MASS SEGREGATION RELAXATION, AND THE COULOMB LOGARITHM IN N-BODY SYSTEMS (AGAIN)

被引:29
作者
FAROUKI, RT [1 ]
SALPETER, EE [1 ]
机构
[1] CORNELL UNIV,CTR RADIOPHYS & SPACE RES,ITHACA,NY 14853
关键词
CELESTIAL MECHANICS; STELLAR DYNAMICS; GALAXIES; CLUSTERING; METHODS; NUMERICAL;
D O I
10.1086/174174
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The question of the upper cutoff b(max) in the ''Coulomb logarithm'' for self-gravitating N-body systems has been reexamined, based on both large-scale mass segregation and cumulative squared changes in orbital energies as measures of relaxation. Simulations of greater scope than those of an earlier study of the authors, together with a more sophisticated statistical procedure for estimating b(max), unequivocally support the conclusion of that study-namely, b(max) has a roughly constant value comparable to the half-mass radius R, rather than a value is similar to N-1/3 R representative of the mean interparticle spacing that decreases with N. The ratios of the relaxation times observed in simulations using different softening lengths for the gravitational potential exhibit an N-dependence that agrees quantitatively with the postulate b(max) almost-equal-to R, but is conspicuously inconsistent with b(max) almost-equal-to N-1/3 R. These findings do not corroborate those of Smith (1992).
引用
收藏
页码:676 / 683
页数:8
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