An examination of the adiabatic approximation in cosmic ray propagation theory

Details An examination of the adiabatic approximation in cosmic ray propagation theory An examination of the adiabatic approximation in cosmic ray propagation theory

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icrc....3..850s&link_type=abstract

In: International Cosmic Ray Conference, 14th, Munich, West Germany, August 15-29, 1975, Conference Papers. Volume 3. (A76-26851

Physics

2

Approximation, Cosmic Rays, Magnetic Fields, Particle Motion, Propagation Modes, Adiabatic Conditions, Average, Distribution Functions, Power Series, Truncation Errors, Turbulent Diffusion

Scientific paper

A theory for the pitch-angle scattering of cosmic rays in a turbulent magnetic field can be derived from first principles by applying both the quasi-linear and adiabatic approximations to the master equation for the ensemble averaged distribution function. A proof of the failure of these approximations, taken together, is given. Some predictions of the quasi-linear theory, are given. New wave-like propagation modes have been discovered.

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