A Two-stage Formalism for Common-envelope Phases of Massive Stars

We propose a new simple formalism to predict the orbital separations after common-envelope phases with massive-star donors. We focus on the fact that massive red supergiants tend to have a sizable radiative layer between the dense helium core and the convective envelope. Our formalism treats the common-envelope phase in two stages: dynamical inspiral through the outer convective envelope and thermal timescale mass transfer from the radiative intershell. With fiducial choices of parameters, the new formalism typically predicts much wider separations compared to the classical energy formalism. Moreover, our formalism predicts that final separations strongly depend on the donor evolutionary stage and companion mass. Our formalism provides a physically motivated alternative option for population synthesis studies to treat common-envelope evolution. This treatment will impact predictions for massive-star binaries, including gravitational-wave sources, X-ray binaries, and stripped-envelope supernovae.