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Quantum Evaporation of a Naked Singularity

2005/06/30 by Rituparno Goswami, Pankaj S. Joshi, Parampreet Singh · 11 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Noncommutative and Quantum Gravity Theories #astro-ph #gr-qc #hep-th

paper · pdf · doi:10.1103/physrevlett.96.031302

published as Phys.Rev.Lett. 96 (2006) 031302 · 4 pages, 2 figures. Minor changes to match published version in Physical Review Letters

arxiv created 2006/01/22 · openalex publication_date 2006/01/27 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/01

Abstract

We investigate here quantum effects in gravitational collapse of a scalar field model which classically leads to a naked singularity. We show that nonperturbative semiclassical modifications near the singularity, based on loop quantum gravity, give rise to a strong outward flux of energy. This leads to the dissolution of the collapsing cloud before the singularity can form. Quantum gravitational effects thus censor naked singularities by avoiding their formation. Further, quantum gravity induced mass flux has a distinct feature which may lead to a novel observable signature in astrophysical bursts.

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