Pith. sign in

REVIEW 4 cited by

Improvement of low energy atmospheric neutrino flux calculation using the JAM nuclear interaction model

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

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

arxiv 1102.2688 v1 pith:ILHEVSRE submitted 2011-02-14 astro-ph.HE

Morihiro Honda , Takaaki Kajita , Katsuaki Kasahara , Shoichi Midorikawa This is my paper · ORCID
classification astro-ph.HE
keywords atmosphericcalculationfluxneutrinointeractionmodelbettersome
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

We present the calculation of the atmospheric neutrino fluxes with an interaction model named JAM, which is used in PHITS (Particle and Heavy-Ion Transport code System). The JAM interaction model agrees with the HARP experiment a little better than DPMJET-III. After some modifications, it reproduces the muon flux below 1~GeV/c at balloon altitudes better than the modified-DPMJET-III which we used for the calculation of atmospheric neutrino flux in previous works. Some improvements in the calculation of atmospheric neutrino flux are also reported.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 4 Pith papers

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

  1. Composite asymmetric dark matter with a dark photon portal: Multimessenger tests

    hep-ph 2024-12 conditional novelty 6.0 of 10

    Decaying composite dark matter in the 1 to 10 GeV mass range is most strongly constrained by AMS-02 positron data, needing lifetimes above roughly 10^26 seconds.

  2. Neutrino Oscillation Tomography of the Earth with the Hyper-Kamiokande Detector

    hep-ex 2024-11 conditional novelty 6.0 of 10

    Hyper-Kamiokande could measure the average core density with an uncertainty around -14%/+40% at nominal resolution, improving to about -8%/+10% with better resolution, after 6500 days.

  3. Reduction of the Uncertainty in the Atmospheric Neutrino Flux Prediction Below 1 GeV Using Accurately Measured Atmospheric Muon Flux

    astro-ph.HE 2019-08 conditional novelty 6.0 of 10

    A variation-based analysis shows that constraining atmospheric muon flux with precision data can reduce sub-GeV atmospheric neutrino flux uncertainty, most effectively when muons are measured at 3000-5000 m altitude sites.

  4. Super-Kamiokande Strongly Constrains Leptophilic Dark Matter Capture in the Sun

    astro-ph.HE 2025-01 unverdicted novelty 5.0 of 10

    Super-Kamiokande data constrains the DM-electron scattering cross-section for leptophilic dark matter to ~4e-41 cm2 below 100 GeV, exceeding direct detection by over an order of magnitude.

Pith tools