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 asymptotic...
Many and very general arguments indicate that the event horizon behaves as a stretched membrane. We ...
Geodesic motion determines important features of spacetimes. Null unstable geodesics are closely rel...
We prove that, in a class of spherically symmetric spacetimes exhibiting stable trapping of null geo...
Some exotic compact objects, including supersymmetric microstate geometries and certain boson stars,...
We investigate the classical stability of supersymmetric, asymptotically flat, microstate geometries...
There are still many important unsolved problems in general relativity, two of which are the stabil...
Open Access.It has been known classically that a star with an ergoregion but no event horizon is uns...
Recently certain nonsupersymmetric solutions of type IIb supergravity were constructed [V. Jejjala, ...
Supersymmetric microstate geometries with five non-compact dimensions have recently been shown by Ep...
Gravitational-wave astronomy can give us access to the structure of black holes, potentially probing...
Supersymmetric microstate geometries were recently conjectured (Eperon et al. in JHEP 10:031, 2016. ...
We prove that a large class of smooth solutions ψ to the linear wave equation □ g ψ=0 on subextremal...
In this Letter, we introduce the nonlinear partial differential equation ∂2τπ∝(→∇π)2 showing a new t...
Rotating, ultra-compact stars in general relativity can have an ergoregion, in which all trajectorie...
Spinning horizonless compact objects may be unstable against an "ergoregion instability." We investi...
Many and very general arguments indicate that the event horizon behaves as a stretched membrane. We ...
Geodesic motion determines important features of spacetimes. Null unstable geodesics are closely rel...
We prove that, in a class of spherically symmetric spacetimes exhibiting stable trapping of null geo...
Some exotic compact objects, including supersymmetric microstate geometries and certain boson stars,...
We investigate the classical stability of supersymmetric, asymptotically flat, microstate geometries...
There are still many important unsolved problems in general relativity, two of which are the stabil...
Open Access.It has been known classically that a star with an ergoregion but no event horizon is uns...
Recently certain nonsupersymmetric solutions of type IIb supergravity were constructed [V. Jejjala, ...
Supersymmetric microstate geometries with five non-compact dimensions have recently been shown by Ep...
Gravitational-wave astronomy can give us access to the structure of black holes, potentially probing...
Supersymmetric microstate geometries were recently conjectured (Eperon et al. in JHEP 10:031, 2016. ...
We prove that a large class of smooth solutions ψ to the linear wave equation □ g ψ=0 on subextremal...
In this Letter, we introduce the nonlinear partial differential equation ∂2τπ∝(→∇π)2 showing a new t...
Rotating, ultra-compact stars in general relativity can have an ergoregion, in which all trajectorie...
Spinning horizonless compact objects may be unstable against an "ergoregion instability." We investi...
Many and very general arguments indicate that the event horizon behaves as a stretched membrane. We ...
Geodesic motion determines important features of spacetimes. Null unstable geodesics are closely rel...
We prove that, in a class of spherically symmetric spacetimes exhibiting stable trapping of null geo...