Holographic dark energy with time varying \(n^2\) parameter in non-flat universe

DOI10.1007/s10773-014-2197-3zbMath1317.83027arXiv1411.0125OpenAlexW2094561619MaRDI QIDQ2348627

Bushra Majeed, Azad A. Siddiqui, Mubasher Jamil

Publication date: 15 June 2015

Published in: International Journal of Theoretical Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1411.0125

zbMATH Keywords

holographic dark energyFRW universe

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Astrophysical cosmology (85A40)

Related Items (1)

Anisotropic cosmological model in presence of holographic dark energy and quintessence

Cites Work

• Power-law entropy corrected holographic dark energy model
• FRW and Bianchi type I cosmology of f-essence
• Reconstructing interacting entropy-corrected holographic scalar field models of dark energy in the non-flat universe
• The cosmological constant and dark energy
• Effective Field Theory, Black Holes, and the Cosmological Constant
• Cosmological parameters from SDSS and WMAP
• The world as a hologram
• Power-law entropy-corrected Ricci dark energy and dynamics of scalar fields
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae

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