To understand the radiative processes of pulsars and fast radio bursts with the FAST

Fuente: arXiv
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Main Authors: 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
Format: Preprint
Published: 2026
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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