1. You are Here：

Full metadata record
DC FieldValueLanguage
dc.contributor.author謝念潔en_US
dc.contributor.authorHsieh, Nien-Chiehen_US
dc.contributor.author林貴林en_US
dc.contributor.authorLin, Guey-Linen_US
dc.date.accessioned2014-12-12T01:41:09Z-
dc.date.available2014-12-12T01:41:09Z-
dc.date.issued2009en_US
dc.identifier.urihttp://140.113.39.130/cdrfb3/record/nctu/#GT079727507en_US
dc.identifier.urihttp://hdl.handle.net/11536/45261-
dc.description.abstract非常高能量的微中子是由天體和宇宙線起源而來。不同的微中子來源會導致不同的微中子味比例。本論文中，我們在不同能量範圍下比較GRB微中子流量和GZK微中子流量，藉由計算這兩個來源積分而來的流量比例，作為選擇微中子閾值能量的方法。我們提出一個統計方法，由微中子望遠鏡的味量測去重建微中子流量的比例。zh_TW
dc.description.abstractVery high energy neutrinos come from astrophysical sources and GZK interactions. Different neutrino sources produce different neutrino flavor ratios. In this thesis, we compare GRB neutrino flux with GZK neutrino flux in different energy ranges. The ratio between integrated neutrinos fluxes from these two sources are calculated
as a function of chosen neutrino threshold energy. We propose a statistical method to reconstruct such a ratio from flavor measurements of neutrino telescopes.		en_US
dc.language.isoen_USen_US
dc.subject微中子zh_TW
dc.subject流量zh_TW
dc.subjectNeutrinoen_US
dc.subjectFluxen_US
dc.title天體微中子與宇宙線起源之微中子流量比較zh_TW
dc.titleThe comparison of neutrino flux from astrophysical sources and that from GZK interactions.en_US
dc.typeThesisen_US
dc.contributor.department物理研究所zh_TW
Appears in Collections:Thesis


Files in This Item:

  1. 750701.pdf

If it is a zip file, please download the file and unzip it, then open index.html in a browser to view the full text content.

Related Contents
Loading...