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Features of the energy spectrum of cosmic rays above $2.5{\times} 10^{18}$ eV using the Pierre Auger Observatory

descriptionPublicationkeyboard_double_arrow_right Research , Article , Preprint , Other literature type 01 Jan 2020Embargo end date: 01 Jan 2020 English Publisher:RWTH Aachen UniversityJournal:Physical Review Letters, volume 125, page 121,106 (issn: 0031-9007,

Authors: The Pierre Auger Collaboration; Aab, A.; Abreu, P.; Aglietta, M.; Albury, J. M.; Allekotte, I.; Almela, A.; +193 Authors

The Pierre Auger Collaboration; Aab, A.; Abreu, P.; Aglietta, M.; Albury, J. M.; Allekotte, I.; Almela, A.; Castillo, J. Alvarez; Alvarez-Muñiz, J.; Batista, R. Alves; Anastasi, G. A.; Anchordoqui, L.; Andrada, B.; Andringa, S.; Aramo, C.; Ferreira, P. R. Araújo; Asorey, H.; Assis, P.; Avila, G.; Badescu, A. M.; Bakalova, A.; Balaceanu, A.; Barbato, F.; Luz, R. J. Barreira; Becker, K. H.; Bellido, J. A.; Berat, C.; Bertaina, M. E.; Bertou, X.; Biermann, P. L.; Bister, T.; Biteau, J.; Blanco, A.; Blazek, J.; Bleve, C.; Boháčová, M.; Boncioli, D.; Bonifazi, C.; Arbeletche, L. Bonneau; Borodai, N.; Botti, A. M.; Brack, J.; Bretz, T.; Briechle, F. L.; Buchholz, P.; Bueno, A.; Buitink, S.; Buscemi, M.; Caballero-Mora, K. S.; Caccianiga, L.; Calcagni, L.; Cancio, A.; Canfora, F.; Caracas, I.; Carceller, J. M.; Caruso, R.; Castellina, A.; Catalani, F.; Cataldi, G.; Cazon, L.; Cerda, M.; Chinellato, J. A.; Choi, K.; Chudoba, J.; Chytka, L.; Clay, R. W.; Cerutti, A. C. Cobos; Colalillo, R.; Coleman, A.; Coluccia, M. R.; Conceição, R.; Condorelli, A.; Consolati, G.; Contreras, F.; Convenga, F.; Covault, C. E.; Dasso, S.; Daumiller, K.; Dawson, B. R.; Day, J. A.; de Almeida, R. M.; de Jesús, J.; de Jong, S. J.; De Mauro, G.; Neto, J. R. T. de Mello; De Mitri, I.; de Oliveira, J.; Franco, D. de Oliveira; de Souza, V.; De Vito, E.; Debatin, J.; del Río, M.; Deligny, O.; Dembinski, H.; Dhital, N.; Di Giulio, C.; Di Matteo, A.; Castro, M. L. Díaz; Dobrigkeit, C.; D'Olivo, J. C.; Dorosti, Q.; Anjos, R. C. dos; Dova, M. T.; Ebr, J.; Engel, R.; Epicoco, I.; Erdmann, M.; Escobar, C. O.; Etchegoyen, A.; Falcke, H.; Farmer, J.; Farrar, G.; Fauth, A. C.; Fazzini, N.; Feldbusch, F.; Fenu, F.; Fick, B.; Figueira, J. M.; Filipčič, A.; Fodran, T.; Freire, M. M.; Fujii, T.; Fuster, A.; Galea, C.; Galelli, C.; García, B.; Vegas, A. L. Garcia; Gemmeke, H.; Gesualdi, F.; Gherghel-Lascu, A.; Ghia, P. L.; Giaccari, U.; Giammarchi, M.; Giller, M.; Glombitza, J.; Gobbi, F.; Gollan, F.; Golup, G.; Berisso, M. Gómez; Vitale, P. F. Gómez; Gongora, J. P.; González, N.; Goos, I.; Góra, D.; Gorgi, A.; Gottowik, M.; Grubb, T. D.; Guarino, F.; Guedes, G. P.; Guido, E.; Hahn, S.; Halliday, R.; Hampel, M. R.; Hansen, P.; Harari, D.; Harvey, V. M.; Haungs, A.; Hebbeker, T.; Heck, D.; Hill, G. C.; Hojvat, C.; Hörandel, J. R.; Horvath, P.; Hrabovský, M.; Huege, T.; Hulsman, J.; Insolia, A.; Isar, P. G.; Johnsen, J. A.; Jurysek, J.; Kääpä, A.; Kampert, K. H.; Keilhauer, B.; Kemp, J.; Klages, H. O.; Kleifges, M.; Kleinfeller, J.; Köpke, M.; Mezek, G. Kukec; Lago, B. L.; LaHurd, D.; Lang, R. G.; de Oliveira, M. A. Leigui; Lenok, V.; Letessier-Selvon, A.; Lhenry-Yvon, I.; Presti, D. Lo; Lopes, L.; López, R.; Lorek, R.; Luce, Q.; Lucero, A.; Payeras, A. Machado; Malacari, M.; Mancarella, G.; Mandat, D.; Manning, B. C.; Manshanden, J.; Mantsch, P.; Marafico, S.;

doi: 10.18154/rwth-2020-10166 , 10.18154/rwth-2020-10131 , 10.48550/arxiv.2008.06488

arXiv: 2008.06488

Features of the energy spectrum of cosmic rays above $2.5{\times} 10^{18}$ eV using the Pierre Auger Observatory

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Abstract

Physical review letters 125(12), 121106 (2020). doi:10.1103/PhysRevLett.125.121106

Published by APS, College Park, Md.

Related Organizations

Universities Space Research Association
United States
Universities Space Research Association
United States

Keywords

High Energy Astrophysical Phenomena (astro-ph.HE), cosmic radiation: energy spectrum, FOS: Physical sciences, power spectrum, 530, Auger, energy dependence, mass spectrum, observatory, 5/3, spectral, energy: density, Astrophysics - High Energy Astrophysical Phenomena

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	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Top 10%