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arXiv · 2407.10357

Solar neutrino capture by 128, 130Te isotopes and Baksan Large Neutrino Telescope Project

A. N. Fazliakhmetov·Yu. S. Lutostansky·B. K. Lubsandorzhiev·G. A. Koroteev·V. N. Tikhonov
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Abstract

This paper discusses the charge-exchange strength functions $S(E)$ of the isotopes $^{128,130}$Te. The experimental data of the $S(E)$ strength functions obtained from $(^{3}\mathrm{He}, t)$ reactions, as well as the $S(E)$ strength functions calculated in the microscopic theory of finite fermi-systems, are analyzed. The resonance structure of the strength function $S(E)$ is examined, and the Gamow-Teller and Pygmy resonances are identified. The resonance structure of the strength function $S(E)$ is vital for the calculation and analysis of the process of neutrino capture by atomic nuclei.

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A. N. Fazliakhmetov, Yu. S. Lutostansky, B. K. Lubsandorzhiev, G. A. Koroteev, V. N. Tikhonov. 2024-07-14. Solar neutrino capture by 128, 130Te isotopes and Baksan Large Neutrino Telescope Project. https://arxiv.org/abs/2407.10357

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