We present a regular class of exact black hole solutions of the Einstein equations coupled with a nonlinear electrodynamics source. For weak fields the nonlinear electrodynamics becomes the Maxwell theory, and asymptotically the solutions behave as the Reissner-Nordström one. The class is endowed with four parameters, which can be thought of as the mass m, charge q, and a sort of dipole and quadrupole moments α and β, respectively. For α ≥ 3, β ≥ 4, and |q| ≤ 2s c m the corresponding solutions are regular charged black holes. For α = 3, they also satisfy the weak energy condition. For α = β = 0 we recover the Reissner-Nordström singular solution and for α = 3, β = 4 the family includes a previous regular black hole reported by the authors.
Keywords Regular black hole · Nonlinear electrodynamicsOne of the active research topics on black hole physics in recent years has been related with its interior behavior. It is clear now that black holes are not necessarily singular and several examples of regular exact black hole solutions has been reported in the literature [1][2][3][4].The research on this subject started with the pioneering work of Bardeen [5] who proposed the first regular black hole model (see also Refs. [4,6,7]). The Bardeen model is a regular black hole satisfying the weak energy condition and it was a crucial guidance on the ulterior investigations related