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相关论文: Thawing models in the presence of a generalized Ch…

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The class of Chaplygin gas models regarded as a candidate of dark energy can be realized by a scalar field, which could drive the variation of the fine structure constant $\alpha$ during the cosmic time. This phenomenon has been observed…

宇宙学与河外天体物理 · 物理学 2014-11-12 Chao-Jun Feng , Xin-Zhou Li

In this paper we investigate the global dynamics for the minimally coupled scalar field representation of the modified Chaplygin gas in the context of flat FLRW cosmology. The tool for doing this is a new set of bounded variables that lead…

宇宙学与河外天体物理 · 物理学 2013-09-25 Claes Uggla

In the paper, we have presented a higher-dimensional cosmological model with a generalized Chaplygin-type gas to explain the recent acceleration of the universe. Dimensional reduction is feasible in this model, and our solutions are…

广义相对论与量子宇宙学 · 物理学 2025-07-01 D. Panigrahi , B. C. Paul , S. Chatterjee

The goal of this paper is to discuss phase space analysis of some interacting Chaplygin gas models in General Relativity. Chaplygin gas is one of the fluids actively considered in modern cosmology due to the fact that it is a joint model of…

广义相对论与量子宇宙学 · 物理学 2015-09-09 M. Khurshudyan , R. Myrzakulov

In this work the modified Chaplygin gas is related to a cosmological scalar field. Analytical results, more general than the solutions previously shown in the literature, are presented for the case when the curvature is absent, and one…

广义相对论与量子宇宙学 · 物理学 2008-03-03 Sandro Silva e Costa

The dynamics of a cosmological model fueled by scalar field dark matter with a cosh-like potential plus a cosmological constant is investigated in detail. It is revealed that the late-time attractor is always the de Sitter solution, and…

宇宙学与河外天体物理 · 物理学 2009-12-31 Tonatiuh Matos , Jose-Ruben Luevano , Israel Quiros , L. Arturo Urena-Lopez , Jose Alberto Vazquez

We investigate spatially flat isotropic cosmological models which contain a scalar field with an exponential potential and a perfect fluid with a linear equation of state. We include an interaction term, through which the energy of the…

天体物理学 · 物理学 2008-11-26 Andrew P. Billyard , Alan A. Coley

The generalized Chaplygin gas model represents an attempt to unify dark matter and dark energy. It is characterized by a fluid with an equation of state $p = - A/\rho^\alpha$. It can be obtained from a generalization of the DBI action for a…

宇宙学与河外天体物理 · 物理学 2015-03-17 J. C. Fabris , T. C. C. Guio , M. Hamani Daouda , O. F. Piattella

In the frame of the scalar field model with non minimal kinetic coupling to gravity, we study the cosmological solutions of the Chaplygin gas model of dark energy. By appropriately restricting the potential, we found the scalar field, the…

高能物理 - 理论 · 物理学 2011-07-28 L. N. Granda , E. Torrente-Lujan , J. J. Fernandez-Melgarejo

We present a scalar-field formulation of the generalized Chaplygin gas (GCG) and modified Chaplygin gas (MCG) models, in which the cosmic fluid dynamics are reproduced by canonical Lagrangians with analytically derived energy density…

宇宙学与河外天体物理 · 物理学 2025-09-23 Yi-Syuan Wu , Chuan-Jui Li , W. F. Kao

Even though many scalar field models of dark energy have been considered in the literature, there is another interesting class of dark energy models involving a fluid known as a Chaplygin gas. In addition to describing the dark energy, both…

广义相对论与量子宇宙学 · 物理学 2021-06-14 Amin Rezaei Akbarieh , Mohammad Ahmadi , Yousef Izadi , Shahabeddin M. Aslmarand , Warner A. Miller

We investigate the dynamical properties of a class of spatially homogeneous and isotropic cosmological models containing a barotropic perfect fluid and multiple scalar fields with independent exponential potentials. We show that the…

广义相对论与量子宇宙学 · 物理学 2009-10-31 A. A. Coley , R. J. van den Hoogen

The goal of this paper is to study new cosmological models where the dark energy is a varying Chaplygin gas. This specific dark energy model with non-linear EoS had been often discussed in modern cosmology. Contrary to previous studies, we…

广义相对论与量子宇宙学 · 物理学 2021-05-04 M. Khurshudyan , R. Myrzakulov

In this work, we have extended the analysis on the generalized Chaplygin gas (GCG) model as the unification of dark energy and dark matter. Specifically, we have shown that the model of our consideration known as the new generalized…

广义相对论与量子宇宙学 · 物理学 2022-04-13 Abdulla Al Mamon , Andronikos Paliathanasis , Subhajit Saha

We investigate a kind of interacting Chaplygin gas model in which the Chaplygin gas plays the role of dark energy and interacts with cold dark matter particles. We find that there exists a stable scaling solution at late times with the…

天体物理学 · 物理学 2009-11-13 Hongsheng Zhang , Zong-Hong Zhu

We investigate in detail the asymptotic properties of tachyon cosmology for a broad class of self-interaction potentials. The present approach relies in an appropriate re-definition of the tachyon field, which, in conjunction with a method…

广义相对论与量子宇宙学 · 物理学 2011-03-28 Israel Quiros , Tame Gonzalez , Dania Gonzalez , Yunelsy Napoles , Ricardo Garcia-Salcedo , Claudia Moreno

In this paper, we attempt to explore the possibility of a obtaining a viable emergent universe scenario supported by a type of fluid known as the extended Chaplygin gas, which extends a modification to the equation of state of the well…

广义相对论与量子宇宙学 · 物理学 2025-08-13 Rikpratik Sengupta , Anirban Chanda , B C Paul , M Kalam

In this paper, we reexamine the generalized Chaplygin gas (GCG) cosmology with the sign-changeable interaction. The dynamical analysis show that there exists de-Sitter attractors in this model, which means that the late-time behaviors of…

广义相对论与量子宇宙学 · 物理学 2015-10-13 Ping Xi , Ping Li

In this work, considering the background dynamics of flat Friedmann-Lemaitre-Robertson-Walker(FLRW) model of the universe, we investigate a scalar field model as dark energy candidate which interacting with the pressure-less dust as dark…

广义相对论与量子宇宙学 · 物理学 2023-05-25 Goutam Mandal , Soumya Chakraborty , Sudip Mishra , Sujay Kr. Biswas

The generalized Chaplygin gas, which interpolates between a high density relativistic era and a non-relativistic matter phase, is a popular dark energy candidate. We consider a generalization of the Chaplygin gas model, by assuming the…

广义相对论与量子宇宙学 · 物理学 2008-11-26 C. S. J. Pun , L. Á. Gergely , M. K. Mak , Z. Kovács , G. M. Szabó , T. Harko
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