Inspiraling compact binaries as standard sirens will become an invaluable tool for cosmology when we enter the gravitational-wave detection era. However, a degeneracy in the information carried by gravitational waves between the total rest-frame mass M and the redshift z of the source implies that neither can be directly extracted from the signal; only the combination M(1+z), the redshifted mass, can be directly extracted from the signal. Recent work has shown that for third-generation detectors, a tidal correction to the gravitational-wave phase in the late-inspiral signal of binary neutron star systems can be used to break the mass-redshift degeneracy. Here, we propose to use the signature encoded in the postmerger signal allowing the acc...
We present a robust method to characterize the gravitational wave emission from the remnant of a neu...
We present a robust method to characterize the gravitational wave emission from the remnant of a neu...
The observation of binary neutron star merger GW170817, along with its optical counterpart, provided...
Inspiraling compact binaries as standard sirens will become an invaluable tool for cosmology when we...
Inspiraling compact binaries as standard sirens will become an invaluable tool for cosmology when we...
Precision cosmology is crucial to understand the different energy components in the Universe and the...
Gravitational waves emitted during the coalescence of binary neutron star systems are self-calibrati...
We investigate a novel approach to measuring the Hubble constant using gravitational-wave (GW) signa...
Finite-size effects on the gravitational wave signal from a neutron star merger typically manifest a...
Recent observations support the hypothesis that a large fraction of "short-hard" gamma-ray bursts (S...
Detection of gravitational waves from the inspiral phase of binary neutron star coalescence will all...
A recent study has shown that redshift information can be directly extracted from gravitational wave...
Gravitational wave astronomy has established its role in measuring the equation of state governing c...
A recent study has shown that redshift information can be directly extracted from gravitational wave...
Proposed space-based gravitational-wave detectors such as BBO and DECIGO can detect ~ 106 neutron st...
We present a robust method to characterize the gravitational wave emission from the remnant of a neu...
We present a robust method to characterize the gravitational wave emission from the remnant of a neu...
The observation of binary neutron star merger GW170817, along with its optical counterpart, provided...
Inspiraling compact binaries as standard sirens will become an invaluable tool for cosmology when we...
Inspiraling compact binaries as standard sirens will become an invaluable tool for cosmology when we...
Precision cosmology is crucial to understand the different energy components in the Universe and the...
Gravitational waves emitted during the coalescence of binary neutron star systems are self-calibrati...
We investigate a novel approach to measuring the Hubble constant using gravitational-wave (GW) signa...
Finite-size effects on the gravitational wave signal from a neutron star merger typically manifest a...
Recent observations support the hypothesis that a large fraction of "short-hard" gamma-ray bursts (S...
Detection of gravitational waves from the inspiral phase of binary neutron star coalescence will all...
A recent study has shown that redshift information can be directly extracted from gravitational wave...
Gravitational wave astronomy has established its role in measuring the equation of state governing c...
A recent study has shown that redshift information can be directly extracted from gravitational wave...
Proposed space-based gravitational-wave detectors such as BBO and DECIGO can detect ~ 106 neutron st...
We present a robust method to characterize the gravitational wave emission from the remnant of a neu...
We present a robust method to characterize the gravitational wave emission from the remnant of a neu...
The observation of binary neutron star merger GW170817, along with its optical counterpart, provided...