J. P. Lundquist (Avtor), Serguei Vorobiov (Avtor), Lukas Merten (Avtor), Anita Reimer (Avtor), Margot Boughelilba (Avtor), Paolo Da Vela (Avtor), Fabrizio Tavecchio (Avtor), Giacomo Bonnoli (Avtor), Chiara Righi (Avtor)

Povzetek

This study comprehensively investigates the gamma-ray dim population of Fanaroff–Riley Type 0 (FR0) radio galaxies as potentially significant sources of ultra–high energy cosmic rays (UHECRs, E > 10[sup]18 eV) detected on Earth. While individual FR0 luminosities are relatively low compared to the more powerful Fanaroff–Riley Type 1 and Type 2 galaxies, FR0s are substantially more prevalent in the local universe, outnumbering the more energetic galaxies by a factor of ∼5 within a redshift of z ≤ 0.05. Employing CRPropa3 simulations, we estimate the mass composition and energy spectra of UHECRs originating from FR0 galaxies for energies above 10[sup]18.6 eV. This estimation fits data from the Pierre Auger Observatory (Auger) using three extensive air shower models; both constant and energy-dependent observed elemental fractions are considered. The simulation integrates an approximately isotropic distribution of FR0 galaxies, extrapolated from observed characteristics, with UHECR propagation in the intergalactic medium, incorporating various plausible configurations of extragalactic magnetic fields, both random and structured. We then compare the resulting emission spectral indices, rigidity cutoffs, and elemental fractions with recent Auger results. In total, 25 combined energy-spectrum and mass-composition fits are considered. Beyond the cosmic-ray fluxes emitted by FR0 galaxies, this study predicts the secondary photon and neutrino fluxes from UHECR interactions with intergalactic cosmic photon backgrounds. The multimessenger approach, encompassing observational data and theoretical models, helps elucidate the contribution of low-luminosity FR0 radio galaxies to the total cosmic-ray energy density.

Ključne besede

ultra-high-energy cosmic rays;UHECRs;UHECR energy spectrum;Pierre Auger Observatory;UHECR mass composition;UHECR sources;extragalactic magnetic fields;UHECR propagation;CRPropa tool;

Podatki

Jezik: Angleški jezik
Leto izida:
Tipologija: 1.01 - Izvirni znanstveni članek
Organizacija: UNG - Univerza v Novi Gorici
UDK: 52
COBISS: 221024771 Povezava se bo odprla v novem oknu
ISSN: 1538-4357
Št. ogledov: 82
Št. prenosov: 1
Ocena: 0 (0 glasov)
Metapodatki: JSON JSON-RDF JSON-LD TURTLE N-TRIPLES XML RDFA MICRODATA DC-XML DC-RDF RDF

Ostali podatki

Strani: str. 1-20
Letnik: ǂVol. ǂ978
Zvezek: ǂno. ǂ1, [article no.] 20
Čas izdaje: 2025
DOI: 10.3847/1538-4357/ad8cd7
ID: 25632767
Priporočena dela:
, ǂa ǂmulti-messenger study of energy spectra/composition emission and intergalactic magnetic field propagation
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