Black hole solutions in Einstein–Maxwell–Yang–Mills–Gauss–Bonnet theory

Abstract

We consider Maxwell and Yang-Mills (YM) fields together, interacting through gravity both in Einstein and Gauss-Bonnet (GB) theories. For this purpose we choose two different sets of Maxwell and metric ansaetze. In our first ansatz, asymptotically for r→0 (and N>4) the Maxwell field dominants over the YM field. In the other asymptotic region, r→∞, however, the YM field becomes dominant. For N=3 and N=4, where the GB term is absent, we recover the well-known Ba\U{f1}ados-Teitelboim-Zanelli (BTZ) and Reissner-Nordstr\U{f6}m (RN) metrics, respectively. The second ansatz corresponds to the case of constant radius function for SN−2 part in the metric. This leads to the Bertotti-Robinson (BR) type solutions in the underlying theory.