arXiv · 2303.17752
Interaction of solar neutrinos with $^{98,100}$Mo isotopes and the influence of nuclear resonances
Abstract
The process of neutrino interaction with $^{98}$Mo and $^{100}$Mo isotopes is studied taking into consideration the effect of charge-exchange resonances. The experimental data on the strength functions $S(E)$ obtained in charge-exchange reactions $(p; n)$ and $(^3\mathrm{He}, t)$ and the strength functions $S(E)$ calculated within the theory of finite Fermi systems were used. We studied the effect of the resonance structure of $S(E)$ on the cross sections for solar-neutrino. We investigated the contribution of each high-lying resonance to the capture cross section $\sigma(E_{\nu})$. The contributions of all components of the solar neutrino spectrum are calculated. We estimate the contribution of different components of solar neutrinos as the background for the double-beta decay experiments on $^{100}$Mo.
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Yu. S. Lutostansky, A. N. Fazliakhmetov, G. A. Koroteev, V. N. Tikhonov, A. Yu. Lutostansky, N. V. Klochkova, A. P. Osipenko, N. A. Belogortseva, E. Yu. Zemskov. 2023-03-31. Interaction of solar neutrinos with $^{98,100}$Mo isotopes and the influence of nuclear resonances. https://arxiv.org/abs/2303.17752
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