Add to ORKGTidal effects due to the presence of matter in binary neutron star inspiral cause the gravitational wave phase to accumulate more rapidly than in binary black hole inspiral. We report a comparison of numerical waveforms from an extended set of simulations of inspiraling neutron-star binaries, computed by systematically varying the parameters of the equation of state above nuclear density. We calculate the signal strength of the difference between waveforms and obtain improved estimates of the accuracy with which second and third generation gravitational wave detectors can constrain the neutron-star equations of state. We also show how a observation of N events at varying distances improves the measurability
Fisher matrix and related studies have suggested that, with second-generation gravitational-wave det...
We develop a model for frequency-domain gravitational waveforms from inspiraling binary neutron star...
Finite size effects come into play during the late stages of neutron star binary inspiral, with the ...
Tidal effects due to the presence of matter in binary neutron star inspiral cause the gravitational ...
Gravitational waves from binary neutron star (BNS) and black hole/neutron star (BHNS) inspirals are ...
Using an extended set of equations of state and a multiple-group multiple-code collaborative effort ...
The strong tidal forces that arise during the last stages of the life of a black hole-neutron star b...
We report the results of a first study that uses numerical simulations to estimate the accuracy with...
The combined observation of gravitational and electromagnetic waves from the coalescence of two neut...
To detect the gravitational-wave (GW) signal from binary neutron stars and extract information about...
The early part of the gravitational wave signal of binary neutron-star inspirals can potentially yie...
International audienceThe combined observation of gravitational and electromagnetic waves from the c...
Recently exploratory studies were performed on the possibility of constraining the neutron star equa...
With the increasing sensitivity of gravitational-wave detectors, we expect to observe multiple binar...
Fisher matrix and related studies have suggested that, with second-generation gravitational-wave det...
Fisher matrix and related studies have suggested that, with second-generation gravitational-wave det...
We develop a model for frequency-domain gravitational waveforms from inspiraling binary neutron star...
Finite size effects come into play during the late stages of neutron star binary inspiral, with the ...
Tidal effects due to the presence of matter in binary neutron star inspiral cause the gravitational ...
Gravitational waves from binary neutron star (BNS) and black hole/neutron star (BHNS) inspirals are ...
Using an extended set of equations of state and a multiple-group multiple-code collaborative effort ...
The strong tidal forces that arise during the last stages of the life of a black hole-neutron star b...
We report the results of a first study that uses numerical simulations to estimate the accuracy with...
The combined observation of gravitational and electromagnetic waves from the coalescence of two neut...
To detect the gravitational-wave (GW) signal from binary neutron stars and extract information about...
The early part of the gravitational wave signal of binary neutron-star inspirals can potentially yie...
International audienceThe combined observation of gravitational and electromagnetic waves from the c...
Recently exploratory studies were performed on the possibility of constraining the neutron star equa...
With the increasing sensitivity of gravitational-wave detectors, we expect to observe multiple binar...
Fisher matrix and related studies have suggested that, with second-generation gravitational-wave det...
Fisher matrix and related studies have suggested that, with second-generation gravitational-wave det...
We develop a model for frequency-domain gravitational waveforms from inspiraling binary neutron star...
Finite size effects come into play during the late stages of neutron star binary inspiral, with the ...