A comparison of the dynamical and model-derived parameters of the pulsating eclipsing binary KIC 9850387

We aim to unravel the interior mixing profile of pulsating eclipsing binary KIC9850387 by comparing its dynamical parameters and derived through a combination evolutionary asteroseismic modelling. created grid stellar models using code \textsc{mesa} performed an isochrone-cloud (isocloud) based modelling system. then generated pulsational pulsation \textsc{gyre} on age constraints from Finally, we observed $\ell=1$ $\ell=2$ period-spacing patterns, utilising different combinations observational constraints, merit functions, observables obtain strong properties primary star. Through found that system comprises two main-sequence components at $1.2\pm0.1$ Gyr. also provided stronger than Overall, high levels posited this is result intrinsic non-tidal mechanisms due similar behaviour in single stars. investigated high-frequency regime evidence surface effect as well rotational splitting form prograde-retrograde dipole g$_{1}$ mode doublet with missing zonal mode. find extracted patterns are only barely compliant, reinforcing need for homogeneous analyses samples binaries calibrating profiles.