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تسجيل مستخدم جديدSpin induced multipole moments for the gravitational wave amplitude from binary inspirals to 2.5 Post-Newtonian order
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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.
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