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Acernese F, Agathos M, Aiello L, Allocca A, Amato A, Ansoldi S, Antier S, Arène M, Arnaud N, Ascenzi S, Astone P, Aubin F, Babak S, Bacon P, Badaracco F, Bader MKM, Baird J, Baldaccini F, Ballardin G, Baltus G, Barbieri C, Barneo P, Barone F, Barsuglia M, Barta D, Basti A, Bawaj M, Bazzan M, Bejger M, Belahcene I, Bernuzzi S, Bersanetti D, Bertolini A, Bischi M, Bitossi M, Bizouard MA, Bobba F, Boer M, Bogaert G, Bondu F, Bonnand R, Boom BA, Boschi V, Bouffanais Y, Bozzi A, Bradaschia C, Branchesi M, Breschi M, Briant T, Brighenti F, Brillet A, Brooks J, Bruno G, Bulik T, Bulten HJ, Buskulic D, Cagnoli G, Calloni E, Canepa M, Carapella G, Carbognani F, Carullo G, Casanueva Diaz J, Casentini C, Castañeda J, Caudill S, Cavalier F, Cavalieri R, Cella G, Cerdá-Durán P, Cesarini E, Chaibi O, Chassande-Mottin E, Chiadini F, Chierici R, Chincarini A, Chiummo A, Christensen N, Chua S, Ciani G, Ciecielag P, Cieślar M, Ciolfi R, Cipriano F, Cirone A, Clesse S, Cleva F, Coccia E, Cohadon PF, Cohen D, Colpi M, Conti L, Cordero-Carrión I, Corezzi S, Corre D, Cortese S, Coulon JP, Croquette M, Cudell JR, Cuoco E, et alAcernese F, Agathos M, Aiello L, Allocca A, Amato A, Ansoldi S, Antier S, Arène M, Arnaud N, Ascenzi S, Astone P, Aubin F, Babak S, Bacon P, Badaracco F, Bader MKM, Baird J, Baldaccini F, Ballardin G, Baltus G, Barbieri C, Barneo P, Barone F, Barsuglia M, Barta D, Basti A, Bawaj M, Bazzan M, Bejger M, Belahcene I, Bernuzzi S, Bersanetti D, Bertolini A, Bischi M, Bitossi M, Bizouard MA, Bobba F, Boer M, Bogaert G, Bondu F, Bonnand R, Boom BA, Boschi V, Bouffanais Y, Bozzi A, Bradaschia C, Branchesi M, Breschi M, Briant T, Brighenti F, Brillet A, Brooks J, Bruno G, Bulik T, Bulten HJ, Buskulic D, Cagnoli G, Calloni E, Canepa M, Carapella G, Carbognani F, Carullo G, Casanueva Diaz J, Casentini C, Castañeda J, Caudill S, Cavalier F, Cavalieri R, Cella G, Cerdá-Durán P, Cesarini E, Chaibi O, Chassande-Mottin E, Chiadini F, Chierici R, Chincarini A, Chiummo A, Christensen N, Chua S, Ciani G, Ciecielag P, Cieślar M, Ciolfi R, Cipriano F, Cirone A, Clesse S, Cleva F, Coccia E, Cohadon PF, Cohen D, Colpi M, Conti L, Cordero-Carrión I, Corezzi S, Corre D, Cortese S, Coulon JP, Croquette M, Cudell JR, Cuoco E, Curylo M, D'Angelo B, D'Antonio S, Dattilo V, Davier M, Degallaix J, De Laurentis M, Deléglise S, Del Pozzo W, De Pietri R, De Rosa R, De Rossi C, Dietrich T, Di 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, Drago M, Ducoin JG, Durante O, D'Urso D, Eisenmann M, Errico L, Estevez D, Fafone V, Farinon S, Feng F, Fenyvesi E, Ferrante I, Fidecaro F, Fiori I, Fiorucci D, Fittipaldi R, Fiumara V, Flaminio R, Font JA, Fournier JD, Frasca S, Frasconi F, Frey V, Fronzè G, Garufi F, Gemme G, Genin E, Gennai A, Ghosh A, Giacomazzo B, Gosselin M, Gouaty R, Grado A, Granata M, Greco G, Grignani G, Grimaldi A, Grimm SJ, Gruning P, Guidi GM, Guixé G, Guo Y, Gupta P, Halim O, Harder T, Harms J, Heidmann A, Heitmann H, Hello P, Hemming G, Hennes E, Hinderer T, Hofman D, Huet D, Hui V, Idzkowski B, Iess A, Intini G, Isac JM, Jacqmin