Celestial Lw 1+∞ charges from a twistor action

The celestial Lw1+∞ symmetries in asymptotically flat spacetimes have a natural geometric interpretation on twistor space in terms of Poisson diffeomorphisms. Using this framework, we provide a first-principle derivation of the canonical generators associated with these symmetries starting from the...

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Main Authors: Kmec, A, Mason, L, Ruzziconi, R, Srikant, AY
Format: Journal article
Language:English
Published: Springer 2024
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author Kmec, A
Mason, L
Ruzziconi, R
Srikant, AY
author_facet Kmec, A
Mason, L
Ruzziconi, R
Srikant, AY
author_sort Kmec, A
collection OXFORD
description The celestial Lw1+∞ symmetries in asymptotically flat spacetimes have a natural geometric interpretation on twistor space in terms of Poisson diffeomorphisms. Using this framework, we provide a first-principle derivation of the canonical generators associated with these symmetries starting from the Poisson BF twistor action for self-dual gravity. We express these charges as surface integrals over the celestial sphere in terms of spacetime data at null infinity. The connection between twistor space and spacetime expressions at I is achieved via an integral formula for the asymptotic Bianchi identities due to Bramson and Tod. Finally, we clarify how Lw1+∞ transformations are symmetries of gravity from a phase space perspective by showing the invariance of the asymptotic Bianchi identities.
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spelling oxford-uuid:9e1cb99e-6a9d-416f-aeb7-c3c1e49dedd22024-11-05T20:07:23ZCelestial Lw 1+∞ charges from a twistor actionJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:9e1cb99e-6a9d-416f-aeb7-c3c1e49dedd2EnglishJisc Publications RouterSpringer2024Kmec, AMason, LRuzziconi, RSrikant, AYThe celestial Lw1+∞ symmetries in asymptotically flat spacetimes have a natural geometric interpretation on twistor space in terms of Poisson diffeomorphisms. Using this framework, we provide a first-principle derivation of the canonical generators associated with these symmetries starting from the Poisson BF twistor action for self-dual gravity. We express these charges as surface integrals over the celestial sphere in terms of spacetime data at null infinity. The connection between twistor space and spacetime expressions at I is achieved via an integral formula for the asymptotic Bianchi identities due to Bramson and Tod. Finally, we clarify how Lw1+∞ transformations are symmetries of gravity from a phase space perspective by showing the invariance of the asymptotic Bianchi identities.
spellingShingle Kmec, A
Mason, L
Ruzziconi, R
Srikant, AY
Celestial Lw 1+∞ charges from a twistor action
title Celestial Lw 1+∞ charges from a twistor action
title_full Celestial Lw 1+∞ charges from a twistor action
title_fullStr Celestial Lw 1+∞ charges from a twistor action
title_full_unstemmed Celestial Lw 1+∞ charges from a twistor action
title_short Celestial Lw 1+∞ charges from a twistor action
title_sort celestial lw 1 ∞ charges from a twistor action
work_keys_str_mv AT kmeca celestiallw1chargesfromatwistoraction
AT masonl celestiallw1chargesfromatwistoraction
AT ruzziconir celestiallw1chargesfromatwistoraction
AT srikantay celestiallw1chargesfromatwistoraction