PaperPanorama

Nuclear Theory·nucl-th

Tuesday·August 5, 2025

13 papers7 primary·6 cross-listed

  1. 01

    [Submitted on 1 Aug 2025]

    Criticality analysis of nuclear binding energy neural networks

    S.A. Sundberg · R.J. Furnstahl

    Machine learning methods, in particular deep learning methods such as artificial neural networks (ANNs) with many layers, have become widespread and useful tools in nuclear physics. However, these ANNs are typically treated as ``black boxes'', with their architecture (width, depth, and weight/bias initialization) and the training algorithm and parameters chosen empirically by optimizing learning based on limited exploration. We test a non-empirical approach to understanding and optimizing nuclear physics ANNs by adapting a criticality analysis based on renormalization group flows in terms of the hyperparameters for weight/bias initialization, training rates, and the ratio of depth to width. This treatment utilizes the statistical properties of neural network initialization to find a generating functional for network outputs at any layer, allowing for a path integral formulation of the ANN outputs as a Euclidean statistical field theory. We use a prototypical example to test the applicability of this approach: a simple ANN for nuclear binding energies. We find that with training using a stochastic gradient descent optimizer, the predicted criticality behavior is realized, and optimal performance is found with critical tuning. However, the use of an adaptive learning algorithm leads to somewhat superior results without concern for tuning and thus obscures the analysis. Nevertheless, the criticality analysis offers a way to look within the black box of ANNs, which is a first step towards potential improvements in network performance beyond using adaptive optimizers.

    Comments:
    23 pages, 14 figures
    Subjects:
    Nuclear Theory (nucl-th); High Energy Physics — Phenomenology (hep-ph)
    arXiv:
    2508.01001 [pdf]
    J.Phys.G(2025)·2 citations
  2. 02

    [Submitted on 2 Aug 2025]

    Exactness of the normal-ordered two-body truncation of three-nucleon forces

    Maxwell Rothman · Ben Johnson-Toth · Francesca Bonaiti · Gaute Hagen · Matthias Heinz · Thomas Papenbrock

    Reference-state-based many-body methods start from Hamiltonians that are normal ordered with respect to the reference state. In low-energy nuclear physics applications normal-ordered Hamiltonians consisting of two- and three-nucleon forces are usually truncated at the two-body rank with residual three-nucleon operators being discarded. Benchmark computations have shown that this truncation is accurate, but we lack an understanding about why it works. We show that the normal-ordered two-body truncation is exact for zero-range three-body forces when nuclei are computed using the coupled cluster with singles and doubles method. As the nuclear three-nucleon force is short ranged and a three-body contact is a leading term in effective field theories of quantum chromodynamics, our result provides an analytical basis for the popular normal-ordered two-body approximation.

    Comments:
    6 pages, 2 figures, 1 table
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    2508.01507 [pdf]
    PRC(2025)·9 citations
  3. 03

    [Submitted on 4 Aug 2025]

    nuclear contact coefficients in the generalized contact formalism

    E. Proietti · L.E. Marcucci · M. Viviani

    We present a theoretical calculation for the and 4 nuclear contact coefficients within the generalized contact formalism, using both local and non-local chiral potentials. The Hyperspherical Harmonics method is employed to calculate the nuclear wave functions, from which we derive two-body momentum distributions and density functions to extract the contact coefficients. We have extracted the contact coefficients from two-body momentum distributions or from density functions, for a given nucleus and potential, and we have found that the generalized contact formalism predictions are verified in the triplet spin channel for local and non-local potentials. On the other hand, some significant tensions exist for the singlet channels, especially when studied with non-local potentials. We have also analyzed the model-independence of the ratios between the contact coefficients, and we have found to be quite satisfied. This study extends previous works based on local interaction models only.

    Comments:
    29 pages, 25 figures and 4 tables. New version accepted for publication
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    2508.02200 [pdf]
    PRC(2026)·0 citations
  4. 04

    [Submitted on 4 Aug 2025]

    Tribute to Toshimitsu Yamazaki (1934-2025): Quest for Exotic Hadronic Matter

    Avraham Gal🇮🇱

    In this talk I pay tribute to Toshimitsu Yamazaki who died earlier this year. Yamazaki's leading contributions to Hadronic Physics, in particular to Strangeness Nuclear Physics in Japan and elsewhere, are well known. Two of the five Recurring Themes of his research, as listed in the Japan Academy site, are highlighted here: (i) Discovery of deeply bound pionic-atom states, and (ii) Search for kaonic nuclei -- Kaonic Proton Matter (KPM). I conclude by reviewing briefly my own recent work, confirming Farrar's conjecture that a deeply bound dibaryon is not ruled out by the weak-decay observation of hypernuclei. However, the relatively long lifetime of such a deeply bound is much too short to qualify it for a Dark-Matter candidate.

