Theory of post-Newtonian radiation and reaction
Ofek Birnholtz, Shahar Hadar, Barak Kol

TL;DR
This paper develops a unified, gauge-invariant effective field theory framework for post-Newtonian gravitational radiation and reaction, introducing novel methods for zone matching and multipole calculations, applicable to scalar, electromagnetic, and gravitational fields.
Contribution
It reformulates the post-Newtonian radiation and reaction theory using gauge-invariant fields, 2-way multipoles, and a double-field action, unifying outgoing radiation and reaction forces in a novel way.
Findings
Derived a simplified expression for radiation source multipoles.
Calculated the leading outgoing radiation and reaction force with minimal complexity.
Presented a new +1PN correction to mass multipoles in gravitational theory.
Abstract
We address issues with extant formulations of dissipative effects in the effective field theory (EFT) which describes the post-Newtonian (PN) inspiral of two gravitating bodies by (re)formulating several parts of the theory. Novel ingredients include gauge invariant spherical fields in the radiation zone; a system zone which preserves time reversal such that its violation arises not from local odd propagation but rather from interaction with the radiation sector in a way which resembles the balayage method; 2-way multipoles to perform zone matching within the EFT action; and a double-field radiation-reaction action which is the non-quantum version of the Closed Time Path formalism and generalizes to any theory with directed propagators including theories which are defined by equations of motion rather than an action. This formulation unifies the treatment of outgoing radiation and its…
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