Retrograde polish doughnuts around boson stars

DOI10.1088/1475-7516/2021/03/063zbMath1485.85019arXiv2011.10288OpenAlexW3107455540MaRDI QIDQ5026022

Matheus C. Teodoro, Jutta Kunz, Lucas G. Collodel

Publication date: 7 February 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2011.10288

zbMATH Keywords

gravityaccretionastrophysical fluid dynamics

Mathematics Subject Classification ID

Toric varieties, Newton polyhedra, Okounkov bodies (14M25) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Orbital mechanics (70M20) Stability and instability of geophysical and astrophysical flows (76E20) Motion of the gyroscope (70E05)

Cites Work

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• Efficient vectorizable PDE solvers
• Boson stars: Rotation, formation, and evolution
• Shadows of Kerr black holes with and without scalar hair
• Circular geodesics and thick tori around rotating boson stars
• General relativistic boson stars
• Comparing timelike geodesics around a Kerr black hole and a boson star
• On tidal disruption of clouds and disk formation near boson stars
• Spinning and excited black holes in Einstein-scalar-Gauss–Bonnet theory
• Relativistic thick discs in the Kerr–de Sitter backgrounds
• Geons
• Dynamical boson stars

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