The Multiple Images of the Plasma Lensing FRB  

作　　者：Yu-Bin Wang Zhi-Gang Wen Rai Yuen Na Wang Jian-Ping Yuan Xia Zhou 

机构地区：[1]Xinjiang Astronomical Observatory,Chinese Academy of Sciences,Urumqi 830011,China [2]University of Chinese Academy of Sciences,Beijing 100049,China [3]Key Laboratory of Radio Astronomy,Chinese Academy of Sciences,Nanjing 210008,China [4]Xinjiang Key Laboratory of Radio Astrophysics,Urumqi 830011,China

出　　处：《Research in Astronomy and Astrophysics》2022年第6期190-203,共14页天文和天体物理学研究（英文版）

基　　金：supported by the National Natural Science Foundation of China(grant Nos.12041304,11873080 and 12033001);supported by the 2021 project Xinjiang Uygur Autonomous Region of China for Tianshan elites,and the National SKA Program of China(grant Nos.U1838109,2020SKA0120100 and 12041301);supported by the Key Laboratory of Xinjiang Uygur Autonomous Region No.2020D04049;the National SKA Program of China No.2020SKA0120200;the 2018 Project of Xinjiang Uygur Autonomous Region of China for Flexibly Fetching in Upscale Talents;supported by CAS“Light of West China”Program No.2018-XBQNXZ-B-025;partly supported by the Operation,Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments,budgeted from the Ministry of Finance of China(MOF)and administrated by the CAS。

摘　　要：We investigate the formation of multiple images as the radio signals from fast radio bursts(FRBs)pass through the plane of a plasma clump.The exponential model for the plasma clump is adopted to analyze the properties of the multiple images.By comparing with the classical dispersion relations,we find that one image has exhibited specific inverse properties to others,such as their delay times at high frequency is higher than that at low frequency,owing to the lensing effects of the plasma clump.We demonstrate that these inverse effects should be observable in some repeating FRBs.Our results predict deviation in the estimated dispersion measure(DM)across multiple images,consistent with the observations of FRB 121102 and FRB 180916.J0158+65.If other plasma lenses have effects similar to an exponential lens,we find that they should also give rise to a similar dispersion relation in the multiple images.For some repeating FRBs,analysis of the differences in time delay and in DM between multiple images at different frequencies can serve as a method to reveal the plasma distribution.

关 键 词：GALAXIES distances and redshifts GALAXIES ISM gravitational lensing:strong-ISM structure-scattering 

分 类 号：P161[天文地球—天文学]