in general relativity

Pramana ◽  
2011 ◽  
Vol 76 (4) ◽  
pp. 681-690 ◽  
Author(s):  
ANIL KUMAR YADAV ◽  
VINEET KUMAR YADAV ◽  
LALLAN YADAV
Keyword(s):  
General Relativity ◽  
Bianchi Type ◽  
Cosmological Models ◽  
Type V ◽  
Bianchi Type V

Numerical nucleosynthesis results for Bianchi type-V cosmological models

1986 ◽  
Vol 123 (2) ◽  
pp. 411-414 ◽  
Author(s):  
Mark S. Madsen ◽  
D. R. Matravers ◽  
Davin Milun
Keyword(s):  
Bianchi Type ◽  
Cosmological Models ◽  
Type V ◽  
Bianchi Type V

Exact Bianchi type-V perfect fluid cosmological models in Brans–Dicke theory of gravitation

2008 ◽  
Vol 315 (1-4) ◽  
pp. 211-214 ◽  
Author(s):  
V. U. M. Rao ◽  
T. Vinutha ◽  
M. Vijaya Shanthi ◽  
K. V. S. Sireesha
Keyword(s):  
Perfect Fluid ◽  
Bianchi Type ◽  
Cosmological Models ◽  
Theory Of Gravitation ◽  
Type V ◽  
Bianchi Type V

Bianchi type VI cosmological model with electromagnetic field in Lyra geometry

2016 ◽  
Vol 94 (10) ◽  
pp. 992-1000 ◽  
Author(s):  
M. Abdel-Megied ◽  
E.A. Hegazy
Keyword(s):  
Electromagnetic Field ◽  
Cosmological Model ◽  
Bianchi Type ◽  
Lyra Geometry ◽  
Geometrical Properties ◽  
Special Cases ◽  
Type V ◽  
Tensor Formula ◽  
Shear Tensor ◽  
Bianchi Type V

Bianchi type VI cosmological model in the presence of electromagnetic field with variable magnetic permeability in the framework of Lyra geometry is presented. An exact solution is introduced by considering that the eigenvalue [Formula: see text] of the shear tensor [Formula: see text] is proportional to the scalar expansion Θ of the model, that is, C = (AB)L, where A, B, and C are the coefficients of the metric and L is a constant. Bianchi type V, III, and I cosmological models are given as special cases of Bianchi type VI. Physical and geometrical properties of the models are discussed.

SOME BIANCHI TYPE-V COSMOLOGICAL MODELS IN BRANS–DICKE THEORY

2010 ◽  
Vol 25 (18n19) ◽  
pp. 3817-3824 ◽  
Author(s):  
J. K. SINGH
Keyword(s):  
Magnetic Field ◽  
Bianchi Type ◽  
Cosmological Models ◽  
Energy Conditions ◽  
Type V ◽  
The Magnetic Field ◽  
Bianchi Type V

The Bianchi type-V cosmological models have been investigated in the context of Brans–Dicke theory in the presence as well as absence of the magnetic field. The physical and kinematical behaviors of the models have been discussed. The energy conditions of the models have also been examined.

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