Measurement of the atmospheric muon spectrum from 20 to 3000 GeV
- Autores
- Dova, María Teresa; L3 Collaboration
- Año de publicación
- 2004
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The absolute muon flux between 20 and 3000 GeV is measured with the L3 magnetic muon spectrometer for zenith angles ranging from 0º to 58º. Due to the large exposure of about 150 m2 sr d, and the excellent momentum resolution of the L3 muon chambers, a precision of 2.3% at 150 GeV in the vertical direction is achieved. The ratio of positive to negative muons is studied between 20 and 500 GeV, and the average vertical muon charge ratio is found to be 1.285 ± 0.003(stat.)± 0.019(syst.).
La lista completa de autores puede verse en el archivo asociado.
Facultad de Ciencias Exactas - Materia
-
Física
Atmospheric muon spectrum
Cosmic rays
High-energy hadronic interactions - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by/3.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/78385
Ver los metadatos del registro completo
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Measurement of the atmospheric muon spectrum from 20 to 3000 GeVDova, María TeresaL3 CollaborationFísicaAtmospheric muon spectrumCosmic raysHigh-energy hadronic interactionsThe absolute muon flux between 20 and 3000 GeV is measured with the L3 magnetic muon spectrometer for zenith angles ranging from 0º to 58º. Due to the large exposure of about 150 m2 sr d, and the excellent momentum resolution of the L3 muon chambers, a precision of 2.3% at 150 GeV in the vertical direction is achieved. The ratio of positive to negative muons is studied between 20 and 500 GeV, and the average vertical muon charge ratio is found to be 1.285 ± 0.003(stat.)± 0.019(syst.).La lista completa de autores puede verse en el archivo asociado.Facultad de Ciencias Exactas2004-09-23info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf15-32http://sedici.unlp.edu.ar/handle/10915/78385enginfo:eu-repo/semantics/altIdentifier/issn/0370-2693info:eu-repo/semantics/altIdentifier/doi/10.1016/j.physletb.2004.08.003info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/3.0/Creative Commons Attribution 3.0 Unported (CC BY 3.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T16:52:51Zoai:sedici.unlp.edu.ar:10915/78385Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 16:52:51.288SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Measurement of the atmospheric muon spectrum from 20 to 3000 GeV |
| title |
Measurement of the atmospheric muon spectrum from 20 to 3000 GeV |
| spellingShingle |
Measurement of the atmospheric muon spectrum from 20 to 3000 GeV Dova, María Teresa Física Atmospheric muon spectrum Cosmic rays High-energy hadronic interactions |
| title_short |
Measurement of the atmospheric muon spectrum from 20 to 3000 GeV |
| title_full |
Measurement of the atmospheric muon spectrum from 20 to 3000 GeV |
| title_fullStr |
Measurement of the atmospheric muon spectrum from 20 to 3000 GeV |
| title_full_unstemmed |
Measurement of the atmospheric muon spectrum from 20 to 3000 GeV |
| title_sort |
Measurement of the atmospheric muon spectrum from 20 to 3000 GeV |
| dc.creator.none.fl_str_mv |
Dova, María Teresa L3 Collaboration |
| author |
Dova, María Teresa |
| author_facet |
Dova, María Teresa L3 Collaboration |
| author_role |
author |
| author2 |
L3 Collaboration |
| author2_role |
author |
| dc.subject.none.fl_str_mv |
Física Atmospheric muon spectrum Cosmic rays High-energy hadronic interactions |
| topic |
Física Atmospheric muon spectrum Cosmic rays High-energy hadronic interactions |
| dc.description.none.fl_txt_mv |
The absolute muon flux between 20 and 3000 GeV is measured with the L3 magnetic muon spectrometer for zenith angles ranging from 0º to 58º. Due to the large exposure of about 150 m2 sr d, and the excellent momentum resolution of the L3 muon chambers, a precision of 2.3% at 150 GeV in the vertical direction is achieved. The ratio of positive to negative muons is studied between 20 and 500 GeV, and the average vertical muon charge ratio is found to be 1.285 ± 0.003(stat.)± 0.019(syst.). La lista completa de autores puede verse en el archivo asociado. Facultad de Ciencias Exactas |
| description |
The absolute muon flux between 20 and 3000 GeV is measured with the L3 magnetic muon spectrometer for zenith angles ranging from 0º to 58º. Due to the large exposure of about 150 m2 sr d, and the excellent momentum resolution of the L3 muon chambers, a precision of 2.3% at 150 GeV in the vertical direction is achieved. The ratio of positive to negative muons is studied between 20 and 500 GeV, and the average vertical muon charge ratio is found to be 1.285 ± 0.003(stat.)± 0.019(syst.). |
| publishDate |
2004 |
| dc.date.none.fl_str_mv |
2004-09-23 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://sedici.unlp.edu.ar/handle/10915/78385 |
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eng |
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eng |
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info:eu-repo/semantics/altIdentifier/issn/0370-2693 info:eu-repo/semantics/altIdentifier/doi/10.1016/j.physletb.2004.08.003 |
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openAccess |
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