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The Future of Solar Neutrinos
Annual Review of Nuclear and Particle Science ( IF 9.1 ) Pub Date : 2021-09-21 , DOI: 10.1146/annurev-nucl-011921-061243
Gabriel D. Orebi Gann 1, 2 , Kai Zuber 3 , Daniel Bemmerer 4 , Aldo Serenelli 5, 6, 7
Affiliation  

In this article we review the current state of the field of solar neutrinos, including flavor oscillations, nonstandard effects, solar models, cross section measurements, and the broad experimental program thus motivated and enabled. We describe the historical discoveries that contributed to current knowledge, and define critical open questions to be addressed in the next decade. We discuss standard solar models, including uncertainties and problems related to the solar composition, and review experimental and model solar neutrino fluxes, including future prospects. We review the state of the art of the nuclear reaction data relevant for solar fusion in the proton–proton chain and carbon–nitrogen–oxygen cycle. Finally, we review the current and future experimental programs that can address outstanding questions in this field.

中文翻译:


太阳中微子的未来

在本文中,我们回顾了太阳中微子领域的当前状态,包括风味振荡、非标准效应、太阳模型、横截面测量以及由此激发和启用的广泛实验计划。我们描述了对当前知识做出贡献的历史发现,并定义了未来十年要解决的关键开放性问题。我们讨论标准太阳模型,包括与太阳组成有关的不确定性和问题,并回顾实验和模型太阳中微子通量,包括未来前景。我们回顾了与质子-质子链和碳-氮-氧循环中的太阳聚变相关的核反应数据的最新技术水平。最后,我们回顾了当前和未来可以解决该领域悬而未决问题的实验计划。

更新日期:2021-09-22
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