Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors
J. AbadieLIGO—California Institute of Technology, Pasadena, CA 91125, USAB. P. AbbottLIGO—California Institute of Technology, Pasadena, CA 91125, USAR. AbbottLIGO—California Institute of Technology, Pasadena, CA 91125, USAM. R. AbernathyUniversity of Glasgow, Glasgow G12 8QQ, UKT. AccadiaLaboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), IN2P3/CNRS, Université de Savoie, F-74941 Annecy-le-Vieux, FranceF AcerneseINFN, sezione di NapoliC. AdamsLIGO—Livingston Observatory, Livingston, LA 70754, USAR. X. AdhikariLIGO—California Institute of Technology, Pasadena, CA 91125, USAP. AjithLIGO—California Institute of Technology, Pasadena, CA 91125, USAB. AllenAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyG. AllenStanford University, Stanford, CA 94305, USAE. Amador CeronUniversity of Wisconsin—Milwaukee, WI 53201, USAR. S. AminLouisiana State University, Baton Rouge, LA 70803, USAS. B. AndersonLIGO—California Institute of Technology, Pasadena, CA 91125, USAW. G. AndersonUniversity of Wisconsin—Milwaukee, WI 53201, USAF. AntonucciINFN, Sezione di RomaS AoudiaInstitut de Physique de Rennes, CNRS, Université de Rennes 1, 35042 Rennes, FranceMusfira ArainUniversity of Florida, Gainesville, FL 32611, USAM. C. ArayaLIGO—California Institute of Technology, Pasadena, CA 91125, USAM. AronssonLIGO—California Institute of Technology, Pasadena, CA 91125, USAK. G. ArunESPCI, CNRS, F-75005 Paris, FranceY. AsoLIGO—California Institute of Technology, Pasadena, CA 91125, USAS AstonUniversity of Birmingham, Birmingham, B15 2TT, UKP. AstoneINFN, Sezione di RomaDaniel AtkinsonP. AufmuthLeibniz Universität Hannover, D-30167 Hannover, GermanyC. AulbertAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyS. BabakAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, GermanyP. T. BakerMontana State University, Bozeman, MT 59717, USAG. BallardinEuropean Gravitational Observatory (EGO), I-56021 Cascina (Pi), ItalyS. W. BallmerLIGO—California Institute of Technology, Pasadena, CA 91125, USAD. BarkerS. BarnumSonoma State University, Rohnert Park, CA 94928, USAF. BaroneUniversità di Napoli 'Federico II' Complesso Universitario di Monte S. Angelo, I-80126 NapoliB. BarrUniversity of Glasgow, Glasgow G12 8QQ, UKP BarrigaUniversity of Western Australia, Crawley, WA 6009, AustraliaL BarsottiLIGO—Massachusetts Institute of Technology, Cambridge, MA 02139, USAM. BarsugliaUniversité Paris CitéM. A. BartonI. BartosColumbia University, New York, NY 10027, USAR. BassiriUniversity of Glasgow, Glasgow G12 8QQ, UKM. BastarrikaUniversity of Glasgow, Glasgow G12 8QQ, UKJ. BauchrowitzAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyTh. S. BauerNikhef, National Institute for Subatomic Physics, PO Box 41882, 1009 DB AmsterdamB. BehnkeAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, GermanyM. G. BekerNikhef, National Institute for Subatomic Physics, PO Box 41882, 1009 DB AmsterdamM. BenacquistaThe University of Texas at Brownsville and Texas Southmost College, Brownsville, TX 78520, USAA. BertoliniAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyJ. BetzwieserLIGO—California Institute of Technology, Pasadena, CA 91125, USAN. BeveridgeUniversity of Glasgow, Glasgow G12 8QQ, UKP. T. BeyersdorfSan Jose State University, San Jose, CA 95192, USAS. BigottaINFN, Sezione di PisaI. A. BilenkoMoscow State University, Moscow 119992, RussiaG BillingsleyLIGO—California Institute of Technology, Pasadena, CA 91125, USAJ. BirchLIGO—Livingston Observatory, Livingston, LA 70754, USAS BirindelliUniversité Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 NiceR. BiswasUniversity of Wisconsin—Milwaukee, WI 53201, USAM. BitossiUniversità di PisaM. A. BizouardLAL, Université Paris-Sud, IN2P3/CNRS, F-91898 OrsayE BlackLIGO—California Institute of Technology, Pasadena, CA 