Nonlinear saturation of gravito-inertial modes excited by tidal resonances in binary neutron stars

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Fig. 6.

Power and dissipation balance of the tidally excited fluid motions as a function of the tidal forcing frequency, $\hat{ω}$ $\hat{\omega}$ , with the split formulation of the tidal forcing with N/Ω_s = 3.24. Similar to Fig. 3, the pure g-mode frequency (Eq. (33)) is designated by crosses.

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