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.
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.
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Presenters
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Liam H Scarlett
Curtin University of Technology, Curtin University
Authors
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Liam H Scarlett
Curtin University of Technology, Curtin University
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Corey T Plowman
Curtin University
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Mark C Zammit
Los Alamos National Laboratory (LANL)
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Igor Bray
Curtin University of Technology
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Dmitry V Fursa
Faculty of Science and Engineering, Curtin University, Curtin,Perth,WA, Australia, Curtin Univ of Technology
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Richard C Bergmayr
Max Planck Institute for Plasma Physics
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Dirk Wünderlich
Max Planck Institute for Plasma Physics
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Ursel E Fantz
Max Planck Institute for Plasma Physics
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Marco Padovani
INAF–Osservatorio Astrofisico di Arcetri
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Daniele Galli
INAF–Osservatorio Astrofisico di Arcetri
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Tommaso Grassi
Max-Planck-Institut für Extraterrestrische Physik