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Resolving Spacetime Singularities within Asymptotic Safety

Lando Bosma, Benjamin Knorr, and Frank Saueressig
Phys. Rev. Lett. 123, 101301 – Published 5 September 2019

Abstract

A key incentive of quantum gravity is the removal of spacetime singularities plaguing the classical theory. We compute the nonperturbative momentum dependence of a specific structure function within the gravitational asymptotic safety program which encodes the quantum corrections to the graviton propagator for momenta above the Planck scale. The resulting quantum-corrected Newtonian potential approaches a constant negative value as the distance between the two point masses goes to zero, thereby removing the classical singularity. The generic nature of the underlying mechanism suggests that it will remain operative in the context of black hole and cosmic singularities.

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  • Received 19 April 2019

DOI:https://doi.org/10.1103/PhysRevLett.123.101301

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsParticles & Fields

Authors & Affiliations

Lando Bosma*, Benjamin Knorr, and Frank Saueressig

  • Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University Nijmegen, Heyendaalseweg 135, 6525 AJ Nijmegen, Netherlands

  • *l.bosma@science.ru.nl
  • b.knorr@science.ru.nl
  • f.saueressig@science.ru.nl

Article Text

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Issue

Vol. 123, Iss. 10 — 6 September 2019

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