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- W2611745797 abstract "The recent LIGO detection of gravitational waves from black-hole binaries offers the exciting possibility of testing gravitational theories in the previously inaccessible strong-field, highly relativistic regime. While the LIGO detections are so far consistent with the predictions of General Relativity, future gravitational-wave observations will allow us to explore this regime to unprecedented accuracy. One of the generic predictions of theoriesof gravity that extend General Relativity is the violation of the strong equivalence principle, i.e. strongly gravitating bodies such as neutron stars and black holes follow trajectories that depend on their nature and composition. This has deep consequences for gravitational-wave emission, which takes place with additional degrees of freedom besides the tensor polarizations of General Relativity. I will briefly review the formalism needed to describe these extra emission channels, and show that binary black-hole observations probe a set of gravitational theories that are largely disjoint from those that are testable with binary pulsars or neutron stars." @default.
- W2611745797 created "2017-05-12" @default.
- W2611745797 creator A5049026088 @default.
- W2611745797 date "2017-11-22" @default.
- W2611745797 modified "2023-10-14" @default.
- W2611745797 title "Testing the strong equivalence principle with gravitational-wave observations of binary black holes" @default.
- W2611745797 doi "https://doi.org/10.22323/1.294.0029" @default.
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