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Anirudh Pradhan
Researcher at GLA University
Publications - 384
Citations - 6214
Anirudh Pradhan is an academic researcher from GLA University. The author has contributed to research in topics: Dark energy & Universe. The author has an hindex of 39, co-authored 328 publications receiving 5152 citations. Previous affiliations of Anirudh Pradhan include Yahoo! & Universiti Putra Malaysia.
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Anisotropic compact stars in the Buchdahl model: A comprehensive study
S. K. Maurya,Ayan Banerjee,Mahmood K. Jasim,Jitendra Kumar,Amit Kumar Prasad,Anirudh Pradhan +5 more
TL;DR: In this paper, the authors presented a class of relativistic solutions describing spherically symmetric and static anisotropic stars in hydrostatic equilibrium, including the Vaidya-Tikekar and Finch-Skea solutions.
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Bianchi Type-$V$ cosmology in $f(R,T)$ gravity with $\Lambda(T)$
Nasr Ahmed,Anirudh Pradhan +1 more
TL;DR: In this article, a new class of cosmological models in modified theories of gravity was proposed by Harko et al. where the gravitational Lagrangian is given by an arbitrary function of Ricci scalar and the trace of the stress energy tensor.
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Early viscous universe with variable gravitational and cosmological ‘constants’
TL;DR: In this paper, a unified description of the early evolution of universe is presented with a number of possible assumptions on the bulk viscous term and cosmological constant in which an inflationary phase is followed by radiation-dominated phase.
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Bianchi Type- V Cosmology in f( R, T) Gravity with Λ( T)
Nasr Ahmed,Anirudh Pradhan +1 more
TL;DR: In this article, the authors considered the cosmological constant Λ as a function of the trace of the stress energy-momentum-tensor, and dub such a model "Λ(T) gravity" where they have specified a certain form of Λ (T).
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Bianchi Type-III String Cosmological Models with Time Dependent Bulk Viscosity
Raj Bali,Anirudh Pradhan +1 more
TL;DR: In this article, the determinate model of the universe was obtained by assuming that the coefficient of bulk viscosity ξ is inversely proportional to the expansion θ in the model and expansion σ is proportional to shear σ.