Sensitivity studies for third-generation gravitational wave observatories
S. HildSUPA, School of Physics and Astronomy, The University of Glasgow, Glasgow, G12 8QQ, UKM. R. AbernathySUPA, School of Physics and Astronomy, The University of Glasgow, Glasgow, G12 8QQ, UKF. AcerneseINFN, Sezione di Napoli, ItalyPau Amaro‐SeoaneInstitut de Ciències de l’Espai (CSIC-IEEC), Campus UAB, Torre C-5, parells, 2na planta, ES-08193, Bellaterra, Barcelona, SpainNils AnderssonUniversity of Southampton, Southampton SO17 1BJ, UKK. G. ArunLAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, FranceF. BaroneINFN, Sezione di Napoli, ItalyB. BarrSUPA, School of Physics and Astronomy, The University of Glasgow, Glasgow, G12 8QQ, UKM. BarsugliaAstroParticule et Cosmologie (APC), CNRS; Observatoire de Paris, Université Denis Diderot, Paris VII, FranceM. G. BekerNikhef, Science Park 105, 1098 XG Amsterdam, The NetherlandsN. BeveridgeSUPA, School of Physics and Astronomy, The University of Glasgow, Glasgow, G12 8QQ, UKS. BirindelliUniversité Nice ‚Sophia–Antipolis', CNRS, Observatoire de la Côte d’Azur, F-06304 Nice, FranceS. BoseWashington State University, Pullman, WA 99164, USAL. BosiINFN, Sezione di Perugia, I-6123 Perugia, ItalyS. BracciniINFN, Sezione di Pisa, ItalyC. BradaschiaINFN, Sezione di Pisa, ItalyT. BulikAstronomical Observatory, University of warsaw, Al Ujazdowskie 4, 00-478 Warsaw, PolandE. CalloniINFN, Sezione di Napoli, ItalyG. CellaINFN, Sezione di Pisa, ItalyEric MottinAstroParticule et Cosmologie (APC), CNRS; Observatoire de Paris, Université Denis Diderot, Paris VII, FranceS. ChelkowskiUniversity of Birmingham, Birmingham, B15 2TT, UKA. ChincariniINFN, Sezione di Genova, I-16146 Genova, ItalyJ. A. ClarkCardiff University, Cardiff, CF24 3AA, UKE. CocciaINFN, Sezione di Roma Tor Vergata I-00133 Roma, ItalyC. N. ColacinoINFN, Sezione di Pisa, ItalyJ. ColasEuropean Gravitational Observatory (EGO), I-56021 Cascina (Pi), ItalyA. CummingSUPA, School of Physics and Astronomy, The University of Glasgow, Glasgow, G12 8QQ, UKL. CunninghamSUPA, School of Physics and Astronomy, The University of Glasgow, Glasgow, G12 8QQ, UKE. CuocoEuropean Gravitational Observatory (EGO), I-56021 Cascina (Pi), ItalyS. L. DanilishinMoscow State University, Moscow, 119992, RussiaK. DanzmannMax–Planck–Institut für Gravitationsphysik and Leibniz Universität Hannover, D-30167 Hannover, GermanyR. De SalvoLIGO, California Institute of Technology, Pasadena, CA 91125, USAT. DentCardiff University, Cardiff, CF24 3AA, UKR. De RosaINFN, Sezione di Napoli, ItalyL. Di FioreINFN, Sezione di Napoli, ItalyA. Di VirgilioINFN, Sezione di Pisa, ItalyM. DoetsVU University Amsterdam, De Boelelaan 1081, 1081 HV, Amsterdam, The NetherlandsV. FafoneINFN, Sezione di Roma Tor Vergata I-00133 Roma, ItalyP. FalferiINFN, Gruppo Collegato di Trento, Sezione di Padova; Istituto di Fotonica e Nanotecnologie, CNR-Fondazione Bruno Kessler, I-38123 Povo, Trento, ItalyR. FlaminioLaboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, F-69622 Villeurbanne, Lyon, FranceJ. FrancLaboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, F-69622 Villeurbanne, Lyon, FranceF. FrasconiINFN, Sezione di Pisa, ItalyA. FreiseUniversity of Birmingham, Birmingham, B15 2TT, UKDaniel FriedrichMax–Planck–Institut für Gravitationsphysik and Leibniz Universität Hannover, D-30167 Hannover, GermanyP. FuldaUniversity of Birmingham, Birmingham, B15 2TT, UKJ. GairUniversity of Cambridge, Madingley Road, Cambridge, CB3 0HA, UKG. GemmeINFN, Sezione di Genova, I-16146 Genova, ItalyÉ. GeninEuropean Gravitational Observatory (EGO), I-56021 Cascina (Pi), ItalyA. GennaiUniversity of Birmingham, Birmingham, B15 2TT, UKA. GiazottoEuropean Gravitational Observatory (EGO), I-56021 Cascina (Pi), ItalyKostas GlampedakisTheoretical Astrophysics (TAT) Eberhard-Karls-Universität Tübingen, Auf der Morgenstelle 10, D-72076 Tübingen, GermanyChristian GräfMax–Planck–Institut für Gravitationsphysik and Leibniz Universität Hannover, D-30167 Hannover, GermanyM. GranataAstroParticule et Cosmologie (APC), CNRS; Observatoire de Paris, Université Denis Diderot, Paris VII, FranceH. GroteMax–Planck–Institut für Gravitationsphysik and Leibniz Universität