Spatially regular charged black holes supporting charged massive scalar clouds

We prove that, as opposed to the familiar charged Reissner-Nordstr\"om black-hole spacetime, the spatially regular charged Ay\'on-Beato-Garc\'a (ABG) black-hole spacetime can support charged scalar clouds, spatially regular stationary matter configurations which are made of linearized charged massive scalar fields. Interestingly, we reveal the fact that the composed black-hole-field system is amenable to an analytical treatment in the regime Q/M1 of weakly charged black holes and large-mass fields, in which case it is proved that the dimensionless physical parameter M must lie in the narrow interval (3240{6859}, 1623) here M, Q are the mass and electric charge of the central black hole and, q are the proper mass and charge coupling constant of the supported scalar field. In particular, we explicitly prove that, for weakly charged black holes, the discrete resonance spectrum (M, Q, , q;n) {}₍=₀^n= of the composed charged-ABG-black-hole-charged-massive-scalar-field cloudy configurations can be determined analytically in the eikonal large-mass regime.