Extreme gravity tests with gravitational waves from compact binary coalescences: (I) inspiral–merger

Editor’s Choice (Review Article)
Part of the following topical collections:
  1. Testing the Kerr spacetime with gravitational-wave and electromagnetic observations

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 systems 

Notes

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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© Springer Science+Business Media, LLC, part of Springer Nature 2018

Authors and Affiliations

  1. 1.Department of Physics and AstronomyThe University of MississippiUniversityUSA
  2. 2.Department of PhysicsUniversity of VirginiaCharlottesvilleUSA
  3. 3.Department of Physics, eXtreme Gravity InstituteMontana State UniversityBozemanUSA

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