Hannover, D-30167 Hannover, GermanyG. M. GuidiINFN, Sezione di Firenze, I-50019 Sesto Fiorentino, ItalyA. G. GurkovskyMoscow State University, Moscow, 119992, RussiaG. HammondSUPA, School of Physics and Astronomy, The University of Glasgow, Glasgow, G12 8QQ, UKM HannamCardiff University, Cardiff, CF24 3AA, UKJ. HarmsLIGO, California Institute of Technology, Pasadena, CA 91125, USAD. HeinertFriedrich–Schiller–Universität Jena PF, D-07737 Jena, GermanyM. HendrySUPA, School of Physics and Astronomy, The University of Glasgow, Glasgow, G12 8QQ, UKI. S. HengSUPA, School of Physics and Astronomy, The University of Glasgow, Glasgow, G12 8QQ, UKE. HennesNikhef, Science Park 105, 1098 XG Amsterdam, The NetherlandsJ. HoughINFN, Sezione di Napoli, ItalyS. HusaDepartament de Fisica, Universitat de les Illes Balears, Cra. Valldemossa Km. 7.5, E-07122 Palma de Mallorca, SpainS. H. HuttnerSUPA, School of Physics and Astronomy, The University of Glasgow, Glasgow, G12 8QQ, UKGareth JonesCardiff University, Cardiff, CF24 3AA, UKF. Y. KhaliliMoscow State University, Moscow, 119992, RussiaK. KokeyamaUniversity of Birmingham, Birmingham, B15 2TT, UKKostas D. KokkotasTheoretical Astrophysics (TAT) Eberhard-Karls-Universität Tübingen, Auf der Morgenstelle 10, D-72076 Tübingen, GermanyB. KrishnanMax Planck Institute for Gravitational Physics (Albert Einstein Institute) Am Mühlenberg 1, D-14476 Potsdam, GermanyT.G.F. LiNikhef, Science Park 105, 1098 XG Amsterdam, The NetherlandsM. LorenziniINFN, Sezione di Firenze, I-50019 Sesto Fiorentino, ItalyH. LückMax–Planck–Institut für Gravitationsphysik and Leibniz Universität Hannover, D-30167 Hannover, GermanyE. MajoranaINFN, Sezione di Roma 1, I-00185 Roma, ItalyIlya MandelDepartment of Physics and Astronomy, Northwestern University, Evanston, IL 60208, USAV. MandicUniversity of Minnesota, Minneapolis, MN 55455, USAM. MantovaniINFN, Sezione di Pisa, ItalyI. W. MartinSUPA, School of Physics and Astronomy, The University of Glasgow, Glasgow, G12 8QQ, UKC. MichelLaboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, F-69622 Villeurbanne, Lyon, FranceY. MinenkovINFN, Sezione di Roma Tor Vergata I-00133 Roma, ItalyN. MorgadoLaboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, F-69622 Villeurbanne, Lyon, FranceS. MoscaINFN, Sezione di Napoli, ItalyB. MoursLAPP-IN2P3/CNRS, Université de Savoie, F-74941 Annecy-le-Vieux, FranceH. Müller‐EbhardtMax–Planck–Institut für Gravitationsphysik and Leibniz Universität Hannover, D-30167 Hannover, GermanyP. G. MurraySUPA, School of Physics and Astronomy, The University of Glasgow, Glasgow, G12 8QQ, UKR. NawrodtFriedrich–Schiller–Universität Jena PF, D-07737 Jena, GermanyJohn H. NelsonSUPA, School of Physics and Astronomy, The University of Glasgow, Glasgow, G12 8QQ, UKR. O’ShaughnessyThe Pennsylvania State University, University Park, PA 16802, USAC. D. OttCaltech–CaRT, Pasadena, CA 91125, USAC. PalombaINFN, Sezione di Roma 1, I-00185 Roma, ItalyA. PaoliEuropean Gravitational Observatory (EGO), I-56021 Cascina (Pi), ItalyG ParguezEuropean Gravitational Observatory (EGO), I-56021 Cascina (Pi), ItalyA. PasqualettiEuropean Gravitational Observatory (EGO), I-56021 Cascina (Pi), ItalyR. PassaquietiINFN, Sezione di Pisa, ItalyD. PassuelloINFN, Sezione di Pisa, ItalyL. PinardLaboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, F-69622 Villeurbanne, Lyon, FranceW. PlastinoINFN, Sezione di Roma Tre and Università di Roma Tre, Dipartimento di Fisica, I-00146 Roma, ItalyR. PoggianiINFN, Sezione di Pisa, ItalyP. PopolizioEuropean Gravitational Observatory (EGO), I-56021 Cascina (Pi), Italy
2011en
ABI
Аннотация
Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope (ET), a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this paper we describe sensitivity models for ET and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10 Hz where a complex Class. Quantum Grav. 28 (2011) 094013 S Hild et al mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates. We develop the most accurate sensitivity model, referred to as ET-D, for a third-generation detector so far, including the most relevant fundamental noise contributions.
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