scholarly journals Viscous Fluid Bianchi Type V Cosmological Models with Late Time Acceleration

2016 ◽  
Vol 1 (3) ◽  
Author(s):  
J. P. Singh ◽  
◽  
Prashant S. Baghel ◽  
Abhay Singh ◽  
◽  
...  
Keyword(s):  
Viscous Fluid ◽  
Bianchi Type ◽  
Cosmological Models ◽  
Late Time ◽  
Late Time Acceleration ◽  
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

scholarly journals Chaotic inflation in spatially homogeneous Bianchi type V space–time

2017 ◽  
Vol 95 (12) ◽  
pp. 1267-1270
Author(s):  
Raj Bali ◽  
P. Kumari
Keyword(s):  
Bianchi Type ◽  
Space Time ◽  
Late Time ◽  
De Sitter ◽  
Spatially Homogeneous ◽  
Inflationary Parameters ◽  
Type V ◽  
The Universe ◽  
Anisotropic Phase ◽  
Bianchi Type V

Chaotic inflationary scenario in spatially homogeneous Bianchi type V space–time following Linde (Phys. Lett. B, 129, 177 (1983). doi: 10.1016/0370-2693(83)90837-7 ) and the condition [Formula: see text] based on theory of super cooling during the cosmological phase transition proposed by Kirzhnits and Linde (Ann. Phys. 101, 195 (1976). doi: 10.1016/0003-4916(76)90279-7 ), is discussed. It has been found that the model represents anisotropic phase of the Universe in general but at late time, it isotropizes. The deceleration parameter q = −1 indicates that the model leads to de Sitter space–time. It is found that inflationary parameters, namely, slow roll parameters, and anisotropic parameters are in excellent agreement with the Planck Collaboration’s 2013 results (Astron. Astrophys. 571, A22 (2014). doi: 10.1051/0004-6361/201321569 ).

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