Enregistré dans:
Détails bibliographiques
Auteurs principaux: Anchordoqui, Luis A., Castillo, Karem Peñaló
Format: Preprint
Publié: 2025
Sujets:
Accès en ligne:https://arxiv.org/abs/2503.13315
Tags: Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
_version_ 1866917169085808640
author Anchordoqui, Luis A.
Castillo, Karem Peñaló
author_facet Anchordoqui, Luis A.
Castillo, Karem Peñaló
contents Motivated by a recent proposal that points to the Sombrero galaxy as a source of the highest energy cosmic rays, we investigate the feasibility of accelerating light and heavy nuclei in the supermassive black hole located at the center of this dormant galaxy. We show that cosmic ray nuclei concentrated in the immediate vicinity of the supermassive black hole could be efficiently accelerated up to the maximum observed energies without suffering catastrophic spallations. Armed with our findings we stand against the conventional wisdom and conjecture that accelerators of the highest energy cosmic rays must anti-correlate with the (electromagnetic) source power.
format Preprint
id arxiv_https___arxiv_org_abs_2503_13315
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Sombrero Galaxy as an Accelerator of Ultrahigh Energy Cosmic Ray Nuclei
Anchordoqui, Luis A.
Castillo, Karem Peñaló
High Energy Astrophysical Phenomena
Motivated by a recent proposal that points to the Sombrero galaxy as a source of the highest energy cosmic rays, we investigate the feasibility of accelerating light and heavy nuclei in the supermassive black hole located at the center of this dormant galaxy. We show that cosmic ray nuclei concentrated in the immediate vicinity of the supermassive black hole could be efficiently accelerated up to the maximum observed energies without suffering catastrophic spallations. Armed with our findings we stand against the conventional wisdom and conjecture that accelerators of the highest energy cosmic rays must anti-correlate with the (electromagnetic) source power.
title Sombrero Galaxy as an Accelerator of Ultrahigh Energy Cosmic Ray Nuclei
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2503.13315