article Open AccessTop 1% cited
Exploring the sensitivity of next generation gravitational wavedetectors
Classical and Quantum Gravity · 2017 · Vol. 34(4) · pp. 044001–044001
B. P. Abbott(California Institute of Technology)R. Abbott(California Institute of Technology)T. D. Abbott(Louisiana State University)M. R. Abernathy(American University)K. Ackley(University of Florida)C. Adams(LIGO Scientific Collaboration)P. Addesso(University of Sannio)R. X. Adhikari(California Institute of Technology)V. B. Adya(Max Planck Institute for Gravitational Physics)C. Affeldt(Max Planck Institute for Gravitational Physics)N. Aggarwal(Massachusetts Institute of Technology)O. D. Aguiar(Instituto Nacional de Pesquisas Espaciais)A. Ain(Inter-University Centre for Astronomy and Astrophysics)P. Ajith(Tata Institute of Fundamental Research)B. Allen(Leibniz University Hannover)P. A. Altin(Australian National University)S. B. Anderson(California Institute of Technology)W. G. Anderson(University of Wisconsin–Milwaukee)K. Arai(California Institute of Technology)M. C. Araya(California Institute of Technology)C. C. Arceneaux(University of Mississippi)J. S. Areeda(California State University, Fullerton)K. G. Arun(Chennai Mathematical Institute)G. Ashton(University of Southampton)M. Ast(Universität Hamburg)S. M. Aston(LIGO Scientific Collaboration)P. Aufmuth(Leibniz University Hannover)C. Aulbert(Max Planck Institute for Gravitational Physics)S. Bagnasco(Max Planck Institute for Gravitational Physics)P. T. Baker(Montana State University)S. Ballmer(Syracuse University)J. C. Barayoga(California Institute of Technology)S. E. Barclay(University of Glasgow)B. C. Barish(California Institute of Technology)D. BarkerB. Barr(University of Glasgow)L. Barsotti(Massachusetts Institute of Technology)J. BartlettI. Bartos(Columbia University)R. Bassiri(Stanford University)J. C. BatchC. Baune(Max Planck Institute for Gravitational Physics)A. S. Bell(University of Glasgow)B. K. Berger(California Institute of Technology)G. Bergmann(Max Planck Institute for Gravitational Physics)C. P. L. Berry(University of Birmingham)J. Betzwieser(LIGO Scientific Collaboration)S. Bhagwat(Syracuse University)R. Bhandare(Raja Ramanna Centre for Advanced Technology)I. A. Bilenko(Lomonosov Moscow State University)G. Billingsley(California Institute of Technology)J. Birch(LIGO Scientific Collaboration)R. Birney(University of the West of Scotland)Sébastien Biscans(Massachusetts Institute of Technology)A. Bisht(Leibniz University Hannover)C. Biwer(Syracuse University)J. K. Blackburn(California Institute of Technology)C. D. Blair(The University of Western Australia)D. G. Blair(The University of Western Australia)R. M. BlairO. Bock(Max Planck Institute for Gravitational Physics)C. Bogan(Max Planck Institute for Gravitational Physics)A. Bohé(Max Planck Institute for Gravitational Physics)C. Bond(University of Birmingham)R. Bork(California Institute of Technology)S. Bose(Inter-University Centre for Astronomy and Astrophysics)P. R. Brady(University of Wisconsin–Milwaukee)V. B. Braginsky(Lomonosov Moscow State University)J. E. Brau(University of Oregon)M. Brinkmann(Max Planck Institute for Gravitational Physics)P. Brockill(University of Wisconsin–Milwaukee)J. E. Broida(Carleton College)A. F. Brooks(California Institute of Technology)D. Brown(Syracuse University)D. Brown(University of Birmingham)N. M. Brown(Massachusetts Institute of Technology)S. Brunett(California Institute of Technology)C. C. Buchanan(Louisiana State University)A. Buikema(Massachusetts Institute of Technology)A. Buonanno(Max Planck Institute for Gravitational Physics)Robert L. Byer(Stanford University)M. Cabero(Max Planck Institute for Gravitational Physics)L. Cadonati(Georgia Institute of Technology)C. Cahillane(California Institute of Technology)J. Calderón Bustillo(Georgia Institute of Technology)T. A. Callister(California Institute of Technology)J. B. Camp(Goddard Space Flight Center)K. C. Cannon(The University of