  The conventional approach describes the spherical domain walls by the same
state equation as the flat ones. In such case they also must be gravitationally
repulsive, what is seemingly in contradiction with Birkhoff's theorem. However
this theorem is not valid for the solutions which do not display Minkowski
geometry in the infinity. In this paper the solution of Einstein equations
describing the stable gravitationally repulsive spherical domain wall is
considered within the thin-wall formalism for the case of the non-Minkowskian
asymptotics.
