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Numerical evaluation of the nonlinear Gribov-Levin-Ryskin-Mueller-Qiu evolution equations for nuclear parton distribution functions

J. Rausch, V. Guzey, and M. Klasen
Phys. Rev. D 107, 054003 – Published 2 March 2023

Abstract

We numerically study for the first time the nonlinear GLR-MQ evolution equations for nuclear parton distribution function (nPDFs) to next-to-leading order accuracy and quantify the impact of gluon recombination at small x. Using the nCTEQ15 nPDFs as input, we confirm the importance of the nonlinear corrections for small x103, whose magnitude increases with a decrease of x and an increase of the atomic number A. We find that at x=105 and for heavy nuclei, after the upward evolution from Q0=2GeV to Q=10GeV, the quark singlet Ω(x,Q2) and the gluon G(x,Q2) distributions become reduced by 9%–15%, respectively. The relative effect is much stronger for the downward evolution from Q0=10GeV to Q=2GeV, where we find that Ω(x,Q2) is suppressed by 40%, while G(x,Q2) is enhanced by 140%. These trends propagate into the F2A(x,Q2) nuclear structure function and the FLA(x,Q2) longitudinal structure function, which after the downward evolution become reduced by 45% and enhanced by 80%, respectively. Our analysis indicates that the nonlinear effects are most pronounced in FLA(x,Q2) and are already quite sizable at x103 for heavy nuclei. We have checked that our conclusions very weakly depend on the choice of input nPDFs. In particular, using the EPPS21 nPDFs as input, we obtain quantitatively similar results.

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  • Received 5 December 2022
  • Accepted 20 February 2023

DOI:https://doi.org/10.1103/PhysRevD.107.054003

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

J. Rausch1,2, V. Guzey3,4, and M. Klasen2,5

  • 1Humboldt University Berlin, Department of Physics, Newtonstraße 15, 12489 Berlin, Germany
  • 2Institut für Theoretische Physik, Westfälische Wilhelms-Universität Münster, Wilhelm-Klemm-Straße 9, 48149 Münster, Germany
  • 3University of Jyvaskyla, Department of Physics, P.O. Box 35, FI-40014 Jyvaskyla, Finland
  • 4University of Helsinki, Helsinki Institute of Physics, P.O. Box 64, FI-00014 Helsinki, Finland
  • 5School of Physics, The University of New South Wales, Sydney, New South Wales 2052, Australia

Article Text

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Issue

Vol. 107, Iss. 5 — 1 March 2023

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