TY - JOUR
T1 - Ion Acceleration in Driven Magnetic Reconnection during High-energy-Density Plasma Interaction
AU - Pongkitiwanichakul, Peera
AU - Fox, William
AU - Ruffolo, David
AU - Malakit, Kittipat
AU - Lezhnin, Kirill V.
AU - Matteucci, Jack
AU - Bhattacharjee, Amitava
N1 - Publisher Copyright:
© 2021. The American Astronomical Society. All rights reserved..
PY - 2021/2/1
Y1 - 2021/2/1
N2 - Strongly driven magnetic reconnection occurs in astrophysical events and also in laboratory experiments with laser-produced plasma. We have performed 2.5D particle-in-cell simulations of collisions of two high-energy-density plasmas resulting in strongly driven magnetic reconnection that demonstrates significant non-thermal ion acceleration. Such acceleration is significant only when the plasma beta is sufficiently low that the Alfvén speed at the reconnection inflow exceeds the thermal speed. Under these conditions, the most energetic ions are primarily accelerated by the Hall electric field in the reconnection outflow, especially at the trailing edge of an emerging plasmoid in the outflow. Laboratory experiments in the near future should be able to confirm these predictions and their applicability to astrophysical situations.
AB - Strongly driven magnetic reconnection occurs in astrophysical events and also in laboratory experiments with laser-produced plasma. We have performed 2.5D particle-in-cell simulations of collisions of two high-energy-density plasmas resulting in strongly driven magnetic reconnection that demonstrates significant non-thermal ion acceleration. Such acceleration is significant only when the plasma beta is sufficiently low that the Alfvén speed at the reconnection inflow exceeds the thermal speed. Under these conditions, the most energetic ions are primarily accelerated by the Hall electric field in the reconnection outflow, especially at the trailing edge of an emerging plasmoid in the outflow. Laboratory experiments in the near future should be able to confirm these predictions and their applicability to astrophysical situations.
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U2 - 10.3847/1538-4357/abccd3
DO - 10.3847/1538-4357/abccd3
M3 - Article
AN - SCOPUS:85101630372
SN - 0004-637X
VL - 907
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 86
ER -