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Features of the energy spectrum of cosmic rays above 2.5��1018 eV using the pierre auger observatory
descriptionPublicationkeyboard_double_arrow_right Article 2020 France, Germany, Colombia, Colombia Publisher:American Physical Society (APS)
Authors: Pierre Auger Collaboration; Aab, A.; Abreu, P.; Aglietta, M.; +196 Authors
Pierre Auger Collaboration; Aab, A.; Abreu, P.; Aglietta, M.; Albury, J. M.; Allekotte, I.; Almela, A.; Alvarez Castillo, J.; Alvarez-Muñiz, J.; Alves Batista, R.; Anastasi, G. A.; Anchordoqui, L.; Andrada, B.; Andringa, S.; Aramo, C.; Araújo Ferreira, P. R.; Asorey, H.; Assis, P.; Avila, G.; Badescu, A. M.; Bakalova, A.; Balaceanu, A.; Barbato, F.; Barreira Luz, R. J.; 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.; Bonneau Arbeletche, L.; 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.; Cobos Cerutti, A. C.; 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.; Almeida, R. M. de; Jesús, J. de; Jong, S. J. de; De Mauro, G.; Mello Neto, J. R. T. de; De Mitri, I.; Oliveira, J. de; Oliveira Franco, D. de; Souza, V. de; De Vito, E.; Debatin, J.; Río, M. del; Deligny, O.; Dembinski, H.; Dhital, N.; Di Giulio, C.; Di Matteo, A.; Díaz Castro, M. L.; 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.; Garcia Vegas, A. L.; Gemmeke, H.; Gesualdi, F.; Gherghel-Lascu, A.; Ghia, P. L.; Giaccari, U.; Giammarchi, M.; Giller, M.; Glombitza, J.; Gobbi, F.; Gollan, F.; Golup, G.; Gómez Berisso, M.; Gómez Vitale, P. F.; 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.; Kukec Mezek, G.; Lago, B. L.; LaHurd, D.; Lang, R. G.; Leigui de Oliveira, M. A.; Lenok, V.; Letessier-Selvon, A.; Lhenry-Yvon, I.; Lo Presti, D.; Lopes, L.; López, R.; Lorek, R.; Luce, Q.; Lucero, A.; Machado Payeras, A.; Malacari, M.; Mancarella, G.; Mandat, D.; Manning, B. C.; Manshanden, J.; Mantsch, P.; Marafico, S.;
doi: 10.5445/ir/1000125497
pmid: 33016715
handle: 11407/5957
doi: 10.5445/ir/1000125497
pmid: 33016715
handle: 11407/5957
We report a measurement of the energy spectrum of cosmic rays above 2.5��10$^{18}$ eV based on 215 030 events. New results are presented: at about 1.3��10$^{19}$ eV, the spectral index changes from 2.51��0.03(stat)��0.05(syst) to 3.05��0.05(stat)��0.10(syst), evolving to 5.1��0.3(stat)��0.1(syst) beyond 5��10$^{19}$ eV, while no significant dependence of spectral features on the declination is seen in the accessible range. These features of the spectrum can be reproduced in models with energy-dependent mass composition. The energy density in cosmic rays above 5��10$^{18}$ eV is [5.66��0.03(stat)��1.40(syst)]��10$^{53}$ erg Mpc$^{-3}$.
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Physical Review Letters
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HAL-IN2P3 (Institut national de physique nucléaire et de physique des particules)
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Université Grenoble Alpes: HAL
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Features of the energy spectrum of cosmic rays above 2.5��1018 eV using the pierre auger observatory
descriptionPublicationkeyboard_double_arrow_right Article 2020 France, Germany, Colombia, Colombia Publisher:American Physical Society (APS)
Authors: Pierre Auger Collaboration; Aab, A.; Abreu, P.; Aglietta, M.; +196 Authors
Pierre Auger Collaboration; Aab, A.; Abreu, P.; Aglietta, M.; Albury, J. M.; Allekotte, I.; Almela, A.; Alvarez Castillo, J.; Alvarez-Muñiz, J.; Alves Batista, R.; Anastasi, G. A.; Anchordoqui, L.; Andrada, B.; Andringa, S.; Aramo, C.; Araújo Ferreira, P. R.; Asorey, H.; Assis, P.; Avila, G.; Badescu, A. M.; Bakalova, A.; Balaceanu, A.; Barbato, F.; Barreira Luz, R. J.; 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.; Bonneau Arbeletche, L.; 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.; Cobos Cerutti, A. C.; 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.; Almeida, R. M. de; Jesús, J. de; Jong, S. J. de; De Mauro, G.; Mello Neto, J. R. T. de; De Mitri, I.; Oliveira, J. de; Oliveira Franco, D. de; Souza, V. de; De Vito, E.; Debatin, J.; Río, M. del; Deligny, O.; Dembinski, H.; Dhital, N.; Di