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pro vyhledávání: '"R G, Ma"'
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Autor:
L. Y. Zhang, J. Su, J. J. He, R. J. deBoer, D. Kahl, M. Wiescher, D. Odell, Y. J. Chen, X. Y. Li, J. G. Wang, L. Zhang, F. Q. Cao, H. Zhang, Z. C. Zhang, T. Y. Jiao, Y. D. Sheng, L. H. Wang, L. Y. Song, X. Z. Jiang, Z. M. Li, E. T. Li, S. Wang, G. Lian, Z. H. Li, B. Guo, X. D. Tang, L. T. Sun, Q. Wu, J. Q. Li, B. Q. Cui, L. H. Chen, R. G. Ma, N. C. Qi, W. L. Sun, X. Y. Guo, P. Zhang, Y. H. Chen, Y. Zhou, J. F. Zhou, J. R. He, C. S. Shang, M. C. Li, J. P. Cheng, W. P. Liu
Publikováno v:
Physical Review C. 106
Autor:
B, Gao, T Y, Jiao, Y T, Li, H, Chen, W P, Lin, Z, An, L H, Ru, Z C, Zhang, X D, Tang, X Y, Wang, N T, Zhang, X, Fang, D H, Xie, Y H, Fan, L, Ma, X, Zhang, F, Bai, P, Wang, Y X, Fan, G, Liu, H X, Huang, Q, Wu, Y B, Zhu, J L, Chai, J Q, Li, L T, Sun, S, Wang, J W, Cai, Y Z, Li, J, Su, H, Zhang, Z H, Li, Y J, Li, E T, Li, C, Chen, Y P, Shen, G, Lian, B, Guo, X Y, Li, L Y, Zhang, J J, He, Y D, Sheng, Y J, Chen, L H, Wang, L, Zhang, F Q, Cao, W, Nan, W K, Nan, G X, Li, N, Song, B Q, Cui, L H, Chen, R G, Ma, S Q, Yan, J H, Liao, Y B, Wang, S, Zeng, D, Nan, Q W, Fan, N C, Qi, W L, Sun, X Y, Guo, P, Zhang, Y H, Chen, Y, Zhou, J F, Zhou, J R, He, C S, Shang, M C, Li, S, Kubono, W P, Liu, R J, deBoer, M, Wiescher, M, Pignatari
The ^{13}C(α,n)^{16}O reaction is the main neutron source for the slow-neutron-capture process in asymptotic giant branch stars and for the intermediate process. Direct measurements at astrophysical energies in above-ground laboratories are hindered
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::32fb9ef1ad6a097337fa83b95df12888
Autor:
J. Su, SongPo Xu, You Zhou, Z. C. Zhang, E. T. Li, Feng-Shou Zhang, Z. M. Li, X. Tang, Qi Wu, X. Y. Li, J. Li, Yue Chen, J. J. He, X. Y. Guo, Y. H. Zhang, Michael Wiescher, Richard deBoer, H. Y. Zhang, Litao Sun, Jing Zhou, N. C. Qi, G. Lian, X. Z. Jiang, T. Y. Jiao, J. R. He, H. S. Xu, Z. G. Hu, B. Guo, Mengran Li, Peng Zhang, L. Zhang, Y. D. Sheng, D. Kahl, Jie Wang, Shuangxi Wang, Lei Wang, Ye Chen, Lufeng Zhang, B. Q. Cui, C. S. Shang, L. H. Chen, J. P. Chen, J. Q. Li, Hai-Hui Zhao, X. H. Zhou, W. L. Sun, Z. H. Li, F. Q. Cao, R. G. Ma, L. Y. Song, W. P. Liu
Publikováno v:
Physical Review Letters. 127
Fluorine is one of the most interesting elements in nuclear astrophysics, where the ^{19}F(p,α)^{16}O reaction is of crucial importance for Galactic ^{19}F abundances and CNO cycle loss in first generation Population III stars. As a day-one campaign
Autor:
