ausblenden:
Schlagwörter:
Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE,Nuclear Experiment, nucl-ex
MPINP:
Hochenergie-Astrophysik Theorie - Abteilung Hofmann
Zusammenfassung:
Using publicly available Monte Carlo codes as well as compilation of published data on pp interactions for proton kinetic energy below 2 GeV, we parametrize the energy spectra and production rates of γ-rays by simple but quite accurate (≤20%) analytical expressions in a broad range from the kinematic threshold to PeV energies.