Superradiant instabilities of rotating black branes and strings
Vitor Cardoso, Shijun Yoshida

TL;DR
This paper investigates a universal superradiant instability affecting rotating black branes and strings, revealing conditions for instability and stability across different dimensions, with implications for both theoretical physics and laboratory analogs.
Contribution
It identifies a new superradiant instability mechanism in rotating black branes, analyzing its dependence on dimensionality and providing numerical instability timescales.
Findings
Black brane Kerr_4 x R^p is unstable due to superradiance.
Black branes Kerr_d x R^p are stable for d>4.
Laboratory simulation of the instability with acoustic black branes is feasible.
Abstract
Black branes and strings are generally unstable against a certain sector of gravitational perturbations. This is known as the Gregory-Laflamme instability. It has been recently argued that there exists another general instability affecting many rotating extended black objects. This instability is in a sense universal, in that it is triggered by any massless field, and not just gravitational perturbations. Here we investigate this novel mechanism in detail. For this instability to work, two ingredients are necessary: (i) an ergo-region, which gives rise to superradiant amplification of waves, and (ii) ``bound'' states in the effective potential governing the evolution of the particular mode under study. We show that the black brane Kerr_4 x R^p is unstable against this mechanism, and we present numerical results for instability timescales for this case. On the other hand, and quite…
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