PaperPanorama

Nuclear Theory·nucl-th

Wednesday·April 22, 2026

7 papers5 primary·2 cross-listed

  1. 01

    A novel approach to proton-boron-11 fusion

    Hong-Yi Wang · Yu-Qi Li · Qian Wu · Zhu-Fang Cui

    Proton-boron-11 (p-B) fusion is a highly attractive aneutronic pathway for clean energy production, offering abundant fuel, negligible neutron activation, and the potential for direct energy conversion of charged particles. However, its practical implementation is severely hindered by the extremely high Coulomb barrier, necessitating ignition temperatures far beyond those of conventional deuterium-tritium reactions. In this work, we propose a novel approach to enhance the low-energy fusion cross-section by introducing a negative muon (). Instead of relying on the thermal equilibrium formation of a muonic molecule, we investigate a kinetic scenario in which a muonic hydrogen atom (p) is formed first and subsequently bombarded with a B nucleus. We quantitatively characterize the dynamic screening of the proton's Coulomb field by the tightly bound cloud, the resulting modified Coulomb potential substantially lowers the effective barrier at intermediate separations. We also evaluate the penetrability, reaction cross-section, and reactivity of the p-B system, the results indicate that the inclusion of enhances the tunneling probability by several orders of magnitude at incident energies below 100~keV, thereby significantly reducing the threshold for the nuclear reaction. This mechanism offers a promising alternative perspective for catalyzing p-B fusion, and also suggests a potential ignition pathway.

    nucl-thphysics.plasm-ph1 citation
  2. 02

    Geometric Bias and Centrality Dependence of Jet Quenching in High-Energy Nuclear Collisions

    Changle Sun🇨🇳 · Yichao Dang🇨🇳 · Shanshan Cao🇨🇳

    Jet quenching provides a valuable measure of the opacity of the quark-gluon plasma (QGP) produced in high-energy heavy-ion collisions. However, substantial suppression of charged hadron spectra is observed in highly peripheral collisions, despite the expectation of negligible jet-QGP interactions in this regime. To address this, we develop a HIJING-based initial condition model that accounts for the impact parameter dependence of both inelastic nucleon-nucleon (NN) collisions and the number of hard partonic scatterings per inelastic NN collision. This dependence introduces a geometric bias effect on the jet yield within a given centrality class of nucleus-nucleus (AA) collisions, suppressing the high-transverse-momentum hadron spectrum in peripheral collisions due to dilute nucleon overlap at large AA impact parameters. By combining this improved initial condition model with a linear Boltzmann transport model for jet-QGP interactions, we obtain a satisfactory description of the centrality dependence of charged hadron suppression in Pb+Pb collisions at TeV.

    nucl-thhep-phnucl-exUniverse(2026)·0 citations
  3. 03

    Theoretical estimates for the synthesis of superheavy nuclei with Ca, Ti, V, and Cr projectiles: effects of reaction values and mass-model dependence

    K. Kawai · Y. Aritomo · K. Nakajima · S. Takagi · N. Nishimura

    Fusion reactions with 48Ca beams, which have been used for synthesis of nuclei, face practical limitations for the synthesis of nuclei with because of the limited availability of suitable target nuclei. We estimate evaporation-residue (ER) cross sections for the reactions 48Ca + 254Es, 50Ti + 249Bk, 51V + 248Cm, and 54Cr + 243Am and examine the role of nuclear-mass-model uncertainties. We employ a hybrid framework for the three stages of the fusion reaction. The capture stage is described by the coupled-channels method, the formation stage by a Langevin approach, and the de-excitation stage by a statistical model. Using the nuclear properties from the FRDM2012 mass model, the maximum values of ER cross section summed over all xn channels are calculated to be 233, 206, 33, and 38 fb for the 48Ca + 254Es, 50Ti + 249Bk, 51V + 248Cm, and 54Cr + 243Am reactions, respectively. The relationship between the reaction Q value and the Coulomb-barrier height is found to be a key factor in comparing reactions leading to the same atomic number. In particular, the relatively small Q value magnitude of the 51V + 248Cm reaction leads to a higher excitation energy and a reduced survival probability, giving the smallest ER cross section among the reactions considered. We also find a significant mass-model dependence on the survival probability. Using the nuclear properties predicted by several mass tables yields differences in the survival probability ranging from about one to several orders of magnitude. This difference mainly originates from the neutron binding energy and shell-correction energy predicted by the nuclear mass models. The ER cross sections for the synthesis of Z = 119 nuclei are governed by both the relative relationship between the reaction Q value and the Coulomb-barrier height and nuclear-mass-model uncertainties that strongly affect the survival probability.

    nucl-thPRC(2026)·0 citations
  4. 04

    Shell effects and the neutron emission within the multi-dimensional Langevin model for nuclear fission

