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Magnetic Field-line Curvature and Its Role in Particle Acceleration by Magnetically Dominated Turbulence

  • Authors: Samuel T. Sebastian, Luca Comisso

Samuel T. Sebastian and Luca Comisso 2025 The Astrophysical Journal Letters 994 .

  • Provider: AAS Journals

Caption: Figure 6.

Time evolution of the proton energy spectrum ﹩dN/d\mathrm{ln}(\gamma -1)﹩ for the reference simulation (δB0/B0 = 1). Over time, the particle spectrum develops a high-energy power-law tail with index p = ﹩-d\mathrm{log}N/d\mathrm{log}(\gamma -1)\simeq 2.7﹩.

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