2020 Evanescent ergosurface instability
Joe Keir
Anal. PDE 13(6): 1833-1896 (2020). DOI: 10.2140/apde.2020.13.1833

Abstract

Some exotic compact objects, including supersymmetric microstate geometries and certain boson stars, possess evanescent ergosurfaces: time-like submanifolds on which a Killing vector field, which is time-like everywhere else, becomes null. We show that any manifold possessing an evanescent ergosurface but no event horizon exhibits a linear instability of a peculiar kind: either there are solutions to the linear wave equation which concentrate a finite amount of energy into an arbitrarily small spatial region, or the energy of waves measured by a stationary family of observers can be amplified by an arbitrarily large amount. In certain circumstances we can rule out the first type of instability. We also provide a generalisation to asymptotically Kaluza–Klein manifolds. This instability bears some similarity with the “ergoregion instability” of Friedman (Comm. Math. Phys. 63:3 (1978), 243–255), and we use many of the results from the recent proof of this instability by Moschidis (Comm. Math. Phys. 358:2 (2018), 437–520).

Citation

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Joe Keir. "Evanescent ergosurface instability." Anal. PDE 13 (6) 1833 - 1896, 2020. https://doi.org/10.2140/apde.2020.13.1833

Information

Received: 19 October 2018; Revised: 13 June 2019; Accepted: 13 August 2019; Published: 2020
First available in Project Euclid: 22 September 2020

zbMATH: 07271846
MathSciNet: MR4150262
Digital Object Identifier: 10.2140/apde.2020.13.1833

Subjects:
Primary: 35L05 , 35Q75 , 58J45 , 83C57
Secondary: 83E50

Keywords: evanescent ergosurface , General relativity , instability , microstate

Rights: Copyright © 2020 Mathematical Sciences Publishers

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Vol.13 • No. 6 • 2020
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