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Ultrahigh energy cosmic rays and new particle physics
The current status of the ultrahigh energy cosmic ray (UHE CR) enigma and several proposed solutions involving particle physics beyond the standard model are discussed. Emphasis is given to top--down models, and as a main example, supermassive dark matter as galactic source for UHE CR and the status...
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Lenguaje: | eng |
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2000
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Acceso en línea: | https://dx.doi.org/10.1063/1.1363517 http://cds.cern.ch/record/476858 |
_version_ | 1780896692254539776 |
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author | Kachelriess, M. |
author_facet | Kachelriess, M. |
author_sort | Kachelriess, M. |
collection | CERN |
description | The current status of the ultrahigh energy cosmic ray (UHE CR) enigma and several proposed solutions involving particle physics beyond the standard model are discussed. Emphasis is given to top--down models, and as a main example, supermassive dark matter as galactic source for UHE CR and the status of its experimental signatures (galactic anisotropy, chemical composition and clustering) is reviewed. Then different approaches to calculate fragmentation spectra of supermassive particles are discussed. Finally, it is argued that UHE neutrinos cannot be - neither directly or indirectly - responsible for the observed vertical air showers. |
id | cern-476858 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2000 |
record_format | invenio |
spelling | cern-4768582023-03-14T20:21:12Zdoi:10.1063/1.1363517http://cds.cern.ch/record/476858engKachelriess, M.Ultrahigh energy cosmic rays and new particle physicsAstrophysics and AstronomyThe current status of the ultrahigh energy cosmic ray (UHE CR) enigma and several proposed solutions involving particle physics beyond the standard model are discussed. Emphasis is given to top--down models, and as a main example, supermassive dark matter as galactic source for UHE CR and the status of its experimental signatures (galactic anisotropy, chemical composition and clustering) is reviewed. Then different approaches to calculate fragmentation spectra of supermassive particles are discussed. Finally, it is argued that UHE neutrinos cannot be - neither directly or indirectly - responsible for the observed vertical air showers.The current status of the UltraHigh Energy Cosmic Ray (UHE CR) enigma and several proposed solutions involving particle physics beyond the standard model are discussed. Emphasis is given to top-down models, and as a main example, supermassive dark matter as galactic source for UHE CR and the status of its experimental signatures (galactic anisotropy, chemical composition and clustering) is reviewed. Then different approaches to calculate fragmentation spectra of supermassive particles are discussed. Finally, it is argued that UHE neutrinos cannot be—neither directly or indirectly—responsible for the observed UHE CR events.The current status of the ultrahigh energy cosmic ray (UHE CR) enigma and several proposed solutions involving particle physics beyond the standard model are discussed. Emphasis is given to top--down models, and as a main example, supermassive dark matter as galactic source for UHE CR and the status of its experimental signatures (galactic anisotropy, chemical composition and clustering) is reviewed. Then different approaches to calculate fragmentation spectra of supermassive particles are discussed. Finally, it is argued that UHE neutrinos cannot be - neither directly or indirectly - responsible for the observed vertical air showers.astro-ph/0011231CERN-TH-2000-324CERN-TH-2000-324oai:cds.cern.ch:4768582000-11-13 |
spellingShingle | Astrophysics and Astronomy Kachelriess, M. Ultrahigh energy cosmic rays and new particle physics |
title | Ultrahigh energy cosmic rays and new particle physics |
title_full | Ultrahigh energy cosmic rays and new particle physics |
title_fullStr | Ultrahigh energy cosmic rays and new particle physics |
title_full_unstemmed | Ultrahigh energy cosmic rays and new particle physics |
title_short | Ultrahigh energy cosmic rays and new particle physics |
title_sort | ultrahigh energy cosmic rays and new particle physics |
topic | Astrophysics and Astronomy |
url | https://dx.doi.org/10.1063/1.1363517 http://cds.cern.ch/record/476858 |
work_keys_str_mv | AT kachelriessm ultrahighenergycosmicraysandnewparticlephysics |