2004/10/31 by Dominic Brecher, Jianyang He, Moshe Rozali · 2 citations
Mathematics · Physics and Astronomy · #Anti-de Sitter space #Astronomy #Black Holes and Theoretical Physics #Black hole (networking) #Classical mechanics #Cosmology and Gravitation Theories #De Sitter universe #Event horizon #Geodesic #Geometry #Horizon #Instability #Mathematical physics #Mathematics #Noncommutative and Quantum Gravity Theories #Physics #Quantum mechanics #Space (punctuation) #Universe #White hole #de Sitter–Schwarzschild metric #hep-th
paper · pdf · doi:10.1088/1126-6708/2005/04/004
published as JHEP0504:004,2005 · 1+37 pages, 20 ps and eps figures, LaTeX. References added and changes made to section 5
arxiv created 2004/11/09 · openalex publication_date 2005/04/26 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We study the region inside the event horizon of charged black holes in five dimensional asymptotically anti-de Sitter space, using as a probe two-sided correlators which are dominated by spacelike geodesics penetrating the horizon. The spacetimes we investigate include the Reissner-Nordstrom black hole and perturbations thereof. The perturbed spacetimes can be found exactly, enabling us to perform a local scan of the region between the inner and outer horizons. Surprisingly, the two-sided correlators we calculate seem to be geometrically protected from the instability of the inner horizon.