Figure 23

Figure 23: Gravitational waveforms observed along the axis perpendicular to the orbital plane for Q = 3 and a = 0 with very stiff (2H), stiff (H), moderate (HB), and soft (B) EOS. The simulation was performed by the KT group. The solid and dashed curves denote the numerical results and results derived by the Taylor-T4 formula. D is the distance from the source and m = M + M 0 BH NS. The left and right axes show the normalized amplitude (2 cDh ∕Gm0) and physical amplitude for D = 100 Mpc, respectively. This figure is taken from [107].