Role of firehose instability in diffusive shock acceleration
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Abstract:
Comparison of the contribution of pressure anisotropy to growth rates of instability with the contribution of current anisotropy of distribution function of the accelerated particles is carried out in shock prefronts of the supernova remnants. It is shown that the contribution of anisotropy of pressure can be important at disturbance scales close to gyroradii of the fastest accelerated particles.