Relaxation of collisionless self-gravitating matter - The final state

Details Relaxation of collisionless self-gravitating matter - The final state Relaxation of collisionless self-gravitating matter - The final state

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.238.1261z&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 238, June 1, 1989, p. 1261-1280. Research supported by

Statistics

Computation

22

Computational Astrophysics, Gravitational Effects, Matter (Physics), Density Distribution, Distribution Functions, Evolution (Development), Relaxation

Scientific paper

In a recent paper Wiechen et al. (1988) have presented a new concept for the relaxation of collisionless self-gravitating matter. This paper is concerned with the problem of how to calculate final states of violent relaxation quantitatively, incorporating the energy distance of an initial distribution from its lowest energy state that is accessible under conservation of phase space density. The loss of information due to the relaxation is controlled by that energy distance. The dynamical evolution of an initial distribution is treated numerically for an example with spherical symmetry. The results are in good agreement with the predictions of the relaxation model.

Affiliated with

Also associated with

No associations

Rating

Relaxation of collisionless self-gravitating matter - The final state does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Relaxation of collisionless self-gravitating matter - The final state, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Relaxation of collisionless self-gravitating matter - The final state will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1855931