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相关论文: No slow-roll inflation \`a la Generalized Chaplygi…

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In this work, we study an inflationary scenario in the presence of Generalized Chaplygin Gas (GCG). We show that in Einstein gravity, GCG is not a suitable candidate for inflation; but in a five dimensional brane world scenario, it can work…

宇宙学与河外天体物理 · 物理学 2014-10-22 Bikash R Dinda , Sumit Kumar , Anjan A. Sen

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 warm intermediate inflationary model in the context of Generalized Chaplygin Gas is investigated. We study this model in the weak and strong dissipative regimes, considering a generalized form of the dissipative coefficient…

广义相对论与量子宇宙学 · 物理学 2016-02-17 Ramón Herrera , Nelson Videla , Marco Olivares

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

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

In this paper, we revisit generalized Chaplygin gas (GCG) model as a unified dark matter and dark energy model. The energy density of GCG model is given as $\rho_{GCG}/\rho_{GCG0}=[B_{s}+(1-B_{s})a^{-3(1+\alpha)}]^{1/(1+\alpha)}$, where…

宇宙学与河外天体物理 · 物理学 2015-06-04 Lixin Xu , Jianbo Lu , Yuting Wang

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

We study the dynamics of inflation in a generalized scalar-torsion gravity scenario by assuming a canonical scalar field non-minimally coupled to torsion with a Galileon-type self-interaction. After obtaining the field equations for a flat…

广义相对论与量子宇宙学 · 物理学 2019-08-26 Manuel Gonzalez-Espinoza , Giovanni Otalora , Nelson Videla , Joel Saavedra

The generalized Chaplygin gas (GCG) model in spatially flat universe is investigated. The cosmological consequences led by GCG model including the evolution of EoS parameter, deceleration parameter and dimensionless Hubble parameter are…

广义相对论与量子宇宙学 · 物理学 2011-06-10 M. Malekjani , A. Khodam-Mohammadi , N. Nazari-Pooya

The present paper is devoted to find a new generalization of the generalized Chaplygin gas. Therefore, starting from the Hubble parameter associated to the Chaplygin scalar field and using some elliptic identities, the elliptic…

广义相对论与量子宇宙学 · 物理学 2015-07-30 J. R. Villanueva

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

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

The generalized Chaplygin gas (GCG) model is the prototype of a unified model of dark energy (DE) and dark matter (DM). It is characterized by equation-of-state (EoS) parameters $A$ and $\alpha$. We use a statistical analysis of the 2dFGRS…

宇宙学与河外天体物理 · 物理学 2010-04-22 J. C. Fabris , H. E. S. Velten , W. Zimdahl

We study the Generalized Chaplygin gas model (GCGM) using Gamma-ray bursts as cosmological probes. In order to avoid the so-called circularity problem we use cosmology-independent data set and Bayesian statistics to impose constraints on…

宇宙学与河外天体物理 · 物理学 2011-08-19 R. C. Freitas , S. V. B. Gonçalves , H. E. S. Velten

We present a simple toy model corresponding to a network of frustrated topological defects of domain walls or cosmic strings that exist previous to the standard slow-roll inflationary era of the universe. Such a network (i) can produce a…

宇宙学与河外天体物理 · 物理学 2013-05-22 Mariam Bouhmadi-Lopez , Pisin Chen , Yu-Chien Huang , Yu-Hsiang Lin

In the simplest scenario for inflation, i. e. in the single-field inflation, it is presented an inflaton field with properties equivalent to a generalized Chaplygin gas. Their study is performed using the Hamilton-Jacobi approach to…

宇宙学与河外天体物理 · 物理学 2015-06-17 Sergio del Campo

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 generalize the constant-roll condition for minimally coupled canonical scalar field inflation. Particularly, we shall assume that the scalar field satisfies the condition $\ddot{\phi}=\alpha (\phi) V'(\phi)$, and we derive…

广义相对论与量子宇宙学 · 物理学 2022-05-25 V. K. Oikonomou

We consider a Chaplygin gas model with an exponential potential in framework of braneworld inflation. We apply the slow-roll approximation in the high-energy limit to derive various inflationary spectrum perturbation parameters. We show…

高能物理 - 理论 · 物理学 2014-08-12 R. Zarrouki , M. Bennai
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