Studies on the response of a water-Cherenkov detector of the Pierre Auger Observatory to atmospheric muons using an RPC hodoscope

Extensive air showers, originating from ultra-high energy cosmic rays, have been successfully measured through the use of arrays of water-Cherenkov detectors (WCDs). Sophisticated analyses exploiting WCD data have made it possible to demonstrate that shower simulations, based on different hadronic-i...

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Autores:
Tipo de recurso:
Fecha de publicación:
2020
Institución:
Universidad de Medellín
Repositorio:
Repositorio UDEM
Idioma:
eng
OAI Identifier:
oai:repository.udem.edu.co:11407/6023
Acceso en línea:
http://hdl.handle.net/11407/6023
Palabra clave:
Data reduction methods
Large detector systems for particle and astroparticle physics
Large detector-systems performance
Performance of high energy physics detectors
Augers
Cerenkov counters
Charged particles
Cosmology
Observatories
Particle spectrometers
Atmospheric muons
Extensive air showers
Hadronic interaction models
Long term stability
Pierre Auger observatory
Resistive plate chambers
Ultra high-energy cosmic rays
Water Cherenkov detectors
Particle detectors
Rights
License
http://purl.org/coar/access_right/c_16ec
Description
Summary:Extensive air showers, originating from ultra-high energy cosmic rays, have been successfully measured through the use of arrays of water-Cherenkov detectors (WCDs). Sophisticated analyses exploiting WCD data have made it possible to demonstrate that shower simulations, based on different hadronic-interaction models, cannot reproduce the observed number of muons at the ground. The accurate knowledge of the WCD response to muons is paramount in establishing the exact level of this discrepancy. In this work, we report on a study of the response of a WCD of the Pierre Auger Observatory to atmospheric muons performed with a hodoscope made of resistive plate chambers (RPCs), enabling us to select and reconstruct nearly 600 thousand single muon trajectories with zenith angles ranging from 0 to 55. Comparison of distributions of key observables between the hodoscope data and the predictions of dedicated simulations allows us to demonstrate the accuracy of the latter at a level of 2%. As the WCD calibration is based on its response to atmospheric muons, the hodoscope data are also exploited to show the long-term stability of the procedure. © 2020 IOP Publishing Ltd and Sissa Medialab.