English

Helicity Evolution at Small-x

High Energy Physics - Phenomenology 2016-07-15 v3 High Energy Physics - Experiment

Abstract

We construct small-x evolution equations which can be used to calculate quark and anti-quark helicity TMDs and PDFs, along with the g1g_1 structure function. These evolution equations resum powers of αsln2(1/x)\alpha_s \, \ln^2 (1/x) in the polarization-dependent evolution along with the powers of αsln(1/x)\alpha_s \, \ln (1/x) in the unpolarized evolution which includes saturation effects. The equations are written in an operator form in terms of polarization-dependent Wilson line-like operators. While the equations do not close in general, they become closed and self-contained systems of non-linear equations in the large-NcN_c and large-Nc&NfN_c \, \& \, N_f limits. As a cross-check, in the ladder approximation, our equations map onto the same ladder limit of the infrared evolution equations for g1g_1 structure function derived previously by Bartels, Ermolaev and Ryskin.

Keywords

Cite

@article{arxiv.1511.06737,
  title  = {Helicity Evolution at Small-x},
  author = {Yuri V. Kovchegov and Daniel Pitonyak and Matthew D. Sievert},
  journal= {arXiv preprint arXiv:1511.06737},
  year   = {2016}
}

Comments

33 pages, 20 figures; v2: typos corrected, a reference added; v3: more corrections included

R2 v1 2026-06-22T11:50:49.190Z