Authors: Rafael A. Porto, Andreas Ross, Ira Z. Rothstein
Date: 13 Mar 2012
Abstract: Using the NRGR effective field theory formalism we calculate the remaining source multipole moments necessary to obtain the spin contributions to the gravitational wave amplitude to 2.5 Post-Newtonian (PN) order. We also reproduce the tail contribution to the waveform linear in spin at 2.5PN arising from the nonlinear interaction between the current quadrupole and the mass monopole.
© M. Vallisneri 2012 — last modified on 2010/01/29
Tantum in modicis, quantum in maximis