Speed-dependent Threshold for Electron Injection into Diffusive Shock Acceleration

Abstract Finding the injection threshold for diffusive shock acceleration (DSA) of electrons in collisionless shocks has been a longstanding unsolved problem. Using first-principles kinetic simulations, we identify the conditions for electron injection into DSA and quantify the evolution of the nonthermal tail in self-generated electromagnetic turbulence. By analyzing electron trajectories and their momentum gain during shock-recrossing cycles, we demonstrate that electrons start participating in DSA when their speed is large enough to overrun the shock. We develop a minimal model showing that speed-dependent injection reproduces nonthermal electron spectra observed in kinetic simulations. Our findings establish a new criterion for electron DSA, which has broad implications for the shock-powered nonthermal emission from space/astrophysical systems.

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Publication Details

Journal
The Astrophysical Journal Letters
Published
2025-11-20
DOI
https://doi.org/10.3847/2041-8213/ae1ba9
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
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article

Speed-dependent Threshold for Electron Injection into Diffusive Shock Acceleration

Anatoly Spitkovsky, Siddhartha Gupta, Damiano Caprioli
The Astrophysical Journal Letters
Ionosphere and magnetosphere dynamics
article

Speed-dependent Threshold for Electron Injection into Diffusive Shock Acceleration

Anatoly Spitkovsky, Siddhartha Gupta, Damiano Caprioli
article en

Abstract

Abstract Finding the injection threshold for diffusive shock acceleration (DSA) of electrons in collisionless shocks has been a longstanding unsolved problem. Using first-principles kinetic simulations, we identify the conditions for electron injection into DSA and quantify the evolution of the nonthermal tail in self-generated electromagnetic turbulence. By analyzing electron trajectories and their momentum gain during shock-recrossing cycles, we demonstrate that electrons start participating in DSA when their speed is large enough to overrun the shock. We develop a minimal model showing that speed-dependent injection reproduces nonthermal electron spectra observed in kinetic simulations. Our findings establish a new criterion for electron DSA, which has broad implications for the shock-powered nonthermal emission from space/astrophysical systems.

The Astrophysical Journal LettersVol. 994(2)
Fermi National Accelerator Laboratory (US), Princeton University (US), University of Chicago (US), Inter-University Centre for Astronomy and Astrophysics (IN)
Openalex Percentile: Top 76%
Ionosphere and magnetosphere dynamics
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