The reaction rate of radiative n8Li capture in the range from 0.01 to 10 T9

IF 2.6 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
S. Dubovichenko, B. Yeleusheva, N. Burkova, A. Tkachenko
{"title":"The reaction rate of radiative n8Li capture in the range from 0.01 to 10 T9","authors":"S. Dubovichenko, B. Yeleusheva, N. Burkova, A. Tkachenko","doi":"10.3389/fspas.2023.1251743","DOIUrl":null,"url":null,"abstract":"Within the modified potential cluster model (MPCM) with forbidden states, the total cross sections are calculated for capture in the ground and first excited states of the 9Li nucleus in the n8Li channel in the energy range from 10−5 eV to 5 MeV based on Е1 and M1 transitions. The experimentally proved resonance at Ec.m. = 0.232 MeV in the 4P5/2 wave and ab initio-predicted 4P3/2 resonance at 1.32 MeV [Phys. Rev. C 103, 035801 (2021)] are considered. The strong impact of the asymptotic constant and channel spectroscopic factors on the total capture cross sections are responsible for the variation in the absolute values within factor two. As a consequence, the thermal cross sections are σtherm= 24–46.8 mb. The evaluation of σtherm based on the extrapolation of ab initio cross sections yields ∼85 mb. The reaction rate is calculated in the temperature range from 0.01 to 10 T9. The reported reaction rates are compared at the benchmark point 1 T9. The comparison of two datasets [Phys. Rev. C 103, 035801 (2021) and Phys. Rev. C 105, 064608 (2022)] on reaction rates recently calculated in microscopic models in extended temperature intervals shows the essential quantitative and qualitative differences. The comparative joint analysis of the reaction rates of radiative neutron capture on the lithium isotopes 6,7,8Li is suggested for the choice of an optimal interval for the asymptotic constants.","PeriodicalId":46793,"journal":{"name":"Frontiers in Astronomy and Space Sciences","volume":" ","pages":""},"PeriodicalIF":2.6000,"publicationDate":"2023-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Frontiers in Astronomy and Space Sciences","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.3389/fspas.2023.1251743","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

Abstract

Within the modified potential cluster model (MPCM) with forbidden states, the total cross sections are calculated for capture in the ground and first excited states of the 9Li nucleus in the n8Li channel in the energy range from 10−5 eV to 5 MeV based on Е1 and M1 transitions. The experimentally proved resonance at Ec.m. = 0.232 MeV in the 4P5/2 wave and ab initio-predicted 4P3/2 resonance at 1.32 MeV [Phys. Rev. C 103, 035801 (2021)] are considered. The strong impact of the asymptotic constant and channel spectroscopic factors on the total capture cross sections are responsible for the variation in the absolute values within factor two. As a consequence, the thermal cross sections are σtherm= 24–46.8 mb. The evaluation of σtherm based on the extrapolation of ab initio cross sections yields ∼85 mb. The reaction rate is calculated in the temperature range from 0.01 to 10 T9. The reported reaction rates are compared at the benchmark point 1 T9. The comparison of two datasets [Phys. Rev. C 103, 035801 (2021) and Phys. Rev. C 105, 064608 (2022)] on reaction rates recently calculated in microscopic models in extended temperature intervals shows the essential quantitative and qualitative differences. The comparative joint analysis of the reaction rates of radiative neutron capture on the lithium isotopes 6,7,8Li is suggested for the choice of an optimal interval for the asymptotic constants.
辐射俘获n8Li的反应速率在0.01~10T9范围内
在具有禁用态的改进势簇模型(MPCM)中,基于ε1和M1跃迁,计算了n8Li通道中9Li核在10−5 eV至5 MeV能量范围内的基态和第一激发态捕获的总截面。考虑了实验证明的4P5/2波中Ec.m=0.232 MeV的共振和从头计算预测的1.32 MeV的4P3/2共振[Phys.Rev.C10035801(2021)]。渐近常数和通道光谱因子对总捕获截面的强烈影响是因子二内绝对值变化的原因。因此,热横截面为σtherm=24–46.8 mb。基于从头算横截面外推的σtherm评估产生~85 mb。反应速率是在0.01至10T9的温度范围内计算的。报告的反应速率在基准点1 T9处进行比较。两个数据集[Phys.Rev.C 103035801(2021)和Phys.Rev.C 105064608(2022)]关于最近在延长温度区间的微观模型中计算的反应速率的比较显示了本质的定量和定性差异。建议对锂同位素6,7,8Li的辐射中子捕获反应速率进行比较联合分析,以选择渐近常数的最佳区间。
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
Frontiers in Astronomy and Space Sciences
Frontiers in Astronomy and Space Sciences ASTRONOMY & ASTROPHYSICS-
CiteScore
3.40
自引率
13.30%
发文量
363
审稿时长
14 weeks
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信