T, Jaranowski P, Jonker RJG, Katsanevas S, Kéfélian F, Khan I, Khetan N, Koekoek G, Koley S, Królak A, Kutynia A, Laghi D, Lamberts A, La Rosa I, Lartaux-Vollard A, Lazzaro C, Leaci P, Leroy N, Letendre N, Linde F, Llorens-Monteagudo M, Longo A, Lorenzini M, Loriette V, Losurdo G, Lumaca D, Macquet A, Majorana E, Maksimovic I, Man N, Mangano V, Mantovani M, Mapelli M, Marchesoni F, Marion F, Marquina A, Marsat S, Martelli F, Martinez V, Masserot A, Mastrogiovanni S, Mejuto Villa E, Mereni L, Merzougui M, Metzdorff R, Miani A, Michel C, Milano L, Miller A, Milotti E, Minazzoli O, Minenkov Y, Montani M, Morawski F, Mours B, Muciaccia F, Nagar A, Nardecchia I, Naticchioni L, Neilson J, Nelemans G, Nguyen C, Nichols D, Nissanke S, Nocera F, Oganesyan G, Olivetto C, Pagano G, Pagliaroli G, Palomba C, Pang PTH, Pannarale F, Paoletti F, Paoli A, Pascucci D, Pasqualetti A, Passaquieti R, Passuello D, Patricelli B, Perego A, Pegoraro M, Périgois C, Perreca A, Perriès S, Phukon KS, Piccinni OJ, Pichot M, Piendibene M, Piergiovanni F, Pierro V, Pillant G, Pinard L, Pinto IM, Piotrzkowski K, Plastino W, Poggiani R, Popolizio P, Porter EK, Prevedelli M, Principe M, Prodi GA, Punturo M, Puppo P, Raaijmakers G, Radulesco N, Rapagnani P, Razzano M, Regimbau T, Rei L, Rettegno P, Ricci F, Riemenschneider G, Robinet F, Rocchi A, Rolland L, Romanelli M, Romano R, Rosińska D, Ruggi P, Salafia OS, Salconi L, Samajdar A, Sanchis-Gual N, Santos E, Sassolas B, Sauter O, Sayah S, Sentenac D, Sequino V, Sharma A, Sieniawska M, Singh N, Singhal A, Sipala V, Sordini V, Sorrentino F, Spera M, Stachie C, Steer DA, Stratta G, Sur A, Swinkels BL, Tacca M, Tanasijczuk AJ, Tapia San Martin EN, Tiwari S, Tonelli M, Torres-Forné A, Tosta E Melo I, Travasso F, Tringali MC, Trovato A, Tsang KW, Turconi M, Valentini M, van Bakel N, van Beuzekom M, van den Brand JFJ, Van Den Broeck C, van der Schaaf L, Vardaro M, Vasúth M, Vedovato G, Verkindt D, Vetrano F, Viceré A, Vinet JY, Vocca H, Walet R, Was M, Zadrożny A, Zelenova T, Zendri JP, Vahlbruch H, Mehmet M, Lück H, Danzmann K. Increasing the Astrophysical Reach of the Advanced Virgo Detector via the Application of Squeezed Vacuum States of Light. PHYSICAL REVIEW LETTERS 2019; 123:231108. [PMID: 31868444 DOI: 10.1103/physrevlett.123.231108] [Show More Authors] [Citation(s) in RCA: 85] [Impact Index Per Article: 14.2] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/11/2019] [Indexed: 06/10/2023]
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 application of this quantum technology to improve the shot noise limited sensitivity of the Advanced Virgo gravitational-wave detector. A sensitivity enhancement of up to 3.2±0.1 dB beyond the shot noise limit is achieved. This nonclassical improvement corresponds to a 5%-8% increase of the binary neutron star horizon. The squeezing injection was fully automated and over the first 5 months of the third joint LIGO-Virgo observation run O3 squeezing was applied for more than 99% of the science time. During this period several gravitational-wave candidates have been recorded.
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