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相关论文: Cosmic Duality and Statefinder Diagnosis of Spinor…

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We perform in this paper a statefinder diagnostic to a dark energy model with two scalar fields, called "quintom", where one of the scalar fields has a canonical kinetic energy term and the other has a negative one. Several kinds of…

广义相对论与量子宇宙学 · 物理学 2009-09-01 Puxun Wu , Hongwei Yu

In the present work, we perform a comparative study of different interacting dark energy (DE) models using the Statefinder diagnostics. In particular, 17 different forms of the energy transfer rate $Q$ between DE and dark matter (DM) were…

广义相对论与量子宇宙学 · 物理学 2023-10-09 Raul Carrasco , Angel Rincon , Joel Saavedra , Nelson Videla

Statefinder diagnostic is a useful method which can differ one dark energy model from the others. The Statefinder pair $\{r, s\}$ is algebraically related to the equation of state of dark energy and its first time derivative. We apply in…

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

Statefinder diagnostic is a useful method which can differ one dark energy model from each others. In this letter, we apply this method to a holographic dark energy model from Ricci scalar curvature, called the Ricci dark energy model(RDE).…

高能物理 - 理论 · 物理学 2008-12-18 Chao-Jun Feng

Statefinder diagnostic is a convenient method that can differentiate between the various dark energy models. In this article, we analyze the statefinder parameters in symmetric teleparallel cosmology. The $f(Q)$ gravity theory is an…

广义相对论与量子宇宙学 · 物理学 2022-06-27 Raja Solanki , P. K. Sahoo

Observations of high redshift supernovae indicate that the universe is accelerating. The hypothesis of `Dark energy' (cosmological constant, scalar field tracker potentials, braneworld models, etc.) has been advanced to explain this…

天体物理学 · 物理学 2007-05-23 Varun Sahni

The problem of the cosmic coincidence is a longstanding puzzle. This conundrum may be solved by introducing a coupling between the two dark sectors. In this Letter, we study two cases of the coupled quintessence scenario. $(a)$ Assume that…

天体物理学 · 物理学 2009-11-10 Xin Zhang

A new model of dark energy namely "ghost dark energy model" has recently been suggested to interpret the positive acceleration of cosmic expansion. The energy density of ghost dark energy is proportional to the hubble parameter. In this…

广义相对论与量子宇宙学 · 物理学 2015-06-04 M. Malekjani , A. Khodam-Mohammadi

We introduce a new cosmological diagnostic pair $\lbrace r,s\rbrace$ called Statefinder. The Statefinder is dimensionless and, like the Hubble and deceleration parameters $H(z)$ and $q(z)$, is constructed from the scale factor of the…

天体物理学 · 物理学 2011-07-19 Varun Sahni , Tarun Deep Saini , A. A. Starobinsky , Ujjaini Alam

Many dark energy (DE) models have been proposed, in recent years, to explain acceleration of the Universe expansion. It seems necessary to discriminate the various DE models in order to check the viability of each model. Statefinder…

广义相对论与量子宇宙学 · 物理学 2015-04-17 S. Ghaffari , A. Sheykhi , M. H. Dehghani

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

The cosmological dynamics of minimally coupled scalar field that couples to the background matter with thermal interactions is investigated by using statefinder diagnostics. The time evolution of the statefinder pairs $\{r,s\}$ and…

天体物理学 · 物理学 2009-06-23 Wei-Zhong Liu , Dao-Jun Liu

The coming few years are likely to witness a dramatic increase in high quality Sn data as current surveys add more high redshift supernovae to their inventory and as newer and deeper supernova experiments become operational. Given the…

天体物理学 · 物理学 2008-11-26 Ujjaini Alam , Varun Sahni , Tarun Deep Saini , A. A. Starobinsky

The statefinder parameters ($r,s$) in two dark energy models are studied. In the first, we discuss in four-dimensional General Relativity a two fluid model, in which dark energy and dark matter are allowed to interact with each other. In…

天体物理学 · 物理学 2008-11-26 Grigoris Panotopoulos

We study the statefinder parameter in the five-dimensional big bounce model, and apply it to differentiate the attractor solutions of quintessence and phantom field. It is found that the evolving trajectories of these two attractor…

天体物理学 · 物理学 2009-06-23 Baorong Chang , Hongya Liu , Lixin Xu , Chengwu Zhang

We apply in this paper the statefinder parameters to the interacting phantom energy with dark matter. There are two kinds of scaling solutions in this model. It is found that the evolving trajectories of these two scaling solutions in the…

天体物理学 · 物理学 2010-10-27 Baorong Chang , Hongya Liu , Lixin Xu , Chengwu Zhang , Yongli Ping

In this paper we study the duality in two-field Quintom models of Dark Energy. We find that an expanding universe dominated by Quintom-A field is dual to a contracting universe with Quintom-B field.

广义相对论与量子宇宙学 · 物理学 2008-11-26 Yi-Fu Cai , Hong Li , Yun-Song Piao , Xinmin Zhang

A class of dynamical dark energy models, dubbed Spinor Quintom, can be constructed by a spinor field $\psi$ with a nontraditional potential. We find that, if choosing suitable potential, this model is able to allow the equation-of-state to…

高能物理 - 理论 · 物理学 2008-11-26 Yi-Fu Cai , Jing Wang

Using a new method--statefinder diagnostic which can differ one dark energy model from the others, we investigate in this letter the dynamics of Born-Infeld(B-I) type dark energy model. The evolutive trajectory of B-I type dark energy with…

高能物理 - 理论 · 物理学 2008-11-25 Z. G. Huang , H. Q. Lu

In this paper, we study the holographic dark energy model in non-flat universe from the statefinder viewpoint. We plot the evolutionary trajectories of the holographic dark energy model for different values of the parameter $c$ as well as…

广义相对论与量子宇宙学 · 物理学 2010-10-27 M. R. Setare , Jingfei Zhang , Xin Zhang
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