Figure 26

Figure 26: Spectra of gravitational waves from BH-NS binaries for Q = 2, a = 0, and MNS = 1.35M ⊙ with various EOS. The bottom axis denotes the normalized dimensionless frequency f m (= Gf m ∕c3) 0 0 and the left axis the normalized amplitude c2f &tidle;h(f)D ∕Gm 0. The top axis denotes the physical frequency f in Hz and the right axis the effective amplitude &tidle; fh(f ) observed at a distance of 100 Mpc from the binaries. The short-dashed sloped line plotted in the upper left region denotes a planned noise curve of Advanced-LIGO [2] optimized for 1.4M ⊙ NS-NS inspiral detection (“Standard”), the long-dashed slope line denotes a noise curve optimized for burst detection (“Broadband”) and the dot-dashed slope line plotted in the lower right region denotes a planned noise curve of the Einstein Telescope (“ET”) [91, 92]. The upper transverse dashed line is the spectrum derived by the quadrupole formula and the lower one is the spectrum derived by the Taylor-T4 formula, respectively. This figure is taken from [107].