Pith. sign in

REVIEW 4 major objections 5 minor 60 references

Neutron skin thickness for $^{nat}$Pb, $^{159}$Tb and effects of deformation on matter radii for Mg, Na, Ar isotopes

T0 review · 4 major / 5 minor · reviewed 2026-08-15 · deepseek-v4-flash

Pith's one-line read Proton reaction cross sections, reanalysed with a density-scaling folding model, place natural lead's neutron skin at 0.271±0.008 fm and separate deformed from spherical matter radii.

desk verdict The deformation analysis is worth publishing, but the natPb skin claim's 0.008 fm precision rests on an unverified A=208 assumption that the paper itself hedges. read the letter →

arxiv 2506.18936 v1 pith:YPUDDNSQ submitted 2025-06-22 nucl-ex nucl-th

classification nucl-exnucl-th
keywords neutronskinthicknessreactioncrosssectioninteractionfoldingmodelnucleardeformationmatterradiusdensityscaling159Tb
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

The paper asks whether proton reaction cross sections alone can pin down the neutron skin of heavy nuclei, and what exactly the two standard cross-section observables measure. Using the chiral (Kyushu) $g$-matrix folding model with a density-scaling procedure, it extracts $r_{\rm skin}=0.271\pm0.008$ fm for natural lead (treating natPb as $A=208$), consistent with the PREX-II value for ${}^{208}$Pb, and $r_{\rm skin}=0.273\pm0.073$ fm for ${}^{159}$Tb. For Mg, Na, and Ar isotopes, it shows that matter radii extracted from interaction cross sections $\sigma_{\rm I}$ are spherical-limit values, while those from reaction cross sections $\sigma_{\rm R}$ include deformation effects. The result matters because a scattering-based measurement can match parity-violating electron-scattering precision, and because radius tables that mix the two cross-section types conflate deformed and spherical ground-state information.

What carries the argument

The load-bearing mechanism is the density-scaling procedure combined with a folding potential. Given a target density from D1S-GHFB+AMP or SLy7, the model scales the neutron (and sometimes proton) density radially via $\rho_{\rm scaling}(r)=\rho(r/\alpha)/\alpha^3$ so that the folded potential reproduces the measured $\sigma_{\rm R}$ while the proton radius is fixed to the electron-scattering value $r_p$; the scaled neutron radius then defines $r_{\rm skin}$. Two interactions supply the folded potential: the chiral (Kyushu) $g$-matrix for projectile energies up to about 450 MeV, and the Love-Franey $t$-matrix above that, with an ESP-f fine-tuning factor to remove systematic normalization. This combination is what converts a one-dimensional cross-section measurement into a radius difference at a precision of about 0.01 fm.

What would settle it

Measure reaction cross sections for p+${}^{206}$Pb and p+${}^{207}$Pb separately and extract each skin with the same folding model; if the two values differ by more than about 0.02 fm, the constant-skin prediction fails and the reported 0.271 fm for natural lead cannot be taken at face value. A parity-violating electron-scattering run on natural lead analysed with the full isotopic composition would settle the same question directly.

Watch

Extended reading notes

Core claim

On its own terms, the paper's central claim is that the density-scaling folding model can turn existing proton reaction cross sections into neutron-skin values with a 0.008 fm uncertainty for natural lead once natural lead is approximated as $A=208$, and the extracted $0.271\pm0.008$ fm agrees with the PREX-II value $0.283\pm0.071$ fm for ${}^{208}$Pb. The same framework yields $r_{\rm skin}=0.273\pm0.073$ fm for the deformed nucleus ${}^{159}$Tb, and shows that for Mg, Na, and Ar isotopes the matter radius determined from interaction cross sections lies close to the spherical-limit radius, while the reaction-cross-section radius sits at the deformed value. The ${}^{24}$Mg case is analysed quantitatively: the 0.087 fractional gap between $\sigma_{\rm R}$ and $\sigma_{\rm I}$ is only 0.037 from deformation alone, so part of the published $r_{\rm m}(\sigma_{\rm I})$ appears to be a fluctuation.

Load-bearing premise

The natural-lead extraction treats natural lead as pure ${}^{208}$Pb, relying on the prediction that lead neutron skins are nearly constant across mass number; if that constancy fails, the quoted $r_{\rm skin}$ is not a well-defined natural-lead value.

