Working in the geometric approach, we construct the lagrangians of N=1 and
N=2 pure supergravity in four dimensions with negative cosmological constant,
in the presence of a non trivial boundary of space-time. We find that the
supersymmetry invariance of the action requires the addition of topological
terms which generalize at the supersymmetric level the Gauss-Bonnet term.
Supersymmetry invariance is achieved without requiring Dirichlet boundary
conditions on the fields at the boundary, rather we find that the boundary
values of the fieldstrengths are dynamically fixed to constant values in terms
of the cosmological constant \Lambda. From a group-theoretical point of view
this means in particular the vanishing of the OSp(N|4)-supercurvatures at the
boundary.Comment: Some clarifications on the N=1 case, typos correcte