UHECR propagation in the Galaxy: clustering versus isotropy

Details UHECR propagation in the Galaxy: clustering versus isotropy UHECR propagation in the Galaxy: clustering versus isotropy

2001-12-10

arxiv.org/abs/astro-ph/0112227v1

Astrophys.J.572:185-201,2001

Astronomy and Astrophysics

Astrophysics

33 pages, 21 figures (5 in color), 2 tables

Scientific paper

10.1086/340232

Recently the AGASA Collaboration presented data suggesting a significant clustering of ultra-high energy cosmic rays coming from the outer Galaxy region. In this paper we calculate expected cosmic ray arrival distributions for several simple, limiting source location scenarios and investigate the possibility of clustering and correlation effects. The role of the Galactic magnetic field is discussed in detail.

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