6533b833fe1ef96bd129b89c
RESEARCH PRODUCT
Neutrino Structure Functions from GeV to EeV Energies
Alessandro CandidoAlfonso GarciaGiacomo MagniTanjona RabemananjaraJuan RojoRoy Stegemansubject
High Energy Astrophysical Phenomena (astro-ph.HE)Nuclear and High Energy Physics/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyNuclear TheoryParton DistributionsFOS: Physical sciencesDeep Inelastic Scattering or Small-x PhysicsHigh Energy Physics - ExperimentNuclear Theory (nucl-th)High Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Neutrino InteractionsSDG 7 - Affordable and Clean EnergyNuclear Experiment (nucl-ex)Astrophysics - High Energy Astrophysical PhenomenaNuclear Experimentdescription
The interpretation of present and future neutrino experiments requires accurate theoretical predictions for neutrino-nucleus scattering rates. Neutrino structure functions can be reliably evaluated in the deep-inelastic scattering regime within the perturbative QCD (pQCD) framework. At low momentum transfers ($Q^2 \le {\rm few}$ GeV$^2$), inelastic structure functions are however affected by large uncertainties which distort event rate predictions for neutrino energies $E_\nu$ up to the TeV scale. Here we present a determination of neutrino inelastic structure functions valid for the complete range of energies relevant for phenomenology, from the GeV region entering oscillation analyses to the multi-EeV region accessible at neutrino telescopes. Our NNSF$\nu$ approach combines a machine-learning parametrisation of experimental data with pQCD calculations based on state-of-the-art analyses of proton and nuclear parton distributions (PDFs). We compare our determination to other calculations, in particular to the popular Bodek-Yang model. We provide updated predictions for inclusive cross sections for a range of energies and target nuclei, including those relevant for LHC far-forward neutrino experiments such as FASER$\nu$, SND@LHC, and the Forward Physics Facility. The NNSF$\nu$ determination is made available as fast interpolation LHAPDF grids, and can be accessed both through an independent driver code and directly interfaced to neutrino event generators such as GENIE.
year | journal | country | edition | language |
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2023-05-01 |