Numerical simulations of collisions in systems of non-identical particles

Details Numerical simulations of collisions in systems of non-identical particles Numerical simulations of collisions in systems of non-identical particles

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984em%26p...30..229s&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 30, June 1984, p. 229-243. Translation.

Other

13

Astronomical Models, Particle Collisions, Planetary Evolution, Computerized Simulation, Kinetic Energy, Particle Size Distribution, Ring Structures

Scientific paper

The numerical simulations of 200 mutually colliding, non-identical particles indicate that if elasticity depends on the impact velocity, an equipartition of the random kinetic energy is possible if either the particle masses are close to each other, or the number of small particles significantly exceeds that of large particles. On the other hand, if the large particles dominate, the velocities of the smaller particles are at most a few times greater than those of the large ones. In the case of a constant coefficient of restitution no equipartition is observed.

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