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Status of theMg24(α,γ)Si28reaction rate at stellar temperatures
Physical Review C ( IF 3.1 ) Pub Date : 2020-07-07 , DOI: 10.1103/physrevc.102.015801 P. Adsley , A. M. Laird , Z. Meisel
Physical Review C ( IF 3.1 ) Pub Date : 2020-07-07 , DOI: 10.1103/physrevc.102.015801 P. Adsley , A. M. Laird , Z. Meisel
Background: The reaction influences the production of magnesium and silicon isotopes during carbon burning and is one of eight reaction rates found to significantly impact the shape of calculated x-ray burst light curves. The reaction rate is based on measured resonance strengths and known properties of levels in .
中文翻译:
恒星温度下Mg24(α,γ)Si28反应速率的状态
背景:在该反应会影响碳燃烧过程中镁和硅同位素的产生,并且是显着影响所计算的X射线猝发光曲线形状的八种反应速率之一。反应速率是基于测得的共振强度和已知水平的特性。
更新日期:2020-07-07
中文翻译:
恒星温度下Mg24(α,γ)Si28反应速率的状态
背景:在该反应会影响碳燃烧过程中镁和硅同位素的产生,并且是显着影响所计算的X射线猝发光曲线形状的八种反应速率之一。反应速率是基于测得的共振强度和已知水平的特性。