PaperPanorama

Nuclear Theory·nucl-th

Wednesday·August 26, 2026

11 papers4 primary·7 cross-listed

  1. 01

    Deuterium Production in an Effective Field Theory Constructed from On-Shell Amplitudes

    Tim M.P. Tait🇺🇸

    We compute the deuterium-production reaction in an effective field theory whose degrees of freedom are the nuclear states themselves: the amplitude is assembled from on-shell three-point vertices, glued across its factorization channels, and completed by the contact terms consistent with the symmetries. The deuteron enters through the -- vertex, normalized to the measured asymptotic normalization coefficient. Rescattering of the nucleon pair is resummed dispersively, leaving two short-distance constants, an isovector magnetic and an electric dipole contact interaction. A joint Bayesian fit to the thermal capture measurements and the SLEGS photodisintegration data finds both of natural size and determines the thermonuclear rate to 0.22-0.24% across the nucleosynthesis window, including systematics spanning the defensible treatments of the SLEGS data and of the -wave rescattering. Truncating the expansion is bounded separately at 0.12%, of which the next order of contact terms -- degenerate with the two fitted constants -- supplies 0.03%, for a total theory uncertainty of 0.25-0.27%. Propagated through a BBN network, the rate shifts the predicted primordial deuterium by -0.06% and cuts this reaction's contribution to the D/H uncertainty from 0.089% to 0.050%, retiring it from the primordial D/H error budget for practical purposes.

    nucl-thastro-ph.COhep-phhep-th0 citations
  2. 02

    Deformed self-consistent Green's function method for atomic nuclei at second and third order in the algebraic diagrammatic construction

    A. Scalesi · T. Duguet · V. Somà

    The description of atomic nuclei from first principles constitutes one of the central goals of nuclear theory. Polynomial-scaling expansion methods have extended \textit{ab initio} calculations at sub-percent accuracy to medium-mass nuclei and a few closed-shell heavy nuclei, but deformed doubly open-shell heavy and superheavy nuclei remain out of reach. The self-consistent Green's function (SCGF) formalism is here extended to doubly open-shell nuclei by allowing the one-body propagator to spontaneously break SU(2) rotational symmetry. The resulting deformed SCGF (dSCGF) scheme, based on the algebraic diagrammatic construction truncated at first, second, and third order, is implemented in a newly developed many-body suite, \texttt{FoxTrot}. Numerical strategies required to handle the associated, symmetry-unrestricted -scheme working basis are discussed in detail. The method is illustrated through a study of Si based on the 1.8/2.0 (EM) Hamiltonian. The impact of the three-nucleon interaction and of its rank-reduction approximation on the deformed Hartree-Fock total energy curve is examined, and the correlated curve obtained from constrained dSCGF calculations is shown to differ appreciably from the mean-field one. Physical solutions appearing as minima of the correlated curve are shown to be reachable via unconstrained calculations starting from any point along the deformed Hartree-Fock curve, demonstrating the self-consistent character of the method. The Si ground-state binding energy at third order, extrapolated to the infinite basis-size limit, reproduces experiment within , while the excited prolate solution is consistent with the observed shape isomer. The present developments open the way to an accurate ab initio description of all (very) heavy nuclei in the near future.

    nucl-th1 citation
  3. 03

    Self-Consistent Determination of the Transition Temperature Between the and Reactions

    R. Ya. Kezerashvili · N. A. Burkova · A. S. Tkachenko · S. B. Dubovichenko

    We present the first self-consistent theoretical study of the competing and reactions within the same modified potential cluster model (MPCM). For the CN reaction, total cross sections, astrophysical factors, and reaction rates are calculated using interaction potentials constrained by the available scattering and bound-state data. The astrophysical -factor is estimated as ~keV. Combining these results with our recent MPCM calculations for , we determine the transition temperature at which proton capture overtakes neutron capture in the production of . The self-consistent comparison predicts a transition temperature under Maxwell--Boltzmann statistics, significantly higher than previous estimates. The analysis is extended to Tsallis statistics, demonstrating that deviations from thermal equilibrium produce substantial shifts of the transition temperature. These results provide improved nuclear-physics input for astrophysical nucleosynthesis calculations.

    nucl-thastro-ph.SR0 citations
  4. 04

    Resolving the -meson directed-flow puzzle by multi-step meson--baryon dynamics

    Yingjie Zhou🇩🇪 · Taesoo Song🇩🇪 · Susanne Glässel🇩🇪 · Jiaxing Zhao🇩🇪 · Christoph Blume🇩🇪 · Iouri Vassiliev🇩🇪 · Vadim Voronyuk🇷🇺 · Yaping Wang🇨🇳 · Nu Xu🇨🇳 · Jörg Aichelin🇫🇷 · Elena Bratkovskaya🇩🇪

