2015/03/22 by Frank Saueressig, Natalia Alkofer, Giulio D'Odorico +1 · 1 citation
Physics and Astronomy · #hep-th #gr-qc
published as PoS(FFP14)174 (2014) · 6 pages, 3 figures; prepared for the proceedings of the conference "Frontiers of Fundamental Physics 14"
arxiv created 2015/03/22 · arxiv updated 2016/02/23
Black holes are among the most fascinating objects populating our universe. Their characteristic features, encompassing spacetime singularities, event horizons, and black hole thermodynamics, provide a rich testing ground for quantum gravity ideas. In this note we observe that the renormalization group improved Schwarzschild black holes constructed by Bonanno and Reuter within Weinberg's asymptotic safety program constitute a prototypical example of a Hayward geometry used to model non-singular black holes within quantum gravity phenomenology. Moreover, they share many features of a Planck star: their effective geometry naturally incorporates the one-loop corrections found in the effective field theory framework, their Kretschmann scalar is bounded, and the black hole singularity is replaced by a regular de Sitter patch. The role of the cosmological constant in the renormalization group improvement process is briefly discussed.