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相关论文: Dissecting kinetically coupled quintessence: pheno…

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We consider a model where both dark energy and dark matter originate from the coupling of a scalar field with a non-conventional kinetic term to, both, a metric measure and a non-metric measure. An interacting dark energy/dark matter…

广义相对论与量子宇宙学 · 物理学 2015-06-11 Stefano Ansoldi , Eduardo I. Guendelman

We study a model of scalar field with a general non-minimal kinetic coupling to itself and to the curvature, and additional coupling to the Gauss Bonnet 4-dimensional invariant. The model presents rich cosmological dynamics and some of its…

高能物理 - 理论 · 物理学 2012-02-01 L. N. Granda

The coupling between dark sectors provides a possible 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 dark…

宇宙学与河外天体物理 · 物理学 2015-04-15 Weiqiang Yang , Lixin Xu

We examine an extension of the quintom scenario of dark energy, in which a canonical scalar field and a phantom field are coupled through a kinetic interaction. We perform a phase space analysis and show that the kinetic coupling gives rise…

高能物理 - 理论 · 物理学 2014-11-20 Emmanuel N. Saridakis , Joel M. Weller

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

Scalar fields coupled to dark matter by conformal or disformal transformations give rise to a general class of scalar-tensor theories which leads to a rich phenomenology in a cosmological setting. While this possibility has been studied…

广义相对论与量子宇宙学 · 物理学 2023-08-23 Gabriel Gómez

Motivated by the recent Dark Energy Spectroscopic Instrument (DESI) DR2 preference for dynamical dark energy, we study interacting dark energy models in which a canonical quintessence field couples to cold dark matter through a…

宇宙学与河外天体物理 · 物理学 2026-04-20 Stefan Antusch , Stephen F. King , Xin Wang

We consider the evolution of linear perturbations in models with a nonminimal coupling between dark matter and scalar field dark energy. Growth of matter inhomogeneities in two examples of such models proposed in the literature are…

天体物理学 · 物理学 2009-11-11 Tomi Koivisto

We investigate phenomenological interactions between dark matter and dark energy and constrain these models by employing the most recent cosmological data including the cosmic microwave background radiation anisotropies from Planck 2015,…

宇宙学与河外天体物理 · 物理学 2017-01-25 André A. Costa , Xiao-Dong Xu , Bin Wang , E. Abdalla

We assess the viability of successful reconstruction of the evolution of the dark energy equation of state using varying fundamental couplings, such as the fine structure constant or the proton-to-electron mass ratio. We show that the same…

宇宙学与河外天体物理 · 物理学 2015-06-03 P. P. Avelino , L. Losano , R. Menezes , J. C. R. E. Oliveira

We investigate the background dynamics when dark energy is coupled to dark matter in the universe described by Einstein cosmology and Loop Quantum Cosmology. We introduce a new general form of dark sector coupling, which presents us a more…

广义相对论与量子宇宙学 · 物理学 2008-12-18 Songbai Chen , Bin Wang , Jiliang Jing

Coupled dark sector models have gained significant attention, motivated by recent advances in cosmology and the pressing need to address unresolved puzzles. In this work, we study coupled scalar dark sector models inspired by…

高能物理 - 理论 · 物理学 2025-09-05 Saba Rahimy , Elsa M. Teixeira , Ivonne Zavala

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

In order to test the possible interaction between dark energy and dark matter, we investigate observational constraints on a phenomenological scenario, in which the ratio between the dark energy and matter densities is proportional to the…

宇宙学与河外天体物理 · 物理学 2015-05-20 Shuo Cao , Nan Liang , Zong-Hong Zhu

We analyze the coupled quintessence in the light of the linear dynamical systems theory, with two different interactions: i) proportional to the energy density of the dark energy and ii) proportional to the sum of the energy densities of…

广义相对论与量子宇宙学 · 物理学 2017-05-09 Fabrizio F. Bernardi , Ricardo G. Landim

Models with interacting dark energy can alleviate the cosmic coincidence problem by allowing dark matter and dark energy to evolve in a similar fashion. At a fundamental level, these models are specified by choosing a functional form for…

天体物理学 · 物理学 2008-11-26 Rogerio Rosenfeld

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 discuss models of ultralight scalar Dark Matter (DM) with linear and quadratic couplings to the Standard Model (SM). In addition to studying the phenomenology of linear and quadratic interactions separately, we examine their interplay.…

高能物理 - 唯象学 · 物理学 2023-11-27 Abhishek Banerjee , Gilad Perez , Marianna Safronova , Inbar Savoray , Aviv Shalit

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

We study the minimally and non-minimally coupled scalar field models as possible alternatives for dark energy, the mysterious energy component that is driving the accelerated expansion of the universe. After discussing the dynamics at both…

广义相对论与量子宇宙学 · 物理学 2019-12-03 Zahra Davari , Valerio Marra , Mohammad Malekjani