Improved constraints on parton distributions using LHCb, ALICE and HERA heavy-flavour measurements and implications for the predictions for prompt atmospheric-neutrino fluxes
O. Zenaiev, M. V. Garzelli, K. Lipka, S. -O. Moch, A. Cooper-Sarkar, F. Olness, A. Geiser, G. Sigl
TL;DR
This work updates the PROSA PDF analysis by incorporating LHCb and ALICE heavy-flavour measurements together with HERA DIS data to constrain the gluon and sea-quark distributions at very low x. Using NLO QCD in both FFNS and VFNS within xFitter, the study achieves improved low-x gluon constraints (down to x ~ 10^-6) and provides refined predictions for the prompt atmospheric-neutrino flux, with results that align with IceCube limits and other PDF-based predictions. The analysis also assesses systematic and model uncertainties, tests multiple gluon parametrisations, and delivers publicly available PROSA 2019 PDFs for applications in high-energy and astroparticle physics. Overall, the paper demonstrates that forward heavy-flavour data from the LHC substantially enhance our understanding of proton structure at ultra-low x and improve astrophysical flux predictions.
Abstract
The impact of measurements of heavy-flavour production in deep inelastic $ep$ scattering and in $pp$ collisions on parton distribution functions is studied in a QCD analysis at next-to-leading order. Recent combined results of inclusive and heavy-flavour production cross sections in deep inelastic scattering at HERA are investigated together with heavy-flavour production measurements at the LHC. Differential cross sections of charm- and beauty-hadron production measured by the LHCb collaboration at the centre-of-mass energies of 5, 7 and 13 TeV as well as the recent measurements of the ALICE experiment at the centre-of-mass energies of 5 and 7 TeV are explored. These data impose additional constraints on the gluon and the sea-quark distributions at low partonic fractions $x$ of the proton momentum, down to $x\approx10^{-6}$. The impact of the resulting parton distribution function in the predictions for the prompt atmospheric-neutrino fluxes is studied.
