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      Neutrino structure functions from GeV to EeV energies

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          A bstract

          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 ≲ few GeV 2), inelastic structure functions are however affected by large uncertainties which distort event rate predictions for neutrino energies E ν 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 ν 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 ν, SND@LHC, and the Forward Physics Facility. The NNSF ν determination is made available as fast interpolation LHAPDF grids, and it can be accessed both through an independent driver code and directly interfaced to neutrino event generators such as GENIE.

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          Most cited references76

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          Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector

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          We report on results of an all-sky search for high-energy neutrino events interacting within the IceCube neutrino detector conducted between May 2010 and May 2012. The search follows up on the previous detection of two PeV neutrino events, with improved sensitivity and extended energy coverage down to about 30 TeV. Twenty-six additional events were observed, substantially more than expected from atmospheric backgrounds. Combined, both searches reject a purely atmospheric origin for the 28 events at the 4σ level. These 28 events, which include the highest energy neutrinos ever observed, have flavors, directions, and energies inconsistent with those expected from the atmospheric muon and neutrino backgrounds. These properties are, however, consistent with generic predictions for an additional component of extraterrestrial origin.
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            Dynamical parton distributions revisited

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              LHAPDF6: parton density access in the LHC precision era

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                Author and article information

                Contributors
                (View ORCID Profile)
                Journal
                Journal of High Energy Physics
                J. High Energ. Phys.
                Springer Science and Business Media LLC
                1029-8479
                May 2023
                May 18 2023
                : 2023
                : 5
                Article
                10.1007/JHEP05(2023)149
                5e511233-e7d7-4cbc-ac5f-82434cdeb11a
                © 2023

                https://creativecommons.org/licenses/by/4.0

                https://creativecommons.org/licenses/by/4.0

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