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MHV Gluon Scattering Amplitudes from Celestial Current Algebras

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arxiv 2011.00017 v3 pith:QGB5M3HJ submitted 2020-10-30 hep-th

classification hep-th
keywords equationscurrentgluonalgebraamplitudecelestialscatteringsubleading
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We show that the Mellin transform of an $n$-point tree level MHV gluon scattering amplitude, also known as the celestial amplitude in pure Yang-Mills theory, satisfies a system of $(n-2)$ linear first order partial differential equations corresponding to $(n-2)$ positive helicity gluons. Although these equations closely resemble Knizhnik-Zamolodchikov equations for $SU(N)$ current algebra there is also an additional "correction" term coming from the subleading soft gluon current algebra. These equations can be used to compute the leading term in the gluon-gluon OPE on the celestial sphere. Similar equations can also be written down for the momentum space tree level MHV scattering amplitudes. We also propose a way to deal with the non closure of subleading current algebra generators under commutation. This is then used to compute some subleading terms in the mixed helicity gluon OPE and our results match with those obtained from an explicit calculation using the Mellin MHV amplitude.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 410 citations worldwide. Full citation record

  1. Holographic symmetry algebra for the MHV sector revisited

    hep-th 2025-08 conditional novelty 6.0 of 10

    In the MHV sector, the celestial symmetry algebra is a semidirect product of w_{1+∞} (or S) with an infinite Abelian algebra, whose null states supply the two missing KZ equations.

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