A gauge-invariant symplectic potential for tetrad general relativity

Abstract We identify a symplectic potential for general relativity in tetrad and connection variables that is fully gauge-invariant, using the freedom to add surface terms. When torsion vanishes, it does not lead to surface charges associated with the internal Lorentz transformations, and reduces ex...

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Main Authors: Elena De Paoli, Simone Speziale
Format: Article
Language:English
Published: SpringerOpen 2018-07-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP07(2018)040
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spelling doaj-1cbf53cbbd0f47bf8dfbbdb92396e09c2020-11-25T02:09:25ZengSpringerOpenJournal of High Energy Physics1029-84792018-07-012018712210.1007/JHEP07(2018)040A gauge-invariant symplectic potential for tetrad general relativityElena De Paoli0Simone Speziale1Aix Marseille Université, Université de Toulon, CNRS, CPT, UMR 7332Aix Marseille Université, Université de Toulon, CNRS, CPT, UMR 7332Abstract We identify a symplectic potential for general relativity in tetrad and connection variables that is fully gauge-invariant, using the freedom to add surface terms. When torsion vanishes, it does not lead to surface charges associated with the internal Lorentz transformations, and reduces exactly to the symplectic potential given by the Einstein-Hilbert action. In particular, it reproduces the Komar form when the variation is a Li derivative, and the geometric expression in terms of extrinsic curvature and 2d corner data for a general variation. The additional surface term vanishes at spatial infinity for asymptotically flat spacetimes, thus the usual Poincaré charges are obtained. We prove that the first law of black hole mechanics follows from the Noether identity associated with the covariant Lie derivative, and that it is independent of the ambiguities in the symplectic potential provided one takes into account the presence of non-trivial Lorentz charges that these ambiguities can introduce.http://link.springer.com/article/10.1007/JHEP07(2018)040Black HolesClassical Theories of GravityGauge SymmetrySpace-Time Symmetries
collection DOAJ
language English
format Article
sources DOAJ
author Elena De Paoli
Simone Speziale
spellingShingle Elena De Paoli
Simone Speziale
A gauge-invariant symplectic potential for tetrad general relativity
Journal of High Energy Physics
Black Holes
Classical Theories of Gravity
Gauge Symmetry
Space-Time Symmetries
author_facet Elena De Paoli
Simone Speziale
author_sort Elena De Paoli
title A gauge-invariant symplectic potential for tetrad general relativity
title_short A gauge-invariant symplectic potential for tetrad general relativity
title_full A gauge-invariant symplectic potential for tetrad general relativity
title_fullStr A gauge-invariant symplectic potential for tetrad general relativity
title_full_unstemmed A gauge-invariant symplectic potential for tetrad general relativity
title_sort gauge-invariant symplectic potential for tetrad general relativity
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2018-07-01
description Abstract We identify a symplectic potential for general relativity in tetrad and connection variables that is fully gauge-invariant, using the freedom to add surface terms. When torsion vanishes, it does not lead to surface charges associated with the internal Lorentz transformations, and reduces exactly to the symplectic potential given by the Einstein-Hilbert action. In particular, it reproduces the Komar form when the variation is a Li derivative, and the geometric expression in terms of extrinsic curvature and 2d corner data for a general variation. The additional surface term vanishes at spatial infinity for asymptotically flat spacetimes, thus the usual Poincaré charges are obtained. We prove that the first law of black hole mechanics follows from the Noether identity associated with the covariant Lie derivative, and that it is independent of the ambiguities in the symplectic potential provided one takes into account the presence of non-trivial Lorentz charges that these ambiguities can introduce.
topic Black Holes
Classical Theories of Gravity
Gauge Symmetry
Space-Time Symmetries
url http://link.springer.com/article/10.1007/JHEP07(2018)040
work_keys_str_mv AT elenadepaoli agaugeinvariantsymplecticpotentialfortetradgeneralrelativity
AT simonespeziale agaugeinvariantsymplecticpotentialfortetradgeneralrelativity
AT elenadepaoli gaugeinvariantsymplecticpotentialfortetradgeneralrelativity
AT simonespeziale gaugeinvariantsymplecticpotentialfortetradgeneralrelativity
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