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

Open Access

Fig. 8.

₃g-mode resonance with $\hat{ω} = 0.126 N$ $\hat{\omega}=0.126 N$ at ϕ = 0 in the case of small rotation (N/Ω_s = 3.24). Results of the linear code are shown on the left, while that of the nonlinear code are on the right; notice the difference in the color bar for each panel.

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