Zobrazeno 1 - 10
of 206
pro vyhledávání: '"DIXIT, Archana"'
This study explores the properties of quark stars (QS) formulated with an interacting quark matter equation of state (EoS) within the framework of Rastall gravity, a modified theory of gravity. We derive the mass-radius relationships and calculate th
Externí odkaz:
http://arxiv.org/abs/2412.09306
In this work, the cosmic solutions, particularly the well-known $\Lambda$CDM model, are investigated in the framework of the Gauss-Bonnet gravity, where the gravitational action incorporates the Gauss-Bonnet invariant function. We utilize a specializ
Externí odkaz:
http://arxiv.org/abs/2409.16304
In the recently suggested modified non-metricity gravity theory with boundary terms in a flat FLRWspacetime universe, dark energy scenarios of cosmological models are examined in this study. An arbitrary function, $f(Q, C)=Q+{\alpha}C^{2}$, has been
Externí odkaz:
http://arxiv.org/abs/2310.02267
Publikováno v:
International Journal of Geometric Methods in Modern Physics, (2023)
In this paper, we have investigated an anisotropic cosmological model in $f(Q)$ gravity with string fluid in LRS Bianchi type-I universe. We have considered the arbitrary function $f(Q)=Q+\alpha\sqrt{~Q}+2\Lambda$ where $\alpha$ is model free paramet
Externí odkaz:
http://arxiv.org/abs/2302.14104
In this paper, we have analyzed the significance of bulk viscosity in an axially symmetric Bianchi type-I model to study the accelerated expansion of the universe. We have considered four bulk viscosity parameterizations for the matter-dominated cosm
Externí odkaz:
http://arxiv.org/abs/2212.10413
Publikováno v:
Symmetry 2022, 14(12), 2630
In this article, we have discussed the results of our investigation. We consider an anisotropic viscous cosmological model of (LRS) Bianchi type I spacetime universe filled with a viscous fluid under $f(Q)$ gravity. We have studied the modified $f(Q)
Externí odkaz:
http://arxiv.org/abs/2210.13730
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 had been in the decelerating phase in the past. Roles of the two cruc
Externí odkaz:
http://arxiv.org/abs/2204.04451
In this paper, we have examined the viability of the Bianchi type-V universe in Brans-Dicke (BD) theory of gravitation. We have discussed the interacting and non-interacting scenarios between dark matter (DM) and dark energy (DE) of the derived unive
Externí odkaz:
http://arxiv.org/abs/2203.11426
Publikováno v:
International Journal of Modern Physics A, Vol. 36, No. 36 (2021) 2150256
In this paper, we examine the (LRS) Bianchi-type-I cosmological model with holographic dark energy. The exact solutions to the corresponding field equations are obtained by using generalized hybrid expansion law (HEL). The EoS parameter $\omega$ for
Externí odkaz:
http://arxiv.org/abs/2203.05699
In this paper, we have investigated the physical behavior of cosmological models in the framework of modified Teleparallel gravity. This model is established using a Renyi holographic ``dark energy model (RHDE) with a Hubble cutoff. Here we have cons
Externí odkaz:
http://arxiv.org/abs/2109.12963