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Future Prospects for Probing Scalar-Tensor Theories with Gravitational Waves from Mixed Binaries
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The extreme-gravity collisions of binaries with one black hole and one neutron star provide for excellent tests of general relativity. We here study how well one can constrain theories beyond general relativity with additional scalar fields that allow for spontaneous scalarization of neutron stars, and those motivated from string theory. We find that existing bounds can be improved with current gravitational-wave detectors if the black hole mass is sufficiently small. Bounds will further improve by many orders of magnitude with future detections, especially by combining multiple events.
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Cited by 2 Pith papers
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Lorentz-violating matter-gravity couplings in small-eccentricity binary pulsars
Using three small-eccentricity relativistic binary pulsars, this paper obtains order-of-magnitude upper limits on SME matter-gravity coefficients for neutrons, protons, and electrons.
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Parameterized and Consistency Tests of Gravity with Gravitational Waves: Current and Future
A review of ppE and IMR consistency tests of GR with GWs, forecasting that future multi-band detectors can improve bounds on modified gravity by orders of magnitude.
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