“…one concludes they are all regular everywhere. Hence, for s≤s c the singularities appearing in (13) due to the vanishing of A are only coordinate-singularities describing the existence of event horizons, consequently, we are in the presence of black hole solutions for |q| ≤ 2s c m ≈ 1.05 m. It should be notice that metrics possessing regular standard invariants, as (15)- (17), could still present non-regular behavior of the differential invariants, R ;α1···αn R ;α1···αn , R µν;α1···αn R µν;α1···αn , R µναβ;α1···αn R µναβ;α1···αn [42]. Because of the structure of the metric components of our solution (13) and their derivatives, the components of the Riemman tensor behave generically at r = 0 as ∼ g(r)/r a , where g(r) is a function vanishing exponentially as r → 0.…”