{ "id": "2008.07420", "version": "v1", "published": "2020-08-17T15:44:14.000Z", "updated": "2020-08-17T15:44:14.000Z", "title": "Measuring the Hubble Constant with a sample of kilonovae", "authors": [ "Michael W. Coughlin", "Sarah Antier", "Tim Dietrich", "Ryan J. Foley", "Jack Heinzel", "Mattia Bulla", "Nelson Christensen", "David A. Coulter", "Lina Issa", "Nandita Khetan" ], "doi": "10.1038/s41467-020-17998-5", "categories": [ "astro-ph.HE", "astro-ph.CO", "gr-qc" ], "abstract": "Kilonovae produced by the coalescence of compact binaries with at least one neutron star are promising standard sirens for an independent measurement of the Hubble constant ($H_0$). Through their detection via follow-up of gravitational-wave (GW), short gamma-ray bursts (sGRBs) or optical surveys, a large sample of kilonovae (even without GW data) can be used for $H_0$ contraints. Here, we show measurement of $H_0$ using light curves associated with four sGRBs, assuming these are attributable to kilonovae, combined with GW170817. Including a systematic uncertainty on the models that is as large as the statistical ones, we find $H_0 = 73.8^{+6.3}_{-5.8}$\\,$\\mathrm{km}$ $\\mathrm{s}^{-1}$ $\\mathrm{Mpc}^{-1}$ and $H_0 = 71.2^{+3.2}_{-3.1}$\\,$\\mathrm{km}$ $\\mathrm{s}^{-1}$ $\\mathrm{Mpc}^{-1}$ for two different kilonova models that are consistent with the local and inverse-distance ladder measurements. For a given model, this measurement is about a factor of 2-3 more precise than the standard-siren measurement for GW170817 using only GWs.", "revisions": [ { "version": "v1", "updated": "2020-08-17T15:44:14.000Z" } ], "analyses": { "keywords": [ "hubble constant", "inverse-distance ladder measurements", "short gamma-ray bursts", "kilonova models", "promising standard sirens" ], "tags": [ "journal article" ], "publication": { "publisher": "Nature" }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }