Zobrazeno 1 - 10
of 2 116
pro vyhledávání: '"Xie Sheng"'
Autor:
WANG Ya-nan, GUO Dong-fa, LIU Rui-ping, LI Bo-ping, LI Li, XIE Sheng-kai, HE Sheng, WU Yong, ZHOU Liang-hui
Publikováno v:
He huaxue yu fangshe huaxue, Vol 45, Iss 4, Pp 323-331 (2023)
In this paper, based on the research background of recovering uranium from wet-process phosphoric acid(WPA) by amino phosphonate acid chelating resin, the distribution of uranium in single particle amino phosphonate chelating resin was studied. The r
Externí odkaz:
https://doaj.org/article/566a64389b1a4de990c2f45610032808
Publikováno v:
Liang you shipin ke-ji, Vol 31, Iss 4, Pp 48-54 (2023)
In this study, zein-based gluten-free model dough (Z dough) was prepared with zein, corn starch, and wormwood gum. Based on the flour quality test, the kneading torque, water composition and protein distribution of the zein simulated dough with diffe
Externí odkaz:
https://doaj.org/article/05b5e205bee84ca7a2d9c9a44fa1c52e
Publikováno v:
Kongzhi Yu Xinxi Jishu, Iss 1, Pp 39-44 (2023)
With the increasing proportion of renewable energy and power electronic equipment in applications, new-type power systems are bringing more external excitation with growing intensity in the development towards electrification and cleanliness. In orde
Externí odkaz:
https://doaj.org/article/2c55a19feb534aa7b871a70318f9167e
The very high-energy afterglow in GRB 221009A, known as the `Brightest Of All Time' (B.O.A.T.), has been thoroughly analyzed in previous studies. In this paper, we conducted a statistical analysis of the waiting time behavior of 172 TeV photons from
Externí odkaz:
http://arxiv.org/abs/2412.16052
Autor:
Wang, Chen-Wei, Tan, Wen-Jun, Xiong, Shao-Lin, Yi, Shu-Xu, Moradi, Rahim, Li, Bing, Zhang, Zhen, Wang, Yu, Meng, Yan-Zhi, Liu, Jia-Cong, Wang, Yue, Xie, Sheng-Lun, Xue, Wang-Chen, Yu, Zheng-Hang, Zhang, Peng, Zhang, Wen-Long, Zhang, Yan-Qiu, Zheng, Chao
Type I gamma-ray bursts (GRBs) are believed to originate from compact binary merger usually with duration less than 2 seconds for the main emission. However, recent observations of GRB 211211A and GRB 230307A indicate that some merger-origin GRBs cou
Externí odkaz:
http://arxiv.org/abs/2407.02376
Publikováno v:
Open Physics, Vol 17, Iss 1, Pp 313-319 (2019)
Free surface electrospinning is a continuous electrospinning method for low-cost, massive production of nanofibers. The interjet distance λ is a critical parameter in free surface electrospinning, which directly determines the nanofiber production e
Externí odkaz:
https://doaj.org/article/6c7f8d8dad534d31b5df3390b48f1e24
Autor:
Xie, Sheng-Lun, Yu, Yun-Wei, Xiong, Shao-Lin, Lin, Lin, Wang, Ping, Zhao, Yi, Wang, Yue, Zhang, Wen-Long
By using the Fermi/Gamma-ray Burst Monitor data of the X-ray bursts (XRBs) of SGR J1935+2154, we investigate the temporal clustering of the bursts and the cumulative distribution of the waiting time and fluence/flux. It is found that the bursts occur
Externí odkaz:
http://arxiv.org/abs/2404.11877
Autor:
Wang, Ping, Song, Li-Ming, Xiong, Shao-Lin, Zhao, Xiao-Yun, Wang, Jin, Zhao, Shu-Min, Xiao, Shuo, Cai, Ce, Xie, Sheng-Lun, Xue, Wang-Chen, Wang, Chen-Wei, Wang, Yue, Zhang, Wen-Long
Publikováno v:
ApJ 975 188 (2024)
Understanding the nature of repeating fast radio bursts (FRBs) is crucial to probe their underlying physics. In this work, we analyze the waiting time statistics between bursts of three repeating FRBs from four datasets. We find a universally pronoun
Externí odkaz:
http://arxiv.org/abs/2312.12978
Autor:
