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astro-ph2006★ 33 cited
Dynamics of Mesoscale Magnetic Field in Diffusive Shock Acceleration
P. H. Diamond, M. A. Malkov
We present a theory for the generation of mesoscale (, where is the cosmic ray gyroradius) magnetic fields during diffusive shock acceleration. The decay or mo…
astro-ph2005
On the gamma-ray spectra radiated by protons accelerated in SNR shocks near molecular clouds: The case of SNR RX J1713.7-3946
M. A. Malkov, P. H. Diamond, R. Z. Sagdeev
Cosmic rays (CRs) are thought to be accelerated in SNRs. The most favorable situation for proving that the main, hadronic CR component is accelerated there is when CRs interact wit…