How to simulate collective relaxation processes in a stellar disk by numerical experiments

Details How to simulate collective relaxation processes in a stellar disk by numerical experiments How to simulate collective relaxation processes in a stellar disk by numerical experiments

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..333z&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, April 1987, p. 333-337. In Russian. In Russian.

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Computation

Computational Astrophysics, Particle Motion, Relaxation, Rotating Disks, Stellar Gravitation, Stellar Models, Stellar Motions, Stellar Structure

Scientific paper

Methods of a numerically experimental investigation of collective relaxation processes in models of a stellar disk with continuous description of motion of particles stars are provided. It is shown that for correct modelling of a collisionless stellar disk the shape of the "cutoff region" of gravitational interaction at short distances must be ellipsoidal (the "cutoff radius" across the plane of the disk must be smaller than the "cutoff radius" in its plane).

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