Galactic anisotropy as signature of CDM-related Ultra-High Energy Cosmic Rays

Preprint

20 February 1998

preprint
Published by arXiv in arXiv

Abstract

We show that production mechanisms of Ultra-High Energy Cosmic Rays involving quasistable particle-like objects which constitute part of cold dark matter can be tested experimentally by observing Galactic anisotropy in their angular distribution.

Keywords

GALACTIC ANISOTROPY
ENERGY COSMIC
CDM RELATED
DARK MATTER
COSMIC RAYS
ULTRA HIGH

All Related Versions

Version 1, 1998-02-20, ArXiv
Version 2, 1998-09-23, ArXiv
Published version: JETP Letters, 68 (2), 107.

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