L Y, Zhang, J, Su, J J, He, M, Wiescher, R J, deBoer, D, Kahl, Y J, Chen, X Y, Li, J G, Wang, L, Zhang, F Q, Cao, H, Zhang, Z C, Zhang, T Y, Jiao, Y D, Sheng, L H, Wang, L Y, Song, X Z, Jiang, Z M, Li, E T, Li, S, Wang, G, Lian, Z H, Li, X D, Tang, H W, Zhao, L T, Sun, Q, Wu, J Q, Li, B Q, Cui, L H, Chen, R G, Ma, B, Guo, S W, Xu, J Y, Li, N C, Qi, W L, Sun, X Y, Guo, P, Zhang, Y H, Chen, Y, Zhou, J F, Zhou, J R, He, C S, Shang, M C, Li, X H, Zhou, Y H, Zhang, F S, Zhang, Z G, Hu, H S, Xu, J P, Chen, W P, Liu
Publikováno v:
Physical review letters. 127(15)
Fluorine is one of the most interesting elements in nuclear astrophysics, where the ^{19}F(p,α)^{16}O reaction is of crucial importance for Galactic ^{19}F abundances and CNO cycle loss in first generation Population III stars. As a day-one campaign
Autor:
Y. J. Ma, Y. Su, T. L. Ma, S. Q. Yan, Gang Lian, F. R. Xu, Z. Y. Han, Z. H. Li, H. Y. Wu, F. L. Liu, D. Wu, X. Y. Li, Weiping Liu, Y. L. Dang, Y. L. Lyu, Bing Guo, D. Nan, G. Y. Fu, C. Zhou, L. Zhang, Y. P. Shen, Y. Zheng, T. J. Zhang, Y. F. He, C. X. Yuan, H. Zhang, J. Su, Z. Q. Chen, B. Tang, B. Dai, R. G. Ma, X. Ma, Sheng Zeng, Y. J. Li, Y. B. Wang, B. Q. Cui, B. A. Brown, L. H. Chen, C. G. Wang, T. Ge
Publikováno v:
Physical Review C. 103
Autor:
Q. Wu, B. Guo, X. Ma, Y. J. Ma, WeiPing Liu, L. T. Sun, B. Tang, L. H. Chen, B. Q. Cui, G. Lian, Q. H. Huang, R. G. Ma
Publikováno v:
Springer Proceedings in Physics ISBN: 9783030138752
Direct measurement of the cross sections for key nuclear reactions is crucial in verifying extrapolation model, constraining theoretical calculations, and solving key scientific questions in nuclear astrophysics. However, these cross-sections are ext
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::406b68e9506f916f57f6e84ef1e6e517
https://doi.org/10.1007/978-3-030-13876-9_53
https://doi.org/10.1007/978-3-030-13876-9_53
Akademický článek
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Autor:
S. X. Wen, C. Y. He, Yunzuo Liu, H. B. Sun, A. Pasternak, Z. M. Wang, Y. Zheng, X. G. Wu, L. H. Zhu, Z. L. Zhang, Y. Liu, X. Z. Cui, R. Meng, Hong-Yu Zhou, Furong Xu, Y. Wang, R. G. Ma, G. S. Li, C. X. Yang
Publikováno v:
The European Physical Journal A. 27:137-141
High-spin states in 171Ta were populated through the heavy-ion fusion-evaporation reaction 157Gd (19F, 5n)171Ta at 105MeV beam energy. Lifetimes of the levels of the πh 9/21/2[541] band have been measured by using the Doppler shift attenuation metho
Autor:
C. X. Yang, Hui-Bin Sun, Guangsheng Li, R. G. Ma, Zheng Wang, Xiang Li, Xiaoguang Wu, He Chuangye, Yunzuo Liu, S. X. Wen, L. H. Zhu, X. Z. Cui
Publikováno v:
Physical Review C. 81
High-spin states of $^{106}\mathrm{Ag}$ were populated via the fusion-evaporation reaction $^{100}\mathrm{Mo}$ ($^{11}\mathrm{B}$,$5n$)$^{106}\mathrm{Ag}$ at a beam energy of $60$ MeV. A rich level scheme with six band structures has been established