2014/09/30 by Farook Rahaman, Piyali Bhar, Ranjan Sharma +2
Mathematics · Physics and Astronomy · #Anti-de Sitter space #Black Holes and Theoretical Physics #Black hole (networking) #Black hole thermodynamics #Charged black hole #Classical mechanics #Cosmology and Gravitation Theories #De Sitter universe #Entropy (arrow of time) #Event horizon #Extremal black hole #Geodesic #Geometry #Horizon #Mathematical physics #Mathematics #Noncommutative and Quantum Gravity Theories #Noncommutative geometry #Physics #Quantum mechanics #Spacetime #Universe #White hole #de Sitter–Schwarzschild metric #physics.gen-ph
paper · pdf · doi:10.1140/epjc/s10052-015-3320-1
published as Eur. Phys. J. C (2015) 75:107 · 11 pages,16 figures, Accepted in Eur. Phys. J. C (2015)
arxiv created 2015/02/16 · openalex publication_date 2015/03/01 · arxiv updated 2015/03/20 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We report a 3 -D charged black hole solution in an anti-de Sitter space inspired by noncommutative geometry. In this construction, the black hole exhibits two horizons, which turn into a single horizon in the extreme case. We investigate the impacts of electromagnetic field on the location of the event horizon, mass and thermodynamic properties such as Hawking temperature, entropy, and heat capacity of the black hole. The geodesics of the charged black hole are also analyzed.