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相关论文: Cosmological model with interactions in the dark s…

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We model the cosmological substratum by a viscous fluid that is supposed to provide a unified description of the dark sector and pressureless baryonic matter. In the homogeneous and isotropic background the \textit{total} energy density of…

宇宙学与河外天体物理 · 物理学 2015-05-20 W Zimdahl , W S Hipólito-Ricaldi , H E S Velten

Within our recent thermodynamic model of gravity the dark energy is identified with the energy of collective gravitational interactions of all particles in the universe, which is missing in the standard treatments. For a simple model…

综合物理 · 物理学 2014-04-24 Merab Gogberashvili , Igor Kanatchikov

Interactions inside the cosmological dark sector influence the cosmological dynamics. As a consequence, the future evolution of the Universe may be different from that predicted by the $\Lambda$CDM model. We review main features of several…

宇宙学与河外天体物理 · 物理学 2014-04-30 W. Zimdahl

We consider the dark energy model with barotropic equation of state, which interacts with dark matter through gravitation and another force, causing the energy-momentum exchange between them. Both components are described in approximation…

广义相对论与量子宇宙学 · 物理学 2016-09-07 R. Neomenko , B. Novosyadlyj

We study a holographic cosmological model in which the infrared cutoff is set by the Ricci's length and dark matter and dark energy do not evolve on their own but interact non-gravitationally with each other. This greatly alleviates the…

宇宙学与河外天体物理 · 物理学 2011-02-25 Ivan Duran , Diego Pavon

We consider holographic cosmological models of dark energy in which the infrared cutoff is set by the Hubble's radius. We show that any interacting dark energy model with a matter like term able to alleviate the coincidence problem (i.e.,…

宇宙学与河外天体物理 · 物理学 2012-07-03 Iván Durán , Luca Parisi

Any non-gravitational coupling between dark matter and dark energy modifies the cosmological dynamics. Interactions in the dark sector are considered to be relevant to address the coincidence problem. Moreover, in various models the…

宇宙学与河外天体物理 · 物理学 2015-06-04 W. Zimdahl

The dark side of the universe is mysterious and its nature is still unknown. In fact, this poses perhaps as the biggest challenge in the modern cosmology. The two components of the dark sector (dark matter and dark energy) correspond today…

广义相对论与量子宇宙学 · 物理学 2017-02-21 Ricardo C. G. Landim

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

We consider a non-linear interaction between the dark matter and dark energy components of the universe. In particular, within the FLRW geometry, where dark matter is described by a dust fluid and dark energy by an ideal gas with a constant…

宇宙学与河外天体物理 · 物理学 2025-09-24 Marcel van der Westhuizen , David Figueruelo , Rethabile Thubisi , Shambel Sahlu , Amare Abebe , Andronikos Paliathanasis

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

It is argued that cosmological models that feature a flow of energy from dark energy to dark matter may solve the coincidence problem of late acceleration (i.e., "why the energy densities of both components are of the same order precisely…

广义相对论与量子宇宙学 · 物理学 2009-02-06 Sergio del Campo , Ramon Herrera , Diego Pavon

The introduction of an interaction for dark energy to the standard cosmology offers a potential solution to the cosmic coincidence problem. We examine the conditions on the dark energy density that must be satisfied for this scenario to be…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Micheal S. Berger , Hamed Shojaei

We propose a cosmological model that makes a significant step toward solving the coincidence problem of the near similarity at the present of the dark energy and dark matter components. Our cosmology has the following properties: a) among…

天体物理学 · 物理学 2008-11-26 Luca Amendola , Domenico Tocchini-Valentini

Scalar cosmological perturbations are investigated in the framework of a model with interacting dark energy and dark matter. In addition to these constituents, the inhomogeneous Universe is supposed to be filled with the standard…

广义相对论与量子宇宙学 · 物理学 2015-07-24 Maxim Eingorn , Claus Kiefer

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

The paper deals with a theoretical model for interacting dark energy. The interaction between the cold dark matter (dust) and the dark energy has been assumed to be non-gravitational in nature. Exact analytic cosmological solutions are…

广义相对论与量子宇宙学 · 物理学 2015-07-31 Supriya Pan , Subhra Bhattacharya , Subenoy Chakraborty

New systematic classification of cosmological models of the present Universe is introduced. After making the comparison of these models with all existing observational data three viable models remain: the cold dark matter model with the…

天体物理学 · 物理学 2007-05-23 A. A. Starobinsky

We investigate interacting dark energy models in the framework of fractal cosmology. We discuss a fractal FRW universe filled with the dark energy and dark matter which interact with each other. We obtain the equation for the relative…

宇宙学与河外天体物理 · 物理学 2012-05-29 O. A. Lemets , D. A. Yerokhin

A model for a flat homogeneous and isotropic Universe composed of dark energy, dark matter, neutrinos, radiation and baryons is analyzed. The fields of dark matter and neutrinos are supposed to interact with the dark energy. The dark energy…

广义相对论与量子宇宙学 · 物理学 2008-11-26 G. M. Kremer