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- W2043103460 abstract "As a rule, the shock compression controls the spectrum of diffusively accelerated particles. We argue that this is not so if the backreaction of these particles of the shock structure is significant. We present a self-similar solution in which the accelerated particles change the flow structure near the shock so strongly that the total shock compression may become very large. Despite this, the energy spectrum behind the shock is close to E−32 independently of compression." @default.
- W2043103460 created "2016-06-24" @default.
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- W2043103460 date "2000-01-01" @default.
- W2043103460 modified "2023-09-27" @default.
- W2043103460 title "Strong astrophysical shocks as universal accelerators of charged particles" @default.
- W2043103460 cites W2064221922 @default.
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- W2043103460 doi "https://doi.org/10.1016/s0273-1177(99)01236-3" @default.
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