Gravitational Radiation from Inspiralling Compact Binaries Completed at the Third Post-Newtonian Order
Gravitational Radiation from Inspiralling Compact Binaries Completed at the Third Post-Newtonian Order
The gravitational radiation from point particle binaries is computed at the third post-Newtonian (3PN) approximation of general relativity. Three previously introduced ambiguity parameters, coming from the Hadamard self-field regularization of the 3PN source-type mass quadrupole moment, are consistently determined by means of dimensional regularization, and proved to have the values …