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Abstract:

A measurement of the cosmic-ray spectrum for energies exceeding 4×10 18 eV is presented, which is based on the analysis of showers with zenith angles greater than 60° detected with the Pierre Auger Observatory between 1 January 2004 and 31 December 2013. The measured spectrum confirms a flux suppression at the highest energies. Above 5.3×10 18 eV, the "ankle", the flux can be described by a power law E -γ with index γ=2.70 ± 0.02 (stat) ± 0.1 (sys) followed by a smooth suppression region. For the energy (E s ) at which the spectral flux has fallen to one-half of its extrapolated value in the absence of suppression, we find E s =(5.12 ± 0.25 (stat) +1.0 -1.2 (sys))×10 19 eV. © 2015 IOP Publishing Ltd and Sissa Medialab srl.

Registro:

Documento: Artículo
Título:Measurement of the cosmic ray spectrum above 4 × 10 18 eV using inclined events detected with the Pierre Auger Observatory
Autor:Multitudinario:463
Filiación:Centro Atómico Bariloche, Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
Centro de Investigaciones en Láseres y Aplicaciones, CITEDEF, CONICET, Argentina
Departamento de Física, FCEyN, Universidad de Buenos Aires, CONICET, Argentina
IFLP, Universidad Nacional de la Plata, CONICET, La Plata, Argentina
Instituto de Astronomía y Física Del Espacio (IAFE, CONICET-UBA), Buenos Aires, Argentina
Instituto de Física de Rosario (IFIR), CONICET/U.N.R., Facultad de Ciencias Bioquímicas y Farmacéuticas U.N.R., Rosario, Argentina
Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Universidad Tecnológica Nacional, Facultad Regional Mendoza (CONICET/CNEA), Mendoza, Argentina
Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
Observatorio Pierre Auger, Malargüe, Argentina
Observatorio Pierre Auger and Comisión Nacional de Energía Atómica, Malargüe, Argentina
Universidad Tecnológica Nacional, Facultad Regional Buenos Aires, Buenos Aires, Argentina
University of Adelaide, Adelaide, S.A., Australia
Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro, RJ, Brazil
Universidade de São Paulo, Escola de Engenharia de Lorena, Lorena, SP, Brazil
Universidade de São Paulo, Instituto de Física de São Carlos, São Carlos, SP, Brazil
Universidade de São Paulo, Instituto de Física, São Paulo, SP, Brazil
Universidade Estadual de Campinas, IFGW, Campinas, SP, Brazil
Universidade Estadual de Feira de Santana, Brazil
Universidade Federal da Bahia, Salvador, BA, Brazil
Universidade Federal de Pelotas, Pelotas, RS, Brazil
Universidade Federal Do ABC, Santo-André, SP, Brazil
Universidade Federal Do Rio de Janeiro, Instituto de Física, Rio de Janeiro, RJ, Brazil
Universidade Federal Fluminense, EEIMVR, Volta Redonda, RJ, Brazil
Universidad Industrial de Santander, Bucaramanga, Colombia
Charles University, Faculty of Mathematics and Physics, Institute of Particle and Nuclear Physics, Prague, Czech Republic
Institute of Physics, Academy of Sciences of the Czech Republic, Prague, Czech Republic
Palacky University, RCPTM, Olomouc, Czech Republic
Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France
Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris 11, CNRS-IN2P3, France
Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, France
Station de Radioastronomie de Nançay, Observatoire de Paris, CNRS/INSU, France
SUBATECH, École des Mines de Nantes, CNRS-IN2P3, Université de Nantes, France
Bergische Universität Wuppertal, Wuppertal, Germany
Karlsruhe Institute of Technology, Campus South, Institut für Experimentelle Kernphysik (IEKP), Karlsruhe, Germany
Karlsruhe Institute of Technology, Campus North, Institut für Kernphysik, Karlsruhe, Germany
Karlsruhe Institute of Technology, Campus North, Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany
Max-Planck-Institut für Radioastronomie, Bonn, Germany
RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
Universität Hamburg, Hamburg, Germany
Universität Siegen, Siegen, Germany
Università di Milano, Sezione INFN, Milan, Italy
Università di Napoli Federico II, Sezione INFN, Napoli, Italy
Università di Roma II Tor Vergata, Sezione INFN, Roma, Italy
Università di Catania, Sezione INFN, Catania, Italy
Università di Torino, Sezione INFN, Torino, Italy
Dipartimento di Matematica e Fisica E. de Giorgi, Università Del Salento, Sezione INFN, Lecce, Italy
Dipartimento di Scienze Fisiche e Chimiche, Università dell'Aquila, INFN, Italy
Gran Sasso Science Institute (INFN), L'Aquila, Italy
Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo (INAF), Palermo, Italy
INFN, Laboratori Nazionali Del Gran Sasso, Assergi (L'Aquila), Italy
Osservatorio Astrofisico di Torino (INAF), Università di Torino, Sezione INFN, Torino, Italy
Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
Centro de Investigación y de Estudios Avanzados Del IPN (CINVESTAV), México, Mexico
U. Profesional Interdisciplinaria en Ing. y Tecnologias Avanzadas Del Instituto Politecnico Nacional, México, D.F., Mexico
Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, Mexico
Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Michoacán, Mexico
Universidad Nacional Autónoma de México, México, D.F., Mexico
IMAPP, Radboud University, Nijmegen, Netherlands
KVI-Center for Advanced Radiation Technology, University of Groningen, Netherlands
Nikhef, Science Park, Amsterdam, Netherlands
ASTRON, Dwingeloo, Netherlands
Institute of Nuclear Physics PAN, Krakow, Poland
University of Łódź, Łódź, Poland
Laboratorio de Instrumentacao e Fisica Experimental de Particulas-LIP, Instituto Superior Técnico-IST, Universidade de Lisboa-UL, Portugal
Horia Hulubei National Institute for Physics and Nuclear Engineering, Bucharest-Magurele, Romania
Institute of Space Sciences, Bucharest, Romania
University of Bucharest, Physics Department, Romania
University Politehnica of Bucharest, Romania
Experimental Particle Physics Department, J. Stefan Institute, Ljubljana, Slovenia
Laboratory for Astroparticle Physics, University of Nova Gorica, Slovenia
Universidad Complutense de Madrid, Madrid, Spain
Universidad de Alcalá, Alcalá de Henares, Madrid, Spain
Universidad de Granada, C.A.F.P.E., Granada, Spain
Universidad de Santiago de Compostela, Spain
School of Physics and Astronomy, University of Leeds, United Kingdom
Case Western Reserve University, Cleveland, OH, United States
Colorado School of Mines, Golden, CO, United States
Colorado State University, Fort Collins, CO, United States
Colorado State University, Pueblo, CO, United States
Department of Physics and Astronomy, Lehman College, City University of New YorkNY, United States
Fermilab, Batavia, IL, United States
Louisiana State University, Baton Rouge, LA, United States
Michigan Technological University, Houghton, MI, United States
New York University, New York, NY, United States
Northeastern University, Boston, MA, United States
Ohio State University, Columbus, OH, United States
Pennsylvania State University, University Park, PA, United States
University of Chicago, Enrico Fermi Institute, Chicago, IL, United States
University of Hawaii, Honolulu, HI, United States
University of Nebraska, Lincoln, NE, United States
University of New Mexico, Albuquerque, NM, United States
Vrije Universiteit Brussels, Belgium
University of Liverpool, United Kingdom
Palabras clave:cosmic ray experiments; ultra high energy cosmic rays
Año:2015
Volumen:2015
Número:8
DOI: http://dx.doi.org/10.1088/1475-7516/2015/08/049
Título revista:Journal of Cosmology and Astroparticle Physics
Título revista abreviado:J. Cosmol. Astroparticle Phys.
ISSN:14757516
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14757516_v2015_n8_p_Multitudinario

