The Large-scale Anisotropy and Flux (de)magnification of Ultrahigh-energy Cosmic Rays in the Galactic Magnetic Field

We calculate the arrival direction distribution of ultrahigh-energy cosmic rays (UHECRs) with a new suite of models of the Galactic magnetic field (GMF), assuming sources follow the large-scale structure of the Universe. Compared to previous GMF models, the amplitude of the dipole component of the U...

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Detalhes bibliográficos

Principais autores:	Teresa Bister, Glennys R. Farrar, Michael Unger
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2024-01-01
coleção:	The Astrophysical Journal Letters
Assuntos:	Cosmic ray astronomy Cosmic rays Cosmic ray sources Extragalactic magnetic fields Milky Way magnetic fields Ultra-high-energy cosmic radiation
Acesso em linha:	https://doi.org/10.3847/2041-8213/ad856f
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