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  • Refinement of an analytical capture cross section formula
    2025, 49(12): 124106-124106-8. doi: 10.1088/1674-1137/adfe53
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    An analytical formula with high accuracy is proposed for a systematic description of the capture cross sections at near-barrier energies from light to superheavy reaction systems. Based on the empirical barrier distribution method, three key input quantities are refined by introducing nuclear surface correction to the Coulomb parameter z for calculating the barrier height, incorporating the reaction Q-value and shell correction into the barrier distribution width calculations, and considering the deep inelastic scattering effects of superheavy systems on the barrier radius. With these refinements, the accuracy of not only the calculated barrier height but also the predicted capture cross sections is substantially improved. The average deviation (in logarithmic scale) between the predicted cross sections and the experimental data for 426 reaction systems with $ 35 < Z_1 Z_2 < 2600 $ is sharply reduced from 3.485 to 0.113.
  • Polarized neutron beams from polarized deuterium-tritium fusion with applications to magnetic field imaging in high-energy-density plasmas
    2025, 49(12): 124102-124102-10. doi: 10.1088/1674-1137/adec4f
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    When the spins of deuteron and triton are aligned in parallel, the fusion cross-section increases by approximately 50%. The emitted neutrons are anisotropic and polarized in specific directions. The polarized neutron beams can be used to measure strong magnetic fields in high-energy-density plasmas, offering a potential alternative to the well-established proton imaging technique. In contrast to protons, neutrons are not deflected by electromagnetic fields and are not sensitive to electric fields, thus reducing the complexity of magnetic field reconstruction. Three-dimensional spin transport hydrodynamics simulations are employed to investigate the polarized neutron beams generated from spin-polarized deuterium-tritium target implosions. Synthetic polarized neutron images of magnetic fields are generated from Monte Carlo simulations. Based on a comparison of the results of finite-size sources and an ideal point source, a method to compensate the finite-source-size blurring effect is proposed to reduce the error in magnetic field reconstruction.
  • $ D^*_{(s)}\to P $ form factors and their applications to semi-leptonic and non-leptonic weak decays
    2025, 49(12): 123104-123104-14. doi: 10.1088/1674-1137/adfb5d
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    Similar to other heavy flavor mesons, the weak decays of $ D^*_{(s)} $ mesons can provide a platform to verify the standard model, explore new physics, and understand the mechanisms of weak interactions. At present, the theoretical and experimental studies on $ D^*_{(s)} $ mesons are relatively limited. In addition to the dominant electromagnetic decays, the $ D^*_{(s)} $ weak decays should be feasible to explore the $ D^*_{(s)} $ mesons. In this study, we used the covariant light-front quark model to study the form factors of the transitions $ D^*_{(s)}\to \pi, K, \eta_{q, s} $, and then calculated the branching ratios of the semi-leptonic decays $ D^*_{(s)}\to P\ell^{+}\nu_{\ell} $ and the non-leptonic decays $ D^*_{(s)}\to PP, PV $ with $ P=\pi, K, \eta^{(\prime)}, $$ V=\rho, K^*, \phi $, and $ \ell=e, \mu $. The channels $ D_{s}^{*+}\to\eta \ell^{+}\nu_{\ell} $ and $ D^{*+}_{s}\to \eta\rho^{+} $ possess the largest branching ratios, which can reach an order of $ 10^{-6} $ among these decays, and are most likely to be accessible in experiments at future high-luminosity colliders. Furthermore, we predict and discuss the longitudinal polarization fraction $ f_{\rm L} $ and the forward-backward asymmetry $ A_{\rm FB} $ for the considered semi-leptonic $ D^*_{(s)} $ decays.
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ISSN 1674-1137 CN 11-5641/O4

Original research articles, Ietters and reviews Covering theory and experiments in the fieids of

  • Particle physics
  • Nuclear physics
  • Particle and nuclear astrophysics
  • Cosmology
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