Effects of the rotation of the central black hole in a disk galaxy model

DOI10.1007/s11012-022-01577-7zbMath1525.83015OpenAlexW4294771882MaRDI QIDQ6100359

Unnamed Author, Fredy L. Dubeibe, Euaggelos E. Zotos

Publication date: 22 June 2023

Published in: Meccanica (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s11012-022-01577-7

zbMATH Keywords

black hole physicsgalaxies: kinematics and dynamicsgalaxies: structure and chaos

Mathematics Subject Classification ID

Black holes (83C57) Strange attractors, chaotic dynamics of systems with hyperbolic behavior (37D45) Galactic and stellar structure (85A15) Galactic and stellar dynamics (85A05) Orbital mechanics (70M20) Resonance in context of PDEs (35B34) Motion of the gyroscope (70E05)

Cites Work

• Unnamed Item
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• Stability of orbits around a spinning body in a pseudo-Newtonian Hill problem
• Newtonian and pseudo-Newtonian Hill problem
• Physics of black holes. Transl. from the Russian by V. I. Kisin and E. M. Yankovsky
• Pseudo-Newtonian planar circular restricted 3-body problem
• Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
• Alignment indices: a new, simple method for determining the ordered or chaotic nature of orbits

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