{ "id": "2005.01064", "version": "v1", "published": "2020-05-03T12:08:26.000Z", "updated": "2020-05-03T12:08:26.000Z", "title": "Compact intermediate-mass black hole X-ray binaries: potential LISA sources?", "authors": [ "Wen-Cong Chen" ], "comment": "6 pages, 5 figures, ApJ in press", "categories": [ "astro-ph.HE" ], "abstract": "The scientific aim of the space gravitational wave (GW) detector Laser Interferometer Space Antenna (LISA) that was scheduled to launch in the early 2030s is to detect the low-frequency GW signals in the Galaxy. Its main candidate GW sources are compact binaries of white dwarfs and neutron stars. In this work, we examine whether compact intermediate-mass black hole (IMBH) X-ray binaries could be potential LISA sources. Our simulations indicate that IMBH binary with a 1000 $M_{\\odot}$ IMBH and a 3 $M_{\\odot}$ donor star in an orbit of initial orbital period near the so-called bifurcation period of 0.77 d could evolve into an ultra-compact X-ray binary, which will emit GW signals with maximum frequency of 2.5 mHz. According to the evolutionary tracks of characteristic strain, IMBH X-ray binaries with the initial donor-star masses of $1-3~M_{\\odot}$ and the initial orbital periods slightly less than the bifurcation periods will be detectable by the LISA in a distance of 15 kpc. Assuming each of 60 Galactic globular clusters hosts a 1000 $M_{\\odot}$ IMBH, the maximum number of compact IMBH X-ray binaries that LISA will detect in the Galaxy should be less than ten. Therefore, the detectability of compact IMBH X-ray binaries by the LISA is not optimistic.", "revisions": [ { "version": "v1", "updated": "2020-05-03T12:08:26.000Z" } ], "analyses": { "keywords": [ "x-ray binary", "compact intermediate-mass black hole x-ray", "intermediate-mass black hole x-ray binaries", "potential lisa sources", "imbh x-ray binaries" ], "note": { "typesetting": "TeX", "pages": 6, "language": "en", "license": "arXiv", "status": "editable" } } }