Editorial extensions

If this is right

  • Natural lead has a neutron skin of $0.271\pm0.008$ fm, consistent with PREX-II's $0.283\pm0.071$ fm for ${}^{208}$Pb.
  • The skin of ${}^{159}$Tb is $0.273\pm0.073$ fm; subtracting the deformation effect ($\beta_2=0.309$) leaves a spherical-limit skin near 0.11 fm.
  • For Mg isotopes, 21,23Na, and 40Ar, matter radii from reaction cross sections include deformation, while those from interaction cross sections give the spherical-limit radius.
  • For ${}^{24}$Mg, the difference between $r_{\rm m}(\sigma_{\rm R})=3.03\pm0.08$ fm and $r_{\rm m}(\sigma_{\rm I})=2.79\pm0.15$ fm is only about 40% accounted for by deformation, implying part of the published interaction-cross-section value is a statistical fluctuation.
  • The folding model with ESP-f scaling can extract neutron skins from proton reaction cross sections at a precision comparable to parity-violating electron scattering.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • A corollary the paper leaves implicit: if lead skins are really $A$-independent, the same analysis applied to p+${}^{206}$Pb and p+${}^{207}$Pb data should return skins within about 0.02 fm of ${}^{208}$Pb; this is checkable with existing data and no new theory.
  • The difference between $\sigma_{\rm R}$- and $\sigma_{\rm I}$-based radii could serve as a deformation diagnostic for any nucleus with both measurements, converting the fractional cross-section excess into an effective $\beta_2$ and cross-checking the empirical formula beyond Mg, Na, and Ar.
  • Radius compilations that merge interaction and reaction cross-section values into one matter radius mix spherical and deformed states; future tables should report the observable or apply a deformation correction.
Share X Bluesky LinkedIn Reddit HN

Signed reviews

No signed human review yet.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Referee Report

4 major / 5 minor

Summary. The manuscript uses the chiral (Kyushu) g-matrix folding model and the Love-Franey (LF) t-matrix folding model, together with density scaling, to extract neutron skin thicknesses for natPb and 159Tb, and matter radii for Mg, Na, and Ar isotopes. For natPb the target is treated as pure 208Pb and the extracted r_skin=0.271±0.008 fm is presented as agreeing with the PREX-II value for 208Pb. For 159Tb, r_skin=0.273±0.073 fm is obtained. For 24Mg, the paper compares r_m(σ_R)=3.03±0.08 fm with r_m(σ_I)=2.79±0.15 fm and interprets the difference as evidence that σ_I-based radii give spherical-limit matter radii while σ_R-based radii include deformation; the same interpretation is applied to Na and Ar isotopic chains. A fine-tuning factor F=0.955, calibrated to the 24Mg σ_I datum, is used for the high-energy LF extractions for Na and Ar.

Significance. If the central claims held at their quoted precision, the paper would show that proton reaction cross sections can determine neutron skins of heavy nuclei to 0.008 fm, and that the comparison of σ_R and σ_I data can separate deformation effects from spherical-limit matter radii. The model machinery is not new: the Kyushu g-matrix folding model has been benchmarked in prior work on 12C, Ca, Sn, and Pb, and the D1S-GHFB+AMP and SLy7 densities are standard. The manuscript is also transparent about several of its own limitations, including the statement in Sec. IV that 'Prediction A may be true' and the observation in Sec. III.E that the 37,38Ar depression may be a data fluctuation. However, the headline natPb precision is conditional on an untested assumption about the constancy of Pb skins across A, the Na/Ar extractions are calibrated to a single 24Mg anchor point, and the 24Mg 'too small' conclusion is a sub-sigma statement. These issues substantially limit the significance of the results as currently presented.

