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| The detection of gravitational waves from binary black hole mergers enables us to observe the behavior of spacetimes in the strong-field, highly dynamical regime. The LIGO–Virgo–KAGRA collaboration has now observed hundreds of such events, offering several exciting candidates with differing properties. In this talk I will discuss recent results using these gravitational wave observations to test general relativity and probe the spacetime near black holes. I will present the first confident detection of an overtone in the ringdown signal during the postmerger phase of the binary black hole signal. I will also discuss the “direct wave” signal, a recently proposed model for the merger portion of the waveform that depends on the physics close to the black hole horizon. Finally, I will present the first results from applying this model to real data, using it to analyze the loudest gravitational wave event ever detected. |
Luis Lehner