Cosmic ray contributions from rapidly rotating stellar mass black holes: cosmic Ray GeV to EeV proton and anti-proton sources

Cosmic ray contributions from rapidly rotating stellar mass black holes: cosmic Ray GeV to EeV proton and anti-proton sources

In Radio Super Novae (RSNe) a magnetic field of (B × r) = 1016.0±0.12 Gauss × cm is observed; these are the same numbers for Blue Super Giant (BSG) star explosions as for Red Super Giant (RSG) star explosions, despite their very different wind properties. The EHT data for M87 as well for low power r...

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Bibliographic Details
Main Authors: M. Allen, P. L. Biermann, A. Chieffi, R. Chini, D. Frekers, L. Gergely, Gopal-Krishna, B. Harms, I. Jaroschewski, P. S. Joshi, P. P. Kronberg, E. Kun, A. Meli, E.-S. Seo, T. Stanev
Format: Article
Language:English
Published: Frontiers Media S.A. 2024-12-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
cosmic Rays
acceleration
supernovae
black holes
magnetic fields
anti-protons
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2024.1386305/full
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