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arXiv 0810.3937hep-ex
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实验中微子物理学

Experimental Neutrino Physics

Christopher W. Walter

摘要:

这是中微子物理学非凡的十年。10年前的夏天,在1998年高山中微子会议上,超级神冈合作组织报告了中微子改变味道的观测结果,从而确定了中微子质量的存在。几年后,SNO实验解决了长期存在的太阳中微子问题,证明这也是由于中微子振荡。仅仅几年之后,这些效应就被证实了,并且用人造中微子源测量了振荡参数。现在,就在这最后一年,同样的中微子,这是30年前太阳中微子问题的来源,第一次在实时实验中被测量。在这次演讲中,我将解释一系列实验,特别是过去几年的实验,如何建立了中微子物理学的一致框架,并解释一些悬而未决的问题。最后,我将介绍一系列即将进行的实验如何在未来十年解决这些问题。

英文摘要:

It's been a remarkable decade in neutrino physics. Ten years ago this summer, at the 1998 neutrino conference in Takayama, the Super-Kamiokande collaboration reported the observation of neutrinos changing flavor, thereby establishing the existence of neutrino mass. A few years later, the SNO experiment solved the long-standing solar neutrino problem demonstrating that it too was due to neutrino oscillation. Just a few years after that, these effects were confirmed and the oscillation parameters were measured with man-made neutrino sources. Now, just in this last year, the same neutrinos which were the source of the 30 year old solar neutrino problem were measured for the first time in a real-time experiment. In this talk, I will explain how a set of experiments, especially ones in the last few years, have established a consistent framework of neutrino physics and also explain some outstanding questions. Finally, I will cover how a set of upcoming experiments hope to address these questions in the coming decade.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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