Ultra-High Energy Cosmic Rays
- Autores
- Dova, María Teresa
- Año de publicación
- 2013
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- The origin of the ultra high energy cosmic rays (UHECR) with energies above E > 1017 eV, is still unknown. The discovery of their sources will reveal the engines of the most energetic astrophysical accelerators in the universe. This is a written version of a series of lectures devoted to UHECR at the 2013 CERN-Latin-American School of High-Energy Physics. We present an intro- duction to acceleration mechanisms of charged particles to the highest ener- gies in astrophysical objects, their propagation from the sources to Earth, and the experimental techniques for their detection. We also discuss some of the relevant observational results from Telescope Array and Pierre Auger Obser- vatory. These experiments deal with particle interactions at energies orders of magnitude higher than achieved in terrestrial accelerators.
Instituto de Física La Plata - Materia
-
Física
Ultra high energy cosmic rays (UHECR)
Astrophysical particle acceleration
Pierre Auger Observatory - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/195129
Ver los metadatos del registro completo
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Ultra-High Energy Cosmic RaysDova, María TeresaFísicaUltra high energy cosmic rays (UHECR)Astrophysical particle accelerationPierre Auger ObservatoryThe origin of the ultra high energy cosmic rays (UHECR) with energies above E > 1017 eV, is still unknown. The discovery of their sources will reveal the engines of the most energetic astrophysical accelerators in the universe. This is a written version of a series of lectures devoted to UHECR at the 2013 CERN-Latin-American School of High-Energy Physics. We present an intro- duction to acceleration mechanisms of charged particles to the highest ener- gies in astrophysical objects, their propagation from the sources to Earth, and the experimental techniques for their detection. We also discuss some of the relevant observational results from Telescope Array and Pierre Auger Obser- vatory. These experiments deal with particle interactions at energies orders of magnitude higher than achieved in terrestrial accelerators.Instituto de Física La Plata2013-03info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/195129enginfo:eu-repo/semantics/altIdentifier/url/https://cds.cern.ch/record/2019742info:eu-repo/semantics/altIdentifier/doi/10.5170/CERN-2015-001.169info: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:UNLP2026-06-23T11:16:57Zoai:sedici.unlp.edu.ar:10915/195129Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292026-06-23 11:16:57.356SEDICI (UNLP) - Universidad Nacional de La Platafalse |
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Ultra-High Energy Cosmic Rays |
| title |
Ultra-High Energy Cosmic Rays |
| spellingShingle |
Ultra-High Energy Cosmic Rays Dova, María Teresa Física Ultra high energy cosmic rays (UHECR) Astrophysical particle acceleration Pierre Auger Observatory |
| title_short |
Ultra-High Energy Cosmic Rays |
| title_full |
Ultra-High Energy Cosmic Rays |
| title_fullStr |
Ultra-High Energy Cosmic Rays |
| title_full_unstemmed |
Ultra-High Energy Cosmic Rays |
| title_sort |
Ultra-High Energy Cosmic Rays |
| dc.creator.none.fl_str_mv |
Dova, María Teresa |
| author |
Dova, María Teresa |
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Dova, María Teresa |
| author_role |
author |
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Física Ultra high energy cosmic rays (UHECR) Astrophysical particle acceleration Pierre Auger Observatory |
| topic |
Física Ultra high energy cosmic rays (UHECR) Astrophysical particle acceleration Pierre Auger Observatory |
| dc.description.none.fl_txt_mv |
The origin of the ultra high energy cosmic rays (UHECR) with energies above E > 1017 eV, is still unknown. The discovery of their sources will reveal the engines of the most energetic astrophysical accelerators in the universe. This is a written version of a series of lectures devoted to UHECR at the 2013 CERN-Latin-American School of High-Energy Physics. We present an intro- duction to acceleration mechanisms of charged particles to the highest ener- gies in astrophysical objects, their propagation from the sources to Earth, and the experimental techniques for their detection. We also discuss some of the relevant observational results from Telescope Array and Pierre Auger Obser- vatory. These experiments deal with particle interactions at energies orders of magnitude higher than achieved in terrestrial accelerators. Instituto de Física La Plata |
| description |
The origin of the ultra high energy cosmic rays (UHECR) with energies above E > 1017 eV, is still unknown. The discovery of their sources will reveal the engines of the most energetic astrophysical accelerators in the universe. This is a written version of a series of lectures devoted to UHECR at the 2013 CERN-Latin-American School of High-Energy Physics. We present an intro- duction to acceleration mechanisms of charged particles to the highest ener- gies in astrophysical objects, their propagation from the sources to Earth, and the experimental techniques for their detection. We also discuss some of the relevant observational results from Telescope Array and Pierre Auger Obser- vatory. These experiments deal with particle interactions at energies orders of magnitude higher than achieved in terrestrial accelerators. |
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2013 |
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2013-03 |
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eng |
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