A numerical assessment of cosmic-ray energy diffusion through turbulent media

M. Fatuzzo, F. Melia

Research output: Contribution to journalArticlepeer-review

9 Scopus citations


How and where cosmic rays are produced, and how they diffuse through various turbulent media, represent fundamental problems in astrophysics with far-reaching implications, both in terms of our theoretical understanding of high-energy processes in the Milky Way and beyond, and the successful interpretation of space-based and ground based GeV and TeV observations. For example, recent and ongoing detections, e.g., by Fermi (in space) and HESS (in Namibia), of γ-rays produced in regions of dense molecular gas hold important clues for both processes. In this paper, we carry out a comprehensive numerical investigation of relativistic particle acceleration and transport through turbulent magnetized environments in order to derive broadly useful scaling laws for the energy diffusion coefficients.

Original languageEnglish (US)
Article number131
JournalAstrophysical Journal
Issue number2
StatePublished - Apr 1 2014


  • acceleration of particles
  • cosmic rays
  • magnetohydrodynamics (MHD)
  • turbulence

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science


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