Different components appearing in the dissipation of the dynamical tide (Eq. (13)) as a function of stellar age. The change in radius of the radiative-convective boundary is represented in blue, the change in stellar mass in orange, the change in local density at the boundary in green, the change in tidal forcing compared to changes in the stellar radius in red, and change in the derivative of the Brunt-Väisälä frequency in purple. Stellar evolutionary phases (PMS to WD) are indicated.