An Effective Field Theory of Gravity for Extended Objects
Walter D. Goldberger, Ira Z. Rothstein

TL;DR
This paper develops an Effective Field Theory framework for non-relativistic extended objects in gravity, enabling systematic calculations of gravitational radiation and finite size effects in binary systems relevant to gravitational wave detection.
Contribution
It introduces a novel EFT formalism that separates relevant scales and incorporates finite size effects via non-minimal couplings, simplifying high-order post-Newtonian calculations.
Findings
Renormalization of divergences requires non-minimal couplings.
Decoupling of internal structure holds up to order v^6.
Finite size effects appear at order v^10 and can be parameterized by coefficients.
Abstract
We present an Effective Field Theory (EFT) formalism which describes the dynamics of non-relativistic extended objects coupled to gravity. The formalism is relevant to understanding the gravitational radiation power spectra emitted by binary star systems, an important class of candidate signals for gravitational wave observatories such as LIGO or VIRGO. The EFT allows for a clean separation of the three relevant scales: r_s, the size of the compact objects, r the orbital radius and r/v, the wavelength of the physical radiation (where the velocity v is the expansion parameter). In the EFT radiation is systematically included in the v expansion without need to separate integrals into near zones and radiation zones. We show that the renormalization of ultraviolet divergences which arise at v^6 in post-Newtonian (PN) calculations requires the presence of two non-minimal worldline…
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