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Supermassive Star Collapse, m=1 initial density perturbation
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Collapse of a rapidly differentially rotating supermassive star with an initial m=1 density perturbation. The star forms a single off-centered fragment which collapses to a black hole.
Simulation & Visualization by Christian Reisswig (Caltech).
Simulation & Visualization by Christian Reisswig (Caltech).
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