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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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Autor principal: Kachelriess, M.
Lenguaje:eng
Publicado: 2000
Materias:
Acceso en línea:https://dx.doi.org/10.1063/1.1363517
http://cds.cern.ch/record/476858
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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
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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