Classical 3-loop 2-body diagrams
arXiv:1306.3220 · doi:10.1007/JHEP09(2013)069
Abstract
As part of the study of the two-body problem in Einstein's gravity, the fourth post-Newtonian order (4PN) of the two-body effective action is being computed presently by both effective field theory (EFT) methods and others. Diagrams with 3 (or 4) classical loops appear to be a significant obstacle. In this paper we develop a method to compute such 3-loop diagrams and demonstrate it through a specific diagram. We reduce the classical diagrams through shrinking the body worldlines to a form more familiar in Quantum Field Theory. A key ingredient in the evaluation is the Integration By Parts method for Feynman integrals.
15 pages, 6 figures. v2: updated references and credit. v3: added calculation and a minor correction
References in corpus (8)
- Effective field theory calculation of second post-Newtonian binary dynamics
- The dynamics of the gravitational two-body problem at fourth post-Newtonian order and at quadratic order in the Newton constant
- Non-Relativistic Gravitation: From Newton to Einstein and Back
- Classical Effective Field Theory and Caged Black Holes
- Les Houches Lectures on Effective Field Theories and Gravitational Radiation
- Analytic results for planar three-loop four-point integrals from a Knizhnik-Zamolodchikov equation
- Theory of post-Newtonian radiation and reaction
- The Advanced LIGO Gravitational Wave Detector
Cited by in corpus (7)
- Effective Field Theories of Post-Newtonian Gravity: A comprehensive review
- Effective field theory methods to model compact binaries
- NLO gravitational spin-orbit coupling at order
- Renormalizing Love: tidal effects at the third post-Newtonian order
- Gravitoelectric dynamical tides at second post-Newtonian order
- Radiating Love: adiabatic tidal fluxes and modes up to next-to-next-to-leading post-Newtonian order
- Symmetries of Feynman integrals and the Integration By Parts method