A semi-analytic calculation on the atmospheric tau neutrino flux in the GeV to TeV energy range

doi:10.1016/j.astropartphys.2005.11.003

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DC Field	Value	Language
dc.contributor.author	Lee, FF	en_US
dc.contributor.author	Lin, GL	en_US
dc.date.accessioned	2014-12-08T15:17:31Z	-
dc.date.available	2014-12-08T15:17:31Z	-
dc.date.issued	2006-02-01	en_US
dc.identifier.issn	0927-6505	en_US
dc.identifier.uri	http://dx.doi.org/10.1016/j.astropartphys.2005.11.003	en_US
dc.identifier.uri	http://hdl.handle.net/11536/12706	-
dc.description.abstract	We present a semi-analytic calculation on the atmospheric tau neutrino flux in the GeV to TeV energy range. The atmospheric v, flux is calculated for the entire zenith angle range. This flux is contributed by the oscillations of muon neutrinos coming from the two-body pi and K decays and the three-body mu(+/-) decays, and the intrinsic tau neutrino flux surviving the oscillations. The uncertainties in our calculations are discussed in detail. The implications of our result are also discussed. (c) 2005 Elsevier B.V. All rights reserved.	en_US
dc.language.iso	en_US	en_US
dc.subject	tau neutrino	en_US
dc.subject	neutrino oscillation	en_US
dc.subject	atmospheric neutrino flux	en_US
dc.title	A semi-analytic calculation on the atmospheric tau neutrino flux in the GeV to TeV energy range	en_US
dc.type	Article	en_US
dc.identifier.doi	10.1016/j.astropartphys.2005.11.003	en_US
dc.identifier.journal	ASTROPARTICLE PHYSICS	en_US
dc.citation.volume	25	en_US
dc.citation.issue	1	en_US
dc.citation.spage	64	en_US
dc.citation.epage	73	en_US
dc.contributor.department	物理研究所	zh_TW
dc.contributor.department	Institute of Physics	en_US
dc.identifier.wosnumber	WOS:000235422100007	-
dc.citation.woscount	8	-
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