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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 7.

Probability density functions of ΔW_⊥ and ΔW_tot, normalized to the particle energy γ₀m_ic², accumulated over Δt = 0.5 l_c/c starting at t₀ = 2 l_c/c (γ₀ is the particle Lorentz factor at t₀) in the reference simulation. Different colors correspond to three distinct ranges of γ₀.

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