Pith. sign in

REVIEW 1 cited by

The probability density function of the arrival time of \v{C}erenkov light

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 2305.19626 v1 pith:CLLR4DZC submitted 2023-05-31 astro-ph.IM

M. de Jong , E. van Campenhout This is my paper
classification astro-ph.IM
keywords lightarrivaldensitydetectionerenkovfunctionmuonphoto-multiplier
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

The probability density function of the arrival time of \v{C}erenkov light on a photo-multiplier tube has been studied. This study covers light production, transmission and detection. The light production includes the light from a muon, the light from a shower and the light due to the energy loss of a muon. For the transmission of light, the effects of dispersion, absorption and scattering in the medium are considered. For the detection of light, the angular acceptance and the quantum efficiency of the photo-multiplier tube are taken into account.

Discussion (0). Sign in to comment.

Forward citations

Cited by 1 Pith paper

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

  1. Search for an all-sky and a Galactic Ridge diffuse neutrino emission with the first 2 years of KM3NeT/ARCA data

    astro-ph.HE 2026-08 accept novelty 5.0 of 10

    Using 640 days of KM3NeT/ARCA data, the collaboration finds no significant diffuse astrophysical neutrino flux and sets upper limits for all-sky and Galactic Ridge emission.

Pith tools