A thorough search of the sky exposed at the Pierre Auger Cosmic Ray Observatory reveals no statistically significant excess of events in any small solid angle that would be indicative of a flux of neutral particles from a discrete source. The search covers from -90° to +15° in declination using four different energy ranges above 1 EeV (10 18 eV). The method used in this search is more sensitive to neutrons than to photons. The upper limit on a neutron flux is derived for a dense grid of directions for each of the four energy ranges. These results constrain scenarios for the production of ultrahigh energy cosmic rays in the Galaxy. © 2012. The American Astronomical Society. All rights reserved..
Documento: | Artículo |
Título: | A search for point sources of EeV neutrons |
Autor: | Multitudinario:509 |
Filiación: | NYU Abu Dhabi, United Arab Emirates LIP, Instituto Superior Técnico, Technical University of Lisbon, Portugal Istituto di Fisica Dello Spazio Interplanetario (INAF), Università di Torino, Sezione INFN, Torino, Italy University of Wisconsin, Madison, WI, United States Fermilab, Batavia, IL, United States Instituto de Física, Universidade de São Paulo, São Paulo, SP, Brazil Laboratoire AstroParticule et Cosmologie (APC), Université Paris 7, CNRS-IN2P3, Paris, France Centro Atómico Bariloche, Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina New York University, New York, NY, United States Ohio State University, Columbus, OH, United States Facultad Regional Buenos Aires, Universidad Tecnológica Nacional, Buenos Aires, Argentina Instituto de Tecnologías en Detección y Astropartí culas, CNEA, UNSAM, Buenos Aires, Argentina Universidad Nacional Autonoma de Mexico, D.F. Mexico, Mexico Universidad de Santiago de Compostela, Spain IFGW, Universidade Estadual de Campinas, SP Campinas, Brazil Università di Napoli Federico II, Sezione INFN, Napoli, Italy IMAPP, Radboud University Nijmegen, Netherlands University of Wisconsin, Milwaukee, WI, United States Rudjer Boškovi'c Institute, 10000 Zagreb, Croatia IFLP, Universidad Nacional de la Plata, CONICET, La Plata, Argentina Universidad Complutense de Madrid, Madrid, Spain Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France Karlsruhe Institute of Technology-Campus, South-Institut für Experimentelle Kernphysik (IEKP), Karlsruhe, Germany Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier, INPG, CNRS-IN2P3, Grenoble, France Observatorio Pierre Auger and Comisión Nacional de Energía Atómica, Malargüe, Argentina University Politehnica of Bucharest, Romania Karlsruhe Institute of Technology-Campus, North-Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany University of Adelaide, SA Adelaide, Australia Centro Brasileiro de Pesquisas Fisicas, RJ Rio de Janeiro, Brazil Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris 11, CNRS-IN2P3, France Universidade Estadual Do Sudoeste da Bahia, Vitoria da Conquista, BA, Brazil Karlsruhe Institute of Technology-Campus, North-Institut für Kernphysik, Karlsruhe, Germany Bergische Universität Wuppertal, Wuppertal, Germany SUBATECH, École des Mines de Nantes, Université de Nantes, France Max-Planck-Institut für Radioastronomie, Bonn, Germany Universidad de Alcalá, Alcalá de Henares, Madrid, Spain Institute of Physics, Academy of Sciences of the Czech Republic, Prague, Czech Republic Università di Roma II Tor Vergata, Sezione INFN, Roma, Italy Instituto de Física, Universidade Federal Do Rio de Janeiro, RJ Rio de Janeiro, Brazil Institute of Nuclear Physics PAN, Krakow, Poland Colorado State University, Fort Collins, CO, United States Horia Hulubei National Institute for Physics and Nuclear Engineering, Bucharest- Magurele, Romania Colorado State University, Pueblo, CO, United States School of Physics and Astronomy, University of Leeds, United Kingdom