Exploring the sensitivity of next generation gravitational wavedetectors
B. P. AbbottLIGO, California Institute of Technology, Pasadena, CA 91125, USAR. AbbottLIGO, California Institute of Technology, Pasadena, CA 91125, USAT. D. AbbottLouisiana State University, Baton Rouge, LA 70803, USAM. R. AbernathyAmerican University, Washington, DC 20016, USAK. AckleyUniversity of Florida, Gainesville, FL 32611, USAC. AdamsLIGO Livingston Observatory, Livingston, LA 70754, USAP. AddessoUniversity of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, ItalyR. X. AdhikariLIGO, California Institute of Technology, Pasadena, CA 91125, USAV. B. AdyaAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyC. AffeldtAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyN. AggarwalLIGO, Massachusetts Institute of Technology, Cambridge, MA 02139, USAO. D. AguiarInstituto Nacional de Pesquisas Espaciais, 12227-010 São José dos Campos, São Paulo, BrazilA. AinInter-University Centre for Astronomy and Astrophysics, Pune 411007, IndiaP. AjithInternational Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bangalore 560012, IndiaB. AllenUniversity of Wisconsin-Milwaukee, Milwaukee, WI 53201, USAP. A. AltinAustralian National University, Canberra, Australian Capital Territory 0200, AustraliaS. B. AndersonLIGO, California Institute of Technology, Pasadena, CA 91125, USAW. G. AndersonUniversity of Wisconsin-Milwaukee, Milwaukee, WI 53201, USAK. AraiLIGO, California Institute of Technology, Pasadena, CA 91125, USAM. C. ArayaLIGO, California Institute of Technology, Pasadena, CA 91125, USAC. C. ArceneauxThe University of Mississippi, University, MS 38677, USAJ. S. AreedaCalifornia State University Fullerton, Fullerton, CA 92831, USAK. G. ArunChennai Mathematical Institute, Chennai 603103, IndiaG. AshtonUniversity of Southampton, Southampton SO17 1BJ, UKM. AstUniversität Hamburg, D-22761 Hamburg, GermanyS. M. AstonLIGO Livingston Observatory, Livingston, LA 70754, USAP. 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 Potsdam-Golm, GermanyP. T. BakerMontana State University, Bozeman, MT 59717, USAS. BallmerSyracuse University, Syracuse, NY 13244, USAJ. C. BarayogaLIGO, California Institute of Technology, Pasadena, CA 91125, USAS. E. BarclaySUPA, University of Glasgow, Glasgow G12 8QQ, UKB. C. BarishLIGO, California Institute of Technology, Pasadena, CA 91125, USAD. BarkerB. BarrSUPA, University of Glasgow, Glasgow G12 8QQ, UKL. BarsottiLIGO, Massachusetts Institute of Technology, Cambridge, MA 02139, USAJ. BartlettI. BartosColumbia University, New York, NY 10027, USAR. BassiriStanford University, Stanford, CA 94305, USAJ. C. BatchC. BauneAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyA. S. BellSUPA, University of Glasgow, Glasgow G12 8QQ, UKB. K. BergerLIGO, California Institute of Technology, Pasadena, CA 91125, USAG. BergmannAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyC. P. L. BerryUniversity of Birmingham, Birmingham B15 2TT, UKJ. BetzwieserLIGO Livingston Observatory, Livingston, LA 70754, USAS. BhagwatSyracuse University, Syracuse, NY 13244, USAR. BhandareRRCAT, Indore MP 452013, IndiaI. A. BilenkoFaculty of Physics, Lomonosov Moscow State University, Moscow 119991, RussiaG. BillingsleyLIGO, California Institute of Technology, Pasadena, CA 91125, USAJ. BirchLIGO Livingston Observatory, Livingston, LA 70754, USAR. BirneySUPA, University of the West of Scotland, Paisley PA1 2BE, UKSébastien BiscansLIGO, Massachusetts Institute of Technology, Cambridge, MA 02139, USAA. BishtAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyC. BiwerSyracuse University, Syracuse, NY 