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相关论文: Thermodynamical description of the interacting new…

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We present a thermodynamical description of the interaction between holographic dark energy and dark matter. If holographic dark energy and dark matter evolve separately, each of them remains in thermodynamic equilibrium. A small…

高能物理 - 理论 · 物理学 2008-11-26 Bin Wang , Chi-Yong Lin , Diego Pavon , Elcio Abdalla

To explain the accelerating universe driven by dark energy, a so-called "entropy-corrected new agegraphic dark energy" (ECNADE), was recently proposed with the help of quantum corrections to the entropy-area relation in the framework of…

广义相对论与量子宇宙学 · 物理学 2011-04-21 Kayoomars Karami , Ahmad Sheykhi , Mubasher Jamil , F. Felegary , M. M. Soltanzadeh

In the present paper, we provide a thermodynamical interpretation for the holographic dark energy model in a non-flat universe. For this case, the characteristic length is no more the radius of the event horizon ($R_E$) but the event…

高能物理 - 理论 · 物理学 2009-02-25 M R Setare

A so-called "entropy-corrected holographic dark energy" (ECHDE), was recently proposed to explain the dark energy-dominated universe with the help of quantum corrections to the entropy-area relation in the setup of loop quantum cosmology.…

综合物理 · 物理学 2014-11-20 Mubasher Jamil , Ahmad Sheykhi , M. Umar Farooq

Motivated by the recent work of Wang, Lin, Pavon, and Abdalla [1], we generalize their work to the non-flat case. In particular, we provide a thermodynamical interpretation for the holographic dark energy model in a non-flat universe. For…

高能物理 - 理论 · 物理学 2008-11-26 M. R. Setare , Elias C. Vagenas

We consider the new agegraphic model of dark energy with a varying gravitational constant, $G$, in a non-flat universe. We obtain the equation of state and the deceleration parameters for both interacting and noninteracting new agegraphic…

综合物理 · 物理学 2015-05-18 A. Sheykhi , M. R. Setare

In this paper we consider the new agegraphic model of interacting dark energy in non-flat universe. We show that the interacting agegraphic dark energy can be described by a phantom scalar field. Then we show this phantomic description of…

广义相对论与量子宇宙学 · 物理学 2015-05-13 M. R. Setare

In this paper, we point out thermodynamical description of ghost dark energy and its generalization to the early universe. Thereinafter, we find expressions for the entropy changes of these dark energy candidates. In addition, considering…

广义相对论与量子宇宙学 · 物理学 2015-05-06 M. Honarvaryan , A. Sheykhi , H. Moradpour

A so-called "agegraphic dark energy" was recently proposed to explain the dark energy-dominated universe. In this Letter, we generalize the agegraphic dark energy models to the universe with spatial curvature in the presence of interaction…

高能物理 - 理论 · 物理学 2009-10-16 Ahmad Sheykhi

We suggest a correspondence between interacting agegraphic dark energy models and the quintessence scalar field in a non-flat universe. We demonstrate that the agegraphic evolution of the universe can be described completely by a single…

高能物理 - 理论 · 物理学 2010-11-04 A. Sheykhi , A. Bagheri , M. M. Yazdanpanah

Here we consider the entropy-corrected version of the new agegraphic dark energy model in the non-flat FRW universe. We derive the exact differential equation that determines the evolution of the entropy-corrected new agegraphic dark energy…

综合物理 · 物理学 2014-11-20 K. Karami , A. Sorouri

We investigate the interaction between dark energy and dark matter in the framework of irreversible thermodynamics of open systems with matter creation/annihilation. We consider dark energy and dark matter as an interacting two component…

广义相对论与量子宇宙学 · 物理学 2013-02-08 Tiberiu Harko , Francisco S. N. Lobo

In the context of thermodynamics we discuss the way inevitable emerge an interaction between dark components, and in this way, provide a mechanism to understand the limits of the LCDM model and the class of interaction models between dark…

宇宙学与河外天体物理 · 物理学 2019-05-22 Víctor H. Cárdenas , Daniela Grandón , Samuel Lepe

In this work we focus on the thermodynamics consistency of a new set of solutions emerging from a cosmology in which dark matter is able to decay into relativistic particles within the dark sector. It is important to stress that the…

广义相对论与量子宇宙学 · 物理学 2025-07-08 Javier Juárez-Jiménez , Ana A. Avilez-López , Miguel Cruz

The statefinder diagnosic is a useful method for distinguishing different dark energy models. In this paper, we investigate the new agegraphic dark energy model with interaction between dark energy and matter component by using statefinder…

宇宙学与河外天体物理 · 物理学 2014-11-20 Li Zhang , Jinglei Cui , Jingfei Zhang , Xin Zhang

In this study, we consider dark matter and dark energy as grand-canonical systems which are open, non-equilibrium coupled, and interacting systems. For the first time, we propose a new more realistic interaction scheme to explain dynamics…

广义相对论与量子宇宙学 · 物理学 2025-01-03 E. Aydiner

We study the correspondence between the interacting new agegraphic dark energy and the polytropic gas model of dark energy in the non-flat FRW universe. This correspondence allows to reconstruct the potential and the dynamics for the scalar…

高能物理 - 理论 · 物理学 2011-04-07 K. Karami , A. Abdolmaleki

A model of holographic dark energy with an interaction with matter fields has been investigated. Choosing the future event horizon as an IR cutoff, we have shown that the ratio of energy densities can vary with time. With the interaction…

高能物理 - 理论 · 物理学 2009-11-11 Bin Wang , Yungui Gong , Elcio Abdalla

A new dark energy model, named "agegraphic dark energy", has been proposed recently, based on the so-called K\'{a}rolyh\'{a}zy uncertainty relation, which arises from quantum mechanics together with general relativity. In this note, we…

高能物理 - 理论 · 物理学 2009-01-14 Hao Wei , Rong-Gen Cai

In this paper we investigate the interaction between dark matter and dark energy by considering two different interacting scenarios, i.e. the cases of constant interaction function and variable interaction function. By fitting the current…

宇宙学与河外天体物理 · 物理学 2012-03-23 Jianbo Lu , Yabo Wu , Yongyi Jin , Yan Wang
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