Clustering in Highest Energy Cosmic Rays: Physics or Statistics?
Astrophysics
2008-11-26 v1 High Energy Physics - Phenomenology
Abstract
Directional clustering can be expected in cosmic ray observations due to purely statistical fluctuations for sources distributed randomly in the sky. We develop an analytic approach to estimate the probability of random cluster configurations, and use these results to study the strong potential of the HiRes, Auger, Telescope Array and EUSO/OWL/AirWatch facilities for deciding whether any observed clustering is most likely due to non-random sources.
Cite
@article{arxiv.astro-ph/0009378,
title = {Clustering in Highest Energy Cosmic Rays: Physics or Statistics?},
author = {Haim Goldberg and Thomas J. Weiler},
journal= {arXiv preprint arXiv:astro-ph/0009378},
year = {2008}
}
Comments
19 pages, LaTeX, 3 figures