- Záznam pochází z PubMed
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
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Status PubMed-not-MEDLINE Jazyk angličtina Země Francie Médium print-electronic
Typ dokumentu časopisecké články
PubMed
26120280
PubMed Central
PMC4477714
DOI
10.1140/epjc/s10052-015-3471-0
PII: 3471
Knihovny.cz E-zdroje
- Publikační typ
- časopisecké články MeSH
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.
'Horia Hulubei' National Institute for Physics and Nuclear Engineering Bucharest Magurele Romania
Benemérita Universidad Autónoma de Puebla Puebla Mexico
Bergische Universität Wuppertal Wuppertal Germany
Case Western Reserve University Cleveland OH USA
Centro Atómico Bariloche and Instituto Balseiro San Carlos de Bariloche Argentina
Centro Brasileiro de Pesquisas Fisicas Rio de Janeiro RJ Brazil
Centro de Investigación y de Estudios Avanzados del IPN Mexico Mexico
Colorado School of Mines Golden CO USA
Colorado State University Fort Collins CO USA
Colorado State University Pueblo CO USA
Departamento de Física FCEyN Universidad de Buenos Aires y CONICET Buenos Aires Argentina
Department of Physics and Astronomy City University of New York New York USA
Dipartimento di Scienze Fisiche e Chimiche dell'Università dell'Aquila and INFN L'Aquila Italy
Enrico Fermi Institute University of Chicago Chicago IL USA
Faculdade Independente do Nordeste Vitória da Conquista Brazil
IFLP Universidad Nacional de La Plata and CONICET La Plata Argentina
IMAPP Radboud University Nijmegen Nijmegen Netherlands
IMAPP Radboud University Nijmegen Nijmegen Netherlands ; Nikhef Science Park Amsterdam Netherlands
INFN Laboratori Nazionali del Gran Sasso Assergi L'Aquila Italy
Institut de Physique Nucléaire d'Orsay Université Paris 11 CNRS IN2P3 Orsay France
Institute of Nuclear Physics PAN Krakow Poland
Institute of Physics of the Academy of Sciences of the Czech Republic Prague Czech Republic
Institute of Space Sciences Bucharest Magurele Romania
Instituto de Astronomía y Física del Espacio Buenos Aires Argentina
Instituto de Física de São Carlos Universidade de São Paulo São Carlos SP Brazil
Instituto de Física Universidade de São Paulo São Paulo SP Brazil
Instituto de Física Universidade Federal do Rio de Janeiro Rio de Janeiro RJ Brazil
Instituto de Tecnologías en Detección y Astropartículas Buenos Aires Argentina
Instituto de Tecnologías en Detección y Astropartículas Mendoza Argentina
Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo Palermo Italy
Karlsruhe Institute of Technology Campus North Institut für Kernphysik Karlsruhe Germany
KVI Center for Advanced Radiation Technology University of Groningen Groningen Netherlands
Laboratoire de l'Accélérateur Linéaire Université Paris 11 CNRS IN2P3 Orsay France
Laboratory for Astroparticle Physics University of Nova Gorica Nova Gorica Slovenia
Louisiana State University Baton Rouge LA USA
Max Planck Institut für Radioastronomie Bonn Germany
Michigan Technological University Houghton MI USA
New York University New York NY USA
Northeastern University Boston MA USA
Observatorio Pierre Auger and Comisión Nacional de Energía Atómica Malargüe Argentina
Observatorio Pierre Auger Malargüe Argentina
Ohio State University Columbus OH USA
Osservatorio Astrofisico di Torino Università di Torino and Sezione INFN Torino Italy
Palacky University RCPTM Olomouc Czech Republic
Pennsylvania State University University Park PA USA
Physics Department University of Bucharest Bucharest Romania
Rudjer Bošković Institute 10000 Zagreb Croatia
RWTH Aachen University 3 Physikalisches Institut A Aachen Germany
School of Physics and Astronomy University of Leeds Leeds UK
SUBATECH École des Mines de Nantes CNRS IN2P3 Université de Nantes Nantes France
Universidad Complutense de Madrid Madrid Spain
Universidad de Alcalá Alcalá de Henares Madrid Spain
Universidad de Granada and C A F P E Granada Spain
Universidad de Santiago de Compostela Santiago de Compostela Spain
Universidad Michoacana de San Nicolas de Hidalgo Morelia Michoacan Mexico
Universidad Nacional Autonoma de Mexico Mexico D F Mexico
Universidade de São Paulo Escola de Engenharia de Lorena Lorena SP Brazil
Universidade Estadual de Campinas IFGW Campinas SP Brazil
Universidade Estadual de Campinas IFGW Campinas SP Brazil ; Fermilab Batavia IL USA
Universidade Estadual de Feira de Santana Feira de Santana Brazil
Universidade Federal da Bahia Salvador BA Brazil
Universidade Federal do ABC Santo André SP Brazil
Universidade Federal Fluminense EEIMVR Volta Redonda RJ Brazil
Università di Catania and Sezione INFN Catania Italy
Università di Milano and Sezione INFN Milan Italy
Università di Napoli Federico 2 and Sezione INFN Napoli Italy
Università di Roma 2 Tor Vergata and Sezione INFN Roma Italy
Università di Torino and Sezione INFN Torino Italy
Universität Hamburg Hamburg Germany
Universität Siegen Siegen Germany
University of Adelaide Adelaide SA Australia
University of Hawaii Honolulu HI USA
University of Łódź Łódź Poland
University of Nebraska Lincoln NE USA
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