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Black brane viscosity and the Gregory-Laflamme instability

TLDR
In this article, the authors studied long wavelength perturbations of neutral black p-branes in asymptotically flat space and showed that solutions of the relativistic hydrodynamic equations for an effective p + 1-dimensional fluid yield solutions to the vacuum Einstein equations in a derivative expansion.
Abstract
We study long wavelength perturbations of neutral black p-branes in asymptotically flat space and show that, as anticipated in the blackfold approach, solutions of the relativistic hydrodynamic equations for an effective p + 1-dimensional fluid yield solutions to the vacuum Einstein equations in a derivative expansion. Going beyond the perfect fluid approximation, we compute the effective shear and bulk viscosities of the black brane. The values we obtain saturate generic bounds. Sound waves in the effective fluid are unstable, and have been previously related to the Gregory-Laflamme instability of black p-branes. By including the damping effect of the viscosity in the unstable sound waves, we obtain a remarkably good and simple approximation to the dispersion relation of the Gregory-Laflamme modes, whose accuracy increases with the number of transverse dimensions. We propose an exact limiting form as the number of dimensions tends to infinity.

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The large D limit of General Relativity

TL;DR: In this article, it was shown that massless scalar fields can be approximated to leading order in 1/D and the scalar absorption probability can be computed analytically in the large D expansion.
Journal ArticleDOI

Massive spin-2 fields on black hole spacetimes: Instability of the Schwarzschild and Kerr solutions and bounds on the graviton mass

TL;DR: In this paper, it has been shown that the Schwarzschild geometry is linearly unstable for small tensor masses, against a spherically symmetric mode, both against the spherical mode and against long-lived superradiant modes.
Journal ArticleDOI

Black strings, low viscosity fluids, and violation of cosmic censorship.

TL;DR: In this paper, the behavior of 5-dimensional black strings subject to the Gregory-Laflamme instability is described, where at intermediate stages the horizon can be described as a sequence of 3-dimensional spherical black holes joined by black string segments.
Journal ArticleDOI

Numerical methods for finding stationary gravitational solutions

TL;DR: In this paper, the mathematical foundations and a practical guide for the numerical solution of gravitational boundary value problems are explained and several tools and tricks that have been useful throughout the literature are presented.
Journal Article

Publisher's Note: Black Strings, Low Viscosity Fluids, and Violation of Cosmic Censorship

TL;DR: The simulation results imply that the string segments will reach zero radius in finite asymptotic time, whence the classical space-time terminates in a naked singularity, this constitutes a generic violation of cosmic censorship.
References
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Journal ArticleDOI

Viscosity in strongly interacting quantum field theories from black hole physics

TL;DR: It is provided evidence that this value of shear viscosity to volume density of entropy may serve as a lower bound for a wide class of systems, thus suggesting that black hole horizons are dual to the most ideal fluids.
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Quasilocal energy and conserved charges derived from the gravitational action

TL;DR: For spherically symmetric spacetimes, it is shown that the quasilocal energy has the correct Newtonian limit, and includes a negative contribution due to gravitational binding.
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Nonlinear fluid dynamics from gravity

TL;DR: In this article, a derivation of the nonlinear equations of boundary fluid dynamics from gravity from gravity is presented, with specific values for fluid parameters, and an explicit expression for the expansion of this fluid stress tensor including terms up to second order in the derivative expansion.
Journal ArticleDOI

Black strings and p -branes are unstable

TL;DR: P perturbations around black strings and branes can be stabilized if the extra dimensions are compactified to a scale smaller than the minimum wavelength for which instability occurs and thus will not affect large astrophysical black holes in four dimensions.
Journal ArticleDOI

Nonlinear Fluid Dynamics from Gravity

TL;DR: In this paper, a derivation of the nonlinear equations of boundary fluid dynamics from gravity from gravity is presented, with specific values for fluid parameters, and an explicit expression for the expansion of this fluid stress tensor including terms up to second order in the derivative expansion.
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