REVIEW 5 cited by
The hadronic interaction model Sibyll-2.3c and inclusive lepton fluxes
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
The hadronic interaction model Sibyll-2.3c and inclusive lepton fluxes
read the original abstract
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.
Forward citations
Cited by 5 Pith papers
-
A New Source of Millicharged Particles: Secondary Showers in the LHC Forward Absorber
Secondary cascades in the TAXN absorber produce a substantial millicharged particle flux that complements primary production and boosts FORMOSA signals by ~50% for m_χ below 0.1 GeV.
-
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
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...
-
Mountain Muography for China Jinping Underground Laboratory
First muography at CJPL reconstructs directional overburden opacity map in agreement with satellite terrain models and predicts muon fluxes for CJPL-II halls.
-
Constraints on long-range neutrino interactions from a variety of $U(1)^\prime$ symmetries using atmospheric neutrinos at IceCube DeepCore
No evidence for long-range neutrino interactions from a broad class of anomaly-free U(1)' symmetries is found in 8 years of IceCube DeepCore atmospheric data, producing stringent constraints on the corresponding LRI p...
-
High-energy atmospheric muon flux calculations in comparison with recent measurements
QGSM-based prompt muon calculations match IceCube spectra above 500 TeV, while lower charm-production models require extra flux from rare decays of eta, eta', rho, omega, and phi mesons.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.