Neutrino flavor ratio on Earth and at astrophysical sources

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DC 欄位	值	語言
dc.contributor.author	Lai, Kwang-Chang	en_US
dc.contributor.author	Lin, Guey-Lin	en_US
dc.contributor.author	Liu, T. C.	en_US
dc.date.accessioned	2014-12-08T15:07:03Z	-
dc.date.available	2014-12-08T15:07:03Z	-
dc.date.issued	2010-04-01	en_US
dc.identifier.issn	0146-6410	en_US
dc.identifier.uri	http://dx.doi.org/10.1016/j.ppnp.2009.12.064	en_US
dc.identifier.uri	http://hdl.handle.net/11536/5535	-
dc.description.abstract	We present the reconstruction of neutrino flavor ratios at astrophysical sources. For distinguishing the pion source and the muon-damped source to the 3 a level, the neutrino flux ratios, R equivalent to phi(nu(mu))/(phi(nu(e)) + phi(nu(r))) and S equivalent to phi(nu(e))/(phi(nu(r))), need to be measured in accuracies better than 10%. (C) 2010 Elsevier B.V. All rights reserved.	en_US
dc.language.iso	en_US	en_US
dc.title	Neutrino flavor ratio on Earth and at astrophysical sources	en_US
dc.type	Review	en_US
dc.identifier.doi	10.1016/j.ppnp.2009.12.064	en_US
dc.identifier.journal	PROGRESS IN PARTICLE AND NUCLEAR PHYSICS	en_US
dc.citation.volume	64	en_US
dc.citation.issue	2	en_US
dc.citation.spage	420	en_US
dc.citation.epage	422	en_US
dc.contributor.department	物理研究所	zh_TW
dc.contributor.department	Institute of Physics	en_US
dc.identifier.wosnumber	WOS:000283519100065	-
dc.citation.woscount	0	-
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