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JHEP 1205, 054 (2012) 38
Shaping black holes with free fields
Yannis Bardoux 1, Marco M. Caldarelli 1, 2, Christos Charmousis 1, 3
(2012)

Starting from a metric Ansatz permitting a weak version of Birkhoff's theorem we find static black hole solutions including matter in the form of free scalar and p-form fields, with and without a cosmological constant \Lambda. Single p-form matter fields permit multiple possibilities, including dyonic solutions, self-dual instantons and metrics with Einstein-Kaelher horizons. The inclusion of multiple p-forms on the other hand, arranged in a homogeneous fashion with respect to the horizon geometry, permits the construction of higher dimensional dyonic p-form black holes and four dimensional axionic black holes with flat horizons, when \Lambda<0. It is found that axionic fields regularize black hole solutions in the sense, for example, of permitting regular -- rather than singular -- small mass Reissner-Nordstrom type black holes. Their cosmic string and Vaidya versions are also obtained.
1:  Laboratoire de Physique Théorique d'Orsay (LPT)
CNRS : UMR8627 – Université Paris XI - Paris Sud
2:  Centre de Physique Théorique (CPHT)
CNRS : UMR7644 – Polytechnique - X
3:  Laboratoire de Mathématiques et Physique Théorique (LMPT)
CNRS : UMR6083 – Université François Rabelais - Tours
Physics/General Relativity and Quantum Cosmology

Physics/High Energy Physics - Theory
Fulltext link: 
http://fr.arXiv.org/abs/1202.4458