Testing stellar evolution models with a stable mass transfer in the evolution of Algols

In this study, we investigate the stellar evolution models using the open-source software instrument Modules for Experiments in Stellar Astrophysics to study the mass and angular momentum loss in the evolution of Algols. We examine the stability of mass transfer in these systems by the physical principle of Roche lobe overflow. Also, we have investigated the ongoing challenge of chemical mixing and exhibit improvements that allow for the simulation of orbital and stellar parameters via gravitational radiation and magnetic braking.