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Chiral three-nucleon forces for the new local position-space two-nucleon potential in $\textit{ab initio}$ many-body calculations

Nuclear Theory · Submitted 13 Jan 2026 · 70 references

Pith's verdict: A useful but partially circular Hamiltonian parameterization: the radius improvement is real, but the energy agreement is partly fit, not prediction.

T0 · AI review

How this review was made: An AI referee (deepseek-v4-flash) read the paper on August 3, 2026 and answered a fixed list of questions about it. T0 is the starting level every paper gets. The levels describe how deeply Pith has checked the paper, never the authors.

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  4. T3 Formal statement The claims written out in a formal math language a computer can read.
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arXiv ID2601.08199 (version 2)
Pith IDQKYN5IAG, Pith's permanent record of this paper and its review
CitationFurong Xu, Jianguo Li, Rongzhe Hu, Siqin Fan. "Chiral three-nucleon forces for the new local position-space two-nucleon potential in $\textit{ab initio}$ many-body calculations." arXiv:2601.08199 (2026). https://pith.science/paper/QKYN5IAG
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Referee report
The paper

The paper claims

This paper constructs a chiral three-nucleon force with a hybrid local-nonlocal regulator, pairs it with the new local position-space two-nucleon potential, and shows that with only two fitted constants it reproduces ground-state energies a

The reading

The paper aims to resolve a long-standing problem in ab initio nuclear structure: no single chiral Hamiltonian had simultaneously reproduced both binding energies and charge radii across a wide mass range. The authors build a companion three-nucleon force (3NF) for a recently developed local position-space two-nucleon potential, fixing the two 3NF low-energy constants using only the tritium and oxygen-16 ground-state energies. They find that a hybrid local-nonlocal regulator for the 3NF makes the difference: the resulting Hamiltonian describes energies and radii of closed-shell nuclei from 4He to 132Sn within about 2%, and also gives good systematics for several open-shell isotope chains. The purely local 3NF reproduces energies but underestimates radii, so the regulator form is the load-bearing choice. If correct, this yields a single chiral Hamiltonian applicable across the nuclear chart without per-nucleus fitting.

What carries the argument

The key machinery is the hybrid local-nonlocal regulator for the N2LO three-nucleon force, defined as the product of a local regulator suppressing relative-momentum differences and a nonlocal regulator suppressing total Jacobi momenta. This regulator controls how high-momentum components of the interaction are cut off, and the paper demonstrates that this choice, rather than the chiral order alone, determines whether binding energies and radii can be reproduced together. The two accompanying low-energy constants cD and cE are fixed by two uncorrelated observables, the triton and oxygen-16 binding energies, using the similarity renormalization group to evolve the Hamiltonian to a low-momentum

Extended reading notes

Core claim

The central claim is that a N2LO chiral three-nucleon force using a hybrid local-nonlocal regulator, combined with the new local position-space two-nucleon potential, can simultaneously reproduce experimental ground-state energies and charge radii for nuclei spanning 4He to 132Sn. The two 3NF low-energy constants cD and cE are constrained by the ground-state energies of 3H and 16O, and no other nucleus-specific parameters are introduced. With the local-only 3NF regulator, energies come out well but charge radii are systematically too small; switching to the hybrid regulator increases medium-mass radii by about 7% and brings both observables into agreement, with deviations below 2% for all cl

Load-bearing premise

The two three-nucleon constants, fitted only to tritium and oxygen-16, transfer to all other nuclei once the interaction is evolved to low momentum; if they had to be re-fitted per nucleus, the broad agreement across the chart would not follow.

Editorial extensions

If this is right

  • If the claim holds, a single Hamiltonian with only two fitted three-nucleon parameters can predict energies and radii across a wide swath of the nuclear chart, enabling credible ab initio predictions for isotopes not yet measured.
  • The predicted charge density distributions for 16O and 40Ca match electron-scattering data, offering a microscopic account of central nuclear densities that can be tested with further measurements.
  • The success on open-shell isotopic chains means the same interaction can be used with valence-space methods to study mass and radius trends far from stability.
  • The pronounced regulator sensitivity—a 7% shift in radii from local to hybrid—implies that future chiral interactions must treat regulator dependence as a physical observable, not a numerical nuisance.
  • Because only two 3NF constants are fitted to two light-nucleus observables, the agreement in medium-mass nuclei supports the chiral EFT expansion and the chosen power counting for both the 2NF and 3NF.

