Nonlocal black-hole thermodynamics and massive remnants

Details Nonlocal black-hole thermodynamics and massive remnants Nonlocal black-hole thermodynamics and massive remnants

2006-07-20

arxiv.org/abs/hep-th/0607140v1

Physics

High Energy Physics

High Energy Physics - Theory

7 pages, 1 figure included

Scientific paper

To alleviate the black-hole (BH) information problem, we study a holographic-principle-inspired nonlocal model of Hawking radiation in which radiated particles created at different times all have the same temperature corresponding to the instantaneous BH mass. Consequently, the black hole loses mass not only by continuously radiating new particles, but also by continuously warming previously radiated particles. The conservation of energy implies that the radiation stops when the mass of the black hole reaches the half of the initial BH mass, leaving a massive BH remnant with a mass much above the Planck scale.

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