The Measurement and Modelling of Cosmic Ray Muons at KM3NeT Detectors

Fuente: arXiv
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Auteur principal: Kalaczyński, Piotr
Format: Preprint
Publié: 2024
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author Kalaczyński, Piotr
author_facet Kalaczyński, Piotr
contents Atmospheric muons are the most frequently observed form of cosmic radiation. Despite this, the existence of the muon flux component produced in decays of short-lived parent particles, called prompt muon flux still awaits experimental confirmation. This contribution to the muon flux is expected to start dominating at high energies, around PeV, since many of the prompt parent particles are heavy hadrons, containing charm and strange quarks. The aim of this thesis was two-fold: to evaluate the possibility of observing the prompt muon flux and to validate the performance of the KM3NeT detectors. [shortened abstract, the full version is contained in the thesis]
format Preprint
id arxiv_https___arxiv_org_abs_2402_02620
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle The Measurement and Modelling of Cosmic Ray Muons at KM3NeT Detectors
Kalaczyński, Piotr
High Energy Physics - Experiment
Instrumentation and Detectors
Atmospheric muons are the most frequently observed form of cosmic radiation. Despite this, the existence of the muon flux component produced in decays of short-lived parent particles, called prompt muon flux still awaits experimental confirmation. This contribution to the muon flux is expected to start dominating at high energies, around PeV, since many of the prompt parent particles are heavy hadrons, containing charm and strange quarks. The aim of this thesis was two-fold: to evaluate the possibility of observing the prompt muon flux and to validate the performance of the KM3NeT detectors. [shortened abstract, the full version is contained in the thesis]
title The Measurement and Modelling of Cosmic Ray Muons at KM3NeT Detectors
topic High Energy Physics - Experiment
Instrumentation and Detectors
url https://arxiv.org/abs/2402.02620