Rotational evolution of a CB planet with the CTL model of Mignard (1979) (Eq. (29)). The initial conditions were taken from Table 1, with the exception of the initial planetary eccentricity (e₂ (0) = 0.05 in the upper panel and e₂(0) = 0.15 in the bottom panel). Full-line curves indicate the results of filtered numerical integration: excluding the cross tides (in yellow) and considering the full expression (in magenta). Dashed-line curves represent the results of different analytical models: our previous CTL tidal model (Zoppetti et al. 2019) in brown, and the results of the analytical creep tidal model presented in Eq. (16) of this work, expanded up to second-order in α and considering the gaseous limit (γ₂ ≫ n₁, n₂), are shown in grey.