Holographic dark energy satisfying the energy conditions in Lovelock gravity
arXiv:2303.09563 · doi:10.1016/j.aop.2023.169282
Abstract
In this paper, we show that the holographic dark energy density hides in the solutions of Lovelock gravity for black holes. Using the obtained mass and temperature we find density equations. We propose a physical interpretation of the rescaled Lovelock couplings as a topological mass that describes the Lovelock branch. In addition to this, we present new solutions that satisfy the energy conditions according to the Lovelock coupling and the horizon curvatures. This work can be extended to the equation of the state ω_{Λ} of dark energy in third-order Lovelock gravity. We show that the value "-1" represents a stable equilibrium of ω_{Λ}.
16 pages, 2 figures
References in corpus (14)
- A New Model of Agegraphic Dark Energy
- The Cosmology of Modified Gauss-Bonnet Gravity
- Smarr Formula and an Extended First Law for Lovelock Gravity
- Barrow entropic dark energy: A member of generalized holographic dark energy family
- Restoring Holographic Dark Energy in Brane Cosmology
- Extended phase space thermodynamics for third order Lovelock black holes in diverse dimensions
- Phantom and non-phantom dark energy: The cosmological relevance of non-locally corrected gravity
- Isolated critical point from Lovelock gravity
- Topological Black Holes in Lovelock-Born-Infeld Gravity
- Bardeen-like regular black holes in Einstein-Gauss-Bonnet gravity
- Black hole and holographic dark energy
- Quasinormal modes of black holes absorbing dark energy
- Thermodynamics of third order Lovelock anti-de Sitter black holes revisited
- Lovelock black holes with nonmaximally symmetric horizons