Three-dimensional stationary spherically symmetric stellar dynamic models depending on the local energy

DOI10.1134/S0965542522090081MaRDI QIDQ2088679

Jürgen Batt, Alexander L. Skubachevskii, Enno Jörn

Publication date: 6 October 2022

Published in: Computational Mathematics and Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2107.01898

zbMATH Keywords

stationary solutionsnumerical approximationthree-dimensional Vlasov-Poisson system

Mathematics Subject Classification ID

Density estimation (62G07) Other nonlinear integral equations (45G10) Inverse problems for PDEs (35R30) Celestial mechanics (70F15) Galactic and stellar dynamics (85A05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Cites Work

• Stationary spherically symmetric models in stellar dynamics
• Stationary solutions of the flat Vlasov-Poisson system
• Stationary spherically symmetric solutions of the Vlasov-Poisson system in the three-dimensional case
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