Highest energy particle physics with the Pierre Auger Observatory
- Autores
- Mariazzi, Analisa Gabriela
- Año de publicación
- 2014
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Astroparticles offer a new path for research in the field of particle physics, allowing investigations at energies above those accesible with accelerators. Ultra-high energy cosmic rays can be studied via the observation of the showers they generate in the atmosphere. The Pierre Auger Observatory is a hybrid detector for ultra-high energy cosmic rays, combining two complementary measurement techniques used by previous experiments, to get the best possible measurements of these air showers. Shower observations enable one to not only estimate the energy, direction and most probable mass of the primary cosmic particles but also to obtain some information about the properties of their hadronic interactions. Results that are most relevant in the context of determining hadronic interaction characteristics at ultra-high energies will be presented.
Facultad de Ciencias Exactas - Materia
-
Ciencias Exactas
Astronomía
Cosmic rays
Extensive air showers
Hadronic interactions - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/123401
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Highest energy particle physics with the Pierre Auger ObservatoryMariazzi, Analisa GabrielaCiencias ExactasAstronomíaCosmic raysExtensive air showersHadronic interactionsAstroparticles offer a new path for research in the field of particle physics, allowing investigations at energies above those accesible with accelerators. Ultra-high energy cosmic rays can be studied via the observation of the showers they generate in the atmosphere. The Pierre Auger Observatory is a hybrid detector for ultra-high energy cosmic rays, combining two complementary measurement techniques used by previous experiments, to get the best possible measurements of these air showers. Shower observations enable one to not only estimate the energy, direction and most probable mass of the primary cosmic particles but also to obtain some information about the properties of their hadronic interactions. Results that are most relevant in the context of determining hadronic interaction characteristics at ultra-high energies will be presented.Facultad de Ciencias Exactas2014-05-19info: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/10915/123401enginfo:eu-repo/semantics/altIdentifier/issn/2010-1945info:eu-repo/semantics/altIdentifier/arxiv/1403.1181info:eu-repo/semantics/altIdentifier/doi/10.1142/s2010194514603019info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:29:24Zoai:sedici.unlp.edu.ar:10915/123401Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:29:24.719SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Highest energy particle physics with the Pierre Auger Observatory |
title |
Highest energy particle physics with the Pierre Auger Observatory |
spellingShingle |
Highest energy particle physics with the Pierre Auger Observatory Mariazzi, Analisa Gabriela Ciencias Exactas Astronomía Cosmic rays Extensive air showers Hadronic interactions |
title_short |
Highest energy particle physics with the Pierre Auger Observatory |
title_full |
Highest energy particle physics with the Pierre Auger Observatory |
title_fullStr |
Highest energy particle physics with the Pierre Auger Observatory |
title_full_unstemmed |
Highest energy particle physics with the Pierre Auger Observatory |
title_sort |
Highest energy particle physics with the Pierre Auger Observatory |
dc.creator.none.fl_str_mv |
Mariazzi, Analisa Gabriela |
author |
Mariazzi, Analisa Gabriela |
author_facet |
Mariazzi, Analisa Gabriela |
author_role |
author |
dc.subject.none.fl_str_mv |
Ciencias Exactas Astronomía Cosmic rays Extensive air showers Hadronic interactions |
topic |
Ciencias Exactas Astronomía Cosmic rays Extensive air showers Hadronic interactions |
dc.description.none.fl_txt_mv |
Astroparticles offer a new path for research in the field of particle physics, allowing investigations at energies above those accesible with accelerators. Ultra-high energy cosmic rays can be studied via the observation of the showers they generate in the atmosphere. The Pierre Auger Observatory is a hybrid detector for ultra-high energy cosmic rays, combining two complementary measurement techniques used by previous experiments, to get the best possible measurements of these air showers. Shower observations enable one to not only estimate the energy, direction and most probable mass of the primary cosmic particles but also to obtain some information about the properties of their hadronic interactions. Results that are most relevant in the context of determining hadronic interaction characteristics at ultra-high energies will be presented. Facultad de Ciencias Exactas |
description |
Astroparticles offer a new path for research in the field of particle physics, allowing investigations at energies above those accesible with accelerators. Ultra-high energy cosmic rays can be studied via the observation of the showers they generate in the atmosphere. The Pierre Auger Observatory is a hybrid detector for ultra-high energy cosmic rays, combining two complementary measurement techniques used by previous experiments, to get the best possible measurements of these air showers. Shower observations enable one to not only estimate the energy, direction and most probable mass of the primary cosmic particles but also to obtain some information about the properties of their hadronic interactions. Results that are most relevant in the context of determining hadronic interaction characteristics at ultra-high energies will be presented. |
publishDate |
2014 |
dc.date.none.fl_str_mv |
2014-05-19 |
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/10915/123401 |
url |
http://sedici.unlp.edu.ar/handle/10915/123401 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/2010-1945 info:eu-repo/semantics/altIdentifier/arxiv/1403.1181 info:eu-repo/semantics/altIdentifier/doi/10.1142/s2010194514603019 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
dc.format.none.fl_str_mv |
application/pdf |
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reponame:SEDICI (UNLP) instname:Universidad Nacional de La Plata instacron:UNLP |
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Universidad Nacional de La Plata |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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