The runaway instability in general relativistic accretion discs

When an accretion disc falls prey to the runaway instability, a large portion of its mass is devoured by the black hole within a few dynamical times. Despite decades of effort, it is still unclear under what conditions such an instability can occur. The technically most advanced relativistic simulat...

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Bibliographic Details
Published in:Monthly Notices of the Royal Astronomical Society
Main Authors: Korobkin, O., Abdikamalov, E., Stergioulas, N., Schnetter, E., Zink, B., Rosswog, S., Ott, C. D.
Format: Article in Journal/Newspaper
Language:unknown
Published: Royal Astronomical Society 2013
Subjects:
Online Access:https://doi.org/10.1093/mnras/stt166