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In this study, we analyze the dynamics of the interaction between dark matter and curvature-driven dark energy in viable $f(R)$ gravity models using the framework of dynamical system analysis. We incorporate this interaction by introducing…

广义相对论与量子宇宙学 · 物理学 2024-03-11 Anirban Chatterjee , Rahul Roy , Sayantan Dey , Abhijit Bandyopadhyay

We explore the interaction between dark matter and curvature-driven dark energy within viable $f(R)$ gravity models, employing the phase-space analysis approach of linear stability theory. By incorporating an interacting term, denoted as…

广义相对论与量子宇宙学 · 物理学 2024-04-04 Anirban Chatterjee

In this work, we investigate the dynamics of the interacting dark energy and dark matter in viable models of $f(R)$ gravity by using a standard framework of dynamical system analysis. A simple form of the interacting dark energy $Q=3\alpha…

广义相对论与量子宇宙学 · 物理学 2021-09-22 Daris Samart , Bhuddhanubhap Silasan , Phongpichit Channuie

This work explores the dynamical stability of cosmological models where dark matter and dark energy can non-minimally couple to spacetime (scalar) curvature. Two different scenarios are presented here. In the initial case, only dark matter…

广义相对论与量子宇宙学 · 物理学 2023-11-07 Saddam Hussain , Anirban Chatterjee , Kaushik Bhattacharya

In the present study, we investigate the interaction between dark energy and dark matter, particularly emphasizing the effects of curvature in the realm of Friedmann-Lemaitre-Robertson-Walker (FLRW) space-time. We examine the system by…

广义相对论与量子宇宙学 · 物理学 2023-07-07 Trupti Patil , Sukanta Panda

Modified gravity theories have received increased attention lately to understand the late time acceleration of the universe. This viewpoint essentially modifies the geometric components of the universe. Among numerous extension to…

广义相对论与量子宇宙学 · 物理学 2019-05-23 Parth Shah , Gauranga C. Samanta

In this work, we explore the behavior of interacting dark energy and dark matter within a model of $f(Q)$ gravity, employing a standard framework of dynamical system analysis. We consider the power-law $f(Q)$ model incorporating with two…

广义相对论与量子宇宙学 · 物理学 2025-03-10 Gaurav N. Gadbail , Simran Arora , Phongpichit Channuie , P. K. Sahoo

We investigate an interacting quintessence dark energy - dark matter scenario and its impact on structure formation by analyzing the evolution of scalar perturbations. The interaction is introduced by incorporating a non-zero source term…

广义相对论与量子宇宙学 · 物理学 2025-02-06 Anirban Chatterjee , Abhijit Bandyopadhyay , Debasish Majumdar

We investigate an interacting dark energy-dark matter model within the quintessence framework, characterized by the coupling term $Q_0 = \alpha \kappa \rho_m \dot{\phi} \left[1 - \beta R/(6H^2) \right]$, and the scalar field evolves under…

广义相对论与量子宇宙学 · 物理学 2025-10-28 Anirban Chatterjee , Yungui Gong

Motivated by the cosmological constant and the coincidence problems, we consider a cosmological model where the dark sectors are interacting together through a phenomenological decay law $\dot{\rho}_{\Lambda}=Q\rho_{\Lambda}^n$ in a FRW…

宇宙学与河外天体物理 · 物理学 2015-06-16 Vincent Poitras

We study dynamical behaviors of the dark energy models interacting with dark matter and unparticle in the standard flat FRW cosmology. We considered four different interacting models and examined the stability of the critical points. We…

广义相对论与量子宇宙学 · 物理学 2010-04-15 Songbai Chen , Jiliang Jing

In this article, we examine the dynamical system of the $f(R,\mathcal{G})$ gravity model. This $f(R,G)$ model framework is composed of interactions between dark matter and scalar field through the linear coupling term. The key objective of…

广义相对论与量子宇宙学 · 物理学 2025-04-03 Shivani Sharma , R. Chaubey

In this work, in the framework of dynamical system analysis, we focus on the study of the accelerated expansion of the Universe of $f(Q)$ gravity theory where $Q$ be the non-metricity that describes the gravitational interaction. We…

广义相对论与量子宇宙学 · 物理学 2023-02-07 Amit Samaddar , S. Surendra Singh , Shivangi Rathore

This paper investigates the effects of spatial curvature in a model where dark matter and dark energy interact. The analysis employs a range of datasets, including CMB, BAO, Type Ia Supernova, $H(z)$ from cosmic chronometers, $H_0$…

宇宙学与河外天体物理 · 物理学 2025-01-28 Trupti Patil , Sukanta Panda

We consider perturbations in a cosmological model with a small coupling between dark energy and dark matter. We prove that the stability of the curvature perturbation depends on the type of coupling between dark sectors. When the dark…

广义相对论与量子宇宙学 · 物理学 2009-01-16 Jian-Hua He , Bin Wang , Elcio Abdalla

The two dark sectors of the universe - dark matter and dark energy - may interact with each other. Background and linear density perturbation evolution equations are developed for a generic coupling. We then establish the general conditions…

宇宙学与河外天体物理 · 物理学 2010-05-25 M. B. Gavela , D. Hernandez , L. Lopez Honorez , O. Mena , S. Rigolin

To find more deliberate f(R,T) cosmological solutions, we proceed our previous paper further by studying some new aspects of the considered models via investigation of some new cosmological parameters/quantities to attain the most…

广义相对论与量子宇宙学 · 物理学 2017-05-23 Hamid Shabani , Mehrdad Farhoudi

Over the past century, General Relativity (GR) has been a cornerstone of gravitational theory. However, recent cosmological observations, such as the accelerated expansion of the Universe, challenge its completeness and the standard…

广义相对论与量子宇宙学 · 物理学 2025-06-02 Lakhan V. Jaybhaye

We study the phase space dynamics of cosmological models in the theoretical formulations of non-minimal metric-torsion couplings with a scalar field, and investigate in particular the critical points which yield stable solutions exhibiting…

广义相对论与量子宇宙学 · 物理学 2017-08-18 Arshdeep Singh Bhatia , Sourav Sur

Recently, in the context of $f(R)$ modified theories of gravity, a new type of model has been proposed where one directly couples the scalar curvature to matter. As any model in $f(R)$ theory, there are certain conditions which have to be…

广义相对论与量子宇宙学 · 物理学 2015-05-13 Orfeu Bertolami , Miguel Carvalho Sequeira
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