标题： 太阳中微子和太阳 显示英文标题

标题： Solar neutrinos and the sun

摘要： 我们提出了更新的标准太阳模型（SSMs），这些模型结合了最新的核聚变速率结果，最近已发表。 我们展示了高金属丰度和低金属丰度组成的日震学结果，以及另一种由3D模型大气推导出的太阳丰度集，其结果处于中间水平。 对于高金属丰度和低金属丰度模型，我们表明当前的太阳中微子数据无法区分这些模型，因此需要测量CNO通量才能实现这一目标。 讨论了假设测量CNO中微子的若干额外影响，包括在太阳和恒星物理方面的意义。 显示英文摘要

摘要： We present updated standard solar models (SSMs) that incorporate the latest results for nuclear fusion rates, recently published. We show helioseismic results for high and low metallicity compositions and also for an alternative set of solar abundance, derived from 3D model atmospheres, which give intermediate results. For the high and low metallicity models, we show that current solar neutrino data can not differentiate between models and that a measurement of the CNO fluxes is necessary to achieve that goal. A few additional implications of a hypothetical measurement of CNO neutrinos, both in terms of solar and stellar physics, are discussed.