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Abstract:

The Pierre Auger Collaboration has reported evidence for anisotropy in the distribution of arrival directions of the cosmic rays with energies E > Eth = 5.5 × 1019 eV. These show a correlation with the distribution of nearby extragalactic objects, including an apparent excess around the direction of Centaurus A. If the particles responsible for these excesses at E > Eth are heavy nuclei with charge Z, the proton component of the sources shouldłead to excesses in the same regions at energies E/Z. We here report thełack of anisotropies in these directions at energies above Eth/Z (for illustrative values of Z = 6,13,26). If the anisotropies above Eth are due to nuclei with charge Z, and under reasonable assumptions about the acceleration process, these observations imply stringent constraints on the allowed proton fraction at thełower energies. © 2011 IOP Publishing Ltd and SISSA.

Registro:

Documento: Artículo
Título:Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory
Autor:Multitudinario:493
Filiación:Centro Atómico Bariloche, Instituto Balseiro (CNEA- UNCuyo-CONICET), San Carlos de Bariloche, Argentina
Centro Atómico Constituyentes, Buenos Aires, Argentina
Centro de Investigaciones en Láseres y Aplicaciones, CITEFA, CONICET, Argentina
Departamento de Física, FCEyN, Universidad de Buenos Aires y CONICET, Argentina
IFLP, Universidad Nacional de la Plata, CONICET, La Plata, Argentina
Instituto de Astronomía y Física Del Espacio (CONICET- UBA), Buenos Aires, Argentina
Instituto de Física de Rosario (IFIR), CONICET/U.N.R., Facultad de Ciencias Bioquímicas y Farmacíeuticas U.N.R., Rosario, Argentina
National Technological University, Faculty Mendoza (CONICET/CNEA), Mendoza, Argentina
Pierre Auger Southern Observatory, Malargúe, Argentina
Pierre Auger Southern Observatory, Comisión Nacional de Energía Atómica, Malargúe, Argentina
University of Adelaide, Adelaide, SA, Australia
Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro, RJ, Brazil
Pontifícia Universidade Católica, Rio de Janeiro, RJ, Brazil
Universidade de São Paulo, Instituto de Física, 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 Estadual Do Sudoeste da Bahia, Vitoria da Conquista, BA, Brazil
Universidade Federal da Bahia, Salvador, BA, 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
Rudjer Bošković Institute, 10000 Zagreb, Croatia
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, RCATM, Olomouc, Czech Republic
Institut de Physique Nucléaire DOrsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France
Laboratoire AstroParticule et Cosmologie (APC), Université Paris 7, CNRS-IN2P3, Paris, France
Laboratoire de LAccélérateur Linéaire (LAL), Université Paris 11, CNRS-IN2P3, Orsay, 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 Joseph Fourier, CNRS-IN2P3, Grenoble, France
SUBATECH, CNRS-IN2P3, Nantes, France
Bergische Universitát Wuppertal, Wuppertal, 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
Karlsruhe Institute of Technology - Campus South, Institut für Experimentelle Kernphysik (IEKP), Karlsruhe, Germany
Max-Planck-Institut für Radioastronomie, Bonn, Germany
RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
Universitát Hamburg, Hamburg, Germany
Universitát Siegen, Siegen, Germany
Dipartimento di Fisica DellUniversitá, INFN, Genova, Italy
Universitá DellAquila, INFN, LAquila, Italy
Universitá di Milano, Sezione INFN, Milan, Italy
Dipartimento di Fisica DellUniversitá Del Salento, Sezione INFN, Lecce, Italy
Universitá di Napoli Federico II, Sezione INFN, Napoli, Italy
Universitá di Roma II Tor Vergata, Sezione INFN, Roma, Italy
Universitá di Catania, Sezione INFN, Catania, Italy
Universitá di Torino, Sezione INFN, Torino, Italy
Dipartimento di Ingegneria DellInnovazione DellUniversitá Del Salento, Sezione INFN, Lecce, Italy
Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo (INAF), Palermo, Italy
Istituto di Fisica Dello Spazio Interplanetario (INAF), Universitá di Torino, Sezione INFN, Torino, Italy
INFN, Laboratori Nazionali Del Gran Sasso, Assergi (LAquila), Italy
Universitá di Palermo, Sezione INFN, Catania, Italy
Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
Centro de Investigación y de Estudios Avanzados Del IPN (CINVESTAV), México, D.F., Mexico
Universidad Michoacana de San Nicolas de Hidalgo, Morelia, Michoacan, Mexico
Universidad Nacional Autonoma de Mexico, Mexico, D.F., Mexico
IMAPP, Radboud University, Nijmegen, Netherlands
Kernfysisch Versneller Instituut, University of Groningen, Groningen, Netherlands
NIKHEF, Amsterdam, Netherlands
ASTRON, Dwingeloo, Netherlands
Institute of Nuclear Physics, PAN, Krakow, Poland
University of Lódź, Lódź, Poland
LIP, Instituto Superior Técnico, Lisboa, Portugal
J. Stefan Institute, Ljubljana, Slovenia
Laboratory for Astroparticle Physics, University of Nova Gorica, Slovenia
Instituto de Física Corpuscular, CSIC-Universitat de Valéncia, Valencia, Spain
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
Rudolf Peierls Centre for Theoretical Physics, University of Oxford, Oxford, United Kingdom
School of Physics and Astronomy, University of Leeds, United Kingdom
Argonne National Laboratory, Argonne, IL, United States
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
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
Southern University, Baton Rouge, LA, United States
University of Chicago, Enrico Fermi Institute, Chicago, IL, United States
University of Nebraska, Lincoln, NE, United States
University of New Mexico, Albuquerque, NM, United States
University of Wisconsin, Madison, WI, United States
University of Wisconsin, Milwaukee, WI, United States
Institute for Nuclear Science and Technology (INST), Hanoi, Viet Nam
Palabras clave:cosmic ray experiments; ultra high energy cosmic rays
Año:2011
Volumen:2011
Número:6
DOI: http://dx.doi.org/10.1088/1475-7516/2011/06/022
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_v2011_n6_p_Multitudinario

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Citas:

---------- APA ----------
(2011) . Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory. Journal of Cosmology and Astroparticle Physics, 2011(6).
http://dx.doi.org/10.1088/1475-7516/2011/06/022
---------- CHICAGO ----------
Multitudinario:493. "Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory" . Journal of Cosmology and Astroparticle Physics 2011, no. 6 (2011).
http://dx.doi.org/10.1088/1475-7516/2011/06/022
---------- MLA ----------
Multitudinario:493. "Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory" . Journal of Cosmology and Astroparticle Physics, vol. 2011, no. 6, 2011.
http://dx.doi.org/10.1088/1475-7516/2011/06/022
---------- VANCOUVER ----------
Multitudinario:493. Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory. J. Cosmol. Astroparticle Phys. 2011;2011(6).
http://dx.doi.org/10.1088/1475-7516/2011/06/022