Giulio, C.; Di Matteo, A.; Díaz Castro, M. L.; 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.; Garcia Vegas, A. L.; Gemmeke, H.; Gesualdi, F.; Gherghel-Lascu, A.; Ghia, P. L.; Giaccari, U.; Giammarchi, M.; Giller, M.; Glombitza, J.; Gobbi, F.; Gollan, F.; Golup, G.; Gómez Berisso, M.; Gómez Vitale, P. F.; 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.; Kukec Mezek, G.; Lago, B. L.; LaHurd, D.; Lang, R. G.; Leigui de Oliveira, M. A.; Lenok, V.; Letessier-Selvon, A.; Lhenry-Yvon, I.; Lo Presti, D.; Lopes, L.; López, R.; Lorek, R.; Luce, Q.; Lucero, A.; Machado Payeras, A.; Malacari, M.; Mancarella, G.; Mandat, D.; Manning, B. C.; Manshanden, J.; Mantsch, P.; Marafico, S.;
doi: 10.5445/ir/1000125497
pmid: 33016715
handle: 11407/5957
doi: 10.5445/ir/1000125497
pmid: 33016715
handle: 11407/5957
We report a measurement of the energy spectrum of cosmic rays above 2.5��10$^{18}$ eV based on 215 030 events. New results are presented: at about 1.3��10$^{19}$ eV, the spectral index changes from 2.51��0.03(stat)��0.05(syst) to 3.05��0.05(stat)��0.10(syst), evolving to 5.1��0.3(stat)��0.1(syst) beyond 5��10$^{19}$ eV, while no significant dependence of spectral features on the declination is seen in the accessible range. These features of the spectrum can be reproduced in models with energy-dependent mass composition. The energy density in cosmic rays above 5��10$^{18}$ eV is [5.66��0.03(stat)��1.40(syst)]��10$^{53}$ erg Mpc$^{-3}$.
downloaddonwloadFull-Text
KITopen (Karlsruhe I...arrow_drop_down
KITopen (Karlsruhe Institute of Technologie)
Article . 2020
License: CC BY
Full-Text: https://publikationen.bibliothek.kit.edu/1000125497
Data sources: Bielefeld Academic Search Engine (BASE)
https://dx.doi.org/10.5445/ir/...
Article . 2020
License: CC BY
Data sources: Datacite
Hyper Article en Ligne
Article . 2020
Data sources: Hyper Article en Ligne
Mémoires en Sciences de l'Information et de la Communication
Article . 2020
Data sources: Mémoires en Sciences de l'Information et de la Communication
Universidad de Medellin: Repositorio Institucional
Article . 2021
Data sources: Bielefeld Academic Search Engine (BASE)
Physical Review Letters
Article
Data sources: Europe PubMed Central
HAL-IN2P3 (Institut national de physique nucléaire et de physique des particules)
Article . 2020
Data sources: Bielefeld Academic Search Engine (BASE)
Université Grenoble Alpes: HAL
Article . 2020
Data sources: Bielefeld Academic Search Engine (BASE)
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citeCite
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citations 68
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impulse Top 1%
Powered by BIP!
more_vert
downloaddonwloadFull-Text
KITopen (Karlsruhe I...arrow_drop_down
KITopen (Karlsruhe Institute of Technologie)
Article . 2020
License: CC BY
Full-Text: https://publikationen.bibliothek.kit.edu/1000125497
Data sources: Bielefeld Academic Search Engine (BASE)
https://dx.doi.org/10.5445/ir/...
Article . 2020
License: CC BY
Data sources: Datacite
Hyper Article en Ligne
Article . 2020
Data sources: Hyper Article en Ligne
Mémoires en Sciences de l'Information et de la Communication
Article . 2020
Data sources: Mémoires en Sciences de l'Information et de la Communication
Universidad de Medellin: Repositorio Institucional
Article . 2021
Data sources: Bielefeld Academic Search Engine (BASE)
Physical Review Letters
Article
Data sources: Europe PubMed Central
HAL-IN2P3 (Institut national de physique nucléaire et de physique des particules)
Article . 2020
Data sources: Bielefeld Academic Search Engine (BASE)
Université Grenoble Alpes: HAL
Article . 2020
Data sources: Bielefeld Academic Search Engine (BASE)
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Features of the energy spectrum of cosmic rays above 2.5��1018 eV using the pierre auger observatory

Features of the energy spectrum of cosmic rays above 2.5��1018 eV using the pierre auger observatory

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Features of the energy spectrum of cosmic rays above 2.5��1018 eV using the pierre auger observatory

Energy Research
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