Quantum-corrected black hole thermodynamics to all orders in the Planck length

By Khireddine Nouicer. 2007

206 citations recorded by the source corpus.

We investigate the effects to all orders in the Planck length from a generalized uncertainty principle (GUP) on black holes thermodynamics. We calculate the corrected Hawking temperature, entropy, and examine in details the Hawking evaporation process. As a result, the evaporation process is accelerated and the evaporation end-point is a zero entropy, zero heat capacity and finite non-zero temperature black hole remnant (BHR). In particular we obtain a drastic reduction of the decay time, in comparison with the results obtained in the Hawking semi classical picture and with the GUP to leading order in the Planck length.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/7e87d099a47667efe115977de513c106c2ddf5ad

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In Astronomy and Astrophysics

1. Dong-han Yeom
2. Y. Ong
3. Pisin Chen

In Nuclear and High Energy Physics

1. Dong-han Yeom
2. Y. Ong
3. Pisin Chen

In Statistical and Nonlinear Physics

1. Dong-han Yeom
2. Y. Ong
3. Pisin Chen

Citations in the corpus

• Black Hole Remnants and the Information Loss Paradox (2014, background): “Over the years, progresses have been made in both understanding GUP as well as applying GUP to various black holes [which consistently yield remnant pictures] [59–71].”