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Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory.
Aab, A; Abreu, P; Aglietta, M; Ahn, E J; Samarai, I Al; Albuquerque, I F M; Allekotte, I; Allen, J; Allison, P; Almela, A; Castillo, J Alvarez; Alvarez-Muñiz, J; Batista, R Alves; Ambrosio, M; Aminaei, A; Anchordoqui, L; Andringa, S; Aramo, C; Aranda, V M; Arqueros, F; Asorey, H; Assis, P; Aublin, J; Ave, M; Avenier, M; Avila, G; Awal, N; Badescu, A M; Barber, K B; Bäuml, J; Baus, C; Beatty, J J; Becker, K H; Bellido, J A; Berat, C; Bertaina, M E; Bertou, X; Biermann, P L; Billoir, P; Blaess, S; Blanco, M; Bleve, C; Blümer, H; Bohácová, M; Boncioli, D; Bonifazi, C; Bonino, R; Borodai, N; Brack, J; Brancus, I.
Afiliação
  • Aab A; Universität Siegen, Siegen, Germany.
  • Abreu P; Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisbon, Portugal.
  • Aglietta M; Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy.
  • Ahn EJ; Fermilab, Batavia, IL USA.
  • Samarai IA; Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France.
  • Albuquerque IF; Instituto de Física, Universidade de São Paulo, São Paulo, SP Brazil.
  • Allekotte I; Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina.
  • Allen J; New York University, New York, NY USA.
  • Allison P; Ohio State University, Columbus, OH USA.
  • Almela A; Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina ; Universidad Tecnológica Nacional - Facultad Regional Buenos Aires, Buenos Aires, Argentina.
  • Castillo JA; Universidad Nacional Autonoma de Mexico, Mexico, D.F., Mexico.
  • Alvarez-Muñiz J; Universidad de Santiago de Compostela, Santiago de Compostela, Spain.
  • Batista RA; Universität Hamburg, Hamburg, Germany.
  • Ambrosio M; Università di Napoli "Federico II" and Sezione INFN, Napoli, Italy.
  • Aminaei A; IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands.
  • Anchordoqui L; Department of Physics and Astronomy, City University of New York, New York, USA.
  • Andringa S; Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisbon, Portugal.
  • Aramo C; Università di Napoli "Federico II" and Sezione INFN, Napoli, Italy.
  • Aranda VM; Universidad Complutense de Madrid, Madrid, Spain.
  • Arqueros F; Universidad Complutense de Madrid, Madrid, Spain.
  • Asorey H; Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina.
  • Assis P; Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisbon, Portugal.
  • Aublin J; Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France.
  • Ave M; Universidad de Santiago de Compostela, Santiago de Compostela, Spain.
  • Avenier M; Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France.
  • Avila G; Observatorio Pierre Auger and Comisión Nacional de Energía Atómica, Malargüe, Argentina.
  • Awal N; New York University, New York, NY USA.
  • Badescu AM; University Politehnica of Bucharest, Bucharest, Romania.
  • Barber KB; University of Adelaide, Adelaide, SA Australia.
  • Bäuml J; Karlsruhe Institute of Technology - Campus South - Institut für Experimentelle, Kernphysik (IEKP), Karlsruhe, Germany.
  • Baus C; Karlsruhe Institute of Technology - Campus South - Institut für Experimentelle, Kernphysik (IEKP), Karlsruhe, Germany.
  • Beatty JJ; Ohio State University, Columbus, OH USA.
  • Becker KH; Bergische Universität Wuppertal, Wuppertal, Germany.
  • Bellido JA; University of Adelaide, Adelaide, SA Australia.
  • Berat C; Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France.
  • Bertaina ME; Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy.
  • Bertou X; Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina.
  • Biermann PL; Max-Planck-Institut für Radioastronomie, Bonn, Germany.
  • Billoir P; Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France.
  • Blaess S; University of Adelaide, Adelaide, SA Australia.
  • Blanco M; Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France.
  • Bleve C; Dipartimento di Matematica e Fisica "E. De Giorgi" dell'Università del Salento and Sezione INFN, Lecce, Italy.
  • Blümer H; Karlsruhe Institute of Technology - Campus South - Institut für Experimentelle, Kernphysik (IEKP), Karlsruhe, Germany ; Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany.
  • Bohácová M; Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic.
  • Boncioli D; INFN, Laboratori Nazionali del Gran Sasso, Assergi, L'Aquila Italy.
  • Bonifazi C; Instituto de Física, Universidade Federal do Rio de Janeiro, Rio de Janeiro, RJ Brazil.
  • Bonino R; Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy.
  • Borodai N; Institute of Nuclear Physics PAN, Krakow, Poland.
  • Brack J; Colorado State University, Fort Collins, CO USA.
  • Brancus I; 'Horia Hulubei' National Institute for Physics and Nuclear Engineering, Bucharest-Magurele, Romania.
Eur Phys J C Part Fields ; 75(6): 269, 2015.
Article em En | MEDLINE | ID: mdl-26120280
ABSTRACT
Energy-dependent patterns in the arrival directions of cosmic rays are searched for using data of the Pierre Auger Observatory. We investigate local regions around the highest-energy cosmic rays with [Formula see text] eV by analyzing cosmic rays with energies above [Formula see text] eV arriving within an angular separation of approximately 15[Formula see text]. We characterize the energy distributions inside these regions by two independent methods, one searching for angular dependence of energy-energy correlations and one searching for collimation of energy along the local system of principal axes of the energy distribution. No significant patterns are found with this analysis. The comparison of these measurements with astrophysical scenarios can therefore be used to obtain constraints on related model parameters such as strength of cosmic-ray deflection and density of point sources.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Ano de publicação: 2015 Tipo de documento: Article

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Ano de publicação: 2015 Tipo de documento: Article