Cosmic ray transport and acceleration in an evolving shock landscape

Open Access

Fig. 7.

Analytical solution of the Sedov-Taylor blast wave with constant density (dashed line) compared to the Isenberg solution with decreasing density profile (solid line) for E_inj = 10 E_SN, r₀ = 1 kpc, and ρ₀ = 1 m_p/m³. Considerably higher shock speeds are reached for the latter.

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