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Title: A rough end for smooth microstate geometries

Abstract

Supersymmetric microstate geometries with five non-compact dimensions have recently been shown by Eperon, Reall, and Santos (ERS) to exhibit a non-linear instability featuring the growth of excitations at an “evanescent ergosurface” of infinite redshift. We argue that this growth may be treated as adiabatic evolution along a family of exactly supersymmetric solutions in the limit where the excitations are Aichelburg-Sexl-like shockwaves. In the 2-charge system such solutions may be constructed explicitly, incorpo-rating full backreaction, and are in fact special cases of known microstate geometries. In a near-horizon limit, they reduce to Aichelburg-Sexl shockwaves in AdS 3 × S 3 propagating along one of the angular directions of the sphere. Noting that the ERS analysis is valid in the limit of large microstate angular momentum j, we use the above identification to interpret their instability as a transition from rare smooth microstates with large angular momentum to more typical microstates with smaller angular momentum. This entropic driving terminates when the angular momentum decreases to j~√n 1n 5 where the density of microstates is maximal. Finally, we argue that, at this point, the large stringy corrections to such microstates will render them non-linearly stable. We identify a possible mechanism for this stabilizationmore » and detail an illustrative toy model.« less

Authors:
 [1];  [1];  [2]
  1. Univ. of California, Santa Barbara, CA (United States). Dept. of Physics
  2. Harvard Univ., Cambridge, MA (United States). Jefferson Physical Lab., Black Hole Initiative (BHI)
Publication Date:
Research Org.:
Harvard Univ., Cambridge, MA (United States)
Sponsoring Org.:
USDOE Office of Science (SC); National Science Foundation (NSF); John Templeton Foundation
OSTI Identifier:
1368216
Grant/Contract Number:
SC0007870; PHY15-04541; PHY13-16748
Resource Type:
Journal Article: Accepted Manuscript
Journal Name:
Journal of High Energy Physics (Online)
Additional Journal Information:
Journal Name: Journal of High Energy Physics (Online); Journal Volume: 2017; Journal Issue: 5; Journal ID: ISSN 1029-8479
Publisher:
Springer Berlin
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; AdS-CFT Correspondence; Black Holes; Black Holes in String Theory; String Duality

Citation Formats

Marolf, Donald, Michel, Ben, and Puhm, Andrea. A rough end for smooth microstate geometries. United States: N. p., 2017. Web. doi:10.1007/JHEP05(2017)021.
Marolf, Donald, Michel, Ben, & Puhm, Andrea. A rough end for smooth microstate geometries. United States. doi:10.1007/JHEP05(2017)021.
Marolf, Donald, Michel, Ben, and Puhm, Andrea. Wed . "A rough end for smooth microstate geometries". United States. doi:10.1007/JHEP05(2017)021. https://www.osti.gov/servlets/purl/1368216.
@article{osti_1368216,
title = {A rough end for smooth microstate geometries},
author = {Marolf, Donald and Michel, Ben and Puhm, Andrea},
abstractNote = {Supersymmetric microstate geometries with five non-compact dimensions have recently been shown by Eperon, Reall, and Santos (ERS) to exhibit a non-linear instability featuring the growth of excitations at an “evanescent ergosurface” of infinite redshift. We argue that this growth may be treated as adiabatic evolution along a family of exactly supersymmetric solutions in the limit where the excitations are Aichelburg-Sexl-like shockwaves. In the 2-charge system such solutions may be constructed explicitly, incorpo-rating full backreaction, and are in fact special cases of known microstate geometries. In a near-horizon limit, they reduce to Aichelburg-Sexl shockwaves in AdS3 × S3 propagating along one of the angular directions of the sphere. Noting that the ERS analysis is valid in the limit of large microstate angular momentum j, we use the above identification to interpret their instability as a transition from rare smooth microstates with large angular momentum to more typical microstates with smaller angular momentum. This entropic driving terminates when the angular momentum decreases to j~√n1n5 where the density of microstates is maximal. Finally, we argue that, at this point, the large stringy corrections to such microstates will render them non-linearly stable. We identify a possible mechanism for this stabilization and detail an illustrative toy model.},
doi = {10.1007/JHEP05(2017)021},
journal = {Journal of High Energy Physics (Online)},
number = 5,
volume = 2017,
place = {United States},
year = {Wed May 03 00:00:00 EDT 2017},
month = {Wed May 03 00:00:00 EDT 2017}
}

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