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Table 1
Probability that a source configuration leads to a 3σ fluctuation above and below the flux measured by AMS02 and PAMELA.
| Models | PAMELA | AMS02 | ||
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| Model | 50 GeV | 1 TeV | 50 GeV | 1 TeV |
| p(Ψ > ⟨ Ψ ⟩ + 3σ) | p(Ψ > ⟨ Ψ ⟩ + 3σ) | p(Ψ > ⟨ Ψ ⟩ + 3σ) | p(Ψ > ⟨ Ψ ⟩ + 3σ) | |
| p(Ψ < ⟨ Ψ ⟩ −3σ) | p(Ψ < ⟨ Ψ ⟩ −3σ) | p(Ψ < ⟨ Ψ ⟩ −3σ) | p(Ψ < ⟨ Ψ ⟩ −3σ) | |
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| MIN | 0.15 | 0.083 | 0.28 | 0.26 |
| 0.13 | <10-6 | 0.63 | 0.51 | |
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| MED | 0.047 | 0.014 | 0.16 | 0.12 |
| <10-6 | <10-6 | 0.26 | 0.0025 | |
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| MAX | 0.009 | 0.0018 | 0.045 | 0.016 |
| <10-6 | <10-6 | <10-6 | <10-6 | |
Notes. The calculation is made for the three benchmark propagation models MIN, MED, and MAX, and for the two energies 50 GeV and 1 TeV.
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