2D fully kinetic simulations establish that reconnection in current sheets during nonlinear KHI drives localized anisotropic electron energization with suprathermal tails.
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A self-consistent multi-zone kinetic model reproduces SN 1006's spectrum and morphology, finding ~20% CR acceleration efficiency in quasi-parallel shocks, <1% in quasi-perpendicular shocks, and predominantly leptonic gamma-ray emission.
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Reconnection-induced electron energization in magnetospheric Kelvin-Helmholtz dynamics
2D fully kinetic simulations establish that reconnection in current sheets during nonlinear KHI drives localized anisotropic electron energization with suprathermal tails.