Unstable horizons and singularity development in holography
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....
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doaj-dad5d19fac2145c683bf7b792d57322b2020-11-24T20:55:16ZengSpringerOpenJournal of High Energy Physics1029-84792017-07-012017713110.1007/JHEP07(2017)135Unstable horizons and singularity development in holographyPablo Bosch0Alex Buchel1Luis Lehner2Department of Physics & Astronomy and Guelph-Waterloo Physics Institute, University of WaterlooDepartment of Applied MathematicsPerimeter Institute for Theoretical PhysicsAbstract 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.http://link.springer.com/article/10.1007/JHEP07(2017)135Gauge-gravity correspondenceSpacetime Singularities |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Pablo Bosch Alex Buchel Luis Lehner |
spellingShingle |
Pablo Bosch Alex Buchel Luis Lehner Unstable horizons and singularity development in holography Journal of High Energy Physics Gauge-gravity correspondence Spacetime Singularities |
author_facet |
Pablo Bosch Alex Buchel Luis Lehner |
author_sort |
Pablo Bosch |
title |
Unstable horizons and singularity development in holography |
title_short |
Unstable horizons and singularity development in holography |
title_full |
Unstable horizons and singularity development in holography |
title_fullStr |
Unstable horizons and singularity development in holography |
title_full_unstemmed |
Unstable horizons and singularity development in holography |
title_sort |
unstable horizons and singularity development in holography |
publisher |
SpringerOpen |
series |
Journal of High Energy Physics |
issn |
1029-8479 |
publishDate |
2017-07-01 |
description |
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. |
topic |
Gauge-gravity correspondence Spacetime Singularities |
url |
http://link.springer.com/article/10.1007/JHEP07(2017)135 |
work_keys_str_mv |
AT pablobosch unstablehorizonsandsingularitydevelopmentinholography AT alexbuchel unstablehorizonsandsingularitydevelopmentinholography AT luislehner unstablehorizonsandsingularitydevelopmentinholography |
_version_ |
1716791985001463808 |