Ultrahigh energy cosmic ray air showers probe particle physics at energies beyond the reach of accelerators. Here we introduce a new method to test hadronic interaction models without relying on the absolute energy calibration, and apply it to events with primary energy 6-16 EeV (ECM=110-170 TeV), whose longitudinal development and lateral distribution were simultaneously measured by the Pierre Auger Observatory. The average hadronic shower is 1.33±0.16 (1.61±0.21) times larger than predicted using the leading LHC-tuned models EPOS-LHC (QGSJetII-04), with a corresponding excess of muons. © 2016 American Physical Society.
Documento: | Artículo |
Título: | Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory |
Autor: | Multitudinario:437 |
Filiación: | Universität Siegen, Fachbereich 7 Physik - Experimentelle Teilchenphysik, Germany Laboratorio de Instrumentacao e Fisica Experimental de Particulas - LIP, Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Portugal Osservatorio Astrofisico di Torino (INAF), Torino, Italy INFN, Sezione di Torino, Italy Fermi National Accelerator Laboratory, Batavia, IL, United States Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, France Universidade de São Paulo, Inst. de Física, São Paulo, Brazil Centro Atómico Bariloche, Instituto Balseiro (CNEA-UNCuyo-CONICET), Argentina New York University, New York, NY, United States Ohio State University, Columbus, OH, United States Instituto de Tecnologías en Detección y Astropartículas (CNEA CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina Universidad Tecnológica Nacional, Facultad Regional Buenos Aires, Argentina Universidad Nacional Autónoma de México, Mexico Universidad de Santiago de Compostela, Spain INFN, Sezione di Napoli, Italy INFN, Sezione di l'Aquila, Italy Department of Physics and Astronomy, Lehman College, City University of New York, Bronx, NY, United States Universidad Complutense de Madrid, Spain University of Bucharest, Physics Department, Romania Universidad Industrial de Santander, Colombia Observatorio Pierre Auger, Argentina Observatorio Pierre Auger and Comisión Nacional de Energía Atómica, Argentina University Politehnica of Bucharest, Romania Karlsruhe Institute of Technology, Institut für Experimentelle Kernphysik (IEKP), Germany Bergische Universität Wuppertal, Department of Physics, Germany, Germany University of Adelaide, Australia Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, France Università Torino, Dipartimento di Fisica, Italy Max-Planck-Institut für Radioastronomie, Bonn, Germany Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris 11, CNRS-IN2P3, France Institute of Physics (FZU), Academy of Sciences of the Czech Republic, Czech Republic Università Del Salento, Dipartimento di Matematica e Fisica E. de Giorgi, Italy INFN, Sezione di Lecce, Italy Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany INFN Laboratori Del Gran Sasso, Italy Universidade Federal Do Rio de Janeiro (UFRJ), Instituto de Física, Brazil Institute of Nuclear Physics PAN, Poland Colorado State University, Fort Collins, CO, United States Horia Hulubei National Institute for Physics and Nuclear Engineering, Romania RWTH Aachen University, III. Physikalisches Institut A, Germany Universidad de Granada and C.A.F.P.E., Spain Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud Universiteit, Nijmegen, Netherlands Università di Catania, Dipartimento di Fisica e Astronomia, Italy INFN, Sezione di Catania, Italy Universidad Autónoma de Chiapas, Mexico INFN, Sezione di Milano, Italy Institute of Space Science, Romania Universidad Michoacana de San Nicolás de Hidalgo, Mexico Universidade Estadual de Campinas (UNICAMP), Brazil Michigan Technological University, Houghton, MI, United States Università di Napoli Federico II, Dipartimento di Fisica, Italy Pennsylvania State