Modeling holographic dark energy with particle and future horizons

DOI10.1016/J.NUCLPHYSB.2020.115017zbMath1473.83030arXiv1812.06373OpenAlexW2905431446WikidataQ120434935 ScholiaQ120434935MaRDI QIDQ2230465

Samuel Lepe, Miguel Cruz

Publication date: 17 September 2021

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1812.06373

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) Classical and relativistic thermodynamics (80A10) Statistical thermodynamics (82B30) Dark matter and dark energy (83C56)

Related Items (2)

Cosmic evolution of holographic dark energy in f(Q,T) gravity ⋮ Barrow entropic dark energy: a member of generalized holographic dark energy family

Cites Work

• Unnamed Item
• Some simple predictions from \(E_{11}\) symmetry
• Dynamical systems applied to cosmology: dark energy and modified gravity
• Real scalar dark matter: relativistic treatment
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• 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
• Unified dark energy thermodynamics: varying w and the −1-crossing
• DYNAMICS OF DARK ENERGY
• Effective Field Theory, Black Holes, and the Cosmological Constant
• A note on the relations between thermodynamics, energy definitions and Friedmann equations
• Probable Values of the Cosmological Constant in a Holographic Theory

This page was built for publication: Modeling holographic dark energy with particle and future horizons