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(Abridged) Present cosmological constraints and the absence of a direct detection and identification of any dark matter particle candidate leave room to the possibility that the dark sector of the Universe be actually more complex than it…

宇宙学与河外天体物理 · 物理学 2015-06-04 Marco Baldi

Dark energy and dark matter are the dominant sources in the evolution of the late universe. They are currently only indirectly detected via their gravitational effects, and there could be a coupling between them without violating…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Christian G. Boehmer , Gabriela Caldera-Cabral , Ruth Lazkoz , Roy Maartens

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

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

In this review we consider in detail different theoretical topics associated with interaction in the dark sector. We study linear and nonlinear interactions which depend on the dark matter and dark energy densities. We consider a number of…

宇宙学与河外天体物理 · 物理学 2015-03-25 Yu. L. Bolotin , A. Kostenko , O. A. Lemets , D. A. Yerokhin

Models where Dark Matter and Dark Energy interact with each other have been proposed to solve the coincidence problem. We review the motivations underlying the need to introduce such interaction, its influence on the background dynamics and…

宇宙学与河外天体物理 · 物理学 2016-08-24 B. Wang , E. Abdalla , F. Atrio-Barandela , D. Pavon

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

In this paper we have considered an interacting model of dark energy and have looked into the evolution of the dark sectors. By solving the perturbation equations numerically, we have studied the imprints on the growth of matter as well as…

广义相对论与量子宇宙学 · 物理学 2024-05-30 Srijita Sinha , Manisha Banerjee , Sudipta Das

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

In this talk, I have discussed the implications of a multi-component nature of cosmic Dark Matter for the observational bounds on possible long-range fifth-forces mediated by a Dark Energy scalar field. By assuming a simple internal…

宇宙学与河外天体物理 · 物理学 2013-04-19 Marco Baldi

We consider a cosmological model with an interaction between dark matter and dark energy which leaves the background cosmology unaffected and only affects the evolution of the perturbations. This is achieved by introducing a coupling given…

宇宙学与河外天体物理 · 物理学 2019-08-21 Mahnaz Asghari , Jose Beltran Jimenez , Shahram Khosravi , David F. Mota

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

Cosmological analysis based on currently available observations are unable to rule out a sizeable coupling between dark energy and dark matter. However, the signature of the coupling is not easy to grasp, since the coupling is degenerate…

宇宙学与河外天体物理 · 物理学 2011-03-22 Jian-Hua He , Bin Wang , Elcio Abdalla

The covariant generalizations of the background dark sector coupling suggested in G. Mangano, G. Miele and V. Pettorino, Mod. Phys. Lett. A 18, 831 (2003) are considered. The evolution of perturbations is studied with detailed attention to…

广义相对论与量子宇宙学 · 物理学 2011-04-22 N. A. Koshelev

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

Diverse cosmological and astrophysical observations strongly hint at the presence of dark matter and dark energy in the Universe. One of the main goals of Cosmology is to explain the nature of these two components. It may well be that both…

高能物理 - 理论 · 物理学 2023-07-10 Carsten van de Bruck , Gaspard Poulot , Elsa M. Teixeira

It is a puzzle why the densities of dark matter and dark energy are nearly equal today when they scale so differently during the expansion of the universe. This conundrum may be solved if there is a coupling between the two dark sectors. In…

高能物理 - 唯象学 · 物理学 2009-07-09 D. Comelli , M. Pietroni , A. Riotto

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

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

We study the interaction between dark matter and dark energy, with dark energy described by a scalar field having a double exponential effective potential. We discover conditions under which such a scalar field driven solution is a late…

广义相对论与量子宇宙学 · 物理学 2015-08-06 Vartika Gupta , Rakesh Kabir , Amitabha Mukherjee , Daksh Lohiya
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