Exploring the hidden Universe: A novel phenomenological approach for recovering arbitrary gravitational-wave millilensing configurations
arXiv:2302.09870 · doi:10.1093/mnras/stad1302
Abstract
Since the first detection of gravitational waves in 2015, gravitational-wave astronomy has emerged as a rapidly advancing field that holds great potential for studying the cosmos, from probing the properties of black holes to testing the limits of our current understanding of gravity. One important aspect of gravitational-wave astronomy is the phenomenon of gravitational lensing, where massive intervening objects can bend and magnify gravitational waves, providing a unique way to probe the distribution of matter in the universe, as well as finding applications to fundamental physics, astrophysics, and cosmology. However, current models for gravitational-wave millilensing - a specific form of lensing where small-scale astrophysical objects can split a gravitational wave signal into multiple copies - are often limited to simple isolated lenses, which is not realistic for complex lensing scenarios. In this paper, we present a novel phenomenological approach to incorporate millilensing in data analysis in a model-independent fashion. Our approach enables the recovery of arbitrary lens configurations without the need for extensive computational lens modeling, making it a more accurate and computationally efficient tool for studying the distribution of matter in the universe using gravitational-wave signals. When gravitational-wave lensing observations become possible, our method can provide a powerful tool for studying complex lens configurations, including dark matter subhalos and MACHOs.
12 pages, 8 figures
References in corpus (12)
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- lenstronomy II: A gravitational lensing software ecosystem
- Search for gravitational lensing signatures in LIGO-Virgo binary black hole events
- What if LIGO's gravitational wave detections are strongly lensed by massive galaxy clusters?
- Observational signatures of microlensing in gravitational waves at LIGO/Virgo frequencies
- Strong lensing of gravitational waves as seen by LISA
- Anti-lensing: the bright side of voids
- Probing Dark Low-mass Halos and Primordial Black Holes with Frequency-dependent Gravitational Lensing Dispersions of Gravitational Waves
- Stellar-mass microlensing of gravitational waves
- On building a cluster watch-list for identifying strongly lensed supernovae, gravitational waves and kilonovae
- Direct measurement of the distribution of dark matter with strongly lensed gravitational waves
- Measuring the polarization content of gravitational waves with strongly lensed binary black hole mergers