17-19 April 2023
HC Seminar Room
Europe/London timezone

Self-gravitating systems -- such as star clusters, stellar discs, and dark matter halos -- are rich with dynamical phenomena. They exhibit both resonant (long-range) and non-resonant (short-range) dynamics, with unclear transition regimes. The coupling of linear response theory, kinetic theory, quasilinear theory, and N-body approaches for studying self-gravitating systems is now within reach, owing to recent theoretical breakthroughs. This workshop will bring together dynamicists with expertise in all these areas for a direct comparison of techniques.

HC Seminar Room
The Higgs Centre for Theoretical Physics School of Physics and Astronomy James Clerk Maxwell Building, 4305 Peter Guthrie Tait Road Edinburgh EH9 3FD UK
Application for this event is currently open.
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