Galaxy lens reconstruction based on strongly lensed gravitational waves: similarity transformation degeneracy and mass-sheet degeneracy
Jason S.C. Poon, Stefano Rinaldi, Justin Janquart, Harsh Narola, Otto, A. Hannuksela

TL;DR
This paper analyzes the limitations in gravitational wave galaxy lens reconstruction caused by degeneracies, emphasizing the need for electromagnetic observations to improve parameter estimation and cosmological measurements.
Contribution
It provides a detailed review of similarity transformation and mass-sheet degeneracies in GW lensing, and discusses how these affect cosmological inferences and the necessity of EM data.
Findings
GW can only infer scale-free lens parameters and source position.
Two GW signals are insufficient for complete lens modeling; four signals improve accuracy.
Degeneracies impact Hubble constant measurement, but can be mitigated with EM observations.
Abstract
Gravitational wave (GW) galaxy lens reconstruction is a crucial step for many GW lensing science applications. However, dark siren GW lensing (i.e. lensed GW without observed electromagnetic (EM) counterpart) suffers from similarity transformation degeneracy and mass-sheet degeneracy. We review these two degeneracies and discuss their implications on GW-based lens reconstruction and two well-known GW lensing science cases: the Hubble constant measurement and test for modified GW propagation. Building upon previous works, our conclusions are:1) GWs can only infer the scale-free lens mass model parameters, the dimensionless source position, the GW luminosity distance and the time delay scaling (a combination of Einstein radius, lens redshift, and cosmology).2) Lens reconstruction (of singular isothermal ellipsoid lens) with only two GW signals is unlikely to yield a complete lens model,…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Adaptive optics and wavefront sensing · Stellar, planetary, and galactic studies