13244, USAJ. K. BlackburnLIGO, California Institute of Technology, Pasadena, CA 91125, USAC. D. BlairUniversity of Western Australia, Crawley, Western Australia 6009, AustraliaD. G. BlairUniversity of Western Australia, Crawley, Western Australia 6009, AustraliaR. M. BlairO. BockAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyC. BoganAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyA. BohéAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Potsdam-Golm, GermanyC. BondUniversity of Birmingham, Birmingham B15 2TT, UKR. BorkLIGO, California Institute of Technology, Pasadena, CA 91125, USAS. BoseWashington State University, Pullman, WA 99164, USAP. R. BradyUniversity of Wisconsin-Milwaukee, Milwaukee, WI 53201, USAV. B. BraginskyFaculty of Physics, Lomonosov Moscow State University, Moscow 119991, RussiaJ. E. BrauUniversity of Oregon, Eugene, OR 97403, USAM. BrinkmannAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyP. BrockillUniversity of Wisconsin-Milwaukee, Milwaukee, WI 53201, USAJ. E. BroidaCarleton College, Northfield, MN 55057, USAA. F. BrooksLIGO, California Institute of Technology, Pasadena, CA 91125, USAD. BrownSyracuse University, Syracuse, NY 13244, USAN. M. BrownLIGO, Massachusetts Institute of Technology, Cambridge, MA 02139, USAS. BrunettLIGO, California Institute of Technology, Pasadena, CA 91125, USAC. C. BuchananLouisiana State University, Baton Rouge, LA 70803, USAA. BuikemaLIGO, Massachusetts Institute of Technology, Cambridge, MA 02139, USAA. BuonannoAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Potsdam-Golm, GermanyRobert L. ByerStanford University, Stanford, CA 94305, USAM. CaberoAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyL. CadonatiCenter for Relativistic Astrophysics and School of Physics, Georgia Institute of Technology, Atlanta, GA 30332, USAC. CahillaneLIGO, California Institute of Technology, Pasadena, CA 91125, USAJ. Calderón BustilloCenter for Relativistic Astrophysics and School of Physics, Georgia Institute of Technology, Atlanta, GA 30332, USAT. A. CallisterLIGO, California Institute of Technology, Pasadena, CA 91125, USAJ. B. CampNASA/Goddard Space Flight Center, Greenbelt, MD 20771, USAK. C. CannonRESCEU, University of Tokyo, Tokyo, 113-0033, JapanJ. CaoTsinghua University, Beijing 100084, People's Republic of ChinaC. D. CapanoAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, GermanyS. CarideTexas Tech University, Lubbock, TX 79409, USAS. CaudillUniversity of Wisconsin-Milwaukee, Milwaukee, WI 53201, USAM. CavagliàThe University of Mississippi, University, MS 38677, USAC. CepedaLIGO, California Institute of Technology, Pasadena, CA 91125, USAS. J. ChamberlinThe Pennsylvania State University, University Park, PA 16802, USAM. ChanSUPA, University of Glasgow, Glasgow G12 8QQ, UKS. ChaoNational Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of ChinaP. CharltonCharles Sturt University, Wagga Wagga, New South Wales 2678, AustraliaB. D. CheeseboroWest Virginia University, Morgantown, WV 26506, USAHsin-Yu ChenUniversity of Chicago, Chicago, IL 60637, USA
2017en
ABI
Abstract
Abstract The second-generation of gravitational-wave detectors are just starting operation, and have already yielding their first detections. Research is now concentrated on how to maximize the scientific potential of gravitational-wave astronomy. To support this effort, we present here design targets for a new generation of detectors, which will be capable of observing compact binary sources with high signal-to-noise ratio throughout the Universe.
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Citations and references
Cited by 20 references