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Fig. 15

image

Top panel: time evolution of total thermal (solid lines), CR energy (dashed lines), and magnetic energy (dot-dashed lines) in the simulated turbulent ISM boxes for the simulations without shock-acceleration (black), without CR streaming, and without (red) or with (green) obliquity dependency for CR acceleration, and with obliquity and CR streaming (blue) with η0 = 0.1 and . Bottom panel: evolution of the dissipated thermal (solid) and CR (dashed) energy rates at shocks for the same simulations.

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