The first kinetic simulation of expanding Alfvénic turbulence shows formation of parallel suprathermal electron power-law tails that persist through firehose instability.
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In multispecies relativistic turbulence, energization occurs at reconnection current sheets driven by the divergence of the relativistic pressure tensor, with electrons accelerated more efficiently than positrons due to species imbalance.
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Formation of Suprathermal Electron Populations in the Expanding, Turbulent Solar Wind
The first kinetic simulation of expanding Alfvénic turbulence shows formation of parallel suprathermal electron power-law tails that persist through firehose instability.
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Particle-acceleration mechanisms in multispecies relativistic plasmas
In multispecies relativistic turbulence, energization occurs at reconnection current sheets driven by the divergence of the relativistic pressure tensor, with electrons accelerated more efficiently than positrons due to species imbalance.