Fig. 13From: Numerical solution of DGLAP equations using Laguerre polynomials expansion and Monte Carlo methodSea s quark densities in NLO approximation at energy scales Q 2 = 4, 50, 200 GeV2. Comparison with CETQ4M and GRSV98NLO parameterization groups and the results from Ref. Coriano and Savkli (1999) has also been doneBack to article page