To understand the radiative processes of pulsars and fast radio bursts with the FAST
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arXiv
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| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
| Published: |
2026
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| _version_ | 1866911584888029184 |
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| author | Wang, Wei-Yang Cao, Shunshun Huang, Zhipeng Lu, Jiguang Men, Yunpeng Meng, Lingqi Niu, Jiarui Pan, Zhichen Wang, Pengfei Zhou, Dejiang Feng, Yi Han, Jinlin Jiang, Jinchen Liu, Bin Luo, Rui Wang, Honguang Wang, Shuangqiang Wang, Tao Wang, Zhengli Xu, Heng Xu, Jiangwei Xu, Renxin Xu, Yonghua Yan, Yi Yan, Zhen Zhou, Yukai Chen, Siyuan Dai, Yinfeng Ge, Mingyu Jiang, Zejun Lee, Kejia Lian, Yujie Liu, Kuo Qian, Lei Tong, Hao Wang, Lin Wang, Yujie Xu, Zihao Yao, Jumei Yin, Dejiang Zhang, Li Zhu, Weiwei |
| author_facet | Wang, Wei-Yang Cao, Shunshun Huang, Zhipeng Lu, Jiguang Men, Yunpeng Meng, Lingqi Niu, Jiarui Pan, Zhichen Wang, Pengfei Zhou, Dejiang Feng, Yi Han, Jinlin Jiang, Jinchen Liu, Bin Luo, Rui Wang, Honguang Wang, Shuangqiang Wang, Tao Wang, Zhengli Xu, Heng Xu, Jiangwei Xu, Renxin Xu, Yonghua Yan, Yi Yan, Zhen Zhou, Yukai Chen, Siyuan Dai, Yinfeng Ge, Mingyu Jiang, Zejun Lee, Kejia Lian, Yujie Liu, Kuo Qian, Lei Tong, Hao Wang, Lin Wang, Yujie Xu, Zihao Yao, Jumei Yin, Dejiang Zhang, Li Zhu, Weiwei |
| contents | The radiative mechanism of coherent radio emission has remained an enigma since the discovery of pulsars, even the emergence of fast radio bursts (FRBs), which exhibit similarities to the single-pulse behavior of pulsars and have opened a new view for deciphering the long-standing mystery. Besides tremendous efforts in modelling, advanced facilities matter for solving the problem. The authors review the observational breakthroughs from the Five-hundred-meter Aperture Spherical radio Telescope (FAST), which are providing pivotal insights to unravel the underlying physics of pulsars and FRBs. This study offers a novel perspective in the era when pulsars meet FRBs, and further investigations are encouraged to utilize the highly sensitive telescope, the FAST. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2604_09987 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | To understand the radiative processes of pulsars and fast radio bursts with the FAST Wang, Wei-Yang Cao, Shunshun Huang, Zhipeng Lu, Jiguang Men, Yunpeng Meng, Lingqi Niu, Jiarui Pan, Zhichen Wang, Pengfei Zhou, Dejiang Feng, Yi Han, Jinlin Jiang, Jinchen Liu, Bin Luo, Rui Wang, Honguang Wang, Shuangqiang Wang, Tao Wang, Zhengli Xu, Heng Xu, Jiangwei Xu, Renxin Xu, Yonghua Yan, Yi Yan, Zhen Zhou, Yukai Chen, Siyuan Dai, Yinfeng Ge, Mingyu Jiang, Zejun Lee, Kejia Lian, Yujie Liu, Kuo Qian, Lei Tong, Hao Wang, Lin Wang, Yujie Xu, Zihao Yao, Jumei Yin, Dejiang Zhang, Li Zhu, Weiwei High Energy Astrophysical Phenomena The radiative mechanism of coherent radio emission has remained an enigma since the discovery of pulsars, even the emergence of fast radio bursts (FRBs), which exhibit similarities to the single-pulse behavior of pulsars and have opened a new view for deciphering the long-standing mystery. Besides tremendous efforts in modelling, advanced facilities matter for solving the problem. The authors review the observational breakthroughs from the Five-hundred-meter Aperture Spherical radio Telescope (FAST), which are providing pivotal insights to unravel the underlying physics of pulsars and FRBs. This study offers a novel perspective in the era when pulsars meet FRBs, and further investigations are encouraged to utilize the highly sensitive telescope, the FAST. |
| title | To understand the radiative processes of pulsars and fast radio bursts with the FAST |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2604.09987 |