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The coupled dark energy models, in which the quintessence scalar field nontrivially couples to the cold dark matter, have been proposed to explain the coincidence problem. In this paper we study the perturbations of coupled dark energy…

宇宙学与河外天体物理 · 物理学 2010-04-22 Jun-Qing Xia

Models with dark energy decaying into dark matter have been proposed in Cosmology to solve the coincidence problem. We study the effect of such coupling on the cosmic microwave background temperature anisotropies. The interaction changes…

天体物理学 · 物理学 2008-11-26 German Olivares , Fernando Atrio-Brandela , Diego Pavon

Dark energy perturbation affects the growth of matter perturbations even in scenarios with noninteracting dark energy. We investigate the Integrated Sachs Wolfe (ISW) effect in various canonical scalar field models with perturbed dark…

宇宙学与河外天体物理 · 物理学 2013-05-30 H. K. Jassal

Dark energy interacting with dark matter is a promising model to solve the cosmic coincidence problem. We study the signature of such interaction on large scale cosmic microwave background (CMB) temperature anisotropies. Based on the detail…

广义相对论与量子宇宙学 · 物理学 2009-11-06 Jian-Hua He , Bin Wang , Pengjie Zhang

In this paper, we introduce a new interacting mechanism within the dark sector, encompassing both dark energy and dark matter, while grounding our analysis in the familiar framework of the $\mathrm{\Lambda CDM}$ model augmented by baryons…

广义相对论与量子宇宙学 · 物理学 2025-08-13 Martín G. Richarte , Luiz F. Guimarães , Susana J. Landau , Júlio C. Fabris

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

Interacting dark matter-dark energy (IDMDE) models can be taken to account as one of the present challenges that may affect the cosmic structures. In this work, we study the integrated Sachs-Wolfe (ISW) effect in IDMDE models. To this end,…

宇宙学与河外天体物理 · 物理学 2022-11-29 Mina Ghodsi Yengejeh , Saeed Fakhry , Javad T. Firouzjaee , Hojatollah Fathi

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

In trace-free Einstein gravity, the stress-energy tensor of matter is not necessarily conserved and so the theory offers a natural framework for interacting dark energy models where dark energy has a constant equation of state $w=-1$. We…

广义相对论与量子宇宙学 · 物理学 2022-07-29 Marco de Cesare , Edward Wilson-Ewing

The physics of the dark sector has remained one of the controversial areas of modern cosmology at present and hence it naturally attracts massive attention to the scientific community. With the developments of the astronomical data, the…

宇宙学与河外天体物理 · 物理学 2020-06-03 Weiqiang Yang , Supriya Pan , Eleonora Di Valentino , Bin Wang , Anzhong Wang

We extensively study the evolution and distinct signatures of cosmological models, in which dark energy interacts directly with dark matter. We first focus on the imprints of these coupled models on the cosmic microwave background…

宇宙学与河外天体物理 · 物理学 2017-11-15 Jurgen Mifsud , Carsten van de Bruck

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

There is no unique way to describe the dark energy-dark matter interaction, as we have little information about the nature and dynamics of the dark sector. Hence, in many of the phenomenological dark matter fluid interaction models in the…

广义相对论与量子宇宙学 · 物理学 2021-01-13 Joseph P Johnson , S. Shankaranarayanan

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

The impact of large-scale magnetic fields on the interplay between the ordinary and integrated Sachs-Wolfe effects is investigated in the presence of a fluctuating dark energy component. The modified initial conditions of the…

宇宙学与河外天体物理 · 物理学 2010-04-29 Massimo Giovannini

We introduce a new class of interacting dark sector models that couple the intrinsic entropy of dark matter to scalar field dark energy. Using the Lagrangian formulation for relativistic perfect fluids, we construct consistent covariant…

宇宙学与河外天体物理 · 物理学 2026-03-12 Erik Jensko , Elsa M. Teixeira , Vivian Poulin

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

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

Interacting dark energy models have been suggested as alternatives to the standard cosmological model, $\Lambda$CDM. We focus on a phenomenologically interesting class of dark scattering models that is characterised by pure momentum…

宇宙学与河外天体物理 · 物理学 2023-02-08 Maria Tsedrik , Chiara Moretti , Pedro Carrilho , Federico Rizzo , Alkistis Pourtsidou

We consider an interacting field theory model that describes the dark energy - dark matter interaction. Only for a specific interaction term, this interacting field theory description has an equivalent interacting fluid description. For…

宇宙学与河外天体物理 · 物理学 2022-01-26 Joseph P Johnson , Archana Sangwan , S. Shankaranarayanan
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