Extreme gravity tests with gravitational waves from compact binary coalescences: (I) inspiral–merger
Abstract
The observation of the inspiral and merger of compact binaries by the LIGO/Virgo collaboration ushered in a new era in the study of strong-field gravity. We review current and future tests of strong gravity and of the Kerr paradigm with gravitational-wave interferometers, both within a theory-agnostic framework (the parametrized post-Einsteinian formalism) and in the context of specific modified theories of gravity (scalar–tensor, Einstein–dilaton–Gauss–Bonnet, dynamical Chern–Simons, Lorentz-violating, and extra dimensional theories). In this contribution we focus on (i) the information carried by the inspiral radiation, and (ii) recent progress in numerical simulations of compact binary mergers in modified gravity.
Keywords
Modified gravity Gravitational waves Compact binary systemsNotes
Acknowledgements
E.B. was supported by NSF Grants Nos. PHY-1607130 and AST-1716715. N.Y. acknowledges support through the NSF CAREER Grant PHY-1250636 and NASA Grants NNX16AB98G and 80NSSC17M0041.
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