Figure 26: Spectra of gravitational waves from BH-NS binaries for , , and
with various EOS. The bottom axis denotes the normalized dimensionless frequency
and the left axis the normalized amplitude . The top axis
denotes the physical frequency in Hz and the right axis the effective amplitude 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 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].
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