Non-extensive systems do not allow to go to the thermodynamic limit.
Therefore we have to reformulate statistical mechanics without invoking the
thermodynamical limit. I.e. we have to go back to Pre-Gibbsian times. We show
that Boltzmann’s mechanical definition of entropy S as function of the
conserved extensive'' variables energy E, particle number N etc. allows to describe even the most sophisticated cases of phase transitions unambiguously for small’’ systems like nuclei, atomic clusters, and selfgravitating
astrophysical systems: The rich topology of the curvature of S(E,N) shows the
whole Zoo'' of transitions: transitions of 1.order including the surface tension at phase-separation, continuous transitions, critical and multi-critical points. The transitions are the catastrophes’’ of the Laplace
transform from the extensive'' to the intensive’’ variables. Moreover, this
classification of phase transitions is much more natural than the Yang-Lee
criterion.

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