We show that a 3D sourced conformal Carrollian field theory has the right kinematic properties to holographically describe gravity in 4D asymptotically flat spacetime. The external sources encode the leaks of gravitational radiation at null infinity. TheWard identities of this theory are shown to reproduce those of the 2D celestial CFT after relating Carrollian to celestial operators. This suggests a new set of interplays between gravity in asymptotically flat spacetime, sourced conformal Carrollian field theory and celestial CFT.

Carrollian Perspective on Celestial Holography / Donnay, Laura; Fiorucci, Adrien; Herfray, Yannick; Ruzziconi, Romain. - In: PHYSICAL REVIEW LETTERS. - ISSN 0031-9007. - 129:7(2022). [10.1103/PhysRevLett.129.071602]

Carrollian Perspective on Celestial Holography

Donnay, Laura
;
Ruzziconi, Romain
2022-01-01

Abstract

We show that a 3D sourced conformal Carrollian field theory has the right kinematic properties to holographically describe gravity in 4D asymptotically flat spacetime. The external sources encode the leaks of gravitational radiation at null infinity. TheWard identities of this theory are shown to reproduce those of the 2D celestial CFT after relating Carrollian to celestial operators. This suggests a new set of interplays between gravity in asymptotically flat spacetime, sourced conformal Carrollian field theory and celestial CFT.
2022
129
7
071602
10.1103/PhysRevLett.129.071602
https://arxiv.org/abs/2202.04702
Donnay, Laura; Fiorucci, Adrien; Herfray, Yannick; Ruzziconi, Romain
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11767/131606
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