Measurement of the average shape of longitudinal profiles of cosmic-ray air showers at the Pierre Auger Observatory

The profile of the longitudinal development of showers produced by ultra-high energy cosmic rays carries information related to the interaction properties of the primary particles with atmospheric nuclei. In this work, we present the first measurement of the average shower profile in traversed atmos...

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Autores principales: Calcagni, Laura Randa, Dova, María Teresa, Hansen, Patricia María, Mariazzi, Analisa Gabriela, Sciutto, Sergio Juan, Tueros, Matías Jorge, Vergara Quispe, Indira Dajhana, Wahlberg, Hernán Pablo, The Pierre Auger Collaboration
Formato: Articulo Preprint
Lenguaje:Inglés
Publicado: 2019
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/115346
Aporte de:
id I19-R120-10915-115346
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Física
Rayos cósmicos
spellingShingle Física
Rayos cósmicos
Calcagni, Laura Randa
Dova, María Teresa
Hansen, Patricia María
Mariazzi, Analisa Gabriela
Sciutto, Sergio Juan
Tueros, Matías Jorge
Vergara Quispe, Indira Dajhana
Wahlberg, Hernán Pablo
The Pierre Auger Collaboration
Measurement of the average shape of longitudinal profiles of cosmic-ray air showers at the Pierre Auger Observatory
topic_facet Física
Rayos cósmicos
description The profile of the longitudinal development of showers produced by ultra-high energy cosmic rays carries information related to the interaction properties of the primary particles with atmospheric nuclei. In this work, we present the first measurement of the average shower profile in traversed atmospheric depth at the Pierre Auger Observatory. The shapes of profiles are well reproduced by the Gaisser-Hillas parametrization within the range studied, for E &gt; 10<SUP>17:8</SUP> eV. A detailed analysis of the systematic uncertainties is performed using 10 years of data and a full detector simulation. The average shape is quantified using two variables related to the width and asymmetry of the profile, and the results are compared with predictions of hadronic interaction models for different primary particles.
format Articulo
Preprint
author Calcagni, Laura Randa
Dova, María Teresa
Hansen, Patricia María
Mariazzi, Analisa Gabriela
Sciutto, Sergio Juan
Tueros, Matías Jorge
Vergara Quispe, Indira Dajhana
Wahlberg, Hernán Pablo
The Pierre Auger Collaboration
author_facet Calcagni, Laura Randa
Dova, María Teresa
Hansen, Patricia María
Mariazzi, Analisa Gabriela
Sciutto, Sergio Juan
Tueros, Matías Jorge
Vergara Quispe, Indira Dajhana
Wahlberg, Hernán Pablo
The Pierre Auger Collaboration
author_sort Calcagni, Laura Randa
title Measurement of the average shape of longitudinal profiles of cosmic-ray air showers at the Pierre Auger Observatory
title_short Measurement of the average shape of longitudinal profiles of cosmic-ray air showers at the Pierre Auger Observatory
title_full Measurement of the average shape of longitudinal profiles of cosmic-ray air showers at the Pierre Auger Observatory
title_fullStr Measurement of the average shape of longitudinal profiles of cosmic-ray air showers at the Pierre Auger Observatory
title_full_unstemmed Measurement of the average shape of longitudinal profiles of cosmic-ray air showers at the Pierre Auger Observatory
title_sort measurement of the average shape of longitudinal profiles of cosmic-ray air showers at the pierre auger observatory
publishDate 2019
url http://sedici.unlp.edu.ar/handle/10915/115346
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