Gravothermal Expansion in an -Body System
arXiv:astro-ph/9308046 · doi:10.1093/mnras/271.3.706
Abstract
This paper describes the numerical evolution of an -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 the core of such a system expands on a time-scale of thousands of central relaxation times, and here this behaviour is qualitatively confirmed for an -body system of over 3000 bodies. With certain qualifications, this demonstrates the existence in N-body systems of one of the fundamental mechanisms which, in fluid models, drive the gravothermal oscillations discovered by Bettwieser & Sugimoto.
25pp and 12 figures (available from [email protected]), tex
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