On the determination of the last stable orbit for circular general relativistic binaries at the third post-Newtonian approximation
Thibault Damour, Piotr Jaranowski, and Gerhard Schaefer

TL;DR
This paper analytically determines the last stable orbit in circular relativistic binaries at 3PN order, comparing various resummation methods and introducing new approaches to improve accuracy and understanding of the orbit's location.
Contribution
It introduces new resummation techniques and generalizes the effective one-body approach at 3PN level, providing insights into the LSO's dependence on regularization ambiguities.
Findings
All methods agree for a specific parameter value near -9.
The LSO location is sensitive to the ambiguity parameter cm.
Using Shanks transformation improves convergence of estimates.
Abstract
We discuss the analytical determination of the location of the Last Stable Orbit (LSO) in circular general relativistic orbits of two point masses. We use several different ``resummation methods'' (including new ones) based on the consideration of gauge-invariant functions, and compare the results they give at the third post-Newtonian (3PN) approximation of general relativity. Our treatment is based on the 3PN Hamiltonian of Jaranowski and Sch\"afer. One of the new methods we introduce is based on the consideration of the (invariant) function linking the angular momentum and the angular frequency. We also generalize the ``effective one-body'' approach of Buonanno and Damour by introducing a non-minimal (i.e. ``non-geodesic'') effective dynamics at the 3PN level. We find that the location of the LSO sensitively depends on the (currently unknown) value of the dimensionless quantity …
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Pulsars and Gravitational Waves Research