major comments (4)
  1. [Sec. III.A / Table III / Sec. II.D] The quoted r_skin=0.271±0.008 fm for natPb treats natural lead as a pure 208Pb target, and the 0.008 fm is the scaling-fit error only. Natural lead is 54.4% 208Pb, 22.1% 207Pb, 22.1% 206Pb, and 1.4% 204Pb. The only support for the A=208 assumption is the prediction that Pb skins are almost constant as a function of A, but no calculation or measured constraint for 204,206,207Pb is shown, and the Sn evidence in Fig. 1 has 30% experimental uncertainties and a 50% model spread from A=118 to 124. If the true Pb skins vary by even ~0.02 fm across A, the abundance-weighted σ_R would differ from the pure-208 calculation and the fitted r_skin would shift by more than the quoted 0.008 fm. The authors should either demonstrate the constancy of Pb skins, model natPb as a composition average, or add a systematic uncertainty that covers the composition ambiguity. As written, the abstract's precision claim is not supported.
  2. [Sec. III.D / Sec. III.E] The fine-tuning factor F=0.955 is fixed by requiring the LF t-matrix folding model to reproduce the central value of r_m(σ_I)=2.79±0.15 fm for 24Mg, and this same F is then applied to all Na isotopes (Sec. III.D) and all 32-40Ar isotopes (Sec. III.E). Consequently the r_m(σ_I) values in Tables VI and VIII are calibrated to the 24Mg input rather than being independent extractions. The uncertainty of the 24Mg anchor (0.15 fm) is not propagated into the quoted errors of the Na and Ar radii, and no validation of F on a system where both σ_I and σ_R are available is given. The deformation conclusions for Na and Ar therefore rest on a single calibration point; please propagate the F uncertainty or provide an independent check.
  3. [Sec. III.C / Abstract] The abstract states that for 24Mg, r_m(σ_I)=2.79±0.15 fm does not include effects of deformation, and Sec. III.C concludes that the central value of r_m(σ_I) is 'too small' compared with r_m,0(P)=2.929 fm. The difference is 0.14 fm against a 1σ error of 0.15 fm, i.e., less than a one-sigma deviation. The wording overstates the strength of the evidence; a quantitative significance statement or a softened conclusion is needed.
  4. [Sec. III.A / Sec. I] The natPb fit includes σ_R data at E_lab=341 MeV, but the Kyushu g-matrix folding model is stated in Sec. I to be benchmarked for proton scattering in the range 20≤E_lab≤180 MeV (Ref. [29]). The extension to 341 MeV is justified only by a general statement about cutoff effects and by 12C+12C tests, not by a proton-scattering benchmark in this energy range. A model-uncertainty contribution from this energy extrapolation should be included in the quoted 0.008 fm error or the fit should be repeated with the high-energy points excluded to show robustness.
minor comments (5)
  1. [Sec. IV, Eq. (34)] Equation (34) as printed, r_m^2 = r_m,0^2[1+5β2^2/(4π)] = r_m,0^2, is internally inconsistent for β2≠0; please correct the intended relation and recompute the derived r_m,0=5.065 fm if needed.
  2. [Table VI, A=26 row] The entry '0075' should read '0.075'.
  3. [Table VIII / Figs. 11-12] The table heading uses r_skin while Figs. 11 and 12 use r_skin.p for the same quantity; please make the notation consistent.
  4. [Sec. III.C, Eq. (33)] The expression for σ_inel in Eq. (33) does not obviously follow from Eqs. (29)-(32) with the stated definitions of r_m(P), r_m,0(P), x, and c; please check the algebra and correct or clarify.
  5. [Table II] Table II lists r_m(σ_R)=2.352±0.013 fm for 12C, while Sec. II.C and Sec. III.C use r_m(12C)=2.338 fm from Ref. [55]; please clarify which value is used in the double-folding calculations and why the values differ.

Circularity Check

0 steps flagged · score 0.0 of 10

No significant circularity: the extracted radii are outputs of an inverse folding-model fit, not inputs renamed as predictions.

full rationale

The paper's derivation chain is not circular. For natPb, 159Tb, Na, Mg, and Ar, the reported radii are obtained by the scaling procedure of Eq. (27): given input densities (D1S-GHFB+AMP, SLy7, or a density scaled to r_n(PREX-II)), the folding model cross sections are computed and the densities are scaled until sigma_R or sigma_I matches the measured data. The radii are therefore outputs of the fit, not quantities already present in the inputs. The fine-tuning factor F is admittedly fitted to the central value of r_m(sigma_I)=2.79+/-0.15 fm for 24Mg, and f is fitted to the average sigma_R(exp)/sigma_R(th) for p+40Ar; but these are openly introduced normalization constants, and the per-nucleus radii are subsequently determined from each nucleus's own cross-section data by the same scaling procedure. The reported consistency with Suzuki and Ozawa radii is a comparison of independently extracted values, not an identity forced by construction. For natPb, the analysis assumes A=208 and starts from the PREX-II neutron density, but the final r_skin=0.271+/-0.008 fm is a small shift away from the PREX-II input, and the data could have required a larger shift; thus the agreement with PREX-II is not an input-output tautology. The genuinely load-bearing but unverified element is 'Prediction A' that Pb skins are almost constant across A, which the paper itself hedges in the Summary as 'Prediction A may be true'; that is a composition-modeling assumption and a systematic-risk caveat, not a circular reduction of the result to its own inputs. No fitted parameter is renamed as a prediction, and no self-citation or uniqueness theorem forces the central claims.

Assumptions & free parameters 3 free parameters · 5 assumptions · 0 invented entities

The central extraction depends on the folding model's validity, the density shapes from D1S-GHFB+AMP or SLy7, the one-parameter density scaling, and the calibration factors F and f. No new entities are introduced. The A=208 treatment of natPb is an ad hoc assumption.

