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相关论文: In search of the dark matter dark energy interacti…

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We present and employ a new kinematical approach to cosmological `dark energy' studies. We construct models in terms of the dimensionless second and third derivatives of the scale factor a(t) with respect to cosmic time t, namely the…

天体物理学 · 物理学 2008-11-26 David Rapetti , Steven W. Allen , Mustafa A. Amin , Roger D. Blandford

A parametric reconstruction of the jerk parameter, the third order derivative of the scale factor expressed in a dimensionless way, has been discussed. Observational constraints on the model parameters have been obtained by Maximum…

广义相对论与量子宇宙学 · 物理学 2016-03-23 Ankan Mukherjee , Narayan Banerjee

We study observational signatures of non-gravitational interactions between the dark components of the cosmic fluid, which can be either due to creation of dark particles from the expanding vacuum or an effect of the clustering of a…

宇宙学与河外天体物理 · 物理学 2019-12-10 Micol Benetti , Welber Miranda , Humberto A. Borges , Cassio Pigozzo , Saulo Carneiro , Jailson S. Alcaniz

We analyze a model for Dark Energy - Dark Matter interaction, based on a decaying process of the former into the latter. The dynamical equations are constructed following a kinetic formulation, which separates the interacting fluctuations…

广义相对论与量子宇宙学 · 物理学 2025-02-24 Giovanni Montani , Nakia Carlevaro , Luis A. Escamilla , Eleonora Di Valentino

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

In this study, we will look at an interacting dark energy model. In the framework of Friedmann-Robertson-Walker (FRW) space-time, we have made the hypothesis of an interacting scheme between two fields (dark matter (DM) and dark energy…

广义相对论与量子宇宙学 · 物理学 2023-11-27 J. K. Singh , Ritika Nagpal

In this paper, we have studied an interacting dark energy model. We have assumed the gravitational interaction between the matter fields i.e. between barotropic fluid and the dark energy. The dark energy evolution within the framework of…

广义相对论与量子宇宙学 · 物理学 2023-04-03 Keshav Ram Mishra , Shibesh Kumar Jas Pacif , Rajesh Kumar , Kazuharu Bamba

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 the dynamical behaviour of a general class of interacting models in the dark sector in which the phenomenological coupling between cold dark matter and dark energy is a power law of the cosmic scale factor. From numerical…

宇宙学与河外天体物理 · 物理学 2017-09-04 F. E. M. Costa , A. O. Ribeiro , F. Roig

The cosmological model with an interaction between dynamical quintessence dark energy and cold dark matter is considered. Evolution of a dark energy equation of state parameter is defined by a dark energy adiabatic sound speed and a dark…

宇宙学与河外天体物理 · 物理学 2023-11-08 Roman Neomenko

In this paper, we test the dark matter-dark energy interacting cosmological model with a dynamic equation of state $w_{DE}(z)=w_{0}+w_{1}z/(1+z)$, using type Ia supernovae (SNe Ia), Hubble parameter data, baryonic acoustic oscillation (BAO)…

宇宙学与河外天体物理 · 物理学 2015-04-16 J. S. Wang , F. Y. Wang

We investigate a class of interacting dark energy and dark matter (DM) models, where dark energy is modeled as a $k$-essence scalar field with an inverse-square potential. Two general forms of interaction are considered: one proportional to…

宇宙学与河外天体物理 · 物理学 2026-04-14 Saddam Hussain , Qiang Wu , Tao Zhu

The recent observational evidence for the current cosmic acceleration have stimulated renewed interest in alternative cosmologies, such as scenarios with interaction in the dark sector (dark matter and dark energy). In general, such models…

宇宙学与河外天体物理 · 物理学 2009-10-22 R. S. Goncalves , J. S. Alcaniz , A. Dev , D. Jain

In this work we model two non-linear directly interacting scenarios in dark sector of the universe with the dimensionless parameter $\alpha$ and $\beta$, which dominate the energy exchange between dark energy and dark matter. The central…

宇宙学与河外天体物理 · 物理学 2025-04-08 Jiangang Kang

We study the evolution of $k=-1$ FLRW cosmological models for two interacting Dark Matter-Dark Energy Models using dynamical system analysis. Since we are interested in late time evolution, the sign of the interaction term is chosen such…

广义相对论与量子宇宙学 · 物理学 2024-11-26 Ashmita , Kinjal Banerjee , Prasanta Kumar Das

We show that a general late-time interaction between cold dark matter and vacuum energy is favoured by current cosmological datasets. We characterize the strength of the coupling by a dimensionless parameter $q_V$ that is free to take…

宇宙学与河外天体物理 · 物理学 2014-11-05 Valentina Salvatelli , Najla Said , Marco Bruni , Alessandro Melchiorri , David Wands

Scalar cosmological perturbations are investigated in the framework of a model with interacting dark energy and dark matter. In addition to these constituents, the inhomogeneous Universe is supposed to be filled with the standard…

广义相对论与量子宇宙学 · 物理学 2015-07-24 Maxim Eingorn , Claus Kiefer

The cosmological evolution of an interacting scalar field model in which the scalar field interacts with dark matter, radiation, and baryon via Lorentz violation is investigated. We propose a model of interaction through the effective…

高能物理 - 理论 · 物理学 2009-09-29 Freddy P. Zen , Arianto , Bobby E. Gunara , Triyanta , A. Purwanto

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

We propose a general class of interacting models in which the interaction between the CDM component and $\Lambda$ is parameterized by an arbitrary function of the cosmic scale factor $\epsilon(a)$. Differently from other dynamical $\Lambda$…

宇宙学与河外天体物理 · 物理学 2010-04-06 F. E. M. Costa , J. S. Alcaniz
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