The origin of the spectral intensities of cosmic-ray positrons
作者： R. Cowsik , T. Madziwa-Nussinov , B. Burch
DOI: 10.1088/0004-637X/786/2/124
关键词:
摘要: AMS instrument aboard the International Space Station is a high precision capable of collecting large statistics on cosmic ray intensities and as such has started making highly significant contributions to Astroparticle Physics. In order fully benefit from these observations, positron fraction in rays their recent publication other results that will follow, models interpret have be equally good. We enlarge this remark by citing examples currently popular model one our own fitting observed spectra positrons, extending it higher energies. also show what might expect observe mono-energetic source, annihilation dark matter.
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