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QCD-based charge symmetry breaking interaction and the Okamoto-Nolen-Schiffer anomaly

Hiroyuki Sagawa (佐川弘幸)1,2, Tomoya Naito (内藤智也)3,4, Xavier Roca-Maza5,6,7, and Tetsuo Hatsuda (初田哲男)3

  • 1RIKEN Nishina Center for Accelerator-based Science, Wako 351-0198, Japan
  • 2Center for Mathematics and Physics, University of Aizu, Aizu-Wakamatsu, Fukushima 965-8560, Japan
  • 3RIKEN Interdisciplinary Theoretical and Mathematical Sciences Program (iTHEMS), Wako 351-0198, Japan
  • 4Department of Physics, Graduate School of Science, The University of Tokyo, Tokyo 113-0033, Japan
  • 5Departament de Física Quàntica i Astrofísica and Institut de Ciències del Cosmos, Universitat de Barcelona, Martí i Franqués 1, 08028 Barcelona, Spain
  • 6Dipartimento di Fisica, Università degli Studi di Milano, Via Celoria 16, 20133 Milano, Italy
  • 7INFN, Sezione di Milano, Via Celoria 16, 20133 Milano, Italy

Phys. Rev. C 109, L011302 – Published 25 January, 2024

DOI: https://doi.org/10.1103/PhysRevC.109.L011302

Abstract

An approach is proposed to link the charge symmetry breaking (CSB) nuclear interaction and the low-energy constants in quantum chromodynamics (QCD) by matching the CSB effect in nuclear matter. The resulting CSB interaction is applied to study the Okamoto-Nolen-Schiffer anomaly, still lacking a satisfactory microscopic understanding, on the energy differences of mirror nuclei by taking F17−O17, O15−N15, Sc41−Ca41, and Ca39−K39 as typical examples. The magnitude and sign of the QCD-based CSB interactions are found to resolve the anomaly successfully within theoretical uncertainties.

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