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Updated: Aug 8, 2026

Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
Rayleigh-Plateau and Gregory-Laflamme instabilities of black strings
Vitor Cardoso1, Oscar J C Dias
1Department of Physics and Astronomy, The University of Mississippi, University, Mississippi 38677-1848, USA. vcardoso@phy.olemiss.edu
Abstract:
Many and very general arguments indicate that the event horizon behaves as a stretched membrane. We explore this analogy by associating the Gregory-Laflamme instability of black strings with a classical membrane instability known as the Rayleigh-Plateau instability. We show that the key features of the black string instability can be reproduced using this viewpoint. In particular, we get good agreement for the threshold mode in all dimensions and exact agreement for large spacetime dimensionality. The instability time scale is also well described within this model, as well as the dimensionality dependence. It also predicts that general nonaxisymmetric perturbations are stable. We further argue that the instability of ultraspinning black holes follows from this model.
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