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Possible properties of Te V spectra in PKS 2155–304
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作者 Quan-Gui Gao Fang-Wu Lu +5 位作者 Long-Hua Qin Huai-Zhen Li Ju Ma Ji-Yang Ren hai-ru zhao Ting-Feng Yi 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2021年第3期227-234,共8页
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... 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. 展开更多
关键词 radiation mechanisms:non-thermal BL Lacertae objects:individual(PKS 2155–304) gamma rays:galaxies
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