Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
- Autores
- Dova, María Teresa; Hansen, Patricia María; Jarne, Cecilia Gisele; Mariazzi, Analisa Gabriela; Sciutto, Sergio Juan; Wahlberg, Hernán Pablo; The ATLAS Collaboration
- Año de publicación
- 2015
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Energy-dependent patterns in the arrival directions of cosmic rays are searched for using data of the Pierre Auger Observatory. We investigate local regions around the highest-energy cosmic rays with E ≥ 6×1019 eV by analyzing cosmic rays with energies above E ≥ 5×1018 eV arriving within an angular separation of approximately 15º. We characterize the energy distributions inside these regions by two independent methods, one searching for angular dependence of energy-energy correlations and one searching for collimation of energy along the local system of principal axes of the energy distribution. No significant patterns are found with this analysis. The comparison of these measurements with astrophysical scenarios can therefore be used to obtain constraints on related model parameters such as strength of cosmic-ray deflection and density of point sources.
Facultad de Ciencias Exactas - Materia
-
Ciencias Exactas
Física
Radiación cósmica
Astrofísica
Pierre Auger Observatory - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/81264
Ver los metadatos del registro completo
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Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger ObservatoryDova, María TeresaHansen, Patricia MaríaJarne, Cecilia GiseleMariazzi, Analisa GabrielaSciutto, Sergio JuanWahlberg, Hernán PabloThe ATLAS CollaborationCiencias ExactasFísicaRadiación cósmicaAstrofísicaPierre Auger ObservatoryEnergy-dependent patterns in the arrival directions of cosmic rays are searched for using data of the Pierre Auger Observatory. We investigate local regions around the highest-energy cosmic rays with E ≥ 6×10<sup>19</sup> eV by analyzing cosmic rays with energies above E ≥ 5×10<sup>18</sup> eV arriving within an angular separation of approximately 15º. We characterize the energy distributions inside these regions by two independent methods, one searching for angular dependence of energy-energy correlations and one searching for collimation of energy along the local system of principal axes of the energy distribution. No significant patterns are found with this analysis. The comparison of these measurements with astrophysical scenarios can therefore be used to obtain constraints on related model parameters such as strength of cosmic-ray deflection and density of point sources.Facultad de Ciencias Exactas2015-06-20info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/81264enginfo:eu-repo/semantics/altIdentifier/issn/1434-6052info:eu-repo/semantics/altIdentifier/doi/10.1140/epjc/s10052-015-3471-0info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/4.0/Creative Commons Attribution 4.0 International (CC BY 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-03T10:47:22Zoai:sedici.unlp.edu.ar:10915/81264Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-03 10:47:22.815SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory |
title |
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory |
spellingShingle |
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory Dova, María Teresa Ciencias Exactas Física Radiación cósmica Astrofísica Pierre Auger Observatory |
title_short |
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory |
title_full |
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory |
title_fullStr |
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory |
title_full_unstemmed |
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory |
title_sort |
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory |
dc.creator.none.fl_str_mv |
Dova, María Teresa Hansen, Patricia María Jarne, Cecilia Gisele Mariazzi, Analisa Gabriela Sciutto, Sergio Juan Wahlberg, Hernán Pablo The ATLAS Collaboration |
author |
Dova, María Teresa |
author_facet |
Dova, María Teresa Hansen, Patricia María Jarne, Cecilia Gisele Mariazzi, Analisa Gabriela Sciutto, Sergio Juan Wahlberg, Hernán Pablo The ATLAS Collaboration |
author_role |
author |
author2 |
Hansen, Patricia María Jarne, Cecilia Gisele Mariazzi, Analisa Gabriela Sciutto, Sergio Juan Wahlberg, Hernán Pablo The ATLAS Collaboration |
author2_role |
author author author author author author |
dc.subject.none.fl_str_mv |
Ciencias Exactas Física Radiación cósmica Astrofísica Pierre Auger Observatory |
topic |
Ciencias Exactas Física Radiación cósmica Astrofísica Pierre Auger Observatory |
dc.description.none.fl_txt_mv |
Energy-dependent patterns in the arrival directions of cosmic rays are searched for using data of the Pierre Auger Observatory. We investigate local regions around the highest-energy cosmic rays with E ≥ 6×10<sup>19</sup> eV by analyzing cosmic rays with energies above E ≥ 5×10<sup>18</sup> eV arriving within an angular separation of approximately 15º. We characterize the energy distributions inside these regions by two independent methods, one searching for angular dependence of energy-energy correlations and one searching for collimation of energy along the local system of principal axes of the energy distribution. No significant patterns are found with this analysis. The comparison of these measurements with astrophysical scenarios can therefore be used to obtain constraints on related model parameters such as strength of cosmic-ray deflection and density of point sources. Facultad de Ciencias Exactas |
description |
Energy-dependent patterns in the arrival directions of cosmic rays are searched for using data of the Pierre Auger Observatory. We investigate local regions around the highest-energy cosmic rays with E ≥ 6×10<sup>19</sup> eV by analyzing cosmic rays with energies above E ≥ 5×10<sup>18</sup> eV arriving within an angular separation of approximately 15º. We characterize the energy distributions inside these regions by two independent methods, one searching for angular dependence of energy-energy correlations and one searching for collimation of energy along the local system of principal axes of the energy distribution. No significant patterns are found with this analysis. The comparison of these measurements with astrophysical scenarios can therefore be used to obtain constraints on related model parameters such as strength of cosmic-ray deflection and density of point sources. |
publishDate |
2015 |
dc.date.none.fl_str_mv |
2015-06-20 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://sedici.unlp.edu.ar/handle/10915/81264 |
url |
http://sedici.unlp.edu.ar/handle/10915/81264 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/1434-6052 info:eu-repo/semantics/altIdentifier/doi/10.1140/epjc/s10052-015-3471-0 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/4.0/ Creative Commons Attribution 4.0 International (CC BY 4.0) |
eu_rights_str_mv |
openAccess |
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http://creativecommons.org/licenses/by/4.0/ Creative Commons Attribution 4.0 International (CC BY 4.0) |
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application/pdf |
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Universidad Nacional de La Plata |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
repository.mail.fl_str_mv |
alira@sedici.unlp.edu.ar |
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