PAMOP Project: Computations in Support of Experiments and Astrophysical Applications

B. M. McLaughlin (), C. P. Ballance (), M. S. Pindzola (), P. C. Stancil (), S. Schippers () and A. Müller ()
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B. M. McLaughlin: Queen’s University, Centre for Theoretical Atomic Molecular and Optical Physics (CTAMOP), School of Mathematics & Physics, The David Bates Building
C. P. Ballance: Queen’s University, Centre for Theoretical Atomic Molecular and Optical Physics (CTAMOP), School of Mathematics & Physics, The David Bates Building
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
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 ´16, 2016, pp 33-48 from Springer

Abstract: Abstract Our computation effort is primarily concentrated on support of current and future measurements being carried out at various synchrotron radiation facilities around the globe, and photodissociation computations for astrophysical applications. In our work we solve the Schrödinger or Dirac equation for the appropriate collision problem 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. A brief summary of the methodology and ongoing developments implemented in the R-matrix suite of Breit-Pauli and Dirac-Atomic R-matrix codes (DARC) is presented.

Date: 2016
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DOI: 10.1007/978-3-319-47066-5_3

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