來自伽瑪射線爆之微中子

Full metadata record

DC Field	Value	Language
dc.contributor.author	周禹廷	en_US
dc.contributor.author	Chou, Yu-Ting	en_US
dc.contributor.author	林貴林	en_US
dc.contributor.author	Lin, Guey-lin	en_US
dc.date.accessioned	2014-12-12T01:41:09Z	-
dc.date.available	2014-12-12T01:41:09Z	-
dc.date.issued	2010	en_US
dc.identifier.uri	http://140.113.39.130/cdrfb3/record/nctu/#GT079727511	en_US
dc.identifier.uri	http://hdl.handle.net/11536/45265	-
dc.description.abstract	本論文研究來自伽瑪射線爆的微中子其流量以及味組成，首先考慮典型的伽瑪射線爆。其次計算不同磁場大小對微中子流量以及味組成的影響，並探討流量以及味分布以及與不同光學能譜之伽瑪射線爆之關連性。我們主要探討是否有純粹由中子衰變的微中子流。動機來自於Mohara and Gupta發表的研究。我們的結果將與Mohara此篇作比較。	zh_TW
dc.description.abstract	In this thesis we predict the neutrino flux and flavor composition from gamma-ray bursts (GRBs). At first we consider typical gamma-ray bursts. We calculate the magnetic field effects on GRBs with different magnetic field strength. We also consider the flux and flavor composition dependencies on photon spectra indices for different gamma ray bursts. We aim to look for a pure neutron beam. This thesis is motivated by a study by Moharana and Gupta. We compare our result with that of Moharana and Gupta.	en_US
dc.language.iso	zh_TW	en_US
dc.subject	微中子	zh_TW
dc.subject	伽瑪射線爆	zh_TW
dc.subject	震波模型	zh_TW
dc.subject	極高能宇宙射線	zh_TW
dc.subject	neutrino	en_US
dc.subject	shock model	en_US
dc.subject	gamma-ray burst	en_US
dc.subject	ultra high energy cosmic ray	en_US
dc.title	來自伽瑪射線爆之微中子	zh_TW
dc.title	Neutrinos from gamma-ray burst	en_US
dc.type	Thesis	en_US
dc.contributor.department	物理研究所	zh_TW
Appears in Collections:	Thesis

Files in This Item:

751101.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.