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Binaya K. Bishi
Researcher at Visvesvaraya National Institute of Technology
Publications - 38
Citations - 581
Binaya K. Bishi is an academic researcher from Visvesvaraya National Institute of Technology. The author has contributed to research in topics: Deceleration parameter & Cosmological constant. The author has an hindex of 13, co-authored 34 publications receiving 468 citations. Previous affiliations of Binaya K. Bishi include University of Zululand & Sambalpur University.
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Anisotropic cosmological models in $f(R,T)$ gravity with variable deceleration parameter
TL;DR: In this article, the authors considered a time varying deceleration parameter (DP), which generates an accelerating universe to obtain the exact solution of the field equations, and explored the nature of WEC, DEC, SEC and energy density for both the cases.
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Magnetized strange quark model with Big Rip singularity in f(R, T) gravity
TL;DR: In this paper, the exact solutions of the field equations are derived with linearly time varying deceleration parameter, which is consistent with observational data (from SNIa, BAO and CMB) of standard cosmology.
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Magnetized strange quark model with Big Rip singularity in $f(R,T)$ gravity
TL;DR: In this article, the exact solutions of the field equations are derived with linearly time varying deceleration parameter which is consistent with observational data (from SNIa, BAO and CMB) of standard cosmology.
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Magnetized strange quark matter in f(R, T) gravity with bilinear and special form of time varying deceleration parameter
TL;DR: In this paper, the exact solutions of the field equations are obtained under bilinear and special form of time varying deceleration parameter (DP) for the Bianchi type-I model with magnetized strange quark matter (MSQM) distribution and cosmological constant Λ in f(R, T) gravity where R is the Ricci scalar and T the trace of matter source.
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LRS Bianchi type-I cosmological model with constant deceleration parameter in f(R,T) gravity
TL;DR: In this paper, a spatially homogeneous anisotropic LRS Bianchi type-I cosmological model is studied in f(R,T) gravity with a special form of Hubble's parameter, which leads to constant deceleration parameter.