Zobrazeno 1 - 10
of 24
pro vyhledávání: '"C. S. Shang"'
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:
W. P. Liu, Z. H. Li, J. J. He, X. D. Tang, G. Lian, J. Su, Y. P. Shen, Z. An, F. Q. Chao, J. J. Chang, L. H. Chen, H. Chen, X. J. Chen, Y. H. Chen, Z. J. Chen, B. Q. Cui, X. C. Du, X. Fang, C. B. Fu, L. Gan, B. Guo, Z. Y. Han, X. Y. Guo, G. Z. He, J. R. He, A. Heger, S. Q. Hou, H. X. Huang, N. Huang, B. L. Jia, L. Y. Jiang, S. Kubono, J. M. Li, M. C. Li, K. A. Li, E. T. Li, T. Li, Y. J. Li, M. Lugaro, X. B. Luo, H. Y. Ma, S. B. Ma, D. M. Mei, W. Nan, W. K. Nan, N. C. Qi, Y. Z. Qian, J. C. Qin, J. Ren, C. S. Shang, L. T. Sun, W. L. Sun, W. P. Tan, I. Tanihata, S. Wang, P. Wang, Y. B. Wang, Q. Wu, S. W. Xu, S. Q. Yan, L. T. Yang, Y. Yang, X. Q. Yu, Q. Yue, S. Zeng, L. Zhang, H. Zhang, H. Y. Zhang, L. Y. Zhang, N. T. Zhang, P. Zhang, Q. W. Zhang, T. Zhang, X. P. Zhang, X. Z. Zhang, W. Zhao, J. F. Zhou, Y. Zhou
Publikováno v:
Few-Body Systems. 63
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:
C. X. Yu, B. T. Zhang, X. P. Geng, Hao-Yang Xing, Hanxiong Huang, Honghan Gong, J. Li, Qian Yue, Y. D. Liu, Y. Li, Tian Xue, W. Y. Tang, Yang Tian, M. X. Li, K. Kang, B. Sevda, Y. Y. Liu, Cong-Feng Qiao, X. C. Ruan, L. T. Yang, F. K. Lin, L. P. Jia, Zhenyu Zhang, Lei Wang, J. F. Zhou, T. C. Huang, Yan Wang, J. P. Chang, Lakhwinder Singh, Y. C. Mao, H. T. He, Q. Y. Nie, X. Q. Li, M. Agartioglu, Shin-Ted Lin, Z. She, N. C. Qi, M. G. Zhao, G. F. Wang, Q. J. Guo, Y. L. Yan, X. Y. Guo, X. N. Li, Ming Zeng, Feng-Shou Zhang, H. B. Li, Qian Wang, Shengzhou Wu, J. Cheng, Yuanjing Li, Ye Chen, Tianxi Sun, J. W. Hu, N. Yi, Z. Y. Zhou, S. M. He, L. He, Zhi Zeng, H. J. Yu, J.J. Zhu, Y. Wang, C. S. Shang, B. Liao, P. Gu, V. Sharma, Zuowei Liu, Jia-Ming Li, Lei Zhang, Wei Dai, H. P. An, H. Pan, Zhao-Qi Wang, Yin Xu, Zhi Deng, Manoj Kumar Singh, J. H. Ning, Hau-Bin Li, Hao Ma, Jun Ren, Henry T. Wong, S. K. Liu, C. J. Tang, Jing-Han Chen, J. F. Yue
Publikováno v:
Physical Review Letters
We report constraints on the dark photon effective kinetic mixing parameter (${\kappa}$) with data taken from two ${p}$-type point-contact germanium detectors of the CDEX-10 experiment at the China Jinping Underground Laboratory. The 90\% confidence
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4920b4626e8747cce9f0cc07d468052f
https://avesis.deu.edu.tr/publication/details/8007879e-dea9-4b6b-beba-43514ae466af/oai
https://avesis.deu.edu.tr/publication/details/8007879e-dea9-4b6b-beba-43514ae466af/oai
Autor:
X. C. Ruan, Y. C. Mao, Z. She, Ming-Gang Zhao, S. M. He, Qian Yue, Qing Wang, Shiyong Wu, Tao Xue, Hong-Jian He, QiuJu Guo, J. W. Hu, Yin Xu, H. Pan, Tianxi Sun, Z. Y. Zhou, Manoj Kumar Singh, Chang-Jian Tang, Li Wang, B. Liao, ZhongZhi Liu, Q. Y. Nie, Yulan Li, Hanxiong Huang, W. Y. Tang, Zhi Deng, Lei Zhang, Lakhwinder Singh, Hao Yu, Hao Ma, Xia Li, Wei Dai, Hao-Yang Xing, Yucheng Wu, C. S. Shang, Jin Li, Liu Yuanyuan, Jingjun Zhu, Hai-Peng An, Hau-Bin Li, M. Agartioglu, B. T. Zhang, L. He, YuChen Wang, J. H. Ning, Feng-Shou Zhang, T. C. Huang, Yuanjing Li, Xi Jiang, Jing Zhou, R. M. J. Li, X. Y. Guo, Jianmin Li, Ming Zeng, S. K. Liu, Yipeng Wang, Yi Wang, Henry T. Wong, Zhen Wang, Y. L. Yan, H. T. Jia, Zhi Zeng, Yu Liu, C. H. Fang, KangKang Zhao, N. Yi, Vivek Sharma, Yunhua Chen, Y. Y. Liu, Kejun Kang, L. T. Yang, Chunxu Yu, J. P. Chang, Jie Ren, Hui Gong, Jianping Cheng, X. P. Geng, Yang Tian, L. P. Jia, C. Y. Chiang, Jianbo Yue, F. K. Lin, MingXuan Li, Shin-Ted Lin, ZhenYu Zhang, Jing-Han Chen, N. C. Qi, G. F. Wang
We present weakly interacting massive particles (WIMPs) search results performed using two approaches of effective field theory from the China Dark Matter Experiment (CDEX), based on the data from both CDEX-1B and CDEX-10 stages. In the nonrelativist
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e065f22848771e9a269a9879991f3b88
Autor:
Y Wang, Z Zeng, Q Yue, L T Yang, K J Kang, Y J Li, M Agartioglu, H P An, J P Chang, J H Chen, Y H Chen, J P Cheng, C Y Chiang, W H Dai, Z Deng, X P Geng, H Gong, Q J Guo, X Y Guo, L He, S M He, J W Hu, T S Huang, H X Huang, H T Jia, L P Jia, H B Li, J M Li, J Li, M X Li, R M J Li, X Li, Y L Li, B Liao, F K Lin, S T Lin, S K Liu, Y D Liu, Y Y Liu, Z Z Liu, H Ma, Y C Mao, Q Y Nie, J H Ning, H Pan, N C Qi, C K Qiao, J Ren, X C Ruan, C S Shang, V Sharma, Z She, L Singh, M K Singh, T X Sun, C J Tang, W Y Tang, Y Tian, G F Wang, L Wang, Q Wang, Y X Wang, Z Wang, H T Wong, S Y Wu, Y C Wu, H Y Xing, Y Xu, T Xue, Y L Yan, N Yi, C X Yu, H J Yu, J F Yue, M Zeng, B T Zhang, L Zhang, F S Zhang, M G Zhao, J F Zhou, Z Y Zhou, J J Zhu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c82bb664350380c3ccf39cd4e0772a0a
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.