Effective stellar beta-decay rates of nuclei with long-lived isomers: Al-26 and Cl-34

Banerjee Projjwal; Misch G. Wendell; Ghorui Surja K.; Sun Yang

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Effective stellar beta-decay rates of nuclei with long-lived isomers: Al-26 and Cl-34

机译：长寿命异构体的核的有效甾体β - 衰减率：Al-26和Cl-34

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来源
《Physical review, C》 |2018年第6期|共8页
作者
Banerjee Projjwal; Misch G. Wendell; Ghorui Surja K.; Sun Yang;
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作者单位

Shanghai Jiao Tong Univ Sch Phys &

Astron Dept Astron Shanghai 200240 Peoples R China;

Shanghai Jiao Tong Univ Sch Phys &

Astron Dept Phys Shanghai 200240 Peoples R China;

Shanghai Jiao Tong Univ Sch Phys &

Astron Dept Phys Shanghai 200240 Peoples R China;

Shanghai Jiao Tong Univ Sch Phys &

Astron Dept Phys Shanghai 200240 Peoples R China;

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正文语种 eng
中图分类原子核物理学、高能物理学;
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专利

1. Effective stellar beta-decay rates of nuclei with long-lived isomers: Al-26 and Cl-34 [J] . Banerjee Projjwal, Misch G. Wendell, Ghorui Surja K., Physical review, C . 2018,第6期

机译：长寿命异构体的核的有效甾体β - 衰减率：Al-26和Cl-34
2. Reducing Uncertainties in the Production of the Gamma-emitting Nuclei Al-26, Ti-44, and Fe-60 in Core-collapse Supernovae by Using Effective Helium Burning Rates [J] . Austin Sam M., West Christopher, Heger Alexander The Astrophysical Journal. Letters . 2017,第1期

机译：通过使用有效的氦燃烧率，减少核糖核Al-26，Ti-44和Fe-60中的不确定因素
3. Reducing Uncertainties in the Production of the Gamma-emitting Nuclei Al-26, Ti-44, and Fe-60 in Core-collapse Supernovae by Using Effective Helium Burning Rates [J] . Austin Sam M., West Christopher, Heger Alexander The Astrophysical Journal. Letters . 2017,第1期

机译：通过使用有效的氦燃烧率，减少核糖核Al-26，Ti-44和Fe-60中的不确定因素
4. Beta-decay and Electron Capture Rates of Hot Nuclei in Stellar Matter [C] . Semyon V. Sidorov, Alan A. Dzhioev, Tatyana Yu. Tretyakova International Scientific Conference of Young Scientists and Specialists . 2019

机译：恒星物质的β-腐烂和电子捕获率的热核
5. Beta-decay rates of nuclei in ground and excited states and effects on the r-process of nucleosynthesis. [D] . Famiano, Michael Andrew. 2001

机译：处于基态和激发态的核的β衰变速率及其对核合成r过程的影响。
6. Optical evidence for the unification of active galactic nuclei and quasi-stellar objects. [O] . J S Miller 1995

机译：活跃的银河核和准星状物体统一的光学证据。
7. Stellar weak-interaction rates for sd-shell nuclei. I - Nuclear matrix element systematics with application to Al-26 and selected nuclei of importance to the supernova problem [O] . G. M. Fuller, W. A. Fowler, M. J. Newman 1980

机译：SD-Shell核的恒星弱相互作用率。 i - 核基质元素系统，应用于Al-26，并选择对超新星问题的重视核
8. New stellar reaction rates for Mg-25 (p,gamma) Al-26 and Al-25 (p,gamma) Si-26 [R] . Iliadis, C. , Buchmann, P. M. , Endt, P. M. 1995

机译：mg-25（p，γ）al-26和al-25（p，γ）si-26的新恒星反应速率

Effective stellar beta-decay rates of nuclei with long-lived isomers: Al-26 and Cl-34

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