Ab Initio No Core Shell Model - Recent Results and Further Prospects
James P. Vary, Pieter Maris, Hugh Potter, Mark A. Caprio, Robin Smith,, Sven Binder, Angelo Calci, Sebastian Fischer, Joachim Langhammer, Robert, Roth, Hasan Metin Aktulga, Esmond Ng, Chao Yang, Dossay Oryspayev, Masha, Sosonkina, Erik Saule, \"Umit \c{C}ataly\"urek

TL;DR
This paper reviews recent advances in the ab initio No Core Shell Model, highlighting progress enabled by improved nuclear interactions, advanced algorithms, and high-performance computing, with prospects for future developments.
Contribution
It summarizes recent significant results in NCSM and discusses the key factors driving progress in nuclear structure modeling.
Findings
Enhanced nuclear interactions improve experimental data description.
Algorithmic advances enable complex quantum many-body simulations.
High-performance computing accelerates progress in nuclear physics.
Abstract
There has been significant recent progress in solving the long-standing problems of how nuclear shell structure and collective motion emerge from underlying microscopic inter-nucleon interactions. We review a selection of recent significant results within the ab initio No Core Shell Model (NCSM) closely tied to three major factors enabling this progress: (1) improved nuclear interactions that accurately describe the experimental two-nucleon and three-nucleon interaction data; (2) advances in algorithms to simulate the quantum many-body problem with strong interactions; and (3) continued rapid development of high-performance computers now capable of performing floating point operations per second. We also comment on prospects for further developments.
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Taxonomy
TopicsPhysics of Superconductivity and Magnetism · Nuclear physics research studies · Cold Atom Physics and Bose-Einstein Condensates
