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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 cosmological scenarios of generalized Chaplygin gas in a universe governed by Horava-Lifshitz gravity. We consider both the detailed and non-detailed balance versions of the gravitational background, and we include the…

宇宙学与河外天体物理 · 物理学 2012-01-24 Amna Ali , Sourish Dutta , Emmanuel N. Saridakis , Anjan A. Sen

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

In this work, a spherically symmetric and static relativistic anisotropic fluid sphere solution of the Einstein field equations is provided. To build this particular model, we have imposed metric potential $e^{2\lambda(r)}$ and an equation…

广义相对论与量子宇宙学 · 物理学 2020-05-25 Francisco Tello-Ortiz , M. Malaver , Angel Rincon , Y. Gomez-Leyton

A spatially homogeneous and anisotropic Bianchi Type I universe has been studied with {\omega} <-1 without Big Smash. It is demonstrated that if cosmic dark energy behaves like a fluid with equation of state p = {\omega}{\rho} (p and {\rho}…

广义相对论与量子宇宙学 · 物理学 2011-08-04 Anil Kumar Yadav

In this paper, we consider a universe dominated by the extended Chaplygin gas which recently proposed as the last version of Chaplygin gas models. Here, we only consider the second order term which recovers quadratic barotropic fluid…

广义相对论与量子宇宙学 · 物理学 2015-04-01 E. O. Kahya , B. Pourhassan

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

Motivated by recent developments in particle physics and cosmology, there has been growing interest in an unified description of dark matter and dark energy scenarios. In this paper we explore observational constraints from age estimates of…

天体物理学 · 物理学 2011-06-21 J. S. Alcaniz , Deepak Jain , Abha Dev

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 study cosmological dynamics and late-time evolution of an extended induced gravity braneworld scenario. In this scenario, curvature effects are taken into account via the Gauss-Bonnet term in the bulk action and there is also a Chaplygin…

宇宙学与河外天体物理 · 物理学 2015-05-20 Kourosh Nozari , T. Azizi , N. Alipour

The generalized Chaplygin gas (GCG) is a candidate for the unification of dark energy and dark matter, and is parametrized by an exotic equation of state given by $p_{ch}=-A/\rho_{ch}^{\alpha}$, where $A$ is a positive constant and…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Francisco S. N. Lobo

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

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

The general form of the anisotropy parameter of the expansion for Bianchi type-III metric is obtained in the presence of a single diagonal imperfect fluid with a dynamically anisotropic equation of state parameter and a dynamical energy…

广义相对论与量子宇宙学 · 物理学 2014-11-20 Ozgur Akarsu , Can B. Kilinc

This paper discusses a new variable equation of state parameter leading to exact solutions of the Einstein field equations describing traversable wormholes. In addition to generalizing the notion of phantom energy, the equation of state…

广义相对论与量子宇宙学 · 物理学 2010-04-28 Peter K. F. Kuhfittig

We compare the WMAP temperature power spectrum and SNIa data to models with a generalized Chaplygin gas as dark energy. The generalized Chaplygin gas is a component with an exotic equation of state, p_X=-A/\rho^\alpha_X (a polytropic gas…

天体物理学 · 物理学 2009-11-07 L. Amendola , F. Finelli , C. Burigana , D. Carturan

A combination of recent observational results has given rise to what is currently known as the dark energy problem. Although several possible candidates have been extensively discussed in the literature to date the nature of this dark…

天体物理学 · 物理学 2009-11-07 Abha Dev , J. S. Alcaniz , Deepak Jain

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 have explored the possibility of the co-existence of two forms of dark energy in the form of an alternative Generalized Chaplygin Gas (GCG) along with a scalar field of field theoretic or extra dimensional origin in the background of a…

广义相对论与量子宇宙学 · 物理学 2026-01-28 Mahasweta Biswas , Rikpratik Sengupta , Ujjal Debnath

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