Possible correlation between unabsorbed hard X-rays and neutrinos in radio-loud and radio-quiet AGN

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Hauptverfasser: Kun, Emma, Bartos, Imre, Tjus, Julia Becker, Biermann, Peter L., Franckowiak, Anna, Halzen, Francis, del Palacio, Santiago, Woo, Jooyun
Format: Preprint
Veröffentlicht: 2024
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author Kun, Emma
Bartos, Imre
Tjus, Julia Becker
Biermann, Peter L.
Franckowiak, Anna
Halzen, Francis
del Palacio, Santiago
Woo, Jooyun
author_facet Kun, Emma
Bartos, Imre
Tjus, Julia Becker
Biermann, Peter L.
Franckowiak, Anna
Halzen, Francis
del Palacio, Santiago
Woo, Jooyun
contents The first high-energy neutrino source identified by IceCube was a blazar -- an active galactic nucleus driving a relativistic jet towards Earth. Jets driven by accreting black holes are commonly assumed to be needed for high-energy neutrino production. Recently, IceCube discovered neutrinos from Seyfert galaxies, which appears unrelated to jet activity. Here, we show that the observed luminosity ratios of neutrinos and hard X-rays from blazars TXS 0506+056 and GB6 J1542+6129 are consistent with neutrino production in a $γ$-obscured region near a central supermassive black hole, with the X-ray flux corresponding to reprocessed $γ$-ray emission with flux comparable to that of neutrinos. Similar neutrino - hard X-ray flux ratios are found for four Seyfert galaxies, NGC 1068, NGC 4151, CGCG 420-015 and NGC 3079, raising the possibility of a common neutrino production mechanism that may not involve a strong jet.
format Preprint
id arxiv_https___arxiv_org_abs_2404_06867
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Possible correlation between unabsorbed hard X-rays and neutrinos in radio-loud and radio-quiet AGN
Kun, Emma
Bartos, Imre
Tjus, Julia Becker
Biermann, Peter L.
Franckowiak, Anna
Halzen, Francis
del Palacio, Santiago
Woo, Jooyun
High Energy Astrophysical Phenomena
The first high-energy neutrino source identified by IceCube was a blazar -- an active galactic nucleus driving a relativistic jet towards Earth. Jets driven by accreting black holes are commonly assumed to be needed for high-energy neutrino production. Recently, IceCube discovered neutrinos from Seyfert galaxies, which appears unrelated to jet activity. Here, we show that the observed luminosity ratios of neutrinos and hard X-rays from blazars TXS 0506+056 and GB6 J1542+6129 are consistent with neutrino production in a $γ$-obscured region near a central supermassive black hole, with the X-ray flux corresponding to reprocessed $γ$-ray emission with flux comparable to that of neutrinos. Similar neutrino - hard X-ray flux ratios are found for four Seyfert galaxies, NGC 1068, NGC 4151, CGCG 420-015 and NGC 3079, raising the possibility of a common neutrino production mechanism that may not involve a strong jet.
title Possible correlation between unabsorbed hard X-rays and neutrinos in radio-loud and radio-quiet AGN
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2404.06867