Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Xiang-han Cui"'
Autor:
Xiang-han Cui, Zheng-wu Wang, Cheng-min Zhang, Chen-hui Niu, Di Li, Jian-wei Zhang, De-hua Wang
Publikováno v:
The Astrophysical Journal, Vol 956, Iss 1, p 35 (2023)
The radiation mechanism of fast radio bursts (FRBs) has been extensively studied, but still remains elusive. Coherent radiation has been identified as a crucial component in the FRB mechanism, with charged bunches also playing a significant role unde
Externí odkaz:
https://doaj.org/article/0d5e7c9f33b242d8a22be657edda40ad
Autor:
Cheng-Min Zhang, Xiang-Han Cui, Di Li, De-Hua Wang, Shuang-Qiang Wang, Na Wang, Jian-Wei Zhang, Bo Peng, Wei-Wei Zhu, Yi-Yan Yang, Yuan-Yue Pan
Publikováno v:
Universe, Vol 8, Iss 12, p 628 (2022)
The evolutions of a neutron star’s rotation and magnetic field (B-field) have remained unsolved puzzles for over half a century. We ascribe the rotational braking torques of pulsar to both components, the standard magnetic dipole radiation (MDR) an
Externí odkaz:
https://doaj.org/article/2b082deb9ee14de19bbf7f902bf2af25
Autor:
Xiang-Han Cui, Cheng-Min Zhang, Di Li, Jian-Wei Zhang, Bo Peng, Wei-Wei Zhu, Richard Strom, Shuang-Qiang Wang, Na Wang, Qing-Dong Wu, De-Hua Wang, Yi-Yan Yang
Publikováno v:
Astrophysics and Space Science. 367
Fast radio bursts (FRBs) are extremely strong radio flares lasting several micro- to milliseconds and come from unidentified objects at cosmological distances, most of which are only seen once. Based on recently published data in the CHIME/FRB Catalo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::320af45ef998ab9a8c711189be0325d1
https://doi.org/10.1007/s10509-022-04093-y
https://doi.org/10.1007/s10509-022-04093-y
Autor:
Yi-Yan Yang, Wuming Yang, Cheng-Min Zhang, Shaolan Bi, De-Hua Wang, Xianfei Zhang, Xiang-Han Cui, Jianwei Zhang, Di Li
Publikováno v:
Physical Review D. 104
The recently discovered very massive stellar black holes (BHs), i.e., the binary BH (BBH) merger for the gravitational-wave (GW) event GW190521 by LIGO-Virgo O3a with the component masses of ${85}_{\ensuremath{-}14}^{+21}\text{ }\text{ }{M}_{\ensurem
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::40a798e52c0affc78eb9b737860578a0
https://doi.org/10.1103/physrevd.104.103010
https://doi.org/10.1103/physrevd.104.103010
Autor:
Zhen-Qi Diao, Shuangqiang Wang, Yi-Yan Yang, Bo Peng, Weiwei Zhu, Qing-Dong Wu, Cheng-Min Zhang, Richard G. Strom, Jian-Wei Zhang, Chang-Qing Ye, Na Wang, Di Li, Xiang-Han Cui, De-Hua Wang
Fast radio bursts (FRBs) are extremely strong radio flares lasting several milliseconds, most of which come from unidentified objects at a cosmological distance. They can be apparently repeating or not. In this paper, we analyzed 18 repeaters and 12
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f9633cdaa6d82f2dd8bfd7b7dd7ac802
http://arxiv.org/abs/2104.11617
http://arxiv.org/abs/2104.11617
Autor:
Xiang-Han Cui, De-Hua Wang, Jianwei Zhang, Shuangqiang Wang, Qing-Dong Wu, Yi-Yan Yang, Hsiang-Kuang Chang, Bo Peng, Zhen-Qi Diao, Chang-Qing Ye, Di Li, Na Wang, Weiwei Zhu, Cheng-Min Zhang
The properties of the young pulsars and their relations to the supernova remnants (SNRs) have been the interesting topics. At present, 383 SNRs in the Milky Way galaxy have been published, which are associated with 64 radio pulsars and 46 pulsars wit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d635329f068a39749acfded2a1f41bb6
Autor:
Yi-Yan Yang, Shuangqiang Wang, Chang-Qing Ye, Richard G. Strom, Jian-Wei Zhang, Xiang-Han Cui, Na Wang, Di Li, Weiwei Zhu, Cheng-Min Zhang, De-Hua Wang, Bo Peng
Fast Radio Bursts (FRBs) are the short, strong radio pulses lasting several milliseconds. They are subsequently identified, for the most part, as emanating from unknown objects at cosmological distances. At present, over one hundred FRBs have been ve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::910339535ea1df627729b620eb2373a7
Autor:
Wuming Yang, Shaolan Bi, Cheng-Min Zhang, Yi-Yan Yang, De-Hua Wang, Xianfei Zhang, Xiang-Han Cui, Di Li, Jianwei Zhang
Publikováno v:
Chinese Physics B. 30:120401
LIGO-Virgo has observed the gravitational waves (GWs) from the coalescence of binary black hole (BBH) and binary neutron star (BNS) during O1 and O2, and the ones from NS-BH are expected to be hunted in the operating O3 run. The population properties
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8d43dc2d7179cdc70aefd012cf1610fe
https://doi.org/10.1088/1674-1056/abff28
https://doi.org/10.1088/1674-1056/abff28