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相关论文: Generalizing the generalized Chaplygin gas

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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

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 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

We study the nonlinear regime of Unified Dark Energy models, using Generalized Chaplygin Gas cosmologies as a representative example, and introduce a new parameter characterizing the level of small scale clustering in these scenarios. We…

宇宙学与河外天体物理 · 物理学 2015-06-19 P. P. Avelino , K. Bolejko , G. F. Lewis

In this paper we consider a cosmological model whose main components are a scalar field and a generalized Chaplygin gas. We obtain an exact solution for a flat arbitrary potential. This solution have the right dust limit when the Chaplygin…

宇宙学与河外天体物理 · 物理学 2013-10-31 Sergio del Campo , Carlos R. Fadragas , Ramon Herrera , Carlos Leiva , Genly Leon , Joel Saavedra

A modified generalized Chaplygin gas (MGCG) is considered as the unified dark matter-dark energy revisited. The character of MGCG is endued with the dual role, which behaves as matter at early times and as an quiessence dark energy at late…

广义相对论与量子宇宙学 · 物理学 2013-07-05 Xue-Mei Deng

An exotic dark component, named generalized Chaplygin gas (Cg) and parameterized by an equation of state $p = -A/\rho_{Cg}^{\alpha}$ where $A$ and $\alpha$ are arbitrary constants, is one of the possible candidates for dark energy as well…

天体物理学 · 物理学 2009-11-10 J. S. Alcaniz , J. A. S. Lima

A particular generalization of the Chaplygin inflationary model, using the formalism of Hamilton-Jacobi and elliptic functions, results in a more general non-linear Chaplygin-type equation of state (Chaplygin-Jacobi model). We investigate…

广义相对论与量子宇宙学 · 物理学 2025-03-11 J. A. S. Fortunato , W. S. Hipolito-Ricaldi , N. Videla , J. R. Villanueva

We use the Markov Chain Monte Carlo method to investigate a global constraints on the generalized Chaplygin gas (GCG) model as the unification of dark matter and dark energy from the latest observational data: the Constitution dataset of…

宇宙学与河外天体物理 · 物理学 2010-05-07 Lixin Xu , Jianbo Lu

In this work we explore an alternative phenomenological model to Chaplygin gas proposed by H. Hova et. al., consisting on a modification of a perfect fluid, to explain the dynamics of dark matter and dark energy at cosmological scales…

宇宙学与河外天体物理 · 物理学 2019-01-30 A. Hernandez-Almada , Juan Magana , Miguel A. Garcia-Aspeitia , V. Motta

The generalized Chaplygin gas (GCG), which has an unusual perfect fluid equation of state, is another promising candidate for dark energy. We investigate the GCG scenario coupled with a baryonic matter in a newly suggested $f(Q,T)$ gravity,…

广义相对论与量子宇宙学 · 物理学 2022-06-24 Gaurav N. Gadbail , Simran Arora , P. K. Sahoo

The type Ia supernovae observational data are used to estimate the parameters of a cosmological model with cold dark matter and the Chaplygin gas. The Chaplygin gas model depends essentially on four parameters: the Hubble constant, the…

天体物理学 · 物理学 2009-12-30 R. Colistete , J. C. Fabris , S. V. B. Gonçalves , P. E. de Souza

The Chaplygin gas model, characterized by an equation of state of the type $p = - \frac{A}{\rho}$ emerges naturally from the Nambu-Goto action of string theory. This fluid representation can be recast under the form of a tachyonic field…

广义相对论与量子宇宙学 · 物理学 2015-05-13 C. E. M. Batista , J. C. Fabris , M. Morita

Motivated by a recent work of us [1], we reconstruct the different f(T)-gravity models corresponding to a set of dark energy scenarios containing the polytropic, the standard Chaplygin, the generalized Chaplygin and the modified Chaplygin…

综合物理 · 物理学 2012-08-01 K. Karami , A. Abdolmaleki

Recently developed Generalized Cosmic Chaplygin gas (GCCG) is studied as an unified model of dark matter and dark energy. To explain the recent accelerating phase, the Universe is assumed to have a mixture of radiation and GCCG. The mixture…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Writambhara Chakraborty , Ujjal Debnath , Subenoy Chakraborty

In this work we investigate the background dynamics when dark energy is coupled to dark matter with a suitable interaction in the universe described by Loop quantum cosmology. Dark energy in the form of Generalised Cosmic Chaplygin gas is…

综合物理 · 物理学 2015-06-04 Ratul Chowdhury , Prabir Rudra

We use the latest data to investigate observational constraints on the new generalized Chaplygin gas (NGCG) model. Using the Markov Chain Monte Carlo (MCMC) method, we constrain the NGCG model with the type Ia supernovae (SNe Ia) from…

宇宙学与河外天体物理 · 物理学 2015-06-11 Kai Liao , Yu Pan , Zong-Hong Zhu

We study the general properties of a spherically symmetric body described through the generalized Chaplygin equation of state. We conclude that such object, dubbed generalized Chaplygin dark star, should exist within the context of the…

天体物理学 · 物理学 2009-11-13 O. Bertolami , J. Paramos

We propose a phenomenological model for the early universe where there is a smooth transition between an early "quintessence" phase and a radiation dominated era. The matter content is modelled by an appropriately modified Chaplygin gas for…

宇宙学与河外天体物理 · 物理学 2015-03-19 Mariam Bouhmadi-Lopez , Pisin Chen , Yen-Wei Liu

A new diagnostic method, $Om$ is applied to generalized Chaplygin gas (GCG) model as the unification of dark matter and dark energy. On the basis of the recently observed data: the Union supernovae, the observational Hubble data, the SDSS…

天体物理学 · 物理学 2010-11-02 Jianbo Lu , Lixin Xu