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相关论文: Generalized Chaplygin Gas, Accelerated Expansion a…

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We study the cosmological scenario arising from the dynamics of a generalized Chaplygin gas. The equation of state of the system is given in terms of the energy density, $\rho$, and pressure, $p$, by the relationship $p = -…

天体物理学 · 物理学 2007-05-23 M. C. Bento , O. Bertolami , A. A. Sen

The generalized Chaplygin gas (GCG) model allows for an unified description of the recent accelerated expansion of the Universe and the evolution of energy density perturbations. This dark energy - dark matter unification is achieved…

广义相对论与量子宇宙学 · 物理学 2014-11-17 M. C. Bento , O. Bertolami , A. A. Sen

The generalized Chaplygin gas (GCG) model allows for an unified description of the cosmologically recent accelerated expansion of the Universe and of the evolution of energy density perturbations. This dark energy - dark matter unification…

天体物理学 · 物理学 2007-05-23 O. Bertolami

We find exact solution of the Einstein equations in the context of the brane world scenario. We have supposed a {generalized chaplygin gas} equation of state for bulk. This study display a constant energy density and pressure for bulk in…

广义相对论与量子宇宙学 · 物理学 2014-01-20 Kh. Saaidi , A. Mohammadi

The generalized Chaplygin gas (GCG) model explains the recent accelerated expansion of the Universe via an exotic background fluid whose equation of state is given by p=-A/\rho^\alpha, where A is a positive constant and 0<\alpha\le 1. The…

天体物理学 · 物理学 2015-06-24 M. C. Bento , O. Bertolami , A. A. Sen

A model of an emergent universe is obtained in brane world. Here the bulk energy is in the form of cosmological constant, while the brane consists of the Chaplygin gas with the modified equation of state such as $p=A\rho-B/\rho$. Initially…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Asit Banerjee , Tanwi Bandyopadhyay , 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 brane cosmology. Here DGP and the RSII brane models have been considered separately.…

广义相对论与量子宇宙学 · 物理学 2012-03-12 Prabir Rudra , Ujjal Debnath , Ritabrata Biswas

Unification of dark matter and dark energy as short- and long-range manifestations of a single cosmological substance is possible in models described by the generalized Chaplygin gas equation of state. We show it admits halo-like structures…

广义相对论与量子宇宙学 · 物理学 2017-12-20 T. de Beer , J. W. van Holten

Interactions between dark matter and dark energy with a given equation of state are known to modify the cosmic dynamics. On the other hand, the strength of these interactions is subject to strong observational constraints. Here we discuss a…

天体物理学 · 物理学 2015-05-13 Winfried Zimdahl

This thesis concentrates on the accelerated expansion of the Universe recently explored by measurements of redshift and luminosity-distance relations of type Ia Supernovae. We have considered a model of the universe filled with modified…

广义相对论与量子宇宙学 · 物理学 2011-05-06 Writambhara Chakraborty

The generalized Chaplygin gas is characterized by the equation of state p = - A/rho^alpha, with alpha > -1 and w > -1. We generalize this model to allow for the cases where alpha < -1 or w < -1. This generalization leads to three new…

天体物理学 · 物理学 2013-05-29 A. A. Sen , Robert J. Scherrer

In this work we explore the background dynamics when dark energy is coupled to dark matter with a suitable interaction in the universe described by brane cosmology. Here DGP and the RSII brane models have been considered separately. Dark…

综合物理 · 物理学 2015-06-05 Prabir Rudra

We develop a cosmological model based on a quadratic equation of state p/c^2=-(\alpha+1){\rho^2}/{\rho_P}+\alpha\rho-(\alpha+1)\rho_{\Lambda} (where \rho_P is the Planck density and \rho_{\Lambda} the cosmological density) "unifying" vacuum…

宇宙学与河外天体物理 · 物理学 2015-12-01 Pierre-Henri Chavanis

The generalized Chaplygin gas is usually defined as a barotropic perfect fluid with an equation of state $p=-A \rho^{-\alpha}$, where $\rho$ and $p$ are the proper energy density and pressure, respectively, and $A$ and $\alpha$ are positive…

广义相对论与量子宇宙学 · 物理学 2018-08-22 V. M. C. Ferreira , P. P. Avelino

We employ the generalized Chaplygin gas of interacting dark energy to obtain the equation of state for the generalized Chaplygin gas energy density in non-flat universe. By choosing a negative value for $B$ we see that $w_{\rm…

广义相对论与量子宇宙学 · 物理学 2010-10-27 M R Setare

A model of unification of dark matter and dark energy based on the modeling of the speed of sound as a function of the parameter of the equation of state is introduced. It is found that the model in which the speed of sound depends on the…

宇宙学与河外天体物理 · 物理学 2013-04-04 Neven Caplar , Hrvoje Stefancic

In the framework of spatially averaged inhomogeneous cosmologies in classical general relativity, effective Einstein equations govern the dynamics of averaged scalar variables in a scale--dependent way. A particular cosmology may be…

广义相对论与量子宇宙学 · 物理学 2010-08-23 Xavier Roy , Thomas Buchert

A new model for the universe filled with a generalized Chaplygin fluid is considered which unitarily describes as a single vacuum entity both a quintessence scalar field and a cosmological constant, so unifying the notion of dark energy.…

天体物理学 · 物理学 2008-11-26 Pedro F. Gonzalez-Diaz

In this paper we investigate the role played by dark energy in the form of Generalized cosmic Chaplygin gas in an accelerating universe described by FRW cosmology. We have tried to describe the model from the theoretical point of view of a…

广义相对论与量子宇宙学 · 物理学 2013-07-11 Prabir Rudra

This paper is devoted to the investigation of modified Chaplygin gas model in the context of solvable k-essence cosmologies. For this purpose, we construct equations of state parameter of this model for some particular values of the…

综合物理 · 物理学 2012-07-31 M. Sharif , K. R. Yesmakhanova , S. Rani , R. Myrzakulov
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