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- W1528917334 abstract "The interaction rates of dark-matter halos and subhalos, including collisions and mergers, are computed using high-resolution cosmological N-body simulations of the �CDM model. Although the number fraction of subhalos of mass > 2 × 10 11 h −1 M⊙ is only � 10%, we find that the interaction rate of such subhalos is relatively high because they reside in high density environments. At low redshift, the subhalo collisions dominate the total collision rate, and even at z = 3 they are involved in more than 30% of all collisions. About 40% of the “major” mergers (those of mass ratio > 0.3) are between subhalos. Therefore subhalo interactions must be incorporated in models of structure formation. We find that the collision rate between halos in physical density units, is / (1+z) � , with � = 3 4, in agreement with earlier simulations and most observational data. We test previous analytic estimates of the interaction rates of subhalos based on statistical models, which could be very inaccurate because of the small number of subhalos and the variation of conditions within small host halos. We find that, while such statistical estimates may severely overestimate the rate within hosts 6 × 10 11 h −1 M⊙ at all redshifts. The collision rate between subhalos and the central object of their host halo is approximated relatively well using the timescale for dynamical friction in circular orbits. This approximation fails in � 40% of the cases, partly because of deviations from the assumption of circular orbits (especially at low redshift) and partly because of the invalidity of the assumption that the subhalo mass is negligible (especially at high redshift)." @default.
- W1528917334 created "2016-06-24" @default.
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- W1528917334 date "2008-01-01" @default.
- W1528917334 modified "2023-09-27" @default.
- W1528917334 title "Interaction rates of dark-matter halos and subhalos" @default.
- W1528917334 hasPublicationYear "2008" @default.
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