国家自然科学基金(11075219)
- 作品数：9 被引量：0H指数：0
- 相关作者：何建军于祥庆李龙张立勇李二涛更多>>
- 相关机构：中国科学院近代物理研究所深圳大学北京航空航天大学更多>>
- 发文基金：国家自然科学基金国家重点基础研究发展计划更多>>
- 相关领域：理学天文地球更多>>
- 利用转移反应12C(11B,~7Li)16O研究12C（α,γ）16O反应
- ＜正＞
- 杜先超郭冰李志宏李云居苏俊颜胜权白希祥樊启文甘林金孙均景龙李二涛李志常连钢刘建成谌阳平唐晓东王友宝吴志丹曾晟张伟杰柳卫平
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- Indirect Study of 12C(α,γ)16O Reaction via Study of 12C(11B,7Li)16O Transfer Reaction
- C(α,γ)O reaction plays a crucial role in stellar nucleosynthesis.To date the lowest energy of the measurement ...
- DU Xian-chaoGUO BingLI Zhi-hongLI Yun-juSU JunYAN Sheng-quanBAI Xi-xiangFAN Qi-wenGAN LinJIN Sun-junJING LongLI Er-taoLI Zhi-changLIAN GangLIU Jian-chengSHEN Yang-pingTANG Xiao-dongWANG You-baoWU Zhi-danZENG ShengZHANG Wei-jieLIU Wei-ping
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- 16N阈下态中子谱因子及15N（n,γ）16N天体物理反应率
- ＜正＞氟对恒星中的物理条件极其敏感,因此,它对于核合成研究而言是一种重要的元素。产生氟的天体物理场所为渐进巨支（AGB）星。在AGB星中,
- 吴志丹郭冰李志宏李云居苏俊庞丹阳颜胜权李二涛白希祥杜先超樊启文甘林何建军金孙均景龙李龙李志常连钢刘建成谌阳平王友宝于祥庆曾晟张立勇张伟杰柳卫平
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- Spectroscopic Factors for Low-lying 16N Levels and Astrophysical 15N(n,γ)16N Reaction Rate
- Fluorine is a key element for nucleosynthetic studies since it is extremely sensitive to the physical conditio...
- WU Zhi-danGUO BingLI Zhi-hongLI Yun-juSU JunPAN Dan-yangYAN Sheng-quanLI Er-taoBAI Xi-xiangDU Xian-chaoFAN Qi-wenGAN LinHE Jian-junJIN Sun-junJING LongLI LongLI Zhi-changLIAN GangLIU Jian-chengSHEN Yang-pingWANG You-baoYU Xiang-qingZENG ShengZHANG Li-yongZHANG Wei-jieLIU Wei-ping
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- 利用15N（~7Li,~6Li）16N反应导出16F阈下态的能级宽度
- ＜正＞
- 吴志丹郭冰李志宏李云居苏俊庞丹阳颜胜权李二涛白希祥杜先超樊启文甘林何建军金孙均景龙李龙李志常连钢刘建成谌阳平王友宝于祥庆曾晟张东海张立勇张伟杰柳卫平
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- Level Widths of Low-lying 16F States From 15N(7Li,6Li)16N Reaction
- All theF levels are unbound by proton emission.To date,the four low-lyingF levels below1 MeV have been experim...
- WU Zhi-danGUO BingLI Zhi-hongLI Yun-juSU JunPAN Dan-yangYAN Sheng-quanLI Er-taoBAI Xi-xiangDU Xian-chaoFAN Qi-wenGAN LinHE Jian-junJIN Sun-junJING LongLI LongLI Zhi-changLIAN GangLIU Jian-chengSHEN Yang-pingWANG You-baoYU Xiang-qingZENG ShengZHANG Dong-haiZHANG Li-yongZHANG Wei-jieLIU Wei-ping
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