A method tests DSA and diffusion propagation for 1-100 TeV cosmic electrons with Geminga halo and PWN spectral and morphological data from HAWC and Fermi-LAT, finding consistency but limited by wide energy bins in current observations.
K´ ota, Theory and modeling of galactic cosmic rays: Trends and prospects, Space Science Reviews176, 391 (2013)
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Method for testing diffusive shock acceleration and diffusion propagation of 1-100 TeV cosmic electrons with multiwavelength observations of the Geminga halo and pulsar wind nebula
A method tests DSA and diffusion propagation for 1-100 TeV cosmic electrons with Geminga halo and PWN spectral and morphological data from HAWC and Fermi-LAT, finding consistency but limited by wide energy bins in current observations.