Jalilian-Marian, Iancu, McLerran, Weigert, Leonidov, Kovner evolution at next to leading order

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One may expect that the NLO corrections to physical observables in the saturation regime will be large, just as they are in the linear BFKL regime and that further resummations may be necessary. See for example review as well as A. Rezaeian, Phys.Lett. B718 (2013); A. Stasto, B-W Xiao and D. Zaslavsky; e-Print: arXiv:1307.4057; E. Avsar, A. M. Stasto, D. N. Triantafyllopoulos and D. Zaslavsky, JHEP 1110

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