PaperPanorama

Nuclear Theory·nucl-th

Friday·June 7, 2024

7 papers4 primary·3 cross-listed

  1. 01

    Impact of correlations on nuclear binding energies

    Alberto Scalesi🇫🇷 · Thomas Duguet🇫🇷 · Pepijn Demol🇧🇪 · Mikael Frosini🇫🇷 · Vittorio Somà🇫🇷 · Alexander Tichai🇩🇪

    A strong effort will be dedicated in the coming years to extend the reach of ab initio nuclear-structure calculations to heavy doubly open-shell nuclei. In order to do so, the most efficient strategies to incorporate dominant many-body correlations at play in such nuclei must be identified. With this motivation in mind, the present work pedagogically analyses the inclusion of many-body correlations and their impact on binding energies of Calcium and Chromium isotopes. Employing an empirically-optimal Hamiltonian built from chiral effective field theory, binding energies along both isotopic chains are studied via a hierarchy of approximations based on polynomially-scaling expansion many-body methods. The corresponding results are compared to experimental data and to those obtained via valence-space in-medium similarity renormalization group calculations at the normal-ordered two-body level that act as a reference in the present study. The spherical mean-field approximation is shown to display specific shortcomings in Ca isotopes that can be understood analytically and that are efficiently corrected via the consistent addition of low-order dynamical correlations on top of it. While the same setting cannot appropriately reproduce binding energies in doubly open-shell Cr isotopes, allowing the unperturbed mean-field state to break rotational symmetry permits to efficiently capture the static correlations responsible for the phenomenological differences observed between the two isotopic chains. Eventually, the present work demonstrates in a pedagogical way that polynomially-scaling expansion methods based on unperturbed states that possibly break (and restore) symmetries constitute an optimal route to extend ab initio calculations to heavy closed- and open-shell nuclei.

    nucl-thEPJA(2024)·14 citations
  2. 02

    hypernuclei by folding the state-of-the-art interactions

    Faisal Etminan🇮🇷

    I examined a phenomenological Nijmegen and a first principles HAL QCD potentials to study ineractions. A Woods-Saxon type form for potential in the single-folding potential approach is derived by using the spin- and isospin averaged interactions. The possibility of resonance or bound state is searched and accordingly, the low energy scattering phase shift parameters of are calculated. The numerical results show that even though two potentials have significantly dissimilar isospin (I) and spin (S) components, could be only a Coulomb-assisted resonance state that appears about MeV below the threshold of for both model of potentials.

    nucl-thhep-ph0 citations
  3. 03

    Evidence for strong isovector nuclear spin-orbit interaction

    Tong-Gang Yue🇨🇳 · Zhen Zhang🇨🇳 · Lie-Wen Chen🇨🇳

    The nucleon spin-orbit interaction is a cornerstone of nuclear structure theory, yet its isospin dependence remains elusive owing to the lack of clean experimental probes. Here we show that the charge-weak form factor difference in Ca, recently extracted in a model-independent manner by the CREX experiment, exhibits strong sensitivity to the isovector spin-orbit interaction. Using Skyrme-like energy density functionals, we demonstrate that a significantly enhanced isovector spin-orbit interaction, about four times stronger than conventional parametrizations, can resolve the PREX-CREX puzzle, which has challenged modern nuclear theories and our understanding of nuclear symmetry energy, while maintaining a good description of nuclear bulk properties and well-established shell structure of finite nuclei. This enhanced isovector spin-orbit interaction also provides a novel mechanism for the emergence of the , , and magic numbers in neutron-rich nuclei on the mean-field level. These findings point to a strong isospin dependence of the nucleon spin-orbit interaction, which is expected to have important implications for nuclear structures, electroweak nuclear processes, and related problems in nuclear astrophysics.

    nucl-thastro-ph.HEhep-phnucl-exSci.Bull.(2026)·23 citations
  4. 04

    Genetic Programming for the Nuclear Many-Body Problem: a Guide

    Illya Bakurov · Pablo Giuliani · Kyle Godbey · Nathaniel Haut · Wolfgang Banzhaf · Witold Nazarewicz

    Genetic Programming is an evolutionary algorithm that generates computer programs, or mathematical expressions, to solve complex problems. In this Guide, we demonstrate how to use Genetic Programming to develop surrogate models to mitigate the computational costs of modeling atomic nuclei with ever increasing complexity. The computational burden escalates when uncertainty quantification is pursued, or when observables must be globally computed for thousands of nuclei. By studying three models in which the mean field depends on the total particle density self-consistently, we show that by constructing reduced order models supported by Genetic Programming one can speed up many-body computations by several orders of magnitude with a negligible loss in accuracy

    nucl-thJ.Phys.G(2025)·5 citations

Affiliations

first authorsco-authorsvia INSPIRE