The third and a half-post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries
Guillaume Faye(Centre National de la Recherche Scientifique), B. R. Iyer(Raman Research Institute), Luc Blanchet(Centre National de la Recherche Scientifique), S. Marsat(Université Clermont Auvergne)
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