Bianchi Type-V Domain Walls and Quark Matter Cosmological Model with Cosmological Constant $${\varvec{\Lambda}}$$ Λ in $$\varvec{f}\left( {\varvec{R},\varvec{T}} \right)$$ f R , T Gravity

2017 ◽  
Vol 41 (1) ◽  
pp. 33-43 ◽  
Author(s):  
G. P. Singh ◽  
Binaya K. Bishi
Keyword(s):  
Cosmological Model ◽  
Cosmological Constant ◽  
Quark Matter ◽  
Domain Walls ◽  
Bianchi Type ◽  
Type V ◽  
Bianchi Type V

Domain walls and quark matter in Bianchi type-V universe with observational constraints in F(R,T) gravity

2019 ◽  
Vol 17 (01) ◽  
pp. 2050014 ◽  
Author(s):  
Dinesh Chandra Maurya ◽  
Anirudh Pradhan ◽  
Archana Dixit
Keyword(s):  
Quark Matter ◽  
Domain Walls ◽  
Bianchi Type ◽  
Momentum Tensor ◽  
Accelerated Expansion ◽  
Observational Constraints ◽  
Field Equations ◽  
Bianchi Type V Universe ◽  
Type V ◽  
Bianchi Type V

In this study, we investigate the Bianchi type-V cosmological models with quark matter (QM) distribution and domain walls with observational constraints in [Formula: see text] theory of gravity (Harko et al. in Phys. Rev. D 84 (2011) 024020), for a specific choice of the function [Formula: see text] (where [Formula: see text] is Ricci scalar and [Formula: see text] is the trace of the energy–momentum tensor). We have used model-independent methods and hyperbolic expansion scale factors to achieve the deterministic solution of the modified Einstein field equations and these are also tested observationally. The behaviors of QM and domain walls give an idea of accelerated expansion of the Universe which agrees with recent observations of Type Ia Supernovae. We also discuss the physical implications of the derived models.

A Bianchi Type -V Cosmological Model in Brans - Dicke Theory of Gravitation

2007 ◽  
Vol 5 (1) ◽  
pp. 79-84 ◽  
Author(s):  
D.R.K. Reddy ◽  
Atchuta Rao ◽  
Nirupama Devi ◽  
R.L. Naidu
Keyword(s):  
Cosmological Model ◽  
Bianchi Type ◽  
Theory Of Gravitation ◽  
Type V ◽  
Bianchi Type V

Helium formation in a Bianchi type V cosmological model with tilt

1984 ◽  
Vol 1 (4) ◽  
pp. 407-415 ◽  
Author(s):  
D R Matravers ◽  
D L Vogel ◽  
M S Madsen
Keyword(s):  
Cosmological Model ◽  
Bianchi Type ◽  
Type V ◽  
Bianchi Type V

scholarly journals Bianchi type V Ih Bulk-Viscous String Cosmological Model in f(R) Gravity

2019 ◽  
Vol 1344 ◽  
pp. 012038
Author(s):  
M. Vijaya Santhi ◽  
Y. Sobhanbabu ◽  
B. J. M. Rao
Keyword(s):  
Cosmological Model ◽  
Bianchi Type ◽  
String Cosmological Model ◽  
Bulk Viscous ◽  
Type V ◽  
Bianchi Type V

Bianchi type-V cosmological model with purely magnetic solution

2013 ◽  
Vol 346 (2) ◽  
pp. 567-572 ◽  
Author(s):  
Rajesh Kumar ◽  
S. K. Srivastava
Keyword(s):  
Cosmological Model ◽  
Bianchi Type ◽  
Type V ◽  
Bianchi Type V

Bianchi type VI cosmological model with electromagnetic field in Lyra geometry

2016 ◽  
Vol 94 (10) ◽  
pp. 992-1000 ◽  
Author(s):  
M. Abdel-Megied ◽  
E.A. Hegazy
Keyword(s):  
Electromagnetic Field ◽  
Cosmological Model ◽  
Bianchi Type ◽  
Lyra Geometry ◽  
Geometrical Properties ◽  
Special Cases ◽  
Type V ◽  
Tensor Formula ◽  
Shear Tensor ◽  
Bianchi Type V

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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