PaperPanorama

Nuclear Theory·nucl-th

Monday·October 20, 2025

10 papers7 primary·3 cross-listed

  1. 01

    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.

    nucl-thPPNP(2026)·8 citations
  2. 02

    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.

    nucl-thPRC(2026)·3 citations
  3. 03

    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.

    nucl-thhep-phFew Body Syst.(2026)·2 citations
  4. 04

    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.

    nucl-thastro-ph.HEPRC(2025)·0 citations
  5. 05

    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.

    nucl-thPLB(2025)·2 citations
  6. 06

    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.

    nucl-thPRC(2026)·7 citations
  7. 07

    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.

    nucl-th9 citations
  8. 08

    Adiabatic hydrodynamization and quasinormal modes of nonthermal attractors

    Matisse De Lescluze🇧🇪 · Michal P. Heller🇧🇪 · Aleksas Mazeliauskas🇩🇪 · Bruno Scheihing-Hitschfeld🇺🇸 · Clemens Werthmann🇧🇪

    Nonthermal attractors govern the emergent self-similar dynamics of far-from-equilibrium quantum systems, from ultrarelativistic nuclear collisions to cold-atom experiments. Within the framework of adiabatic hydrodynamization, the approach to a nonthermal attractor is described by the decay of excited states of an effective Hamiltonian. Using an exactly solvable kinetic theory -- the longitudinally expanding, overoccupied gluon plasma dominated by small-angle elastic scattering -- we establish a direct correspondence between the eigenmodes of adiabatic hydrodynamization and the quasinormal mode spectrum of the nonthermal attractor. This equivalence suggests a general framework for identifying universal dynamical structures in nonequilibrium systems. As a byproduct, we derive analytic prescaling solutions for strongly longitudinally expanding systems.

    hep-phcond-mat.quant-gashep-thnucl-thPRL(2026)·3 citations
  9. 09

    Universal Relations for Elastic Hybrid Stars and Quark Stars

    Chun-Ming Yip🇨🇳 · Shu Yan Lau🇺🇸 · Kent Yagi🇺🇸

    Some compact stars may contain deconfined quark matter, forming hybrid stars or quark stars. If the quark matter forms an inhomogeneous condensate in the crystalline color superconducting phase, its rigidity may be high enough to noticeably alter the stellar properties. In this paper, we investigate whether these elastic stars follow the universal relations, i.e., relations insensitive to equations of state, that have been well established for fluid stars. We improve upon previous studies by allowing quark matter in the background, static, and spherically symmetric configuration to be sheared. Such background shear can be treated in the form of an effective pressure anisotropy. We then calculate the moment of inertia , tidal deformability , and spin-induced quadrupole moment of these models with pressure anisotropy. The -- universal relations for the elastic hybrid (quark) star models are valid up to a variation of , larger than that for typical fluid star models, when the maximal magnitude of quark matter shear modulus is considered in the crystalline color superconducting phase from realistic calculations. The uncertainty in universal relations related to the stellar compactness for these elastic star models, on the other hand, remain comparable to those for typical fluid star models. Our results demonstrate the validity of universal relations for hybrid stars and quark stars with a realistic degree of pressure anisotropy due to the crystalline color superconducting quark matter.

    astro-ph.HEgr-qcnucl-thPRD(2026)·1 citation
  10. 10

    Probing Composite Structure and Spin-Orbit Coupling with GPDs in He

    Antonio Garcia Vallejo🇺🇸 · Matthew D. Sievert🇺🇸

    In this work, we extend the Impulse Approximation for the generalized parton distributions (GPDs) of a spin-0 composite hadron with spin- constituents to manifestly incorporate the symmetries of the target wave function. The method utilizes a light-front Wigner function representation instead of a spectral density and a basis of Pauli matrices for the spin. It exploits the boost invariance of the light front and rotational invariance in the rest frame to parameterize the Wigner density in terms of only 3 structures. In addition to the isotropic term and a term describing coupling previously observed for transverse momentum dependent parton distributions (TMDs), we also identify a novel coupling to the angular momentum \textit{transfer} which is unique to the case of GPDs. We then apply the framework to a composite He target with simple phenomenological models to identify qualitative experimental signatures of composite-structure effects in light nuclei. The framework we have constructed here can be readily extended to the case of generalized TMDs (GTMDs), while the phenomenological framework is applicable both to analyses of light nucleus data and as training input for AI-assisted applications.

    hep-phnucl-thPRD(2026)·0 citations

Affiliations

first authorsco-authorsvia INSPIRE