Linking gamma-ray spectra of supernova remnants to the cosmic ray injection properties in the aftermath of supernovae

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Fig. 8

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Particle spectra at 30 and 3000 yr calculated with Eq. (3) and the dependence Q_t(t) shown in Fig. 3. Bottom axis is for protons and the upper one is for electrons, under the condition that both populations have the same maximum momentum (parameters used are listed in the caption to Fig. 9).

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