Bianchi Type VI0 Cosmological Models with Perfect Fluid and Dark Energy

2011 ◽  
Vol 50 (11) ◽  
pp. 3299-3312 ◽  
Author(s):  
S. D. Katore ◽  
D. V. Kapse ◽  
G. B. Tayade
2010 ◽  
Vol 332 (2) ◽  
pp. 497-502 ◽  
Author(s):  
K. S. Adhav ◽  
A. S. Bansod ◽  
S. L. Munde ◽  
R. G. Nakwal

2011 ◽  
Vol 50 (8) ◽  
pp. 2573-2581 ◽  
Author(s):  
K. S. Adhav ◽  
A. S. Bansod ◽  
S. L. Munde ◽  
M. S. Desale

2013 ◽  
Vol 2013 ◽  
pp. 1-11
Author(s):  
V. U. M. Rao ◽  
K. V. S. Sireesha ◽  
D. Neelima

The paper deals with spatially homogeneous anisotropic Bianchi type II, VIII , and IX dark energy cosmological models filled with perfect fluid in the framework of Saez-Ballester (1986) theory, and Einstein's general relativity. Assuming that the two sources interact minimally and therefore their energy momentum tensors are conserved separately, we have considered different cases and presented anisotropic as well as isotropic cosmological models. Some important physical and geometrical features of the models, thus obtained, have been discussed.


2011 ◽  
Vol 02 (10) ◽  
pp. 1222-1228 ◽  
Author(s):  
Velagapudi Uma Maheswara Rao ◽  
Mandangi Vijaya Santhi

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