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2002年诺贝尔物理奖的启示 被引量：2

WHAT CAN WE LEARN FROM THE NOBEL PRIZE IN 2002
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摘要 　本文论述2002年诺贝尔物理奖获得者,R.Davis在探测太阳中微子丢失的成就;M.Koshiba在证实存在太阳中微子丢失,探测超新星中微子和大气μ中微子丢失以及证明μ中微子振荡的成就。此外,本文还叙述2002年诺贝尔物理奖给我们的启示。 This paper describes the achievemeuts obtained by the Nobel prize winners R.Davis for detection of Solar neutrino missing and M.Koshiba for confirmation of the Solar neutrino missing, the detection of Supernova neutrino and detection of Atmospheric muon neutrino missing and muon neutrino oscillation. In the meantime, this paper also describes what can we learn from the Nobel prize in 2002.
作者 何景棠
机构地区 中国科学院高能物理研究所
出处 《物理学进展》 CSCD 北大核心 2003年第3期299-311,共13页 Progress In Physics
关键词 太阳中微子丢失 超新星中微子 大气μ中微子丢失 μ中微子振荡 2002年诺贝尔物理奖 X射线天文学 Solar neutrino missing Supernova neutrino Atmospheric muon neutrino missing
分类号 O572.32- [理学—粒子物理与原子核物理]
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参考文献6

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同被引文献26

  • 1M. Amenomori,S. Ayabe,X. J. Bi,D. Chen,S. W. Cui,Danzengluobu,L. K. Ding,X. H. Ding,C. F. Feng,Zhaoyang Feng,Z. Y. Feng,X. Y. Gao,Q. X. Geng,H. W. Guo,H. H. He,M. He,K. Hibino,N. Hotta,Haibing Hu,H. B. Hu,J. Huang,Q. Huang,H. Y. Jia,F. Kajino,K. Kasahara,Y. Katayose,C. Kato,K. Kawata,Labaciren,G. M. Le,A. F. Li,J. Y. Li,H. Lu,S. L. Lu,X. R. Meng,K. Mizutani,J. Mu,K. Munakata,A. Nagai,H. Nanjo,M. Nishizawa,M. Ohnishi,I. Ohta,H. Onuma,T. Ouchi,S. Ozawa,J. R. Ren,T. Saito,T. Y. Saito,M. Sakata,T. K. Sako,T. Sasaki,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,M. Takita,Y. H. Tan,N. Tateyama,S. Torii,H. Tsuchiya,S. Udo,B. Wang,H. Wang,X. Wang,Y. G. Wang,H. R. Wu,L. Xue,Y. Yamamoto,C. T. Yan,X. C. Yang,S. Yasue,Z. H. Ye,G. C. Yu,A. F. Yuan,T. Yuda,H. M. Zhang,J. L. Zhang,N. J. Zhang,X. Y. Zhang,Y. Zhang,Yi Zhang,Zhaxisangzhu,X. X. Zhou.Underground water Cherenkov muon detector array with the Tibet air shower array for gamma-ray astronomy in the 100 TeV region[J]. Astrophysics and Space Science . 2007 (1-4)
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  • 3N ationalR esearch Council.Connecting quarkswith cosmos:eleven science questionsfora new century[M ]. . 2003
  • 4J. B lümer,R . Engel,J. R . Hrandel.Cosmic rays from the knee to the highest energies. Progress in Particle and N uclearPhysics . 2009
  • 5M .A menomori1,et.al.The all-particle spectrumofprim ary cosmic raysin the wide energy rangefrom 1014 eV to 1017 eV observed with the Tibet-IIIair-show erarray. The A strophysicalJournal . 2008
  • 6M .A menomori1,et.al.A re Protons StillD om inant A t The K nee Of The Cosmic-R ay EnergySpectrum. PhysicsLettersB . 2006
  • 7M .A menomori1,et.al.Moon shadow by cosmic raysunderthe influence ofgeom agnetic field andsearch forantiprotonsatm ulti-T eV energies. A stroparticle Physics . 2007
  • 8N ebula.C ygnusX -3 A nd HerculesX -1 U sing The TibetA irShow erA rray. Phys.R ev.Lett . 1992
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物理学进展
2003年 第3期

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