| Texto completo | |
| Autor(es): |
de Oliveira, Caina
;
Lang, Rodrigo Guedes
;
Batista, Pedro
Número total de Autores: 3
|
| Tipo de documento: | Artigo Científico |
| Fonte: | ASTROPHYSICAL JOURNAL; v. 981, n. 2, p. 11-pg., 2025-03-10. |
| Resumo | |
Active galactic nuclei (AGN) are among the main candidates for ultra-high-energy cosmic-ray (UHECR) sources. However, while some theoretical and phenomenological works favor AGNs as the main sources, recent works have shown that using the very-high-energy gamma-ray flux as a proxy for the UHECR flux leads to a bad agreement with data. In this context, the energy spectrum and composition data are hardly fitted. At the same time, the arrival directions map is badly described and a spurious dipole direction is produced. In this work, we propose a possible solution to these contradictions. Using the observed gamma-ray flux as a proxy may carry the implicit assumption of beamed UHECR emission and, consequently, its beam will remain collimated up to its detection on Earth. We show that assuming an isotropic UHECR emission and correcting the gamma-ray emission proxy by Doppler boosting can overcome the problem. The combined fit of the spectrum and composition is improved, with a change of reduced chi(2) from 4.6 to 3.1. In particular, the tension between the observed and modeled dipole directions can be reduced from 5.9 (2.1)sigma away from the data to 3.5 (1.1)sigma for E > 8 EeV (E > 32 EeV). We also show that this effect is particularly important when including AGNs of different classes in the same analysis, such as radio galaxies and blazars. (AU) | |
| Processo FAPESP: | 19/10151-2 - Estudo de raios cósmicos de energias ultra-altas com o AugerPrime |
| Beneficiário: | Carola Dobrigkeit Chinellato |
| Modalidade de apoio: | Auxílio à Pesquisa - Projetos Especiais |
| Processo FAPESP: | 22/01271-7 - Astrofísica de particulas na era do CTA e SWGO |
| Beneficiário: | Luiz Vitor de Souza Filho |
| Modalidade de apoio: | Auxílio Organização - Reunião Científica |
| Processo FAPESP: | 21/01089-1 - Cherenkov Telescope Array: construção e primeiras descobertas |
| Beneficiário: | Luiz Vitor de Souza Filho |
| Modalidade de apoio: | Auxílio à Pesquisa - Projetos Especiais |
| Processo FAPESP: | 20/15453-4 - Mecanismos de produção de astropartículas ultra energéticas |
| Beneficiário: | Cainã de Oliveira |
| Modalidade de apoio: | Bolsas no Brasil - Doutorado |