Published June 1, 2010 | Version v1
Journal article

A new type of dark energy model

  • 1. Department of Astronomy, Beijing Normal University, Beijing 100875 (China)
  • 2. Department of Physics, Yantai University, Yantai 264005 (China)

Description

In this paper, we propose a general form of the equation of state (EoS) which is the function of the fractional dark energy density Ωd. At least, five related models, the cosmological constant model, the holographic dark energy model, the agegraphic dark energy model, the modified holographic dark energy model and the Ricci scalar holographic dark energy model are included in this form. Furthermore, if we consider proper interactions, the interactive variants of those models can be included as well. The phase-space analysis shows that the scaling solutions may exist both in the non-interacting and interacting cases. And the stability analysis of the system could give out the attractor solution which could alleviate the coincidence problem

Availability note (English)

Available from http://dx.doi.org/10.1088/1475-7516/2010/06/003

Additional details

Publishing Information

Journal Title
Journal of Cosmology and Astroparticle Physics
Journal Volume
2010
Journal Issue
06
Journal Page Range
p. 003
ISSN
1475-7516

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
45094137
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ATTRACTORS; COSMOLOGICAL CONSTANT; COSMOLOGICAL MODELS; ENERGY DENSITY; EQUATIONS OF STATE; MATHEMATICAL SOLUTIONS; NONLUMINOUS MATTER; PHASE SPACE; SCALARS; STABILITY
Descriptors DEC
EQUATIONS; MATHEMATICAL MODELS; MATHEMATICAL SPACE; MATTER; SPACE