Resonance strengths in the N-14(p, gamma)O-15 astrophysical key reaction measured with activation

Gyurky Gy; Halasz Z.; Kiss G. G.; Szucs T.; Csik A.; Torok Zs; Huszank R.; Kohan M. G.; Wagner L.; Fulop Zs

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Resonance strengths in the N-14(p, gamma)O-15 astrophysical key reaction measured with activation

机译：用活化测量的N-14（P，γ）O-15天体物理关键反应中的共振优点

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Background: The N-14(p, gamma)O-15 reaction plays a vital role in various astrophysical scenarios. Its reaction rate must be accurately known in the present era of high precision astrophysics. The cross section of the reaction is often measured relative to a low energy resonance, the strength of which must therefore be determined precisely.

机译：背景：N-14（p，γ）O-15反应在各种天体物理场景中起着至关重要的作用。其反应速率必须在高精度天体物理学的现代时代准确。反应的横截面通常相对于低能量共振测量，因此必须精确地确定其强度。

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《Physical review, C》 |2019年第1期|共8页
作者
Gyurky Gy; Halasz Z.; Kiss G. G.; Szucs T.; Csik A.; Torok Zs; Huszank R.; Kohan M. G.; Wagner L.; Fulop Zs;
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作者单位

Inst Nucl Res Atomki H-4001 Debrecen Hungary;

Inst Nucl Res Atomki H-4001 Debrecen Hungary;

Inst Nucl Res Atomki H-4001 Debrecen Hungary;

Inst Nucl Res Atomki H-4001 Debrecen Hungary;

Inst Nucl Res Atomki H-4001 Debrecen Hungary;

Inst Nucl Res Atomki H-4001 Debrecen Hungary;

Inst Nucl Res Atomki H-4001 Debrecen Hungary;

Lulea Univ Technol Dept Engn Sci &

Math S-97187 Lulea Sweden;

HZDR D-01328 Dresden Germany;

Inst Nucl Res Atomki H-4001 Debrecen Hungary;

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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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2. Resonance strengths in the N-14(p, gamma)O-15 astrophysical key reaction measured with activation [J] . Gyurky Gy, Halasz Z., Kiss G. G., Physical review, C . 2019,第1期

机译：用活化测量的N-14（P，γ）O-15天体物理关键反应中的共振优点
3. Measurement of the E-r(c.m.)=259 ke V resonance in the N-14(p,gamma)O-15 reaction [J] . Daigle S., Kelly K. J., Champagne A. E., Physical review, C . 2016,第2期

机译：在N-14（p，γ）O-15反应中测量E-R（C.）= 259ke V共振
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5. Resonance strength measurement at astrophysical energies: The ~(17)0(p,α)~(14)N reaction studied via THM [C] . M.L. Sergi, C. Spitaleri, M. La Cognata, International Conference on Nucleus-Nucleus Collisions . 2016

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6. New measurements for the astrophysically important calcium-40(alpha,gamma)titanium-44 reaction. [D] . Robertson, Daniel J. 2010

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8. Publisher's Note: Asymptotic normalization coefficients for N-14+p -> O-15 and the astrophysical S factor for N-14(p,gamma)O-15 (vol 67, art no 065804, 2003) [O] . Mukhamedzhanov, AM, Bem, P., Brown, BA, 2003

机译：发行者的注释：N-14 + p-> O-15的渐近归一化系数和N-14（p，gamma）O-15的天体S因子（第67卷，艺术品编号0680804，2003）
9. Resonance Strength Measurements and Thermonuclear Reaction Rates for exp 25 Mg(P, gamma ) exp 26 Al [R] . Anderson, M. R., Mitchell, L. W., Sevior, M. E., 1981

机译：exp 25 mg（p，gamma）exp 26 al的共振强度测量和热核反应速率

Resonance strengths in the N-14(p, gamma)O-15 astrophysical key reaction measured with activation

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