Holographic approach for dark energy–dark matter interaction in curved FLRW spacetime
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Publication:3120849
DOI10.1088/1361-6382/aacd9ezbMath1409.83228arXiv1802.00097OpenAlexW2786989586WikidataQ129627624 ScholiaQ129627624MaRDI QIDQ3120849
Publication date: 19 March 2019
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1802.00097
Relativistic cosmology (83F05) Space-time singularities, cosmic censorship, etc. (83C75) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Astrophysical cosmology (85A40)
Related Items (3)
Qualitative description of the universe in the interacting fluids scheme ⋮ Modeling holographic dark energy with particle and future horizons ⋮ Dynamical study of interacting Ricci dark energy model using Chevallier-Polarsky-Lindertype parametrization
Cites Work
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- Matter bounce cosmology with the f ( T ) gravity
- Dark energy model with spinor matter and its quintom scenario
- Cosmological parameters from SDSS and WMAP
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
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