Universität Siegen, Siegen, Germany Universidad de Granada, C. A.F. P.E., Granada, Spain Case Western Reserve University, Cleveland, OH, United States Pennsylvania State University, University Park, PA, United States Università di Milano, Sezione INFN, Milan, Italy Università di Catania and Sezione INFN, Catania, Italy Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo (INAF), Palermo, Italy Dipartimento di Matematica e Fisica E. de Giorgi, Università Del Salento, Sezione INFN, Lecce, Italy Università di Torino, Sezione INFN, Torino, Italy Michigan Technological University, Houghton, MI, United States Observatorio Pierre Auger, Malargüe, Argentina Nikhef, Science Park, Amsterdam, Netherlands University of Chicago, Enrico Fermi Institute, Chicago, IL, United States Instituto de Astronomía y Física Del Espacio (CONICET-UBA), Buenos Aires, Argentina Departamento de Física, FCEyN, Universidad de Buenos Aires y CONICET, Argentina EEIMVR, Universidade Federal Fluminense, RJ Volta Redonda, Brazil Faculty Mendoza (CONICET/CNEA), National Technological University, Mendoza, Argentina Instituto de Física, Universidade de São Paulo, São Carlos, SP, Brazil Kernfysisch Versneller Instituut, University of Groningen, Groningen, Netherlands Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France Università dell'Aquila, INFN, L'Aquila, Italy Institute for Nuclear Science and Technology (INST), Hanoi, Viet Nam III. Physikalisches Institut A, RWTH Aachen University, Aachen, Germany ASTRON, Dwingeloo, Netherlands J. Stefan Institute, Ljubljana, Slovenia Laboratory for Astroparticle Physics, University of Nova Gorica, Slovenia Dipartimento di Fisica dell'Università, INFN, Genova, Italy University of Łódź, Łódź, Poland University of New Mexico, Albuquerque, NM, United States INFN, Laboratori Nazionali Del Gran Sasso, Assergi (L'Aquila), Italy Universidade Estadual de Feira de Santana, Brazil RCPTM, Palacky University, Olomouc, Czech Republic Faculty of Mathematics and Physics, Institute of Particle and Nuclear Physics, Charles University, Prague, Czech Republic Louisiana State University, Baton Rouge, LA, United States Universität Hamburg, Hamburg, Germany Universidade Federal Do ABC, SP Santo André, Brazil Benemérita Universidad Autónoma de Puebla, Puebla, Mexico Universidad Michoacana de San Nicolas de Hidalgo, Michoacan, Morelia, Mexico Centro de Investigación y de Estudios Avanzados Del IPN (CINVESTAV), México, Mexico Southern University, Baton Rouge, LA, United States Rudolf Peierls Centre for Theoretical Physics, University of Oxford, Oxford, United Kingdom University of Hawaii, Honolulu, HI, United States Instituto de Física de Rosario (IFIR), CONICET/U. N.R., Facultad de Ciencias Bioquímicas y Farmacéuticas U. N.R., Rosario, Argentina Centro de Investigaciones en Láseres y Aplicaciones, CITEDEF and CONICET, Argentina Instituto de Física Corpuscular, CSIC, Universitat de València, Valencia, Spain Northeastern University, Boston, MA, United States Universidade Federal da Bahia, BA Salvador, Brazil University of Nebraska, Lincoln, NE, United States Colorado School of Mines, Golden, CO, United States Physics Department, University of Bucharest, Romania Argonne National Laboratory, Argonne, IL, United States Los Alamos National Laboratory, Los Alamos, NM, United States Universidad Autonoma de Chiapas, Mexico University of Maryland, United States Université de Lausanne, Switzerland Konan University, Kobe, Japan |
Palabras clave: | cosmic rays; Galaxy: disk; methods: data analysis |
Año: | 2012 |
Volumen: | 760 |
Número: | 2 |
DOI: | http://dx.doi.org/10.1088/0004-637X/760/2/148 |
Título revista: | Astrophysical Journal |
Título revista abreviado: | Astrophys. J. |
ISSN: | 0004637X |
Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v760_n2_p_Multitudinario |