Simulations of showers arising from high energy neutrinos

• Main Authors: Yu-Lung Hung, 洪瑜隆
• Other Authors: Guey-Lin Lin
• Format: Others
• Language: zh-TW
• Published: 2006
• Online Access: http://ndltd.ncl.edu.tw/handle/42125120283411371870

碩士 === 國立交通大學 === 物理研究所 === 94 === This essay is about the Shower phenomenon caused by Greisen-Zatsepin-Kuzmin neutrions, Active Galactic Nuclei neutrinos and Gamman Ray Burst neutrions. It presents the main energy area measured and directions detected by the detector and tell different message sources apart. Also,the application of Monte-carlo method to high-energy neutrinos is researched. Our DSR(Detector Sensitivity Region) of the simulation. that geometry of shape is sphere. Which center located under the ground six kilometers and it’s radius is one kilometer. We discus two mediums rocksalt and water inside the DSR simulating shower caused by high energy neutrions. And outside the DSR is according to standard density model of the earth.