Titlebook: Handbook of Gravitational Wave Astronomy; Cosimo Bambi,Stavros Katsanevas,Konstantinos D. Ko Living reference work 20200th edition Gravit

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Black Hole-Neutron Star Mergers,tiple binary black hole and binary neutron star systems have been detected, and while we are still waiting for the first confirmed observation of a mixed black hole-neutron star (BHNS) merger, a number of candidate events have been announced over the last observing run of the LIGO-Virgo Collaboratio

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Black-Hole Superradiance: Searching for Ultralight Bosons with Gravitational Waves,ce. This phenomenon is ubiquitous in many physical systems and also occurs for spinning black holes and stars, with far-reaching consequences for gravitational-wave astronomy and searches for new physics with astrophysical compact objects. In particular, ultralight bosonic fields (predicted in a var

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CMB Experiments and Gravitational Waves,sistencies in observations of the universe, including the thermal equilibrium of the CMB at otherwise super-horizon scales, and the observed spatial flatness of the universe. Inflation would expand space by at least 60 e-folds in 10. s in order to explain the observed flatness and homogeneity of the

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Effective Field Theory Methods to Model Compact Binaries,gravitational wave detections from compact binary coalescences will demand even more accurate description of the source dynamics as the sensitivity of detectors increases over years. The analytic modeling of classical gravitational dynamics has been enriched over the last decade of powerful methods

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Emission of Gravitational Radiation in Scalar-Tensor and f(R)-Theories,heories of gravity in the strong field regime. Such tests rely sensitively on the phase evolution of the gravitational waves, which is controlled by the energy momentum carried by such waves out of the system. The weak-field limit of alternative metric theories shows new aspects of gravitation which

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