Tokyo)J. Cao(Tsinghua University)C. D. Capano(Max Planck Institute for Gravitational Physics)S. Caride(Texas Tech University)S. Caudill(University of Wisconsin–Milwaukee)M. Cavaglià(University of Mississippi)C. Cepeda(California Institute of Technology)S. J. Chamberlin(Pennsylvania State University)M. Chan(University of Glasgow)S. Chao(National Tsing Hua University)P. Charlton(Charles Sturt University)B. D. Cheeseboro(West Virginia University)Yu‐Hung Chen(University of Chicago)Yu‐Hung Chen(California Institute of Technology)C. Cheng(National Tsing Hua University)H. S. Cho(Korea Institute of Science & Technology Information)M. Cho(University of Maryland, College Park)J. H. Chow(Australian National University)N. Christensen(Carleton College)Q. Chu(The University of Western Australia)S. Chung(The University of Western Australia)G. Ciani(University of Florida)F. ClaraJ. A. Clark(Georgia Institute of Technology)Christophe ColletteL. Cominsky(Sonoma State University)M. Constancio(Instituto Nacional de Pesquisas Espaciais)D. CookT. R. Corbitt(Louisiana State University)Neil J. Cornish(Montana State University)A. Corsi(Texas Tech University)C. A. Costa(Instituto Nacional de Pesquisas Espaciais)M. W. Coughlin(Carleton College)S. B. Coughlin(Northwestern University)S. T. Countryman(Columbia University)P. Couvares(California Institute of Technology)E. E. Cowan(Georgia Institute of Technology)D. M. Coward(The University of Western Australia)M. J. Cowart(LIGO Scientific Collaboration)D. C. Coyne(California Institute of Technology)R. Coyne(Texas Tech University)K. Craig(University of Glasgow)J. D. E. Creighton(University of Wisconsin–Milwaukee)J. Cripe(Louisiana State University)S. G. Crowder(University of Minnesota)A. Cumming(University of Glasgow)L. Cunningham(University of Glasgow)T. Dal Canton(Max Planck Institute for Gravitational Physics)S. L. Danilishin(University of Glasgow)K. Danzmann(Leibniz University Hannover)N. S. Darman(The University of Melbourne)Anirban Dasgupta(Institute for Plasma Research)C. F. Da Silva Costa(University of Florida)I. Dave(Raja Ramanna Centre for Advanced Technology)G. S. Davies(University of Glasgow)E. J. Daw(University of Sheffield)D. DeBra(Syracuse University)D. DeBra(Stanford University)W. Del Pozzo(University of Birmingham)T. Denker(Max Planck Institute for Gravitational Physics)T. Dent(Max Planck Institute for Gravitational Physics)V. Dergachev(California Institute of Technology)R. T. DeRosa(LIGO Scientific Collaboration)R. DeSalvo(University of Sannio)R. C. Devine(West Virginia University)S. Dhurandhar(Inter-University Centre for Astronomy and Astrophysics)M. C. Díaz(The University of Texas Rio Grande Valley)I. Di Palma(Max Planck Institute for Gravitational Physics)F. Donovan(Massachusetts Institute of Technology)K. L. Dooley(University of Mississippi)S. Doravari(Max Planck Institute for Gravitational Physics)R. Douglas(University of Glasgow)T. P. Downes(University of Wisconsin–Milwaukee)M. Drago(Max Planck Institute for Gravitational Physics)R. W. P. Drever(California Institute of Technology)Jennifer C DriggersS. E. DwyerT. B. Edo(University of Sheffield)M. C. Edwards(Carleton College)A. Effler(LIGO Scientific Collaboration)H-B Eggenstein(Max Planck Institute for Gravitational Physics)P. Ehrens(California Institute of Technology)J. Eichholz(California Institute of Technology)S. S. Eikenberry(University of Florida)W. Engels(California Institute of Technology)R. C. Essick(Massachusetts Institute of Technology)T. Etzel(California Institute of Technology)M. Evans(Massachusetts Institute of Technology)T. Evans(LIGO Scientific Collaboration)R. Everett(Pennsylvania State University)M. Factourovich(Columbia University)H. Fair(Syracuse University)S. Fairhurst(Cardiff University)X. Fan(Tsinghua University)Q. Fang(The University of Western Australia)B. Farr(University of Chicago)Will M. Farr(University of Birmingham)M. Favata(Montclair State University)M. Fays(Cardiff University)H. Fehrmann(Max Planck Institute