    Recent STAR measurements at fixed-target Beam Energy Scan energies have revealed an unexpectedly large directed flow of mesons in Au+Au collisions, comparable to that of protons and baryons and much stronger than that of light strange mesons. Since the is a hidden-strangeness meson with relatively weak interactions with non-strange hadrons, this observation has been interpreted as a possible signal of unconventional baryonic dynamics or exotic baryonic resonances coupled to the channel. Within the framework of the Parton-Hadron-Quantum-Molecular-Dynamics(PHQMD) model, we demonstrate that in the high baryon density region, mesons are produced predominantly through multi-step meson--baryon and meson--hyperon reactions, whose transition amplitudes are constrained by a coupled-channel -matrix calculation based on an extended SU(6) chiral effective Lagrangian. Together with the in-medium broadening of the spectral function, these baryon-driven production channels enhance near-threshold production and imprint the collective motion of the baryon-rich source on the produced mesons.

    nucl-th0 citations
  5. 05

    Universality and Kinematic Dependence of Hadronization Effects in DIS Global Event Shapes

    Radja Boughezal🇺🇸 · Haotian Cao🇺🇸 · Zhong-Bo Kang🇺🇸 · Xiaohui Liu🇨🇳 · Sonny Mantry🇺🇸 · Frank Petriello🇺🇸

    We propose a unified framework for a combined global analysis to constrain leading hadronization effects across the 1-Jettiness class of global event shapes for Deep Inelastic Scattering (DIS). We show that for the subclass of jet-based event shapes where the leading jet direction is determined dynamically event-by-event, the leading hadronization effects can acquire a non-trivial dependence on the hard scattering kinematics. However, this dependence is explicitly calculable, allowing for universality of leading hadronization effects in the 1-Jettiness class. The non-trivial kinematic dependence provides an independent lever arm for simultaneously constraining hadronization effects in the jet-based and DIS thrust event shapes. This universality, combined with the kinematic lever arm, could allow for including the typically ignored peak region, where hadronization effects are most severe, in precision extractions of the strong coupling. We demonstrate the need for such a unified treatment of hadronization effects through comparisons of theoretical predictions with simulation data.

    hep-phnucl-th0 citations
  6. 06

    Femtoscale imaging of the proton with Ioffe-time distributions

    Robert G. Edwards🇺🇸 · Joe Karpie🇺🇸 · Christopher Monahan🇺🇸 · Kostas Orginos🇺🇸 · Anatoly Radyushkin🇺🇸 · David Richards🇺🇸 · Eloy Romero🇫🇷 · Savvas Zafeiropoulos🇫🇷

    Mapping how strongly interacting constituents are distributed within protons is a key goal of nuclear physics and a major direction of the future Electron Ion Collider program. We propose a novel space-time description of hadron structure in terms of impact-parameter Ioffe-time distributions, relating spatial density in the plane transverse to the proton momentum and the time between the probe's absorption and the product's emission in the longitudinal direction. Using lattice Quantum Chromodynamics, we perform the first calculation of the Ioffe-time-dependent mean squared proton radii and compare our results with estimates in the Goloskokov-Kroll model. We derive a relationship between the experimentally measurable Compton form factor and the generalized Ioffe-time distribution, which allows us to perform the first extraction of the Compton form factor from lattice calculations.

    hep-phhep-latnucl-th0 citations
  7. 07

    Neuro-dispersive extractions of light-meson resonances

    Wyatt A. Smith🇺🇸 · Arkaitz Rodas🇺🇸 · Marius D. Thomas🇺🇸 · César Fernández-Ramírez🇪🇸 · Giorgio Foti🇮🇹 · Lin Qiu🇺🇸 · Adam P. Szczepaniak🇺🇸 · Alessandro Pilloni🇮🇹

    We present the first dispersive extraction of resonant poles from analytically continued neural networks. We use S-matrix informed neural networks (SINNs) trained to respect unitarity, analyticity, and crossing symmetry, without fixing a specific amplitude parametrization. The SINN framework controls representation dependence, enables constrained data selection, and enforces first principles. A large ensemble of networks trained on scattering data propagates correlated uncertainties to all derived observables. We obtain robust determinations of the , , and poles of scattering. Scattering lengths are determined alongside the amplitudes, while Adler zeroes emerge as predictions of the analytic structure. The results are stable against variations of the network architecture, and our approach can easily be adjusted for analysis of other reactions relevant to New Physics searches.

