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Author Gonzalez, H.,A.; Rojas, F. doi  openurl
  Title The structure of IR divergences in celestial gluon amplitudes Type
  Year 2021 Publication Journal Of High Energy Physics Abbreviated Journal (down) J. High Energy Phys.  
  Volume Issue 6 Pages 171  
  Keywords Conformal Field Theory; Scattering Amplitudes; Field Theories in Lower Dimensions  
  Abstract The all-loop resummation of SU(N) gauge theory amplitudes is known to factorize into an IR-divergent (soft and collinear) factor and a finite (hard) piece. The divergent factor is universal, whereas the hard function is a process-dependent quantity.We prove that this factorization persists for the corresponding celestial amplitudes. Moreover, the soft/collinear factor becomes a scalar correlator of the product of renormalized Wilson lines defined in terms of celestial data. Their effect on the hard amplitude is a shift in the scaling dimensions by an infinite amount, proportional to the cusp anomalous dimension. This leads us to conclude that the celestial-IR-safe gluon amplitude corresponds to a expectation value of operators dressed with Wilson line primaries. These results hold for finite N.In the large N limit, we show that the soft/collinear correlator can be described in terms of vertex operators in a Coulomb gas of colored scalar primaries with nearest neighbor interactions. In the particular cases of four and five gluons in planar N = 4 SYM theory, where the hard factor is known to exponentiate, we establish that the Mellin transform converges in the UV thanks to the fact that the cusp anomalous dimension is a positive quantity. In other words, the very existence of the full celestial amplitude is owed to the positivity of the cusp anomalous dimension.  
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  ISSN 1029-8479 ISBN Medium  
  Area Expedition Conference  
  Notes WOS:000671162900001 Approved  
  Call Number UAI @ alexi.delcanto @ Serial 1436  
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