Generation of Post-Newtonian Gravitational Radiation via Direct Integration of the Relaxed Einstein Equations
Generation of Post-Newtonian Gravitational Radiation via Direct Integration of the Relaxed Einstein Equations
The completion of a network of advanced laser-interferometric gravitational-wave observatories around 2001 will make possible the study of the inspiral and coalescence of binary systems of compact objects (neutron stars and black holes), using gravitational radiation. To extract useful information from the waves, such as the masses and spins of …