    Comments:
    Presented at the 21st Int'l Conf. Hadron Spectroscopy and Structure (HADRON 2025) March 27-31, 2025, Toyonaka Campus, Osaka University, Japan. To be published as PoS(HADRON2025)263
    Subjects:
    Nuclear Theory (nucl-th); High Energy Physics — Phenomenology (hep-ph); Nuclear Experiment (nucl-ex)
    arXiv:
    2508.02267 [pdf]
    PoS(2026)·0 citations
  5. 05

    [Submitted on 4 Aug 2025]

    Coulomb-Corrected Wormhole Model for Neon-20

    Ruoxin Bai🇬🇧 · N.S. Manton🇬🇧

    Building on the spatial wormhole geometry proposed by Manton and Dunajski, we develop a modified model for the Neon-20 nucleus that incorporates a repulsive Coulomb potential. This reduces the large threshold energy for cluster break-up in the original model and converts most bound states to resonances. We use generalized WKB methods to calculate the energies of bound states, and also the energies and widths of under-barrier and over-barrier resonances. The results align closely with experimental data for the 0_1^+ , 0_1^- and 0_4^+ rotational bands of Neon-20, including the large widths in the higher-nodal 0_4^+ band.

    Comments:
    25 pages, 9 figures
    Subjects:
    Nuclear Theory (nucl-th); High Energy Physics — Theory (hep-th)
    arXiv:
    2508.02428 [pdf]
    NPA(2026)·1 citation
  6. 06

    [Submitted on 4 Aug 2025]

    Density functional theory of renormalization group in nuclear matter

    Yong-rui Chen🇨🇳 · Wei-jie Fu🇨🇳 · Yang-yang Tan🇨🇳

    The density functional renormalization group (density-fRG) is proposed to investigate the density fluctuations within the functional renormalization group approach, which allows us to quantify the medium effect and study physics of high densities. This method is applied to the nucleon-meson effective field theory, also known as the Walecka model, to study the properties of nuclear matter at high baryon densities. It is found that both the attractive and repulsive nucleon meson interactions are screened by the high density medium, which results in a stiffer equation of state (EoS) of nuclear matter in the regime of , then a softer EoS when . Here denotes the saturation baryon density of symmetric nuclear matter. Furthermore, a new phenomenon called the locking of Fermi surface is found. In the locking of Fermi surface the effective energy of quasi-nucleon is always close to the Fermi surface, which are both running with the renormalization group scale.

    Comments:
    18 pages, 13 figures, 1 table
    Subjects:
    Nuclear Theory (nucl-th); High Energy Physics — Phenomenology (hep-ph)
    arXiv:
    2508.02575 [pdf]
    PRC(2026)·2 citations
  7. 07

    [Submitted on 4 Aug 2025]

    Bound states of Be within cluster models based on state-of-the-art HAL QCD charmonium-nucleon interactions

    Faisal Etminan🇮🇷

    The possible bound state of the Be, a charmonium-nucleus system, is investigated. The analysis is carried out within a three-cluster model, where its binary subsystems are represented as and . The hyperspherical harmonics method is employed to facilitate a convenient description of this three-cluster configuration. The calculations are done by employing the effective potentials. These potentials were derived recently based on state-of-the-art lattice QCD calculations, which provided interactions for the spin 3/2 , spin 1/2 , spin 1/2 and spin-averaged interactions, all obtained with nearly physical pion masses. The Coulomb interaction was also incorporated into the current calculations. It is determined that, despite neither the He nor the Be binary subsystems being bound, a bound state of the nuclear system could potentially exist. The maximum central binding energy is found to be approximately 1.71 MeV, based on the spin 1/2 interaction, while a minimum value of about 0.56 MeV is obtained from calculations involving the spin 1/2 interaction.

