High energy tau neutrinos: production, propagation and prospects of observations

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dc.creatorAthar, H.
dc.creatorTseng, Jie-Jun
dc.creatorLin, Guey-Lin
dc.date2003-08-27
dc.date.accessioned2026-07-07T03:50:29Z
dc.date.available2026-07-07T03:50:29Z
dc.descriptionHigh energy tau neutrinos with energy greater than several thousands of GeV may be produced in some astrophysical sites. A summary of the intrinsic high energy tau neutrino flux estimates from some representative astrophysical sites is presented including the effects of neutrino flavor oscillations. The presently envisaged prospects of observations of the oscillated high energy tau neutrino flux are mentioned. In particular, a recently suggested possibility of future observations of Earth-skimming high energy tau neutrinos is briefly discussed.
dc.description4 pages, 2 figs, talk given at 28th International Cosmic Ray Conference (ICRC 2003), Tsukuba, Japan, 31 July-7 Aug, 2003, appeared in its proceedings edited by T. Kajita et al., HE, pp. 1431-1434
dc.identifierhttps://arxiv.org/abs/hep-ph/0308270
dc.identifierhttp://arxiv.org/abs/hep-ph/0308270
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/42788
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleHigh energy tau neutrinos: production, propagation and prospects of observations
dc.typetext

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