A revised flux vector for the collisional evolution of Keplerian orbits

Details A revised flux vector for the collisional evolution of Keplerian orbits A revised flux vector for the collisional evolution of Keplerian orbits

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ap%26ss..56..421h&link_type=abstract

Astrophysics and Space Science, vol. 56, no. 2, July 1978, p. 421-430.

Mathematics

4

Collision Parameters, Computerized Simulation, Kepler Laws, Particle Flux Density, Orbital Elements, Vectors (Mathematics)

Scientific paper

In statistical Keplerian systems the disordered component of collisionally induced motion of matter introduces new terms into the flux vector. This contribution, which is calculated from a transport equation, tends to reduce the density gradient and causes the expansion which is observed in computer simulations of collisional systems. A quantitative comparison with Trulsen's (1972) simulations confirms the revised expression of the flux vector.

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