English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

The general features of the neutrino flux from cosmic ray interactions in theEarth's atmosphere are well characterized. However, the absolute precision ofcalculations is still insufficient and the uncertainty from the modeling ofhadronic interactions in the very forward region remains a major limitation. Inthis work, we benchmark the current generation hadronic models usinghigh-precision atmospheric muon calculations from a few GeV to multiple TeVenergies provided by the MCEq code. We derive corrections to hadronic modelsusing publicly available measurements of the flux and charge ratio ofatmospheric muons from surface and underground detectors. When combining data,the experimental uncertainties are taken into account. We discuss thecalibration method and the strength of the derived constraints.

Calibration of atmospheric neutrino flux calculations using cosmic muon flux and charge ratio measurements