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      Effective Field Theories of Post-Newtonian Gravity

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          Abstract

          This review article presents the progress made over the last decade, since the introduction of effective field theories (EFTs) into post-Newtonian (PN) Gravity. These have been put forward in the context of gravitational waves (GWs) from the compact binary inspiral. The mature development of this interdisciplinary field has resulted in significant advances of wide interest to physics at several levels serving various purposes. The field has firmly demonstrated, that seemingly disparate physical domains, such as quantum field theory (QFT) and classical Gravity, are related, and that the EFT framework is a universal one, where it has proved to supply a robust methodology to boost the progress in PN theory. [abr.] The review is aimed at a broad audience, from general readers new to the field, to specialists and experts in related subjects. The review begins with an overview of the introduction of EFTs into classical Gravity and their development. Then, the basic ideas, which form the conceptual foundation of EFTs are provided, and the strategy of a multi-stage EFT framework, which is deployed for the PN binary inspiral problem, is outlined. The main body of the review is then dedicated to presenting in detail the study of each of the effective theories at each of the intermediate scales in the problem, up to the actual GW observables. [abr.] The review is concluded with the multiple prospects of building on the field, and using further modern field theory insights and tools, to specifically address the study of GWs, as well as expand our fundamental understanding of QFTs and Gravity theories at all scales.

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          Scattering of gravitational radiation by a Schwarzschild black-hole.

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            Stability of the Schwarzschild Metric

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              Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries

              To be observed and analyzed by the network of gravitational wave detectors on ground (LIGO, VIRGO, etc.) and by the future detectors in space (LISA, etc.), inspiralling compact binaries --- binary star systems composed of neutron stars and/or black holes in their late stage of evolution --- require high-accuracy templates predicted by general relativity theory. The gravitational waves emitted by these very relativistic systems can be accurately modelled using a high-order post-Newtonian gravitational wave generation formalism. In this article, we present the current state of the art on post-Newtonian methods as applied to the dynamics and gravitational radiation of general matter sources (including the radiation reaction back onto the source) and inspiralling compact binaries. We describe the post-Newtonian equations of motion, in Lagrangian and Hamiltonian formalisms, pay attention to the self-field regularizations at work, discuss several notions of innermost circular orbits and make comparisons with numerical gravitational self-force computations. The gravitational waveform and energy flux are obtained with high post-Newtonian precision. Some landmark results are discussed in the case of eccentric compact binaries moving on quasi-elliptical orbits, and on spin-orbit coupling effects in black hole binaries.
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                Author and article information

                Journal
                04 July 2018
                Article
                1807.01699
                9351e9e5-c814-409a-b47a-1e351036273c

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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                Custom metadata
                Invited review; 68 pages, 21 figures
                hep-th gr-qc hep-ph

                General relativity & Quantum cosmology,High energy & Particle physics
                General relativity & Quantum cosmology, High energy & Particle physics

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