Bianchi type-III cosmological model in the presence of zero-mass scalar fields

1990 ◽  
Vol 173 (1) ◽  
pp. 157-161
Author(s):  
K. Shanthi ◽  
V. U. M. Rao

2016 ◽  
Vol 13 (05) ◽  
pp. 1650058 ◽  
Author(s):  
Gyan Prakash Singh ◽  
Binaya Kumar Bishi ◽  
Pradyumn Kumar Sahoo

In this paper, we have studied the Bianchi type-III cosmological model in the presence of cosmological constant in the context of [Formula: see text] modified theory of gravity. Here, we have discussed two classes of [Formula: see text] gravity, i.e. [Formula: see text] and [Formula: see text]. In both classes, the modified field equations are solved by the relation expansion scalar [Formula: see text] that is proportional to shear scalar [Formula: see text] which gives [Formula: see text], where [Formula: see text] and [Formula: see text] are metric potentials. Also we have discussed some physical and kinematical properties of the models.



1984 ◽  
Vol 105 (1) ◽  
pp. 67-71 ◽  
Author(s):  
Ramji Tiwari ◽  
D. K. Singh




2010 ◽  
Vol 50 (2) ◽  
pp. 339-348 ◽  
Author(s):  
K. S. Adhav ◽  
M. V. Dawande ◽  
R. S. Thakare ◽  
R. B. Raut


2015 ◽  
Vol 55 (1) ◽  
pp. 526-534 ◽  
Author(s):  
Subrata Kumar Sahu ◽  
Endale Nigatu Kantila ◽  
Dawit Melese Gebru




1992 ◽  
Vol 187 (1) ◽  
pp. 113-117 ◽  
Author(s):  
V. U. M. Rao ◽  
Y. V. S. S. Sanyasiraju


2005 ◽  
Vol 295 (3) ◽  
pp. 331-337 ◽  
Author(s):  
K. S. Adhav ◽  
G. S. Khadekar ◽  
V. G. Mete


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