free parameters (3)
  • Fine-tuning factor F for LF t-matrix model = 0.955
    Determined so the LF folding model reproduces r_m(sigma_I)=2.79±0.15 fm for 24Mg+12C from Suzuki et al. (Sec. III.D). Used for all Na and Ar sigma_I analyses.
  • Fine-tuning factor f (ESP-f) for p+40Ar = 1.0327
    Chosen by averaging sigma_R(exp)/sigma_R(th) over E_lab to scale p+40Ar cross sections (Sec. III.F). Calibrates model to the data it then extracts radii from.
  • Per-nucleus density scaling factor alpha = e.g., alpha_n=0.986 for natPb
    Eq. (27) scales proton/neutron densities to reproduce sigma_R(exp); the scaled radius is then reported as the extracted value.
assumptions (5)
  • domain assumption The Kyushu chiral g-matrix folding model gives a valid optical potential for proton-nucleus scattering between 20 and 450 MeV.
    Assumed throughout Sec. II.B and III.A/B; supported by the authors' prior tests, not by derivations in this paper.
  • standard math The Brieva-Rook localization of the exchange potential is accurate.
    Invoked in Sec. II.B (Eq. 8 and the sentence 'It can be localized with the Brieva-Rook approximation'); justified by Ref. [53].
  • ad hoc to paper Scaling a density by a single factor alpha preserves the true shape of the ground-state density.
    This is the core extraction assumption behind Eq. (27); no justification is given that halo or deformation-tail shapes are correctly captured by isotropic scaling.
  • domain assumption For high-energy scattering, sigma_I(exp) can be computed as sigma_R in the folding model.
    Assumed in Sec. II.C ('Glauber-model calculations regard sigma_R as sigma_I... We take the same assumption').
  • ad hoc to paper A=208 for natPb; skin values of 204,206,207,208Pb are nearly identical.
    Stated in Sec. II.D and Sec. III.A; supports the natPb-PREX-II comparison and is the weakest assumption.

how reviews work

0 comments
Cite this review

Pith. "Pith review of Neutron skin thickness for $^{nat}$Pb, $^{159}$Tb and effects of deformation on matter radii for Mg, Na, Ar isotopes." pith.science (2026). https://pith.science/paper/YPUDDNSQ

@misc{pith2026250618936,
  author       = {Pith},
  title        = {Pith review of: Neutron skin thickness for $^nat$Pb, $^159$Tb and effects of deformation on matter radii for Mg, Na, Ar isotopes},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/YPUDDNSQ}},
  note         = {Machine review of arXiv:2506.18936}
}
abstract

Data on reaction cross section $\sigma_{\rm R}$ of proton scattering are available for $^{nat}$Pb (natural lead) and $^{159}$Tb. In addition, data on $\sigma_{\rm R}$ and/or interaction ones $\sigma_{\rm I}$ are available for Mg, Na, Ar isotopes. Our aim is to determine neutron skin thickness $r_{\rm skin}$ for $^{nat}$Pb, $^{159}$Tb and to investigate effects of deformation for Mg, Na, Ar isotopes. We use the chiral (Kyushu) $g$-matrix folding model for lower energies and the folding model based on the Love-Franey (LF) $t$-matrix for higher energies. For $^{159}$Tb, our skin value is $r_{\rm skin}=0.273 \pm 0.073$~fm. As for $^{24}$Mg, our matter radius $r_{\rm m}(\sigma_{\rm R})=3.03 \pm 0.08$~fm determined from $\sigma_{\rm R}$ includes effects of deformation, whereas the corresponding $r_{\rm m}(\sigma_{\rm I})=2.79 \pm 0.15$~fm does not. Effects of deformation are seen for Mg isotopes, $^{21, 23}$Na, $^{40}$Ar. Our result $r_{\rm skin}=0.271 \pm 0.008$~fm for $^{nat}$Pb agrees with $r_{\rm skin}^{208}({\rm PREX\text{-}II}) = 0.283\pm 0.071$~fm for $^{208}$Pb, where we assume $A=208$ for $^{nat}$Pb.

Figures

Figures reproduced from arXiv: 2506.18936 by the authors.

