Pulsar and supernova-remnant models yield TeV electron features with effective sharpness beta_eff of roughly 2 to 3.6, so a sharper, stable edge would favor exotic origins.
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Astrophysical origins of TeV features in the cosmic-ray lepton spectrum
Pulsar and supernova-remnant models yield TeV electron features with effective sharpness beta_eff of roughly 2 to 3.6, so a sharper, stable edge would favor exotic origins.