Non linear stability of spherical gravitational systems described by the Vlasov-Poisson equation

Author:

Lemou Mohammed

Publisher

Cellule MathDoc/CEDRAM

Reference51 articles.

1. [1] Aly J.-J., On the lowest energy state of a collisionless self-gravitating system under phase volume constraints. MNRAS 241 (1989), 15.

2. [2] Antonov, A. V., Remarks on the problem of stability in stellar dynamics. Soviet Astr., AJ., 4, 859-867 (1961).

3. [3] Antonov, A. V., Solution of the problem of stability of a stellar system with the Emden density law and spherical velocity distribution. J. Leningrad Univ. Se. Mekh. Astro. 7, 135-146 (1962).

4. [4] Arsen’ev, A. A., Global existence of a weak solution of Vlasov’s system of equations, U.S.S.R. Computational Math. and Math. Phys. 15 (1975), 131–141.

5. [5] Batt, J.; Faltenbacher, W.; Horst, E., Stationary spherically symmetric models in stellar dynamics, Arch. Rat. Mech. Anal. 93, 159-183 (1986).

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