Figure 30

Figure 30: Left: Schematic figure of the type-I gravitational-wave spectrum for a high-frequency side with different values of the BH spin but for the same masses of BH and NS, and NS EOS. With increase of the BH spin, the cutoff frequency decreases and the amplitude below the cutoff frequency increases. Right: Three types of the gravitational-wave spectrum. Type-I (i) and type-II (ii) are the same as those shown in Figure 27. Type-III (iii) is shown for the case in which the BH spin is high and the mass ratio (and thus the area of the BH horizon) is large. The filled and open circles denote the cutoff frequencies associated with tidal disruption and with a QNM, respectively.