Σ⁻ atomic X-ray data and inclusive (π⁻,K⁺) quasi-free spectra have established that the Σ⁻-nucleus optical potential is repulsive inside the nuclear surface, weakly attractive outside it, and strongly absorptive ( MeV), but both observables probe mainly the nuclear surface and cannot determine the radial shape of at small radii or the magnitude of its central repulsion: among candidate potentials that fit all existing data, the central repulsion ranges from about 40 MeV (RMF- and LDA-NF-type) to about 80 MeV (DD-type). Harada and Hirabayashi (2009) proposed to break this degeneracy by populating Coulomb-assisted bound states in near-recoilless reactions on medium-heavy targets such as Ni, showing that inclusive spectra discriminate repulsive from attractive interiors but still cannot fix the interior details because of absorption and level overlap. The open problem is the quantitative determination of the interior -nucleus potential through observables and experimental strategies genuinely sensitive to the nuclear interior, validated against the global data set. The authors' own 2023 follow-up analysis of (π⁻,K⁺) spectra still states that the interior radial distribution and its strength at the center are difficult to determine, and the proposed measurement has not been performed.
Background
A hypernucleus is a bound nuclear system in which one or more nucleons are replaced by a hyperon (a baryon containing a strange quark). While Λ hypernuclei are copiously produced and narrow, Σ hypernuclei almost do not exist: the ΣN→ΛN conversion process, allowed because the Λ is about 80 MeV lighter than the Σ, gives any Σ in nuclear matter a large width, estimated early on at roughly 20 MeV (A. Gal and C. B. Dover, Phys. Rev. Lett. 44 (1980) 379). The only firmly established Σ hypernucleus remains He, seen as a few-MeV-bound, several-MeV-wide state in the He reaction (R. S. Hayano et al., Phys. Lett. B 231 (1989) 355).
What can be determined empirically is the Σ⁻-nucleus optical potential, i.e. the complex effective potential generated by the strong ΣN interaction in the medium, with the real part describing binding/repulsion and the imaginary part absorption by ΣN→ΛN conversion. Two data sets constrain it. First, Σ⁻ atoms — Coulomb-bound states of a Σ⁻ captured in an atomic orbit — give strong-interaction shifts and widths of X-ray transitions that probe the potential tail near the nuclear surface; the global analysis by E. Friedman and A. Gal (Phys. Rep. 452 (2007) 89) concluded that the potential is repulsive inside the nucleus with a shallow attractive pocket outside the surface, with little sensitivity to the interior radial shape. Second, inclusive quasi-free spectra — spectra dominated by production on individual nucleons, populating mostly continuum states — measured by the KEK-E438 collaboration (H. Noumi et al., Phys. Rev. Lett. 89 (2002) 072301; P. K. Saha et al., Phys. Rev. C 70 (2004) 044613) demand a repulsive interior with a nonzero imaginary part; semiclassical and distorted-wave analyses (M. Kohno et al., Prog. Theor. Phys. 112 (2004) 895; T. Harada and Y. Hirabayashi, Nucl. Phys. A 759 (2005) 143) reached the same conclusion. The physical origin of the repulsion is usually attributed to the isospin-, channel (the spin-triplet S-wave state of the –nucleon pair), whose quark configuration is Pauli-forbidden in the constituent-quark model, making the interior strength of the repulsion a candidate signal of quark degrees of freedom in nuclear matter.
The unsolved issue is quantitative: phenomenological potentials consistent with all Σ⁻-atomic and data differ strongly inside the nucleus — the density-dependent (DD) potential has a central repulsion of roughly 80 MeV, while relativistic-mean-field (RMF) and local-density (LDA-NF) potentials have about 40 MeV — and no existing observable distinguishes them, because both data types are dominated by the potential outside the nuclear surface and by the continuum.
T. Harada and Y. Hirabayashi (Nucl. Phys. A 829 (2009) 100) therefore studied Coulomb-assisted bound states: in medium-heavy and heavy nuclei the Coulomb attraction on the Σ⁻ can bind levels even against a repulsive strong potential (the 'hybrid' states of T. Yamazaki et al., Phys. Lett. B 207 (1988) 393), and the wave functions sample the nuclear interior with an rms radius comparable to the nuclear radius. They calculated inclusive spectra on Si, Ni and Pb targets within the distorted-wave impulse approximation (DWIA) — the standard framework in which an in-medium two-body amplitude, Fermi-averaged over the momentum distribution of bound nucleons, is sandwiched between distorted incoming-kaon and outgoing-pion waves and nuclear single-particle wave functions. They found that the near-recoilless reaction on Ni at MeV/c (momentum transfer MeV/c) produces a clear bump from the , and components of –Co that would discriminate repulsive from attractive interiors at J-PARC. However, they also concluded that the sizable absorption ( MeV) and the overlapping of levels prevent inclusive spectra from determining the radial distribution inside the nucleus and the strength of the central repulsion; that the candidate potentials used are phenomenological, obtained by fitting to the Σ⁻ atomic X-ray and data; that for heavy nuclei the effect of the Σ-nucleus potential is masked by the Coulomb attraction and the level spacing of the populated Σ⁻ states is very tight, making the inclusive spectra rather insensitive, so that choosing an appropriate nucleus as a target — e.g., Ni — is essential; and that the predicted absolute yields depend on the assumed Fermi-averaged elementary cross sections and distortion parameters, whose in-medium validity is untested.
Problem Statement
Determine quantitatively the interior behavior of the Σ⁻-nucleus optical potential — the radial dependence of at radii inside the nuclear surface and the magnitude of its central repulsion, together with the absorptive strength — to the level at which candidate potentials that fit all existing data but differ at the nuclear center (central repulsions of roughly 40 MeV versus roughly 80 MeV) can be distinguished, and validate the result against the full body of Σ⁻ data (atomic X-ray shifts and widths, inclusive (π⁻,K⁺) spectra, ΣN scattering). The problem, as posed by Harada and Hirabayashi (2009), is to reach this determination through observables genuinely sensitive to the nuclear interior: identify and demonstrate observables and measurement strategies that are genuinely sensitive to the interior potential rather than only to its surface tail — such as near-recoilless spectroscopy of Coulomb-assisted bound states on medium-heavy targets (the calculated optimum being Ni at MeV/c) — and establish, by reaction calculations and measurements, that these observables break the degeneracy among the phenomenological potentials; the input elementary amplitudes (Fermi-averaged cross sections) and distortion parameters entering the yield predictions must themselves be validated against data, including possible medium modifications.
A complete answer either (a) states the resulting interior potential and , with quantified uncertainties, such that the magnitude and radial shape of the central repulsion are no longer degenerate among potentials consistent with the existing Σ⁻ atomic, and ΣN data, or (b) demonstrates, by reaction calculations validated against the existing data, that a specified observable and measurement strategy would break that degeneracy — separating the roughly 40 MeV and roughly 80 MeV central-repulsion families, and not merely reproducing the published inclusive discrimination of repulsive from attractive interiors — stating the required measurement precision together with the target and kinematics. A calculation-based demonstration of route (b) suffices; no new measurement is required.
References
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