Zobrazeno 1 - 10
of 3 088
pro vyhledávání: '"Qi, Bin"'
Autor:
Chen, Jing, Chen, Ji-Yuan, Chen, Jun-Feng, Chen, Xiang, Fu, Chang-Bo, Guo, Jun, Guo, Yi-Han, Khaw, Kim Siang, Li, Jia-Lin, Li, Liang, Li, Shu, Lin, Yu-ming, Liu, Dan-Ning, Liu, Kang, Liu, Kun, Liu, Qi-Bin, Liu, Zhi, Lu, Ze-Jia, Lv, Meng, Song, Si-Yuan, Sun, Tong, Tang, Jian-Nan, Wan, Wei-Shi, Wang, Dong, Wang, Xiao-Long, Wang, Yu-Feng, Wang, Zhen, Wang, Zi-Rui, Wu, Wei-Hao, Yang, Hai-Jun, Yang, Lin, Yang, Yong, Yu, Dian, Yuan, Rui, Zhang, Jun-Hua, Zhang, Yu-Lei, Zhang, Yun-Long, Zhao, Zhi-Yu, Zhou, Bai-Hong, Zhu, Chun-Xiang, Zhu, Xu-Liang, Zhu, Yi-Fan
DarkSHINE is a newly proposed fixed-target experiment initiative to search for the invisible decay of Dark Photon via missing energy/momentum signatures, based on the high repetition rate electron beam to be deployed/delivered by the Shanghai High re
Externí odkaz:
http://arxiv.org/abs/2411.09345
Autor:
Li, Fu-Xing, Qian, Sheng-Bang, Zhu, Li-ying, Liao, Wen-Ping, Zhao, er-gang, Li, Min-Yu, Sun, Qi-Bin, Chang, Lin-Feng, Lin, Wen-Xu
The massive semi-detached binary with a long-term decreasing orbital period may involve a rapid mass-transfer phase in Case A, and thus they are good astrophysical laboratories for investigating the evolution of massive binary stars. In this work, by
Externí odkaz:
http://arxiv.org/abs/2411.03592
Autor:
Shi, Lu, Qi, Bin, Luo, Jiarui, Zhang, Yang, Liang, Zhanzhao, Gao, Zhaowei, Deng, Wenke, Sun, Lin
Functional safety is a critical aspect of automotive engineering, encompassing all phases of a vehicle's lifecycle, including design, development, production, operation, and decommissioning. This domain involves highly knowledge-intensive tasks. This
Externí odkaz:
http://arxiv.org/abs/2410.12475
The IW And-type phenomenon in cataclysmic variables presents a significant challenge to the accretion disk instability model. Using photometric data from the All-Sky Automated Survey for Supernovae, the Zwicky Transient Facility, and the Transiting E
Externí odkaz:
http://arxiv.org/abs/2409.03011
Autor:
Chang, Xiu-Ying, Hou, Pan-Yu, Zhang, Wen-Gang, Meng, Xiang-Qian, Yu, Ye-Fei, Lu, Ya-Nan, Liu, Yan-Qing, Qi, Bin-Xiang, Deng, Dong-Ling, Duan, Lu-Ming
Recent breakthroughs have ushered the quantum network into a new era, where quantum information can be stored, transferred, and processed across multiple nodes on a metropolitan scale. A key challenge in this new era is enhancing the capabilities of
Externí odkaz:
http://arxiv.org/abs/2408.07752
Autor:
Li, Min-Yu, Qian, Sheng-Bang, Zhou, Ai-Ying, Zhu, Li-Ying, Liao, Wen-Ping, Zhao, Er-Gang, Shi, Xiang-Dong, Li, Fu-Xing, Sun, Qi-Bin
Heartbeat stars (HBSs) with tidally excited oscillations (TEOs) are ideal astrophysical laboratories for studying the internal properties of the systems. In this paper, five new HBSs exhibiting TEOs are discovered using TESS photometric data. The orb
Externí odkaz:
http://arxiv.org/abs/2408.01019
Autor:
Li, Min-Yu, Qian, Sheng-Bang, Zhou, Ai-Ying, Zhu, Li-Ying, Liao, Wen-Ping, Zhao, Er-Gang, Shi, Xiang-Dong, Li, Fu-Xing, Sun, Qi-Bin
Heartbeat stars (HBSs) are ideal astrophysical laboratories to study the formation and evolution of binary stars in eccentric orbits and the internal structural changes of their components under strong tidal action. We discover 23 new HBSs based on T
Externí odkaz:
http://arxiv.org/abs/2407.18621
Tilted disk precession exists in different objects. Negative superhumps (NSHs) in cataclysmic variable stars (CVs) are believed to arise from the interaction between the reverse precession of a tilted disk and the streams from the secondary star.Util
Externí odkaz:
http://arxiv.org/abs/2407.04913
Autor:
Li, Qin-Mei, Sun, Qi-Bin
The merger of compact binary stars produces short gamma-ray bursts (sGRBs), involving channels such as neutron star - neutron star (BNS) and neutron star - black hole (NS-BH). The association between sGRB 170817A and gravitational wave GW 170817 prov
Externí odkaz:
http://arxiv.org/abs/2406.17496
Autor:
Li, Ping, Liao, Wen-Ping, Qian, Sheng-Bang, Li, Lin-Jia, Sun, Qi-Bin, Shi, Xiang-Dong, Matekov, Azizbek, Zeng, Qi-Huan, Deng, Zhao-Long, Fang, Xiao-Hui
We reported a cyclic variation of $O-C$ diagram with a semi-amplitude of 0.0033 days and a period of 1.05 years for the pulsating eclipsing binary HZ Dra. The cyclic variation can be explained by the light travel-time effect via the presence of a clo
Externí odkaz:
http://arxiv.org/abs/2405.16365