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相关论文: Interacting quintessence cosmology from Noether sy…

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We investigate the cosmological dynamics of interacting dark energy models in which the interaction function is a nonlinear in terms of the energy densities. Considering explicitly the interaction between a pressureless dark matter and a…

广义相对论与量子宇宙学 · 物理学 2020-01-17 Andronikos Paliathanasis , Supriya Pan , Weiqiang Yang

A matter-coupled scalar field model is presented in obtaining a scalar fifth force when the constraint of the current cosmological constant is satisfied. The interaction potential energy density between the scalar field and matter has a…

广义相对论与量子宇宙学 · 物理学 2020-04-22 Hai-Chao Zhang

We analyze the cosmology of a general Scalar-Tensor theory which encompasses generalized Brans-Dicke theory, Gauss-Bonnet gravity, non-minimal derivative gravity, generalized Galileon gravity and also the general k-essence type models.…

广义相对论与量子宇宙学 · 物理学 2017-03-07 Erfan Masaeli , Meysam Motaharfar , Hamid Reza Sepangi

This study explores the plausibility of an interacting tachyonic scalar, homogeneous in nature, as a promising candidate for dynamic dark energy, offering insights into the observed accelerated expansion of the universe. The…

广义相对论与量子宇宙学 · 物理学 2025-07-16 Tanisha Joshi , S. D Pathak

We consider Noether symmetry approach to find out exact cosmological solutions in $f(T)$-gravity. Instead of taking into account phenomenological models, we apply the Noether symmetry to the $f(T)$ gravity. As a result, the presence of such…

综合物理 · 物理学 2012-05-29 K. Atazadeh , F. Darabi

We consider a model where both dark energy and dark matter originate from the coupling of a scalar field with a non-conventional kinetic term to, both, a metric measure and a non-metric measure. An interacting dark energy/dark matter…

广义相对论与量子宇宙学 · 物理学 2015-06-11 Stefano Ansoldi , Eduardo I. Guendelman

In this paper, based on the works of Capozziello et al., we have studied the Noether symmetry approach in the cosmological model with scalar and gauge fields proposed recently by Soda et al. The correct Noether symmetries and related Lie…

广义相对论与量子宇宙学 · 物理学 2015-04-21 Sun Zhang

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

The cosmological evolution of an interacting scalar field model in which the scalar field interacts with dark matter, radiation, and baryon via Lorentz violation is investigated. We propose a model of interaction through the effective…

高能物理 - 理论 · 物理学 2009-09-29 Freddy P. Zen , Arianto , Bobby E. Gunara , Triyanta , A. Purwanto

In this work it is investigated the evolution of a Universe where a scalar field, non-minimally coupled to space-time curvature, plays the role of quintessence and drives the Universe to a present accelerated expansion. A non-relativistic…

广义相对论与量子宇宙学 · 物理学 2009-11-11 J. B. Binder , G. M. Kremer

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

A linear relationship between the Hubble expansion parameter and the time derivative of the scalar field is assumed in order to derive exact analytic cosmological solutions to Einstein's gravity with two fluids: a barotropic perfect fluid…

广义相对论与量子宇宙学 · 物理学 2009-09-29 Olga Arias , Tame Gonzalez , Israel Quiros

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

A light scalar field, minimally or not-minimally coupled to the metric field, is a well-defined candidate for the dark energy, overcoming the coincidence problem intrinsic to the cosmological constant and avoiding the difficulties of…

天体物理学 · 物理学 2008-11-26 Carlo Schimd , Ismael Tereno

The present work deals with a quintom model of dark energy in the framework of a spatially flat isotropic and homogeneous Friedmann-Lemaitre-Robertson-Walker (FLRW) universe. At first, Lie point symmetry is imposed to the system and the…

广义相对论与量子宇宙学 · 物理学 2016-09-27 Sourav Dutta , Muthusamy Lakshmanan , Subenoy Chakraborty

We study the cosmology of a quintessence scalar field which is equivalent to a non-barotropic perfect fluid of constant pressure. The coincidence problem is alleviated by such a quintessence equation-of-state that interpolates between…

宇宙学与河外天体物理 · 物理学 2013-04-23 Wenzhong Liu , Jun Ouyang , Huanxiong Yang

We derive two field theory models of interacting dark energy, one in which dark energy is associated with the quintessence and another in which it is associated with the tachyon. In both, instead of choosing arbitrarily the potential of…

广义相对论与量子宇宙学 · 物理学 2020-07-10 Sandro M. R. Micheletti

We investigate whether interaction between massive neutrinos and quintessence scalar field is the origin of the late time accelerated expansion of the universe. We present cosmological perturbation theory in neutrinos probe interacting…

天体物理学 · 物理学 2008-03-24 Kiyotomo Ichiki , Yong-Yeon Keum

In this Letter, we find suitable potentials in the multiple scalar fields scenario by using the Noether symmetry approach. We discussed three models with multiple scalar fields: N-quintessence with positive kinetic terms, N-phantom with…

高能物理 - 唯象学 · 物理学 2010-05-07 Yi Zhang , Yun-gui Gong , Zong-Hong Zhu

We analyze scalar field dark energy models minimally and non-minimally coupled to gravity, postulating that a Yukawa-like interacting term is \emph{in form} equivalent for general relativity, teleparallel and symmetric-teleparallel…

广义相对论与量子宇宙学 · 物理学 2025-04-15 Youri Carloni , Orlando Luongo