Unstable horizons and singularity development in holography
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Publication:1696333
DOI10.1007/JHEP07(2017)135zbMATH Open1380.83194arXiv1704.05454OpenAlexW3106404972MaRDI QIDQ1696333
Author name not available (Why is that?)
Publication date: 14 February 2018
Published in: (Search for Journal in Brave)
Abstract: In holographic applications one can encounter scenarios where a long-wavelength instability can arise. In such situations, it is often the case that the dynamical end point of the instability is a new equilibrium phase with a nonlinear scalar hair condensate outside the black hole horizon. We here review holographic setups where symmetric horizons suffer from long-wavelength instabilities where a suitable equilibrium condensate phase does not exist. We study the dynamics of the simplest model in this exotic class, and show that it uncovers arbitrarily large curvatures in the vicinity of the horizon which asymptotically turn such region singular, at finite time with respect to the boundary theory.
Full work available at URL: https://arxiv.org/abs/1704.05454
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