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arXiv physics/0305075physics.geo-phastro-phhep-phnucl-ex
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圣马可及以下的中微子

Neutrinos from San Marco and Below

G. Fiorentini, M. Lissia, F. Mantovani, B. Ricci

摘要:

以圣马可大教堂为例,给出了辐射生热和反中微子产生的数量级估计。讨论了利用反中微子探测天然放射性(地中微子)来确定辐射成因对地热贡献的前景。一个三年的三千吨闪烁体探测器可以清楚地区分不同的地热生产模式。此外,地中微子的研究提供了一种可能性,通过利用地球中Th/U丰度的知识来改进中微子质量和混合的测定。

英文摘要:

Order of magnitude estimates of radiogenic heat and antineutrino production are given, using the San Marco cathedral as an example. Prospects of determining the radiogenic contribution to terrestrial heat by detection of antineutrinos from natural radioactivity (geoneutrinos) are discussed. A three kton scintillator detector in three years can clearly discriminate among different models of terrestrial heat production. In addition, the study of geoneutrinos offers a possibility of improving the determination of neutrino mass and mixing, by exploiting the knowledge of Th/U abundance in the Earth.

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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