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相关论文: New parameterizations of generalized Chaplygin gas…

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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

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 use different combinations of data samples to investigate the new generalized Chaplygin gas (NGCG) model in the context of dark energy (DE) cosmology. Using the available cosmological data, we put constraints on the the free parameters…

宇宙学与河外天体物理 · 物理学 2022-01-19 Fataneh Salahedin , Reza Pazhouhesh , Mohammad Malekjani

Yes, but only for a parameter value that makes it almost coincide with the standard model. We reconsider the cosmological dynamics of a generalized Chaplygin gas (gCg) which is split into a cold dark matter (CDM) part and a dark energy (DE)…

宇宙学与河外天体物理 · 物理学 2017-02-03 R. F. vom Marttens , L. Casarini , W. Zimdahl , W. S. Hipólito-Ricaldi , D. F. Mota

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 investigate observational constraints on the generalized Chaplygin gas (GCG) model as the unification of dark matter and dark energy from the latest observational data: the Union SNe Ia data, the observational Hubble data, the SDSS…

宇宙学与河外天体物理 · 物理学 2014-11-20 Jianbo Lu , Yuanxing Gui , Lixin Xu

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

In this work we consider a class of interacting vacuum corresponding to a generalised Chaplygin gas (gCg) cosmology. In particular we analyse two different scenarios at perturbation level for the same background interaction characterised by…

宇宙学与河外天体物理 · 物理学 2023-06-08 H. A. Borges , C. Pigozzo , P. Hepp , L. O. Baraúna , M. Benetti

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

In this paper, we undertake a unified study of background dynamics and cosmological perturbations in the presence of the Chaplygin gas. This is done by first constraining the background cosmological parameters of different Chaplygin gas…

广义相对论与量子宇宙学 · 物理学 2023-10-12 Shambel Sahlu , Heba Sami , Renier Hough , Maye Elmardi , Anna-Mia Swart , Amare Abebe

We study the linear growth function $f$ for large scale structures in a cosmological scenario where Generalised Chaplygin Gas (GCG) serves as dark energy candidate. We parametrize the growth index parameter as a function of redshift and do…

宇宙学与河外天体物理 · 物理学 2015-05-30 Gaveshna Gupta , Somasri Sen , Anjan A. Sen

We derive constraints on the parameter space of the unified model of dark energy and dark matter, the Generalized Chaplygin Gas (GCG), from the amplitudes and positions of the first few peaks and first trough of the cosmic microwave…

天体物理学 · 物理学 2008-11-26 T. Barreiro , O. Bertolami , P. Torres

Despite the remarkable success of the standard LambdaCDM model in describing the evolution of the universe, several unresolved issues remain, such as the true nature of dark energy, fine-tuning problems, and the persistent Hubble tension.…

广义相对论与量子宇宙学 · 物理学 2025-09-15 Mahendra Goray , Bijan Saha

In this paper, we use the latest observations of quasars covering the redshift range of $0.04<z<5.1$ to investigate a series of Chaplygin gas models as candidates for unified dark matter and dark energy. Based on different combinations of…

宇宙学与河外天体物理 · 物理学 2022-08-15 Jie Zheng , Shuo Cao , Yujie Lian , Tonghua Liu , Yuting Liu , Zong-Hong Zhu

The correspondence of the Gauss-Bonnet (GB) and its modification (MGB) models of dark energy with the standard and generalized Chaplygin gas-scalar field models (SCG and GCG) have been studied in a {\deg}at universe. The exact solution of…

广义相对论与量子宇宙学 · 物理学 2016-11-10 A. Khodam-Mohammadi , E. Karimkhani , A. Alaei

We propose in this paper a new model for describing the unification of dark energy and dark matter. This new model is a further generalization of the generalized Chaplygin gas (GCG) model, thus dubbed new generalized Chaplygin gas (NGCG)…

天体物理学 · 物理学 2009-11-10 Xin Zhang , Feng-Quan Wu , Jingfei Zhang

We study cosmological models with modified Chaplygin gas (in short, MCG) to determine observational constraints on its EoS parameters. The observational data of the background and the growth tests are employed. The background test data…

宇宙学与河外天体物理 · 物理学 2015-04-02 Bikash Chandra Paul , Prasenjit Thakur , Aroonkumar Beesham

We investigate observational constraints on the generalized Chaplygin gas (GCG) model including the gamma-ray bursts (GRBs) at high redshift obtained directly from the Union2 type Ia supernovae (SNe Ia) set. By using the Markov Chain Monte…

宇宙学与河外天体物理 · 物理学 2011-06-02 Nan Liang , Lixin Xu , Zong-Hong Zhu

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
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