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

Open Access

Fig. 9.

Time evolution of the kinetic energy for the nonlinear simulations of ₁g and ₂g modes compared to the linear results (dashed red lines). The lines above correspond to the ₁g mode with $\hat{ω} = 0.348 N$ $\hat{\omega}=0.348 N$ . The lines below correspond to the ₂g− mode with $\hat{ω} = 0.186 N$ $\hat{\omega}= 0.186 N$ , which are rescaled by a factor of 0.1 for improved visibility.

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