Computation of gravitational waves from inspiraling binary neutron stars in quasiequilibrium circular orbits : Formulation and calibration


The last stage of inspiraling binary neutron stars toward merger, which emits gravitational waves of frequency between ∼ 10 and ∼ 1000Hz, is one of the most promising sources of kilometer-size interferometric gravitational wave detectors such as LIGO [1]. Detection of gravitational waves from the inspiraling binaries will be achieved using a matched… (More)


20 Figures and Tables

Slides referencing similar topics