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相关论文: Astronomical bounds on future big freeze singulari…

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It is proposed that dark energy may become dominant over standard matter due to universe expansion (curvature decrease). Two models: non-linear gravity-matter system and modified gravity may provide the effective phantom or effective…

天体物理学 · 物理学 2008-11-26 Shin'ichi Nojiri , Sergei D. Odintsov

Phantom energy which violates the dominant-energy condition and is not excluded by current constraints on the equation of state may be dominating the evolution of the universe now. It has been pointed out that in such a case the fate of the…

天体物理学 · 物理学 2009-11-07 Pedro F. Gonzalez-Diaz

In spite of its rather weird properties which include violation of the dominant-energy condition, the requirement of superluminal sound speed and increasing vacuum-energy density, phantom energy has recently attracted a lot of scientific…

天体物理学 · 物理学 2009-11-10 Pedro F. Gonzalez-Diaz

We investigate the cosmological behavior in a universe governed by time asymmetric extensions of general relativity, which is a novel modified gravity based on the addition of new, time-asymmetric, terms on the Hamiltonian framework, in a…

广义相对论与量子宇宙学 · 物理学 2015-11-11 Genly Leon , Emmanuel N. Saridakis

In this work, gravitational collapse of a spherical cloud, consists of both dark matter and dark energy in the form of modified Chaplygin gas is studied. It is found that dark energy alone in the form of modified Chaplygin gas forms black…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Ujjal Debnath , Subenoy Chakraborty

In this work, we have considered interacting dynamical model taking variable modified Chaplygin gas which plays as dark energy coupled to cold dark matter in the flat FRW universe. Since the nature of dark energy and dark matter is still…

综合物理 · 物理学 2015-03-19 Jhumpa Bhadra , Ujjal Debnath

Despite the interest in dark matter and dark energy, it has never been shown that they are in fact two separate substances. We provide the first strong evidence that they are separate by ruling out a broad class of so-called unified dark…

天体物理学 · 物理学 2008-11-26 Havard Sandvik , Max Tegmark , Matias Zaldarriaga , Ioav Waga

We investigate several varying-mass dark-matter particle models in the framework of phantom cosmology. We examine whether there exist late-time cosmological solutions, corresponding to an accelerating universe and possessing dark energy and…

广义相对论与量子宇宙学 · 物理学 2014-11-18 Genly Leon , Emmanuel N. Saridakis

In this paper, we consider three different models of dark energy in higher dimensional space-time and discuss about some cosmological parameters numerically. The first model is a single component universe including viscous varying modified…

广义相对论与量子宇宙学 · 物理学 2014-06-13 M. Khurshudyan , J. Sadeghi , M. Hakobyan , H. Farahani , R. Myrzakulov

We review the several models of the dark energy, which may generate the accelerated expansion of the present universe. We also discuss the the Big Rip singularity, which may occur when the equation of the state parameter w is less than -1.…

高能物理 - 理论 · 物理学 2007-05-23 Shin'ichi Nojiri

Any unified dark matter cosmology can be decomposed into dark matter interacting with vacuum energy, without introducing any additional degrees of freedom. We present observational constraints on an interacting vacuum plus dark energy…

宇宙学与河外天体物理 · 物理学 2013-04-16 Yuting Wang , David Wands , Lixin Xu , Josue De-Santiago , Alireza Hojjati

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

Future singularities arising in a family of models for the expanding Universe, characterized by sharing a convenient parametrization of the energy budget in terms of the deceleration parameter, are classified. Finite-time future…

广义相对论与量子宇宙学 · 物理学 2019-01-23 Emilio Elizalde , Martiros Khurshudyan , Shin'ichi Nojiri

In the paper, we have presented a higher-dimensional cosmological model with a generalized Chaplygin-type gas to explain the recent acceleration of the universe. Dimensional reduction is feasible in this model, and our solutions are…

广义相对论与量子宇宙学 · 物理学 2025-07-01 D. Panigrahi , B. C. Paul , S. Chatterjee

While modelling our late time cosmically accelerated universe, it is popular to involve different dark energy models, the equation of state of which can be taken as a function of the redshift and some unknown parameters. Barboza and Alcaniz…

综合物理 · 物理学 2019-09-25 Swetalina Bhowmik , Ritabrata Biswas

We consider a model of the Universe with variable G and {\Lambda}. Subject of our interest is a phenomenological model for {\Lambda} proposed and considered in this article first time (up to our knowledge). Modification based on an…

广义相对论与量子宇宙学 · 物理学 2015-01-13 M. Khurshudyan , J. Sadeghi , E. Chubaryan , H. Farahani

Explanations to the accelerated expansion of the Universe are usually sought either in modifications of Einstein gravity or in new forms of energy density. An example of modified gravity is the braneworld Dvali-Gabadadze-Porrati (DGP) model…

天体物理学 · 物理学 2008-04-22 Matts Roos

The big freeze is a singularity that shows up in some dark energy models. We address here its possible avoidance in quantum cosmology, more precisely in the framework of quantum geometrodynamics.

广义相对论与量子宇宙学 · 物理学 2010-02-26 Mariam Bouhmadi-Lopez , Claus Kiefer , Barbara Sandhoefer , Paulo Vargas Moniz

Observations provide increasingly strong evidence that the universe is accelerating. This revolutionary advance in cosmological observations confronts theoretical cosmology with a tremendous challenge, which it has so far failed to meet.…

天体物理学 · 物理学 2008-11-26 Ruth Durrer , Roy Maartens

The evolution of a universe modelled as a mixture of generalised Chaplygin gas and ordinary matter field is studied for a Robertson Walker type of spacetime. This model could interpolate periods of a radiation dominated, matter dominated…

广义相对论与量子宇宙学 · 物理学 2017-02-14 D. Panigrahi , S. Chatterjee