    Comments:
    14 pages, 1 figure , 1 table
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    2508.02653 [pdf]
    PRC(2025)·4 citations
  8. 08

    [Submitted on 1 Aug 2025] (cross-list from hep-ph)

    Re-optimization of a deep neural network model for electron-carbon scattering using new experimental data

    Beata E. Kowal🇵🇱 · Krzysztof M. Graczyk🇵🇱 · Artur M. Ankowski🇵🇱 · Rwik Dharmapal Banerjee🇵🇱 · Jose L. Bonilla🇵🇱 · Hemant Prasad🇵🇱 · Jan T. Sobczyk🇵🇱

    We present an updated deep neural network model for inclusive electron-carbon scattering. Using the bootstrap model [Phys.Rev.C 110 (2024) 2, 025501] as a prior, we incorporate recent experimental data, as well as older measurements in the deep inelastic scattering region, to derive a re-optimized posterior model. We examine the impact of these new inputs on model predictions and associated uncertainties. Finally, we evaluate the resulting cross-section predictions in the kinematic range relevant to the Hyper-Kamiokande and DUNE experiments.

    Comments:
    15 pages, 12 figures, some additional comments added
    Subjects:
    High Energy Physics — Phenomenology (hep-ph); Machine Learning (cs.LG); Nuclear Experiment (nucl-ex); Nuclear Theory (nucl-th)
    arXiv:
    2508.00996 [pdf]
    PRC(2025)·0 citations
  9. 09

    [Submitted on 3 Aug 2025] (cross-list from hep-lat)

    Lattice Calculation of Short-Range Contributions to Neutrinoless Double-Beta Decay at Physical Pion Mass

    Peter Boyle🇺🇸 · Felix Erben🇨🇭 · Xu Feng🇨🇳 · Jonathan M. Flynn🇬🇧 · Nicolas Garron🇬🇧 · Taku Izubuchi🇺🇸 · Luchang Jin🇺🇸 · Rajnandini Mukherjee🇬🇧 · J. Tobias Tsang🇨🇭 · Xin-Yu Tuo🇺🇸

    Neutrinoless double-beta () decays provide an excellent probe for determining whether neutrinos are Dirac or Majorana fermions. The short-range matrix elements associated with the process contribute at leading order in the decay channel through pion exchange between nucleons. However, current lattice calculations show notable discrepancies in predicting these short-range contributions. To address this issue, we perform a lattice QCD calculation of the matrix elements using domain wall fermion ensembles at the physical pion mass generated by the RBC and UKQCD Collaborations. To mitigate contamination from around-the-world effects, we develop a new method to reconstruct and subtract them directly from lattice data. We then perform a nonperturbative renormalization using the RI/SMOM scheme. Compared with previous studies, this work reduces the uncertainties in the matrix elements and provides an independent cross-check that helps to reconcile the discrepancies among previous lattice calculations.

    Comments:
    26 pages, 13 figures
    Subjects:
    High Energy Physics — Lattice (hep-lat); High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
    arXiv:
    2508.01900 [pdf]
    PRD(2026)·1 citation
  10. 10

    [Submitted on 4 Aug 2025] (cross-list from astro-ph.HE)

    -process in Core-Collapse Supernovae: Imprints of General Relativistic Effects

    Alexander Friedland · Derek J. Li · Giuseppe Lucente · Ian Padilla-Gay · Amol V. Patwardhan

    The origin of a number of proton-rich isotopes in the solar system has been a long-standing puzzle. A promising explanation is the -process, which is posited to operate in the neutrino-driven outflows that form inside core-collapse supernovae after shock revival. While recent studies have analyzed several relevant physical effects that influence the efficiency of this process, the impact of General Relativity (GR) on it remains unexplored. We perform a comparative analysis of the time-integrated -process yields in Newtonian and fully GR calculations, using detailed models of time-evolving outflow profiles. The GR effects are seen to suppress the production of seed nuclei, significantly boosting the resulting -nuclide abundances. Our reference GR model, with an 18~ progenitor, reproduces both the relative and absolute solar system abundances of the entire set of the nuclides in the mass range . The yields are suboptimal in our 12.75~ GR model, where the outflow transitions to the supersonic regime several seconds into the explosion, suppressing further -nuclide production. In both models, most of the production of the crucial and isotopes occurs relatively early, 1--3 seconds after shock revival. In contrast, a large fraction of the shielded isotope is produced in the subsequent ejecta. The impact of GR on this isotope is especially large, with its final abundance boosted by a factor of 25 compared to a Newtonian calculation. In summary, with the GR effects taken into account, the -process in a sufficiently massive progenitor can provide a unifying explanation for the origin of all nuclei in the solar system up to Pd.

