Gamma-Rays Produced in Cosmic-Ray Interactions and TeV-band ...

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FIG. 11: The confidence regions for the cut-off energy E max and the spectral index s derived under the constraint σ ≥ 0 as for cosmic-ray modified shock acceleration. The slow turnover by a negative curvature in the general 3-parameter fit is here replaced by a hard cut-off with E max < 140 TeV with 3 sigma confidence. 30
Page 1 and 2: Gamma-Rays Produced in Cosmic-Ray I
Page 3 and 4: I. INTRODUCTION It is generally bel
Page 5 and 6: threshold up to a few GeV [8]. In a
Page 7 and 8: the nuclear cascades in the nuclear
Page 9 and 10: For the two-body decay process, it
Page 11 and 12: generated by a cosmic-ray particle
Page 13 and 14: of cosmic-ray electrons must be exp
Page 15 and 16: in the power-law index s statistica
Page 17 and 18: collisions of cosmic rays with arbi
Page 19 and 20: [26] T. K. Gaisser, Cosmic Rays and
Page 21 and 22: FIG. 2: The energy spectra of the
Page 23 and 24: FIG. 4: The energy spectra of γ-ra
Page 25 and 26: FIG. 6: Diffuse γ-ray spectrum at
Page 27 and 28: FIG. 8: The confidence regions for
Page 29: FIG. 10: The confidence regions for

Gamma-Rays Produced in Cosmic-Ray Interactions and TeV-band ...

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