New simulations carried out in part on the ATERUI II supercomputer in Japan have found that the reason ions exist at higher temperatures than electrons in space plasma is because they are better able to absorb energy from compressive turbulent fluctuations in the plasma. These findings have important implications for understanding observations of various astronomical objects such as the images of the accretion disk and shadow of the M87 supermassive black hole captured by the Event Horizon Telescope.
In addition to the normal three states of matter (solid, liquid, and gas) which we see around us every day, there is an additional state called plasma which exists only at high temperatures. Under these conditions, electrons become separated from their parent atoms leaving behind positively charged ions. In space plasma the electrons and ions rarely collide with each other, meaning that they can coexist in different conditions, such as at different temperatures. However, there is no obvious reason why they should have different temperatures unless some force affects them differently. So why ions are usually hotter than electrons in space plasma has long been a mystery.
One way to heat plasma is by turbulence. Chaotic fluctuations in turbulence smoothly mix with particles, and then their energy is converted into heat. To determine the roles of different types of fluctuations in plasma heating, an international team led by Yohei Kawazura at Tohoku University in Japan performed the world’s first simulations of space plasma including two types of fluctuations, transverse oscillations of magnetic field lines and longitudinal oscillations of pressure. They used nonlinear hybrid gyrokinetic simulations which are particularly good at modeling slow fluctuations. These simulations were conducted on several supercomputers, including ATERUI II at the National Astronomical Observatory of Japan.
The results showed that the longitudinal fluctuations like to mix with ions but leave electrons. On the other hand, the transverse fluctuations can mix with both ions and electrons. “Surprisingly, the longitudinal fluctuations are picky about the partner species to mix with,” says Kawazura. This is a key result for understanding the ion-to-electron heating ratios in plasmas observed in space, like that around the supermassive black hole in Galaxy M87.
Reference: “Ion versus Electron Heating in Compressively Driven Astrophysical Gyrokinetic Turbulence” by Y. Kawazura, A. A. Schekochihin, M. Barnes, J. M. TenBarge, Y. Tong, K. G. Klein and W. Dorland, 11 December 2020, Physical Review X.
DOI: 10.1103/PhysRevX.10.041050
Funding: Science and Technology Facilities Council, Japan Society for the Promotion of Science, UK Engineering and Physical Sciences Research Council, National Science Foundation Solar, Heliospheric, and INterplanetary Environment, National Aeronautics and Space A.
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