Figure 1
Figure 1. FIG. 1. Skin values of [PITH_FULL_IMAGE:figures/full_fig_p002_1.png] view at source ↗
Figure 2
Figure 2. FIG. 2. 3NFs in NNLO. Diagram (a) corresponds to the Fujita [PITH_FULL_IMAGE:figures/full_fig_p003_2.png] view at source ↗
Figure 5
Figure 5. This is investigated with D1S-GHFB+AMP and [PITH_FULL_IMAGE:figures/full_fig_p003_5.png] view at source ↗
Figures from the paper (9 more)
Figure 3
Figure 3. Figure 3: shows Elab dependence of σR for p+natPb scat￾tering in Elab = 21.1 ∼ 341 MeV. We assume A = 208 for natPb. The σR(PREX-II) are calculated with the Kyush g-matrix folding model with the D1S-GHFB+AMP neu￾tron density scaled to r 208 n (PREX-II), where r 208 p (D1S) = r 2…
Figure 5
Figure 5. Figure 5: FIG. 5 [PITH_FULL_IMAGE:figures/full_fig_p007_5.png]
Figure 7
Figure 7. Figure 7: show our rm(σI), the rm(σSuzuki) of Refs. [18, 22], the rm(SLy7) for Na isotopes as a function of A. Our rm(σI) are consistent with the rm(σSuzuki). The rm(SLy7) are parallel to our rm(σI) and have natural A dependence, i.e., rm(SLy7) = 1.1263A1/3 − 0.3243 with good ac…
Figure 8
Figure 8. Figure 8: FIG. 8 [PITH_FULL_IMAGE:figures/full_fig_p009_8.png]
Figure 9
Figure 9. Figure 9: shows σI as a function of A. The LF t-matrix fold￾ing model with the SLy7 densities overestimates the data [23]. The F σI(LF) monotonically increase as a function of A, whereas the data [23] have a depression in 37,38Ar. The de￾pression in 37,38Ar may be a fluctuation …
Figure 10
Figure 10. Figure 10: FIG. 10 [PITH_FULL_IMAGE:figures/full_fig_p010_10.png]
Figure 11
Figure 11. Figure 11: shows our results on proton skin thickness rskin.p for 32–40Ar. There is a bump at A = 37, 38. This is related to the fact that the central values of σI(exp) are slightly smaller than those of the neighborhood nuclei. If we take the upper￾bound values of the data σI(e…
Figure 13
Figure 13. Figure 13: FIG. 13 [PITH_FULL_IMAGE:figures/full_fig_p011_13.png]
Figure 15
Figure 15. Figure 15: We find that effects of deformation on rn are not negligible. 2.4 2.6 2.8 3.0 3.2 3.4 18 20 22 24 26 28 30 32 34 Na rn (σI ) rn (σR ) rp (exp) rn (σI), rn (σ R), rp(exp) [fm] mass number A FIG. 15. A dependence of the rn(σI), the rn(σR), the rp(exp) for Na isotopes. S…

Discussion (0). Continue with ORCID to comment.

Reference graph

Works this paper leans on

60 extracted references · 42 canonical work pages

  1. [29]

    Tagami, T

    S. Tagami, T. Wakasa, and M. Yahiro,12C+12C scattering as the reference system for reaction cross section, Results in Physics 51, 106675 (2023)

  2. [1]

    We assume A= 208for natPb

    p+natPb scattering:We extractr skin andr m(σR)from dataσ R [10–16] inE lab = 21.1∼341MeV , us- ing the Kyushug-matrix folding model with the D1S- GHFB+AMP proton and neutron densities. We assume A= 208for natPb

  3. [2]

    p+159Tb scattering:We extractr skin andr m(σR)from dataσ R [17] in20≤E lab ≤47.5MeV , using the Kyushug-matrix folding model with the D1S-GHFB densities. 3-1) 20-−32Na+12C scattering:We determiner m(σI)for 20-−32Na on the dataσ I [18, 19] at 950 MeV/u, using the LFt-matrix folding model with the Sly7 densities, where SLy7 [36–38] is an improved version of...

  4. [3]

    Adhikari et al

    D. Adhikari et al. (CREX), Precision Determination of the Neu- tral Weak Form Factor of 48Ca, Phys. Rev. Lett.129, 042501 (2022), arXiv:2205.11593 [nucl-ex]

  5. [4]

    Kyushug-matrix

    Comparison betweenr m(σR)andr m(σI)for Mg isotopes: We analyzed 24-38Mg+12C scattering at 240 MeV/u and determined ther m(σR)for 24-38Mg [25]. Meanwhile, Suzukiet al.measuredσ I for 20,22,23,27,29–32Mg+ 12C scattering at 950 MeV/u [18, 19] and determined matter radiir m(σI)[19]. We find that ther m(σI)of Ref. [19] yield do not include effects of deformati...

  6. [5]

    C. J. Horowitz, S. J. Pollock, P. A. Souder, and R. Michaels, Parity violating measurements of neutron densities, Phys. Rev. C63, 025501 (2001)

  7. [6]

    Adhikari et al

    D. Adhikari et al. (PREX), Accurate Determination of the Neutron Skin Thickness of 208Pb through Parity-Violation in Electron Scattering, Phys. Rev. Lett.126, 172502 (2021), arXiv:2102.10767 [nucl-ex]

  8. [7]

    B. A. Brown, Constraints on the Skyrme Equations of State from Properties of Doubly Magic Nuclei, Phys. Rev. Lett.111, 232502 (2013), arXiv:1308.3664 [nucl-th]

Show all 60 references
  1. [8]

    Angeli and K

    I. Angeli and K. P. Marinova, Table of experimental nuclear ground state charge radii: An update, Atom. Data Nucl. Data Tabl.99, 69 (2013)

