3-11 July 2007
Merida, Mexico
Mexico/General timezone
- icrc2007@icrc2007.unam.mx
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Contribution Poster
Merida, Mexico
-
Regency (Hyatt)
HE.1.3.A
Cosmic ray and neutrino physics with space detectors
Speakers
- Mr. Jorge COTZOMI
Primary authors
- Mr. Jorge COTZOMI (Moscow State University- Universidad Autonoma de Puebla)
Co-authors
- Prof. Nikolay KALMYKOV (D.V.Skobeltsyn Institute of Nuclear Physics of M.V.Lomonosov Moscow State University)
- Dr. Humberto SALAZAR (Universidad Autonoma de Puebla)
- Dr. Alfonso ROSADO (Universidad Autonoma de Puebla)
- Dr. Sergey SHARAKIN (D.V.Skobeltsyn Institute of Nuclear Physics of M.V.Lomonosov Moscow State University)
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Abstract content
Simulations of ultra high energy showers that may be generated by different primaries and observed with space detectors are performed. A special driver is developed which enables to treat neutrino as a primary particle in the framework of the traditional codes (AIRES, CORSIKA). Possibilities of the TUS detector employment for ultra high energy neutrino studies are discussed.
Reference
Proceedings of the 30th International Cosmic Ray Conference; Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia (eds.); Universidad Nacional Autónoma de México, Mexico City, Mexico, 2008; Vol. 4 (HE part 1), pages 179-182