PaperPanorama

Nuclear Theory·nucl-th

Monday·October 20, 2025

10 papers7 primary·3 cross-listed

  1. 01

    [Submitted on 16 Oct 2025]

    Ab initio symmetry-adapted approaches to nuclear reactions

    Kristina D Launey🇺🇸 · Grigor H. Sargsyan🇺🇸 · Alexis Mercenne🇺🇸 · Jutta E. Escher🇺🇸 · Darin C. Mumma🇺🇸

    In this review, we discuss recent applications of the ab initio symmetry-adapted no-core shell-model (SA-NCSM) theory for study and prediction of structure and reactions of stable and unstable nuclei from light to medium mass range. We explore structure properties of neutron-rich He, Mg, and Li isotopes, with a focus on nuclear collectivity, clustering, and spectroscopic factors, as well as multi-particle excitations of utmost significance in the proximity of the drip lines. In addition, we present extensions of the SA-NCSM with continuum for determining the microscopic structure of reaction fragments, which enables calculations of reaction cross sections for targets from the lightest He to Ca, rooted in first principles. We illustrate this for neutron and proton elastic scattering, deuteron and alpha capture reactions, and alpha knock-out reactions. Furthermore, we discuss microscopic optical potentials with uncertainty quantification, a critical ingredient in many reaction models, and reaction observables with uncertainties that stem from the underlying chiral potential. We also discuss the impact of alpha clustering on reactions of significance to nuclear astrophysics, as well as on beta decays and beyond-the-standard-model physics.

    Comments:
    Review article (submitted to Progress in Particle and Nuclear Physics)
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    2510.15171 [pdf]
    PPNP(2026)·8 citations
  2. 02

    [Submitted on 17 Oct 2025]

    Universal Relation for the Neutron Star Maximum Mass within Relativistic Mean-Field Theories

    Gihwan Nam🇰🇷 · Yeunhwan Lim🇰🇷 · Jeremy W. Holt🇺🇸

    We obtain a universal relation for the neutron star maximum mass arising from a particular combination of the saturation density (), the effective mass (), and (when present) the vector meson self-coupling constant () within the relativistic mean-field model framework. Observations of massive neutron stars heavier than have eliminated the softest equation of state from consideration and impose strong constraints on nuclear interactions used to model dense nuclear matter. To date there have been numerous attempts to refine relativistic mean-field models by including the presence of additional mesons, such as the delta meson, and couplings. We show that current RMF models, including our own constructions, exhibit a maximum neutron star mass that is primarily determined by the combination of the saturation density, the effective mass at saturation, and the vector meson self-coupling constant. When constraining the pure neutron matter equation of state using chiral effective field theory (ChEFT) at low densities, 250 parameter sets were generated to derive an empirical formula for the maximum mass of neutron stars and apply the formula with the present relativistic mean field models.

    Comments:
    19 pages, 12 figures
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    2510.15356 [pdf]
    PRC(2026)·3 citations
  3. 03

    [Submitted on 17 Oct 2025]

    New Elementary Operator for Kaon Photoproduction on the Nucleon and Nuclei

    Terry Mart🇮🇩 · Jovan Alfian Djaja🇮🇩

    A new elementary operator for kaon photoproduction on the nucleon and nuclei has been developed within a Feynman diagrammatic framework. By fitting the unknown coupling strengths at the electromagnetic and hadronic vertices of the baryon resonances to all available experimental data across the six isospin channels, the model achieves excellent agreement with the data. The operator includes 26 nucleon resonances in the channels and 17 additional resonances in the channels. For applications to nuclear reactions, such as hypernuclear photoproduction, the operator is formulated in Pauli space, allowing a straightforward implementation of the nonrelativistic approximation. Several alternative forms for expressing the operator output are proposed. In one of them, the spin operators and photon polarization vectors are separated from the operator, since both are frame dependent, thereby enhancing its versatility in nuclear applications.

