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- W2079100844 abstract "The phase of inflationary expansion in the early Universe produces superheavy relics in a mass window between 10 12 and 10 14 GeV. Decay or annihilation of these superheavy relics an explain the observed ultrahigh-energy cosmic rays beyond the Greisen–Zatsepin–Kuzmin cutoff. We emphasize that the pattern of cosmic-ray arrival directions seen by the Pierre Auger observatory will decide between the different proposals for the origin of ultrahigh-energy cosmic rays.PACS Nos.: 98.70.Sa, 98.70.–f, 95.35.+d, 14.80.–j" @default.
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- W2079100844 date "2006-01-15" @default.
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- W2079100844 title "Superheavy dark matter and ultrahigh-energy cosmic rays" @default.
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- W2079100844 doi "https://doi.org/10.1139/p06-035" @default.
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