Parametrizing gravitational-wave polarizations
Maximiliano Isi

TL;DR
This paper reviews the formalism of gravitational wave polarizations, clarifies polarization angle definitions, explores signal parametrizations, and discusses their implications for data analysis, providing guidance for improved GW signal modeling and interpretation.
Contribution
It introduces a comprehensive review of GW polarization formalisms, clarifies polarization angle concepts, and evaluates various parametrizations for different GW analysis applications.
Findings
Identifies three distinct definitions of polarization angle.
Shows any GW signal can be expressed as a superposition of elliptical states.
Analyzes the suitability of different parametrizations for various GW data analysis scenarios.
Abstract
We review the formalism underlying the modeling of gravitational wave (GW) polarizations, and the coordinate frames used to define them. In the process, we clarify the notion of "polarization angle" and identify three conceptually distinct definitions. We describe how those are related and how they arise in the practice of GW data analysis, explaining in detail the relevant conventions that have become the LIGO-Virgo standard. Furthermore, we show that any GW signal can be expressed as a superposition of elliptical (i.e., fully-polarized) states, and examine the properties and possible parametrizations of such elementary states. We discuss a variety of common parametrizations for fully-polarized modes, and compute Jacobians for the coordinate transformations relating them. This allows us to examine the suitability of each parametrization for different applications, including unmodeled…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Gamma-ray bursts and supernovae · Astrophysical Phenomena and Observations
