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相关论文: An interacting model for the cosmological dark sec…

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A cosmological model in an Einstein-Cartan framework endowed with torsion is studied. For a torsion function assumed to be proportional to Hubble expansion function, namely $\phi=-\alpha H$, the contribution of torsion function as a dark…

广义相对论与量子宇宙学 · 物理学 2022-04-27 S. H. Pereira , A. M. Vicente , J. F. Jesus , R. F. L. Holanda

We investigate the cosmological dynamics of interacting Logarithmic Entropy Corrected Holographic Dark Energy model with Cold Dark Matter. Fixed points are determined and their corresponding cosmological models are presented. Moreover, the…

广义相对论与量子宇宙学 · 物理学 2016-09-27 F. Darabi , F. Felegary , M. R. Setare

We explore a model of interacting dark energy where the dark energy density is related by the holographic principle to the Hubble parameter, and the decay of the dark energy into matter occurs at a rate comparable to the current value of…

天体物理学 · 物理学 2008-12-18 Micheal S. Berger , Hamed Shojaei

We analyze a cosmological model featuring an interaction between dark energy and dark matter in light of the measurements of the Cosmic Microwave Background released by three independent experiments: the most recent data by the Planck…

宇宙学与河外天体物理 · 物理学 2023-07-13 Yuejia Zhai , William Giarè , Carsten van de Bruck , Eleonora Di Valentino , Olga Mena , Rafael C. Nunes

We extend the cosmological couplings proposed in Sun et al. and Wei, where they suggested interactions with change of signs along the cosmological evolution. Our extension liberates the changes of sign of the interaction from the…

广义相对论与量子宇宙学 · 物理学 2014-09-25 Mónica Forte

We investigate an interacting dark energy model which allows for the kinetic term of the scalar field to couple to dark matter via a power-law interaction. The model is characterised by scaling solutions at early times, which are of high…

宇宙学与河外天体物理 · 物理学 2022-12-06 Elsa M. Teixeira , Bruno J. Barros , Vasco M. C. Ferreira , Noemi Frusciante

In the present work, motivated by the work of Cai and Su [Phys. Rev. D {\bf 81}, 103514 (2010)], we propose a new type of interaction in dark sector, which can change its sign when our universe changes from deceleration to acceleration. We…

广义相对论与量子宇宙学 · 物理学 2011-01-21 Hao Wei

We study the collider, astrophysical and cosmological constraints on the dark matter sector of a conformal model within the framework of both the freeze out as well as the freeze in mechanism. The model has a dark sector with strong self…

高能物理 - 唯象学 · 物理学 2019-12-25 Prasenjit Sanyal , Alekha C. Nayak , Gopal Kashyap , Pankaj Jain

Non-gravitational interaction between dark matter and dark energy has been considered in a spatially flat Friedmann-Lema\^{i}tre-Robertson-Walker (FLRW) universe. The interaction rate is assumed to be linear in the energy densities of dark…

广义相对论与量子宇宙学 · 物理学 2020-07-07 Supriya Pan , Jaume de Haro , Weiqiang Yang , Jaume Amorós

In this paper, we introduce a new interacting mechanism within the dark sector, encompassing both dark energy and dark matter, while grounding our analysis in the familiar framework of the $\mathrm{\Lambda CDM}$ model augmented by baryons…

广义相对论与量子宇宙学 · 物理学 2025-08-13 Martín G. Richarte , Luiz F. Guimarães , Susana J. Landau , Júlio C. Fabris

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

We discuss models for the cosmological dark sector in which the energy density of a scalar field approximates Einstein's cosmological constant and the scalar field value determines the dark matter particle mass by a Yukawa coupling. A model…

天体物理学 · 物理学 2009-11-10 Glennys R. Farrar , P. J. E. Peebles

We consider three cosmological models with linear interaction between the dark components and obtain restrictions on the coupling constant in terms of the cosmographic parameters. It enables us to find constraints on the coupling constant…

宇宙学与河外天体物理 · 物理学 2016-04-27 Yu. L. Bolotin , V. A. Cherkaskiy , O. A. Lemets

In this work we explore two possible scenarios that can be considered to extend a recent proposed model by the authors known as reconstructed mimetic cosmology. This study is complemented with an statistical analysis for each case. The…

广义相对论与量子宇宙学 · 物理学 2021-07-23 Víctor H. Cárdenas , Miguel Cruz , Samuel Lepe

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

We present a model in which the dark matter particle is frozen-in at MeV scale. In this model, the mediator between the standard model sector and the dark sector can automatically provide a self-interaction for dark matter. The interaction…

高能物理 - 唯象学 · 物理学 2018-12-17 Haipeng An , Ran Huo , Wanqiang Liu

We consider an interacting field theory model that describes the dark energy - dark matter interaction. Only for a specific interaction term, this interacting field theory description has an equivalent interacting fluid description. For…

宇宙学与河外天体物理 · 物理学 2022-01-26 Joseph P Johnson , Archana Sangwan , S. Shankaranarayanan

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 showcase cosmology's ability to constrain long-range forces between dark matter particles. Specifically, we consider a fermionic dark matter interacting via a Yukawa-coupled light scalar, focusing on regimes where the dark forces are…

高能物理 - 唯象学 · 物理学 2025-11-14 Peter W. Graham , Harikrishnan Ramani , Olivier Simon , Erwin H. Tanin

A cosmological scenario where dark matter interacts with a variable vacuum energy for a spatially flat Friedmann-Robertson-Walker space-time is proposed and analysed to show that with a linear equation of state and a particular interaction…

广义相对论与量子宇宙学 · 物理学 2017-09-11 Emiliano Marachlian , Iván E. Sánchez G. , Osvaldo P. Santillán