Solar models using OPLIB monochromatic opacities

Opacity is a key ingredient in describing the transport of energy in stars. There are several methods for calculating stellar opacities, resulting in different tables (OPAL, OP, OPAS, and OPLIB). These opacities are available in two distinct forms: tables that regroup the Rosseland mean opacity pre-calculated at predefined chemical mixtures, and monochromatic opacity spectra of individual chemical elements, which allow for the computation of Rosseland mean opacity for a precise mixture. This study presents our implementation of the OPLIB monochromatic opacity data in Cesam2k20 and compares the solar-calibrated model obtained with these opacities to helioseismic data in order to evaluate the improvements made by using monochromatic opacities. We implemented the OPLIB monochromatic opacity data in the Cesam2k20 stellar evolution code following the method already used for the OP monochromatic opacity data. We found that calibrated solar models produced with monochromatic opacity data (OP and OPLIB) agree better overall with helioseismic constraints than those produced with pre-calculated opacity tables.