    Comments:
    47 pages plus 17 pages in appendices, 19 figures. Results and conclusions unchanged. Accepted for publication in JCAP
    Subjects:
    High Energy Astrophysical Phenomena (astro-ph.HE); High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
    arXiv:
    2508.02055 [pdf]
    JCAP(2026)·3 citations
  11. 11

    [Submitted on 4 Aug 2025] (cross-list from hep-ph)

    Gravitational form factors of the nucleon from the chiral effective model

    Daisuke Fujii · Mamiya Kawaguchi · Mitsuru Tanaka

    We investigate the confining pressure and associated global property, i.e, D-term, of the nucleon using the skyrmion approach formulated within scale-invariant chiral perturbation theory. In this framework, the nucleon is modeled as a skyrmion, and a scalar meson is introduced to incorporate the effects of the scale anomaly via low-energy theorems. The contributions from the current quark mass and gluonic dynamics to the scale anomaly are encoded through the pion and scalar meson masses, respectively. By decomposing the nucleon's energy-momentum tensor, we isolate the anomalous components and analyze their role in generating pressure. We find that the gluonic contribution to the scale anomaly plays a dominant role in producing confining pressure. In comparison with results from conventional chiral perturbation theory in the chiral limit, the total pressure derived from sChPT provides improved qualitative agreement with lattice QCD results. We also evaluate the D-term and compare it with recent lattice and model-independent determinations.

    Comments:
    6pages, 1 figures
    Subjects:
    High Energy Physics — Phenomenology (hep-ph); High Energy Physics — Theory (hep-th); Nuclear Theory (nucl-th)
    arXiv:
    2508.02207 [pdf]
    PoS(2026)·0 citations
  12. 12

    [Submitted on 4 Aug 2025] (cross-list from hep-ph)

    Nuclear modification factor in collisions at RHIC and LHC energies in scenarios with and without quark-gluon plasma formation in collisions

    B.G. Zakharov🇷🇺

    We calculate the away-side hadron-triggered modification factor in collisions at RHIC and LHC energies for scenarios with and without quark-gluon plasma formation in collision. We find that for both scenarios theoretical results for agree well with the available data for 2.76 TeV Pb+Pb and 0.2 TeV Au+Au collisions. We make predictions for in 7 TeV O+O collisions that are planned at the LHC. Our results show that measuring in the whole centrality interval and at small centrality (%) may give information on the presence of jet quenching in collisions.

    Comments:
    6 pages, 2 figures
    Subjects:
    High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
    arXiv:
    2508.02623 [pdf]
    JETP Lett.(2025)·0 citations
  13. 13

    [Submitted on 4 Aug 2025] (cross-list from astro-ph.HE)

    PSR J0614-3329: A NICER case for Strange Quark Stars

    Swarnim Shirke🇮🇳 · Rajesh Maiti🇮🇳 · Debarati Chatterjee🇮🇳

    Precise measurements of neutron star masses and radii by the NICER mission impose important constraints on the nuclear equation of state. The most recent NICER measurement of PSR J0614-3329 reported an equatorial radius of km for a mass of . Considering all the NICER measurements to date, we find substantial evidence using Bayesian hypothesis ranking for strange quark stars over physically motivated models of neutron stars compatible with this low radius. This provides a strong case for quark matter in neutron stars and also for the possible existence of strange quark stars, a consequence of the Bodmer-Witten hypothesis, suggesting that they could be considered among the population of compact stars during analyses of astrophysical data. Using a wide sample of equations of state, we report the nucleonic equations of state that best fit current observations and rule out one model of strange quark matter.

    Comments:
    14 pages, 3 figures, 3 tables. Comments are welcome
    Subjects:
    High Energy Astrophysical Phenomena (astro-ph.HE); Solar and Stellar Astrophysics (astro-ph.SR); High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
    arXiv:
    2508.02652 [pdf]
    11 citations

Affiliations

first authorsco-authorsvia INSPIRE