Celestial $Lw_{1+\infty}$ charges from a twistor action
Adam Kmec, Lionel Mason, Romain Ruzziconi, Akshay Yelleshpur Srikant

TL;DR
This paper derives celestial $Lw_{1+ abla}$ charges in asymptotically flat spacetimes using twistor space, connecting symmetries to gravitational phase space and null infinity data.
Contribution
It provides a first-principle derivation of celestial symmetry generators from a twistor action, linking geometric and spacetime perspectives.
Findings
Charges expressed as surface integrals over celestial sphere
Connection established between twistor space and spacetime at null infinity
Symmetries shown to preserve asymptotic Bianchi identities
Abstract
The celestial 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 is achieved via an integral formula for the asymptotic Bianchi identities due to Bramson and Tod. Finally, we clarify how transformations are symmetries of gravity from a phase space perspective by showing the invariance of the asymptotic Bianchi identities.
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Taxonomy
TopicsGeophysics and Gravity Measurements · Cosmology and Gravitation Theories · Relativity and Gravitational Theory