Reading between the lines

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

  • Beyond the paper, the same two-constant calibration could be tested on infinite nuclear matter saturation properties; the paper does not report this, and a mismatch there would clarify how far the LEC transferability extends.
  • Beyond the paper, a third constraint such as the 4He charge radius could break the residual cD-cE correlation left after the triton fit, potentially sharpening predictions for exotic nuclei where experimental data are sparse.
  • Beyond the paper, the findings suggest that regulator form, rather than chiral order alone, may be the dominant sensitivity for nuclear radii; a systematic comparison at next chiral order could expose whether this sensitivity persists.
  • Beyond the paper, one could test whether the hybrid-regulated 3NF also improves spectroscopic observables such as electromagnetic transitions and beta-decay strengths, since those operators are consistently evolved in the same framework.
Original abstract

Three-nucleon force (3NF) plays an important role in understanding the structure of finite nuclei and the saturation properties of infinite nuclear matter. More specifically, 3NF should be necessary for each two-nucleon force (2NF) to obtain more accurate description of nuclear systems. 3NF derived from the chiral effective field theory has been successful in $\textit{ab initio}$ calculations of atomic nuclei. Most of established chiral nuclear forces have a nonlocal form in the momentum space. In this work, we construct a companion chiral 3NF specifically tailored to the new Idaho local position-space 2NF, and calculate binding energies and radii of nuclei up to $^{132}$Sn. We find that a chiral 3NF with hybrid local and nonlocal regulators has advantages in improving the nuclear structure calculations of both binding energies and radii with the new Idaho 2NF. The two low-energy constants of 3NF are constrained by the ground-state energies of $^3$H and $^{16}$O as suggested in a recent work.

The compiled record

The paper's own sentences, arranged, kept beside the review and separate from it. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 5,075 input tokens.

What the abstract itself states, as probabilities: claims first 0.07 · states limitation 0.14 · human participants 0.01 · controlled comparison 0.10 · randomized assignment 0.01 · states quantitative result 0.16 · compares with prior results 0.36 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v2. Results and the main claim are underlined; .

Three-nucleon force (3NF) plays an important role in understanding the structure of finite nuclei and the saturation properties of infinite nuclear matter. More specifically, 3NF should be necessary for each two-nucleon force (2NF) to obtain more accurate description of nuclear systems. 3NF derived from the chiral effective field theory has been successful in $\textit{ab initio}$ calculations of atomic nuclei. Most of established chiral nuclear forces have a nonlocal form in the momentum space. In this work, we construct a companion chiral 3NF specifically tailored to the new Idaho local position-space 2NF, and calculate binding energies and radii of nuclei up to $^{132}$Sn. We find that a chiral 3NF with hybrid local and nonlocal regulators has advantages in improving the nuclear structure calculations of both binding energies and radii with the new Idaho 2NF. The two low-energy constants of 3NF are constrained by the ground-state energies of $^3$H and $^{16}$O as suggested in a recent work.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 Three-nucleon force (3NF) plays an important role in understanding the structure of finite nuclei and the saturation properties of infinite nuclear matter. background 1.00 0.04 0.03 asserted 1.00
s1 More specifically, 3NF should be necessary for each two-nucleon force (2NF) to obtain more accurate description of nuclear systems. 3NF derived from the chiral effective field theory has been successful in $\textit{ab initio}$ calculations of atomic nuclei. background 1.00 0.06 0.05 asserted 0.69
s2 Most of established chiral nuclear forces have a nonlocal form in the momentum space. background 0.92 0.03 0.02 asserted 1.00
s3 In this work, we construct a companion chiral 3NF specifically tailored to the new Idaho local position-space 2NF, and calculate binding energies and radii of nuclei up to $^{132}$Sn. contribution 0.99 0.97 0.12 asserted 0.99
s4 We find that a chiral 3NF with hybrid local and nonlocal regulators has advantages in improving the nuclear structure calculations of both binding energies and radii with the new Idaho 2NF. result 0.98 0.96 0.82 asserted 1.00
s5 The two low-energy constants of 3NF are constrained by the ground-state energies of $^3$H and $^{16}$O as suggested in a recent work. method 0.99 0.43 0.05 asserted 0.92

What kind of paper the classifier reports this is: method or tool 0.55 · evidence from simulation or computation 1.00.

