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相关论文: Dissecting kinetically coupled quintessence: pheno…

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We consider a cosmology in which dark matter and a quintessence scalar field responsible for the acceleration of the Universe are allowed to interact. Allowing for both conformal and disformal couplings, we perform a global analysis of the…

宇宙学与河外天体物理 · 物理学 2017-02-22 Carsten van de Bruck , Jurgen Mifsud , Jack Morrice

The main goal of this work is to propose a generalized model of interacting dark energy which allows for the kinetic term of a scalar field to couple to the matter species a priori in the action. We derive the modified field equations, and…

广义相对论与量子宇宙学 · 物理学 2019-04-01 Bruno J. Barros

We present a scenario in which a scalar field dark energy is coupled to the trace of the energy momentum tensor of the baryonic matter fields. In the slow-roll regime, this interaction could give rise to the cosmological features of dark…

宇宙学与河外天体物理 · 物理学 2011-02-02 Alejandro Aviles , Jorge L. Cervantes-Cota

We present and examine a kinetically coupled tachyon dark energy model, where a tachyon scalar field interacts with the matter sector. More specifically, we deduce this cosmological setting from a generalised interacting dark energy model…

广义相对论与量子宇宙学 · 物理学 2024-12-31 Francesco Pace , Alberto Rozas-Fernández , Özgen Tunç Türker

We perform a detailed analysis of a theoretically motivated dark energy quintessence model which interacts with the dark matter sector of the universe. Utilising the current observational datasets from the Cosmic Microwave Background,…

广义相对论与量子宇宙学 · 物理学 2025-09-12 Atul Ashutosh Samanta , Abhijith Ajith , Sukanta Panda

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

We do a detailed analysis of a well-theoretically motivated interacting dark energy scalar field model with a time-varying interaction term. Using current cosmological datasets from CMB, BAO, Type Ia Supernova, $H(z)$ measurements from…

宇宙学与河外天体物理 · 物理学 2024-06-11 Trupti Patil , Ruchika , Sukanta Panda

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

We investigate an interacting dark energy-dark matter model within the quintessence framework, characterized by the coupling term $Q_0 = \alpha \kappa \rho_m \dot{\phi} \left[1 - \beta R/(6H^2) \right]$, and the scalar field evolves under…

广义相对论与量子宇宙学 · 物理学 2025-10-28 Anirban Chatterjee , Yungui Gong

The coupling between the dark components provides a new approach to mitigate the coincidence problem of cosmological standard model. In this paper, dark energy is treated as a fluid with a constant equation of state, whose coupling with…

宇宙学与河外天体物理 · 物理学 2014-08-18 Weiqiang Yang , Lixin Xu

We explore quintessence models of dark energy which exhibit non-minimal coupling between the dark matter and the dark energy components of the cosmic fluid. The kind of coupling chosen is inspired in scalar-tensor theories of gravity. We…

天体物理学 · 物理学 2009-11-13 Tame Gonzalez , Genly Leon , Israel Quiros

We study a coupled quintessence model in which the interaction with the dark matter sector is a function of the quintessence potential. Such a coupling can arise from a field dependent mass term for the dark matter field. The dynamical…

宇宙学与河外天体物理 · 物理学 2011-01-20 Laura Lopez-Honorez , Olga Mena , Grigoris Panotopoulos

We investigate a cosmological model in which dark energy, represented by a quintessential scalar field, is directly coupled to a dark-matter perfect fluid. We are interested in solutions of cosmological relevance, namely those for which a…

广义相对论与量子宇宙学 · 物理学 2022-12-07 Robertus Potting , Paulo M. Sá

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

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 the evolution of linear perturbations in a quintessence model in which the scalar field is non-minimally coupled to cold dark matter. We consider the effects of this coupling on both cosmic microwave background temperature…

天体物理学 · 物理学 2009-02-18 Seokcheon Lee , Guo-Chin Liu , Kin-Wang Ng

We consider scalar field models of dark energy interacting with dark matter through a coupling proportional to the contraction of the four-derivative of the scalar field with the four-velocity of the dark matter fluid. The coupling is…

广义相对论与量子宇宙学 · 物理学 2018-02-07 Jibitesh Dutta , Wompherdeiki Khyllep , Nicola Tamanini

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

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

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
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