Built on

M. S. Santos et al., First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy Survey Galaxies and the LIGO/Virgo Binary–Black-hole Merger GW170814, Astrophys. J
Original
1901
Earlier work this paper cites.
M. Lagos, M. Fishbach, P. Landry and D. E. Holz, Standard sirens with a running Planck mass, Phys. Rev. D
Original
1901
Earlier work this paper cites.
J. Z. Qi et al., Testing the Etherington distance duality relation at higher redshifts: Combined radio quasar and gravitational wave data, Phys. Rev. D
Original
1902
Earlier work this paper cites.
X. Fu, L. Zhou and J. Chen, Testing the cosmic distance-duality relation from future gravitational wave standard sirens, Phys. Rev. D
Original
1903
Earlier work this paper cites.
W. Yang, S. Pan, E. Di Valentino, B. Wang and A. Wang, Forecasting Interacting Vacuum-Energy Models using Gravitational Waves
Original
1904
Earlier work this paper cites.
S. Capozziello, R. D’Agostino and O. Luongo, Extended gravity cosmography, Int. J. Mod. Phys. D
Original
1904
Earlier work this paper cites.
W. Yang et al., Listening to the sound of dark sector interactions with gravitational wave standard sirens, JCAP
Original
1905
Earlier work this paper cites.
R. C. Nunes, M. E. S. Alves and J. C. N. de Araujo, Forecast constraints on f(T) gravity with gravitational waves from compact binary coalescences, Phys. Rev. D
Original
1905
Earlier work this paper cites.
C. Dalang and L. Lombriser, Limitations on Standard Sirens tests of gravity from screening, JCAP
Original
1906
Earlier work this paper cites.
X. Gao and X. Y. Hong, Propagation of the gravitational waves in a cosmological background
Original
1906
Earlier work this paper cites.
J. F. Zhang, H. Y. Dong, J. Z. Qi and X. Zhang, Prospect for constraining holographic dark energy with gravitational wave standard sirens from the Einstein Telescope
Original
1906
Earlier work this paper cites.
E. Belgacem et al., Testing modified gravity at cosmological distances with LISA standard sirens, JCAP
Original
1906
Earlier work this paper cites.
X. Gao and X. Y. Hong, Propagation of the gravitational waves in a cosmological background
Original
1906
Earlier work this paper cites.
Z. Carson, B. C. Seymour and K. Yagi, Future Prospects for Probing Scalar-Tensor Theories with Gravitational Waves from Mixed Binaries
Original
1907
Earlier work this paper cites.
E. Belgacem, Y. Dirian, A. Finke, S. Foffa and M. Maggiore, Nonlocal gravity and gravitational-wave observations, JCAP
Original
1907
Earlier work this paper cites.
R. D’Agostino and R. C. Nunes, Probing observational bounds on scalar-tensor theories from standard sirens, Phys. Rev. D
Original
1907
Earlier work this paper cites.
E. Belgacem et al., Cosmology and dark energy from joint gravitational wave-GRB observations, JCAP
Original
1907
Earlier work this paper cites.
G. Calcagni et al., Quantum gravity and gravitational-wave astronomy, JCAP
Original
1907
Earlier work this paper cites.
D. Jeong and M. Kamionkowski, Gravitational waves, CMB polarization, and the Hubble tension
Original
1908
Earlier work this paper cites.
W. J. Wolf and M. Lagos, Standard Sirens as a novel probe of dark energy
Original
1910
Earlier work this paper cites.
Z. Carson and K. Yagi, Parameterized and inspiral-merger-ringdown consistency tests of gravity with multi-band gravitational wave observations
Original
1911
Earlier work this paper cites.
C. Dalang, P. Fleury and L. Lombriser, Horndeski and the Sirens
Original
1912
Earlier work this paper cites.
J. B. Jimenez, J. M. Ezquiaga and L. Heisenberg, Probing cosmological fields with gravitational wave oscillations
Original
1912
Earlier work this paper cites.
C. Dalang, P. Fleury and L. Lombriser, Horndeski and the Sirens
Original
1912
Earlier work this paper cites.
G. W. Horndeski, Second-order scalar-tensor field equations in a four-dimensional space, Int. J. Theor. Phys
1974
Earlier work this paper cites.
B. F. Schutz, Determining the Hubble constant from gravitational wave observations, Nature
1986
Earlier work this paper cites.
L. Amendola, Cosmology with nonminimal derivative couplings, Phys. Lett. B
1993
Earlier work this paper cites.
W. H. Press, S. A. Teukolsky, W. T. Vetterling and B. P. Flannery, Numerical Recipes
1994
Earlier work this paper cites.
N. Seto, S. Kawamura and T. Nakamura, Possibility of Direct Measurement of the Acceleration of the Universe Using 0.1 Hz Band Laser Interferometer Gravitational Wave Antenna in Space, Phys. Rev. Lett
2001
Earlier work this paper cites.
W. Yang, S. Pan, D. F. Mota and M. Du, Forecasting Dark-Energy Anisotropic Stress using gravitational-waves
Original
2001
Earlier work this paper cites.

Similar

M. Lagos and H. Zhu, Gravitational couplings in Chameleon models
Original
2003
Cited alongside, same era.
D. E. Holz and S. A. Hughes, Using Gravitational-Wave Standard Sirens, Astrophys. J
2005
Cited alongside, same era.
C. Gordon, K. Land and A. Slosar, Cosmological Constraints from Type Ia Supernovae Peculiar Velocity Measurements, Phys. Rev. Lett
Original
2007
Cited alongside, same era.
M. Punturo et al., The third generation of gravitational wave observatories and their science reach, Class. Quant. Grav
2009
Cited alongside, same era.
C. Cutler and D. E. Holz, Ultrahigh precision cosmology from gravitational waves, Phys. Rev. D
Original
2009
Cited alongside, same era.

Then

J. M. Ezquiaga and M. Zumalacárregui, Dark Energy After GW170817: Dead Ends and the Road Ahead, Phys. Rev. Lett
Original
2017
Later among the works it cites.
D. Bettoni, J. M. Ezquiaga, K. Hinterbichler and M. Zumalacarregui, Speed of gravitational waves and the fate of scalar-tensor gravity, Phys. Rev. D
Original
2017
Later among the works it cites.
H. Audleyet et al., Laser Interferometer Space Antenna
Original
2017
Later among the works it cites.
R. G. Cai and T. Yang, Estimating cosmological parameters by the simulated data of gravitational waves from the Einstein Telescope, Phys. Rev. D
Original
2017
Later among the works it cites.
J. Gleyzes, Parametrizing modified gravity for cosmological surveys, Phys. Rev. D

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Reading the bibliography…

2019

Forecasts on the speed of gravitational waves at high $z$

Bonilla, Alexander, D'Agostino, Rocco, Nunes, Rafael C. et al.

Understand

The observation of GW170817 binary neutron star (BNS) merger event has imposed strong bounds on the speed of gravitational waves (GWs) locally, inferring that the speed of GWs propagation is equal to the speed of light.

Current GW detectors in operation will not be able to observe BNS merger to long cosmological distance, where possible cosmological corrections on the cosmic expansion history are expected to play an important role, specially for investigating possible deviations from general relativity.
Future GW detectors designer projects will be able to detect many coalescences of BNS at high $z$, such as the third generation of the ground GW detector called Einstein Telescope (ET) and the space-based detector deci-hertz interferometer gravitational wave observatory (DECIGO).
In this paper, we relax the condition $c_T/c = 1$ to investigate modified GW propagation where the speed of GWs propagation is not necessarily equal to the speed of light.