A Photo-Hadronic Model of the Large Scale Jet of PKS 0637-752
Masaaki Kusunose, Fumio Takahara

TL;DR
This paper proposes a photo-hadronic model where high-energy protons produce secondary electrons/positrons via Bethe-Heitler and photo-pion processes, explaining the X-ray emission from PKS 0637-752 without conflicting with Fermi LAT limits.
Contribution
It introduces a novel photo-hadronic mechanism for jet X-ray emission, emphasizing secondary leptons from proton interactions as the primary source.
Findings
Reproduces PKS 0637-752's X-ray spectrum with proton power >10^{49} erg/s
Secondary leptons from Bethe-Heitler process dominate X-ray emission
Optical flux is explained by secondary leptons or jet beaming
Abstract
Strong X-ray emission from large scale jets of radio loud quasars still remains an open problem. Models based on inverse Compton scattering off CMB photons by relativistically beamed jets have recently been ruled out, since Fermi LAT observations for 3C 273 and PKS 0637-752 give the upper limit far below the model prediction. Synchrotron emission from a separate electron population with multi-hundred TeV energies remains a possibility although its origin is not well known. We examine a photo-hadronic origin of such high energy electrons/positrons, assuming that protons are accelerated up to eV and produce electrons/positrons through Bethe-Heitler process and photo-pion production. These secondary electrons/positrons are injected at sufficiently high energies and produce X-rays and -rays by synchrotron radiation without conflicting with the Fermi LAT upper limits. We…
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