Thermodynamics of Apparent Horizon in Brane World Scenarios
From MaRDI portal
Publication:3540761
DOI10.1143/PTPS.172.100zbMath1153.83398arXiv0712.2142OpenAlexW2015846340MaRDI QIDQ3540761
Publication date: 24 November 2008
Published in: Progress of Theoretical Physics Supplement (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0712.2142
Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30) String and superstring theories; other extended objects (e.g., branes) in quantum field theory (81T30) Classical and relativistic thermodynamics (80A10)
Related Items
Hawking radiation of apparent horizon in a FRW universe as tunneling beyond semiclassical approximation ⋮ Lanczos-Lovelock gravity from a thermodynamic perspective ⋮ Gravitational field equations near an arbitrary null surface expressed as a thermodynamic identity ⋮ Why does the universe expand? ⋮ Does the entropy of the universe tend to a maximum? ⋮ Black holes, cosmological solutions, future singularities, and their thermodynamical properties in modified gravity theories ⋮ A thermodynamic motivation for dark energy ⋮ Viscous cosmology and thermodynamics of apparent horizon in modified Friedman-Robertson-Walkers universe ⋮ Deformation of codimension-2 surfaces and horizon thermodynamics ⋮ Thermodynamics of evolving Lorentzian wormhole at apparent and event horizons ⋮ Conservative entropic forces ⋮ A NOTE ON THE HAWKING RADIATION CALCULATED BY THE QUASICLASSICAL TUNNELING METHOD ⋮ THE FRIEDMANN EQUATIONS IN DEFORMED HOŘAVA–LIFSHITZ GRAVITY AND DEBYE MODEL ⋮ A NOTE ON THE UNIFIED FIRST LAW IN f(R) GRAVITY THEORY ⋮ Modified Bekenstein-Hawking system in \(f(R)\) gravity ⋮ Corrections to Hawking-like radiation for a Friedmann-Robertson-Walker universe ⋮ THERMODYNAMICS OF FRIEDMANN EQUATION AND MASSLIKE FUNCTION IN GENERAL BRANEWORLD ⋮ Black holes and black hole thermodynamics without event horizons
