I am an astrophysicist studying the evolution of planetary interiors and the dynamics of magnetic fields in neutron stars. During my PhD, I focused on understanding the magnetic field's evolution, its role in radio-emission, and modeling gravitational-wave mountains in neutron stars using numerical simulations. Neutron stars have central densities higher than nuclear matter, making them an ideal laboratory for studying fundamental physics. I performed magnetohydrodynamical simulations of isolated neutron stars to obtain equilibrium magnetic field solutions. In 2022, I transitioned to a postdoctoral position focused on researching solar system planets and exoplanets. As the lead developer of the APPLE Code, a sophisticated stellar evolution code, I integrated accurate physical processes relevant to planets, including convection, radiation, and element diffusion. This code enables detailed studies of the evolution, composition, and internal structure of gas and ice giant planets.