Observation of the Suppression of the Flux of Cosmic Rays above 4 × 10¹⁹ eV

The energy spectrum of cosmic rays above 2.5 × 10¹⁸ eV, derived from 20,000 events recorded at the Pierre Auger Observatory, is described. The spectral index γ of the particle flux, J ∝ E<sup>-γ</sup>, at energies between 4 × 10¹⁸ eV and 4 × 10¹⁹ eV is 2.69 ± 0.02(stat) ± 0.06(syst), ste...

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Autores principales: Badagnani, Daniel Omar, Dova, María Teresa, Epele, Luis Nicolás, Gómez Albarracín, Flavia Alejandra, Grunfeld, Christian Martín, Hansen, Patricia María, Manceñido, Mónica E., Mariazzi, Analisa Gabriela, Moreno, Juan Cruz, Sciutto, Sergio Juan, Tarutina, Tatiana, Tueros, Matías Jorge, Veiga, Alejandro Luis, Wahlberg, Hernán Pablo, The Pierre Auger Collaboration
Formato: Articulo
Lenguaje:Inglés
Publicado: 2008
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/126615
Aporte de:
id I19-R120-10915-126615
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Exactas
Física
energy spectrum
cosmic rays
spectral index
particle flux
spellingShingle Ciencias Exactas
Física
energy spectrum
cosmic rays
spectral index
particle flux
Badagnani, Daniel Omar
Dova, María Teresa
Epele, Luis Nicolás
Gómez Albarracín, Flavia Alejandra
Grunfeld, Christian Martín
Hansen, Patricia María
Manceñido, Mónica E.
Mariazzi, Analisa Gabriela
Moreno, Juan Cruz
Sciutto, Sergio Juan
Tarutina, Tatiana
Tueros, Matías Jorge
Veiga, Alejandro Luis
Wahlberg, Hernán Pablo
The Pierre Auger Collaboration
Observation of the Suppression of the Flux of Cosmic Rays above 4 × 10¹⁹ eV
topic_facet Ciencias Exactas
Física
energy spectrum
cosmic rays
spectral index
particle flux
description The energy spectrum of cosmic rays above 2.5 × 10¹⁸ eV, derived from 20,000 events recorded at the Pierre Auger Observatory, is described. The spectral index γ of the particle flux, J ∝ E<sup>-γ</sup>, at energies between 4 × 10¹⁸ eV and 4 × 10¹⁹ eV is 2.69 ± 0.02(stat) ± 0.06(syst), steepening to 4.2 ± 0.4(stat) ± 0.06(syst) at higher energies. The hypothesis of a single power law is rejected with a significance greater than 6 standard deviations. The data are consistent with the prediction by Greisen and by Zatsepin and Kuz'min.
format Articulo
Articulo
author Badagnani, Daniel Omar
Dova, María Teresa
Epele, Luis Nicolás
Gómez Albarracín, Flavia Alejandra
Grunfeld, Christian Martín
Hansen, Patricia María
Manceñido, Mónica E.
Mariazzi, Analisa Gabriela
Moreno, Juan Cruz
Sciutto, Sergio Juan
Tarutina, Tatiana
Tueros, Matías Jorge
Veiga, Alejandro Luis
Wahlberg, Hernán Pablo
The Pierre Auger Collaboration
author_facet Badagnani, Daniel Omar
Dova, María Teresa
Epele, Luis Nicolás
Gómez Albarracín, Flavia Alejandra
Grunfeld, Christian Martín
Hansen, Patricia María
Manceñido, Mónica E.
Mariazzi, Analisa Gabriela
Moreno, Juan Cruz
Sciutto, Sergio Juan
Tarutina, Tatiana
Tueros, Matías Jorge
Veiga, Alejandro Luis
Wahlberg, Hernán Pablo
The Pierre Auger Collaboration
author_sort Badagnani, Daniel Omar
title Observation of the Suppression of the Flux of Cosmic Rays above 4 × 10¹⁹ eV
title_short Observation of the Suppression of the Flux of Cosmic Rays above 4 × 10¹⁹ eV
title_full Observation of the Suppression of the Flux of Cosmic Rays above 4 × 10¹⁹ eV
title_fullStr Observation of the Suppression of the Flux of Cosmic Rays above 4 × 10¹⁹ eV
title_full_unstemmed Observation of the Suppression of the Flux of Cosmic Rays above 4 × 10¹⁹ eV
title_sort observation of the suppression of the flux of cosmic rays above 4 × 10¹⁹ ev
publishDate 2008
url http://sedici.unlp.edu.ar/handle/10915/126615
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