72nd Annual Gaseous Electronics Conference
Volume 64, Number 10
Monday–Friday, October 28–November 1 2019;
College Station, Texas
Session LW1: Electron and Positron Collisions with Atoms
1:45 PM–3:45 PM,
Wednesday, October 30, 2019
Room: Century I
Chair: Dmitry Fursa, Curtin University
Abstract: LW1.00001 : Electron Scattering from Complex Atoms and Ions: Current Status and Future Prospects.*
1:45 PM–2:15 PM
Preview Abstract
Abstract
Author:
Klaus Bartschat
(Drake University)
Accurate data for electron collisions with atoms
and ions are required for many modelling applications in a variety of fields,
including astrophysics, atmospheric physics, as well as plasma physics over a
wide range of electron temperatures [1]. Since it is virtually impossible to
measure all the data needed for state-of-the-art collisional radiative models
(CRMs), much of the responsibility for generating sufficiently comprehensive
datasets has been put on theory.
Consequently, a variety of methods have been developed and applied since the
early days of quantum mechanics [2]. They include special-purpose approaches
that are suitable but also limited to particular processes (e.g., elastic
scattering), perturbative techniques (e.g., first- and second-order plane-wave
or distorted-wave methods, which are usually limited to sufficiently high
energies), and the non-perturbative close-coupling (CC) approach that is based
on an (in principle complete) expansion of the projectile + target scattering
wave function. CC methods were originally designed for low energies and
near-threshold resonances, but the inclusion of so-called
``pseudo-states'' has extended the regime of applicability
tremendously, even enabling the calculation of ionization cross sections.
While the problem for electron collisions with light (quasi-)one- and
(quasi-)two-electron targets (H, He, light alkalis and alkaline-earth elements,
and the corresponding iso-electronic ions) is considered to be essentially
solved, this is by no means the case for heavy, complex, open-shell targets.
Examples include Fe and its lowly charged ions, which are of tremendous
importance for astrophysics, the heavy noble gases (Ne$-$Xe) for modelling of
various plasmas, and targets like W and its ions where data are needed to model
fusion reactors.
In this talk, I will introduce the basic ideas behind a selection of methods,
discuss their strengths and weaknesses, and concentrate on how to assess the
quality of the data [3] that are available from a number of databases
maintained worldwide.
[1] K. Bartschat, Journal of Physics B {\bf 51} (2018) 132001.
[2] K. Bartschat, J. Tennyson, and O. Zatsarinny, Plasma Processes and Polymers
{\bf 49} (2017) 1600093.
[3] H.K. Chung {\it et al.}, Journal of Physics D {\bf 49} (2016)
363002.
*Work performed, in part, in collaboration with Oleg Zatsarinny and supported by the NSF under PHY-1520970, PHY-1803844, OAC-1834740, and XSEDE-090031.