期刊文献+
任意字段
题名或关键词
题名
关键词
文摘
作者
第一作者
机构
刊名
分类号
参考文献
作者简介
基金资助
栏目信息

Detection of supernova neutrinos at spallation neutron sources

Detection of supernova neutrinos at spallation neutron sources
原文传递
导出
摘要 After considering supernova shock effects, Mikheyev-Smirnov-Wolfenstein effects, neutrino collective ef- fects, and Earth matter effects, the detection of supernova neutrinos at the China Spallation Neutron Source is studied and the expected numbers of different flavor supernova neutrinos observed through various reaction chan- nels are calculated with the neutrino energy spectra described by the Fermi-Dirac distribution and the ＂beta fit＂ distribution respectively. Furthermore, the numerical calculation method of supernova neutrino detection on Earth is applied to some other spallation neutron sources, and the total expected numbers of supernova neutrinos observed through different reactions channels are given. After considering supernova shock effects, Mikheyev-Smirnov-Wolfenstein effects, neutrino collective ef- fects, and Earth matter effects, the detection of supernova neutrinos at the China Spallation Neutron Source is studied and the expected numbers of different flavor supernova neutrinos observed through various reaction chan- nels are calculated with the neutrino energy spectra described by the Fermi-Dirac distribution and the ＂beta fit＂ distribution respectively. Furthermore, the numerical calculation method of supernova neutrino detection on Earth is applied to some other spallation neutron sources, and the total expected numbers of supernova neutrinos observed through different reactions channels are given.
作者 黄明阳 郭新恒 杨炳麟
机构地区 Institute of High Energy Physics(IHEP) Dongguan Institute of Neutron Science(DINS) College of Nuclear Science and Technology Department of Physics and Astronomy Institute of Theoretical Physics
出处 《Chinese Physics C》 SCIE CAS CSCD 2016年第7期15-21,共7页 中国物理C（英文版）
基金 Supported by National Natural Science Foundation of China(11205185,11175020,11275025,11575023)
关键词 neutron source supernova neutrinos neutrino effects NUMBER neutron source, supernova neutrinos, neutrino effects, number
分类号 O572.321 [理学—粒子物理与原子核物理]
  • 相关文献

参考文献62

  • 1A. Mirizzi, I. Tamborra, H K. Kotake, K. Sato and K 971-1143 (2006).
  • 2K. Kotake, K. Sato and K. Takahashi, Rept. Prog. Phys., 69: 971-1143 (2006).
  • 3X. H. Guo, M. Y. Huang and B. L. Young, Chin. Phys. C, 34(2): 257-261 (2010).
  • 4K. Hirata, T. Kajita, M. Koshiba et al, Phys. Rev. Lett., 58: 1490-1493 (1987).
  • 5R. M. Bionta, G. Blewitt, C. B. Bratton et al, Phys. Rev. Lett., 58:1494-1496 (1987).
  • 6K. Scholberg, Ann. Rev. Nucl. Part. Sci., 62:81-103 (2012).
  • 7CSNS Project Team, China Spallation Neutron Source Feasi- bility Research Report, Institute of High Energy Physics and Institute of Physics, Chinese Academy of Sciences, 2009 (in Chinese).
  • 8J. Wei, S. N. Fu, J. Y. Tang et al, Chin. Phys. C, 33(11): 1033-1042 (2009).
  • 9S. Wang, S. X. Fang, S. N. Fu et al, Chin. Phys. C, 33 (Suppl. II): 1-3 (2009).
  • 10M. Y. Huang, S. Wang, J. Qiu et al, Chin. Phys. C, 37 (6): 067001 (2013).
Chinese Physics C
2016年 第7期

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部