{ "id": "2006.14936", "version": "v1", "published": "2020-06-26T12:29:22.000Z", "updated": "2020-06-26T12:29:22.000Z", "title": "Parameter estimation for strong phase transitions in supranuclear matter using gravitational-wave astronomy", "authors": [ "Peter T. H. Pang", "Tim Dietrich", "Ingo Tews", "Chris Van Den Broeck" ], "comment": "17 pages, 11 figures", "categories": [ "astro-ph.HE", "gr-qc", "nucl-th" ], "abstract": "At supranuclear densities, explored in the core of neutron stars, a strong phase transition from hadronic matter to more exotic forms of matter might be present. To test this hypothesis, binary neutron-star mergers offer a unique possibility to probe matter at densities that we can not create in any existing terrestrial experiment. In this work, we show that, if present, strong phase transitions can have a measurable imprint on the binary neutron-star coalescence and the emitted gravitational-wave signal. We construct a new parameterization of the supranuclear equation of state that allows us to test for the existence of a strong phase transition and extract its characteristic properties purely from the gravitational-wave signal of the inspiraling neutron stars. We test our approach using a Bayesian inference study simulating 600 signals with three different equations of state and find that for current gravitational-wave detector networks already twelve events might be sufficient to verify the presence of a strong phase transition. Finally, we use our methodology to analyze GW170817 and GW190425, but do not find any indication that a strong phase transition is present at densities probed during the inspiral.", "revisions": [ { "version": "v1", "updated": "2020-06-26T12:29:22.000Z" } ], "analyses": { "keywords": [ "strong phase transition", "supranuclear matter", "gravitational-wave astronomy", "parameter estimation", "neutron stars" ], "note": { "typesetting": "TeX", "pages": 17, "language": "en", "license": "arXiv", "status": "editable" } } }