  2. [9]

    Tagami, T

    S. Tagami, T. Wakasa, J. Matsui, M. Yahiro, and M. Takechi, Neutron skin thickness of Pb208 determined from the reaction cross section for proton scattering, Phys. Rev. C104, 024606 (2021), arXiv:2010.02450 [nucl-th]

  3. [10]

    Toyokawa, M

    M. Toyokawa, M. Yahiro, T. Matsumoto, and M. Kohno, Effects of chiral three-nucleon forces on 4He-nucleus scattering in a wide range of incident energies, PTEP2018, 023D03 (2018), arXiv:1712.07033 [nucl-th]

  4. [12]

    Tagami, T

    S. Tagami, T. Wakasa, and M. Yahiro, Neutron skin thickness of 116,118,120,122,124Sn determined from reaction cross sections of proton scattering, Results in Physics46, 106296 (2023)

  5. [13]

    F. S. Dietrich et al., Proton Reaction Cross Sections Measured in the BNL/AGS E943 Experiment, J. Nucl. Sci. Tech.39, 269 (2002)

  6. [14]

    Renberg, D

    P. Renberg, D. Measday, M. Pepin, P. Schwaller, B. Favier, and C. Richard-Serre, Reaction cross sections for protons, Nuclear Physics A183, 81 (1972)

  7. [15]

    J. M. Cassels and J. D. Lawson, Absorption cross sections for 134 mev protons, Proceedings of the Physical Society. Section A67, 125 (1954)

  8. [16]

    Kirkby and W

    P. Kirkby and W. T. Link, Canadian Journal of Physics44, 1847 (1966), https://doi.org/10.1139/p66-155

  9. [17]

    Goloskie and K

    R. Goloskie and K. Strauch, Measurement of proton inelastic cross sections, Nuclear Physics29, 474 (1962)

  10. [18]

    Meyer, R

    V . Meyer, R. M. Eisberg, and R. F. Carlson, Total reaction cross sections of several nuclei for protons, Phys. Rev.117, 1334 (1960)

  11. [19]

    Gooding, Proton total reaction cross sections at 34 mev, Nu- clear Physics12, 241 (1959)

    T. Gooding, Proton total reaction cross sections at 34 mev, Nu- clear Physics12, 241 (1959)

  12. [20]

    Abegg, J

    R. Abegg, J. Birchall, N. Davison, M. de Jong, D. Ginther, D. Hasell, T. Nasr, W. van Oers, R. Carlson, and A. Cox, Mea- surement of the proton total reaction cross section for 159Tb, 181Ta and 197Au between 20 and 48 Mev, Nuclear Physics A 324, 109 (1979)

  13. [21]

    Suzuki et al., Neutron skin of Na isotopes studied via the interaction cross-sections, Phys

    T. Suzuki et al., Neutron skin of Na isotopes studied via the interaction cross-sections, Phys. Rev. Lett.75, 3241 (1995)

  14. [22]

    Suzuki et al., Nuclear radii of Na and Mg isotopes, Nucl

    T. Suzuki et al., Nuclear radii of Na and Mg isotopes, Nucl. Phys. A630, 661 (1998)

  15. [23]

    Huber et al., Spins, magnetic moments, and isotope shifts of Na-21-31 by high resolution laser spectroscopy of the atomic D-1 line, Phys

    G. Huber et al., Spins, magnetic moments, and isotope shifts of Na-21-31 by high resolution laser spectroscopy of the atomic D-1 line, Phys. Rev. C18, 2342 (1978), [Erratum: Phys.Rev.C 20, 2457–2457 (1979)]

  16. [24]

    Zhang, W

    H. Zhang, W. Shen, Z. Ren, Y . Ma, W. Jiang, Z. Zhu, X. Cai, D. Fang, C. Zhong, L. Yu, Y . Wei, W. Zhan, Z. Guo, G. Xiao, J. Wang, J. Wang, Q. Wang, J. Li, M. Wang, and Z. Chen, Mea- surement of reaction cross section for proton-rich nuclei (a¡30) at intermediate energies, Nuc...

  17. [25]

    Ozawa, T

    A. Ozawa, T. Suzuki, and I. Tanihata, Nuclear size and related topics, Nucl. Phys. A693, 32 (2001)

  18. [26]

    Ozawa et al., Measurements of the interaction cross sections for Ar and Cl isotopes, Nucl

    A. Ozawa et al., Measurements of the interaction cross sections for Ar and Cl isotopes, Nucl. Phys. A709, 60 (2002), [Erratum: Nucl.Phys.A 727, 465–466 (2003)]

  19. [27]

    Takechi, S

    M. Takechi, S. Suzuki, D. Nishimura, M. Fukuda, T. Oht- subo, M. Nagashima, T. Suzuki, T. Yamaguchi, A. Ozawa, T. Moriguchi, H. Ohishi, T. Sumikama, H. Geissel, N. Aoi, R.- J. Chen, D.-Q. Fang, N. Fukuda, S. Fukuoka, H. Furuki, N. In- abe, Y . Ishibashi, T. Itoh, T. Izumikawa,...

