Celestial Liouville Theory for Yang-Mills Amplitudes
arXiv:2209.02724 · doi:10.1016/j.physletb.2022.137588
Abstract
We consider Yang-Mills theory with the coupling constant and theta angle determined by the vacuum expectation values of a dynamical (complex) dilaton field. We discuss the tree-level N-gluon MHV scattering amplitudes in the presence of a nontrivial background dilaton field and construct the corresponding celestial amplitudes by taking Mellin transforms with respect to the lightcone energies. In this way, we obtain two-dimensional CFT correlators of primary fields on the celestial sphere. We show that the celestial Yang-Mills amplitudes evaluated in the presence of a spherical dilaton shockwave are given by the correlation functions of primary field operators factorized into the holomorphic current operators times the "light" Liouville operators. They are evaluated in the semiclassical limit of Liouville theory (the limit of infinite central charge) and are determined by the classical Liouville field describing metrics on the celestial sphere.
arXiv comment12 pages
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- Lorentz Symmetry and IR Structure of The BFSS Matrix Model
- Integrable Field Theories and Their CCFT Duals
- Celestial self-dual Yang-Mills theory: a new formula and the OPE limit
- Spectral representation in Klein space: simplifying celestial leaf amplitudes
- Celestial Gluon Amplitudes from the Outside In
- Entanglement Rényi entropies in celestial holography