Collapse of a Rotating Supermassive Star to a Supermassive Black Hole: Fully Relativistic Simulations
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference27 articles.
1. SYMMETRY WITHOUT SYMMETRY: NUMERICAL SIMULATION OF AXISYMMETRIC SYSTEMS USING CARTESIAN GRIDS
2. Gravothermal Collapse of Self-Interacting Dark Matter Halos and the Origin of Massive Black Holes
3. Evolution of Rotating Supermassive Stars to the Onset of Collapse
4. The fate of dense stellar systems
5. Apparent horizons for boosted or spinning black holes
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