
Plasma Physics (physics.plasm-ph)
Tue, 05 Sep 2023
1.Average-atom Ziman resistivity calculations in expanded metallic plasmas: effect of mean ionization definition
Authors:Nadine Wetta, Jean-Christophe Pain
Abstract: We present calculations of electrical resistivity for expanded boron, aluminum, titanium and copper plasmas using the Ziman formulation in the framework of the average-atom model. Our results are compared to experimental data, as well as with other theoretical calculations, relying on the Ziman and Kubo-Greenwood formulations, and based on average-atom models or quantum-molecular-dynamics simulations. The impact of the definition of ionization, paying a particular attention to the consistency between the latter and the perfect free electron gas assumption made in the formalism, is discussed. We propose a definition of the mean ionization generalizing to expanded plasmas the idea initially put forward for dense plasmas, consisting in dropping the contribution of quasi-bound states from the ionization due to continuum ones. It is shown that our recommendation for the calculation of the quasi-bound density of states provides the best agreement with measurements.
2.3D simulations of positive streamers in air in a strong external magnetic field
Authors:Zhen Wang, Anbang Sun, Saša Dujko, Ute Ebert, Jannis Teunissen
Abstract: We study how external magnetic fields from 0 to 40 T influence positive streamers in atmospheric air, using 3D PIC-MCC (particle-in-cell, Monte Carlo collision) simulations. When a magnetic field B is applied perpendicular to the background field E, the streamers tend to branch quite symmetrically in the plane spanned by E and B. With a stronger magnetic field the branching angle increases, and for the 40 T case the branches grow almost parallel to the magnetic field. We also observe a deviation in the -ExB direction, which is related to the ExB drift of electrons. Both with a perpendicular and with a parallel magnetic field, the streamer radius decreases with the magnetic field strength.