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相关论文: Dilaton Coupled Quintessence Model in the $\omega-…

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In this paper, we regard dilaton in Weyl-scaled induced gravitational theory as coupled Quintessence, which is called DCQ model by us. Parametrization of the dark energy model is a good method by which we can construct the scalar potential…

高能物理 - 理论 · 物理学 2008-11-26 Z. G. Huang , Q. Q. Sun , W. Fang , H. Q. Lu

Based on dilatonic dark energy model, we consider two cases: dilaton field with positive kinetic energy(coupled quintessence) and with negative kinetic energy(phantom). In the two cases, we investigate the existence of attractor solutions…

高能物理 - 理论 · 物理学 2007-05-23 Z. G. Huang , H. Q. Lu , W. Fang

We studied the dilaton cosmology based on Weyl-Scaled induced gravity. The potential of dilaton field is taken as exponential form. An analytical solution of Einstein equation is found. The dilaton can be a candidate for dark energy that…

高能物理 - 理论 · 物理学 2007-05-23 H. Q. Lu , Z. G. Huang , W. Fang , K. F. Zhang

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 discuss some cosmological consequences of a general model of coupled quintessence in which the phenomenological coupling between the cold dark matter and dark energy is a function of the cosmic scale factor $\epsilon(a)$. This class of…

宇宙学与河外天体物理 · 物理学 2010-12-23 F. E. M. Costa

An oscillating scalar field as a quintessence model for dark energy is proposed. The case of a power-law potential is particularly intriguing and is the focus of the present article. In this model the equation of state w_{OQ} of dark energy…

天体物理学 · 物理学 2007-11-26 Je-an Gu

We investigate an interacting dark energy model which allows for the kinetic term of the scalar field to couple to dark matter via a power-law interaction. The model is characterised by scaling solutions at early times, which are of high…

宇宙学与河外天体物理 · 物理学 2022-12-06 Elsa M. Teixeira , Bruno J. Barros , Vasco M. C. Ferreira , Noemi Frusciante

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

In this paper we obtain some cosmological solutions that describe the present period of accelerating expansion of the universe in the framework of a geometrical gauge scalar-tensor theory of gravity. The background geometry in the model is…

广义相对论与量子宇宙学 · 物理学 2023-03-08 José Edgar Madriz Aguilar , M. Montes , A. Bernal

We propose a novel coupled dark energy model which is assumed to occur as a q-deformed scalar field and investigate whether it will provide an expanding universe phase. We consider the q-deformed dark energy as coupled to dark matter…

广义相对论与量子宇宙学 · 物理学 2016-12-09 Emre Dil

We study a coupled quintessence model in which the interaction with the dark matter sector is a function of the quintessence potential. Such a coupling can arise from a field dependent mass term for the dark matter field. The dynamical…

宇宙学与河外天体物理 · 物理学 2011-01-20 Laura Lopez-Honorez , Olga Mena , Grigoris Panotopoulos

Quantum theory of dilaton gravity coupled to a nonlinear sigma model with a maximally symmetric target space is studied in $2+\epsilon$ dimensions. The ultraviolet stable fixed point for the curvature of the nonlinear sigma model demands a…

高能物理 - 理论 · 物理学 2015-06-26 S. Kojima , N. Sakai , Y. Tanii

We investigate a coupled quintessence cosmological model in which a dark-energy scalar field with an exponential potential interacts directly with a dark-matter fluid through a dissipative term inspired by warm inflation. The evolution…

广义相对论与量子宇宙学 · 物理学 2024-10-07 Paulo M. Sá

We explore a novel cosmological model based on coupled fields in the framework of scalar tensor theories, considering the specific interplay between gravity and scalar fields. The model further extends a recent axion-dilaton system by…

广义相对论与量子宇宙学 · 物理学 2025-11-25 Mihai Marciu

In this work we consider a cosmological model in which dark energy is portrayed by a canonical scalar field which is allowed to couple to the other species by means of a disformal transformation of the metric. We revisit the current…

广义相对论与量子宇宙学 · 物理学 2020-04-06 Elsa M. Teixeira , Ana Nunes , Nelson J. Nunes

In this work, we have considered dilaton dark energy model in Weyl-scaled induced gravitational theory in presence of barotropic fluid. It is to be noted that the dilaton field behaves as a quintessence. Here we have discussed the role of…

综合物理 · 物理学 2015-05-28 Piyali Bagchi Khatua , Shuvendu Chakraborty , Ujjal Debnath

Dark energy can be characterized by a canonical scalar field, known as quintessence. Quintessence allows for a dynamical equation of state $-1 \le \omega \le -\frac{1}{3}$. A previous study by Oikonomou and Chatzarakis have shown that a…

宇宙学与河外天体物理 · 物理学 2024-09-11 Sreerag Radhakrishnan , Sarath Nelleri , Navaneeth Poonthottathil

Coupled dark sector models have gained significant attention, motivated by recent advances in cosmology and the pressing need to address unresolved puzzles. In this work, we study coupled scalar dark sector models inspired by…

高能物理 - 理论 · 物理学 2025-09-05 Saba Rahimy , Elsa M. Teixeira , Ivonne Zavala

The perfect dilaton-spin fluid (as a model of the dilaton matter, the particles of which are endowed with intrinsic spin and dilaton charge) is considered as the source of the gravitational field in a Weyl-Cartan spacetime. The variational…

广义相对论与量子宇宙学 · 物理学 2011-07-19 Olga V. Babourova , Boris N. Frolov

In this paper, we investigate the dynamics of Born-Infeld(B-I) phantom model in the $\omega-\omega'$ plane, which is defined by the equation of state parameter for the dark energy and its derivative with respect to $N$(the logarithm of the…

高能物理 - 理论 · 物理学 2008-11-26 Z. G. Huang , X. H. Li , Q. Q. Sun
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