for Gravitational Physics)M. M. Fejer(Stanford University)E. Fenyvesi(Eötvös Loránd University)E. C. Ferreira(Instituto Nacional de Pesquisas Espaciais)R. P. Fisher(Syracuse University)M. Fletcher(University of Glasgow)Z. Frei(Eötvös Loránd University)A. Freise(University of Birmingham)R. Frey(University of Oregon)P. Fritschel(Massachusetts Institute of Technology)V. V. Frolov(LIGO Scientific Collaboration)P. Fulda(University of Florida)M. Fyffe(LIGO Scientific Collaboration)H. A. Gabbard(University of Mississippi)J. R. Gair(University of Edinburgh)S. G. Gaonkar(Inter-University Centre for Astronomy and Astrophysics)G. Gaur(Indian Institute of Technology Gandhinagar)N. Gehrels(Goddard Space Flight Center)Peng Geng(The University of Texas Rio Grande Valley)J. George(Raja Ramanna Centre for Advanced Technology)L. Gergely(University of Szeged)Abhirup Ghosh(Tata Institute of Fundamental Research)Archisman Ghosh(Tata Institute of Fundamental Research)J. A. Giaime(Louisiana State University)K. D. Giardina(LIGO Scientific Collaboration)K. Gill(Embry–Riddle Aeronautical University)A. Glaefke(University of Glasgow)E. GoetzE. Goetz(University of Florida)L. Gondán(Eötvös Loránd University)G. González(Louisiana State University)A. Gopakumar(Tata Institute of Fundamental Research)Neil Gordon(University of Glasgow)M. L. Gorodetsky(Lomonosov Moscow State University)S. E. Gossan(California Institute of Technology)C. Graef(University of Glasgow)P. B. Graff(University of Maryland, College Park)A. Grant(University of Glasgow)S. Gras(Massachusetts Institute of Technology)C. GrayA. C. Green(University of Birmingham)H. Grote(Max Planck Institute for Gravitational Physics)S. Grünewald(Max Planck Institute for Gravitational Physics)X. Guo(Tsinghua University)A. Gupta(Inter-University Centre for Astronomy and Astrophysics)Manoj Gupta(Institute for Plasma Research)K. E. Gushwa(California Institute of Technology)E. K. Gustafson(California Institute of Technology)R. Gustafson(University of Michigan)J. J. Hacker(California State University, Fullerton)E. D. Hall(Washington State University)E. D. Hall(California Institute of Technology)G. Hammond(University of Glasgow)M. Haney(Tata Institute of Fundamental Research)M. M. Hanke(Max Planck Institute for Gravitational Physics)J. HanksC. Hanna(Pennsylvania State University)M. D. Hannam(Cardiff University)J. Hanson(LIGO Scientific Collaboration)T. Hardwick(Louisiana State University)I. W. Harry(American University)I. W. Harry(Max Planck Institute for Gravitational Physics)M. J. Hart(University of Glasgow)M. T. Hartman(University of Florida)C.‐J. Haster(University of Birmingham)K. Haughian(University of Glasgow)M. C. Heintze(LIGO Scientific Collaboration)M. Hendry(University of Glasgow)I. S. Heng(University of Glasgow)J. Hennig(University of Glasgow)J. Henry(Rochester Institute of Technology)A. W. Heptonstall(California Institute of Technology)M. Heurs(Leibniz University Hannover)S. Hild(University of Glasgow)D. Hoak(University of Massachusetts Amherst)K. Holt(LIGO Scientific Collaboration)D. E. Holz(University of Chicago)P. Hopkins(Cardiff University)J. Hough(University of Glasgow)E. A. Houston(University of Glasgow)E. J. Howell(The University of Western Australia)Yi-Ming Hu(Max Planck Institute for Gravitational Physics)S. Huang(National Tsing Hua University)E. A. Huerta(University of Illinois Urbana-Champaign)B. Hughey(Embry–Riddle Aeronautical University)S. Husa(Universitat de les Illes Balears)S. H. Huttner(University of Glasgow)T. Huynh–Dinh(LIGO Scientific Collaboration)N. Indik(Max Planck Institute for Gravitational Physics)D. R. IngramR. Inta(Texas Tech University)H. N. Isa(University of Glasgow)M. Isi(California Institute of Technology)T. Isogai(Massachusetts Institute of Technology)B. R. Iyer(Tata Institute of Fundamental Research)K. IzumiH. Jang(Korea Institute of Science & Technology Information)K. Jani(Georgia Institute of Technology)S. Jawahar(University of Strathclyde)L. K. Jian(The