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Testing for uniformity of Ultra-High Energy Cosmic Ray arrival directions

High Energy Astrophysical Phenomena 2016-05-24 v1

Abstract

Arrival directions of ultra-high energy cosmic rays (UHECRs) exhibit mainly an isotropic distribution with some small deviations in particular energy bins. In this paper, the Yakutsk array data are tested for circular uniformity of arrival directions in right ascension using 2 methods appropriate for the energy ranges below and above 101810^{18} eV. No statistically significant deviation from uniformity is found in the arrival directions of cosmic rays (CRs) detected within the observation period 1974--2000.

Keywords

Cite

@article{arxiv.1602.08814,
  title  = {Testing for uniformity of Ultra-High Energy Cosmic Ray arrival directions},
  author = {A. A. Ivanov},
  journal= {arXiv preprint arXiv:1602.08814},
  year   = {2016}
}

Comments

Preprint of an article submitted for consideration in IJMPD \c{opyright} 2016 [copyright World Scientific Publishing Company] http://www.worldscientific.com/worldscinet/ijmpd