2007/08/31 by F. Briscese, Fabio Briscese, E. Elizalde · 3 citations
Physics and Astronomy · #Advanced Differential Geometry Research #Black Holes and Theoretical Physics #Black hole (networking) #Black hole thermodynamics #Classical mechanics #Computer science #Cosmology and Gravitation Theories #Entropy (arrow of time) #General relativity #Gravitation #Hawking radiation #Lagrangian #Mathematical physics #Noether's theorem #Physics #Quantum mechanics #Schwarzschild metric #Schwarzschild radius #Theoretical physics #hep-th
paper · pdf · doi:10.1103/physrevd.77.044009
published as Phys.Rev.D77:044009,2008 · 5 pages, 3 figures, revtex file, version to appear in PRD
arxiv created 2008/01/13 · openalex publication_date 2008/02/07 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
An analysis of some modified-gravity models, based on the study of pure Schwarzschild and of Schwarzschild--de Sitter black holes, and involving the use of the Noether charge method, is carried out. Corrections to the classical Einsteinian black hole entropy appear. It is shown explicitly how the condition of positive entropy can be used in order to constrain the viability of modified-gravity theories.