Bianchi type V and VI0 cosmological models in Lyra geometry

Anisotropic solutions in f(R) gravity

“…In this context, it is interesting to investigate some anisotropic models in the framework of f (R) gravity. The importance of the effects of anisotropy in the universe has led many authors to investigate anisotropic models with or without matter in the field equations [68][69][70][71][72].…”

Bianchi Type V Barotropic Perfect Fluid Cosmological Model in Lyra Geometry

“…The model (5.4) has Point Type singularity at T = 0. The model (5.4) obtained for stiff perfect fluid is the same as obtained by Singh and Singh [39].…”

“…Beesham [25], Maharaj and Beesham [26], Coley [27], Lorentz [28], Roy and Singh [29], Banerjee and Sanyal [30], Roy and Prasad [31], Nayak and Sahoo [32], Bali and Singh [33], Bali and Sharma [34], Bali and Meena [35,36], Singh et al [37], Bali and Jain [38]. Singh and Singh [39] have investigated some Bianchi Type V and VI 0 cosmological models in Lyra geometry. To get the deterministic models of the universe, they have discussed a stiff perfect fluid p = ρ model where p the isotropic pressure and ρ the matter density.…”

Bianchi type-V cosmological model with perfect fluid using negative constant deceleration parameter in a scalar tensor theory based on Lyra Manifold

“…Dieter Lorenz (1981), Nayak (1983), Shri Ram and Singh (1984), Baillie and Madsen (1985), Beesham (1986), Venkateswarlu and Reddy (1989a,1989b,1989c, Singh and Singh (1991), Krori et al (1994), Roy and Prasad (1994), Nayak and Sahoo (1996), Camci et al (2001), Pradhan et al (2005, Bali and Singh (2005) are some of the authors who worked on Bianchi type-V model. Recently Rao et al (2007) have obtained Bianchi type-V cosmological model in SaezBallester theory of gravitation with perfect fluid distribution.…”