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Mitigating Noise in Interferometric Gravitational Wave Detectors

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Figure

Figure 1.1: The two orthogonal gravitational wave polarization modes, h+ and h×,as a function of phase
Figure 2.1: Illustration of a gravitational wave’s effect on the orthogonal arms of aMichelson interferometer.
Figure 2.2: A Michelson interferometer with Fabry-Pérot arm cavities. Labeledare the input test masses (ITMs), end test masses (ETMs), and the beamsplitter(BS).
Figure 2.4: A Michelson interferometer with Fabry-Pérot arm cavities and powerrecycling
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