    Comments:
    18 pages, 9 figures, contribution to 9th International Conference on Asia-Pacific Few-body problem in Physics (APFB2025), Ho Chi Minh City, Vietnam. Submitted to Few-Body Systems
    Subjects:
    Nuclear Theory (nucl-th); High Energy Physics — Phenomenology (hep-ph)
    arXiv:
    2510.15482 [pdf]
    Few Body Syst.(2026)·2 citations
  4. 04

    [Submitted on 17 Oct 2025]

    Antikaon condensation in magnetized neutron star matter within the framework of the -cut scheme

    Fei Wu · Chen Wu

    This study investigates the effects of strong magnetic fields on antikaon condensation in neutron star matter using the extended FSUGold model model. It is found that the presence of strong magnetic fields alters the threshold density of antikaon condensation significantly, which means the threshold density of antikaon condensation is shifted to higher density compared with the magnetic field-free case. In the presence of strong magnetic fields, the equation of state (EoS) becomes stiffer than that of the zero field case. The effects of the -cut scheme on the EoS are also researched when the appearance of antikaon condensation is occurred. Through careful choice of the parameter of the -cut scheme, we are able to produce a maximum mass neutron star heavier than 2.

    Comments:
    25 pages, 8 figures
    Subjects:
    Nuclear Theory (nucl-th); High Energy Astrophysical Phenomena (astro-ph.HE)
    arXiv:
    2510.15521 [pdf]
    PRC(2025)·0 citations
  5. 05

    [Submitted on 17 Oct 2025]

    Faddeev-type calculation of nonelastic breakup in deuteron-nucleus scattering

    A. Deltuva🇱🇹

    The nonelastic breakup (NEB), one of channels in inclusive reactions, is studied using the Faddeev-type scattering theory. The NEB differential cross section is obtained in terms of the imaginary part of the neutron-nucleus optical potential sandwiched between the Alt-Grassberger-Sandhas three-body transition operators. The momentum-space calculations including the Coulomb force are extended to higher charge numbers. Well converged numerical results are obtained for the energy distribution of the NEB cross section, being roughly consistent with previous works. The spin-dependent interaction terms do not play a significant role. The optical potential nonlocality effect shows up at higher proton energies, but is comparable to local potential uncertainties.

    Comments:
    7+ pages, 4 figures, published Phys. Lett. B 868 (2025) 139825
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    2510.15619 [pdf]
    PLB(2025)·2 citations
  6. 06

    [Submitted on 17 Oct 2025]

    Reexamining the perturbative renormalizability of the coupled triplets

    Manuel Pavon Valderrama🇨🇳

    I reexamine the perturbative renormalizability of chiral two-pion exchange in two-nucleon scattering for coupled triplets when one-pion exchange has been fully iterated at leading order. Improving over previous works, it is shown that only two counterterms are required to obtain cutoff independent results, which is one less than in naive dimensional analysis. The explanation for this reduction is the existence of an attractive and repulsive eigenchannel in the one-pion exchange potential for the coupled triplets: the attractive eigenchannel can be renormalized like a regular attractive uncoupled triplet, while the repulsive eigenchannel is always finite regardless of whether there are counterterms or not. I discuss the implications of this finding for the power counting of the - and - partial waves.

    Comments:
    19 pages, 3 figures, corresponds to the published version
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    2510.15789 [pdf]
    PRC(2026)·7 citations
  7. 07

    [Submitted on 17 Oct 2025]

    Quantum Monte Carlo Calculations of Light Nuclei with Fully Propagated Theoretical Uncertainties

    Ryan Curry🇨🇦 · Kai Hebeler🇩🇪 · Stefano Gandolfi🇺🇸 · Alexandros Gezerlis🇨🇦 · Achim Schwenk🇩🇪 · Rahul Somasundaram🇺🇸 · Ingo Tews🇺🇸

    We report on the first quantum Monte Carlo calculations of helium isotopes with fully propagated theoretical uncertainties from the interaction to the many-body observables. To achieve this, we build emulators for solutions to the Faddeev equations for the binding energy and Gamow-Teller matrix element of , as well as for auxiliary-field diffusion Monte Carlo calculations of the charge radius, employing local two- and three-body interactions up to next-to-next-to-leading order in chiral effective field theory. We use these emulators to determine the posterior distributions for all low-energy couplings that appear in the interaction up to this order using Bayesian inference while accounting for theoretical uncertainties. We then build emulators for auxiliary-field diffusion Monte Carlo for helium isotopes and propagate the full posterior distributions to these systems. Our approach serves as a framework for studies of atomic nuclei with consistently treated and correlated theoretical uncertainties.

    Comments:
    8 pages, 4 figures
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    2510.15860 [pdf]
    9 citations

Affiliations

first authorsco-authorsvia INSPIRE