Possible correlation between unabsorbed hard x rays and neutrinos in radio-loud and radio-quiet active galactic nuclei
Artikel i vetenskaplig tidskrift, 2024

The first high-energy neutrino source identified by IceCube was a blazar - an active galactic nucleus driving a relativistic jet toward 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 TXS0506+056 and GB6J1542+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.

Författare

Emma Kun

Ruhr-Universität Bochum

Magyar Tudomanyos Akademia

Research Centre For Astronomy and Earth Sciences

Imre Bartos

College of Liberal Arts and Sciences

Julia Tjus

Magyar Tudomanyos Akademia

Ruhr-Universität Bochum

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

Peter L. Biermann

University of Alabama

Max-Planck-Gesellschaft

A. Franckowiak

Ruhr-Universität Bochum

F. Halzen

Wisconsin IceCube Particle Astrophysics Center

Santiago Del Palacio

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

Jooyun Woo

Columbia University

Physical Review D - Particles, Fields, Gravitation and Cosmology

24700010 (ISSN) 24700029 (eISSN)

Vol. 110 12 123014

Exploring the Hidden Dusty Nuclei of Galaxies (HIDDeN)

Europeiska forskningsrådet (ERC) (789410), 2018-10-01 -- 2023-09-30.

Ämneskategorier (SSIF 2011)

Subatomär fysik

Astronomi, astrofysik och kosmologi

DOI

10.1103/PhysRevD.110.123014

Mer information

Senast uppdaterat

2024-12-16