Measurement of the shadowing of high-energy cosmic rays by the Moon: a search for TeV-energy antiprotons
- Autores
- Dova, María Teresa; L3 Collaboration
- Año de publicación
- 2005
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The shadowing of high-energy cosmic rays by the Moon has been observed with a significance of 9.4 standard deviations with the L3 + C muon spectrometer at CERN. A significant effect of the Earth magnetic field is observed. Since no event deficit on the east side of the Moon has been observed, an upper limit at 90% confidence level on the antiproton to proton ratio of 0.11 is obtained for primary energies around 1 TeV.
Facultad de Ciencias Exactas - Materia
-
Ciencias Exactas
Física
Radiación cósmica
Luna
Protones - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/79549
Ver los metadatos del registro completo
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Measurement of the shadowing of high-energy cosmic rays by the Moon: a search for TeV-energy antiprotonsDova, María TeresaL3 CollaborationCiencias ExactasFísicaRadiación cósmicaLunaProtonesThe shadowing of high-energy cosmic rays by the Moon has been observed with a significance of 9.4 standard deviations with the L3 + C muon spectrometer at CERN. A significant effect of the Earth magnetic field is observed. Since no event deficit on the east side of the Moon has been observed, an upper limit at 90% confidence level on the antiproton to proton ratio of 0.11 is obtained for primary energies around 1 TeV.Facultad de Ciencias Exactas2005-03-16info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf411-434http://sedici.unlp.edu.ar/handle/10915/79549enginfo:eu-repo/semantics/altIdentifier/issn/0927-6505info:eu-repo/semantics/altIdentifier/doi/10.1016/j.astropartphys.2005.02.002info: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:UNLP2025-10-22T16:53:24Zoai:sedici.unlp.edu.ar:10915/79549Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 16:53:25.151SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Measurement of the shadowing of high-energy cosmic rays by the Moon: a search for TeV-energy antiprotons |
| title |
Measurement of the shadowing of high-energy cosmic rays by the Moon: a search for TeV-energy antiprotons |
| spellingShingle |
Measurement of the shadowing of high-energy cosmic rays by the Moon: a search for TeV-energy antiprotons Dova, María Teresa Ciencias Exactas Física Radiación cósmica Luna Protones |
| title_short |
Measurement of the shadowing of high-energy cosmic rays by the Moon: a search for TeV-energy antiprotons |
| title_full |
Measurement of the shadowing of high-energy cosmic rays by the Moon: a search for TeV-energy antiprotons |
| title_fullStr |
Measurement of the shadowing of high-energy cosmic rays by the Moon: a search for TeV-energy antiprotons |
| title_full_unstemmed |
Measurement of the shadowing of high-energy cosmic rays by the Moon: a search for TeV-energy antiprotons |
| title_sort |
Measurement of the shadowing of high-energy cosmic rays by the Moon: a search for TeV-energy antiprotons |
| 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 |
Ciencias Exactas Física Radiación cósmica Luna Protones |
| topic |
Ciencias Exactas Física Radiación cósmica Luna Protones |
| dc.description.none.fl_txt_mv |
The shadowing of high-energy cosmic rays by the Moon has been observed with a significance of 9.4 standard deviations with the L3 + C muon spectrometer at CERN. A significant effect of the Earth magnetic field is observed. Since no event deficit on the east side of the Moon has been observed, an upper limit at 90% confidence level on the antiproton to proton ratio of 0.11 is obtained for primary energies around 1 TeV. Facultad de Ciencias Exactas |
| description |
The shadowing of high-energy cosmic rays by the Moon has been observed with a significance of 9.4 standard deviations with the L3 + C muon spectrometer at CERN. A significant effect of the Earth magnetic field is observed. Since no event deficit on the east side of the Moon has been observed, an upper limit at 90% confidence level on the antiproton to proton ratio of 0.11 is obtained for primary energies around 1 TeV. |
| publishDate |
2005 |
| dc.date.none.fl_str_mv |
2005-03-16 |
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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 |
| format |
article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
http://sedici.unlp.edu.ar/handle/10915/79549 |
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http://sedici.unlp.edu.ar/handle/10915/79549 |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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info:eu-repo/semantics/altIdentifier/issn/0927-6505 info:eu-repo/semantics/altIdentifier/doi/10.1016/j.astropartphys.2005.02.002 |
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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) |
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openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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