What do we mean by detecting earth-skimming of neutrinos?
| dc.citation.epage | 1132 | en_US |
| dc.citation.issue | 13-16 | en_US |
| dc.citation.spage | 1125 | en_US |
| dc.citation.volume | 19 | en_US |
| dc.contributor.author | Lin, GL | en_US |
| dc.contributor.department | 物理研究所 | zh_TW |
| dc.contributor.department | Institute of Physics | en_US |
| dc.date.accessioned | 2014-12-08T15:39:09Z | |
| dc.date.available | 2014-12-08T15:39:09Z | |
| dc.date.issued | 2004-05-30 | en_US |
| dc.description.abstract | In this talk, we elaborate the strategy for detecting the Earth-skimming tau neutrinos. We first show that there are non-negligible astrophysical tau neutrino fluxes due to neutrino flavor oscillations. We then illustrate the idea of detecting Earth-skimming tau neutrinos. In particular, we point out that the tau-lepton flux resulting from neutrino-nucleon scatterings inside the earth is controlled by the tau-lepton range. We demonstrate this observation by showing the tau-lepton flux induced by the GZK tau-neutrino flux. The question on the energy resolutions of tau neutrinos in this detection strategy is briefly discussed. | en_US |
| dc.identifier.issn | 0217-7323 | en_US |
| dc.identifier.journal | MODERN PHYSICS LETTERS A | en_US |
| dc.identifier.uri | https://ir.lib.nycu.edu.tw/handle/11536/26758 | |
| dc.identifier.wosnumber | WOS:000221914800027 | |
| dc.language.iso | en_US | en_US |
| dc.subject | earth-skimming neutrinos | en_US |
| dc.subject | tau leptons | en_US |
| dc.title | What do we mean by detecting earth-skimming of neutrinos? | en_US |
| dc.type | Article; Proceedings Paper | en_US |
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