{ "id": "1110.4442", "version": "v1", "published": "2011-10-20T04:50:17.000Z", "updated": "2011-10-20T04:50:17.000Z", "title": "Effects of hyperons in binary neutron star mergers", "authors": [ "Yuichiro Sekiguchi", "Kenta Kiuchi", "Koutarou Kyutoku", "Masaru Shibata" ], "comment": "5 pages, 5 figures, accepted for publication in PRL", "categories": [ "astro-ph.HE", "gr-qc", "hep-ph", "nucl-th" ], "abstract": "Numerical simulations for the merger of binary neutron stars are performed in full general relativity incorporating both nucleonic and hyperonic finite-temperature equations of state (EOS) and neutrino cooling for the first time. It is found that even for the hyperonic EOS, a hypermassive neutron star is first formed after the merger for the typical total mass $\\approx$ 2.7M\\bigodot, and subsequently collapses to a black hole (BH). It is shown that hyperons play a substantial role in the post-merger dynamics, torus formation around the BH, and emission of gravitational waves (GWs). In particular, the existence of hyperons is imprinted in GWs. Therefore, GW observations will provide a potential opportunity to explore the composition of the neutron star matter.", "revisions": [ { "version": "v1", "updated": "2011-10-20T04:50:17.000Z" } ], "analyses": { "subjects": [ "04.30.-w", "04.25.D-", "26.60.Kp", "97.60.Jd" ], "keywords": [ "binary neutron star mergers", "neutron star matter", "hyperonic finite-temperature equations", "hypermassive neutron star", "full general relativity incorporating" ], "tags": [ "journal article" ], "publication": { "doi": "10.1103/PhysRevLett.107.211101", "journal": "Physical Review Letters", "year": 2011, "month": "Nov", "volume": 107, "number": 21, "pages": 211101 }, "note": { "typesetting": "TeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable", "inspire": 940599, "adsabs": "2011PhRvL.107u1101S" } } }