Isotropic–nematic phase transitions in gravitational systems
We examine dense self-gravitating stellar systems dominated by a central potential, such as nuclear star clusters hosting a central supermassive black hole. Different dynamical properties of these systems evolve on vastly different timescales. In particular, the orbital-plane orientations are typica...
Main Authors: | , , |
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Format: | Journal article |
Language: | English |
Published: |
IOP Publishing
2017
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