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dc.contributor.author董念恩en_US
dc.contributor.authorNien-En Tungen_US
dc.contributor.author林貴林en_US
dc.date.accessioned2014-12-12T02:57:49Z-
dc.date.available2014-12-12T02:57:49Z-
dc.date.issued2006en_US
dc.identifier.urihttp://140.113.39.130/cdrfb3/record/nctu/#GT009327501en_US
dc.identifier.urihttp://hdl.handle.net/11536/79306-
dc.description.abstract利用大氣微中子的天頂角異向性及高天頂角度區及低天頂角度區簇射數目比來探求 銀河系外微中子來源和判段實際大氣prompt微中子的粒子模型zh_TW
dc.description.abstractWe examine the prompt and conventional atmospheric neutrino fluxes where different models for the prompt flux are employed. Due to different angular dependencies between the prompt flux and the conventional ones, we compare the shower event ratio due to the prompt flux to that due to the conventional flux. This is important to separate the prompt atmospheric neutrino flux from the conventional component. The determination of the former is useful for testing the models for charm productions.en_US
dc.language.isoen_USen_US
dc.subject大氣zh_TW
dc.subject微中子zh_TW
dc.subject簇射zh_TW
dc.subjectconventionalen_US
dc.subjectgamma ray bursten_US
dc.subjectneutrinoen_US
dc.subjectprompten_US
dc.subjectshoweren_US
dc.titleTeV到PeV能區的微中子天文學zh_TW
dc.titleNeutrino Astronomy in the TeV to PeV Energy Rangeen_US
dc.typeThesisen_US
dc.contributor.department物理研究所zh_TW
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