Helicity Evolution at Small x: Summary of Recent Developments

preprint2016arXivOpen access

Abstract

We construct small-xx 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 αs ln⁡2(1/x)α_s \, \ln^2 (1/x) in the polarization-dependent evolution along with the powers of αs ln⁡(1/x)α_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. We construct a numerical solution of the helicity evolution equations in the large-NcN_c limit. Employing the extracted intercept, we are able to predict directly from theory the behavior of the quark helicity PDFs at small xx, which should have important phenomenological consequences. We also give an estimate of how much of the proton's spin may be at small xx and what impact this has on the so-called "spin crisis." Based on JHEP 1601 (2016) 072 (arXiv:1511.06737), arXiv:1610.06197 and arXiv:1610.06188.

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