Increasing the Astrophysical Reach of the Advanced Virgo Detector via the Application of Squeezed Vacuum States of Light.

F, Acernese; M, Agathos; L, Aiello; A, Allocca; A, Amato; S, Ansoldi; S, Antier; M, Arène; N, Arnaud; S, Ascenzi; P, Astone; F, Aubin; S, Babak; P, Bacon; F, Badaracco; MKM, Bader; J, Baird; F, Baldaccini; G, Ballardin; G, Baltus; C, Barbieri; P, Barneo; F, Barone; M, Barsuglia; D, Barta; A, Basti; M, Bawaj; M, Bazzan; M, Bejger; I, Belahcene; S, Bernuzzi; D, Bersanetti; A, Bertolini; M, Bischi; M, Bitossi; MA, Bizouard; F, Bobba; M, Boer; G, Bogaert; F, Bondu; R, Bonnand; BA, Boom; V, Boschi; Y, Bouffanais; A, Bozzi; C, Bradaschia; M, Branchesi; M, Breschi; T, Briant; F, Brighenti; A, Brillet; J, Brooks; G, Bruno; T, Bulik; HJ, Bulten; D, Buskulic; G, Cagnoli; E, Calloni; M, Canepa; G, Carapella; F, Carbognani; G, Carullo; Diaz J, Casanueva; C, Casentini; J, Castañeda; S, Caudill; F, Cavalier; R, Cavalieri; G, Cella; P, Cerdá-Durán; E, Cesarini; O, Chaibi; E, Chassande-Mottin; F, Chiadini; R, Chierici; A, Chincarini; A, Chiummo; N, Christensen; S, Chua; G, Ciani; P, Ciecielag; M, Cieślar; R, Ciolfi; F, Cipriano; A, Cirone; S, Clesse; F, Cleva; E, Coccia; PF, Cohadon; D, Cohen; M, Colpi; L, Conti; I, Cordero-Carrión; S, Corezzi; D, Corre; S, Cortese; JP, Coulon; M, Croquette; JR, Cudell; E, Cuoco; M, Curylo; B, D'Angelo; S, D'Antonio; V, Dattilo; M, Davier; J, Degallaix; Laurentis M, De; S, Deléglise; Pozzo W, Del; Pietri R, De; Rosa R, De; Rossi C, De; T, Dietrich; Fiore L, Di; Giorgio C, Di; Giovanni F, Di; Giovanni M, Di; Girolamo T, Di; Lieto A, Di; Pace S, Di; Palma I, Di; Renzo F, Di; M, Drago; JG, Ducoin; O, Durante; D, D'Urso; M, Eisenmann; L, Errico; D, Estevez; V, Fafone; S, Farinon; F, Feng; E, Fenyvesi; I, Ferrante; F, Fidecaro; I, Fiori; D, Fiorucci; R, Fittipaldi; V, Fiumara; R, Flaminio; JA, Font; JD, Fournier; S, Frasca; F, Frasconi; V, Frey; G, Fronzè; F, Garufi; G, Gemme; E, Genin; A, Gennai; A, Ghosh; B, Giacomazzo; M, Gosselin; R, Gouaty; A, Grado; M, Granata; G, Greco; G, Grignani; A, Grimaldi; SJ, Grimm; P, Gruning; GM, Guidi; G, Guixé; Y, Guo; P, Gupta; O, Halim; T, Harder; J, Harms; A, Heidmann; H, Heitmann; P, Hello; G, Hemming; E, Hennes; T, Hinderer; D, Hofman; D, Huet; V, Hui; B, Idzkowski; A, Iess; G, Intini; JM, Isac; T, Jacqmin; P, Jaranowski; RJG, Jonker; S, Katsanevas; F, Kéfélian; I, Khan; N, Khetan; G, Koekoek; S, Koley; A, Królak; A, Kutynia; D, Laghi; A, Lamberts; Rosa I, La; A, Lartaux-Vollard; C, Lazzaro; P, Leaci; N, Leroy; N, Letendre

doi:10.1103/physrevlett.123.231108

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Increasing the Astrophysical Reach of the Advanced Virgo Detector via the Application of Squeezed Vacuum States of Light.

Shared by NobleBlocks on Dec 1, 2019 • 12:00 AM UTC

Authors:

Acernese F

Agathos M

Aiello L

Abstract

Current interferometric gravitational-wave detectors are limited by quantum noise over a wide range of their measurement bandwidth. One method to overcome the quantum limit is the injection of squeezed vacuum states of light into the interferometer's dark port. Here, we report on the successful appl...

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