{ "id": "2502.04472", "version": "v1", "published": "2025-02-06T19:48:26.000Z", "updated": "2025-02-06T19:48:26.000Z", "title": "Challenges and Opportunities for time-delay cosmography with multi-messenger gravitational lensing", "authors": [ "Simon Birrer", "Graham P. Smith", "Anowar J. Shajib", "Dan Ryczanowski", "Nikki Arendse" ], "comment": "9 pages, 2 figures, accepted to be published in Philosophical Transactions A", "doi": "10.1098/rsta.2024.0130", "categories": [ "astro-ph.CO" ], "abstract": "Strong gravitational lensing of variable sources, such as quasars or supernovae, can be used to constrain cosmological parameters through a technique known as \"time-delay cosmography''. Competitive constraints on the Hubble constant have been achieved with electromagnetic observations of lensed quasars and lensed supernovae. Gravitational wave (GW) astronomy may open up a new channel for time-delay cosmography with GW signal replacing the electromagnetic (EM) one. We highlight the similarities of using GW signals to be applied to time-delay cosmography compared to EM signal. We then discuss key differences between GW and EM signals and their resulting advantages and inconveniences from the angle of the current state-of-the-art using quasars and lensed supernovae for time-delay cosmography. We identify the astrometric precision requirement of the images as a key challenge to overcome and highlight the potentially significant impact that near-perfect time-delay measurements of lensed GWs can bring to the table.", "revisions": [ { "version": "v1", "updated": "2025-02-06T19:48:26.000Z" } ], "analyses": { "keywords": [ "time-delay cosmography", "multi-messenger gravitational lensing", "em signal", "gw signal", "opportunities" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 9, "language": "en", "license": "arXiv", "status": "editable" } } }