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Second post-Newtonian order radiative dynamics of inspiralling compact binaries in the Effective Field Theory approach
Adam K. Leibovich, Natália T. Maia, Ira Z. Rothstein +1
We use the Effective Field Theory (EFT) framework to compute the mass quadrupole moment, the equation of motion, and the power loss of inspiralling compact binaries at the second o…
Conservative dynamics of binary systems to fourth Post-Newtonian order in the EFT approach II: Renormalized Lagrangian
Stefano Foffa, Rafael A. Porto, Ira Rothstein +1
We complete the derivation of the conservative dynamics of binary systems to fourth Post-Newtonian (4PN) order in the effective field theory (EFT) approach. We present a self-conta…
On the Apparent Ambiguities in the Post-Newtonian Expansion for Binary Systems
Rafael A. Porto, Ira Z. Rothstein
We discuss the source of the apparent ambiguities arising in the calculation of the dynamics of binary black holes within the Post-Newtonian framework. Divergences appear in both t…
Deriving analytic solutions for compact binary inspirals without recourse to adiabatic approximations
Chad R. Galley, Ira Z. Rothstein
We utilize the dynamical renormalization group formalism to calculate the real space trajectory of a compact binary inspiral for long times via a systematic resummation of secularl…
Reply to "Comment on 'Finite size corrections to the radiation reaction force in classical electrodynamics'"
Chad R. Galley, Adam K. Leibovich, Ira Z. Rothstein
We reply to P. Forgács, T. Herpay, and P. Kovács (arXiv: 1202.6289).
Spin induced multipole moments for the gravitational wave amplitude from binary inspirals to 2.5 Post-Newtonian order
Rafael A. Porto, Andreas Ross, Ira Z. Rothstein
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 t…