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相关论文: Chaplygin DGP cosmologies

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Recently it was found that dark energy in the form of phantom generalized Chaplygin gas may lead to a new form of the cosmic doomsday, the big freeze singularity. Like the big rip singularity, the big freeze singularity would also take…

天体物理学 · 物理学 2009-11-13 Artyom V. Yurov , Artyom V. Astashenok , Pedro F. Gonzalez-Diaz

The Modified Chaplygin Gas (MCG) model is revisited to examine its ability to describe the full cosmic evolution within a single framework. Because the field equations are highly nonlinear, no closed analytical solution for the scale factor…

广义相对论与量子宇宙学 · 物理学 2025-12-23 D. Panigrahi , S. Chatterjee , B. C. Paul

We study dynamical dark energy models that allow for general late time behaviour while admitting non-phantom dynamics at early times, including thawing, scaling$+$thawing, and effective fluid extensions. Using current cosmological data, we…

宇宙学与河外天体物理 · 物理学 2025-12-24 Sk. Sohail , Sonej Alam , Md. Wali Hossain

We construct a DGP-inspired braneworld model where induced gravity on the brane is modified in the spirit of $f(R)$ gravity and stringy effects are taken into account by incorporation of the Gauss-Bonnet term in the bulk action. We explore…

广义相对论与量子宇宙学 · 物理学 2009-09-28 Kourosh Nozari , Narges Rashidi

We extend the Chaplygin gas model for dark matter and dark energy unification by promoting the Chaplygin gas parameter A to the potential for an extra scalar with canonical kinetic energy. The hybrid model allows for accelerated Hubble…

天体物理学 · 物理学 2009-11-10 Neven Bilic , Gary B. Tupper , Raoul D. Viollier

A new model describing the dark sector of the universe is established. The model involves Bose-Einstein condensate (BEC) as dark energy (DE) and an excited state above it as dark matter (DM). The condensate is assumed to have a negative…

广义相对论与量子宇宙学 · 物理学 2011-05-24 V. A. Popov

We propose a simple higher-derivative braneworld gravity model which contains a stable accelerating branch, in the absence of cosmological constant or potential, that can be used to describe the late time cosmic acceleration. This model has…

高能物理 - 理论 · 物理学 2009-11-11 Claudia de Rham , Andrew J. Tolley

In this manuscript, we investigate late-time cosmology and the evolution of cosmic structures using an interacting dark fluid model in which dark matter (DM) and dark energy (DE) interact through a diffusive mechanism. To provide a…

宇宙学与河外天体物理 · 物理学 2025-12-01 Shambel Sahlu , Upala Mukhopadhyay , Remudin R. Mekuria , Amare Abebe

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

This paper investigates a newly proposed fluid description of dark energy within the framework of the late-time accelerated expansion of the universe. Our primary objective is to explore the theoretical foundation of the proposed equation…

广义相对论与量子宇宙学 · 物理学 2025-03-11 Tamal Mukhopadhyay , Banadipa Chakraborty , Ujjal Debnath , Anirudh Pradhan

We investigate general braneworld models, with a non-minimally coupled phantom bulk field and arbitrary brane and bulk matter contents. We show that the effective dark energy of the brane-universe acquires a dynamical nature, as a result of…

高能物理 - 理论 · 物理学 2009-03-27 M. R. Setare , E. N. Saridakis

We consider late-time cosmology in a (phantom) scalar-tensor theory with an exponential potential, as a dark energy model with equation of state parameter close to -1 (a bit above or below this value). Scalar (and also other kinds of)…

高能物理 - 理论 · 物理学 2009-09-17 Emilio Elizalde , Shin'ichi Nojiri , Sergei D. Odintsov

The hypothesis that dark matter and dark energy are unified through the Chaplygin gas is reexamined. Using a generalization of the spherical model which incorporates effects of the acoustic horizon we show that an initially perturbative…

天体物理学 · 物理学 2007-05-23 Neven Bilic , Robert J. Lindebaum , Gary B. Tupper , Raoul D. Viollier

Braneworld models with induced gravity have the potential to replace dark energy as the explanation for the current accelerating expansion of the Universe. The original model of Dvali, Gabadadze and Porrati (DGP) demonstrated the existence…

高能物理 - 理论 · 物理学 2008-11-26 Marcela Carena , Joseph Lykken , Minjoon Park , Jose Santiago

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

We study the late-time evolution of the Universe where dark energy (DE) is parametrized by a modified generalized Chaplygin gas (mGCG) on top of cold dark matter (CDM). We also take into account the radiation content of the Universe. In…

广义相对论与量子宇宙学 · 物理学 2015-12-22 Mariam Bouhmadi-López , Maxim Brilenkov , Ruslan Brilenkov , João Morais , Alexander Zhuk

In this article we study cosmic dynamics in the context of normal branch of DGP braneworld model. Using the current Planck data, we best fit the model and cosmological parameters in non-flat $\Lambda$DGP. With the transition redshift as a…

广义相对论与量子宇宙学 · 物理学 2016-11-09 A. Ravanpak , H. Farajollahi , G. F. Fadakar

The DGP (Dvali, Gabadaze and Porrati) braneworld cosmology gives an alternative to dark energy. In DGP cosmology the alleged cosmic acceleration is generated by the modification of gravity theory. Nonlinear evolution of matter density…

宇宙学与河外天体物理 · 物理学 2020-08-21 Ankan Mukherjee

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

We show that a generalised phantom Chaplygin gas can present a future singularity in a finite future cosmic time. Unlike the big rip singularity, this singularity happens for a finite scale factor, but like the big rip singularity, it would…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Mariam Bouhmadi-Lopez , Pedro F. Gonzalez-Diaz , Prado Martin-Moruno