On the role of irregular forces in weakly non-stationary self-gravitating systems

Details On the role of irregular forces in weakly non-stationary self-gravitating systems On the role of irregular forces in weakly non-stationary self-gravitating systems

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974afz....10..611a&link_type=abstract

Astrofizika, vol. 10, Nov. 1974, p. 611-624. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Collision Parameters, Gravitational Effects, Stellar Gravitation, Stellar Systems, Two Body Problem, Binary Stars, Conservation Laws, Stellar Evolution, Stellar Mass, Stellar Motions

Scientific paper

A suitable simple approximation of the collision integral is proposed. The conservation of energy and the Boltzmann's H-theorem are fulfilled. The role of irregular forces in a weakly nonstationary self-gravitating system is investigated by means of this approximation. The Jeans' critical wavelength is not affected by the magnitude of irregular forces. The increments are decreased by the irregular forces in all typical cases.

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