Neutrino flavor ratio on Earth and at astrophysical sources
| dc.citation.epage | 422 | en_US |
| dc.citation.issue | 2 | en_US |
| dc.citation.spage | 420 | en_US |
| dc.citation.volume | 64 | en_US |
| dc.citation.woscount | 0 | |
| 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.contributor.department | 物理研究所 | zh_TW |
| dc.contributor.department | Institute of Physics | 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.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.identifier.doi | 10.1016/j.ppnp.2009.12.064 | en_US |
| dc.identifier.issn | 0146-6410 | en_US |
| dc.identifier.journal | PROGRESS IN PARTICLE AND NUCLEAR PHYSICS | en_US |
| dc.identifier.uri | http://dx.doi.org/10.1016/j.ppnp.2009.12.064 | en_US |
| dc.identifier.uri | https://ir.lib.nycu.edu.tw/handle/11536/5535 | |
| dc.identifier.wosnumber | WOS:000283519100065 | |
| 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 |