Publication Date:
2018-01-04
Description:
Author(s): D. Kahl, H. Yamaguchi (山口英斉), S. Kubono (久保野茂), A. A. Chen, A. Parikh, D. N. Binh, J. Chen (陈俊), S. Cherubini, N. N. Duy, T. Hashimoto (橋本尚志), S. Hayakawa (早川勢也), N. Iwasa (岩佐直仁), H. S. Jung (정효순), S. Kato (加藤静吾), Y. K. Kwon (권영관), S. Nishimura (西村俊二), S. Ota (大田晋輔), K. Setoodehnia, T. Teranishi (寺西高), H. Tokieda (時枝紘史), T. Yamada (山田拓), C. C. Yun (윤종철), and L. Y. Zhang (张立勇) Background: Type I x-ray bursts are the most frequently observed thermonuclear explosions in the galaxy, resulting from thermonuclear runaway on the surface of an accreting neutron star. The S 30 ( α , p ) reaction plays a critical role in burst models, yet insufficient experimental information is availab... [Phys. Rev. C 97, 015802] Published Wed Jan 03, 2018
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics
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