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Neutron activation ofGa69andGa71atkBT≈25keV
Physical Review C ( IF 3.1 ) Pub Date : 2021-02-12 , DOI: 10.1103/physrevc.103.025802 Kathrin Göbel , Clemens Beinrucker , Benjamin Brückner , Philipp Erbacher , Stefan Fiebiger , Micaela Fonseca , Michael Heftrich , Tanja Heftrich , Franz Käppeler , Antonin Krása , Deniz Kurtulgil , Claudia Lederer-Woods , Ralf Plag , Arjan Plompen , René Reifarth , Stefan Schmidt , Kerstin Sonnabend , Mario Weigand
Physical Review C ( IF 3.1 ) Pub Date : 2021-02-12 , DOI: 10.1103/physrevc.103.025802 Kathrin Göbel , Clemens Beinrucker , Benjamin Brückner , Philipp Erbacher , Stefan Fiebiger , Micaela Fonseca , Michael Heftrich , Tanja Heftrich , Franz Käppeler , Antonin Krása , Deniz Kurtulgil , Claudia Lederer-Woods , Ralf Plag , Arjan Plompen , René Reifarth , Stefan Schmidt , Kerstin Sonnabend , Mario Weigand
Background: About 50% of heavy elements are produced by the slow neutron capture process ( process) in stars. The element gallium is mostly produced during the weak process in massive stars.
中文翻译:
Ga69和Ga71atkBT≈25keV的中子活化
背景:约50%的重元素是通过缓慢的中子捕获过程产生的(过程)。元素镓主要在弱势期间产生 大质量恒星的过程。
更新日期:2021-02-12
中文翻译:
Ga69和Ga71atkBT≈25keV的中子活化
背景:约50%的重元素是通过缓慢的中子捕获过程产生的(过程)。元素镓主要在弱势期间产生 大质量恒星的过程。