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On the escape of particles from cosmic ray modified shocks

Description: The solution of the problem of particle acceleration in the non-linear regime, when the dynamical reaction of the accelerated particles cannot be neglected, shows strong shock modification.When stationarity is imposed by hand, the solution may show a prominent energy flux away from the shock towards upstream infinity. This feature is peculiar of cosmic ray modified shocks, while being energetically insignificant in the test particle regime. The escape flux appears also in situations in which it… more
Date: July 1, 2008
Creator: Caprioli, D.; /Pisa, Scuola Normale Superiore; Blasi, P.; /Fermilab, /Arcetri Observ.; Amato, E. & Observ., /Arcetri
Partner: UNT Libraries Government Documents Department
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Dynamical Feedback of Self-generated Magnetic Fields in Cosmic Rays Modified Shocks

Description: We present a semi-analytical kinetic calculation of the process of non-linear diffusive shock acceleration (NLDSA) which includes magnetic field amplification due to cosmic ray induced streaming instability, the dynamical reaction of the amplified magnetic field and the possible effects of turbulent heating. This kinetic calculation allows us to show that the net effect of the amplified magnetic field is to enhance the maximum momentum of accelerated particles while reducing the concavity of th… more
Date: July 1, 2008
Creator: Caprioli, D.; /Pisa, Scuola Normale Superiore; Blasi, P.; /Fermilab, /Arcetri Observ.; Amato, E.; Observ., /Arcetri et al.
Partner: UNT Libraries Government Documents Department
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