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Ab initio computations of the fourth-order charge density moments of $^{48}$Ca and $^{208}$Pb

T. Miyagi, M. Heinz, A. Schwenk

TL;DR

We address how high-precision measurements of charge-density moments can inform neutron radii in neutron-rich nuclei. Using ab initio IMSRG calculations with chiral EFT Hamiltonians, the study computes charge form factors for ${}^{48}\mathrm{Ca}$ and ${}^{208}\mathrm{Pb}$ and establishes strong correlations between $R_\mathrm{ch}^4$, $R_\mathrm{ch}^2$, and $R_\mathrm{n}^2$, enabling predictions for $R_\mathrm{ch}^4$ that agree with previous extractions. It finds a comparatively weak connection between $R_\mathrm{ch}^4$ and the neutron skin $R_\mathrm{skin}$, limiting model-independent extraction of skins from $R_\mathrm{ch}^4$ alone, though combined radii constraints and complementary measurements remain informative. The work emphasizes the role of precise $F_\mathrm{ch}(q^2)$ data and Gaussian-process methods for robust moment extraction and provides reference values for upcoming electron-scattering experiments.

Abstract

Neutron skins of neutron-rich nuclei connect nuclei with the matter in neutron stars. High-precision measurements of nuclear charge densities to extract higher-order moments are proposed to be sensitive to neutron radii and skin thicknesses. We investigate the charge density of $^{48}$Ca and $^{208}$Pb, leading candidates for such studies, with ab initio nuclear structure calculations. We find strong correlations between the fourth-order charge density moment $R_\mathrm{ch}^4$ and the charge and neutron radii, allowing us to predict $R_\mathrm{ch}^4$ for $^{48}$Ca and $^{208}$Pb. We find a substantially weaker correlation between the fourth-order charge density moment and the neutron skin, limiting the ability of high-precision electron scattering to determine the neutron skin in a model-independent manner.

Ab initio computations of the fourth-order charge density moments of $^{48}$Ca and $^{208}$Pb

TL;DR

We address how high-precision measurements of charge-density moments can inform neutron radii in neutron-rich nuclei. Using ab initio IMSRG calculations with chiral EFT Hamiltonians, the study computes charge form factors for and and establishes strong correlations between , , and , enabling predictions for that agree with previous extractions. It finds a comparatively weak connection between and the neutron skin , limiting model-independent extraction of skins from alone, though combined radii constraints and complementary measurements remain informative. The work emphasizes the role of precise data and Gaussian-process methods for robust moment extraction and provides reference values for upcoming electron-scattering experiments.

Abstract

Neutron skins of neutron-rich nuclei connect nuclei with the matter in neutron stars. High-precision measurements of nuclear charge densities to extract higher-order moments are proposed to be sensitive to neutron radii and skin thicknesses. We investigate the charge density of Ca and Pb, leading candidates for such studies, with ab initio nuclear structure calculations. We find strong correlations between the fourth-order charge density moment and the charge and neutron radii, allowing us to predict for Ca and Pb. We find a substantially weaker correlation between the fourth-order charge density moment and the neutron skin, limiting the ability of high-precision electron scattering to determine the neutron skin in a model-independent manner.

Paper Structure

This paper contains 7 sections, 5 equations, 3 figures.

Figures (3)

  • Figure 1: Predictions of $R_\mathrm{ch}^2$, $R_\mathrm{ch}^4$, and $R_\mathrm{n}^2$ (for ${}^{48}\mathrm{Ca}$ and ${}^{208}\mathrm{Pb}$ on the left and right, respectively) using the $\Delta\mathrm{NNLO}_\mathrm{GO}$Jiang2020PRC_DN2LOGO and $\mathrm{1.8/2.0}~\mathrm{(EM7.5)}$Arthuis2024arxiv_LowResForces Hamiltonians and the 34 nonimplausible Hamiltonians from Ref. Hu2022NP_Pb208. We show best fit lines to the correlations between $R_\mathrm{ch}^4$, $R_\mathrm{ch}^2$, and $R_\mathrm{n}^2$ for the nonimplausible Hamiltonians, each with a conservative error band. The Pearson correlation coefficient $r$ for each correlation is given in the top left. Using these correlations and experimental determinations of $R_\mathrm{ch}^2$ for ${}^{48}\mathrm{Ca}$Noel2024JHEP_ChargeDensities and ${}^{208}\mathrm{Pb}$Kurasawa2021PTEP_R4Measurement and a theoretical prediction of $R_\mathrm{n}^2$Heinz2024inprep_MuToEResponses, we provide predictions for $R_\mathrm{ch}^4$ of ${}^{48}\mathrm{Ca}$ and ${}^{208}\mathrm{Pb}$.
  • Figure 2: Predictions of $R_\mathrm{skin}$ and $R_\mathrm{ch}^4$ (for ${}^{48}\mathrm{Ca}$ and ${}^{208}\mathrm{Pb}$ on the left and right, respectively) using the $\Delta\mathrm{NNLO}_\mathrm{GO}$Jiang2020PRC_DN2LOGO and $\mathrm{1.8/2.0}~\mathrm{(EM7.5)}$Arthuis2024arxiv_LowResForces Hamiltonians and the 34 nonimplausible Hamiltonians from Ref. Hu2022NP_Pb208. We compare with our determinations of $R_\mathrm{ch}^4$ from Fig. \ref{['fig:rch4_correlation']}, which are based on experimental $R_\mathrm{ch}^2$ measurements Kurasawa2021PTEP_R4MeasurementNoel2024JHEP_ChargeDensities and a theoretical $R_\mathrm{n}^2$ prediction for ${}^{48}\mathrm{Ca}$Heinz2024inprep_MuToEResponses. We also compare with literature values for $R_\mathrm{skin}$ (above), from parity-violating electron scattering (CREX/PREX, black) Adhikari2021Adhikari2022, electric dipole responses (Birkhan et al./Tamii et al., pink) Tamii2011PRLBirkhan2017PRL, hadronic probes (Kłos et al, Zenihiro et al., red) Klos2007Zenihiro2010, ab initio predictions (Hagen et al., brown; Hu et al., orange; Heinz et al., purple) Hagen2016NP_Ca48SkinHu2022NP_Pb208Heinz2024inprep_MuToEResponses, nonrelativistic density-functional theory (DFT) predictions using the SV-min functional (Reinhard et al., olive) Reinhard2021PRLReinhard2022PRL, and inferences from experimental data based on relativistic and nonrelativistic DFT correlations (Kurasawa et al., light and dark gray, respectively) Kurasawa2021PTEP_R4Measurement.
  • Figure 3: Point-proton form factor (left), point-proton mean-squared radius $R_\mathrm{p}^2$ (middle), and fourth-order moment of point-proton density distribution $R_\mathrm{p}^4$ (right) for $^{3}$He. In the left panel, the form factor and its first and second derivatives are shown. The circles are points used to train the GP, whose 95% confidence intervals are given by shaded areas. The dashed curves are computed with cubic spline interpolation. In the middle panel, $R_\mathrm{p}^2$ are computed with the GPs trained with the $n$ lowest $q^{2}$ points, and the $68\%$ and $95\%$ confidence intervals are given by the bars. The solid, dashed, and dotted lines are computed with the $R_\mathrm{p}^2$ operator, slope of the spline interpolation, and the radial integral of the density obtained with the spline interpolation, respectively. The right panel is the same except for $R_\mathrm{p}^4$.