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학술연구/단체지원/교육 등 연구자 활동을 지속하도록 DBpia가 지원하고 있어요.
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초록· 키워드
오류제보하기
The radiative proton capture on <SUP>15</SUP>N targets, i.e., <SUP>15</SUP>N(p, γ)<SUP>16</SUP>O, is an important thermonuclear reaction of the CNO cycle in stellar environments. This reaction is a key process in the cycle because it initiates the NO cycle by producing <SUP>16</SUP>O. In this study, we investigated the <SUP>15</SUP>N(p, γ)<SUP>16</SUP>O reaction within the framework of cluster effective field theory. We construct an effective Lagrangian to describe the reaction at stellar energies and calculate the astrophysical S factor. The parameters of our calculations, such as low-energy constants, resonance energy, and decay width of the <SUP>16</SUP>O resonance are determined by fitting empirical data of the S factor at the range of 72.8 keV ≤ E<SUB>cm</SUB> ≤ 368.3 keV. The S factor value for this reaction at extremely low energy is then determined to be S(E = 0) = 30.4 keV·b, which is consistent with the estimates of R-matrix approaches.
목차
Ⅰ. INTRODUCTION
Ⅱ. EFFECTIVE LAGRANGIAN
Ⅲ. RADIATIVE CAPTURE AMPLITUDE
Ⅳ. RESULTS
Ⅴ. SUMMARY
REFERENCES
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