TeV到PeV能區的微中子天文學

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DC Field	Value	Language
dc.contributor.author	董念恩	en_US
dc.contributor.author	Nien-En Tung	en_US
dc.contributor.author	林貴林	en_US
dc.date.accessioned	2014-12-12T02:57:49Z	-
dc.date.available	2014-12-12T02:57:49Z	-
dc.date.issued	2006	en_US
dc.identifier.uri	http://140.113.39.130/cdrfb3/record/nctu/#GT009327501	en_US
dc.identifier.uri	http://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.abstract	We 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.iso	en_US	en_US
dc.subject	大氣	zh_TW
dc.subject	微中子	zh_TW
dc.subject	簇射	zh_TW
dc.subject	conventional	en_US
dc.subject	gamma ray burst	en_US
dc.subject	neutrino	en_US
dc.subject	prompt	en_US
dc.subject	shower	en_US
dc.title	TeV到PeV能區的微中子天文學	zh_TW
dc.title	Neutrino Astronomy in the TeV to PeV Energy Range	en_US
dc.type	Thesis	en_US
dc.contributor.department	物理研究所	zh_TW
Appears in Collections:	Thesis

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