extending the zoo of candidate sites for UHECR acceleration
Abstract
Fanaroff-Riley (FR) 0 radio galaxies form a low-luminosity extension to the well-established ultra-high-energy cosmic-ray (UHECR) candidate accelerators FR-1 and FR-2 galaxies. Their much higher number density — up to a factor five times more numerous than FR-1 with z ≤ 0.05 — makes them good candidate sources for an isotropic contribution to the observed UHECR flux.
Here, the acceleration and survival of UHECR in prevailing conditions of the FR-0 environment are discussed.
First, an average spectral energy distribution (SED) is compiled based on the FR0CAT. These photon fields, composed of a jet and a host galaxy component, form a minimal target photon field for the UHECR, which will suffer from electromagnetic pair production, photo-disintegration, photo-meson production losses, and synchrotron radiation. The two most promising acceleration scenarios based on Fermi-I order and gradual shear acceleration are discussed as well as different
escape scenarios.
When an efficient acceleration mechanism precedes gradual shear acceleration, e.g., Fermi-I orothers, FR-0 galaxies are likely UHECR accelerators. Gradual shear acceleration requires a jet
Lorentz factor of Gamma>1.6, to be faster than the corresponding escape. In less optimistic models, a contribution to the cosmic-ray flux between the knee and ankle is expected to be relatively independent of the realized turbulence and acceleration.
Keywords
jetted active galaxies;FR-0 radiogalaxies;ultra-high energy cosmic rays;cosmic ray acceleration;cosmic ray energy losses;
Data
Language: |
English |
Year of publishing: |
2022 |
Typology: |
1.08 - Published Scientific Conference Contribution |
Organization: |
UNG - University of Nova Gorica |
UDC: |
539.1 |
COBISS: |
73062147
|
ISSN: |
1824-8039 |
Views: |
1389 |
Downloads: |
0 |
Average score: |
0 (0 votes) |
Metadata: |
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Other data
URN: |
URN:SI:UNG |
Pages: |
str. 1-8 |
Chronology: |
2022 |
ID: |
13283802 |