Electron acceleration in laboratory-produced turbulent collisionless shocks

Astrophysical collisionless shocks are among the most powerful particle accelerators in the Universe. Generated by violent interactions of supersonic plasma flows with the interstellar medium, supernova remnant shocks are observed to amplify magnetic fields 1 and accelerate electrons and protons to...

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Veröffentlicht in:	Nature physics 2020-09, Vol.16 (9), p.916-920
Hauptverfasser:	Fiuza, F., Swadling, G. F., Grassi, A., Rinderknecht, H. G., Higginson, D. P., Ryutov, D. D., Bruulsema, C., Drake, R. P., Funk, S., Glenzer, S., Gregori, G., Li, C. K., Pollock, B. B., Remington, B. A., Ross, J. S., Rozmus, W., Sakawa, Y., Spitkovsky, A., Wilks, S., Park, H.-S.
Format:	Artikel
Sprache:	eng
Schlagworte:	639/766/1960/1134 639/766/1960/1135 70 PLASMA PHYSICS AND FUSION TECHNOLOGY ASTRONOMY AND ASTROPHYSICS astrophysical plasmas Atomic Classical and Continuum Physics collisionless shocks Complex Systems Computational fluid dynamics Computer simulation Condensed Matter Physics Electron acceleration high-energy-density plasmas High-energy-density plasmas, astrophysical plasmas, collisionless shocks, particle acceleration Injection Interstellar matter Laboratories Letter Mathematical and Computational Physics Molecular Optical and Plasma Physics particle acceleration Particle accelerators Particle physics Physics Physics - Plasma physics Physics and Astronomy Plasmas (physics) Relativistic effects Relativistic particles Supernova remnants Theoretical Turbulence
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