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Astrophysical S-factor of the 12N(p,)13O Reaction Determined from the (12N,13O) Proton Transfer Reaction

机译：在（12N，13O）质子转移反应中测定的12N（P，）13O反应的astrophysicals off

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The reaction cross section of the radiative proton capture on the drip line nucleus 12N was studied at the Cyclotron Institute at Texas A&M University. We have employed the indirect Asymptotic Normalization Coefficient method to determine the direct radiative component of the astrophysical S-factor of the 12N(p,)13O reaction. A value of 0.31(5) keV·b was found at zero energy. Interference between direct and resonant captures leads to a further enhancement of a factor of two. The reaction was investigated in relation to the evolution of hydrogen-rich massive objects, Population III stars, because of the role that it may play in the hot pp chain nuclear burning processes occurring in such stars.

机译：在德克萨斯A＆M大学的回旋历研究所研究了滴灌的质子捕获的反应横截面。我们采用间接渐近归一化系数方法来确定12N（P，）13O反应的天体物理S型的直接辐射成分。在零能量下发现0.31（5）kev·b的值。直接和谐振捕获之间的干扰导致进一步增强了两倍。研究了反应，研究了富含氢的大量物体，III颗恒星的演变，因为它可能在这种恒星中发生的热PP链核燃料过程中可能发挥作用。

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《Carpathian School of Physics》|2008年||共5页
会议地点
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A. Banu; T. Al.-Abdullah; V. Burjan; F. Carstoiu; C. Fu; C. A. Gagliardi; M. McCleskey; G. Tbcaru; L. Trache; R. E. Tribble;
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中图分类 P14-532;
关键词
Population III stars; radiative proton capture; ANC; DWBA;

机译：人口三星;辐射质子捕获;ANC;DWBA;

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1. 2-26 Experimental Measurement of 12N,13O on natPb Elastic Scattering Above the Coulomb Barriers [J] . Liu Xingquan, Yang Yanyun, Wang Jiansong, 中国科学院近代物理研究所和兰州重离子研究装置年报：英文版 . 2016,第001期
2. Measurement of 2H(12N, 13O)n Angular Distribution and Determination of Astrophysical 12N（p, γ）13O Reaction Rate [J] . GUO, Bing, SU, 中国原子能科学研究院年报：英文版 . 2012,第001期

机译：2 H（ 12 N， 13 O）n角分布的测量和天体物理 12 N（p ，γ） 13 O反应速率
3. Astrophysical Rates for 12N(p,γ)13O Direct Capture Reaction [J] . LI Zhi-Hong 中国物理快报：英文版 . 2006,第012期

机译：12N（p，γ）13O直接捕获反应的天文学速率
4. Estimates of the astrophysical S-factors for proton radiative capture by ~(10)B and ~(24)Mg nuclei using the ANCs from proton transfer reactions [J] . Artemov S.V., Igamov S.B., Karakhodzhaev A.A., International journal of modern physics, E. Nuclear physics . 2010,第5a6期

机译：使用质子转移反应的ANC估算〜（10）B和〜（24）Mg原子质子辐射俘获的天体S因子
5. Astrophysical S-factor of the 12N(p,)13O Reaction Determined from the (12N,13O) Proton Transfer Reaction [C] . A. Banu, T. Al.-Abdullah, V. Burjan, Carpathian School of Physics . 2008

机译：在（12N，13O）质子转移反应中测定的12N（P，）13O反应的astrophysicals off
6. Extracting the asymptotic normalization coefficients in neutron transfer reactions to determine the reaction rates for magnesium-22(proton,gamma)-aluminum-23 and fluorine-17(proton,gamma)-neon-18. [D] . Al-Abdullah, Tariq Abdalhamed. 2007

机译：提取中子转移反应的渐近归一化系数，以确定镁22（质子，γ）-铝23和氟17（质子，γ）-氖的反应速率。
7. Pathway of proton transfer in bacterial reaction centers: second-site mutation Asn-M44-->Asp restores electron and proton transfer in reaction centers from the photosynthetically deficient Asp-L213-->Asn mutant of Rhodobacter sphaeroides. [O] . S H Rongey, M L Paddock, G Feher, 2018

机译：细菌反应中心质子转移的途径：二级位点突变Asn-M44-> Asp恢复了光合缺陷型球形红球菌Asp-L213-> Asn突变体在反应中心的电子和质子转移。
8. Astrophysical S factor for the radiative capture 12N(p,gamma)13O determined from the 14N(12N,13O)13C proton transfer reaction [O] . Banu, A., Al-Abdullah, T., Fu, C., 2008

机译：用于辐射捕获的天体物理s因子12N（p，γ）13O 由14N（12N，13O）13C质子转移反应确定

Astrophysical S-factor of the 12N(p,)13O Reaction Determined from the (12N,13O) Proton Transfer Reaction

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