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Fig. 4

image

As in Fig. 3, but adopting additional mechanisms on the basis of fiducial model 2. In panels A–C three cases with aRRK = 0, 0.05, and 0.1 are considered, respectively. In panel D a case with faster diffusion rates Eb = 0.3Ed is considered. In panels E–H a scenario with a shock passage is considered, where T = 10 and 20 K represent the temperature when the shocks occurs in the warm-up phase (ttotal = 3 × 105 yr and 3.459 × 105 yr, respectively). Peak temperatures Tpeak = 200 and 1000 K are the temperatures during shock passage, and t = 102 yr is the duration the passage. In panels I–L a scenario with an X-ray burst is considered, which is described in the models by the elevated cosmic ray ionization rate of ζCR = 1.3 × 10−14 s−1 and 1.3 × 10−13 s−1, T = 10 and 20 K, and the X-ray burst duration is t = 102 yr. After the shock passage and the X-ray burst, all parameters are the same as in fiducial model 2.

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