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Hawking radiation as quantum tunneling from a noncommutative Schwarzschild black hole

2008/01/31 by Kourosh Nozari, S. Hamid Mehdipour · 8 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Black hole (networking) #General relativity #Gravitation #Gravitational wave #Hawking radiation #Mathematical physics #Micro black hole #Noncommutative and Quantum Gravity Theories #Noncommutative geometry #Noncommutative quantum field theory #Physics #Quantum Electrodynamics and Casimir Effect #Quantum electrodynamics #Quantum mechanics #Schwarzschild metric #Schwarzschild radius #White hole #gr-qc

paper · pdf · doi:10.1088/0264-9381/25/17/175015

published as Class.Quant.Grav.25:175015,2008 · 19 Pages, 4 Figures, revised, new material and references added

arxiv created 2008/05/21 · openalex publication_date 2008/08/19 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We study the tunneling process through the quantum horizon of a Schwarzschild black hole in noncommutative spacetime. This is done by considering the effect of smearing of the particle mass as a Gaussian profile in flat spacetime. We show that even in this noncommutative setup there will be no correlation between the different modes of radiation, which reflects the fact that information does not come out continuously during the evaporation process at least at late time. However, due to spacetime noncommutativity, information might be preserved by a stable black hole remnant.

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