Fast radio bursts(FRBs)are extragalactic radio transients with millisecond duration and brightness temperature.An FRB-associated X-ray burst(XRB)was recently found to arise from the Galactic magnetar SGR J1935+2154.Fo...Fast radio bursts(FRBs)are extragalactic radio transients with millisecond duration and brightness temperature.An FRB-associated X-ray burst(XRB)was recently found to arise from the Galactic magnetar SGR J1935+2154.Following the model of Dai,in which an FRB may originate from a magnetar encountering an asteroid,we focus on explaining the spectrum of the XRB associated with FRB 200428 from SGR J1935+2154.Collisions between asteroidal fragments and the magnetar surface produce a fireball,which further expands relativistically.Due to the velocity difference among some shells in the fireball,internal shocks would form far away from the magnetar,and further emit X-ray emission.We propose that the FRB-associated XRB can be produced by synchrotron emission from the internal shocks,and then constrain the physical parameters by the observed XRB spectrum.展开更多
基金supported by the National Key Research and Development Program of China(Grant Nos.2017YFA0402600,2018YFA0404204)the National SKA Program of China(Grant No.2020SKA0120300)+9 种基金the National Natural Science Foundation of China(NSFC,Grant Nos.11833003,U2038105)supported by the National Natural Science Foundation of China(NSFC,Grant No.12003028)support from the National Natural Science Foundation of China(NSFC,Grant No.U1838113)the National Natural Science Foundation of China(NSFC,Grant Nos.11833003 and U2038105)the Program for Innovative Talents,Entrepreneur in JiangsuYunnan University(Grant No.C176220100087)support by Fundamental Research Funds for the Central Universities(14380046)the National Key Research and Development Programs of China(2018YFA0404204)the science research grants from the China Manned Space Project with NO.CMS-CSST-2021-B11the Program for Innovative Talents,Entrepreneur in Jiangsu。
文摘Fast radio bursts(FRBs)are extragalactic radio transients with millisecond duration and brightness temperature.An FRB-associated X-ray burst(XRB)was recently found to arise from the Galactic magnetar SGR J1935+2154.Following the model of Dai,in which an FRB may originate from a magnetar encountering an asteroid,we focus on explaining the spectrum of the XRB associated with FRB 200428 from SGR J1935+2154.Collisions between asteroidal fragments and the magnetar surface produce a fireball,which further expands relativistically.Due to the velocity difference among some shells in the fireball,internal shocks would form far away from the magnetar,and further emit X-ray emission.We propose that the FRB-associated XRB can be produced by synchrotron emission from the internal shocks,and then constrain the physical parameters by the observed XRB spectrum.
