PAMOP: Large-Scale Calculations Supporting Experiments and Astrophysical Applications

B. M. McLaughlin (), C. P. Ballance (), M. S. Pindzola (), P. C. Stancil (), J. F. Babb (), S. Schippers () and A. Müller ()
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B. M. McLaughlin: Queen’s University Belfast, Centre for Theoretical Atomic, Molecular and Optical Physics (CTAMOP), School of Mathematics & Physics
C. P. Ballance: Queen’s University Belfast, Centre for Theoretical Atomic, Molecular and Optical Physics (CTAMOP), School of Mathematics & Physics
M. S. Pindzola: Auburn University, Department of Physics, 206 Allison Laboratory
P. C. Stancil: University of Georgia, Department of Physics and Astronomy and the Center for Simulational Physics
J. F. Babb: Harvard Smithsonian Center for Astrophysics, Institute for Theoretical Atomic and Molecular Physics
S. Schippers: Justus-Liebig-Universität Giessen, I. Physikalisches Institut
A. Müller: Justus-Liebig-Universität Giessen, Institut für Atom- und Molekülphysik

A chapter in High Performance Computing in Science and Engineering ' 17, 2018, pp 37-59 from Springer

Abstract: Abstract Our prime computation effort is to support current and future measurements of atomic photoionization cross-sections being performed at various synchrotron radiation facilities around the globe, and computations for astrophysical applications. In our work we solve the Schrödinger or Dirac equation using the R-matrix or R-matrix with pseudo-states approach from first principles. The time dependent close-coupling (TDCC) method is also used in our work. Finally, we present cross-sections and rates determined for diatom-diatom and radiative collision processes between atoms and ions currently of great interest to astrophysics.

Date: 2018
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Persistent link: https://EconPapers.repec.org/RePEc:spr:sprchp:978-3-319-68394-2_3

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DOI: 10.1007/978-3-319-68394-2_3

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