Bianchi type-VI0 cosmological models with anisotropic dark energy

2010 ◽  
Vol 332 (2) ◽  
pp. 497-502 ◽  
Author(s):  
K. S. Adhav ◽  
A. S. Bansod ◽  
S. L. Munde ◽  
R. G. Nakwal
Keyword(s):  
Dark Energy ◽  
Bianchi Type ◽  
Cosmological Models ◽  
Anisotropic Dark Energy ◽  
Bianchi Type Vi0

scholarly journals Bianchi Type- II Universe with Anisotropic Dark Energy in Lyra Geometry

2017 ◽  
Vol 2 (4) ◽  
pp. 231-237
Author(s):  
R. K. Dubey ◽  
◽  
Shri Ram ◽  
Neelam Yadav ◽  
Vipendra Dwivedi ◽  
...  
Keyword(s):  
Dark Energy ◽  
Bianchi Type ◽  
Lyra Geometry ◽  
Type Ii ◽  
Anisotropic Dark Energy

scholarly journals Anisotropic magnetized holographic Ricci dark energy cosmological models

2017 ◽  
Vol 95 (4) ◽  
pp. 381-392 ◽  
Author(s):  
M. Vijaya Santhi ◽  
V.U.M. Rao ◽  
Y. Aditya
Keyword(s):  
General Relativity ◽  
Dark Energy ◽  
Deceleration Parameter ◽  
Bianchi Type ◽  
Cosmological Models ◽  
Field Equations ◽  
Ricci Dark Energy ◽  
Theor Phys ◽  
Linearly Varying Deceleration Parameter ◽  
Spatially Homogeneous

In this paper, we have considered spatially homogeneous and anisotropic Bianchi type-III space–time filled with matter and anisotropic modified holographic Ricci dark energy in general relativity. We have solved Einstein’s field equations using the following possibilities: (i) hybrid expansion law proposed by Akarsu et al. (JCAP, 01, 022 (2014)); (ii) a varying deceleration parameter considered by Mishra et al. (Int. J. Theor. Phys. 52, 2546 (2013)); and (iii) a linearly varying deceleration parameter given by Akarsu and Dereli (Int. J. Theor. Phys. 51, 612 (2012)). We have presented the cosmological models in each of the preceding cases and studied their evolutions. We have also discussed physical and kinematical properties of the models.

scholarly journals Bianchi type III models with anisotropic dark energy

2009 ◽  
Vol 42 (4) ◽  
pp. 763-775 ◽  
Author(s):  
Özgür Akarsu ◽  
Can Battal Kılınç
Keyword(s):  
Dark Energy ◽  
Bianchi Type ◽  
Type Iii ◽  
Anisotropic Dark Energy
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