Qualitative description of the universe in the interacting fluids scheme
From MaRDI portal
Publication:2423340
DOI10.1016/J.NUCLPHYSB.2019.114623zbMath1415.83072arXiv1902.09684OpenAlexW2917409677WikidataQ64290864 ScholiaQ64290864MaRDI QIDQ2423340
Miguel Cruz, Gerardo Morales-Navarrete, Samuel Lepe
Publication date: 21 June 2019
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1902.09684
Relativistic cosmology (83F05) Space-time singularities, cosmic censorship, etc. (83C75) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Volterra integral equations (45D05)
Related Items (1)
Cites Work
- Holographic dark energy
- Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
- Holographic approach for dark energy–dark matter interaction in curved FLRW spacetime
- Effective Field Theory, Black Holes, and the Cosmological Constant
- Cosmological evolution with interaction between dark energy and dark matter
- Probable Values of the Cosmological Constant in a Holographic Theory
- The cosmological constant problem
This page was built for publication: Qualitative description of the universe in the interacting fluids scheme