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Anisotropic universe models in gravity
We investigate the cosmological reconstruction in an anisotropic universe for both the
homogeneous and inhomogeneous content of the universe. Special attention is given to …
homogeneous and inhomogeneous content of the universe. Special attention is given to …
Quadratically varying deceleration parameter in gravity
RK Tiwari, D Sofuoğlu - … Journal of Geometric Methods in Modern …, 2020 - World Scientific
In this paper, we have proposed a new form for the varying deceleration parameter that is a
generalization of the form of Ö. Akarsu and T. Dereli [Cosmological models with linearly …
generalization of the form of Ö. Akarsu and T. Dereli [Cosmological models with linearly …
Anisotropic Universe Models with Perfect Fluid and Scalar Field in f(R,T) Gravity
In this paper, we study the behavior of perfect fluid and massless scalar field for
homogeneous and anisotropic Bianchi type I universe model in f (R, T) gravity, where R is …
homogeneous and anisotropic Bianchi type I universe model in f (R, T) gravity, where R is …
An axially symmetric transitioning models with observational constraints
In this study, we have demonstrated the expansion history of an axially symmetric Bianchi
type-I model of the universe. Our model as of now presents an accelerating universe, which …
type-I model of the universe. Our model as of now presents an accelerating universe, which …
Study of Bianchi I anisotropic model in f(R,T) gravity
We discuss the Bianchi type I model with perfect fluid as matter content in f (R, T) gravity,
where R is the Ricci scalar and T is the trace of the energy-momentum tensor. We obtain …
where R is the Ricci scalar and T is the trace of the energy-momentum tensor. We obtain …
Observational constraint in Kantowski–Sachs f (R) gravity model with strange quark matter
In this paper, we have discussed the cosmological consequence of the f (R) dark energy
scenario with the Kantowski-Sachs space-time in the context of strange quark matter with …
scenario with the Kantowski-Sachs space-time in the context of strange quark matter with …
Phase transition of LRS Bianchi type-I cosmological model in gravity
RK Tiwari, D Sofuoğlu, VK Dubey - International Journal of …, 2020 - World Scientific
In this work, LRS Bianchi type-I cosmological model with perfect fluid source in f (R, T)
gravity theory, where R is the Ricci scalar and T is the trace of the stress energy-momentum …
gravity theory, where R is the Ricci scalar and T is the trace of the stress energy-momentum …
Magnetized strange quark matter solutions in f (R, T) gravity with cosmological constant
In this research, we have studied magnetized strange quark matter (SQM) solutions for
Friedmann-Robertson-Walker (FRW) universe in f (R, T) gravity. To obtain exact solutions of …
Friedmann-Robertson-Walker (FRW) universe in f (R, T) gravity. To obtain exact solutions of …
Quark and strange quark matter in f(R) gravity for Bianchi type I and V space-times
Behaviors of quark matter and strange quark matter which exist in the first seconds of the
early Universe in f (R) gravity are studied for Bianchi I and V universes. In this respect, we …
early Universe in f (R) gravity are studied for Bianchi I and V universes. In this respect, we …
Anisotropic solutions in f (R) gravity
Anisotropic cosmological models are investigated in f (R) gravity in the metric formalism.
Plane symmetric models with anisotropy in the expansion rates are considered. The …
Plane symmetric models with anisotropy in the expansion rates are considered. The …