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...

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Bibliographic Details
Main Authors: Roupas, Z, Kocsis, B, Tremaine, S
Format: Journal article
Language:English
Published: IOP Publishing 2017