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相关论文: Interacting quintessence from a variational approa…

200 篇论文

We investigate a cosmological model in which dark energy, represented by a quintessential scalar field, is coupled to a dark-matter perfect fluid in the spatially flat Friedmann-Robertson-Walker Universe. This allows an energy exchange in…

广义相对论与量子宇宙学 · 物理学 2023-08-22 Yousef Bisabr

We study the effective Lagrangian, at leading order in derivatives, that describes the propagation of density and metric fluctuations in a fluid composed by an arbitrary number of interacting components. Our results can be applied to any…

高能物理 - 理论 · 物理学 2014-06-05 Guillermo Ballesteros , Brando Bellazzini , Lorenzo Mercolli

In this paper, we consider two-component dark energy models in Lyra manifold. The first component is assumed as a quintessence field while the second model may be a viscous polytropic gas, a viscous Van der Waals gas or a viscous modified…

广义相对论与量子宇宙学 · 物理学 2014-09-03 M. Khurshudyan , J. Sadeghi , R. Myrzakulov , A. Pasqua , H. Farahani

We investigate the role of a possible coupling of dark matter and dark energy. In particular, we explore the consequences of such an interaction for the coincidence problem, i.e., for the question, why the energy densities of dark matter…

天体物理学 · 物理学 2016-11-09 W. Zimdahl , D. Pavon , L. P. Chimento , A. S. Jakubi

We study a cosmological model in which phantom dark energy is coupled to dark matter by phenomenologically introducing a coupled term to the equations of motion of dark energy and dark matter. This term is parameterized by a dimensionless…

高能物理 - 理论 · 物理学 2009-11-10 Rong-Gen Cai , Anzhong Wang

We analyse three cosmological scenarios with interaction in the dark sector, which are particular cases of a general expression for the energy flux from vacuum to matter. In the first case the interaction leads to a transition from an…

宇宙学与河外天体物理 · 物理学 2015-03-31 L. P. Chimento , S. Carneiro

This study examines interacting quintessence dark energy models and their observational constraints for a general parameterization of the quintessence potential, which encompasses a broad range of popular potentials. Four different forms of…

宇宙学与河外天体物理 · 物理学 2023-07-25 Nandan Roy

From a variational action with non-minimal coupling with a scalar field and classical scalar and fermionic interaction, cosmological field equations can be obtained. Imposing a FLRW metric the equations lead directly to a cosmological model…

广义相对论与量子宇宙学 · 物理学 2011-11-29 Samuel Lepe , Javier Lorca , Francisco Peña , Yerko Vásquez

Cosmological models involving an interaction between dark matter and dark energy have been proposed in order to solve the so-called coincidence problem. Different forms of coupling have been studied, but there have been claims that…

天体物理学 · 物理学 2009-06-23 Miguel Quartin , Mauricio O. Calvao , Sergio E. Joras , Ribamar R. R. Reis , Ioav Waga

The dynamics of interacting dark matter-dark energy models is characterized through an interaction rate function quantifying the energy flow between these dark sectors. In most of the interaction functions, the expansion rate Hubble…

宇宙学与河外天体物理 · 物理学 2021-05-05 Weiqiang Yang , Supriya Pan , Llibert Aresté Saló , Jaume de Haro

Interacting dark energy models may play a crucial role in explaining several important observational issues in modern cosmology and also may provide a solution to current cosmological tensions. Since the phenomenology of the dark sector…

宇宙学与河外天体物理 · 物理学 2023-12-06 Weiqiang Yang , Supriya Pan , Olga Mena , Eleonora Di Valentino

A unified model of dark energy and matter is presented using the modified variable Chaplygin gas for interacting dark energy in a non-flat universe. The two entities interact with each other non-gravitationally which involves a coupling…

天体物理学 · 物理学 2008-12-18 Mubasher Jamil , Muneer A. Rashid

In this paper the coupling between dark energy and the other components of the cosmological fluid has been studied. Firstly, it will be shown that the application of general cosmological equations, deduced by the authors in a previous work,…

宇宙学与河外天体物理 · 物理学 2010-06-02 Alberto C. Balfagon , Raul Ramirez-Satorras , Angel R. Martinez

The interacting and holographic dark energy models involve two important quantities. One is the characteristic size of the holographic bound and the other is the coupling term of the interaction between dark energy and dark matter. Rather…

高能物理 - 理论 · 物理学 2008-11-26 Bo Hu , Yi Ling

We propose a new non-minimally coupled quintessence model to account for the late-time dark energy dynamics indicated by recent DESI measurements. Within this framework, the quintessence density begins to decrease only when it starts to…

宇宙学与河外天体物理 · 物理学 2026-04-10 Jia-Qi Wang , Rong-Gen Cai , Zong-Kuan Guo , Yun-He Li , Shao-Jiang Wang , Xin Zhang

Non-gravitational interaction between two barotropic dark fluids, namely the pressureless dust and the dark energy in a spatially flat Friedmann-Lema\^{i}tre-Robertson-Walker model has been discussed. It is shown that for the interactions…

宇宙学与河外天体物理 · 物理学 2018-04-30 Supriya Pan , Ankan Mukherjee , Narayan Banerjee

We consider a self-consistent and physical approach to interacting dark energy models described by a Lagrangian, and identify a new class of models with variable dark energy sound speed. We show that if the interaction between dark energy…

宇宙学与河外天体物理 · 物理学 2018-04-18 Mark S. Linton , Alkistis Pourtsidou , Robert Crittenden , Roy Maartens

We investigated a possible interaction between cold dark matter and dark energy, corresponding to a well-known interacting dark energy model discussed in the literature within the context of resolving the Hubble tension. We put constraints…

宇宙学与河外天体物理 · 物理学 2024-08-21 David Benisty , Supriya Pan , Denitsa Staicova , Eleonora Di Valentino , Rafael C. Nunes

In this paper we generalize the kinetic mixing idea to time reparametrization invariant theories, namely, relativistic point particles and cosmology in order to obtain new insights for dark matter and energy. In the first example, two…

广义相对论与量子宇宙学 · 物理学 2015-06-30 Ashok Das , Jorge Gamboa , Miguel Pino

In standard cosmologies, dark energy interacts only gravitationally with dark matter. An extension to this picture is interacting quintessence (IQ) model, where scalar field coupled directly to cold dark matter. The percentage deviation is…

宇宙学与河外天体物理 · 物理学 2019-10-23 Azam Hussain