This study has indicated that the resonance structure of the charge-exchange strength function S(E) strongly affects the cross section for solar neutrino capture σ(E) by the ¹²⁷I nucleus. The effect of each resonance on the energy dependence of σ(E) for an iodine detector has been analyzed. It has been shown that all high-lying charge-exchange resonances should be taken into account in the calculations of the cross section σ(E), and the highest energy resonances in the strength function S(E) determine the formation of the stable ¹²⁶Xe isotope at the capture of a high-energy solar neutrino by the ¹²⁷I nucleus and the subsequent neutron emission from the formed ¹²⁷Xe isotope. The calculations with the inclusion of the neutron separation energy S_n in the ¹²⁷Xe nucleus show that the inclusion of the neutron separation energy S_n reduces the neutrino capture rate, particularly for boron and hep neutrinos, and the ¹²⁶Xe/¹²⁷Xe isotope ratio is an indicator of these hard neutrinos. It has been found that the formation of the ¹²⁶Xe isotope is accompanied by the emission of gamma-ray photons with a certain energy. It has been shown that the analysis of the ¹²⁶Xe/¹²⁷Xe isotope ratio in the formed xenon gas mixture and the detection of gamma emission in ¹²⁶Xe open new capabilities of the iodine detector for the detection of solar neutrinos and make it possible to separate the important boron component of the solar spectrum.

中文翻译：

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太阳中微子碘探测器的新功能

这项研究表明，电荷交换强度函数S（E）的共振结构强烈影响¹²⁷ I核对太阳中微子俘获σ（E）的截面。分析了每种共振对碘检测器的σ（E）能量依赖性的影响。已经表明，在计算横截面σ（E）时应考虑所有高电荷交换共振，并且强度函数S（E）中最高的能量共振决定了稳定体¹²⁶的形成。Xe同位素在高能太阳中微子的俘获下¹²⁷ I核和随后形成的¹²⁷ Xe同位素的中子发射。由于包含的中子分离能量的计算š _Ñ在¹²⁷ Xe的细胞核显示，中子分离能量列入小号_Ñ降低中微子捕获率，特别是对于硼和HEP中微子，和¹²⁶的Xe / ¹²⁷ Xe的同位素比是这些硬中微子的指标。已经发现，¹²⁶ Xe同位素的形成伴随着具有一定能量的伽马射线光子的发射。已经证明对¹²⁶ Xe / ¹²⁷的分析形成的氙气混合物中的Xe同位素比和¹²⁶ Xe中的γ发射检测为检测太阳中微子提供了碘检测器的新功能，并使分离太阳光谱中重要的硼成分成为可能。