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- W3099157084 abstract "We calculate the solar-modulated energy spectra of cosmic-ray antiprotons (p's) from two candidate primary sources, i.e., evaporating primordial black holes and the annihilation of neutralino dark matter, as well as for the secondary p's produced by cosmic-ray interactions with interstellar gas. A large enhancement toward the solar minimum phase emerges in the low-energy flux of p's from the primary sources, whereas the flux of the secondary p's, falling steeply below 2 GeV, does not significantly vary. This enables us to conduct a very sensitive search for primary p components by precisely measuring the p spectrum, especially at low energies, throughout the forthcoming solar minimum phase." @default.
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- W3099157084 date "1996-12-01" @default.
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- W3099157084 title "Expected enhancement of the primary antiproton flux at the solar minimum" @default.
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- W3099157084 doi "https://doi.org/10.1016/s0370-2693(96)01363-9" @default.
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