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相关论文: Interactions in the dark sector of the Universe

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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

We argue that interactions in the dark sector may have a crucial impact on the cosmological dynamics. In particular, the future cosmic evolution may be very different from that predicted by the LCDM model. An example is a scenario in which…

宇宙学与河外天体物理 · 物理学 2013-02-07 W. Zimdahl , C. Z. Vargas , W. S. Hipólito-Ricaldi

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 briefly discuss the intriguing case of a phenomenological non-gravitational coupling in the dark sector, where the interaction is parameterized as an energy transfer either from dark matter to dark energy or the opposite. We show that a…

宇宙学与河外天体物理 · 物理学 2017-07-04 Riccardo Murgia

We study observational signatures of non-gravitational interactions between the dark components of the cosmic fluid, which can be either due to creation of dark particles from the expanding vacuum or an effect of the clustering of a…

宇宙学与河外天体物理 · 物理学 2019-12-10 Micol Benetti , Welber Miranda , Humberto A. Borges , Cassio Pigozzo , Saulo Carneiro , Jailson S. Alcaniz

In this work we model two non-linear directly interacting scenarios in dark sector of the universe with the dimensionless parameter $\alpha$ and $\beta$, which dominate the energy exchange between dark energy and dark matter. The central…

宇宙学与河外天体物理 · 物理学 2025-04-08 Jiangang Kang

Since physics of the dark sector components of the Universe is not yet well-understood, the phenomenological studies of non-minimal interaction in the dark sector could possibly pave the way to theoretical and experimental progress in this…

宇宙学与河外天体物理 · 物理学 2021-08-03 Suresh Kumar

We discuss the evolution of density perturbations of dark matter and dark energy in cosmological models which admit future singularities in a finite time. Up to now geometrical tests of the evolution of the universe do not differentiate…

宇宙学与河外天体物理 · 物理学 2015-04-10 Tomasz Denkiewicz

We revise the cosmological interaction between dark energy and dark matter. More precisely, we focus on models that support compartmentalization or co-existence in the dark sector of the universe. Within the framework of a homogeneous and…

广义相对论与量子宇宙学 · 物理学 2024-11-25 Andronikos Paliathanasis , Kevin Duffy , Amlan Halder , Amare Abebe

We propose a general class of interacting models in which the interaction between the CDM component and $\Lambda$ is parameterized by an arbitrary function of the cosmic scale factor $\epsilon(a)$. Differently from other dynamical $\Lambda$…

宇宙学与河外天体物理 · 物理学 2010-04-06 F. E. M. Costa , J. S. Alcaniz

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

We study the effect of an explicit interaction between two scalar fields components describing dark matter in the context of a recent proposal framework for interaction. We find that, even assuming a very small coupling, it is sufficient to…

宇宙学与河外天体物理 · 物理学 2020-10-28 Victor H. Cardenas , Samuel Lepe

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

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

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

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

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

A cosmological model is proposed for the current Universe consisted of non-interacting baryonic matter and interacting dark components. The dark energy and dark matter are coupled through their effective barotropic indexes, which are…

天体物理学 · 物理学 2009-06-15 Luis P. Chimento , Monica Forte , Gilberto M. Kremer

We investigate a phenomenological non-gravitational coupling between dark energy and dark matter, where the interaction in the dark sector is parameterized as an energy transfer either from dark matter to dark energy or the opposite. The…

宇宙学与河外天体物理 · 物理学 2016-04-11 Riccardo Murgia , Stefano Gariazzo , Nicolao Fornengo
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