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arXiv 0710.2944nucl-ex
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~(13)C和~(13)N第一个T=1/2,J^pi=3/2态的Gamow-Teller强度及其对Ia型超新星的意义

Gamow-Teller strength for the analog transitions to the first T=1/2, J^pi=3/2- states in 13C and 13N and the implications for Type Ia supernovae

R. G. T. Zegers, E. F. Brown, H. Akimune, Sam M. Austin, A. M. van den Berg, B. A. Brown, D. A. Chamulak, Y. Fujita, M. Fujiwara, S. Gal`es, M. N. Harakeh, H. H… 展开作者

R. G. T. Zegers, E. F. Brown, H. Akimune, Sam M. Austin, A. M. van den Berg, B. A. Brown, D. A. Chamulak, Y. Fujita, M. Fujiwara, S. Gal`es, M. N. Harakeh, H. Hashimoto, R. Hayami, G. W. Hitt, M. Itoh, T. Kawabata, K. Kawase, M. Kinoshita, K. Nakanishi, S. Nakayama, S. Okamura, Y. Shimbara, M. Uchida, H. Ueno, T. Yamagata, M. Yosoi

摘要:

利用420 MeV的~(13)C(~ 3 He,t)反应,计算了~(13)C基态到T=1/2,J^pi=3/2-激发态的跃迁强度.与以前的(p,n)~(13)C研究结果相比,本文的结果与壳模型计算和其它核的经验单位截面系统学符合得很好,并用于研究类似的~(13)N(e-,v_e)~(13)C反应,它在Ia型超新星爆发前的对流阶段起作用。虽然从(3 He,t)和(p,n)数据的结果之间的差异显着影响推断的电子捕获率和净热沉积在恒星由于这种转变,对爆炸前的演变的整体影响是很小的。

英文摘要:

The Gamow-Teller strength for the transition from the ground state of 13C to the T=1/2, J^pi=3/2- excited state at 3.51 MeV in 13N is extracted via the 13C(3He,t) reaction at 420 MeV. In contrast to results from earlier (p,n) studies on 13C, a good agreement with shell-model calculations and the empirical unit cross section systematics from other nuclei is found. The results are used to study the analog 13N(e-,v_e)13C reaction, which plays a role in the pre-explosion convective phase of type Ia supernovae. Although the differences between the results from the (3He,t) and (p,n) data significantly affect the deduced electron-capture rate and the net heat-deposition in the star due to this transition, the overall effect on the pre-explosive evolution is small.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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