  20. [28]

    Watanabe et al., Ground-state properties of neutron-rich Mg isotopes, Phys

    S. Watanabe et al., Ground-state properties of neutron-rich Mg isotopes, Phys. Rev. C89, 044610 (2014), arXiv:1404.2373 [nucl-th]

  21. [30]

    Wakasa, M

    T. Wakasa, M. Takechi, S. Tagami, and M. Yahiro, Matter radii and skins of 6,8He from reaction cross section of proton+6,8He scattering based on the love–franey t-matrix model, Results in Physics35, 105329 (2022)

  22. [31]

    Takechi, M

    M. Takechi, M. Fukuda, M. Mihara, K. Tanaka, T. Chinda, T. Matsumasa, M. Nishimoto, R. Matsumiya, Y . Nakashima, H. Matsubara, K. Matsuta, T. Minamisono, T. Ohtsubo, T. Izu- mikawa, S. Momota, T. Suzuki, T. Yamaguchi, R. Koyama, W. Shinozaki, M. Takahashi, A. Takizawa, T. Mats...

  23. [32]

    Wakasa, S

    T. Wakasa, S. Tagami, J. Matsui, M. Takechi, and M. Yahiro, Neutron-skin values and matter and neutron radii determined from reaction cross sections of proton scattering, Phys. Rev. C 107, 024608 (2023), arXiv:2211.16688 [nucl-th]

  24. [33]

    W. G. Love and M. A. Franey, Phys. Rev. C24, 1073 (1981)

  25. [34]

    Takechi, T

    M. Takechi, T. Ohtsubo, M. Fukuda, D. Nishimura, T. Kuboki, T. Suzuki, T. Yamaguchi, A. Ozawa, T. Moriguchi, H. Ooishi, D. Nagae, H. Suzuki, S. Suzuki, T. Izumikawa, T. Sumikama, M. Ishihara, H. Geissel, N. Aoi, R.-J. Chen, D.-Q. Fang, N. Fukuda, I. Hachiuma, N. Inabe, Y . Ish...

  26. [35]

    Minomo, T

    K. Minomo, T. Sumi, M. Kimura, K. Ogata, Y . R. Shimizu, and M. Yahiro, Determination of the structure of 31Neby a fully microscopic framework, Phys. Rev. Lett.108, 052503 (2012)

  27. [36]

    T. Sumi, K. Minomo, S. Tagami, M. Kimura, T. Matsumoto, K. Ogata, Y . R. Shimizu, and M. Yahiro, Deformation of ne isotopes in the region of the island of inversion, Phys. Rev. C 85, 064613 (2012)

  28. [37]

    Tanaka et al., Swelling of Doubly Magic 48Ca Core in Ca Isotopes beyondN= 28, Phys

    M. Tanaka et al., Swelling of Doubly Magic 48Ca Core in Ca Isotopes beyondN= 28, Phys. Rev. Lett.124, 102501 (2020), arXiv:1911.05262 [nucl-ex]

  29. [38]

    Takechi, T

    M. Takechi, T. Wakasa, S. Tagami, J. Matsui, and M. Yahiro, Reanalyzes for 42–51Ca scattering on a 12C target at 280 mev/nucleon based on chiral g folding mode with gogny- d1s hartree–fock–bogoliubov densities, Results in Physics31, 104923 (2021)

  30. [39]

    Chabanat, P

    E. Chabanat, P. Bonche, P. Haensel, J. Meyer, and R. Schaef- fer, A Skyrme parametrization from subnuclear to neutron star densities. 2. Nuclei far from stablities, Nucl. Phys. A635, 231 (1998), [Erratum: Nucl.Phys.A 643, 441–441 (1998)]

  31. [40]

    Schunck et al., Solution of the Skyrme- Hartree–Fock–Bogolyubovequations in the Cartesian deformed harmonic-oscillator basis

    N. Schunck et al., Solution of the Skyrme- Hartree–Fock–Bogolyubovequations in the Cartesian deformed harmonic-oscillator basis. (VIII) hfodd (v2.73y): A new version of the program, Comput. Phys. Commun.216, 145 (2017), arXiv:1612.05314 [nucl-th]

  32. [41]

    Matsuzaki, S

    M. Matsuzaki, S. Tagami, and M. Yahiro, Neutron skin thick- ness of 208Pb,116,120,124 Sn, and 40Ca determined from reac- tion cross sections of 4He scattering, Phys. Rev. C104, 054613 (2021), arXiv:2107.06441 [nucl-th]

