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Gravitational waves from binary systems in circular orbits: Does the post-Newtonian expansion converge?
L. E. Simone, S. W. Leonard, E. Poisson +1
Gravitational radiation can be expressed in terms of an infinite series of radiative, symmetric trace-free (STF) multipole moments which can be connected to the behavior of the sou…
Gravitational radiation from compact binary systems: gravitational waveforms and energy loss to second post-Newtonian order
Clifford M. Will, Alan G. Wiseman
We derive the gravitational waveform and gravitational-wave energy flux generated by a binary star system of compact objects (neutron stars or black holes), accurate through second…
Gravitational waveforms from inspiralling compact binaries to second-post-Newtonian order
Luc Blanchet, Bala R. Iyer, Clifford M. Will +1
The two independent ``plus" and ``cross" polarization waveforms associated with the gravitational waves emitted by inspiralling, non-spinning, compact binaries are presented, ready…