# The third and a half-post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries

@article{Faye2012TheTA, title={The third and a half-post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries}, author={G. Faye and S. Marsat and L. Blanchet and B. Iyer}, journal={Classical and Quantum Gravity}, year={2012}, volume={29}, pages={175004} }

We compute the quadrupole mode of the gravitational waveform of inspiralling compact binaries at the third and half-post-Newtonian (3.5PN) approximation of general relativity. The computation is performed using the multipolar post-Newtonian formalism, and restricted to binaries without spins moving on quasi-circular orbits. The new inputs mainly include the 3.5PN terms in the mass quadrupole moment of the source, and the control of required subdominant corrections to the contributions of… CONTINUE READING

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