1. Azimuthal asymmetry in the risetime of the surface detector signals of the Pierre Auger Observatory.
- Author
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Arqueros Martínez, Fernando, García Pinto, Diego, Minaya Flores, Ignacio Andrés, Rosado Vélez, Jaime, Vázquez Peñas, José Ramón, Arqueros Martínez, Fernando, García Pinto, Diego, Minaya Flores, Ignacio Andrés, Rosado Vélez, Jaime, and Vázquez Peñas, José Ramón
- Abstract
© 2016 American Physical Society. Artículo firmado por más de 10 autores (Pierre Auger Collaboration). The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargue. We are very grateful to the following agencies and organizations for financial support: Comision Nacional de Energia Atomica, Agencia Nacional de Promocion Cientifica y Tecnologica (ANPCyT), Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET), Gobierno de la Provincia de Mendoza, Municipalidad de Malargue, NDM Holdings and Valle Las Lenas, in gratitude for their continuing cooperation over land access, Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundacao de Amparo a Pesquisa do Estado de Rio de Janeiro (FAPERJ), Sao Paulo Research Foundation (FAPESP) Grants No. 2010/07359-6 and No. 1999/05404-3, Ministerio de Ciencia e Tecnologia (MCT), Brazil; Grant No. MSMT-CR LG13007, No. 7AMB14AR005, and the Czech Science Foundation Grant No. 14-17501S, Czech Republic; Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Regional Ile-de-France, Departement Physique Nucleaire et Corpusculaire (PNC-IN2P3/CNRS), Departement Sciences de l'Univers (SDU-INSU/CNRS), Institut Lagrange de Paris (ILP) Grant No. LABEX ANR-10-LABX- 63, within the Investissements d'Avenir Programme Grant No. ANR-11-IDEX-0004-02, France; Bundesministerium fur Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Finanzministerium Baden-Wurttemberg, Helmholtz Alliance for Astroparticle Physics (HAP), Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Ministerium fur Wissenschaft und Forschung, Nordrhein Westfalen, Ministerium fur Wissenschaft, Forschung und Kunst, Baden-Wurttember, Germany; Istituto Nazionale, The azimuthal asymmetry in the risetime of signals in Auger surface detector stations is a source of information on shower development. The azimuthal asymmetry is due to a combination of the longitudinal evolution of the shower and geometrical effects related to the angles of incidence of the particles into the detectors. The magnitude of the effect depends upon the zenith angle and state of development of the shower and thus provides a novel observable, (sec theta)(max), sensitive to the mass composition of cosmic rays above 3 x 10(18) eV. By comparing measurements with predictions from shower simulations, we find for both of our adopted models of hadronic physics (QGSJETII-04 and EPOS-LHC) an indication that the mean cosmic-ray mass increases slowly with energy, as has been inferred from other studies. However, the mass estimates are dependent on the shower model and on the range of distance from the shower core selected. Thus the method has uncovered further deficiencies in our understanding of shower modeling that must be resolved before the mass composition can be inferred from (sec theta)(max)., Czech Science Foundation, Czech Republic, Centre de Calcul, France, Centre National de la Recherche Scientifique (CNRS), France, Conseil Regional Ile-de-France, France, Departement Physique Nucleaire et Corpusculaire, France, Departement Sciences de l'Univers (SDU-INSU/CNRS), France, Institut Lagrange de Paris (ILP), within the Investissements d'Avenir Programme, France, Bundesministerium fur Bildung und Forschung (BMBF), Germany, Deutsche Forschungsgemeinschaft (DFG), Germany, Finanzministerium Baden-Wurttemberg, Germany, Helmholtz Alliance for Astroparticle Physics (HAP), Germany, Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Germany, Ministerium fur Wissenschaft und Forschung, Germany, Nordrhein Westfalen, Germany, Ministerium fur Wissenschaft, Germany, Forschung und Kunst, Germany, Baden-Wurttember, Germany, Istituto Nazionale di Fisica Nucleare (INFN), Italy, Istituto Nazionale di Astrofisica (INAF), Italy, Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR), Italy, Gran Sasso Center for Astroparticle Physics (CFA), Italy, CETEMPS Center of Excellence, Italy, Ministero degli Affari Esteri (MAE), Italy, Ministerie van Onderwijs, Netherlands, Cultuur en Wetenschap, Netherlands, Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Netherlands, Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands, National Centre for Research and Development, Poland, National Science Centre, Poland, Portuguese national funds, Portugal, FEDER funds within Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia (COMPETE), Portugal, Romanian Authority for Scientific Research ANCS, Romania, CNDI-UEFISCDI, Romania, Minister of National Education, Romania, Programme Space Technology and Advanced Research (STAR), Romania, Slovenian Research Agency, Slovenia, Comunidad de Madrid, Spain, FEDER funds, Spain, Ministerio de Educacion y Ciencia, Spain, Xunta de Galicia, Spain, European Community 7th Framework Program, Spain, Science and Technology Facilities Council, United Kingdom, Marie Curie-IRSES/EPLANET, European Union 7th Framework Program, UNESCO, Depto. de Estructura de la Materia, Física Térmica y Electrónica, Fac. de Ciencias Físicas, TRUE, pub
- Published
- 2023