A comparison between repeating bursts of FRB 121102 and giant pulses from Crab pulsar and its applications
Fen Lyu1,2(), Yan-Zhi Meng1,3, Zhen-Fan Tang1, Ye Li1,4, Jun-Jie Wei1, Jin-Jun Geng3,5(), Lin Lin6, Can-Min Deng7(), Xue-Feng Wu1,8()
1. Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023, China 2. University of Chinese Academy of Sciences, Beijing 100049, China 3. School of Astronomy and Space Science, Nanjing University, Nanjing 210023, China 4. Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, China 5. Institute of Astronomy and Astrophysics, University of Tübingen, Auf der Morgenstelle 10, D-72076, Tübingen, Germany 6. Department of Astronomy, Beijing Normal University, Beijing 100875, China 7. Department of Astronomy, University of Science and Technology of China, Hefei 230026, China 8. School of Astronomy and Space Sciences, University of Science and Technology of China, Hefei 230026, China
There are some similarities between bursts of repeating fast radio bursts (FRBs) and giant pulses (GPs) of pulsars. To explore possible relations between them, we study the cumulative energy distributions of these two phenomena using the observations of repeating FRB 121102 and the GPs of Crab pulsar. We find that the power-law slope of GPs (with fluence≥130 Jy·ms) is 2.85±0.10. The energy distribution of FRB 121102 can be well fitted by a smooth broken power-law function. For the bursts of FRB 121102 above the break energy (1.22 ×1037 erg), the best-fitting slope is , similar to the index of GPs at the same observing frequency (∼1.4 GHz). We further discuss the physical origin of the repeating FRB 121102 in the framework of the super GPs model. And we find that the super GPs model involving a millisecond pulsar is workable and favored for explaining FRB 121102 despite that the magnetar burst model is more popular.
. [J]. Frontiers of Physics, 2021, 16(2): 24503.
Fen Lyu, Yan-Zhi Meng, Zhen-Fan Tang, Ye Li, Jun-Jie Wei, Jin-Jun Geng, Lin Lin, Can-Min Deng, Xue-Feng Wu. A comparison between repeating bursts of FRB 121102 and giant pulses from Crab pulsar and its applications. Front. Phys. , 2021, 16(2): 24503.
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