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

2024/07/14 by A. N. Fazliakhmetov, Yu. S. Lutostansky, Fazliakhmetov, A. N. +7
Physics and Astronomy · #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #Neutrino Physics Research #Nuclear Experiment (nucl-ex) #Nuclear Theory (nucl-th) #Particle physics theoretical and experimental studies

paper · pdf · doi:10.48550/arxiv.2407.10357

openalex publication_date 2024/07/14 · openalex created_date 2024/07/17 · openalex updated_date 2026/07/28

Abstract

This paper discusses the charge-exchange strength functions S(E) of the isotopes 128,130Te. The experimental data of the S(E) strength functions obtained from (3He, 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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