University, University Park, PA, United States Case Western Reserve University, Cleveland, OH, United States University of Chicago, Chicago, IL, United States SUBATECH, École des Mines de Nantes, CNRS-IN2P3, Université de Nantes, France Station de Radioastronomie de Nançay, France Università Del Salento, Dipartimento di Ingegneria, Italy Instituto de Astronomía y Física Del Espacio (IAFE CONICET-UBA), Argentina Departamento de Fisica and Departamento de Ciencias de la Atmosfera y Los Oceanos, FCEyN, Universidad de Buenos Aires, Argentina Universidade Federal Fluminense, Brazil Nationaal Instituut voor Kernfysica en Hoge Energie Fysica (NIKHEF), Netherlands Universidade de São Paulo, Inst. de Física de São Carlos, São Carlos, Brazil Universidad de Alcalá de Henares, Spain Università di Roma Tor Vergata, Dipartimento di Fisica, Italy INFN, Sezione di Roma Tor Vergata, Italy Università dell'Aquila, Dipartimento di Chimica e Fisica, Italy Universidade Federal Do Paraná, Setor Palotina, Brazil IFLP, Universidad Nacional de la Plata, CONICET, Argentina Universität Hamburg II, Institut für Theoretische Physik, Germany Stichting Astronomisch Onderzoek in Nederland (ASTRON), Dwingeloo, Netherlands Experimental Particle Physics Department, J. Stefan Institute, Slovenia Laboratory for Astroparticle Physics, University of Nova Gorica, Slovenia Instituto de Física de Rosario (IFIR), CONICET/U.N.R., Facultad de Ciencias Bioquímicas y Farmacéuticas U.N.R., Argentina Instituto de Tecnologías en Detección y Astropartículas (CNEA CONICET, UNSAM), Universidad Tecnológica Nacional, Facultad Regional Mendoza (CONICET/CNEA), Argentina Karlsruhe Institute of Technology, Institut für Prozessdatenverarbeitung und Elektronik (IPE), Germany University of Łódź, Poland University of Hawaii, Honolulu, HI, United States Universidade Estadual de Feira de Santana (UEFS), Brazil Palacky University, RCPTM, Czech Republic Colorado School of Mines, Golden, CO, United States Universidade Federal Do ABC (UFABC), Brazil Benemérita Universidad Autónoma de Puebla (BUAP), Mexico Università di Milano, Dipartimento di Fisica, Italy Centro de Investigación y de Estudios Avanzados Del IPN (CINVESTAV), Mexico Louisiana State University, Baton Rouge, LA, United States University of New Mexico, Albuquerque, NM, United States Centro Brasileiro de Pesquisas Fisicas (CBPF), Brazil KVI - Center for Advanced Radiation Technology, University of Groningen, Netherlands Universidade Federal de Pelotas, Brazil University Prague, Institute of Particle and Nuclear Physics, Czech Republic Centro de Investigaciones en Láseres y Aplicaciones, CITEDEF, CONICET, Argentina Northeastern University, Boston, MA, United States U. Profesional Interdisciplinaria en Ing. y Tecnologias Avanzadas Del Instituto Politecnico Nacional, Mexico Universidade Federal da Bahia, Brazil University of Nebraska, Lincoln, NE, United States INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo, Italy Universidade de São Paulo, Escola de Engenharia de Lorena, Brazil School of Physics and Astronomy, University of Leeds, Leeds, United Kingdom Deutsches Elektronen-Synchrotron (DESY), Zeuthen, Germany Vrije Universiteit Brussels, Brussels, Belgium |
Palabras clave: | Augers; Cosmic ray detectors; Cosmology; High energy physics; Observatories; Tellurium compounds; Energy calibration; Hadronic interaction models; Hadronic interactions; Hadronic showers; Lateral distributions; Pierre Auger observatory; Ultra-high energies; Ultrahigh-energy cosmic rays; Cosmic rays |
Año: | 2016 |
Volumen: | 117 |
Número: | 19 |
DOI: | http://dx.doi.org/10.1103/PhysRevLett.117.192001 |
Título revista: | Physical Review Letters |
Título revista abreviado: | Phys Rev Lett |
ISSN: | 00319007 |
CODEN: | PRLTA |
Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00319007_v117_n19_p_Multitudinario |