University of Western Australia)F. Jiménez‐Forteza(Universitat de les Illes Balears)W. W. Johnson(Louisiana State University)D. I. Jones(University of Southampton)R. Jones(University of Glasgow)L. Ju(The University of Western Australia)K. Haris(Indian Institute of Science Education and Research Thiruvananthapuram)C. V. Kalaghatgi(Cardiff University)V. Kalogera(Northwestern University)S. Kandhasamy(University of Mississippi)G. Kang(Korea Institute of Science & Technology Information)J. B. Kanner(California Institute of Technology)S. J. Kapadia(Max Planck Institute for Gravitational Physics)S. Karki(University of Oregon)K. S. Karvinen(Max Planck Institute for Gravitational Physics)M. Kasprzack(Louisiana State University)E. Katsavounidis(Massachusetts Institute of Technology)W. Katzman(LIGO Scientific Collaboration)S. Kaufer(Leibniz University Hannover)T. Kaur(The University of Western Australia)K. KawabeM. S. Kehl(University of Toronto)D. Keitel(Universitat de les Illes Balears)D. B. Kelley(Syracuse University)W. Kells(California Institute of Technology)R. Kennedy(University of Sheffield)J. S. Key(The University of Texas Rio Grande Valley)F. Y. Khalili(Lomonosov Moscow State University)S. Khan(Cardiff University)Z. Khan(Institute for Plasma Research)Е. А. Хазанов(Institute of Applied Physics)N. KijbunchooChi-Woong Kim(Korea Institute of Science & Technology Information)Chunglee Kim(Korea Institute of Science & Technology Information)Jinwoo Kim(Pusan National University)K. Kim(Hanyang University)Nakwoo Kim(Stanford University)W. Kim(The University of Adelaide)Y.-M. Kim(Pusan National University)S. J. Kimbrell(Georgia Institute of Technology)E. J. King(The University of Adelaide)Peter KingJ. S. KisselBernd Klein(Northwestern University)L. Kleybolte(Universität Hamburg)S. Klimenko(University of Florida)S. M. Koehlenbeck(Max Planck Institute for Gravitational Physics)V. Kondrashov(California Institute of Technology)A. Kontos(Massachusetts Institute of Technology)M. Korobko(Universität Hamburg)W. Z. Korth(California Institute of Technology)D. B. Kozak(California Institute of Technology)V. Kringel(Max Planck Institute for Gravitational Physics)C. Krueger(Leibniz University Hannover)G. Kuehn(Max Planck Institute for Gravitational Physics)P. Kumar(University of Toronto)S. Kumar(Institute for Plasma Research)L. Kuo(National Tsing Hua University)B. D. Lackey(Syracuse University)M. LandryJ. Lange(Rochester Institute of Technology)B. Lantz(Stanford University)P. D. Lasky(Monash University)M. Laxen(LIGO Scientific Collaboration)A. Lazzarini(California Institute of Technology)S. Leavey(University of Glasgow)E. O. Lebigot(Tsinghua University)Chang‐Hwan Lee(Pusan National University)H. K. Lee(Hanyang University)Hyung Mok Lee(Seoul National University)K. Lee(University of Glasgow)A. Lenon(Syracuse University)J. R. Leong(Max Planck Institute for Gravitational Physics)Y. Levin(Monash University)J. B. Lewis(California Institute of Technology)T G F Li(Chinese University of Hong Kong)A. Libson(Massachusetts Institute of Technology)T. B. Littenberg(University of Alabama in Huntsville)N. A. Lockerbie(University of Strathclyde)A. L. Lombardi(University of Massachusetts Amherst)L. T. London(Cardiff University)J. E. Lord(Syracuse University)M. Lormand(LIGO Scientific Collaboration)J. D. Lough(Leibniz University Hannover)H. Lück(Leibniz University Hannover)A. P. Lundgren(Max Planck Institute for Gravitational Physics)Ryan S. Lynch(Massachusetts Institute of Technology)Y. Ma(The University of Western Australia)B. Machenschalk(Max Planck Institute for Gravitational Physics)M. MacInnis(Massachusetts Institute of Technology)D. M. Macleod(Louisiana State University)F. Magaña‐Sandoval(Syracuse University)L. Magaña Zertuche(Syracuse University)R. M. Magee(Washington State University)V. Mandic(University of Minnesota)V. Mangano(University of Glasgow)G. L. Mansell(Australian National University)M Manske(University of Wisconsin–Milwaukee)Szabolcs Márka(Columbia