Abstract
We perform ab initio calculations of three-point mass differences in the odd- and even-mass 39−49Ca isotopes to probe nuclear superfluidity via empirical neutron pairing gaps. We also quantify the sensitivity of those gaps to the parameters of the interaction at mean-field level. Recent studies employing accurate chiral nuclear interactions have found these gaps to be too small. We show that experimental values can be reproduced at mean-field level by substantially increasing the attraction of the singlet S-wave two-nucleon contact interaction, but doing so induces an unphysical bound state of the dineutron. The sensitivity of these predictions to the full calibration of the nuclear interaction is then studied by performing Bayesian posterior sampling in a delta-full chiral effective field theory at third chiral order. We find that pairing gaps remain largely unaffected, leaving the explanation of nuclear superfluidity as a future task for improved many-body modeling and refined interactions at higher chiral orders.
| Original language | English |
|---|---|
| Journal | Physical Review C |
| Volume | 113 |
| Issue number | 5 |
| DOIs | |
| State | Published - May 11 2026 |
Funding
Acknowledgments. The authors thank T. Duguet and V. Somà for useful comments on the manuscript. This work is inspired by discussions at the ESNT workshop ‘Ab initio many-body calculations: where has the nuclear pairing gone?’ (Saclay, 2025). A.S. thanks H. Hergert for providing benchmarks for the implementation of three-body forces in the HFB code. This work was supported by the Swedish Research Council (Grants No. 2020-05127, No. 2021-04507, and No. 2024-04681). This work was also supported by the U.S. Department of Energy (DOE), Office of Science, under SciDAC-5 (NUCLEI Collaboration). Computer time was provided by the Innovative and Novel Computational Impact on Theory and Experiment (INCITE) program. This research used resources from the Oak Ridge Leadership Computing Facility located at ORNL, which is supported by the Office of Science of the Department of Energy under Contract No. DE-AC05-00OR22725.
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