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We address the post-collapse dynamics of a self-gravitating gas of Brownianparticles in D dimensions, in both canonical and microcanonical ensembles. Inthe canonical ensemble, the post-collapse evolution is marked by the formationof a Dirac peak with increasing mass. The density profile outside the peakevolves self-similarly with decreasing central density and increasing coreradius. In the microcanonical ensemble, the post-collapse regime is marked bythe formation of a ``binary''-like structure surrounded by an almost uniformhalo with high temperature. These results are consistent with thermodynamicalpredictions

Postcollapse dynamics of self-gravitating Brownian particles and bacterial populations