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Amplitude from crossing-symmetric celestial OPE

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arxiv 2503.21512 v1 pith:FA6CFF46 submitted 2025-03-27 hep-th

classification hep-th
keywords celestialamplitudesmethodpurereconstructscatteringamplitudeassuming
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Assuming the existence of crossing symmetric celestial OPE, we propose a method to reconstruct four-point massless scattering amplitudes in the framework of celestial holography. This method relies only on CFT techniques and a remarkable property: scattering amplitudes can be derived from a single conformal block coefficient in celestial CFT. Utilizing this method, we reconstruct the MHV amplitudes in pure Yang-Mills, pure gravity, and Einstein-Yang-Mills theories.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Shadow Celestial Operator Product Expansions

    hep-th 2025-05 conditional novelty 6.0 of 10

    Shadowing a celestial primary multiplies its OPE coefficients by a fixed ratio of Gamma functions, universal across theories and applicable to three-point functions with mixed ordinary and shadow operators.

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