University)Z. Márka(Columbia University)A. S. Markosyan(Stanford University)E. Maros(California Institute of Technology)I. W. Martin(University of Glasgow)Д. В. Мартынов(Massachusetts Institute of Technology)K. Mason(Massachusetts Institute of Technology)T. J. Massinger(Syracuse University)M. Masso‐Reid(University of Glasgow)F. Matichard(Massachusetts Institute of Technology)L. Matone(Columbia University)N. Mavalvala(Massachusetts Institute of Technology)N. Mazumder(Washington State University)R. McCarthyD. E. McClelland(Australian National University)S. McCormick(LIGO Scientific Collaboration)S. C. McGuire(Southern University and Agricultural and Mechanical College)G. McIntyre(California Institute of Technology)J. McIver(California Institute of Technology)D. J. McManus(Australian National University)T. McRae(Australian National University)S. T. McWilliams(West Virginia University)D. Meacher(Pennsylvania State University)G. D. Meadors(Max Planck Institute for Gravitational Physics)A. Melatos(The University of Melbourne)G. MendellR. A. Mercer(University of Wisconsin–Milwaukee)E. L. MerilhS. Meshkov(California Institute of Technology)C. Messenger(University of Glasgow)C. Messick(Pennsylvania State University)P. M. Meyers(University of Minnesota)H. Miao(University of Birmingham)H. Middleton(University of Birmingham)Е. Е. Михайлов(William & Mary)A. L. Miller(University of Florida)A. L. Miller(Northwestern University)B. B. Miller(Northwestern University)J. Miller(Massachusetts Institute of Technology)M. Millhouse(Montana State University)J. Ming(Max Planck Institute for Gravitational Physics)S. Mirshekari(ICTP South American Institute for Fundamental Research)C. Mishra(Tata Institute of Fundamental Research)S. Mitra(Inter-University Centre for Astronomy and Astrophysics)V. P. Mitrofanov(Lomonosov Moscow State University)G. Mitselmakher(University of Florida)R. Mittleman(Massachusetts Institute of Technology)S. R. P. Mohapatra(Massachusetts Institute of Technology)B. C. Moore(Montclair State University)C. J. Moore(University of Cambridge)D. MoraruG. MorenoS. R. Morriss(The University of Texas Rio Grande Valley)K. Mossavi(Max Planck Institute for Gravitational Physics)C. M. Mow‐Lowry(University of Birmingham)G. Mueller(University of Florida)A. W. Muir(Cardiff University)Arunava Mukherjee(Tata Institute of Fundamental Research)D. Mukherjee(University of Wisconsin–Milwaukee)S. Mukherjee(The University of Texas Rio Grande Valley)N. Mukund(Inter-University Centre for Astronomy and Astrophysics)A. Mullavey(LIGO Scientific Collaboration)J. Münch(The University of Adelaide)D. Murphy(Columbia University)P. G. Murray(University of Glasgow)A. Mytidis(University of Florida)R. K. Nayak(Indian Institute of Science Education and Research Kolkata)K. Nedkova(University of Massachusetts Amherst)T. J. N. Nelson(LIGO Scientific Collaboration)A. Neunzert(University of Michigan)G. Newton(University of Glasgow)T. Nguyen(Australian National University)A. B. Nielsen(Max Planck Institute for Gravitational Physics)A. Nitz(Max Planck Institute for Gravitational Physics)D. Nolting(LIGO Scientific Collaboration)M. E. N. Normandin(The University of Texas Rio Grande Valley)L. K. Nuttall(Syracuse University)J. OberlingE. Ochsner(University of Wisconsin–Milwaukee)J. O’Dell(Rutherford Appleton Laboratory)E. Oelker(Massachusetts Institute of Technology)G. H. Ogin(Whitman College)J. J. Oh(National Institute for Mathematical Sciences)S. H. Oh(National Institute for Mathematical Sciences)F. Ohme(Cardiff University)M. Oliver(Universitat de les Illes Balears)P. Oppermann(Max Planck Institute for Gravitational Physics)Richard J. Oram(LIGO Scientific Collaboration)B. O’Reilly(LIGO Scientific Collaboration)R. O’Shaughnessy(Rochester Institute of Technology)D. J. Ottaway(The University of Adelaide)H. Overmier(LIGO Scientific Collaboration)B. J. Owen(Texas Tech University)A. Pai(Indian Institute of Science Education and Research Thiruvananthapuram)S. A. Pai(Raja Ramanna