SVP data and codes
These data (for C, N, O, Ne, Na, Mg, Al, Si, S, Ar, Ca and Fe) and codes have been first released in 2020, and are discussed by Alecian & LeBlanc, 2020 (MNRAS). The new version (November 2024) contains several improvements in the codes, the SVP data have not changed. A new release of the SVP data is planned for 2025.
Instructions to use the codes and data (content of the READme file).
To install the standalone code with the data needed to compute radiative accelerations, download the following file:
svp_standalone_nov24.tar.gz
This package includes the codes and data necessary for the implementation of the SVP method in stellar evolution programs.
It is recommended to update the 2020 version by this new version (November 2024). Changes are detailed in the READme file.
The figures showing calculated radiative accelerations for all elements and all models mentionned in Alecian & LeBlanc (2020), are gathered in the following tar.gz:
g_rad_vs_Teff.tar.gz
Some tables of SVP parameters for particular stellar models are also available here.
See also comparisons of radiative accelerations obtained with other methods [by Hui-Bon-Hoa (2024)].
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Update: November 2024