2009/03/31 by Rabin Banerjee, Bibhas Ranjan Majhi · 3 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Black hole (networking) #Black hole thermodynamics #Classical mechanics #Cosmology and Gravitation Theories #Entropy (arrow of time) #Formalism (music) #Hawking #Hawking radiation #Micro black hole #Physics #Quantum Electrodynamics and Casimir Effect #Quantum mechanics #Quantum tunnelling #Theoretical physics #White hole #gr-qc #hep-th
paper · pdf · doi:10.1016/j.physletb.2009.04.005
published as Phys.Lett.B675:243-245,2009 · LaTex, 6 pages, no figures, minor modifications, to appear in Phys. Lett. B
arxiv created 2009/04/05 · openalex publication_date 2009/04/09 · arxiv updated 2014/11/18 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We obtain, using a reformulation of the tunneling mechanism, the Hawking black body spectrum with the appropriate temperature for a black hole. This is a new result in the tunneling formalism of discussing Hawking effect. Our results are given for a spherically symmetric geometry that is asymptotically flat.