{ "id": "2408.15017", "version": "v1", "published": "2024-08-27T12:51:05.000Z", "updated": "2024-08-27T12:51:05.000Z", "title": "Unveiling the central engine of core-collapse supernovae in the Local Universe: NS or BH?", "authors": [ "Maurice H. P. M. van Putten", "Maryam A. Abchouyeh", "Massimo Della Valle" ], "comment": "20 pages, 9 figures, to appear in ApJL", "categories": [ "astro-ph.HE" ], "abstract": "The physical trigger powering supernovae following the core collapse of massive stars is believed to involve a neutron star (NS) or a black hole (BH), depending largely on progenitor mass. A potentially distinct signature is a long-duration gravitational wave (GW) burst from BH central engines by their ample energy reservoir $E_J$ in angular momentum, far more so than an NS can provide. A natural catalyst for this radiation is surrounding high-density matter in the form of a non-axisymmetric disk or torus. Here, we derive a detailed outlook on LVK probes of core-collapse supernovae CC-SNe during the present observational run O4 based on their event rate, an association with normal long GRBs and mass-scaling of GW170817B/GRB170817A. For BH central engines of mass $M$, GW170817B predicts a descending GW-chirp of energy ${\\cal E}_{GW}\\simeq 3.5\\% M_\\odot c^2 \\left(M/M_0\\right)$ at frequency $f_{GW}\\lesssim 700\\,{\\rm Hz}\\left(M_0/M\\right)$, where $M_0\\simeq 2.8\\,M_\\odot$. For a few tens of events per year well into the Local Universe within 50-100Mpc, probes at the detector-limited sensitivity are expected to break the degeneracy between their NS or BH central engines {by GW calorimetry.", "revisions": [ { "version": "v1", "updated": "2024-08-27T12:51:05.000Z" } ], "analyses": { "keywords": [ "local universe", "bh central engines", "long-duration gravitational wave", "ample energy reservoir", "core-collapse supernovae cc-sne" ], "note": { "typesetting": "TeX", "pages": 20, "language": "en", "license": "arXiv", "status": "editable" } } }