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arXiv · 1808.04330

High-energy neutrino flare from cloud-jet interaction in the blazar PKS 0502+049

Hao-Ning He·Yoshiyuki Inoue·Susumu Inoue·Yun-Feng Liang
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Abstract

Following the detection of a $\sim$300 TeV neutrino potentially associated with the flaring blazar TXS 0506+056, an excess of neutrinos around its position in 2014-2015 was revealed by IceCube. However, its contemporaneous quiescence in $\gamma$-rays is challenging to interpret consistently. Meanwhile, the blazar PKS 0502+049, positioned within the neutrino localization uncertainties, was seen to be flaring in $\gamma$-rays. We show that dense, line-emitting gas clouds that interact with its jet and induce cosmic ray acceleration and hadronuclear interaction can plausibly explain the 2014-2015 neutrino flare.

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Hao-Ning He, Yoshiyuki Inoue, Susumu Inoue, Yun-Feng Liang. 2018-08-13. High-energy neutrino flare from cloud-jet interaction in the blazar PKS 0502+049. https://arxiv.org/abs/1808.04330

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