Centre for Advanced Technology)J. R. Palamos(University of Oregon)O. Palashov(Institute of Applied Physics)A. Pal‐Singh(Universität Hamburg)H. Pan(National Tsing Hua University)C. Pankow(Northwestern University)F. Pannarale(Cardiff University)B. C. Pant(Raja Ramanna Centre for Advanced Technology)M. A. Papa(Max Planck Institute for Gravitational Physics)H. R. Paris(Stanford University)W. Parker(LIGO Scientific Collaboration)D. Pascucci(University of Glasgow)Z. Patrick(Stanford University)B. L. Pearlstone(University of Glasgow)M. Pedraza(California Institute of Technology)L. Pekowsky(Syracuse University)A. Pele(LIGO Scientific Collaboration)S. Penn(Hobart and William Smith Colleges)A. Perreca(California Institute of Technology)L. M. Perri(Northwestern University)M. Phelps(University of Glasgow)V. Pierro(University of Sannio)I. M. Pinto(University of Sannio)M. Pitkin(University of Glasgow)M. Poe(University of Wisconsin–Milwaukee)A. Post(Max Planck Institute for Gravitational Physics)J. Powell(University of Glasgow)J. Prasad(Inter-University Centre for Astronomy and Astrophysics)V. Predoi(Cardiff University)T. Prestegard(University of Minnesota)Larry R. Price(California Institute of Technology)M. Prijatelj(Max Planck Institute for Gravitational Physics)M. Principe(University of Sannio)S. Privitera(Max Planck Institute for Gravitational Physics)L. Prokhorov(Lomonosov Moscow State University)O. Puncken(Max Planck Institute for Gravitational Physics)M. Pürrer(Max Planck Institute for Gravitational Physics)H. Qi(University of Wisconsin–Milwaukee)J. Qin(The University of Western Australia)S. Qiu(Monash University)V. Quetschke(The University of Texas Rio Grande Valley)E. A. Quintero(California Institute of Technology)R. Quitzow-James(University of Oregon)F. J. RaabD. S. Rabeling(Australian National University)H. RadkinsP. Raffai(Eötvös Loránd University)S. Raja(Raja Ramanna Centre for Advanced Technology)C. Rajan(Raja Ramanna Centre for Advanced Technology)M. Rakhmanov(The University of Texas Rio Grande Valley)V. Raymond(Max Planck Institute for Gravitational Physics)J. Read(California State University, Fullerton)C. M. ReedS. Reid(University of the West of Scotland)D. H. Reitze(California Institute of Technology)H. Rew(William & Mary)S. D. Reyes(Syracuse University)K. Riles(University of Michigan)Maria L. Rizzo(Rochester Institute of Technology)N. A. Robertson(California Institute of Technology)R. Robie(University of Glasgow)J. G. Rollins(California Institute of Technology)V. J. Roma(University of Oregon)G. Romanov(William & Mary)J. H. Romie(LIGO Scientific Collaboration)S. Rowan(University of Glasgow)A. Rüdiger(Max Planck Institute for Gravitational Physics)K. RyanS. Sachdev(California Institute of Technology)T. SadeckiL. Sadeghian(University of Wisconsin–Milwaukee)Mairi Sakellariadou(University of London)M. Saleem(Indian Institute of Science Education and Research Thiruvananthapuram)F. Salemi(Max Planck Institute for Gravitational Physics)A. Samajdar(Indian Institute of Science Education and Research Kolkata)L. Sammut(Monash University)E. J. Sanchez(California Institute of Technology)V. SandbergB. Sandeen(Northwestern University)J. R. Sanders(Syracuse University)B. S. Sathyaprakash(Cardiff University)P. R. Saulson(Syracuse University)S. Sato(University of Michigan)R. L. SavageA. Sawadsky(Leibniz University Hannover)P. Schale(University of Oregon)R. Schilling(Max Planck Institute for Gravitational Physics)P. Schmidt(Max Planck Institute for Gravitational Physics)P. Schmidt(California Institute of Technology)R. Schnabel(Universität Hamburg)R. M. S. Schofield(University of Oregon)A. Schönbeck(Universität Hamburg)E. Schreiber(Max Planck Institute for Gravitational Physics)D. Schuette(Leibniz University Hannover)B. F. Schutz(Max Planck Institute for Gravitational Physics)J. Scott(University of Glasgow)S. M. Scott(Australian National University)D. Sellers(LIGO Scientific Collaboration)A. S. Sengupta(Indian Institute of Technology