Full metadata record
DC FieldValueLanguage
dc.contributor.authorAthar, Hen_US
dc.contributor.authorCheung, KMen_US
dc.contributor.authorLin, GLen_US
dc.contributor.authorTseng, JJen_US
dc.date.accessioned2019-04-02T06:04:42Z-
dc.date.available2019-04-02T06:04:42Z-
dc.date.issued2003-01-01en_US
dc.identifier.urihttp://hdl.handle.net/11536/150736-
dc.description.abstractWe compare the tau neutrino flux arising from the galaxy and the earth atmosphere for 10(3) <= E/GeV <= 10(11). The intrinsic and oscillated tau neutrino fluxes from both sources are calculated. The intrinsic galactic v(tau) flux (E >= 10(3) GeV) is calculated by considering the interactions of high-energy cosmic-rays with the matter present in our galaxy, whereas the oscillated galactic v, flux is coming from the oscillation of the galactic v(mu), flux. For the intrinsic atmospheric v, flux, we extend the validity of a previous calculation from E <= 10(6) GeV up to E <= 10(11) GeV. The oscillated atmospheric v, flux is, on the other hand, rather suppressed. We find that, for 10(3) <= E/GeV <= 5.10(7), the oscillated v(tau) flux along the galactic plane dominates over the maximal intrinsic atmospheric v(tau) flux, i.e., the flux along the horizontal direction.en_US
dc.language.isoen_USen_US
dc.titleComparison of high-energy galactic and atmospheric tau neutrino fluxen_US
dc.typeProceedings Paperen_US
dc.identifier.journalPROCEEDINGS OF THE 2002 INTERNATIONAL SYMPOSIUM ON COSMOLOGY AND PARTICLE ASTROPHYSICSen_US
dc.citation.spage181en_US
dc.citation.epage189en_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.identifier.wosnumberWOS:000229639400014en_US
dc.citation.woscount0en_US
Appears in Collections:Conferences Paper