GRAVOTHERMAL EXPANSION IN AN N-BODY SYSTEM

This paper describes the numerical evolution of an N-body system with a slight 'temperature inversion'; i.e. the maximum velocity dispersion occurs not at the centre but further out. Fluid models predict that t he core of such a system expands on a time-scale of thousands of centr al relaxation times, and here this behaviour is qualitatively confirme d for an N-body system of over 3000 bodies. With certain qualification s, this demonstrates the existence in N-body systems of one of the fun damental mechanisms that, in fluid models, drive the gravothermal osci llations discovered by Bettwieser and Sugimoto.