Proposed space-based gravitational-wave detectors such as BBO and DECIGO can detect ~ 106 neutron star (NS) binaries and determine the luminosity distance to the binaries with high precision. Combining the luminosity distance and electromagnetically derived redshift, one would be able to probe cosmological expansion out to high redshift. In this paper, we show that the Hubble parameter as a function of redshift can be directly measured with monopole and dipole components of the luminosity distance on the sky. As a result, the measurement accuracies of the Hubble parameter in each redshift bin up to z=1 are 3-14%, 1.5-8%, and 0.8-4% for the observation time 1 yr, 3 yr, and 10 yr, respectively
On 17 August 2017, the Advanced LIGO and Virgo detectors observed the gravitational-wave event GW170...
The intrinsic peak luminosity of Type Ia supernovae (SNIa) depends on the value of Newton's gravitat...
The observation of binary neutron star merger GW170817, along with its optical counterpart, provided...
The joint observation of the gravitational-wave and electromagnetic signal from the binary neutron-s...
Precision cosmology is crucial to understand the different energy components in the Universe and the...
Recent observations have accumulated compelling evidence that some short gamma-ray bursts (SGRBs) ar...
Gravitational waves emitted during the coalescence of binary neutron star systems are self- calibrat...
Observations of the gravitational radiation from well-localized, inspiraling compact-object binaries...
Gravitational waves (GWs) from compact binary stars at cosmological distances are promising and powe...
Inspiraling compact binaries as standard sirens will become an invaluable tool for cosmology when we...
Recent observations support the hypothesis that a large fraction of "short-hard" gamma-ray bursts (S...
Inspiraling compact binaries as standard sirens will become an invaluable tool for cosmology when we...
We develop a method for implementing a proposal on utilizing knowledge of neutron star (NS) equation...
Gravitational waves (GWs) from compact binary coalescences encode the absolute luminosity distances ...
We investigate a novel approach to measuring the Hubble constant using gravitational-wave (GW) signa...
On 17 August 2017, the Advanced LIGO and Virgo detectors observed the gravitational-wave event GW170...
The intrinsic peak luminosity of Type Ia supernovae (SNIa) depends on the value of Newton's gravitat...
The observation of binary neutron star merger GW170817, along with its optical counterpart, provided...
The joint observation of the gravitational-wave and electromagnetic signal from the binary neutron-s...
Precision cosmology is crucial to understand the different energy components in the Universe and the...
Recent observations have accumulated compelling evidence that some short gamma-ray bursts (SGRBs) ar...
Gravitational waves emitted during the coalescence of binary neutron star systems are self- calibrat...
Observations of the gravitational radiation from well-localized, inspiraling compact-object binaries...
Gravitational waves (GWs) from compact binary stars at cosmological distances are promising and powe...
Inspiraling compact binaries as standard sirens will become an invaluable tool for cosmology when we...
Recent observations support the hypothesis that a large fraction of "short-hard" gamma-ray bursts (S...
Inspiraling compact binaries as standard sirens will become an invaluable tool for cosmology when we...
We develop a method for implementing a proposal on utilizing knowledge of neutron star (NS) equation...
Gravitational waves (GWs) from compact binary coalescences encode the absolute luminosity distances ...
We investigate a novel approach to measuring the Hubble constant using gravitational-wave (GW) signa...
On 17 August 2017, the Advanced LIGO and Virgo detectors observed the gravitational-wave event GW170...
The intrinsic peak luminosity of Type Ia supernovae (SNIa) depends on the value of Newton's gravitat...
The observation of binary neutron star merger GW170817, along with its optical counterpart, provided...