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Numerical modeling of relativistic particle shock acceleration

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Figure

Table 3. Subluminal high relativistic shocks: spectral indices (σ)for different shock Lorentz factors (�), two inclination angles (ψ)with a very small pitch angle diffusion angle (θ ≤ 10/ �) and maxi-mum attained energies Emax.
Fig. 1. An exemplary graph showing differential particle spectra forshock Lorentz factors of 5, 20, 50 (respectively from lower to uppera shock inclination of 45o, scattering of θ < π/4 and three differentgraph).

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