An interacting dark energy model in a non-flat universe

DOI10.1007/s10714-013-1576-zzbMath1274.83163OpenAlexW2112614428WikidataQ126173893 ScholiaQ126173893MaRDI QIDQ376244

Shanshan Gao, Ya-Bo Wu, Jian-Bo Lu, Mo-Lin Liu

Publication date: 4 November 2013

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10714-013-1576-z

zbMATH Keywords

interacting cosmic modelnon-flat universepower-law form of dark energy density

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Astrophysical cosmology (85A40)

Related Items (1)

Can the coincidence problem be solved by a cosmological model of coupled dark energy and dark matter?

Cites Work

• A dark energy model characterized by the age of the Universe
• Which cosmological model-with dark energy or modified FRW dynamics?
• Combined constraints on modified Chaplygin gas model from cosmological observed data: Markov chain Monte Carlo approach
• Interacting dark energy with inhomogeneous equation of state
• The Abell cluster A586 and the detection of violation of the equivalence principle
• CONSTRAINTS ON VARIABLE CHAPLYGIN GAS MODEL FROM TYPE IA SUPERNOVAE AND BARYON ACOUSTIC OSCILLATIONS
• TIME VARIABLE COSMOLOGICAL CONSTANT OF HOLOGRAPHIC ORIGIN WITH INTERACTION IN BRANS–DICKE THEORY
• Interacting quintessence

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