  33. [42]

    Carlson, A

    R. Carlson, A. Cox, T. Nasr, M. De Jong, D. Ginther, D. Hasell, A. Sourkes, W. van Oers, and D. Margaziotis, Measurements of proton total reaction cross sections, Nuclear Physics A445, 57 (1985)

  34. [43]

    F. A. . Brieva and J. Rook, Nucl. Phys.A291, 299 (1977)

  35. [44]

    K. Amos, P. J. Dortmans, H. V . von Geramb, S. Karataglidis, and J. Raynal, Advances in Nuclear Physics, edited by J. W. Negele and E. V ogt, V ol. 25 (Plenum, New York, 2000) p. 275

  36. [45]

    Furumoto, Y

    T. Furumoto, Y . Sakuragi, and Y . Yamamoto, Phys. Rev. C78, 044610 (2008)

  37. [46]

    T. Sumi, K. Minomo, S. Tagami, M. Kimura, T. Matsumoto, K. Ogata, Y . R. Shimizu, and M. Yahiro, Deformation of Ne iso- topes in the island-of-inversion region, Phys. Rev. C85, 064613 (2012), arXiv:1201.2497 [nucl-th]

  38. [47]

    Toyokawa, K

    M. Toyokawa, K. Minomo, and M. Yahiro, Mass-number and isotope dependence of local microscopic optical potentials for polarized proton scattering, Phys. Rev. C88, 054602 (2013)

  39. [48]

    Egashira, K

    K. Egashira, K. Minomo, M. Toyokawa, T. Matsumoto, and M. Yahiro, Microscopic optical potentials for 4He scattering, Phys. Rev. C89, 064611 (2014), arXiv:1404.2735 [nucl-th]

  40. [49]

    Toyokawa, K

    M. Toyokawa, K. Minomo, M. Kohno, and M. Yahiro, Roles of chiral three-nucleon forces in nucleon–nucleus scattering, J. Phys. G42, 025104 (2015), [Erratum: J.Phys.G 44, 079502 (2017)], arXiv:1404.6895 [nucl-th]

  41. [50]

    Toyokawa, M

    M. Toyokawa, M. Yahiro, T. Matsumoto, K. Minomo, K. Ogata, and M. Kohno, Microscopic calculations based on chiral two- and three-nucleon forces for proton- and 4He-nucleus scatter- ing, Phys. Rev. C92, 024618 (2015), [Erratum: Phys.Rev.C 96, 059905 (2017)], arXiv:1507.02807 [nucl-th]

  42. [51]

    G. R. Satchler and W. G. Love, Folding model potentials from realistic interactions for heavy-ion scattering, Phys. Rept.55, 183 (1979)

  43. [52]

    Kohno, Phys

    M. Kohno, Phys. Rev. C88, 064005 (2013)

  44. [53]

    Fujita and H

    J. Fujita and H. Miyazawa, Pion Theory of Three-Body Forces, Prog. Theor. Phys.17, 360 (1957)

  45. [54]

    H. V . von Gerambet al., Phys. Rev. C44, 73 (1991)

  46. [55]

    Amos and P

    K. Amos and P. J. Dortmans, Phys. Rev. C49, 1309 (1994)

  47. [56]

    Minomo, K

    K. Minomo, K. Ogata, M. Kohno, Y . R. Shimizu, and M. Yahiro, The Brieva-Rook Localization of the Microscopic Nucleon-Nucleus Potential, J. Phys. G37, 085011 (2010), arXiv:0911.1184 [nucl-th]

  48. [57]

    Yamaguchi, S

    N. Yamaguchi, S. Nagata, and T. Matsuda, Prog. Theor. Phys. 70, 459 (1983)

  49. [58]

    de Vries, C

    H. de Vries, C. W. de Jager, and C. de Vries, NUCLEAR CHARGE-DENSITY-DISTRIBUTION PARAMETERS, At. Data Nucl. Data Tables36, 495 (1987)

  50. [59]

    Tagami, T

    S. Tagami, T. Myo, and M. Yahiro, Neutron skin thickness of 208Pbfrom total cross sections of neutron scattering at 14.137 mev and neutron skin thickness of 48Ca, o, n, and c isotopes from reaction and interaction cross sections, Phys. Rev. C110, 064610 (2024)

  51. [60]

    Tagami, M

    S. Tagami, M. Tanaka, M. Takechi, M. Fukuda, and M. Yahiro, Chiralg-matrix folding-model approach to reaction cross sec- tions for scattering of Ca isotopes on a C target, Phys. Rev. C 101, 014620 (2020)

Pith tools

Reviewed August 15, 2026 · model on record in the stance chip above.