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• W2014202272 endingPage "012050" @default.
• W2014202272 startingPage "012050" @default.
• W2014202272 abstract "We investigate new paths to black hole formation by considering the general relativistic evolution of a differentially rotating polytrope with toroidal shape. We find that this polytrope is unstable to nonaxisymmetric modes, which leads to a fragmentation into self-gravitating, collapsing components. In the case of one such fragment, we apply a simplified adaptive mesh refinement technique to follow the evolution to the formation of an apparent horizon centered on the fragment. This is the first study of the one-armed instability in full general relativity." @default.
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• W2014202272 date "2007-05-01" @default.
• W2014202272 modified "2023-09-26" @default.
• W2014202272 title "Supermassive Black Hole Formation through Rotational Instabilities" @default.
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• W2014202272 doi "https://doi.org/10.1088/1742-6596/68/1/012050" @default.
• W2014202272 hasPublicationYear "2007" @default.
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