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Cosmic-Ray Acceleration from Turbulence in Molecular Clouds

  • Authors: Brandt A. L. Gaches, Stefanie Walch, and A. Lazarian

2021 The Astrophysical Journal Letters 917 L39.

  • Provider: AAS Journals

Caption: Figure 1.

Basic schematic of the proposed mechanism. Top left: we assume a power-law power spectrum related to a line width–size relation. Top right: the turbulence driven at scale, , corresponds to an average density and magnetic field “seen” by the turbulence. Bottom right: Within the turbulence there are reconnection regions of width Δ (Equation (18)). Here, protons bounce between the reconnection fronts. Bottom left: the resulting acceleration, via the Fermi mechanism, results in a power-law energy distribution.

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