Next-Generation Ab Initio Symmetry-Adapted No-Core Shell Model and Its Impact on Nucleosynthesis
Jerry Draayer, Louisiana State University
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Umit Catalyurek, Pieter Maris, Erik Saule, Masha Sosonkina, Jerry Draayer, Tomas Dytrych, Kristina Launey, James Vary, Daniel Langr, Tomas Oberhuber, Robert BakerOur recently developed next-generation symmetry-adapted no-core shell model (SA-NCSM), which builds on first principles and symmetries of nuclear dynamics, targets ab initio descriptions of intermediate-mass nuclei, including short-lived nuclei not yet accessible to experiment but key to understanding astrophysical processes. While the implementation of the SA-NCSM for massively parallel computer systems achieves good load-balancing and scales beyond tens of thousands of processors, its computational complexity requires the Blue Waters petascale resources. This makes the SA-NCSM code ideal for runs on the Blue Waters system, while addressing long-standing challenges of importance to nuclear theory and experiment, as well as to astrophysics.
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