Gandhinagar)A. Sergeev(Institute of Applied Physics)D. A. Shaddock(Australian National University)T. ShafferM. S. Shahriar(Northwestern University)M. Shaltev(Max Planck Institute for Gravitational Physics)B. Shapiro(Stanford University)P. Shawhan(University of Maryland, College Park)A. Sheperd(University of Wisconsin–Milwaukee)D. H. Shoemaker(Massachusetts Institute of Technology)D. M. Shoemaker(Georgia Institute of Technology)K. Siellez(Georgia Institute of Technology)X. Siemens(University of Wisconsin–Milwaukee)D. SiggA. D. Silva(Instituto Nacional de Pesquisas Espaciais)A. Singer(California Institute of Technology)L. P. Singer(Goddard Space Flight Center)A. Singh(Leibniz University Hannover)R. Singh(Louisiana State University)A. M. Sintes(Universitat de les Illes Balears)B. J. J. Slagmolen(Australian National University)J. R. Smith(California State University, Fullerton)N. D. Smith(California Institute of Technology)R. J. E. Smith(California Institute of Technology)E. J. Son✉(National Institute for Mathematical Sciences)B. Sorazu(University of Glasgow)T. Souradeep(Inter-University Centre for Astronomy and Astrophysics)A. K. Srivastava(Institute for Plasma Research)A. Staley(Columbia University)M. Steinke(Max Planck Institute for Gravitational Physics)J. Steinlechner(University of Glasgow)S. Steinlechner(University of Glasgow)D. Steinmeyer(Leibniz University Hannover)B. C. Stephens(University of Wisconsin–Milwaukee)R. Stone(The University of Texas Rio Grande Valley)K. A. Strain(University of Glasgow)N. A. Strauss(Carleton College)S. Strigin(Lomonosov Moscow State University)R. Sturani(ICTP South American Institute for Fundamental Research)A. L. Stuver(LIGO Scientific Collaboration)T. Z. Summerscales(Andrews University)L. Sun(The University of Melbourne)S Sunil(Institute for Plasma Research)P. J. Sutton(Cardiff University)M. J. Szczepańczyk(Embry–Riddle Aeronautical University)D. Talukder(University of Oregon)D. B. Tanner(University of Florida)M. Tápai(University of Szeged)S. P. Tarabrin(Max Planck Institute for Gravitational Physics)A. Taracchini(Max Planck Institute for Gravitational Physics)R. Taylor(California Institute of Technology)T. Theeg(Max Planck Institute for Gravitational Physics)M. P. Thirugnanasambandam(California Institute of Technology)E. G. Thomas(University of Birmingham)M. Thomas(LIGO Scientific Collaboration)P. ThomasK. A. Thorne(LIGO Scientific Collaboration)E. Thrane(Monash University)V. Tiwari(Cardiff University)K. V. Tokmakov(University of Strathclyde)K. Toland(University of Glasgow)C. Tomlinson(University of Sheffield)Z. Tornasi(University of Glasgow)C. Torres(The University of Texas Rio Grande Valley)C I Torrie(California Institute of Technology)D. Töyrä(University of Birmingham)G. Traylor(LIGO Scientific Collaboration)D. Trifirò(University of Mississippi)M. Tse(Massachusetts Institute of Technology)D. Tuyenbayev(The University of Texas Rio Grande Valley)D. Ugolini(Trinity University)B. Krishnan(Tata Institute of Fundamental Research)A. L. Urban(University of Wisconsin–Milwaukee)S. A. Usman(Syracuse University)H. Vahlbruch(Leibniz University Hannover)G. Vajente(California Institute of Technology)G. Valdes(The University of Texas Rio Grande Valley)D. C. Vander‐Hyde(Syracuse University)A A van Veggel(University of Glasgow)S. Vass(California Institute of Technology)R. Vaulin(Massachusetts Institute of Technology)A. Vecchio(University of Birmingham)J. Veitch(University of Birmingham)P. J. Veitch(The University of Adelaide)K. Venkateswara(University of Washington)S. Vinciguerra(University of Birmingham)D. J. Vine(University of the West of Scotland)S. Vitale(Massachusetts Institute of Technology)T. Vo(Syracuse University)C. VorvickD. V. Voss(University of Florida)W. D. Vousden(University of Birmingham)S. P. Vyatchanin(Lomonosov Moscow State University)A. R. Wade(Australian National University)L. E. Wade(Kenyon College)M. Wade(Kenyon College)M. Walker(Louisiana State University)L. Wallace(California