Loading…

Helicity evolution at small x : Flavor singlet and nonsinglet observables

We extend our earlier results for the quark helicity evolution at small x [J. High Energy Phys. 01 (2016) 072] to derive the small-x asymptotics of the flavor singlet and flavor nonsinglet quark helicity TMDs and PDFs and of the g1 structure function. In the flavor singlet case we rederive the evolu...

Full description

Saved in:
Bibliographic Details
Published in:Physical review. D 2017-01, Vol.95 (1), Article 014033
Main Authors: Kovchegov, Yuri V., Pitonyak, Daniel, Sievert, Matthew D.
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:We extend our earlier results for the quark helicity evolution at small x [J. High Energy Phys. 01 (2016) 072] to derive the small-x asymptotics of the flavor singlet and flavor nonsinglet quark helicity TMDs and PDFs and of the g1 structure function. In the flavor singlet case we rederive the evolution equations obtained in our previous paper on the subject [J. High Energy Phys. 01 (2016) 072], performing additional cross-checks of our results. In the flavor nonsinglet case we construct new small-x evolution equations by employing the large-Nc limit. All evolution equations resum double-logarithmic powers of αsln2(1/x) in the polarization-dependent evolution along with the single-logarithmic powers of αsln(1/x) in the unpolarized evolution which includes saturation effects. We solve the linearized flavor nonsinglet equation analytically, obtaining an intercept which agrees with the one calculated earlier by Bartels, Ermolaev and Ryskin [Z. Phys. C 70, 273 (1996)] using the infrared evolution equations. Our numerical solution of the linearized large-Nc evolution equations for the flavor singlet case is presented in the accompanying Letter [Phys. Rev. Lett. 118, 052001 (2017)] and is further discussed here.
ISSN:2470-0010
2470-0029
DOI:10.1103/PhysRevD.95.014033