Abstract

Given a bounded domain D⊂RnD \subset {\mathbb R}^n strictly starlike with respect to 0∈D ,0 \in D\,, we define a quasi-inversion w.r.t. the boundary ∂D .\partial D \,. We show that the quasi-inversion is bi-Lipschitz w.r.t. the chordal metric if and only if every "tangent line" of ∂D\partial D is far away from the origin. Moreover, the bi-Lipschitz constant tends to 1,1, when ∂D\partial D approaches the unit sphere in a suitable way. For the formulation of our results we use the concept of the αα-tangent condition due to F. W. Gehring and J. Väisälä (Acta Math. 1965). This condition is shown to be equivalent to the bi-Lipschitz and quasiconformal extension property of what we call the polar parametrization of ∂D\partial D. In addition, we show that the polar parametrization, which is a mapping of the unit sphere onto ∂D ,\partial D\,, is bi-Lipschitz if and only if DD satisfies the αα-tangent condition.

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