Hidden symmetry of the static response of black holes: applications to Love numbers

Abstract We show that any static linear perturbations around Schwarzschild black holes enjoy a set of conserved charges which forms a centrally extended Schrödinger algebra sh $$ \mathfrak{sh} $$ (1) = sl $$ \mathfrak{sl} $$ (2, ℝ) ⋉ H $$ \mathcal{H} $$ . The central charge is given by the black hol...

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Main Authors: Jibril Ben Achour, Etera R. Livine, Shinji Mukohyama, Jean-Philippe Uzan
Format: Article
Language:English
Published: SpringerOpen 2022-07-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP07(2022)112
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author Jibril Ben Achour
Etera R. Livine
Shinji Mukohyama
Jean-Philippe Uzan
author_facet Jibril Ben Achour
Etera R. Livine
Shinji Mukohyama
Jean-Philippe Uzan
author_sort Jibril Ben Achour
collection DOAJ
description Abstract We show that any static linear perturbations around Schwarzschild black holes enjoy a set of conserved charges which forms a centrally extended Schrödinger algebra sh $$ \mathfrak{sh} $$ (1) = sl $$ \mathfrak{sl} $$ (2, ℝ) ⋉ H $$ \mathcal{H} $$ . The central charge is given by the black hole mass, echoing results on black hole entropy from near-horizon diffeomorphism symmetry. The finite symmetry transformations generated by these conserved charges correspond to Galilean and conformal transformations of the static field and of the coordinates. This new structure allows one to discuss the static response of a Schwarzschild black hole in the test field approximation from a symmetry-based approach. First we show that the (horizontal) symmetry protecting the vanishing of the Love numbers recently exhibited by Hui et al., dubbed the HJPSS symmetry, coincides with one of the sl $$ \mathfrak{sl} $$ (2, ℝ) generators of the Schrödinger group. Then, it is demonstrated that the HJPSS symmetry is selected thanks to the spontaneous breaking of the full Schrödinger symmetry at the horizon down to a simple abelian sub-group. The latter can be understood as the symmetry protecting the regularity of the test field at the horizon. In the 4-dimensional case, this provides a symmetry protection for the vanishing of the Schwarzschild Love numbers. Our results trivially extend to the Kerr case.
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spelling doaj.art-e6346cd68fe14ebaaf1145a8c3dd80ff2022-12-22T01:30:28ZengSpringerOpenJournal of High Energy Physics1029-84792022-07-012022713110.1007/JHEP07(2022)112Hidden symmetry of the static response of black holes: applications to Love numbersJibril Ben Achour0Etera R. Livine1Shinji Mukohyama2Jean-Philippe Uzan3Arnold Sommerfeld Center for Theoretical PhysicsEcole Normale Supérieure de LyonCenter for Gravitational Physics, Yukawa Institute for Theoretical PhysicsInstitut d’Astrophysique de Paris, CNRS UMR 7095, Sorbonne UniversitésAbstract We show that any static linear perturbations around Schwarzschild black holes enjoy a set of conserved charges which forms a centrally extended Schrödinger algebra sh $$ \mathfrak{sh} $$ (1) = sl $$ \mathfrak{sl} $$ (2, ℝ) ⋉ H $$ \mathcal{H} $$ . The central charge is given by the black hole mass, echoing results on black hole entropy from near-horizon diffeomorphism symmetry. The finite symmetry transformations generated by these conserved charges correspond to Galilean and conformal transformations of the static field and of the coordinates. This new structure allows one to discuss the static response of a Schwarzschild black hole in the test field approximation from a symmetry-based approach. First we show that the (horizontal) symmetry protecting the vanishing of the Love numbers recently exhibited by Hui et al., dubbed the HJPSS symmetry, coincides with one of the sl $$ \mathfrak{sl} $$ (2, ℝ) generators of the Schrödinger group. Then, it is demonstrated that the HJPSS symmetry is selected thanks to the spontaneous breaking of the full Schrödinger symmetry at the horizon down to a simple abelian sub-group. The latter can be understood as the symmetry protecting the regularity of the test field at the horizon. In the 4-dimensional case, this provides a symmetry protection for the vanishing of the Schwarzschild Love numbers. Our results trivially extend to the Kerr case.https://doi.org/10.1007/JHEP07(2022)112Global SymmetriesBlack HolesClassical Theories of Gravity
spellingShingle Jibril Ben Achour
Etera R. Livine
Shinji Mukohyama
Jean-Philippe Uzan
Hidden symmetry of the static response of black holes: applications to Love numbers
Journal of High Energy Physics
Global Symmetries
Black Holes
Classical Theories of Gravity
title Hidden symmetry of the static response of black holes: applications to Love numbers
title_full Hidden symmetry of the static response of black holes: applications to Love numbers
title_fullStr Hidden symmetry of the static response of black holes: applications to Love numbers
title_full_unstemmed Hidden symmetry of the static response of black holes: applications to Love numbers
title_short Hidden symmetry of the static response of black holes: applications to Love numbers
title_sort hidden symmetry of the static response of black holes applications to love numbers
topic Global Symmetries
Black Holes
Classical Theories of Gravity
url https://doi.org/10.1007/JHEP07(2022)112
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