Abstract
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 and , including not only stationary configurations but also time-dependent ones.
- Received 15 June 2015
- Corrected 28 July 2017
DOI:https://doi.org/10.1103/PhysRevD.92.024048
© 2015 American Physical Society
Corrections
28 July 2017