Collisional-radiative modeling projects using convergent close-coupling collision data

ORAL  · Invited

Abstract

The development of the molecular convergent close-coupling (MCCC) method has enabled large-scale convergence studies to be performed for molecular targets for the first time. Over the last decade we have been applying this technology to the electron-H2 scattering system, with the long-term goal of producing a complete collision data set for application in collisional-radiative models. Previously, the majority of available data were either from small close-coupling calculations valid only at low energies, or semi-classical calculations valid only at high energies. There was also little vibrationally- and rotationally-resolved data available.

Motivated by fusion and astrophysical applications, we have produced cross sections numbering in the hundreds of thousands for electrons scattering on H2 and its five isotopologues, considering rovibrational levels in the first 20 electronic states. These data have allowed detailed collisional-radiative models for low-temperature hydrogen plasmas to be constructed for the first time. In this talk, we provide an update on our collaborations with researchers who are using MCCC cross sections in plasma modeling applications, primarily in the studies of tokamak divertor plasmas and cosmic-ray propagation in molecular clouds. We will also present new results for proton-H2 collisions, calculated using a newly-developed semi-classical implementation of the MCCC method.

*This research was supported by the Australian Government through the Australian Research Council's Discovery Projects funding scheme (project DP240101184). L.H.S is the recipient of an Australian Research Council Discovery Early Career Researcher Award (project number DE240100176) funded by the Australian Government. M.C.Z would like to specifically acknowledge the Los Alamos National Laboratory (LANL) ASC PEM Atomic Physics Project. LANL is operated by Triad National Security, LLC, for the National Nuclear Security Administration of the U.S. Department of Energy under Contract No. 89233218NCA000001. This work was supported by resources provided by the Pawsey Supercomputing Centre with funding from the Australian Government and the Government of Western Australia.

Presenters

  • Liam H Scarlett

    • Curtin University
    • Curtin University of Technology

Authors

  • Liam H Scarlett

    • Curtin University
    • Curtin University of Technology
  • Corey T Plowman

    • Curtin University
  • Mark C Zammit

    • Los Alamos National Laboratory (LANL)
  • Igor Bray

    • Curtin University of Technology
  • Dmitry V Fursa

    • Faculty of Science and Engineering, Curtin University, Curtin,Perth,WA, Australia
    • Curtin Univ of Technology
  • Richard C Bergmayr

    • Max Planck Institute for Plasma Physics
  • Dirk Wünderlich

    • Max Planck Institute for Plasma Physics
  • Ursel E Fantz

    • Max Planck Institute for Plasma Physics
  • Marco Padovani

    • INAF–Osservatorio Astrofisico di Arcetri
  • Daniele Galli

    • INAF–Osservatorio Astrofisico di Arcetri
  • Tommaso Grassi

    • Max-Planck-Institut für Extraterrestrische Physik