Abstract
Modeling collisionless magnetic reconnection rate is an outstanding challenge in basic plasma physics research. While the seemingly universal rate of an order is often reported in the low- β regime, it is not clear how reconnection rate scales with a higher plasma β . Due to the complexity of the pressure tensor, the available reconnection rate model is limited to the low plasma- β regime, where the thermal pressure is arguably negligible. However, the thermal pressure effect becomes important when . Using first-principle kinetic simulations, we show that both the reconnection rate and outflow speed drop as β gets larger. A simple analytical framework is derived to take account of the self-generated pressure anisotropy and pressure gradient in the force balance around the diffusion region, explaining the varying trend of key quantities and reconnection rates in these simulations with different β . The predicted scaling of the normalized reconnection rate is in the high- β limit, where β i 0 is the ion β of the inflow plasma.
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CITATION STYLE
Li, X., & Liu, Y.-H. (2021). The Effect of Thermal Pressure on Collisionless Magnetic Reconnection Rate. The Astrophysical Journal, 912(2), 152. https://doi.org/10.3847/1538-4357/abf48c
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