Binary Relaxation in Cold Collapse of a Self-Gravitating N-Body System

Details Binary Relaxation in Cold Collapse of a Self-Gravitating N-Body System Binary Relaxation in Cold Collapse of a Self-Gravitating N-Body System

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994pthph..91...17y&link_type=abstract

Progress of Theoretical Physics, Vol. 91, No. 1, pp. 17-26.

Physics

Scientific paper

Binary relaxation in a cold collapse system is examined. Though the virial ratio k oscillates violently in this system, it does not exceed 2 because the system is bounded. We find that binary relaxation is not negligible after the first collapse if the maximum virial ratio kmax becomes as large as 2 - O(N-1) during the collapse. But it seems that such a large virial ratio cannot be realized in any galactic system.

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