Effective Field Theory for Gravitational Radiation in General Relativity and beyond
Massimiliano Maria Riva

TL;DR
This thesis develops an effective field theory approach to gravitational radiation in general relativity and scalar-tensor theories, simplifying calculations and extending methods to include scalar fields and alternative gravity models.
Contribution
It introduces the Kaluza-Klein parametrization for higher-order post-Newtonian calculations and extends it to conformally-coupled scalar-tensor gravity, providing new tools for binary system analysis.
Findings
Validated the effective field theory approach for binary black holes in GR
Extended the Kaluza-Klein parametrization to scalar-tensor gravity
Derived the gravitational action with a conformally coupled scalar field
Abstract
The topic of this thesis is the so-called Non-Relativistic General Relativity, an effective field theory approach proposed by Goldberger and Rothstein to study the conservative and dissipative dynamics of binary systems of compact objects in the post-Newtonian expansion. In the first part of the thesis we review this approach in the simplest possible case: a binary of non-spinning black holes at leading post-Newtonian order, both for the conservative and dissipative sector in general relativity. In the second part of the thesis we present the so-called Kaluza-Klein parametrization of the metric. Introduced by Kol and Smolkin, it allows to simplify the computations in the conservative sector at higher order in the post-Newtonian expansion. We then extend this parametrization to (conformally-coupled) scalar-tensor gravity. In particular, we derive in details the gravitational action…
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Pulsars and Gravitational Waves Research