91125, USAJ. K. BlackburnLIGO—California Institute of Technology, Pasadena, CA 91125, USALindy BlackburnLIGO—Massachusetts Institute of Technology, Cambridge, MA 02139, USAD. G. BlairUniversity of Western Australia, Crawley, WA 6009, AustraliaB. BlandM. BlomNikhef, National Institute for Subatomic Physics, PO Box 41882, 1009 DB AmsterdamA BlombergUniversity of Massachusetts—Amherst, MA 01003, USAC BoccaraESPCI, CNRS, F-75005 Paris, FranceO BockAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyT. P. BodiyaLIGO—Massachusetts Institute of Technology, Cambridge, MA 02139, USAR. BondarescuThe Pennsylvania State University, University Park, PA 16802, USAF. BonduUniversité Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 NiceL BonelliUniversità di PisaR. BorkLIGO—California Institute of Technology, Pasadena, CA 91125, USAM. BornAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyS. BoseWashington State University, Pullman, WA 99164, USAL BosiUniversità di Perugia, I-6123 Perugia, ItalyMichael BoyleCaltech-CaRT, Pasadena, CA 91125, USAS BracciniUniversità di PisaC. BradaschiaINFN, Sezione di PisaP. R. BradyUniversity of Wisconsin—Milwaukee, WI 53201, USAV. B. BraginskyMoscow State University, Moscow 119992, RussiaJ. BrauUniversity of Oregon, Eugene, OR 97403, USAJ. BreyerAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyD. O. BridgesLIGO—Livingston Observatory, Livingston, LA 70754, USAA BrilletUniversité Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 NiceM. BrinkmannAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyV. BrissonESPCI, CNRS, F-75005 Paris, FranceM. BritzgerAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyA. F. BrooksLIGO—California Institute of Technology, Pasadena, CA 91125, USAD. BrownSyracuse University, Syracuse, NY 13244, USAR. BudzyńskiInstitute of Astronomy 65-265 Zielona Góra, PolandT. BulikInstitute of Astronomy 65-265 Zielona Góra, PolandH. J. BultenVU University Amsterdam, De Boelelaan 1081, 1081 HV Amsterdam, The NetherlandsA. BuonannoUniversity of Maryland, College Park, MD 20742, USAJ. Burguet–CastellUniversity of Wisconsin—Milwaukee, WI 53201, USAO. BurmeisterAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyD. BuskulicLaboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), IN2P3/CNRS, Université de Savoie, F-74941 Annecy-le-Vieux, FranceRobert L. ByerStanford University, Stanford, CA 94305, USAL. CadonatiUniversity of Massachusetts—Amherst, MA 01003, USAG. CagnoliINFN, Sezione di Firenze, I-50019 Sesto Fiorentino
2010en
ABI
Аннотация
We present an up-to-date, comprehensive summary of the rates for all types of compact binary coalescence sources detectable by the Initial and Advanced versions of the ground-based gravitational-wave detectors LIGO and Virgo. Astrophysical estimates for compact-binary coalescence rates depend on a number of assumptions and unknown model parameters, and are still uncertain. The most confident among these estimates are the rate predictions for coalescing binary neutron stars which are based on extrapolations from observed binary pulsars in our Galaxy. These yield a likely coalescence rate of 100 per Myr per Milky Way Equivalent Galaxy (MWEG), although the rate could plausibly range from 1 per Myr per MWEG to 1000 per Myr per MWEG. We convert coalescence rates into detection rates based on data from the LIGO S5 and Virgo VSR2 science runs and projected sensitivities for our Advanced detectors. Using the detector sensitivities derived from these data, we find a likely detection rate of 0.02 per year for Initial LIGO-Virgo interferometers, with a plausible range between 0.0002 and 0.2 per year. The likely binary neutron-star detection rate for the Advanced LIGO-Virgo network increases to 40 events per year, with a range between 0.4 and 400 per year.
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