• Open Access

Carrollian Perspective on Celestial Holography

Laura Donnay, Adrien Fiorucci, Yannick Herfray, and Romain Ruzziconi
Phys. Rev. Lett. 129, 071602 – Published 12 August 2022

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. The Ward 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.

  • Figure
  • Received 4 March 2022
  • Accepted 7 July 2022

DOI:https://doi.org/10.1103/PhysRevLett.129.071602

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & FieldsGravitation, Cosmology & Astrophysics

Authors & Affiliations

Laura Donnay1,*, Adrien Fiorucci1,†, Yannick Herfray2,‡, and Romain Ruzziconi1,§

  • 1Institute for Theoretical Physics, TU Wien Wiedner Hauptstrasse 8-10/136, A-1040 Vienna, Austria
  • 2Service de Physique de l’Univers, Champs et Gravitation, Université de Mons, 20 place du Parc, 7000 Mons, Belgium

  • *Corresponding author. laura.donnay@tuwien.ac.at
  • Corresponding author. adrien.fiorucci@tuwien.ac.at
  • Corresponding author. yannick.herfray@umons.ac.be
  • §Corresponding author. romain.ruzziconi@tuwien.ac.at

Article Text

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Issue

Vol. 129, Iss. 7 — 12 August 2022

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