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Three-Dimensional Stationary Spherically Symmetric Stellar Dynamic Models DEpending on Local Energy - MaRDI portal

Three-Dimensional Stationary Spherically Symmetric Stellar Dynamic Models DEpending on Local Energy

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Publication:6371976

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DOI10.1134/S0965542522090081zbMath1511.85001arXiv2107.01898MaRDI QIDQ6371976

Jürgen Batt, Alexander L. Skubachevskii, Enno Jörn

Publication date: 5 July 2021

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)

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