- 學位論文
天體微中子與宇宙線起源之微中子流量比較
The comparison of neutrino flux from astrophysical sources and that from GZK interactions.
並列摘要
Very 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.
參考文獻
[2] T. Kashti and E. Waxman, Phys. Rev. Lett. 95, 181101 (2005).
[3] E. Waxman and J. N. Bahcall, Phys. Rev. D 59, 023002 (1998).
[4] E. Waxman and J. N. Bahcall, Phys. Rev. Lett. 78, 2292 (1997).
[6] E. Waxman, Phys. Rev. Lett. 75, 386 (1995).
[8] For a review, see, for example, H. Athar, Chinese Journal of Physics Vol. 42 , No. 1.
延伸閱讀
- Chen, T. H. (2020). 透過暗物質及中子衰變異常的微中子模型 [master's thesis, Tamkang University]. Airiti Library. https://www.airitilibrary.com/Article/Detail?DocID=U0002-1607202013435700
- Lin, Y. H. (2016). 微中子在暗質間接探測之應用 [doctoral dissertation, National Chiao Tung University]. Airiti Library. https://www.airitilibrary.com/Article/Detail?DocID=U0030-0803201714425678
- Leung, C. H. (2020). 宇宙微中子之無線電波探測研究 [master's thesis, National Taiwan University]. Airiti Library. https://doi.org/10.6342/NTU202001239
- 黃梆碩（2021）。太陽質子事件對內輻射帶質子通量的時空分佈影響：范艾倫探測器觀測分析〔碩士論文，淡江大學〕。華藝線上圖書館。https://www.airitilibrary.com/Article/Detail?DocID=U0002-1906202111475100
- Tsai, S. R. (2005). Estimation of the Sensitivity of Neutrino Telescope (Nutel) [master's thesis, National Taiwan University]. Airiti Library. https://doi.org/10.6342/NTU.2005.01658