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The hadronic interaction model Sibyll-2.3c and inclusive lepton fluxes

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arxiv 1806.04140 v2 pith:HA4CGENQ submitted 2018-06-11 hep-ph astro-ph.HE

Anatoli Fedynitch , Felix Riehn , Ralph Engel , Thomas K. Gaisser , Todor Stanev This is my paper
classification hep-phastro-ph.HE
keywords fluxessibyll-2hadronicinclusiveinteractionsleptonsacceleratoraims
verification ladder T0 review T1 audit T2 compute T3 formal
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Muons and neutrinos from cosmic ray interactions in the atmosphere originate from decays of mesons in air-showers. Sibyll-2.3c aims to give a precise description of hadronic interactions in the relevant phase space for conventional and prompt leptons in light of new accelerator data, including that from the LHC. Sibyll is designed primarily as an event generator for use in simulation of extensive air showers. Because it has been tuned for forward physics as well as the central region, it can also be used to calculate inclusive fluxes. The purpose of this paper is to describe the use of Sibyll-2.3c for calculation of fluxes of atmospheric leptons.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Proton-air interaction properties at $\sqrt{s} \simeq 100$ TeV from shower-depth measurements with the Pierre Auger Observatory and their connection to the Muon Puzzle

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    Using a universal relation found across hadronic interaction models, Auger's deeper-than-predicted shower maxima imply increased elasticity and hadronic energy fraction in proton–air collisions, needing 2.8–4.6× ampli...

  2. A New Method for Measuring the Pion-Air Cross Section at Multi-TeV Energies Using Muon Bundle Properties in Deep Underground Detectors

    astro-ph.HE 2025-07 conditional novelty 5.0 of 10

    Simulations show that underground muon bundle counts could constrain the inelastic pion-air cross section to roughly 10-15% near 1-2 TeV.

  3. Neutrino Physics and Astrophysics at Colliders

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    A review of collider neutrino experiments, covering first FASERv and SND@LHC measurements, FPF prospects for neutrino cross sections, new physics searches, and astrophysics applications.

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