1.7 M_⊙ stellar model at X_c = 0.5 with f_rot,s = 1 d⁻¹ and δf = 0.0 (light grey), 0.4 (grey), and 0.8 (black), and the corresponding pulsations with (k, m)=(−1, −1). Top left panel: Brunt-Väisälä frequency profile. Middle left panel: considered stellar rotation profiles. Bottom left panel: period spacing patterns computed with GYRE v5.1 for the different rotation profiles. Right panel: the integrand of Eq. (3) (top) and the rotation kernel (bottom) for the pulsation mode with (n, k, m)=(−35, −1, −1).