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Planck star phenomenology

It is possible that black holes hide a core of Planckian density, sustained by quantum-gravitational pressure. As a black hole evaporates, the core remembers the initial mass and the final explosion occurs at macroscopic scale. We investigate possible phenomenological consequences of this idea. Under several rough assumptions, we estimate that up to several short gamma-ray bursts per day, around 10 MeV, with isotropic distribution, can be expected coming from a region of a few hundred light years around us.

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Co-authorshipAuthorshipAuthorshipTopic signalTopic signalTopic signalTopic signalRelated contextRelated contextRelated contextWPlanck star phenomenologypreprint / 2014AAurelien BarrauResearcherACarlo RovelliResearcherThep-ph13193 worksTastro-ph.CO6979 worksTgr-qc10727 worksThep-th13268 works
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Planck star phenomenology

preprint / 2014

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