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Numerical models of neutrino and gamma-ray emission from magnetic reconnection in the core of radio-galaxies

Abstract:

Non-blazar radio-galaxies emitting in the very-high-energy (VHE; >100 GeV) regime offer a unique perspective for probing particle acceleration and emission processes in black hole (BH) accretion-jet systems. The misaligned nature of these sources indicates the presence of an emission component that could be of hadronic origin and located in the core region. Here we consider turbulent magnetic reconnection in the BH accretion flow of radio-galaxies as a potential mechanism for cosmic-ray (CR) ...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.22323/1.329.0014

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
ORCID:
0000-0003-2656-064X
Publisher:
Sissa Medialab
Journal:
Proceedings of Science More from this journal
Volume:
329
Article number:
14
Publication date:
2019-05-13
Acceptance date:
2018-09-11
Event title:
International Conference on Black Holes as Cosmic Batteries: UHECRs and Multimessenger Astronomy
Event location:
Foz do Iguaçu, Brasil
Event start date:
2018-09-12
Event end date:
2018-09-15
DOI:
EISSN:
1824-8039
Language:
English
Keywords:
Pubs id:
984349
Local pid:
pubs:984349
Deposit date:
2021-08-04

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