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Testing Lorentz invariance by binary black holes

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Academic year: 2021

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Figure 1.1 – Comparison between the orbital decay prediction for PSR B1913+16, using general relativity (in solid line), and the measured orbital decay (in points)
Figure 1.2 – Scheme of the optical layout for the LIGO interferometers. Figure extracted from [21].
Figure 1.3 – Reconstructed waveform h(t) for the detection of GW150914 in Livingston (left) and Hanford (right)
Figure 1.4 – The average spectral noise sensitivity of the Advanced LIGO detectors mea- mea-sured in order to determine the significance of GW150914
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