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On Carrollian and celestial correlators in general dimensions

Abstract:
Carrollian holography is a framework for flat space holography, suggesting that gravity in asymptotically flat spacetime in D dimensions is dual to a conformal Carrollian field theory in D – 1 dimensions living at null infinity. In this work, we elaborate on the definition of Carrollian amplitudes for massless scalar fields in general dimensions and provide explicit expressions for the two-, three-, and four-point functions. We show that these amplitudes naturally arise from Lorentzian holographic correlators in AdS/CFT through a correspondence between the flat space limit in the bulk and the Carrollian limit at the boundary. Finally, we use the relation between Carrollian and celestial holography to derive explicit expressions for celestial amplitudes in D dimensions, which are reinterpreted as correlators of the celestial CFT in D − 2 dimensions.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1007/jhep10(2025)187

Authors

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Institution:
University of Oxford
Division:
MPLS
Department:
Mathematical Institute
Role:
Author
ORCID:
0000-0003-1559-3307
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Mathematical Institute
Role:
Author
ORCID:
0000-0002-4359-7586
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Mathematical Institute
Role:
Author
ORCID:
0000-0003-2254-0879


Publisher:
Springer
Journal:
Journal of High Energy Physics More from this journal
Volume:
2025
Issue:
10
Article number:
187
Publication date:
2025-10-22
Acceptance date:
2025-09-27
DOI:
EISSN:
1029-8479
ISSN:
1126-6708


Language:
English
Keywords:
Pubs id:
2310061
Local pid:
pubs:2310061
Source identifiers:
3407410
Deposit date:
2025-10-24
ARK identifier:
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