Self-Similar Approach to Violent Relaxation

dc.creatorHenriksen, Richard
dc.creatorWidrow, Lawrence M.
dc.date1996-12-02
dc.date.accessioned2026-07-25T20:16:42Z
dc.descriptionWe consider the evolution of an initially cold, spherically symmetric system of self-gravitating particles. At early times the system undergoes self-similar collapse of the type described by Fillmore & Goldreich and Bertschinger. This stage of phase mixing soon gives way to a period of violent relaxation driven by an instability in the similarity solution. The onset of violent relaxation is illustrated by numerical simulations and supported by non-linear analysis of the ``scaled'' collisionless Boltzmann and Poisson equations.
dc.description5 pages, 2 postscript figures in compressed format, submitted to Physical Review Letters
dc.identifierhttps://arxiv.org/abs/astro-ph/9612023
dc.identifierhttp://arxiv.org/abs/astro-ph/9612023
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/70087
dc.subjectAstrophysics
dc.titleSelf-Similar Approach to Violent Relaxation
dc.typetext

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