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相关论文: Dissecting kinetically coupled quintessence: pheno…

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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

We investigate a cosmological model in which dark energy, represented by a quintessential scalar field, is coupled to a dark-matter perfect fluid in the spatially flat Friedmann-Robertson-Walker Universe. This allows an energy exchange in…

广义相对论与量子宇宙学 · 物理学 2023-08-22 Yousef Bisabr

We investigate a scenario where a dark energy quintessence field $\phi$ with positive kinetic energy is coupled with dark matter. With two different self-interaction potentials for the field and a particular choice of the coupling function,…

宇宙学与河外天体物理 · 物理学 2025-12-22 Amlan Chakraborty , Prolay K. Chanda , Subinoy Das , Koushik Dutta

The existence of dark energy is essential to explain the cosmic accelerated expansion. We consider a homogenous interacting tachyonic scalar field as a possible candidate for the dynamical dark energy. The interaction between the tachyonic…

广义相对论与量子宇宙学 · 物理学 2023-05-02 V K Ojha , Adithya A Rao , S D Pathak

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

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

A component of dark energy has been recently proposed to explain the current acceleration of the Universe. Unless some unknown symmetry in Nature prevents or suppresses it, such a field may interact with the pressureless component of dark…

天体物理学 · 物理学 2010-05-12 J. F. Jesus , R. C. Santos , J. S. Alcaniz , J. A. S. Lima

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

This study explores the dynamics and phase-space behavior of a multi-component dark energy model, where the dark sector consists of a minimally coupled canonical scalar field and the cosmological constant, using a dynamical system analysis…

广义相对论与量子宇宙学 · 物理学 2025-05-16 Prasanta Sahoo , Nandan Roy , Himadri Shekhar Mondal

In standard cosmologies, dark energy interacts only gravitationally with dark matter. An extension to this picture is interacting quintessence (IQ) model, where scalar field coupled directly to cold dark matter. The percentage deviation is…

宇宙学与河外天体物理 · 物理学 2019-10-23 Azam Hussain

We investigate a string-inspired dark energy scenario featuring a scalar field with a coupling to the Gauss-Bonnet invariant. Such coupling can trigger the onset of late dark energy domination after a scaling matter era. The universe may…

高能物理 - 理论 · 物理学 2008-11-26 Tomi Koivisto , David F. Mota

We constrain interacting dark matter and dark energy (IDMDE) models using a 450-degree-square cosmic shear data from the Kilo Degree Survey (KiDS) and the angular power spectra from Planck's latest cosmic microwave background measurements.…

宇宙学与河外天体物理 · 物理学 2018-02-27 Rui An , Chang Feng , Bin Wang

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

We propose a new dark energy model for solving the cosmological fine-tuning and coincidence problems. A default assumption is that the fine-tuning problem disappears if we do not interpret dark energy as vacuum energy. The key idea to…

宇宙学与河外天体物理 · 物理学 2020-03-27 S. X. Tián

Interactions between dark matter and dark energy which result in a power-law behavior (with respect to the cosmic scale factor) of the ratio between the energy densities of the dark components (thus generalizing the LCDM model) have been…

宇宙学与河外天体物理 · 物理学 2012-06-14 David R. Castro , Hermano Velten , Winfried Zimdahl

We consider a field theory model of coupled dark energy which treats dark energy as a three-form field and dark matter as a spinor field. By assuming the effective mass of dark matter as a power-law function of the three-form field and…

宇宙学与河外天体物理 · 物理学 2018-04-04 YanHong Yao , YangJie Yan , XinHe Meng

In this paper we study a model of interacting dark energy - dark matter where the ratio between these components is not constant, changing from early to late times in such a way that the model can solve or alleviate the cosmic coincidence…

宇宙学与河外天体物理 · 物理学 2022-04-12 J. F. Jesus , A. A. Escobal , D. Benndorf , S. H. Pereira

We study the cosmic evolution of an interacting scalar field radiation model, in which a minimally coupled scalar field exchanges energy with the radiation sector through an exponential coupling. Extending previous formulations, a…

宇宙学与河外天体物理 · 物理学 2026-01-01 Dorian Araya , Felipe Herrera , Nelson Videla

In this work, we study two scalar field driven dark energy models characterized by the axion potential and the inverse power law potential, each coupled to dark matter through a momentum exchange interaction. By formulating the dynamics as…

宇宙学与河外天体物理 · 物理学 2025-06-27 Prasanta Sahoo , Nandan Roy , Himadri Shekhar Mondal

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