Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory
We present a detailed study of the large-scale anisotropies of cosmic rays with energies above 4 EeV measured using the Pierre Auger Observatory. For the energy bins [4,8] EeV and E ≥ 8 EeV, the most significant signal is a dipolar modulation in right ascension at energies above 8 EeV, as previousl...
Autores principales: | , , , , , , , , |
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Formato: | Articulo |
Lenguaje: | Inglés |
Publicado: |
2018
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Materias: | |
Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/125623 |
Aporte de: |
id |
I19-R120-10915-125623 |
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record_format |
dspace |
institution |
Universidad Nacional de La Plata |
institution_str |
I-19 |
repository_str |
R-120 |
collection |
SEDICI (UNLP) |
language |
Inglés |
topic |
Física Cosmic ray Physics Dipole Amplitude Pierre auger observatory Context (language use) Astrophysics Cosmic cancer database Right ascension Anisotropy Observatory Auger Astroparticle physics |
spellingShingle |
Física Cosmic ray Physics Dipole Amplitude Pierre auger observatory Context (language use) Astrophysics Cosmic cancer database Right ascension Anisotropy Observatory Auger Astroparticle physics Calcagni, Laura Randa Dova, María Teresa Hansen, Patricia María Mariazzi, Analisa Gabriela Sciutto, Sergio Juan Tueros, Matías Jorge Vergara Quispe, Indira Dajhana Wahlberg, Hernán Pablo The Pierre Auger Collaboration Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory |
topic_facet |
Física Cosmic ray Physics Dipole Amplitude Pierre auger observatory Context (language use) Astrophysics Cosmic cancer database Right ascension Anisotropy Observatory Auger Astroparticle physics |
description |
We present a detailed study of the large-scale anisotropies of cosmic rays with energies above 4 EeV measured using the Pierre Auger Observatory. For the energy bins [4,8] EeV and E ≥ 8 EeV, the most significant signal is a dipolar modulation in right ascension at energies above 8 EeV, as previously reported. In this paper we further scrutinize the highest-energy bin by splitting it into three energy ranges. We find that the amplitude of the dipole increases with energy above 4 EeV. The growth can be fitted with a power law with index β=0.79 ± 0.19. The directions of the dipoles are consistent with an extragalactic origin of these anisotropies at all the energies considered. Additionally we have estimated the quadrupolar components of the anisotropy: they are not statistically significant. We discuss the results in the context of the predictions from different models for the distribution of ultrahigh-energy sources and cosmic magnetic fields. |
format |
Articulo Articulo |
author |
Calcagni, Laura Randa Dova, María Teresa Hansen, Patricia María Mariazzi, Analisa Gabriela Sciutto, Sergio Juan Tueros, Matías Jorge Vergara Quispe, Indira Dajhana Wahlberg, Hernán Pablo The Pierre Auger Collaboration |
author_facet |
Calcagni, Laura Randa Dova, María Teresa Hansen, Patricia María Mariazzi, Analisa Gabriela Sciutto, Sergio Juan Tueros, Matías Jorge Vergara Quispe, Indira Dajhana Wahlberg, Hernán Pablo The Pierre Auger Collaboration |
author_sort |
Calcagni, Laura Randa |
title |
Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory |
title_short |
Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory |
title_full |
Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory |
title_fullStr |
Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory |
title_full_unstemmed |
Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory |
title_sort |
large-scale cosmic-ray anisotropies above 4 eev measured by the pierre auger observatory |
publishDate |
2018 |
url |
http://sedici.unlp.edu.ar/handle/10915/125623 |
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Repositorios |
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1764820451955048450 |