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Possible properties of Te V spectra in PKS 2155–304

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摘要 We present a one-zone homogeneous lepton-hadronic model and obtain steady-state spectra by solving the time-dependent equations to study a plausible origin of hard TeV spectra in PKS 2155-304.In this model,we assume a steady electron and proton injection rate in the source and solve the non-linear time-dependent kinematic equations that self-consistently consist of proton-photon interaction,synchrotron radiation of electron/positron pairs and proton,inverse Compton scattering,and synchrotron self-absorption.We employ this model to reproduce the multi-wavelength spectrum of PKS 2155-304,then find that the possible bump located at E~1 TeV which may originate from the synchrotron radiation of secondary electrons produced by Bethe-Heitler pair production,resulting in the hard TeV spectrum.
出处 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2021年第3期227-234,共8页 天文和天体物理学研究(英文版)
基金 partially supported by the National Natural Science Foundation of China(Grant Nos.12063006,11803027and 11863007) Yunnan Local Colleges Applied Basic Research Projects(Grant Nos.202001BA070001-031,2017FH001-102,2018FH001-015,2019FH001-012 and2019FH001-076) Science Research Foundation of Yunnan Education Department of China(Grant Nos.2017ZZX177,2018JS422 and 2019J0733) the financial support from the Hundred Talents Program of Yuxi(Grant Nos.2019)。
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