Circular geodesics and thick tori around rotating boson stars

DOI10.1088/0264-9381/32/23/235022zbMath1329.83058arXiv1510.04191OpenAlexW3103358438MaRDI QIDQ3466391

R. Monceau-Baroux, F. H. Vincent, Zakaria Meliani, Odele Straub, Eric Gourgoulhon, Philippe Grandclément

Publication date: 1 February 2016

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1510.04191

zbMATH Keywords

black holegravitationhydrodynamicsboson starsaccretion disk

Mathematics Subject Classification ID

Black holes (83C57) Applications of differential geometry to physics (53Z05) Galactic and stellar structure (85A15) Equations of motion in general relativity and gravitational theory (83C10) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (5)

Comparing timelike geodesics around a Kerr black hole and a boson star ⋮ On tidal disruption of clouds and disk formation near boson stars ⋮ The Milky Way's supermassive black hole: how good a case is it? A challenge for astrophysics \& philosophy of science ⋮ Dynamical boson stars ⋮ Retrograde polish doughnuts around boson stars

Uses Software

• KADATH
• HARMRAD

Cites Work

• KADATH: a spectral solver for theoretical physics
• Dynamical boson stars
• Unnamed Item
• Unnamed Item

This page was built for publication: Circular geodesics and thick tori around rotating boson stars