Helicity at Small xx: Oscillations Generated by Bringing Back the Quarks

preprint2020arXivOpen access

Abstract

We construct a numerical solution of the recently-derived large-Nc&NfN_c \& N_f small-xx helicity evolution equations with the aim to establish the small-xx asymptotics of the quark helicity distribution beyond the large-NcN_c limit explored previously in the same framework. (Here NcN_c and NfN_f are the numbers of quark colors and flavors.) While the large-NcN_c helicity evolution involves gluons only, the large-Nc&NfN_c \& N_f evolution includes contributions from quarks as well. We find that adding quarks to the evolution makes quark helicity distribution oscillate as a function of xx. Our numerical results in the large-Nc&NfN_c \& N_f limit lead to the xx-dependence of the flavor-singlet quark helicity distribution which is well-approximated by \begin{align} ΔΣ(x, Q^2)\bigg|_{\mbox{large-}N_c \& N_f} \sim \left( \frac{1}{x} \right)^{α_h^q} \, \cos \left[ ω_q \, \ln \left( \frac{1}{x} \right) + φ_q \right]. \end{align} The power αhqα_h^q exhibits a weak NfN_f-dependence, and, for all NfN_f values considered, remains very close to αhq(Nf=0)=(4/3)αsNc/(2π)α_h^q (N_f=0) = (4/\sqrt{3}) \sqrt{α_s N_c/(2 π)} obtained earlier in the large-NcN_c limit. The novel oscillation frequency ωqω_q and phase shift φqφ_q depend more strongly on the number of flavors NfN_f (with ωq=0ω_q =0 in the pure-glue large-NcN_c limit). The typical period of oscillations for ΔΣΔΣ is rather long, spanning many units of rapidity. We speculate whether the oscillations we find are related to the sign variation with xx seen in the strange quark helicity distribution extracted from the data.

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