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Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy.
Aab, A; Abreu, P; Aglietta, M; Ahn, E J; Al Samarai, I; Albuquerque, I F M; Allekotte, I; Allison, P; Almela, A; Alvarez Castillo, J; Alvarez-Muñiz, J; Alves Batista, R; Ambrosio, M; Aminaei, A; Anastasi, G A; Anchordoqui, L; Andringa, S; Aramo, C; Arqueros, F; Arsene, N; Asorey, H; Assis, P; Aublin, J; Avila, G; Awal, N; Badescu, A M; 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 G; Blanco, A; Blanco, M; Blazek, J; Bleve, C; Blümer, H; Bohácová, M; Boncioli, D; Bonifazi, C; Borodai, N; Brack, J; Brancus, I; Bretz, T; Bridgeman, A; Brogueira, P.
Afiliação
  • Aab A; Universität Siegen, Fachbereich 7 Physik - Experimentelle Teilchenphysik, Siegen, Germany.
  • Abreu P; Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisboa, Portugal.
  • Aglietta M; Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy.
  • Ahn EJ; Fermilab, Batavia, Illinois, USA.
  • Al Samarai I; Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France.
  • Albuquerque IF; Universidade de São Paulo, Instituto de Física, São Paulo, São Paulo, Brazil.
  • Allekotte I; Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina.
  • Allison P; Ohio State University, Columbus, Ohio, USA.
  • Almela A; Universidad Tecnológica Nacional - Facultad Regional Buenos Aires, Buenos Aires, Argentina.
  • Alvarez Castillo J; Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina.
  • Alvarez-Muñiz J; Universidad Nacional Autónoma de México, México, Distrito Federal, Mexico.
  • Alves Batista R; Universidad de Santiago de Compostela, Santiago de Compostela, Spain.
  • Ambrosio M; Universität Hamburg, II. Institut für Theoretische Physik, Hamburg, Germany.
  • Aminaei A; Università di Napoli "Federico II" and Sezione INFN, Napoli, Italy.
  • Anastasi GA; IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands.
  • Anchordoqui L; Università di Catania and Sezione INFN, Catania, Italy.
  • Andringa S; Department of Physics and Astronomy, Lehman College, City University of New York, Bronx, New York, USA.
  • Aramo C; Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisboa, Portugal.
  • Arqueros F; Università di Napoli "Federico II" and Sezione INFN, Napoli, Italy.
  • Arsene N; Universidad Complutense de Madrid, Madrid, Spain.
  • Asorey H; University of Bucharest, Physics Department, Bucharest, Romania.
  • Assis P; Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina.
  • Aublin J; Universidad Industrial de Santander, Bucaramanga, Colombia.
  • Avila G; Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisboa, Portugal.
  • Awal N; Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France.
  • Badescu AM; Observatorio Pierre Auger and Comisión Nacional de Energía Atómica, Malargüe, Argentina.
  • Baus C; New York University, New York, New York, USA.
  • Beatty JJ; University Politehnica of Bucharest, Bucharest, Romania.
  • Becker KH; Karlsruhe Institute of Technology, Institut für Experimentelle Kernphysik (IEKP), Karlsruhe, Germany.
  • Bellido JA; Ohio State University, Columbus, Ohio, USA.
  • Berat C; Bergische Universität Wuppertal, Fachbereich C - Physik, Wuppertal, Germany.
  • Bertaina ME; University of Adelaide, Adelaide, South Australia, Australia.
  • Bertou X; Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France.
  • Biermann PL; Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy.
  • Billoir P; Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina.
  • Blaess SG; Max-Planck-Institut für Radioastronomie, Bonn, Germany.
  • Blanco A; Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France.
  • Blanco M; University of Adelaide, Adelaide, South Australia, Australia.
  • Blazek J; Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisboa, Portugal.
  • Bleve C; Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France.
  • Blümer H; Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic.
  • Bohácová M; Dipartimento di Matematica e Fisica "E. De Giorgi" dell'Università del Salento and Sezione INFN, Lecce, Italy.
  • Boncioli D; Karlsruhe Institute of Technology, Institut für Experimentelle Kernphysik (IEKP), Karlsruhe, Germany.
  • Bonifazi C; Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany.
  • Borodai N; Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic.
  • Brack J; INFN, Laboratori Nazionali del Gran Sasso, Assergi (L'Aquila), Italy.
  • Brancus I; Universidade Federal do Rio de Janeiro, Instituto de Física, Rio de Janeiro, Rio de Janeiro, Brazil.
  • Bretz T; Institute of Nuclear Physics PAN, Krakow, Poland.
  • Bridgeman A; Colorado State University, Fort Collins, Colorado, USA.
  • Brogueira P; "Horia Hulubei" National Institute for Physics and Nuclear Engineering, Bucharest-Magurele, Romania.
Phys Rev Lett ; 116(24): 241101, 2016 Jun 17.
Article em En | MEDLINE | ID: mdl-27367377
ABSTRACT
We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8±0.7(stat)±6.7(syst) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principles calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the direct calibration of any cosmic-ray radio detector against the well-established energy scale of the Pierre Auger Observatory.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Phys Rev Lett Ano de publicação: 2016 Tipo de documento: Article País de afiliação: Alemanha

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Phys Rev Lett Ano de publicação: 2016 Tipo de documento: Article País de afiliação: Alemanha