Quantum-mechanical corrections to the Schwarzschild black-hole metric

P. Bargueño, S. Bravo Medina, M. Nowakowski, D. Batic

Research output: Contribution to journalArticlepeer-review

19 Scopus citations

Abstract

Motivated by quantum-mechanical corrections to the Newtonian potential, which can be translated into a h-correction to the g00 component of the Schwarzschild metric, we construct a quantum-mechanically corrected metric assuming -g00 = grr. We show how the Bekenstein blackhole entropy S receives its logarithmic contribution provided the quantum-mechanical corrections to the metric are negative. In this case the standard horizon at the Schwarzschild radius rS increases by small terms proportional to h and a remnant of the order of Planck mass emerges.

Original languageBritish English
Article number60006
JournalEurophysics Letters
Volume117
Issue number6
DOIs
StatePublished - Mar 2017

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