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Topics in Gravitational Physics: Tidal Coupling in Gravitational Wave Searches and Mach’s Principle

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Figure

Figure 3.1 shows the fitted noise strain
Figure 3.2: The ISCO wave frequency as a function of black-hole spin.
Figure 3.3: Square-root of�proportional to the IMRI distance ⟨(S/N)2⟩ for IMRI waves from an inspirling 1.4M⊙ NS at a distanceof 100Mpc as a function of the central black hole’s mass
Table 3.1: Profile of IMRIs in advanced LIGO band. The column “∆wave cycles spent between 10Hz and 10N>10M%” lists the ratio of theM, to the total wave cycles spent in the advanced LIGOband (i.e., from 10Hz to Fisco) [The calculation of is based on Eq
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