Abstract

We study the post-Minkowskian (PM) and post-Newtonian (PN) expansions of the gravitational three-body effective potential. At order 2PM a formal result is given in terms of a differential operator acting on the maximal generalized cut of the one-loop triangle integral. We compute the integral in all kinematic regions and show that the leading terms in the PN expansion are reproduced. We then perform the PN expansion unambiguously at the level of the integrand. Finding agreement with the 2PN three-body potential after integration, we explicitly present new ${G}^{2}{v}^{4}$-contributions at order 3PN and outline the generalization to ${G}^{2}{v}^{2n}$. The integrals that represent the essential input for these results are obtained by applying the recent Yangian bootstrap directly to their $\ensuremath{\epsilon}$-expansion around three dimensions. The coordinate space Yangian generator that we employ to obtain these integrals can be understood as a special conformal symmetry in a dual momentum space.

Highlights

  • The three-body problem in Newtonian gravity has been a source of inspiration in mathematics and physics since the time of Newton himself

  • As observations indicate that many galaxies, including our own, contain supermassive black holes in their core, these N-body interactions might be important for the dynamics of multiple-star systems in their vicinity [3]

  • With the advent of gravitational wave astronomy [4,5,6] the gravitational radiation emitted by mergers of compact binaries is observable

Read more

Summary

INTRODUCTION

The three-body problem in Newtonian gravity has been a source of inspiration in mathematics and physics since the time of Newton himself. The relation between the world-line quantum field theory and the scattering amplitude approach was recently clarified in [64] Despite this progress, for the N-body problem nothing is known beyond 1PM order at which there are no genuine higher body interactions [61]. It is the aim of this paper to improve on this and to construct the 2PM effective potential in the three-body case (the essential 2PM formulae straightforwardly generalize to N bodies) This in turn may be employed to determine all the velocity dependent contributions to the potential at order G2 in the post-Newtonian expansion, i.e., the terms of order v2nG2m3=r2. VII provide all three-body terms at the 3PN order that scale quartically in velocities and show that they reproduce the known results in the twobody limit

EFFECTIVE FIELD THEORY
POST-NEWTONIAN EXPANSION AND INTEGRAL BOOTSTRAP
THE 2PN EXPANSION
NEW CONTRIBUTIONS AT 3PN
V: L3ðDPNÞ
VIII. CONCLUSIONS AND OUTLOOK
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call