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相关论文: New Cosmographic Constraints on the Dark Energy an…

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In this work the observational constraints on interaction coupling parameter between dynamical dark energy and cold dark matter were obtained using CMB, BAO and SN Ia data. The dark energy in considered models is dynamical and evolution of…

宇宙学与河外天体物理 · 物理学 2025-12-17 Roman Neomenko

The coupled dark energy model provides a possible approach to mitigate the coincidence problem of cosmological standard model. Here, the coupling term is assumed as $\bar{Q}=3H\xi_x\bar{\rho}_x$, which is related to the interaction rate and…

宇宙学与河外天体物理 · 物理学 2016-10-11 Weiqiang Yang , Hang Li , Yabo Wu , Jianbo Lu

Cosmology with a three-form field interacting with cold dark matter is considered. In particular, the mass of the dark matter particles is assumed to depend upon the amplitude of the three-form field invariant. In comparison to coupled…

宇宙学与河外天体物理 · 物理学 2015-06-12 Tomi S. Koivisto , Nelson J. Nunes

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 present work deals with holographic dark energy models with Hubble horizon as the infra-red cut-off. The interaction rate between dark energy and dark matter has been reconstructed with three different choices of the interaction term.…

宇宙学与河外天体物理 · 物理学 2019-04-17 Purba Mukherjee , Ankan Mukherjee , H. K. Jassal , Ananda Dasgupta , Narayan Banerjee

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

We investigate a phenomenological non-gravitational coupling between dark energy and dark matter, where the interaction in the dark sector is parameterized as an energy transfer either from dark matter to dark energy or the opposite. The…

宇宙学与河外天体物理 · 物理学 2016-04-11 Riccardo Murgia , Stefano Gariazzo , Nicolao Fornengo

We consider a generic cosmological model which allows for non-gravitational direct couplings between dark matter and dark energy. The distinguishing cosmological features of these couplings can be probed by current cosmological…

宇宙学与河外天体物理 · 物理学 2018-01-17 Carsten van de Bruck , Jurgen Mifsud

Cosmological analysis based on currently available observations are unable to rule out a sizeable coupling between dark energy and dark matter. However, the signature of the coupling is not easy to grasp, since the coupling is degenerate…

宇宙学与河外天体物理 · 物理学 2011-03-22 Jian-Hua He , Bin Wang , Elcio Abdalla

Coupled dark matter-dark energy scenarios are modeled via a dimensionless parameter $\xi$, which controls the strength of their interaction. While this coupling is commonly assumed to be constant, there is no underlying physical law or…

宇宙学与河外天体物理 · 物理学 2019-10-16 Weiqiang Yang , Olga Mena , Supriya Pan , Eleonora Di Valentino

We reexamine interactions between the dark sectors of cosmology, with a focus on robust constraints that can be obtained using only mildly nonlinear scales. While it is well known that couplings between dark matter and dark energy can be…

宇宙学与河外天体物理 · 物理学 2018-09-18 V Miranda , Mariana Carrillo González , Elisabeth Krause , Mark Trodden

We investigate the impacts of interaction between dark matter and dark energy in the context of two dark energy models, holographic and ghost dark energy. In fact, using the dynamical system analysis, we obtain the cosmological consequence…

广义相对论与量子宇宙学 · 物理学 2017-07-26 Hanif Golchin , Sara Jamali , Esmaeil Ebrahimi

We consider the cosmological constraints on theories in which there exists a nontrivial coupling between the dark matter sector and the sector responsible for the acceleration of the universe, in light of the most recent supernovae, large…

天体物理学 · 物理学 2008-12-30 Rachel Bean , Eanna E. Flanagan , Istvan Laszlo , Mark Trodden

We consider the interaction between dark matter and dark energy in the framework of holographic dark energy, and propose a natural and physically plausible form of interaction, in which the interacting term is proportional to the product of…

宇宙学与河外天体物理 · 物理学 2014-05-27 Yin-zhe Ma , Yan Gong , Xuelei Chen

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

Models in which dark energy interacts with dark matter have been proposed in the literature to help explain why dark energy should only come to dominate in recent times. In this paper, we present a dynamical framework to calculate…

天体物理学 · 物理学 2009-03-12 Sirichai Chongchitnan

Coupled cosmologies can predict values for the cosmological parameters at low redshifts which may differ substantially from the parameters values within non-interacting cosmologies. Therefore, low redshift probes, as the growth of structure…

宇宙学与河外天体物理 · 物理学 2011-08-08 Francesco De Bernardis , Matteo Martinelli , Alessandro Melchiorri , Olga Mena , Asantha Cooray

Models where Dark Matter and Dark Energy interact with each other have been proposed to solve the coincidence problem. We review the motivations underlying the need to introduce such interaction, its influence on the background dynamics and…

宇宙学与河外天体物理 · 物理学 2016-08-24 B. Wang , E. Abdalla , F. Atrio-Barandela , D. Pavon

Any non-gravitational coupling between dark matter and dark energy modifies the cosmological dynamics. Interactions in the dark sector are considered to be relevant to address the coincidence problem. Moreover, in various models the…

宇宙学与河外天体物理 · 物理学 2015-06-04 W. Zimdahl

A cosmological model of dark energy interacting with dark matter and another general component of the universe is investigated. We found general constraints on these models imposing an accelerated expansion. The same is also studied in the…

高能物理 - 唯象学 · 物理学 2008-11-26 Norman Cruz , Samuel Lepe , Francisco Pena
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