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Citas:

---------- APA ----------
(2015) . Measurement of the cosmic ray spectrum above 4 × 10 18 eV using inclined events detected with the Pierre Auger Observatory. Journal of Cosmology and Astroparticle Physics, 2015(8).
http://dx.doi.org/10.1088/1475-7516/2015/08/049
---------- CHICAGO ----------
Multitudinario:463. "Measurement of the cosmic ray spectrum above 4 × 10 18 eV using inclined events detected with the Pierre Auger Observatory" . Journal of Cosmology and Astroparticle Physics 2015, no. 8 (2015).
http://dx.doi.org/10.1088/1475-7516/2015/08/049
---------- MLA ----------
Multitudinario:463. "Measurement of the cosmic ray spectrum above 4 × 10 18 eV using inclined events detected with the Pierre Auger Observatory" . Journal of Cosmology and Astroparticle Physics, vol. 2015, no. 8, 2015.
http://dx.doi.org/10.1088/1475-7516/2015/08/049
---------- VANCOUVER ----------
Multitudinario:463. Measurement of the cosmic ray spectrum above 4 × 10 18 eV using inclined events detected with the Pierre Auger Observatory. J. Cosmol. Astroparticle Phys. 2015;2015(8).
http://dx.doi.org/10.1088/1475-7516/2015/08/049