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相关论文: Can dark matter-dark energy interaction alleviate …

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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

Interacting dark energy (IDE) models, in which dark matter (DM) and dark energy (DE) exchange energy through a non-gravitational interaction, have long been proposed as candidates to address key challenges in modern cosmology. These include…

广义相对论与量子宇宙学 · 物理学 2025-10-20 Marcel van der Westhuizen , Amare Abebe , Eleonora Di Valentino

Interacting dark energy models have been suggested as alternatives to the standard cosmological model, $\Lambda$CDM. We focus on a phenomenologically interesting class of dark scattering models that is characterised by pure momentum…

宇宙学与河外天体物理 · 物理学 2023-02-08 Maria Tsedrik , Chiara Moretti , Pedro Carrilho , Federico Rizzo , Alkistis Pourtsidou

The coupled dark energy models, in which the quintessence scalar field nontrivially couples to the cold dark matter, have been proposed to explain the coincidence problem. In this paper we study the perturbations of coupled dark energy…

宇宙学与河外天体物理 · 物理学 2010-04-22 Jun-Qing Xia

We investigate various scenarios which include interaction forms between dark matter and dark energy that exhibit sign reverse, namely where the transfer of energy between the dark fluids changes sign during evolution. We study the…

宇宙学与河外天体物理 · 物理学 2019-11-06 Supriya Pan , Weiqiang Yang , Chiranjeeb Singha , Emmanuel N. Saridakis

The $H_0$ tension between low- and high- redshift measurements is definitely a serious issue faced by current cosmologists since it ranges from 4$\sigma$ to 6$\sigma$. To relieve this tension, in this paper we propose a new interacting dark…

宇宙学与河外天体物理 · 物理学 2024-05-31 Yan-Hong Yao , Xin-He Meng

We study the interacting dark energy model with time varying dark energy equation of state. We examine the stability in the perturbation formalism and the degeneracy among the coupling between dark sectors, the time-dependent dark energy…

宇宙学与河外天体物理 · 物理学 2015-05-27 Xiao-Dong Xu , Jian-Hua He , Bin Wang

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 study a cosmological model based on the holographic principle that allows an interaction between dark energy and dark matter with a Hubble infrared cutoff. We adopt an agnostic point of view with respect to the form of the interaction…

广义相对论与量子宇宙学 · 物理学 2022-02-22 Celia Escamilla-Rivera , Aldo Gamboa

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 use observations of cosmic microwave background anisotropies, supernova luminosities and the baryon acoustic oscillation signal in the galaxy distribution to constrain the cosmological parameters in a simple interacting dark energy model…

宇宙学与河外天体物理 · 物理学 2010-03-18 Jussi Valiviita , Roy Maartens , Elisabetta Majerotto

Dark energy might interact with dark matter in a direct, non-gravitational way, which can help remedy several theoretical defects. In order to find out the properties of interacting dark energy models, it is necessary to investigate the…

宇宙学与河外天体物理 · 物理学 2019-05-15 Ji-Ping Dai , Junqing Xia

The coincidence problem of late cosmic acceleration gets significantly alleviated when a suitable interaction between matter and dark energy, either of phantom type or not, enters the picture. We show that a class of models featuring this…

天体物理学 · 物理学 2007-05-23 German Olivares , Diego Pavon , Fernando Atrio-Barandela

We consider a recently proposed model in which dark matter interacts with a thermal background of dark radiation. Dark radiation consists of relativistic degrees of freedom which allow larger values of the expansion rate of the universe…

宇宙学与河外天体物理 · 物理学 2018-01-24 Manuel A. Buen-Abad , Martin Schmaltz , Julien Lesgourgues , Thejs Brinckmann

We investigate a spatially flat Friedmann-Robertson-Walker (FRW) scenario with two interacting components, dark matter and variable vacuum energy (VVE) densities, plus two decoupled components, one is a baryon term while the other behaves…

广义相对论与量子宇宙学 · 物理学 2015-08-21 Iván E. Sánchez G

We investigate a universe filled with interacting dark matter, holographic dark energy, and dark radiation for the spatially flat Friedmann-Robertson-Walker (FRW) spacetime. We use a linear interaction to reconstruct all the component…

广义相对论与量子宇宙学 · 物理学 2013-04-12 Luis P. Chimento , Martín G. Richarte

We study dynamical behaviors of the dark energy models interacting with dark matter and unparticle in the standard flat FRW cosmology. We considered four different interacting models and examined the stability of the critical points. We…

广义相对论与量子宇宙学 · 物理学 2010-04-15 Songbai Chen , Jiliang Jing

The interaction between dark matter and dark energy can be incorporated into field theory models of dark energy that have proved successful in alleviating the coincidence problem. We review recent advances in this field, including new…

宇宙学与河外天体物理 · 物理学 2024-02-02 B Wang , E Abdalla , F Atrio-Barandela , D Pavón

A component of dark energy has been recently proposed to explain the current acceleration of the Universe. Unless some unknown symmetry in Nature prevents or suppresses it, such a field may interact with the pressureless component of dark…

天体物理学 · 物理学 2010-05-12 J. F. Jesus , R. C. Santos , J. S. Alcaniz , J. A. S. Lima

We study a two-parameter extension of the cosmological standard model $\Lambda$CDM in which cold dark matter interacts with a new form of dark radiation. The two parameters correspond to the energy density in the dark radiation fluid…

宇宙学与河外天体物理 · 物理学 2016-03-14 Julien Lesgourgues , Gustavo Marques-Tavares , Martin Schmaltz