New prospects for iodine detector and Solar neutrinos registration
The neutrino capture cross section σ(E) by 127I nucleus is studied with proper consideration of the nuclear strength function S(E) and its resonance structure. The calculations of giant Gamow-Teller, analog and pigmy resonances are realized based on the framework of the self-consistent finite Fermi...
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| Published in: | Physics letters. B Vol. 826; p. 136905 |
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10-03-2022
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| Abstract | The neutrino capture cross section σ(E) by 127I nucleus is studied with proper consideration of the nuclear strength function S(E) and its resonance structure. The calculations of giant Gamow-Teller, analog and pigmy resonances are realized based on the framework of the self-consistent finite Fermi systems theory. The results are compared with known experimental (p,n) reaction data that confirmed the significant influence of high-lying resonances on the cross section values. In the case when the energy of incident neutrino is higher than the sum of neutron emission threshold Sn and reaction threshold the 126Xe isotope is produced. Comparison of experimental yields for 127Xe and 126Xe isotopes can give the sensitive indicator of the metallicity for different Solar models. The results allow to confirm the advantages of the iodine detector for detecting hard astrophysical and accelerator neutrinos. |
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| AbstractList | The neutrino capture cross section σ(E) by 127I nucleus is studied with proper consideration of the nuclear strength function S(E) and its resonance structure. The calculations of giant Gamow-Teller, analog and pigmy resonances are realized based on the framework of the self-consistent finite Fermi systems theory. The results are compared with known experimental (p,n) reaction data that confirmed the significant influence of high-lying resonances on the cross section values. In the case when the energy of incident neutrino is higher than the sum of neutron emission threshold Sn and reaction threshold the 126Xe isotope is produced. Comparison of experimental yields for 127Xe and 126Xe isotopes can give the sensitive indicator of the metallicity for different Solar models. The results allow to confirm the advantages of the iodine detector for detecting hard astrophysical and accelerator neutrinos. |
| ArticleNumber | 136905 |
| Author | Fazliakhmetov, Almaz N. Klochkova, Nadezhda V. Lutostansky, Yuri S. Koroteev, Grigory A. Lutostansky, Andrey Y. Osipenko, Alexey P. Tikhonov, Victor N. |
| Author_xml | – sequence: 1 givenname: Yuri S. orcidid: 0000-0002-7391-5696 surname: Lutostansky fullname: Lutostansky, Yuri S. email: lutostansky@yandex.ru organization: National Research Center “Kurchatov Institute”, 123182 Moscow, Russia – sequence: 2 givenname: Almaz N. surname: Fazliakhmetov fullname: Fazliakhmetov, Almaz N. organization: National Research Center “Kurchatov Institute”, 123182 Moscow, Russia – sequence: 3 givenname: Grigory A. surname: Koroteev fullname: Koroteev, Grigory A. organization: National Research Center “Kurchatov Institute”, 123182 Moscow, Russia – sequence: 4 givenname: Nadezhda V. surname: Klochkova fullname: Klochkova, Nadezhda V. organization: National Research Center “Kurchatov Institute”, 123182 Moscow, Russia – sequence: 5 givenname: Andrey Y. surname: Lutostansky fullname: Lutostansky, Andrey Y. organization: National Research Center “Kurchatov Institute”, 123182 Moscow, Russia – sequence: 6 givenname: Alexey P. surname: Osipenko fullname: Osipenko, Alexey P. organization: National Research Center “Kurchatov Institute”, 123182 Moscow, Russia – sequence: 7 givenname: Victor N. surname: Tikhonov fullname: Tikhonov, Victor N. organization: National Research Center “Kurchatov Institute”, 123182 Moscow, Russia |
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| Cites_doi | 10.1103/RevModPhys.90.015008 10.1103/PhysRevLett.60.768 10.1016/S0920-5632(99)00383-7 10.1103/PhysRevC.68.054613 10.31857/S1234567820110014 10.1103/PhysRevD.53.4202 10.1103/PhysRevLett.67.430 10.1086/428929 10.1103/PhysRevC.50.1702 10.1016/S0375-9474(99)00070-6 10.1103/PhysRevC.59.500 10.1103/PhysRevLett.67.426 10.1088/1674-1137/41/3/030003 10.1016/0375-9474(94)00769-J 10.3847/1538-4357/835/2/202 10.3367/UFNr.0181.201109g.0975 10.1103/PhysRevLett.12.303 |
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| Title | New prospects for iodine detector and Solar neutrinos registration |
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