High energy physics in the atmosphere: Phenomenology of cosmic ray air showers
- Autores
- Anchordoqui, Luis A.; Dova, Maria Teresa; Mariazzi, Analisa Gabriela; Thomas P. McCauley; Paul, Thomas; Reucroft, Stephen; Swain, John
- Año de publicación
- 2004
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The properties of cosmic rays with energies above 106 GeV have to be deduced from the spacetime structure and particle content of the air showers which they initiate. In this review we summarize the phenomenology of these giant air showers. We describe the hadronic interaction models used to extrapolate results from collider data to ultra high energies, and discuss the prospects for insights into forward physics at the LHC. We also describe the main electromagnetic processes that govern the longitudinal shower evolution, as well as the lateral spread of particles. Armed with these two principal shower ingredients and motivation from the underlying physics, we provide an overview of some of the different methods proposed to distinguish primary species. The properties of neutrino interactions and the potential of forthcoming experiments to isolate deeply penetrating showers from baryonic cascades are also discussed. We finally venture into a terra incognita endowed with TeV-scale gravity and explore anomalous neutrino-induced showers. © 2004 Elsevier Inc. All rights reserved.
Fil: Anchordoqui, Luis A.. Northeastern University; Estados Unidos
Fil: Dova, Maria Teresa. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Fil: Mariazzi, Analisa Gabriela. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Fil: Thomas P. McCauley. Northeastern University; Estados Unidos
Fil: Paul, Thomas. Northeastern University; Estados Unidos
Fil: Reucroft, Stephen. Northeastern University; Estados Unidos
Fil: Swain, John. Northeastern University; Estados Unidos - Materia
-
Cosmic Rays
Extensive Air Showers - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/72427
Ver los metadatos del registro completo
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High energy physics in the atmosphere: Phenomenology of cosmic ray air showersAnchordoqui, Luis A.Dova, Maria TeresaMariazzi, Analisa GabrielaThomas P. McCauleyPaul, ThomasReucroft, StephenSwain, JohnCosmic RaysExtensive Air Showershttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The properties of cosmic rays with energies above 106 GeV have to be deduced from the spacetime structure and particle content of the air showers which they initiate. In this review we summarize the phenomenology of these giant air showers. We describe the hadronic interaction models used to extrapolate results from collider data to ultra high energies, and discuss the prospects for insights into forward physics at the LHC. We also describe the main electromagnetic processes that govern the longitudinal shower evolution, as well as the lateral spread of particles. Armed with these two principal shower ingredients and motivation from the underlying physics, we provide an overview of some of the different methods proposed to distinguish primary species. The properties of neutrino interactions and the potential of forthcoming experiments to isolate deeply penetrating showers from baryonic cascades are also discussed. We finally venture into a terra incognita endowed with TeV-scale gravity and explore anomalous neutrino-induced showers. © 2004 Elsevier Inc. All rights reserved.Fil: Anchordoqui, Luis A.. Northeastern University; Estados UnidosFil: Dova, Maria Teresa. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaFil: Mariazzi, Analisa Gabriela. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaFil: Thomas P. McCauley. Northeastern University; Estados UnidosFil: Paul, Thomas. Northeastern University; Estados UnidosFil: Reucroft, Stephen. Northeastern University; Estados UnidosFil: Swain, John. Northeastern University; Estados UnidosAcademic Press Inc Elsevier Science2004-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/72427Anchordoqui, Luis A.; Dova, Maria Teresa; Mariazzi, Analisa Gabriela; Thomas P. McCauley; Paul, Thomas; et al.; High energy physics in the atmosphere: Phenomenology of cosmic ray air showers; Academic Press Inc Elsevier Science; Annals of Physics (New York); 314; 1; 12-2004; 145-2070003-4916CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0003491604001381info:eu-repo/semantics/altIdentifier/doi/10.1016/j.aop.2004.07.003info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-10T13:19:29Zoai:ri.conicet.gov.ar:11336/72427instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-10 13:19:30.123CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
High energy physics in the atmosphere: Phenomenology of cosmic ray air showers |
| title |
High energy physics in the atmosphere: Phenomenology of cosmic ray air showers |
| spellingShingle |
High energy physics in the atmosphere: Phenomenology of cosmic ray air showers Anchordoqui, Luis A. Cosmic Rays Extensive Air Showers |
| title_short |
