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Family of Chiral Two- plus Three-Nucleon Interactions for Accurate Nuclear Structure Studies

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arxiv 1911.04955 v1 pith:Q4YWVUCR submitted 2019-11-12 nucl-th

classification nucl-th
keywords interactionschiralenergiesnuclearaccurateconstantscutoffdependence
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We present a family of nucleon-nucleon (NN) plus three-nucleon (3N) interactions up to N3LO in the chiral expansion that provides an accurate ab initio description of ground-state energies and charge radii up to the medium-mass regime with quantified theory uncertainties. Starting from the NN interactions proposed by Entem, Machleidt and Nosyk, we construct 3N interactions with consistent chiral order, non-local regulator, and cutoff value and explore the dependence of nuclear observables over a range of mass numbers on the 3N low-energy constants. By fixing these constants using the 3-H and 16-O ground-state energies, we obtain interactions that robustly reproduce experimental energies and radii for large range from p-shell nuclei to the nickel isotopic chain and resolve many of the deficiencies of previous interactions. Based on the order-by-order convergence and the cutoff dependence of nuclear observables, we assess the uncertainties due the interaction, which yield a significant contribution to the total theory uncertainty.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. A Gaussian Process framework for constraining the nuclear equation of state from microscopic calculations with correlated uncertainties

    nucl-th 2026-08 conditional novelty 6.0 of 10

    GPDiff fits a hierarchical Gaussian process to microscopic asymmetric-matter energies and propagates correlated uncertainties to EOS parameters and neutron-star matter properties.

  2. From bare two-nucleon interaction to nuclear matter and finite nuclei in a relativistic framework

    nucl-th 2025-07 conditional novelty 6.0 of 10

    A leading-order relativistic chiral two-nucleon force, with four constants fit to scattering data, describes nuclear matter saturation and medium-mass nuclei binding energies and radii without three-nucleon forces.

  3. Nuclear and neutron matter in the relativistic Brueckner-Hartree-Fock theory with next-to-leading order covariant chiral nuclear force

    nucl-th 2025-06 conditional novelty 6.0 of 10

    The authors find that NLO covariant chiral nuclear forces in relativistic Brueckner-Hartree-Fock theory reproduce the empirical saturation energy, density, and incompressibility of symmetric nuclear matter at cutoff 5...

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