Asymptotic structure of N = 2 $$ \mathcal{N}=2 $$ supergravity in 3D: extended super-BMS3 and nonlinear energy bounds

Abstract The asymptotically flat structure of N = 2 0 $$ \mathcal{N}=\left(2,0\right) $$ supergravity in three spacetime dimensions is explored. The asymptotic symmetries are found to be spanned by an extension of the super-BMS3 algebra, endowed with two independent affine û(1) currents of electric...

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Main Authors: Oscar Fuentealba, Javier Matulich, Ricardo Troncoso
Format: Article
Language:English
Published: SpringerOpen 2017-09-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP09(2017)030
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spelling doaj-4ae4396a5dca433aa97bf4f57f6778f72020-11-24T21:19:11ZengSpringerOpenJournal of High Energy Physics1029-84792017-09-012017913110.1007/JHEP09(2017)030Asymptotic structure of N = 2 $$ \mathcal{N}=2 $$ supergravity in 3D: extended super-BMS3 and nonlinear energy boundsOscar Fuentealba0Javier Matulich1Ricardo Troncoso2Centro de Estudios Científicos (CECs)Centro de Estudios Científicos (CECs)Centro de Estudios Científicos (CECs)Abstract The asymptotically flat structure of N = 2 0 $$ \mathcal{N}=\left(2,0\right) $$ supergravity in three spacetime dimensions is explored. The asymptotic symmetries are found to be spanned by an extension of the super-BMS3 algebra, endowed with two independent affine û(1) currents of electric and magnetic type. These currents are associated to U(1) fields being even and odd under parity, respectively. Remarkably, although the U(1) fields do not generate a backreaction on the metric, they provide nontrivial Sugawara-like contributions to the BMS3 generators, and hence to the energy and the angular momentum. Consequently, the entropy of flat cosmological spacetimes endowed with U(1) fields acquires a nontrivial dependence on the zero modes of the û(1) charges. If the spin structure is odd, the ground state corresponds to Minkowski spacetime, and although the anticommutator of the canonical supercharges is linear in the energy and in the electric-like û(1) charge, the energy becomes bounded from below by the energy of the ground state shifted by the square of the electric-like û(1) charge. If the spin structure is even, the same bound for the energy generically holds, unless the absolute value of the electric-like charge is less than minus the mass of Minkowski spacetime in vacuum, so that the energy has to be nonnegative. The explicit form of the global and asymptotic Killing spinors is found for a wide class of configurations that fulfills our boundary conditions, and they exist precisely when the corresponding bounds are saturated. It is also shown that the spectra with periodic or antiperiodic boundary conditions for the fermionic fields are related by spectral flow, in a similar way as it occurs for the N = 2 $$ \mathcal{N}=2 $$ super-Virasoro algebra. Indeed, our supersymmetric extension of BMS3 can be recovered from the Inönü-Wigner contraction of the superconformal algebra with N = 2 2 $$ \mathcal{N}=\left(2,2\right) $$ , once the fermionic generators of the right copy are truncated.http://link.springer.com/article/10.1007/JHEP09(2017)030Conformal and W SymmetrySpace-Time SymmetriesGauge-gravity correspondenceSupergravity Models
collection DOAJ
language English
format Article
sources DOAJ
author Oscar Fuentealba
Javier Matulich
Ricardo Troncoso
spellingShingle Oscar Fuentealba
Javier Matulich
Ricardo Troncoso
Asymptotic structure of N = 2 $$ \mathcal{N}=2 $$ supergravity in 3D: extended super-BMS3 and nonlinear energy bounds
Journal of High Energy Physics
Conformal and W Symmetry
Space-Time Symmetries
Gauge-gravity correspondence
Supergravity Models
author_facet Oscar Fuentealba
Javier Matulich
Ricardo Troncoso
author_sort Oscar Fuentealba
title Asymptotic structure of N = 2 $$ \mathcal{N}=2 $$ supergravity in 3D: extended super-BMS3 and nonlinear energy bounds
title_short Asymptotic structure of N = 2 $$ \mathcal{N}=2 $$ supergravity in 3D: extended super-BMS3 and nonlinear energy bounds
title_full Asymptotic structure of N = 2 $$ \mathcal{N}=2 $$ supergravity in 3D: extended super-BMS3 and nonlinear energy bounds
title_fullStr Asymptotic structure of N = 2 $$ \mathcal{N}=2 $$ supergravity in 3D: extended super-BMS3 and nonlinear energy bounds
title_full_unstemmed Asymptotic structure of N = 2 $$ \mathcal{N}=2 $$ supergravity in 3D: extended super-BMS3 and nonlinear energy bounds
title_sort asymptotic structure of n = 2 $$ \mathcal{n}=2 $$ supergravity in 3d: extended super-bms3 and nonlinear energy bounds
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2017-09-01
description Abstract The asymptotically flat structure of N = 2 0 $$ \mathcal{N}=\left(2,0\right) $$ supergravity in three spacetime dimensions is explored. The asymptotic symmetries are found to be spanned by an extension of the super-BMS3 algebra, endowed with two independent affine û(1) currents of electric and magnetic type. These currents are associated to U(1) fields being even and odd under parity, respectively. Remarkably, although the U(1) fields do not generate a backreaction on the metric, they provide nontrivial Sugawara-like contributions to the BMS3 generators, and hence to the energy and the angular momentum. Consequently, the entropy of flat cosmological spacetimes endowed with U(1) fields acquires a nontrivial dependence on the zero modes of the û(1) charges. If the spin structure is odd, the ground state corresponds to Minkowski spacetime, and although the anticommutator of the canonical supercharges is linear in the energy and in the electric-like û(1) charge, the energy becomes bounded from below by the energy of the ground state shifted by the square of the electric-like û(1) charge. If the spin structure is even, the same bound for the energy generically holds, unless the absolute value of the electric-like charge is less than minus the mass of Minkowski spacetime in vacuum, so that the energy has to be nonnegative. The explicit form of the global and asymptotic Killing spinors is found for a wide class of configurations that fulfills our boundary conditions, and they exist precisely when the corresponding bounds are saturated. It is also shown that the spectra with periodic or antiperiodic boundary conditions for the fermionic fields are related by spectral flow, in a similar way as it occurs for the N = 2 $$ \mathcal{N}=2 $$ super-Virasoro algebra. Indeed, our supersymmetric extension of BMS3 can be recovered from the Inönü-Wigner contraction of the superconformal algebra with N = 2 2 $$ \mathcal{N}=\left(2,2\right) $$ , once the fermionic generators of the right copy are truncated.
topic Conformal and W Symmetry
Space-Time Symmetries
Gauge-gravity correspondence
Supergravity Models
url http://link.springer.com/article/10.1007/JHEP09(2017)030
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