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相关论文: Interacting dark matter and q-deformed dark energy…

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We propose a novel coupled dark energy model which is assumed to occur as a q-deformed scalar field and investigate whether it will provide an expanding universe phase. We consider the q-deformed dark energy as coupled to dark matter…

广义相对论与量子宇宙学 · 物理学 2016-12-09 Emre Dil

In this work we investigate the evolution of a Universe consisted of a scalar field, a dark matter field and non-interacting baryonic matter and radiation. The scalar field, which plays the role of dark energy, is non-minimally coupled to…

广义相对论与量子宇宙学 · 物理学 2007-05-23 J. B. Binder , G. M. Kremer

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

We analyze a universe filled with interacting dark matter, a scalar field accommodated as dark radiation along with dark energy plus a decoupled radiation term within the framework of spatially flat Friedmann-Robertson-Walker (FRW)…

广义相对论与量子宇宙学 · 物理学 2013-08-06 Luis P. Chimento , Martín G. Richarte

The cosmological history and evolution are examined for gravitational models with interaction in the dark sector of the universe. In particular, we consider the dark energy to be described by a phantom scalar field and the dark matter $\rho…

广义相对论与量子宇宙学 · 物理学 2024-12-11 Andronikos Paliathanasis , Amlan Halder , Genly Leon

The cosmological model of dark energy interacting with cold dark matter without coupling to the baryonic matter, is studied in the background of both classical Einstein and loop quantum cosmology. We consider two types of interacting…

宇宙学与河外天体物理 · 物理学 2014-11-20 Song Li , Yongge Ma

We investigate the interacting dark sector composed of dark matter, dark energy, and dark radiation for a spatially flat Friedmann-Robertson-Walker (FRW) background by introducing a three-dimensional internal space spanned by the…

宇宙学与河外天体物理 · 物理学 2015-06-18 Luis P. Chimento , Martín G. Richarte

We investigate the interaction between the dark sectors from the point of view of a dynamical system analysis. A general setup for interacting dark energy models that incorporates both quintessence and phantom fields through a switch…

广义相对论与量子宇宙学 · 物理学 2025-05-16 Chonticha Kritpetch , Nandan Roy , Narayan Banerjee

We explore a cosmological framework in which a Gauss-Bonnet (GB) coupled scalar field, acting as dark energy, interacts with a fermionic dark matter field through a coupling obtained from the point of view of particle physics. This setup is…

宇宙学与河外天体物理 · 物理学 2026-04-06 Simran Arora , Saddam Hussain , Benjamin Rose , Anzhong Wang

In this paper we study new cosmological models involving new forms of non-gravitational interaction between cold dark matter and dark energy. The main purpose is to demonstrate the applicability of the forms of interaction to the problem in…

广义相对论与量子宇宙学 · 物理学 2017-08-09 Martiros Khurshudyan , Asatur Khurshudyan

An interaction between dark matter and dark energy is usually introduced by a phenomenological modification of the matter conservation equations, while the Einstein equations are left unchanged. Starting from some general and fundamental…

广义相对论与量子宇宙学 · 物理学 2015-09-16 Nicola Tamanini

It may well happen that the two main components of the dark sector of the Universe, dark matter and dark energy, do not evolve separately but interact nongravitationally with one another. However, given our current lack of knowledge on the…

广义相对论与量子宇宙学 · 物理学 2015-07-02 Sergio del Campo , Ramon Herrera , Diego Pavon

In this work it is investigated general models with interactions between two canonical scalar fields and between one non-canonical (tachyon-type) and one canonical scalar field. The potentials and couplings to the gravity are selected…

广义相对论与量子宇宙学 · 物理学 2013-10-15 Rudinei C. de Souza , Gilberto M. Kremer

Dark energy and dark matter are only indirectly measured via their gravitational effects. It is possible that there is an exchange of energy within the dark sector, and this offers an interesting alternative approach to the coincidence…

广义相对论与量子宇宙学 · 物理学 2009-03-24 Gabriela Caldera-Cabral , Roy Maartens , L. Arturo Urena-Lopez

We investigate the impact on the classical dynamics of dark matter particles and dark energy of a non-minimal coupling in the dark sector, assuming that the mass of the dark matter particles is coupled to a dark energy scalar field. We show…

宇宙学与河外天体物理 · 物理学 2015-05-06 P. P. Avelino

In this work we study a phenomenological non-gravitational interaction between dark matter and dark energy. The scenario studied in this work extends the usual interaction model proportional to the derivative of the dark component density…

宇宙学与河外天体物理 · 物理学 2018-08-14 Josue De-Santiago , Iván E. Sánchez G. , David Tamayo

We consider a cosmological scenario endowed with an interaction between the universe's dark components $-$ dark matter and dark energy. Specifically, we assume the dark matter component to be a pressure-less fluid, while the dark energy…

广义相对论与量子宇宙学 · 物理学 2021-08-03 Andronikos Paliathanasis , Genly Leon , Wompherdeiki Khyllep , Jibitesh Dutta , Supriya Pan

Dark matter interacts gravitationally, but it presumably interacts weakly through other channels, especially with respect to regular luminous matter. We look at different ways in which dark matter may couple to other fields. We briefly…

综合物理 · 物理学 2018-09-27 Kevin J. Ludwick

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

In this work it is investigated the evolution of a Universe where a scalar field, non-minimally coupled to space-time curvature, plays the role of quintessence and drives the Universe to a present accelerated expansion. A non-relativistic…

广义相对论与量子宇宙学 · 物理学 2009-11-11 J. B. Binder , G. M. Kremer
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