    hep-phnucl-th0 citations
  8. 08

    S-matrix informed neural networks for amplitude analysis

    Wyatt A. Smith🇺🇸 · Arkaitz Rodas🇺🇸 · Marius D. Thomas🇺🇸 · César Fernández-Ramírez🇪🇸 · Giorgio Foti🇮🇹 · Lin Qiu🇺🇸 · Adam P. Szczepaniak🇺🇸 · Alessandro Pilloni🇮🇹

    Reconstructing scattering amplitudes from finite, noisy, and mutually inconsistent measurements is an ill-posed inverse problem common to many reactions relevant to particle physics. We introduce S-matrix informed neural networks (SINNs), and demonstrate their ability to learn scattering amplitudes directly from data while respecting first principles. We further develop a novel data selection procedure, which uses the response of constrained neural network ensembles to identify a set of experiments compatible with first principles, and with each other. We apply this framework to scattering, producing reusable amplitudes and correlated uncertainties without relying on a fixed functional form. We validate our results against residual model dependencies and training biases through closure tests and ablations. We find negligible impact of model architecture on our results. Our workflow unifies physics-constrained representation learning, data selection, and uncertainty quantification. Our strategy is transferable to other scattering processes, and other constrained physics problems limited by inconsistent data.

    hep-phcs.LGnucl-th0 citations
  9. 09

    Testing the QGP Star Hypothesis: The oMEGACat BH-2 System as a Candidate Color-Superconducting Quark-Gluon Plasma Star

    Herman J. Mosquera Cuesta🇪🇸

    The recent discovery of a long-period binary system in the globular cluster Centauri, oMEGACat BH-2 \citep{Whitaker2026}, provides an unprecedented opportunity to probe the true nature of compact dark objects. The system's massive, dark companion has been inferred to have a mass of , which places it in the ``mass gap'' between neutron stars and the canonical stellar-mass black holes. In this Letter, we explore the hypothesis that the oMEGACat BH-2 companion is not a classical black hole, but a stable, self-bound Quark-Gluon Plasma (QGP) star, as described by recent general relativistic models that incorporate Nonlinear Electrodynamics (NLED) and the asymptotic freedom of Quantum Chromodynamics (QCD) \citep{Mosquera2025}. We compare the inferred mass of the companion with the novel Mass-Radius (-) relation predicted by the QGP star model. We find that the inferred mass of the Centauri object lies squarely within the wide mass spectrum predicted for hypermassive QGP stars ( to ). Although this consistency is not enough for claiming evidence, it suggests that oMEGACat BH-2 may be the first observed candidate for a QGP star, representing a stable, non-singular end-state of stellar collapse. We argue that future astrometric monitoring with JWST and radio-telescopes like FAST and SKA can further constrain the oMEGACat BH-2 orbital parameters. Meanwhile, gravitational-wave follow-ups for the and modes by observatories like LIGO, VIRGO, KAGRA, LISA, ET and CE can be crucial for distinguishing a classical black hole from the ``gravitational eternally collapsing `kompact' object'' (\GECKO) state of our QGP star model.

    astro-ph.HEgr-qchep-phnucl-th0 citations
  10. 10

    Resummed Power Corrections in Nuclear DVCS

    John Terry🇺🇸

    Generalized Parton Distributions (GPDs) encode the three-dimensional structure of hadrons, yet their modification in nuclear matter remains largely unconstrained. We report the first derivation of resummed QCD power corrections to deeply virtual Compton scattering on nuclei. Extending techniques from inclusive deep inelastic scattering, we identify the nuclear-enhanced higher-twist contributions generated by coherent final-state scattering of the struck quark in the medium and resum them to all orders. The corrections are enhanced by an effective nuclear size and result in an exclusive analogue of dynamical nuclear shadowing. The shift is controlled by a parameter already fixed by inclusive nuclear data, so no new nonperturbative input enters. We present quantitative predictions for nuclear modifications of beam-spin observables at the Electron--Ion Collider.

    hep-phnucl-exnucl-th0 citations
  11. 11

    STAR Highlights II: Study of Small Systems and the Search for New, Exotic Physics

    Jiangyong Jia

    Twenty-five years of RHIC operation have produced a uniquely diverse dataset, which enables a broad physics program. This contribution highlights recent STAR results in four areas: exotic-state searches and ultra-peripheral collisions; the onset of quark--gluon plasma (QGP) signatures in small systems; radial flow and its fluctuations; and polarization and spin correlations.

    nucl-exnucl-th0 citations

Affiliations

first authorsco-authorsvia INSPIRE