Dynamics of self-gravitating systems : Variations on a theme by Michel Henon

TL;DR

This paper revisits Michel Henon's early work on the dynamics of large self-gravitating systems, exploring conditions for core collapse, binary formation, and subsequent evolution, emphasizing the ongoing relevance of these classical problems.

Contribution

It analyzes the conditions for singularity formation and the evolution of self-gravitating clusters, extending Henon's original insights into modern contexts.

Findings

Conditions for core collapse are identified.

Mechanisms for binary star formation are discussed.

Implications for cluster evaporation are examined.

Abstract

In this contribution to the volume in memoriam of Michel Henon, we thought appropriate to look at his early scientific work devoted to the dynamics of large assemblies of interacting masses. He predicted in his PhD thesis that, in such a system, first a collapse of mass occurs at the center and that later binaries stars are formed there. Henceforth, the negative energy of binding of pairs becomes a source of positive energy for the rest of the cluster which evaporate because of that. We examine under what conditions such a singularity can occur, and what could happen afterwards. We hope to show that this fascinating problem of evolution of self-gravitating clusters keeps its interest after the many years passed since Henon thesis, and is still worth discussing now.