Kavli Affiliate: Lile Wang |Summary:Binary black holes (BBHs) in gaseous medium, such as active galactic nucleus (AGN) disks, are important gravitational-wave sources, yet the gas-driven torque that governs their orbital evolution remains to be fully understood. Most existing studies of BBHs in gas often approximate the net torque as the sum of independent dynamical friction […]
Continue.. From Inspiral to Expansion: The Wake-Driven Torque on Binary Black Holes in Gaseous Medium