  We obtain a family of regular static, spherically symmetric solutions in
Einstein--Cartan theory with an electromagnetic field and a nonminimally
coupled scalar field with the correct sign of kinetic energy density. At
different values of its parameters, the solution, being asemptotically flat at
large values of the radial coordinate, describes (i) twice asemptotically flat
symmetric wormholes, (ii) asymmetric wormholes with an AdS asymptotic at the
"far end", (iii) regular black holes with an extremal horizon or two simple
horizons, and (iv) black universes with a de Sitter asymptotic at the "far
end". As in other black universe models, it is a black hole as seen by a
distant observer, but beyond its horizon there is a nonsingular expanding
universe. In all these cases, both the metric and the torsion are regular in
the whole space.
