From Boundary Data to Bound States III: Radiative Effects
Gihyuk Cho, Gregor K\"alin, Rafael A. Porto

TL;DR
This paper extends the boundary-to-bound correspondence to include radiative effects, deriving new mappings between scattering and bound orbits, and analyzing the impact of tail effects and non-local contributions on gravitational wave observables.
Contribution
It introduces a comprehensive framework incorporating radiative and tail effects into the boundary-to-bound correspondence, applicable to generic orbits and eccentricities.
Findings
The B2B map holds for radiative effects in the adiabatic limit.
Logarithmic contributions are preserved between unbound and bound orbits.
Non-local effects do not smoothly transition to quasi-circular orbits.
Abstract
We extend the "boundary-to-bound" (B2B) correspondence to incorporate radiative as well as conservative radiation-reaction effects. We start by deriving a map between the total change in observables due to gravitational wave emission during hyperbolic-like motion and in one period of an elliptic-like orbit, which is valid in the adiabatic expansion for non-spinning as well as aligned-spin configurations. We also discuss the inverse problem of extracting the associated fluxes from scattering data. Afterwards we demonstrate, to all orders in the Post-Minkowskian expansion, the link between the radiated energy and the ultraviolet pole in the radial action in dimensional regularization due to tail effects. This implies, as expected, that the B2B correspondence for the conservative sector remains unchanged for local-in-time radiation-reaction tail effects with generic orbits. As a side…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Cosmology and Gravitation Theories · High-pressure geophysics and materials
