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    <responseDate>2026-10-12T00:35:35Z</responseDate>
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    <identifier>10.57760/sciencedb.j00186.00910</identifier>
    <datestamp>2026-04-09T20:43:02Z</datestamp>
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  <dc:date>2026-04-09</dc:date>
  <dc:title>Data of Effect of tensor force on octupole deformation in neutron-rich Ba isotopes within the Skyrme-Hartree-Fock framework</dc:title>
  <dc:identifier>doi:10.57760/sciencedb.j00186.00910</dc:identifier>
  <dc:language>en</dc:language>
  <dc:description>All data in this dataset are generated using the open‑source code Skyax, which solves the nuclear Skyrme&amp;ndash;Hartree&amp;ndash;Fock equations in coordinate space under the assumption of axial symmetry. The calculations employ the [specify Skyrme parametrization, e.g., SLy5, SMAi, TIJ, and so on ] energy density functional. Pairing correlations are treated within the BCS approximation. Reflection symmetry is broken, so octupole deformations are explicitly included. Constrained calculations are performed in the (&amp;beta;2,&amp;beta;3) plane: &amp;beta;2 is varied from &amp;minus;0.5 to 0.5 with a step of 0.05, and &amp;beta;3 from 0 to 0.5 with a step of 0.05. At each deformation point, convergence is achieved when the variation of the total energy is below 10&amp;minus;6 MeV and the multipole moments are stable to within 10&amp;minus;3 b. Numerical discretization uses a cylindrical grid with mesh sizes dz=dr=0.6 fm and grid points nz=nr=50, corresponding to a box of size z_max&amp;asymp;r_max&amp;asymp;30 fm.The dataset is organised into folders, each corresponding to a specific figure in the associated article. For figures that involve a small number of deformation points, the full Skyax output files (including densities, single‑particle energies, and multipole moments) are provided in plain text format. For figures with a large number of deformation points (e.g., potential energy surfaces over a dense grid), the raw output files are not uploaded due to their size. Instead, each such folder contains:the input file (*.in) that fully specifies the calculation,and a job submission script (for the SLURM/PBS/Torque queuing system) that reproduces all individual runs.The user can therefore regenerate every data point by running the provided script on a compatible computing cluster. No data are missing; all results are fully reproducible via the provided input files.No experimental uncertainties apply because this is a purely computational dataset. Numerical errors arising from the finite grid and iteration convergence are estimated to be below 0.01 MeV for binding energies and below 0.005 for deformation parameters &amp;beta;2 and &amp;beta;3, as verified by grid‑refinement tests (e.g., using dz=dr=0.4 fm for selected nuclei). The dataset contains no missing entries.The Skyax code is freely available at&amp;nbsp;10.1016/j.cpc.2020.107603. The executable provided is compiled for Linux; users may also compile the source code themselves using the included Makefile.</dc:description>
  <dc:subject>Octupole deformation; Tensor-force effects; Shell-structure evolution; Skyrme energy density functiona; Spin-orbit splittings</dc:subject>
  <dc:creator>Xian-Rong Zhou</dc:creator>
  <dc:creator>Huai-Tong Xue</dc:creator>
  <dc:rights>PUBLIC</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by/4.0/</dc:rights>
  <dc:type>dataset</dc:type>
  <dc:publisher>Science Data Bank</dc:publisher>
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