    F.A. Ivanyuk · S.V. Radionov · C. Ishizuka · S. Chiba

    We solve the Langevin equations for the time evolution of parameters that describe the shape of fissioning system. On each integration step, we calculate the probability of neutron emission and estimate whether a neutron would be emitted or not. If yes, we decrease the excitation energy of the nucleus by the neutron separation energy plus the average energy of the emitted neutron, switch to the layer of potential energy surface with a smaller number of neutrons and continue the process of integration. If the trajectory reaches the scission point, we check how many neutrons were emitted along this trajectory. The pre-scission neutron multiplicity is defined by the ratio of the total number of emitted neutrons to the total number of fission trajectories. Besides , the mass distribution of fission fragments, the distribution of emitted neutrons with respect to the fission stage (deformation of system) and the distribution of emitted neutrons with respect to their energies are calculated. The calculated quantities are compared with the available experimental data.

    nucl-th0 citations
  5. 05

    Probing the neutron-skin thickness through photoproduction in ultra-peripheral collisions

    Haoyuan Li🇨🇳 · Lu-Meng Liu🇨🇳 · Jinhui Chen🇨🇳 · Yu-Gang Ma🇨🇳 · Chunjian Zhang🇨🇳

    We study the impact of neutron-skin thickness on photoproduction in ultra-peripheral collisions. Within the Color Glass Condensate framework, we calculate coherent and incoherent cross sections and examine their dependence on the momentum transfer for different neutron-skin thicknesses. We find a clear imprint of the neutron skin on the spectra: a larger neutron skin leads to a smoother and more extended color-density profile, suppressing the coherent cross section at large while enhancing the incoherent cross section through increased event-by-event configurational fluctuations in the nuclear periphery. We further show that the ratio of incoherent to coherent integrated cross sections provides a particularly sensitive and robust observable, with reduced theoretical uncertainties. These results establish diffractive vector-meson photoproduction in ultra-peripheral collisions as a powerful tomographic tool to constrain the neutron-skin thickness and the transverse gluon distribution at the LHC and future Electron-Ion Colliders.

    nucl-thnucl-exChin.Phys.Lett.(2026)·1 citation
  6. 06

    Equation of State for warm Neutron Star outer crusts

    David Barba-González · Conrado Albertus · M. Ángeles Pérez-García

    We describe the equation of state (EoS) of a warm ion plasma as obtained by performing microscopic many-body simulations using Molecular Dynamics computational techniques. Using the cold one-component plasma (OCP) composition in the Neutron Star (NS) outer crust assumed in Murarka et al. (2022) with a representative heavy nucleus for each density, we refine previous calculations. We include electron screening and modeling of ions as finite-size Gaussian distributions in the interaction potential, together with an efficient Ewald energy summation procedure. From this, the EoS relation is obtained as a function of baryonic density and temperature in the NS outer crust under conditions , MeV. In order to improve the usability of our results we provide tabulated data values along with a neural network parametrization available in the Zenodo repository, see https://zenodo.org/records/15348712. We find that even at moderate temperatures, thermal effects of ions are key in the higher density region closer to the inner crust, when described using a thermal effective parametrization based on the thermal adiabatic index . We compare our results with other EoS in the literature performing a critical discussion.

    astro-ph.HEastro-ph.SRnucl-thphysics.plasm-ph0 citations
  7. 07

    Proton induced reactions on 118Sn target at energies up to 18 MeV

    G. H. Hovhannisyan · N.S. Gharibyan · T. M. Bakhshiyan · A. R. Balabekyan · S.V. Gaginyan · G.V. Martirosyan · A. Manukyan · R.K. Dallakyan · A. Aprahamian

    Proton-induced reactions on enriched 118Sn up to 18 MeV have been investigated. Using the stacked-foil activation technique, the excitation functions of the reactions 118Sn(p,n)118Sb, 118Sn(p,2n)117Sb, 118Sn(p,{\alpha})115mIn, and 118Sn(p,x)117mSn were measured. The available experimental data show good agreement with our measurements. The cross sections for the 118Sn(p,x)117mSn and 118Sn(p,{\alpha})115mIn reactions are reported for the first time. The measured cross sections were compared not only with previously published experimental results, but also with theoretical predictions from the TENDL-2023 (TALYS-based evaluated nuclear data library), TENDL-2025 and JENDL-5 (Japanese Evaluated Nuclear Data Library) libraries. Discrepancies between experimental and theoretical data were observed for reactions involving composite-particle emission, such as alpha particles and deuterons. These differences suggest that while current models adequately describe simple two-nucleon emission channels, further refinements are needed, particularly for modeling composite-particle emission at lower proton energies.

    nucl-exnucl-thEPJA(2026)·0 citations

Affiliations

first authorsco-authorsvia INSPIRE