A 2026 evaluation framework by Ding and Sun (arXiv:2606.27541) found a strong linear correlation (Pearson coefficient 0.977) between theory–experiment binding-energy deviations of single- and double- hypernuclei computed with relativistic density functionals, anchored on the four double- systems with established binding-energy data (core nuclei He, Be, Be, B), and used it to propagate empirical single- constraints into evaluated interaction energies for heavier nuclei. The evaluated values systematically exceed direct functional predictions calibrated only to the NAGARA event, implying absorbed beyond-mean-field physics of unknown origin. The open problem is twofold and joint: establish whether the correlation is robust, framework-independent, and valid across the mass range by reproducing or refuting it within independent theoretical frameworks, and quantitatively identify which microscopic mechanisms — few-body clustering, core polarization, coupled-channel – mixing, or pairing — dominate the discrepancy between evaluated and direct predictions.
Background
A hypernucleus is an atomic nucleus containing one or more hyperons — baryons carrying strangeness, such as the (lambda, mass 1116 MeV, isospin zero) — in addition to protons and neutrons. Double- hypernuclei (strangeness ) are the only existing window onto the hyperon–hyperon interaction inside nuclear matter, which is otherwise unconstrained because free scattering data do not exist; this interaction matters both for fundamental baryon–baryon physics and for the composition of neutron-star cores, where hyperons are expected to appear. The key observable is the interaction energy , where and are the single- and double- separation energies: it isolates the extra binding due to the second beyond twice the single- binding, i.e. the effective attraction in the nuclear medium. Only a handful of double- events exist, all from nuclear-emulsion experiments: the NAGARA event (He, Takahashi et al. 2001; its interaction energy was revised to MeV in the E373 analysis of Ahn et al. 2013), which established weak attraction and remains the sole calibration anchor for the coupling in most models; an E373 event interpreted as Be (Ahn et al. 2013) and a J-PARC E07 event interpreted as Be (Ekawa et al. 2019); and a new B candidate with an B core found by machine-learning-assisted emulsion analysis (He et al. 2025). On the theory side, relativistic density functionals (RDF — covariant mean-field models with meson-mediated interactions, here the relativistic Hartree–Fock functionals PKO1/PKO2 and the density-dependent relativistic mean-field functionals TW99, PKDD, DD-ME2, DD-MEX) describe both sectors uniformly; alternative frameworks include the Skyrme–Hartree–Fock approach (non-relativistic mean field; Zhou et al. 2007) and ab initio few-body/quantum-Monte-Carlo methods rooted in chiral effective field theory (the systematic low-energy expansion of nuclear forces; Tong et al. 2025). Ding and Sun (2026) computed theory–experiment deviations of binding energies in both sectors and found a robust linear correlation, MeV, from the four light systems with double- data (core nuclei He, Be, Be, B). Exploiting it, they transferred the abundant empirical single- constraints to the data-sparse sector, obtaining evaluated and with quantified uncertainties for heavier nuclei. The evaluated stay below about 5 MeV, peak in the medium-mass region, and are systematically larger than direct RDF predictions whose coupling is fitted only to NAGARA; the authors attribute the difference to correlations beyond the mean field — few-body cluster structure, core polarization (the distortion of the core nucleus by the hyperons), coupled-channel – mixing (the mixing of double- states with states containing the hyperon, which share strangeness ), and possible Cooper pairing — but explicitly do not disentangle these mechanisms. The correlation itself rests on only four data points from light nuclei, and its validity for medium-mass and heavy systems, or within other theoretical frameworks, is assumed but unverified.
Problem Statement
Determine whether the linear correlation between single- and double- binding-energy deviations found by Ding and Sun (2026) — MeV, established within relativistic density functionals from the four light systems with double- data — is a robust, framework-independent property of hypernuclear many-body theory, by reproducing, refining, or refuting it within independent theoretical frameworks (e.g. Skyrme–Hartree–Fock or ab initio methods), where a refutation in any single framework is decisive whereas a determination of framework-independence requires concordance across more than one such framework, and characterizing its slope, intercept, statistical significance, and possible mass dependence toward medium-mass and heavy double- systems; and identify, quantitatively and in controlled model studies, which of these microscopic mechanisms — few-body clustering, core polarization, coupled-channel – mixing, or pairing — dominate the systematic difference between the correlation-evaluated and direct functional predictions calibrated only to the NAGARA event. These two legs serve one objective: turning the correlation-based evaluation into a validated, physically understood predictor of interaction energies across the nuclear chart, with predictions concrete enough to be confronted with upcoming double- measurements at J-PARC (Japan Proton Accelerator Research Complex) and HIAF (China's High Intensity heavy-ion Accelerator Facility) (the measurements themselves are the ultimate empirical test but are not part of what a theoretical answer must supply).
References
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- X. D. Sun, S. C. Han, J. N. Hu, A. Li, 'Exploring hyperon Skyrme forces in multi-Λ hypernuclei and neutron star matter', Mon. Not. R. Astron. Soc. 546, stag233 (2026), doi:10.1093/mnras/stag233, https://doi.org/10.1093/mnras/stag233 (preprint arXiv:2602.03388, https://arxiv.org/abs/2602.03388)