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

More documents

Recommendations

Info

FIG. 7: The TeV-band γ-ray spectrum observed from RX J1713-3946 with HESS, shown in comparison with the best-fit model of hadronic gamma-ray production. Note that both data and model are normalized at 0.97 TeV. Data in the energy range between 1 GeV and 200 GeV would be very valuable and may be provided by GLAST in the near future. 26
FIG. 8: The confidence regions for the spectral curvature σ and the spectral index s. The dark shaded area corresponds to 68% probability, or 1 sigma, the medium gray area indicates 95% confidence, or 2 sigma, and light gray is for 99.7% probability or 3 sigma. 27
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: FIG. 6: Diffuse γ-ray spectrum at
Page 29 and 30: FIG. 10: The confidence regions for

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

You also want an ePaper? Increase the reach of your titles

Delete template?

Save as template?