de Sitter Thermodynamics: A glimpse into non equilibrium
arXiv:0801.4591 · doi:10.1103/PhysRevD.77.104013
Abstract
In this article is shown that the thermodynamical evolution of a Schwarzschild de Sitter space is the evaporation of its black hole. The result is extended in higher dimensions to Lovelock theories of gravity with a single positive cosmological constant.
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- Regular black holes with and its evolution in Lovelock gravity
- Pure Lovelock Gravity regular black holes
- Our Universe from the cosmological constant
- Gravitational Decoupling algorithm modifies the value of the conserved charges and thermodynamics properties in Lovelock Unique Vacuum theory
- Black holes inside cosmic voids
- How the Schwarzschild-de Sitter horizons remain in thermal equilibrium at vastly different temperatures