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相关论文: Dynamical stability of an interacting quintessence…

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The current Universe is composed by a mixture of relativistic species, baryonic matter, dark matter and dark energy which evolve in a non-trivial way at perturbative level. An advanced description of the cosmological dynamics should include…

宇宙学与河外天体物理 · 物理学 2020-07-22 Winfried Zimdahl , Júlio Fabris , Hermano Velten , Ramón Herrera

The work deals with homogeneous and isotropic, flat FRW model of the universe which is filled up with non-interacting dark matter and dark energy to compatible with recent observational evidences. By choosing the dark energy in the form of…

广义相对论与量子宇宙学 · 物理学 2013-05-09 Nilanjana Mahata , Subenoy Chakraborty

Main aim of this work is to give a suitable explanation of present accelerating universe through an acceptable interactive dynamical cosmological model. A three-fluid cosmological model is introduced in the background of…

广义相对论与量子宇宙学 · 物理学 2022-02-16 Giridhari Deogharia , Mayukh Bandyopadhyay , Ritabrata Biswas

We consider a set of non-linear interactions between dark matter and dark energy which comprises couplings proportional to products of (powers of) the energy densities of both dark components and of the total energy. We demonstrate that…

宇宙学与河外天体物理 · 物理学 2015-06-03 Fabiola Arévalo , Anna Paula Ramos Bacalhau , Winfried Zimdahl

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

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

We consider scalar field models of dark energy interacting with dark matter through a coupling proportional to the contraction of the four-derivative of the scalar field with the four-velocity of the dark matter fluid. The coupling is…

广义相对论与量子宇宙学 · 物理学 2018-02-07 Jibitesh Dutta , Wompherdeiki Khyllep , Nicola Tamanini

We employ a linear stability analysis approach to explore the dynamics of matter and curvature-driven dark energy interactions within the framework of two types of viable $f(R)$ gravity models. The interaction is modeled via a source term…

广义相对论与量子宇宙学 · 物理学 2025-04-21 Anirban Chatterjee , Yungui Gong

In this paper we review in detail a number of approaches that have been adopted to try and explain the remarkable observation of our accelerating Universe. In particular we discuss the arguments for and recent progress made towards…

高能物理 - 理论 · 物理学 2008-11-26 Edmund J. Copeland , M. Sami , Shinji Tsujikawa

Dark Energy is some of the weirdest and most mysterious stuff in the universe that tends to increase the rate of expansion of the universe. Two commonly known forms of dark energy are the cosmological constant, a constant energy density…

广义相对论与量子宇宙学 · 物理学 2010-04-28 Ishwaree P. Neupane , Holly Trowland

We investigate the cosmological evolution of the power law K-essence dark energy (DE) model $F(X)= -\sqrt{X} + X$ with a new interaction $Q = \alpha\rho _m\rho _{\phi }H^{-1}$ in FRWL spacetime. The evolution behavior of dark energy under…

广义相对论与量子宇宙学 · 物理学 2022-01-21 Qile Zhang , Wei Fang , Chenggang Shu

We apply the tools of the dynamical system theory in order to revisit and uncover the structure of a nongravitational interaction between pressureless dark matter and dark energy described by a scalar field $\phi$. For a coupling function…

广义相对论与量子宇宙学 · 物理学 2021-12-08 Patrocinio Pérez , Ulises Nucamendi , Roberto De Arcia

The late time accelerated expansion of the universe can be realized using scalar fields with given self-interacting potentials. Here we consider a straightforward approach where a three cosmic fluid mixture is assumed. The fluids are…

广义相对论与量子宇宙学 · 物理学 2018-07-25 Parth Shah , Gauranga C. Samanta , Salvatore Capozziello

The Aether Scalar Tensor (AeST) theory is an extension of General Relativity (GR), proposed for addressing galactic and cosmological observations without dark matter.The action for the theory includes a function that can currently only be…

广义相对论与量子宇宙学 · 物理学 2024-12-03 João Luís Rosa , Tom Zlosnik

In this work, we have carried on dynamical system analysis of hessence field coupling with dark matter in $f(T)$ gravity. We have analysed the critical points due to autonomous system. The resulting autonomous system is non-linear. So, we…

广义相对论与量子宇宙学 · 物理学 2017-07-20 Jyotirmay Das Mandal , Ujjal Debnath

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

The stability criteria for spatially flat homogeneous and isotropic cosmological dynamical system is investigated with the interaction of a scalar field endowed with a perfect fluid.In this paper, we depict the dynamical system perspective…

广义相对论与量子宇宙学 · 物理学 2021-01-25 S. Surendra Singh , Chingtham Sonia

We investigate the cosmological dynamics of a homogeneous scalar field non-minimally coupled to torsion gravity, which also interacts with cold dark matter through energy and momentum transfer. The matter and radiation perfect fluids are…

广义相对论与量子宇宙学 · 物理学 2025-02-05 Carlos Rodriguez-Benites , Manuel Gonzalez-Espinoza , Giovanni Otalora , Manuel Alva-Morales

We perform for the first time a dynamical system analysis of both the background and perturbation equations, of $\Lambda$CDM cosmology and quintessence scenario with an exponential potential. In the former case the perturbations do not…

广义相对论与量子宇宙学 · 物理学 2019-08-21 Spyros Basilakos , Genly Leon , G. Papagiannopoulos , Emmanuel N. Saridakis

Dark energy models can be seen as dynamical systems. In this paper we show that multi-field models with a curved field space give rise to new critical points and we analyse their stability. These are new accelerating solutions in late-time…

广义相对论与量子宇宙学 · 物理学 2020-05-27 Michele Cicoli , Giuseppe Dibitetto , Francisco G. Pedro