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Supercluster Magnetic Fields and Anisotropy of Cosmic Rays above 10**(19) eV

1999/03/09 by Martin Lemoine, G. Sigl, Guenter Sigl +5 · 2 citations
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Dark Matter and Cosmic Phenomena #Solar and Space Plasma Dynamics #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/9903124

4 latex pages, 4 postscript figures included, uses revtex.sty in two column format and epsf.sty, submitted to Physical Review Letters. Links and further material at http://astro.uchicago.edu/home/web/sigl/r2e.html

arxiv created 1999/03/09 · arxiv updated 2009/12/01

Abstract

We predict energy spectra and angular distributions of nucleons above 10**(19) eV that originate from sources distributed in the Local Supercluster, which is also supposed to contain a large scale magnetic field of strength between 0.05 and 0.5 micro Gauss. We show that this model can explain all present-day features of ultra-high energy cosmic rays, at least for field strengths close to 0.5 micro Gauss. The large-scale anisotropy and the clustering predicted by this scenario will allow strong discrimination against other models with next generation experiments.

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