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It is demonstrated that dark energy, driven by tachyons having non-minimal coupling with curvature and self-interacting inverse cubic potential, decays to cold dark matter in the late universe. It is found that this penomenon yields a…

广义相对论与量子宇宙学 · 物理学 2007-05-23 S. K. Srivastava

Recent attempts to explain the dark matter and energy content of the universe have involved some radical extensions of standard physics, including quintessence, phantom energy, additional space dimensions and variations in the speed of…

天体物理学 · 物理学 2009-11-10 P. C. W. Davies

We consider a mixture of varying Generalized Chaplyagin gas [1] interacting with a Tachyonic fluid in framework of GR. We suppose, that a Tachyonic fluid and Generalized Chaplyagin gas was separated somehow from Darkness of the Universe.…

综合物理 · 物理学 2013-02-06 Martiros Khurshudyan

In this paper, we consider three different models of dark energy in higher dimensional space-time and discuss about some cosmological parameters numerically. The first model is a single component universe including viscous varying modified…

广义相对论与量子宇宙学 · 物理学 2014-06-13 M. Khurshudyan , J. Sadeghi , M. Hakobyan , H. Farahani , R. Myrzakulov

In this paper we consider two models of quintessence scalar fields with different potentials. Interaction with generalized cosmic Chaplygin gas is also investigated. Cosmological parameters are studied and graphical behavior is analyzed. We…

广义相对论与量子宇宙学 · 物理学 2014-07-08 M. Khurshudyan , E. Chubaryan , B. Pourhassan

I present a model in which dark energy interacts with matter. The former is represented by a variable equation of state. It is shown that the phantom crossing takes place at zero redshift, moreover, stable scaling solution of the Friedmann…

高能物理 - 理论 · 物理学 2010-01-11 Mubasher Jamil

This paper deals with dark and phantom energy in the tachyon and sub-quantum models for dark energy. We obtain that the simplest condition for such a regime to occur in these scenarios is that the scalar field be Wick rotated to imaginary…

高能物理 - 理论 · 物理学 2007-05-23 Pedro F. Gonzalez-Diaz

Recently tachyonic field has been depicted as dark energy model to represent the present acceleration of the Universe. In this paper we have considered mixture of tachyonic fluid with a perfect fluid. For this purpose we have considered…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Writambhara Chakraborty , Ujjal Debnath

Dynamical models for dark energy are an alternative to the cosmological constant. It is important to investigate properties of perturbations in these models and go beyond the smooth FRLW cosmology. This allows us to distinguish different…

宇宙学与河外天体物理 · 物理学 2019-12-04 Manvendra Pratap Rajvanshi , J. S. Bagla

We investigate a kind of interacting Chaplygin gas model in which the Chaplygin gas plays the role of dark energy and interacts with cold dark matter particles. We find that there exists a stable scaling solution at late times with the…

天体物理学 · 物理学 2009-11-13 Hongsheng Zhang , Zong-Hong Zhu

We discuss an interacting tachyonic dark energy model in the context of the holographic principle. The potential of the holographic tachyon field in interaction with dark matter is constructed. The model results are compared with CMB shift…

广义相对论与量子宇宙学 · 物理学 2010-05-25 Sandro M. R. Micheletti

In this paper, we study the holographic dark energy density and interacting extended Chaplygin gas energy density in the Einstein gravity. We reconstruct the scalar field and the scalar potential describing the extended Chaplygin gas. In…

广义相对论与量子宇宙学 · 物理学 2015-04-28 J. Sadeghi , H. Farahani , B. Pourhassan

An action of general form is proposed for a Universe containing matter, radiation and dark energy. The latter is interpreted as a tachyon field non-minimally coupled to the scalar curvature. The Palatini approach is used when varying the…

广义相对论与量子宇宙学 · 物理学 2017-04-28 Lucas Gardai Collodel , Gilberto Medeiros Kremer

This paper deals with a cosmological model in which the universe is filled with tachyon dark energy in order to describe current and future accelerating expansion. We obtain that the simplest condition for the regime of phantom energy to…

天体物理学 · 物理学 2009-11-10 Pedro F. Gonzalez-Diaz

A model for the universe on the basis of a self interacting fermionic tachyon field is investigated here. It is shown that, devising a self interaction potential of a proper form, the fermionic tachyon field is capable of producing an…

广义相对论与量子宇宙学 · 物理学 2023-03-29 Salomeh Khoeini-Moghaddam , Farzan Momeni , Fatemeh Yousefabadi

In this paper we consider a correspondence between the holographic dark energy density and tachyon energy density in FRW universe. Then we reconstruct the potential and the dynamics of the tachyon field which describe tachyon cosmology.

高能物理 - 理论 · 物理学 2008-11-26 M R Setare

In this paper a possibility to accelerated the expansion of the large scale universe due to interacting varying Chaplygin gas of a specific form and a tachyonic matter is considered. A specific form of the potential and appropriate values…

综合物理 · 物理学 2017-08-16 Martiros Khurshudyan

We propose an holographic quintessence and tachyon models of dark energy. The correspondence between the quintessence and tachyon energy densities with the holographic density, allows the reconstruction of the potentials and the dynamics…

广义相对论与量子宇宙学 · 物理学 2009-11-19 L. N. Granda

Here, non-minimally coupled tachyon to gravity is considered as a source of "dark energy". It is demonstrated that with expansion of the universe, tachyon dark energy decays to "dark matter" providing a solution to "cosmic coincidence…

广义相对论与量子宇宙学 · 物理学 2007-05-23 S. K. Srivastaca

In this work we investigate the background dynamics when dark energy is coupled to dark matter with a suitable interaction in the universe described by Einstein-Aether gravity. Dark energy in the form of Modified Chaplygin gas is…

综合物理 · 物理学 2014-08-21 Chayan Ranjit , Prabir Rudra , Sujata Kundu