Gravitational wave lensing as a probe of halo properties and dark matter

TL;DR

This paper investigates how gravitational wave lensing phenomena, such as diffraction and central images, can be used to probe properties of gravitational lenses and dark matter, with forecasts for detection capabilities of LISA and advanced LIGO.

Contribution

It introduces a detailed analysis of wave- and geometric-optics effects in GW lensing for specific halo models and forecasts parameter measurement precision, including dark matter properties.

Findings

Wave-optics effects enable parameter measurement even without central images.

LISA and advanced LIGO can measure lens mass, impact parameter, and core size with high precision.

Potential to constrain dark matter models using GW lensing signatures.

Abstract

Just like light, gravitational waves (GWs) are deflected and magnified by gravitational fields as they propagate through the Universe. However, their low frequency, phase coherence and feeble coupling to matter allow for distinct lensing phenomena, such as diffraction and central images, that are challenging to observe through electromagnetic sources. Here we explore how these phenomena can be used to probe features of gravitational lenses. We focus on two variants of the singular isothermal sphere, with 1) a variable slope of the matter density and 2) a central core. We describe the imprints of these features in the wave- and geometric-optics regimes, including the prospect of detecting central images. We forecast the capacity of LISA and advanced LIGO to study strongly lensed signals and measure the projected lens mass, impact parameter and slope or core size. A broad range of lens masses allows all parameters to be measured with precision up to $\sim 1/{\rm SNR}$, despite large degeneracies. Thanks to wave-optics corrections, all parameters can be measured, even when no central image forms. Although GWs are sensitive to projected quantities, we compute the probability distribution of lens redshift, virial mass and projection scale given a cosmology. As an application, we consider the prospect of constraining self-interacting and ultra-light dark matter, showing the regions of parameter space accessible to strongly-lensed GWs. The distinct GW signatures will enable novel probes of fundamental physics and astrophysics, including the properties of dark matter and the central regions of galactic halos.