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相关论文: FRW type of cosmology with a Chaplygin gas

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The generalized Chaplygin gas model, characterized by the equation of state $p = - \frac{B}{\rho^{\alpha}}$, is investigated within the framework of a Robertson-Walker spacetime. The resulting field equations governing this model are highly…

广义相对论与量子宇宙学 · 物理学 2025-07-02 D Panigrahi

We consider a FRW cosmological model with an exotic fluid known as Chaplygin gas. We show that the resulting evolution of the universe is not in disagreement with the current observation of cosmic acceleration. The model predict an…

广义相对论与量子宇宙学 · 物理学 2009-11-07 A. Yu. Kamenshchik , U. Moschella , V. Pasquier

We apply methods of dynamical systems to study the behaviour of universe dominated by the generalized Chaplygin gas. We reduce the dynamics to a 2-dimensional Hamiltonian system and study its behaviour for various ranges of parameters. The…

天体物理学 · 物理学 2009-11-10 Marek Szydlowski , Wojciech Czaja

In this work, we have considered the Friedmann-Robertson-Walker (FRW) model of the universe where bounce occurs and the universe is filled with Generalized Cosmic Chaplygin Gas (GCCG) or Variable Modified Chaplygin Gas (VMCG). We have…

广义相对论与量子宇宙学 · 物理学 2018-12-11 Tanwi Bandyopadhyay , Ujjal Debnath

Addressing the late-time accelerated expansion of the universe, known as the "dark energy problem", remains a central challenge in cosmology. While the cosmological constant is the standard explanation, alternative models such as…

广义相对论与量子宇宙学 · 物理学 2025-10-27 Gilberto Aguilar-Pérez , Miguel Cruz , Mohsen Fathi , Daniel de Jesús García-Castro , J. R. Villanueva

A flat FLRW cosmological model with perfect fluid comprising of variable Chaplygin gas has been studied in context of f(R; T) gravity with particle creation. The considered scale factors describe the accelerated expansion of universe due to…

广义相对论与量子宇宙学 · 物理学 2020-02-12 N. Hulke , G. P. Singh , Binaya K. Bishi , A. Singh

Cosmologies with a Chaplygin gas have recently been explored with the objective of explaining the transition from a dust dominated epoch towards an accelerating expansion stage. We consider the hypothesis that the transition to the…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Mariam Bouhmadi-Lopez , Paulo Vargas Moniz

We study the conditions for the consistency of the Friedmann-Robertson-Walker (FRW) metric with the dynamical Chern-Simons modified gravity. It turns out to be that in this situation the accelerated expansion of the Universe takes place,…

高能物理 - 理论 · 物理学 2011-07-14 C. Furtado , J. R. Nascimento , A. Yu. Petrov , A. F. Santos

The evolution of a Universe modelled as a mixture of a Chaplygin gas and radiation is determined by taking into account irreversible processes. This mixture could interpolate periods of a radiation dominated, a matter dominated and a…

广义相对论与量子宇宙学 · 物理学 2015-06-25 G. M. Kremer

In order to account for the observed cosmic acceleration, a modification of the ansatz for the variation of density in Friedman-Robertson-Walker (FRW) models given by Islam is proposed. The modified ansatz leads to an equation of state…

综合物理 · 物理学 2017-11-13 Abdussattar , S R Prajapati

The Friedmann-Robertson-Walker(FRW) model with dynamical Dark Energy(DE) in the form of modified Chaplygin gas(MCG) has been investigated. The evolution equations are reduced to an autonomous system on the two dimensional phase plane and it…

广义相对论与量子宇宙学 · 物理学 2015-05-28 Nairwita Mazumder , Ritabrata Biswas , Subenoy Chakraborty

In this paper, we have considered a model of modified Chaplygin gas in VSL theory with variable gravitational constant $G$. We have shown that the evolution of the universe starts from radiation era to phantom model. The whole evolution of…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Anup Kumar Singha , Ujjal Debnath

A time-varying cosmological "constant" Lambda is consistent with Einstein's equation, provided matter and/or radiation is created or destroyed to compensate for it. Supposing an empty primordial universe endowed with a very large…

广义相对论与量子宇宙学 · 物理学 2014-11-17 R. Aldrovandi , J. P. Beltran Almeida , J. G. Pereira

In this paper, we have studied $F(R,T)$ gravity as an arbitrary function of curvature and torsion scalars in Friedmann--Lema\^{\i}tre--Robertson--Walker (FLRW) background. Then, we have considered interacting model between $F(R,T)$ gravity…

广义相对论与量子宇宙学 · 物理学 2023-07-19 Ali R. Amani , S. L. Dehneshin

In this paper we study the evolution of the FRW universe filled with variable modified Chaplygin gas (VMCG). We begin with a thermodynamical treatment of VMCG described by the equation of state $P = A\rho-B\rho^{-\alpha}$, and obtain its…

广义相对论与量子宇宙学 · 物理学 2025-08-11 Samarjit Chakraborty , Sarbari Guha , D. Panigrahi

In this work, we investigate the cosmological dynamics of a spatially flat Friedmann--Lema\^itre--Robertson--Walker Universe in the framework of generalized \( \mathcal{F}(\mathcal{R},\Sigma,\mathcal{T}) \) gravity by incorporating…

广义相对论与量子宇宙学 · 物理学 2026-05-15 N. Myrzakulov , S. H. Shekh , Anirudh Pradhan , M. Zeyauddin

The present work is an attempt for emergent universe scenario with modified Chaplygin gas. The universe is chosen as spatially flat FRW space-time with modified Chaplygin gas as the only cosmic substratum. It is found that emergent scenario…

综合物理 · 物理学 2016-01-12 Sourav Dutta , Sudeshna Mukerji , Subenoy Chakraborty

In this paper we have examined the validity of the generalized second law of thermodynamics (GSLT) in an expanding Friedmann Robertson Walker (FRW) universe filled with different variants of Chaplygin gases. Assuming that the universe is a…

综合物理 · 物理学 2021-02-19 Samarjit Chakraborty , Sarbari Guha

The standard model of cosmology is investigated using time dependent cosmological constant $\Lambda$ and Newton's gravitational constant $G$. The total energy content is described by the modified Chaplygin gas equation of state. It is found…

广义相对论与量子宇宙学 · 物理学 2009-03-12 Mubasher Jamil , Farook Rahaman , Mehedi Kalam

In this paper the accelerating expansion of our universe at the late cosmic evolution time in a generally modified (extended) \emph{Chaplygin gas} (Dark Fluid) model is detailed, which is characterized by two parameters ($m$, $\alpha$).…

天体物理学 · 物理学 2007-05-23 Xin-He Meng , Ming-Guang Hu , Jie Ren
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