What was examined, and what was not

sources read
  • arXiv listing abstract v2
not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
levels run
  • P abstract
not run
  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

Figures
Figure 1. Relation between cD and cE obtained by the constraint of the 3H binding energy, for the local and lnl 3NF regulators. Shadows indicate the EFT uncertainty of 300 keV. The blue and red filled dots are the final optimized results by considering the 16O binding energy for 2NF(local)+3NF(local) and 2NF(local)+3NF(lnl), respectively. Nmax = 44 HO shells. The 3H NCSM calculation with such large model space should be considered to be exact, and the many-body uncertainty should be ignored. The dominant un￾certainty should be from the χEFT truncation. Uncertainties caused by χEFT can be…
Figure 2. Ground-state energies of selected medium-mass doubly-closed-shell nuclei, calculated by IMSRG with increasing the cD value in a step of 1.0, starting from cD = −6.0 for the local 3NF regulator (a), and from cD = 2.0 for the lnl regulator (b). The black bars indicate experimental data [48]. Fock ground state as [46, 47] Hˆ =E0 +∑ i j fi j{aˆ † i aˆj}+ 1 2!2 ∑ i jkl Γi jkl{aˆ † i aˆ † j aˆlaˆk} + 1 3!2 ∑ i jklmn Wi jklmn{aˆ † i aˆ † j aˆ † k aˆnaˆmaˆl}, (8) where E0, f , Γ and W represent normal-ordered zero-, one-, two- and three-body terms, respectively. In the IMSRG evolu￾tion,…
Figure 3. Ground-state energies per nucleon and charge radii for selected doubly-closed-shell nuclei from 4He to 132Sn. Experimental data are taken from Refs. [48, 50]. See text for details of the interactions and calculations. to derive valence-space effective operators of other observables. The valence-space Hamiltonian is then diagonalized using the parallel shell model code kshell [55]. In the present VS￾IMSRG calculation, the valence space is defined as follows: p shell with 4He core for 14O; sd shell with 16O core for 17-28O, 20-32Mg, 22-34Si, 28-36S, 32-38Ar and 34-38Ca; proton sd and…
Figure 4. Ground-state energies of O, Mg, Si, S, Ar and Ca isotopes, calculated by VS-IMSRG using the new families of 2NF(local) plus 3NF(local) and 2NF(local) plus 3NF(lnl). Experimental data are taken from the 2020 atomic mass evaluation (AME2020) [48]. 14 16 18 20 22 24 26 28 2.0 2.2 2.4 2.6 2.8 3.0 AO Experiment 2NF(local) + 3NF(local) 2NF(local) + 3NF(lnl) 20 22 24 26 28 30 32 34 36 38 40 2.4 2.6 2.8 3.0 3.2 3.4 AMg 22 24 26 28 30 32 34 36 38 40 42 44 2.4 2.6 2.8 3.0 3.2 3.4 ASi 28 30 32 34 36 38 40 42 44 46 48 2.6 2.8 3.0 3.2 3.4 AS 32 34 36 38 40 42 44 46 48 50 52 2.6 2.8 3.0 3.2 3.4…
Figure 6. Charge density distributions of 16O and 40Ca, calculated with 2NF(local)+3NF(local) and 2NF(local)+3NF(lnl), compared with experimen￾tal data [63]. The density of 40Ca is shifted by 0.05 fm−3 for better readability. In this work, we have constructed chiral three-nucleon forces at N2LO , which form new families with the new high-quality local position-space two-nucleon interaction established by the Idaho group. The two low-energy constants, cD and cE, of the 3NF are constrained using the ground-state energies of 3H and 16O. We find that employing a local-nonlocal hybrid…

Showing 5 of the paper's 6 figures. See all figures in the PDF ↗ Figures reproduced from arXiv:2601.08199 by the authors.

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