High energy physics in the atmosphere: Phenomenology of cosmic ray air showers |
| title_full |
High energy physics in the atmosphere: Phenomenology of cosmic ray air showers |
| title_fullStr |
High energy physics in the atmosphere: Phenomenology of cosmic ray air showers |
| title_full_unstemmed |
High energy physics in the atmosphere: Phenomenology of cosmic ray air showers |
| title_sort |
High energy physics in the atmosphere: Phenomenology of cosmic ray air showers |
| dc.creator.none.fl_str_mv |
Anchordoqui, Luis A. Dova, Maria Teresa Mariazzi, Analisa Gabriela Thomas P. McCauley Paul, Thomas Reucroft, Stephen Swain, John |
| author |
Anchordoqui, Luis A. |
| author_facet |
Anchordoqui, Luis A. Dova, Maria Teresa Mariazzi, Analisa Gabriela Thomas P. McCauley Paul, Thomas Reucroft, Stephen Swain, John |
| author_role |
author |
| author2 |
Dova, Maria Teresa Mariazzi, Analisa Gabriela Thomas P. McCauley Paul, Thomas Reucroft, Stephen Swain, John |
| author2_role |
author author author author author author |
| dc.subject.none.fl_str_mv |
Cosmic Rays Extensive Air Showers |
| topic |
Cosmic Rays Extensive Air Showers |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
The properties of cosmic rays with energies above 106 GeV have to be deduced from the spacetime structure and particle content of the air showers which they initiate. In this review we summarize the phenomenology of these giant air showers. We describe the hadronic interaction models used to extrapolate results from collider data to ultra high energies, and discuss the prospects for insights into forward physics at the LHC. We also describe the main electromagnetic processes that govern the longitudinal shower evolution, as well as the lateral spread of particles. Armed with these two principal shower ingredients and motivation from the underlying physics, we provide an overview of some of the different methods proposed to distinguish primary species. The properties of neutrino interactions and the potential of forthcoming experiments to isolate deeply penetrating showers from baryonic cascades are also discussed. We finally venture into a terra incognita endowed with TeV-scale gravity and explore anomalous neutrino-induced showers. © 2004 Elsevier Inc. All rights reserved. Fil: Anchordoqui, Luis A.. Northeastern University; Estados Unidos Fil: Dova, Maria Teresa. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina Fil: Mariazzi, Analisa Gabriela. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina Fil: Thomas P. McCauley. Northeastern University; Estados Unidos Fil: Paul, Thomas. Northeastern University; Estados Unidos Fil: Reucroft, Stephen. Northeastern University; Estados Unidos Fil: Swain, John. Northeastern University; Estados Unidos |
| description |
The properties of cosmic rays with energies above 106 GeV have to be deduced from the spacetime structure and particle content of the air showers which they initiate. In this review we summarize the phenomenology of these giant air showers. We describe the hadronic interaction models used to extrapolate results from collider data to ultra high energies, and discuss the prospects for insights into forward physics at the LHC. We also describe the main electromagnetic processes that govern the longitudinal shower evolution, as well as the lateral spread of particles. Armed with these two principal shower ingredients and motivation from the underlying physics, we provide an overview of some of the different methods proposed to distinguish primary species. The properties of neutrino interactions and the potential of forthcoming experiments to isolate deeply penetrating showers from baryonic cascades are also discussed. We finally venture into a terra incognita endowed with TeV-scale gravity and explore anomalous neutrino-induced showers. © 2004 Elsevier Inc. All rights reserved. |
| publishDate |
2004 |
| dc.date.none.fl_str_mv |
2004-12 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
| status_str |
publishedVersion |
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http://hdl.handle.net/11336/72427 Anchordoqui, Luis A.; Dova, Maria Teresa; Mariazzi, Analisa Gabriela; Thomas P. McCauley; Paul, Thomas; et al.; High energy physics in the atmosphere: Phenomenology of cosmic ray air showers; Academic Press Inc Elsevier Science; Annals of Physics (New York); 314; 1; 12-2004; 145-207 0003-4916 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/72427 |
| identifier_str_mv |
Anchordoqui, Luis A.; Dova, Maria Teresa; Mariazzi, Analisa Gabriela; Thomas P. McCauley; Paul, Thomas; et al.; High energy physics in the atmosphere: Phenomenology of cosmic ray air showers; Academic Press Inc Elsevier Science; Annals of Physics (New York); 314; 1; 12-2004; 145-207 0003-4916 CONICET Digital CONICET |
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eng |
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eng |
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Academic Press Inc Elsevier Science |
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