邻近恒星聚变中微子的预测和探测潜力
Prediction and detection potential of fusion neutrinos from nearby stars
摘要：
计算了太阳附近10秒差距以内的代表恒星的中微子谱和通量的形状。最重要的，具体的恒星物体（α-半人马座系统，天狼星A，南河三，织女星，北落师门和牛郎星）的个人贡献的详细恒星建模确定和调查。潜在的检测的可能性进行了讨论。
英文摘要：
The shapes of neutrino spectra and fluxes from representative stars in the solar neighborhood up to 10 pc are calculated. The individual contribution of the most important, specific stellar objects (the alpha-Centauri system, Sirius A, Procyon, Vega, Fomalhaut and Altair) are determined and investigated by detailed stellar modeling. The possibility for a potential detection is discussed.
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。
