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We analyze the propagation of high-frequency gravitational waves (GW) in scalar-tensor theories of gravity, with the aim of examining properties of cosmological distances as inferred from GW measurements.
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2003
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R. Takahashi and T. Nakamura, “Wave effects in gravitational lensing of gravitational waves from chirping binaries,” Astrophys. J
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J.-P. Macquart, “Scattering of gravitational radiation: Second order moments of the wave amplitude,” Astron. Astrophys
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N. Seto, “Strong gravitational lensing and localization of merging massive black hole binaries with LISA,” Phys. Rev
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T. Pyne and M. Birkinshaw, “The luminosity distance in perturbed flrw spacetimes,” Mon. Not. Roy. Astron. Soc
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D. E. Holz and S. A. Hughes, “Using gravitational-wave standard sirens,” Astrophys. J
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L. Lombriser and A. Taylor, “Breaking a Dark Degeneracy with Gravitational Waves,” JCAP
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M. Crisostomi, K. Koyama, and G. Tasinato, “Extended Scalar-Tensor Theories of Gravity,” JCAP
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T. Baker and M. Trodden, “Multimessenger time delays from lensed gravitational waves,” Phys. Rev
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K. Kyutoku and N. Seto, “Gravitational-wave cosmography with LISA and the Hubble tension,” Phys. Rev
2017
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H. Chen, “Distance measures in gravitational-wave astrophysics and cosmology,” Class. Quant. Grav
2021
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