Xie, Sheng-Lun, Cai, Ce, Yu, Yun-Wei, Xiong, Shao-Lin, Lin, Lin, Zhao, Yi, Zhang, Shuang-Nan, Song, Li-Ming, Wang, Ping, Li, Xiao-Bo, Xue, Wang-Chen, Zhang, Peng, Zheng, Chao, Zhang, Yan-Qiu, Liu, Jia-Cong, Wang, Chen-Wei, Tan, Wen-Jun, Wang, Yue, Yu, Zheng-Hang, Feng, Pei-Yi, Zhang, Jin-Peng, Xiao, Shuo, Zhao, Hai-Sheng, Zhang, Wen-Long, Zhang, Yan-Ting, Huang, Yue, Zhao, Xiao-Yun, Ma, Xiang, Zheng, Shi-Jie, Li, Xin-Qiao, Wen, Xiang-Yang, Gong, Ke, An, Zheng-Hua, Zhang, Da-Li, Yang, Sheng, Liu, Xiao-Jing, Zhang, Fan
Magnetar is a neutron star with an ultrahigh magnetic field ($\sim 10^{14}-10^{15}$ G) which usually manifests as soft gamma-ray repeater (SGR) or anomalous X-ray pulsar (AXP). SGR J1935+2154 is not only one of the most active magnetar detected so fa
Externí odkaz:
http://arxiv.org/abs/2307.01010
Autor:
An, Zheng-Hua, Antier, S., Bi, Xing-Zi, Bu, Qing-Cui, Cai, Ce, Cao, Xue-Lei, Camisasca, Anna-Elisa, Chang, Zhi, Chen, Gang, Chen, Li, Chen, Tian-Xiang, Chen, Wen, Chen, Yi-Bao, Chen, Yong, Chen, Yu-Peng, Coughlin, Michael W., Cui, Wei-Wei, Dai, Zi-Gao, Hussenot-Desenonges, T., Du, Yan-Qi, Du, Yuan-Yuan, Du, Yun-Fei, Fan, Cheng-Cheng, Frontera, Filippo, Gao, He, Gao, Min, Ge, Ming-Yu, Gong, Ke, Gu, Yu-Dong, Guan, Ju, Guo, Dong-Ya, Guo, Zhi-Wei, Guidorzi, Cristiano, Han, Da-Wei, He, Jian-Jian, He, Jun-Wang, Hou, Dong-Jie, Huang, Yue, Huo, Jia, Ji, Zhen, Jia, Shu-Mei, Jiang, Wei-Chun, Kann, David Alexander, Klotz, A., Kong, Ling-Da, Lan, Lin, Li, An, Li, Bing, Li, Chao-Yang, Li, Cheng-Kui, Li, Gang, Li, Mao-Shun, Li, Ti-Pei, Li, Wei, Li, Xiao-Bo, Li, Xin-Qiao, Li, Xu-Fang, Li, Yan-Guo, Li, Zheng-Wei, Liang, Jing, Liang, Xiao-Hua, Liao, Jin-Yuan, Lin, Lin, Liu, Cong-Zhan, Liu, He-Xin, Liu, Hong-Wei, Liu, Jia-Cong, Liu, Xiao-Jing, Liu, Ya-Qing, Liu, Yu-Rong, Lu, Fang-Jun, Lu, Hong, Lu, Xue-Feng, Luo, Qi, Luo, Tao, Ma, Bin-Yuan, Ma, Fu-Li, Ma, Rui-Can, Ma, Xiang, Maccary, Romain, Mao, Ji-Rong, Meng, Bin, Nie, Jian-Yin, Orlandini, Mauro, Ou, Ge, Peng, Jing-Qiang, Peng, Wen-Xi, Qiao, Rui, Qu, Jin-Lu, Ren, Xiao-Qin, Shi, Jing-Yan, Shi, Qi, Song, Li-Ming, Song, Xin-Ying, Su, Ju, Sun, Gong-Xing, Sun, Liang, Sun, Xi-Lei, Tan, Wen-Jun, Tan, Ying, Tao, Lian, Tuo, You-Li, Turpin, Damien, Wang, Jin-Zhou, Wang, Chen, Wang, Chen-Wei, Wang, Hong-Jun, Wang, Hui, Wang, Jin, Wang, Ling-Jun, Wang, Peng-Ju, Wang, Ping, Wang, Wen-Shuai, Wang, Xiang-Yu, Wang, Xi-Lu, Wang, Yu-Sa, Wang, Yue, Wen, Xiang-Yang, Wu, Bo-Bing, Wu, Bai-Yang, Wu, Hong, Xiao, Sheng-Hui, Xiao, Shuo, Xiao, Yun-Xiang, Xie, Sheng-Lun, Xiong, Shao-Lin, Xiong, Sen-Lin, Xu, Dong, Xu, He, Xu, Yan-Jun, Xu, Yan-Bing, Xu, Ying-Chen, Xu, Yu-Peng, Xue, Wang-Chen, Yang, Sheng, Yang, Yan-Ji, Yang, Zi-Xu, Ye, Wen-Tao, Yi, Qi-Bin, Yi, Shu-Xu, Yin, Qian-Qing, You, Yuan, Yu, Yun-Wei, Yu, Wei, Yu, Wen-Hui, Zeng, Ming, Zhang, Bing, Zhang, Bin-Bin, Zhang, Da-Li, Zhang, Fan, Zhang, Hong-Mei, Zhang, Juan, Zhang, Liang, Zhang, Peng, Zhang, Shu, Zhang, Shuang-Nan, Zhang, Wan-Chang, Zhang, Xiao-Feng, Zhang, Xiao-Lu, Zhang, Yan-Qiu, Zhang, Yan-Ting, Zhang, Yi-Fei, Zhang, Yuan-Hang, Zhang, Zhen, Zhao, Guo-Ying, Zhao, Hai-Sheng, Zhao, Hong-Yu, Zhao, Qing-Xia, Zhao, Shu-Jie, Zhao, Xiao-Yun, Zhao, Xiao-Fan, Zhao, Yi, Zheng, Chao, Zheng, Shi-Jie, Zhou, Deng-Ke, Zhou, Xing, Zhu, Xiao-Cheng
GRB 221009A is the brightest gamma-ray burst ever detected since the discovery of this kind of energetic explosions. However, an accurate measurement of the prompt emission properties of this burst is very challenging due to its exceptional brightnes
Externí odkaz:
http://arxiv.org/abs/2303.01203