@article{5e79a6cbb9764d5584b4cc673f3b9393,
title = "LISA Sources in Milky Way Globular Clusters",
abstract = "We explore the formation of double-compact-object binaries in Milky Way (MW) globular clusters (GCs) that may be detectable by the Laser Interferometer Space Antenna (LISA). We use a set of 137 fully evolved GC models that, overall, effectively match the properties of the observed GCs in the MW. We estimate that, in total, the MW GCs contain ∼21 sources that will be detectable by LISA. These detectable sources contain all combinations of black hole (BH), neutron star, and white dwarf components. We predict ∼7 of these sources will be BH-BH binaries. Furthermore, we show that some of these BH-BH binaries can have signal-to-noise ratios large enough to be detectable at the distance of the Andromeda galaxy or even the Virgo cluster.",
author = "Kyle Kremer and Sourav Chatterjee and Katelyn Breivik and Rodriguez, {Carl L.} and Larson, {Shane L.} and Rasio, {Frederic A.}",
note = "Funding Information: This work was supported by NASA ATP Grant No. NNX14AP92G and NSF Grant No. AST-1716762. K. K. acknowledges support by the National Science Foundation Graduate Research Fellowship Program under Grant No. DGE-1324585. S. C. acknowledges support from CIERA, the National Aeronautics and Space Administration through a Chandra Grant No. TM5-16004X/NAS8-03060 issued by the Chandra X-ray Observatory Center (operated by the Smithsonian Astrophysical Observatory for and on behalf of the National Aeronautics Space Administration under Contract No. NAS8-03060), and Hubble Space Telescope Archival research Grant No. HST-AR-14555.001-A (from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA Contract No. NAS5-26555). Publisher Copyright: {\textcopyright} 2018 American Physical Society.",
year = "2018",
month = may,
day = "11",
doi = "10.1103/PhysRevLett.120.191103",
language = "English (US)",
volume = "120",
journal = "Physical Review Letters",
issn = "0031-9007",
publisher = "American Physical Society",
number = "19",
}