Interaction of Solar Neutrinos with 128Te and 130Te

IF 0.48 Q4 Physics and Astronomy

Bulletin of the Russian Academy of Sciences: Physics Pub Date : 2024-08-28 DOI:10.1134/S1062873824707347

Yu. S. Lutostansky, A. N. Fazliakhmetov, B. K. Lubsandorzhiev, N. A. Belogortseva, G. A. Koroteev, A. Yu. Lutostansky, V. N. Tikhonov

{"title":"Interaction of Solar Neutrinos with 128Te and 130Te","authors":"Yu. S. Lutostansky, A. N. Fazliakhmetov, B. K. Lubsandorzhiev, N. A. Belogortseva, G. A. Koroteev, A. Yu. Lutostansky, V. N. Tikhonov","doi":"10.1134/S1062873824707347","DOIUrl":null,"url":null,"abstract":"The interaction of solar neutrinos with the 128Te and 130Te isotopes was studied taking into account the resonance structure of charge-exchange strength functions S(E). An analysis was made of both experimental data on the strength functions S(E) obtained in the reactions (3He, t) and the strength functions S(E) calculated in the microscopic theory of finite Fermi systems. The resonance structure of the S(E) strength function was investigated, and the Gamow–Teller, analog, and pygmy resonances were identified. The capture cross sections σ(E) of solar neutrinos by the two isotopes were calculated with consideration of the resonance structure of the strength function S(E), and the influence of the resonances on the energy dependence σ(E) was analyzed. It was shown that, when calculating the cross section σ(E), the resonance structure of the strength function S(E) should be taken into account.","PeriodicalId":504,"journal":{"name":"Bulletin of the Russian Academy of Sciences: Physics","volume":"88 8","pages":"1223 - 1229"},"PeriodicalIF":0.4800,"publicationDate":"2024-08-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Bulletin of the Russian Academy of Sciences: Physics","FirstCategoryId":"1085","ListUrlMain":"https://link.springer.com/article/10.1134/S1062873824707347","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"Physics and Astronomy","Score":null,"Total":0}

引用次数: 0

Abstract

The interaction of solar neutrinos with the ¹²⁸Te and ¹³⁰Te isotopes was studied taking into account the resonance structure of charge-exchange strength functions S(E). An analysis was made of both experimental data on the strength functions S(E) obtained in the reactions (³He, t) and the strength functions S(E) calculated in the microscopic theory of finite Fermi systems. The resonance structure of the S(E) strength function was investigated, and the Gamow–Teller, analog, and pygmy resonances were identified. The capture cross sections σ(E) of solar neutrinos by the two isotopes were calculated with consideration of the resonance structure of the strength function S(E), and the influence of the resonances on the energy dependence σ(E) was analyzed. It was shown that, when calculating the cross section σ(E), the resonance structure of the strength function S(E) should be taken into account.

Abstract Image

查看原文本刊更多论文

太阳中微子与 128Te 和 130Te 的相互作用

摘要研究了太阳中微子与 128Te 和 130Te 同位素的相互作用，同时考虑了电荷交换强度函数 S(E) 的共振结构。研究分析了在反应（3He, t）中获得的强度函数S(E)的实验数据和有限费米系统微观理论计算的强度函数S(E)。研究了 S(E) 强度函数的共振结构，确定了伽莫-泰勒共振、模拟共振和侏儒共振。考虑到 S(E) 强度函数的共振结构，计算了两种同位素对太阳中微子的俘获截面 σ(E)，并分析了共振对能量依赖性 σ(E)的影响。结果表明，在计算横截面 σ(E) 时，应考虑强度函数 S(E) 的共振结构。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

求助全文

约1分钟内获得全文求助全文

来源期刊

Bulletin of the Russian Academy of Sciences: Physics Physics and Astronomy-Physics and Astronomy (all)

CiteScore

0.90

自引率

0.00%

发文量

251

期刊介绍： Bulletin of the Russian Academy of Sciences: Physics is an international peer reviewed journal published with the participation of the Russian Academy of Sciences. It presents full-text articles (regular, letters to the editor, reviews) with the most recent results in miscellaneous fields of physics and astronomy: nuclear physics, cosmic rays, condensed matter physics, plasma physics, optics and photonics, nanotechnologies, solar and astrophysics, physical applications in material sciences, life sciences, etc. Bulletin of the Russian Academy of Sciences: Physics focuses on the most relevant multidisciplinary topics in natural sciences, both fundamental and applied. Manuscripts can be submitted in Russian and English languages and are subject to peer review. Accepted articles are usually combined in thematic issues on certain topics according to the journal editorial policy. Authors featured in the journal represent renowned scientific laboratories and institutes from different countries, including large international collaborations. There are globally recognized researchers among the authors: Nobel laureates and recipients of other awards, and members of national academies of sciences and international scientific societies.