Published June 1, 2010
| Version v1
Journal article
A new type of dark energy model
Creators
- 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/10.1088/1475-7516/2010/06/003Additional details
Identifiers
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