2015/06/30 by Eloy Ayón-Beato, Eloy Ayón–Beato, Mokhtar Hassaı̈ne +2 · 1 citation
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Black hole (networking) #Computer science #Conformal field theory #Conformal map #Conformal symmetry #Cosmology and Gravitation Theories #Dimension (graph theory) #Geometry #Mathematical physics #Mathematics #Particle physics theoretical and experimental studies #Physics #Primary field #Pure mathematics #Scalar (mathematics) #Theoretical physics #gr-qc #hep-th
paper · pdf · doi:10.1103/physrevd.92.024048
published as Phys. Rev. D 92, 024048 (2015) · 8 pages
openalex publication_date 2015/07/29 · arxiv created 2017/07/17 · arxiv updated 2017/07/18 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Black holes supported by self-interacting conformal scalar fields can be considered as renormalizably dressed since the conformal potential is nothing but the top power-counting renormalizable self-interaction in the relevant dimension. On the other hand, potentials defined by powers which are lower than the conformal one are also phenomenologically relevant since they are in fact super-renormalizable. In this work we provide a new map that allows one to build black holes dressed with all the (super-)renormalizable contributions starting from known conformal seeds. We explicitly construct several new examples of these solutions in dimensions D=3 and D=4, including not only stationary configurations but also time-dependent ones.