Fronsdal fields from gauge functions in Vasiliev’s higher spin gravity

Abstract In this paper, we revisit a number of issues in Vasiliev’s theory related to gauge functions, ordering schemes, and the embedding of Fronsdal fields into master fields. First, we parametrize a broad equivalence class of linearized solutions using gauge functions and integration constants, a...

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Main Authors: David De Filippi, Carlo Iazeolla, Per Sundell
Format: Article
Language:English
Published: SpringerOpen 2019-10-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP10(2019)215
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spelling doaj-f6fa799b428e49a092000841de882bc72020-11-25T03:59:13ZengSpringerOpenJournal of High Energy Physics1029-84792019-10-0120191018410.1007/JHEP10(2019)215Fronsdal fields from gauge functions in Vasiliev’s higher spin gravityDavid De Filippi0Carlo Iazeolla1Per Sundell2Service de Physique de l’Univers, Champs et Gravitation, UMONSNSR Physics Department, G. Marconi UniversityDepartamento de Ciencias Físicas, Universidad Andrés BelloAbstract In this paper, we revisit a number of issues in Vasiliev’s theory related to gauge functions, ordering schemes, and the embedding of Fronsdal fields into master fields. First, we parametrize a broad equivalence class of linearized solutions using gauge functions and integration constants, and show explicitly how Fronsdal fields and their Weyl tensors arise from these data in accordance with Vasiliev’s central on mass shell theorem. We then gauge transform the linearized piece of exact solutions, obtained in a convenient gauge in Weyl order, to the aforementioned class, where we land in normal order. We spell out this map for massless particle and higher spin black hole modes. Our results show that Vasiliev’s equations admit the correct free-field limit for master field configurations that relax the original regularity and gauge conditions in twistor space. Moreover, they support the off-shell Frobenius-Chern-Simons formulation of higher spin gravity for which Weyl order plays a crucial role. Finally, we propose a Fefferman-Graham-like scheme for computing asymptotically anti-de Sitter master field configurations, based on the assumption that gauge function and integration constant can be adjusted perturbatively so that the full master fields approach free master fields asymptotically.http://link.springer.com/article/10.1007/JHEP10(2019)215Higher Spin GravityHigher Spin SymmetryBlack HolesWilson’t Hooft and Polyakov loops
collection DOAJ
language English
format Article
sources DOAJ
author David De Filippi
Carlo Iazeolla
Per Sundell
spellingShingle David De Filippi
Carlo Iazeolla
Per Sundell
Fronsdal fields from gauge functions in Vasiliev’s higher spin gravity
Journal of High Energy Physics
Higher Spin Gravity
Higher Spin Symmetry
Black Holes
Wilson
’t Hooft and Polyakov loops
author_facet David De Filippi
Carlo Iazeolla
Per Sundell
author_sort David De Filippi
title Fronsdal fields from gauge functions in Vasiliev’s higher spin gravity
title_short Fronsdal fields from gauge functions in Vasiliev’s higher spin gravity
title_full Fronsdal fields from gauge functions in Vasiliev’s higher spin gravity
title_fullStr Fronsdal fields from gauge functions in Vasiliev’s higher spin gravity
title_full_unstemmed Fronsdal fields from gauge functions in Vasiliev’s higher spin gravity
title_sort fronsdal fields from gauge functions in vasiliev’s higher spin gravity
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2019-10-01
description Abstract In this paper, we revisit a number of issues in Vasiliev’s theory related to gauge functions, ordering schemes, and the embedding of Fronsdal fields into master fields. First, we parametrize a broad equivalence class of linearized solutions using gauge functions and integration constants, and show explicitly how Fronsdal fields and their Weyl tensors arise from these data in accordance with Vasiliev’s central on mass shell theorem. We then gauge transform the linearized piece of exact solutions, obtained in a convenient gauge in Weyl order, to the aforementioned class, where we land in normal order. We spell out this map for massless particle and higher spin black hole modes. Our results show that Vasiliev’s equations admit the correct free-field limit for master field configurations that relax the original regularity and gauge conditions in twistor space. Moreover, they support the off-shell Frobenius-Chern-Simons formulation of higher spin gravity for which Weyl order plays a crucial role. Finally, we propose a Fefferman-Graham-like scheme for computing asymptotically anti-de Sitter master field configurations, based on the assumption that gauge function and integration constant can be adjusted perturbatively so that the full master fields approach free master fields asymptotically.
topic Higher Spin Gravity
Higher Spin Symmetry
Black Holes
Wilson
’t Hooft and Polyakov loops
url http://link.springer.com/article/10.1007/JHEP10(2019)215
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