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Spin(1)Spin(2) Effects in the Motion of Inspiralling Compact Binaries at Third Order in the Post-Newtonian Expansion

Rafael A. Porto, Ira Z. Rothstein

TL;DR

The paper develops an effective field theory approach (NRGR) to spinning compact binaries and computes the spin-spin and spin-orbit potentials to third post-Newtonian order using a covariant spin supplementary condition within a Routhian formalism. By postponing the SSC to the end of the calculation, the authors maintain a canonical phase-space structure and reproduce the known MP equations, deriving a full 3PN spin-spin potential and spin EOM. They then demonstrate precise equivalence between the covariant-SSC Routhian results and earlier Newton-Wigner SSC results obtained at the action level, including a detailed treatment of frame transformations and precession. They also outline how S^2 (finite-size) corrections enter at higher order and discuss renormalization of divergences into finite-size parameters, with plans for future work on complete S^2 contributions.

Abstract

We use effective field theory techniques to compute the potentials due to spin-spin and spin-orbit effects, from which the spin(1)spin(2) contribution to the motion of spinning compact binaries to third Post-Newtonian (PN) order follow. We use a formalism which allows us to impose the spin supplementarity condition (SSC) in a canonical framework to all orders in the PN expansion. We explicitly show the equivalence with our previous results, obtained using the Newton-Wigner SSC at the level of the action for spin-spin and spin-orbit potentials reported in arXiv:gr-qc/0604099 and arXiv:0712.2032[gr-qc] respectively.

Spin(1)Spin(2) Effects in the Motion of Inspiralling Compact Binaries at Third Order in the Post-Newtonian Expansion

TL;DR

The paper develops an effective field theory approach (NRGR) to spinning compact binaries and computes the spin-spin and spin-orbit potentials to third post-Newtonian order using a covariant spin supplementary condition within a Routhian formalism. By postponing the SSC to the end of the calculation, the authors maintain a canonical phase-space structure and reproduce the known MP equations, deriving a full 3PN spin-spin potential and spin EOM. They then demonstrate precise equivalence between the covariant-SSC Routhian results and earlier Newton-Wigner SSC results obtained at the action level, including a detailed treatment of frame transformations and precession. They also outline how S^2 (finite-size) corrections enter at higher order and discuss renormalization of divergences into finite-size parameters, with plans for future work on complete S^2 contributions.

Abstract

We use effective field theory techniques to compute the potentials due to spin-spin and spin-orbit effects, from which the spin(1)spin(2) contribution to the motion of spinning compact binaries to third Post-Newtonian (PN) order follow. We use a formalism which allows us to impose the spin supplementarity condition (SSC) in a canonical framework to all orders in the PN expansion. We explicitly show the equivalence with our previous results, obtained using the Newton-Wigner SSC at the level of the action for spin-spin and spin-orbit potentials reported in arXiv:gr-qc/0604099 and arXiv:0712.2032[gr-qc] respectively.

Paper Structure

This paper contains 16 sections, 91 equations, 3 figures, 1 table.

Figures (3)

  • Figure 1: Leading order spin--spin interaction.
  • Figure 2: Diagrams contributing to 3PN order which do not involve non--linear interactions. The blob represents a spin insertion and the cross corresponds to a propagator correction.
  • Figure 3: Non--linear contributions to the 3PN spin--spin potential.