On particle acceleration around shocks. II: on the diffuse scattering by moving media

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The probability that a particle, crossing the shock along a given direction, be reflected backwards along another direction, was shown to be the key element in determining the spectrum of non--thermal particles accelerated via Fermi mechanism around a shock. Here an explicit equation for this probability distribution is given, for both the upstream and downstream sections. Though analytically intractable, this equation can be easily solved numerically.
This paper is withdrawn. A revised version, already accepted for publication in The Astrophysical Journal, will be submitted tomorrow

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