Dynamical system analysis of the Bianchi type-V cosmological model in R n -gravity

2021 ◽  
Vol 38 (20) ◽  
pp. 205004
Author(s):  
Thato Tsabone ◽  
Amare Abebe
2007 ◽  
Vol 5 (1) ◽  
pp. 79-84 ◽  
Author(s):  
D.R.K. Reddy ◽  
Atchuta Rao ◽  
Nirupama Devi ◽  
R.L. Naidu

1984 ◽  
Vol 1 (4) ◽  
pp. 407-415 ◽  
Author(s):  
D R Matravers ◽  
D L Vogel ◽  
M S Madsen

2013 ◽  
Vol 346 (2) ◽  
pp. 567-572 ◽  
Author(s):  
Rajesh Kumar ◽  
S. K. Srivastava

2016 ◽  
Vol 94 (10) ◽  
pp. 992-1000 ◽  
Author(s):  
M. Abdel-Megied ◽  
E.A. Hegazy

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.


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