Speaker
Description
The formation and orbital evolution of giant planets are strongly influenced by the physical properties and dynamical evolution of their protoplanetary disks. In this work, we investigate giant planet formation and migration in protoplanetary disks evolving under the combined effects of viscous accretion and magnetically driven disk winds. We adopt an analytical disk model to describe the time evolution of the gas surface density and temperature, coupled with prescriptions for planetary gas accretion, gap opening, and migration driven by planet–disk gravitational interactions. We employ the Kanagawa migration model to account for the reduction of migration torques associated with planetary gap opening, providing a continuous description of migration from low-mass planets to gap-opening giant planets. We examine how disk viscosity, magnetically driven winds, and the evolving gas distribution influence planetary growth and orbital evolution. Our aim is to understand how the relative contributions of viscous accretion and magnetically driven disk winds to disk evolution affect the growth, migration, and final orbital distribution of giant planets.