Journal Article

PUBDB-2021-02286

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Multi-wavelength and neutrino emission from blazar PKS 1502 + 106

de Sousa Ferreira Rodrigues, X. (Corresponding author)DESY* ; Garrappa, S.DESY* ; Gao, S.DESY* ; Paliya, V. S.DESY* ; Franckowiak, A.Extern*DESY* ; Winter, W.DESY*

2021
Univ. Chicago, Ill. [u.a.]

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Please use a persistent id in citations: doi:10.3847/1538-4357/abe87b  doi:10.3204/PUBDB-2020-04053

Report No.: arXiv:2009.04026

Abstract: In July of 2019, the IceCube experiment detected a high-energy neutrino from the direction of the powerful blazar PKS 1502+106. We perform multi-wavelength and multi-messenger modeling of this source, using a fully self-consistent one-zone model, which includes the contribution of external radiation fields typical of flat-spectrum radio quasars (FSRQs). We identify three different activity states of the blazar: the quiescent state, and two distinct flaring states with hard and soft gamma-ray spectra. We find two hadronic models that can both describe the multi-wavelength emission during all three states: a leptohadronic model with a contribution from photo-hadronic processes to X-rays and high-energy gamma rays, and a proton synchrotron model, where the emission from keV to 10 GeV comes from proton synchrotron radiation. Both models predict a substantial neutrino flux, which is correlated with the gamma-ray and soft X-ray fluxes. Our results are compatible with the detection of a neutrino during the quiescent state, based on event rate statistics. Upon an extensive parameter scan, we conclude that the soft X-ray fluxes observed during bright gamma-ray flares strongly suggest a hadronic contribution, which can be interpreted as additional evidence for cosmic ray acceleration in the source independently of neutrino observations. We find that more arguments can be made in favor of the leptohadronic model vis-a-vis the proton synchrotron scenario, such as a lower energetic demand during the quiescent state and the fact that the same model has also been shown to describe the observation of neutrinos from blazar TXS 0506+056. The leptohadronic model would be disfavored for flaring states of PKS 1502+106 if no IceCube events were found from the direction of the source before 2010, which would require an archival search.

Keyword(s): model: hadronic ; neutrino: flux ; cosmic radiation: acceleration ; gamma ray: energy spectrum ; blazar ; photon hadron ; proton synchrotron ; radio wave ; X-ray: flux ; IceCube ; messenger ; synchrotron radiation ; statistics ; quasar

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Contributing Institute(s):

1. Astroteilchenphysik (ZEU-EXP/AT)

Research Program(s):

1. 613 - Matter and Radiation from the Universe (POF4-613) (POF4-613)
2. NEUCOS - Neutrinos and the origin of the cosmic rays (646623) (646623)

Experiment(s):

1. IceCube South Pole Neutrino Observatory

Appears in the scientific report 2021

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Database coverage:
; ; Clarivate Analytics Master Journal List ; Current Contents - Physical, Chemical and Earth Sciences ; Ebsco Academic Search ; Essential Science Indicators ; IF >= 5 ; JCR ; SCOPUS ; Science Citation Index Expanded ; Web of Science Core Collection

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Linked articles:

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Preprint de Sousa Ferreira Rodrigues, X. (Corresponding author)DESY* ; Garrappa, S.DESY* ; Gao, S.DESY* ; Paliya, V. S.DESY* ; Franckowiak, A.DESY* ; Winter, W.DESY*
Multi-wavelength and neutrino emission from blazar PKS 1502+106
[10.3204/PUBDB-2020-04053]     Files  Fulltext by arXiv.org BibTeX | EndNote: XML, Text | RIS

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