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Evolution and endpoint of the black string instability: Large D solution

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arxiv 1506.06772 v2 pith:QARTXS2Z submitted 2015-06-22 hep-th gr-qc

Evolution and endpoint of the black string instability: Large D solution

classification hep-th gr-qc
keywords blackstringsequationslargebranesdescribedimensionsendpoint
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We derive a simple set of non-linear, (1+1)-dimensional partial differential equations that describe the dynamical evolution of black strings and branes to leading order in the expansion in the inverse of the number of dimensions D. These equations are easily solved numerically. Their solution shows that thin enough black strings are unstable to developing inhomogeneities along their length, and at late times they asymptote to stable non-uniform black strings. This proves an earlier conjecture about the endpoint of the instability of black strings in a large enough number of dimensions. If the initial black string is very thin, the final configuration is highly non-uniform and resembles a periodic array of localized black holes joined by short necks. We also present the equations that describe the non-linear dynamics of Anti-deSitter black branes at large D.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Black Hole Ringdown Nonlinearities in the Large-D Limit

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    In the large-D limit, analytic third-order nonlinear corrections to quasinormal modes improve ringdown modeling accuracy by several orders of magnitude for head-on black hole collisions.

  2. On prethermal time crystals from semi-holography

    hep-th 2025-12 unverdicted novelty 5.0

    Semi-holographic systems with perturbative and holographic sectors exhibit prethermal time crystals through dissipationless modes in hydrodynamic channels plus short-wavelength instabilities that produce inhomogeneiti...