Volume 476 - 42nd International Conference on High Energy Physics (ICHEP2024) - Astroparticle Physics and Cosmology Posters
The multi-PMT Optical Module of KM3NeT
I.C. Rea* and  On behalf of the KM3NeT Collaboration
*: corresponding author
Full text: pdf
Pre-published on: December 23, 2024
Published on: April 29, 2025
Abstract
KM3NeT is a research infrastructure with neutrino telescopes at two sites in the Mediterranean Sea for the detection of high-energy cosmic neutrinos. The two underwater telescopes, ARCA and ORCA, are Cherenkov detectors, using similar technology but with different geometrical layouts. In this way, it is possible to cover a large range of neutrino energy and address various science topics ranging from neutrino astronomy to neutrino oscillation research. The main challenge is to instrument a cubic kilometer of detection volume with optical modules for the detection of Cherenkov radiation. The technology of the KM3NeT optical module follows a multi-PMT approach. It contains 31 three-inch photomultiplier tubes for high resolution, good positioning and timing calibration. Its integration process follows a strict protocol as the production takes place in parallel in different integration sites. In this proceeding, we will describe the KM3NeT optical module technology and its integration process.
DOI: https://doi.org/10.22323/1.476.0720
How to cite

Metadata are provided both in article format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in proceeding format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.