Lindblad resonance
= Lindblad resonance
{c}
{title2=$m(\Omega-\Omega_p)=\pm\kappa$}
A rotating gravitational perturbation drives an epicyclic disk response where $m(\Omega-\Omega_p)=\pm\kappa$. The launched <density> waves carry <angular momentum>. For a <planet>, inner and outer waves exert torques of opposite signs, and their imbalance contributes to migration.