Institute of Technology)S. Walsh(Max Planck Institute for Gravitational Physics)H. Wang(University of Birmingham)M. Wang(University of Birmingham)X Wang(Tsinghua University)Y. Wang(The University of Western Australia)R. L. Ward(Australian National University)J. WarnerB. WeaverM. Weinert(Max Planck Institute for Gravitational Physics)A. J. Weinstein(California Institute of Technology)R. Weiss(Massachusetts Institute of Technology)L. Wen(The University of Western Australia)P. Weßels(Max Planck Institute for Gravitational Physics)T. Westphal(Max Planck Institute for Gravitational Physics)K. Wette(Max Planck Institute for Gravitational Physics)J. T. Whelan(Rochester Institute of Technology)B. F. Whiting(University of Florida)R. D. Williams(California Institute of Technology)A. R. Williamson(Cardiff University)J. L. Willis(Abilene Christian University)B. Willke(Leibniz University Hannover)M. H. Wimmer(Leibniz University Hannover)W. Winkler(Max Planck Institute for Gravitational Physics)C. C. Wipf(California Institute of Technology)H. Wittel(Leibniz University Hannover)G. Woan(University of Glasgow)J. Woehler(Max Planck Institute for Gravitational Physics)J. WordenJ. L. Wright(University of Glasgow)D. S. Wu(Max Planck Institute for Gravitational Physics)Guanglei Wu(LIGO Scientific Collaboration)J. Yablon(Northwestern University)W. Yam(Massachusetts Institute of Technology)H. Yamamoto(California Institute of Technology)C. C. Yancey(University of Maryland, College Park)Hang Yu(Massachusetts Institute of Technology)M. Zanolin(Embry–Riddle Aeronautical University)M. Zevin(Northwestern University)L Zhang(California Institute of Technology)M. Zhang(William & Mary)Y. Zhang(Rochester Institute of Technology)C. Zhao(The University of Western Australia)M. Zhou(Northwestern University)Z. Zhou(Northwestern University)X. J. Zhu(The University of Western Australia)M. E. Zucker(California Institute of Technology)S. E. Zuraw(University of Massachusetts Amherst)J. Zweizig(California Institute of Technology)J. Harms(University of Strathclyde)
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.
Pulsars and Gravitational Waves ResearchCold Atom Physics and Bose-Einstein CondensatesGeophysics and Sensor TechnologyPhysicsGravitational waveDetectorSensitivity (control systems)Gravitational-wave observatoryEinstein TelescopeUniverseGravitational-wave astronomyBinary numberAstronomy
Funding
- National Science Foundation
- Massachusetts Institute of Technology
- California Institute of Technology
- Science and Technology Facilities Council
Citations
1,175
FWCI
70.87
field-weighted impact
References
111
Percentile
100%
vs. same field & year
Citations per year
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References
Evidence for Reionization at [ITAL][CLC]z[/CLC][/ITAL] ∼ 6: Detection of a Gunn-Peterson Trough in a [ITAL][CLC]z[/CLC][/ITAL] = 6.28 Quasar
The Astronomical Journal · 2001 · 882 citations
Tidal deformability of neutron stars with realistic equations of state and their gravitational wave signatures in binary inspiral
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology · 2010 · 1,003 citations
Scientific objectives of Einstein Telescope
Classical and Quantum Gravity · 2012 · 524 citations
Advanced Virgo: a second-generation interferometric gravitational wave detector
Classical and Quantum Gravity · 2014 · 3,931 citations
New formalism for two-photon quantum optics. I. Quadrature phases and squeezed states
Physical review. A, General physics · 1985 · 864 citations
Interferometer design of the KAGRA gravitational wave detector
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology · 2013 · 1,016 citations
Sensitivity studies for third-generation gravitational wave observatories
Classical and Quantum Gravity · 2011 · 1,081 citations
Detector configuration of KAGRA–the Japanese cryogenic gravitational-wave detector
Classical and Quantum Gravity · 2012 · 894 citations
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