Celestial Geometry
arXiv:2204.02505 · doi:10.1007/JHEP09(2022)045
Abstract
Celestial holography expresses -matrix elements as correlators in a CFT living on the night sky. Poincaré invariance imposes additional selection rules on the allowed positions of operators. As a consequence, -point correlators are only supported on certain patches of the celestial sphere, depending on the labeling of each operator as incoming/outgoing. Here we initiate a study of the celestial geometry, examining the kinematic support of celestial amplitudes for different crossing channels. We give simple geometric rules for determining this support. For , we can view these channels as tiling together to form a covering of the celestial sphere. Our analysis serves as a stepping off point to better understand the analyticity of celestial correlators and illuminate the connection between the 4D kinematic and 2D CFT notions of crossing symmetry.
27 pages, 6 figures
References in corpus (4)
Cited by in corpus (8)
- Bridging Carrollian and Celestial Holography
- Notes on Resonances and Unitarity from Celestial Amplitudes
- Celestial Supersymmetry
- Celestial amplitudes in an ambidextrous basis
- Celestial Recursion
- Soft and Collinear Limits in Supergravity using Double Copy Formalism
- A Celestial Route to AdS Bulk Locality
- Celestial Eikonal Amplitudes in the Near-Horizon Region