Literature DB >> 31868444

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

F Acernese1,2, M Agathos3, L Aiello4,5, A Allocca6, A Amato7, S Ansoldi8,9, S Antier10, M Arène10, N Arnaud11,12, S Ascenzi4,13, P Astone14, F Aubin15, S Babak10, P Bacon10, F Badaracco4,5, M K M Bader16, J Baird10, F Baldaccini17,18, G Ballardin12, G Baltus19, C Barbieri20,21, P Barneo22, F Barone2,23, M Barsuglia10, D Barta24, A Basti6,25, M Bawaj18,26, M Bazzan27,28, M Bejger29, I Belahcene11, S Bernuzzi3, D Bersanetti30, A Bertolini16, M Bischi31,32, M Bitossi6,12, M A Bizouard33, F Bobba34,35, M Boer33, G Bogaert33, F Bondu36, R Bonnand15, B A Boom16, V Boschi6, Y Bouffanais27,28, A Bozzi12, C Bradaschia6, M Branchesi4,5, M Breschi3, T Briant37, F Brighenti31,32, A Brillet33, J Brooks12, G Bruno38, T Bulik39, H J Bulten16,40, D Buskulic15, G Cagnoli7, E Calloni2,41, M Canepa30,42, G Carapella34,35, F Carbognani12, G Carullo6,25, J Casanueva Diaz6, C Casentini13,43, J Castañeda22, S Caudill16, F Cavalier11, R Cavalieri12, G Cella6, P Cerdá-Durán44, E Cesarini13,45, O Chaibi33, E Chassande-Mottin10, F Chiadini35,46, R Chierici47, A Chincarini30, A Chiummo12, N Christensen33, S Chua37, G Ciani27,28, P Ciecielag29, M Cieślar29, R Ciolfi28,48, F Cipriano33, A Cirone30,42, S Clesse38, F Cleva33, E Coccia4,5, P-F Cohadon37, D Cohen11, M Colpi20,21, L Conti28, I Cordero-Carrión49, S Corezzi17,18, D Corre11, S Cortese12, J-P Coulon33, M Croquette37, J-R Cudell19, E Cuoco12, M Curylo39, B D'Angelo30,42, S D'Antonio13, V Dattilo12, M Davier11, J Degallaix50, M De Laurentis2,41, S Deléglise37, W Del Pozzo6,25, R De Pietri51,52, R De Rosa2,41, C De Rossi12, T Dietrich16, L Di Fiore2, C Di Giorgio34,35, F Di Giovanni44, M Di Giovanni53,54, T Di Girolamo2,41, A Di Lieto6,25, S Di Pace14,55, I Di Palma14,55, F Di Renzo6,25, M Drago4,5, J-G Ducoin11, O Durante34,35, D D'Urso56,57, M Eisenmann15, L Errico2,41, D Estevez15, V Fafone4,13,43, S Farinon30, F Feng10, E Fenyvesi24,58, I Ferrante6,25, F Fidecaro6,25, I Fiori12, D Fiorucci4,5, R Fittipaldi35,59, V Fiumara35,60, R Flaminio15,61, J A Font44,62, J-D Fournier33, S Frasca14,55, F Frasconi6, V Frey11, G Fronzè63, F Garufi2,41, G Gemme30, E Genin12, A Gennai6, Archisman Ghosh16,64,65,66, B Giacomazzo53,54, M Gosselin6,12,25, R Gouaty15, A Grado2,67, M Granata50, G Greco31,32, G Grignani17,18, A Grimaldi53,54, S J Grimm4,5, P Gruning11, G M Guidi31,32, G Guixé22, Y Guo16, P Gupta16, O Halim4,5, T Harder33, J Harms4,5, A Heidmann37, H Heitmann33, P Hello11, G Hemming12, E Hennes16, T Hinderer16,64,66, D Hofman50, D Huet11, V Hui15, B Idzkowski39, A Iess13,43, G Intini14,55, J-M Isac37, T Jacqmin37, P Jaranowski68, R J G Jonker16, S Katsanevas12, F Kéfélian33, I Khan4,13, N Khetan4,5, G Koekoek16,69, S Koley16, A Królak70,71, A Kutynia70, D Laghi6,25, A Lamberts33,72, I La Rosa15, A Lartaux-Vollard11, C Lazzaro28, P Leaci14,55, N Leroy11, N Letendre15, F Linde16,73, M Llorens-Monteagudo44, A Longo74,75, M Lorenzini4,5, V Loriette76, G Losurdo6, D Lumaca13,43, A Macquet33, E Majorana14, I Maksimovic76, N Man33, V Mangano14,55, M Mantovani12, M Mapelli27,28, F Marchesoni18,26,77, F Marion15, A Marquina49, S Marsat10, F Martelli31,32, V Martinez7, A Masserot15, S Mastrogiovanni10, E Mejuto Villa35,78, L Mereni50, M Merzougui33, R Metzdorff37, A Miani53,54, C Michel50, L Milano2,41, A Miller14,55, E Milotti9,79, O Minazzoli33,80, Y Minenkov13, M Montani31,32, F Morawski29, B Mours81, F Muciaccia14,55, A Nagar45,63,82, I Nardecchia13,43, L Naticchioni14,55, J Neilson35,78, G Nelemans16,83, C Nguyen10, D Nichols16,66, S Nissanke16,66, F Nocera12, G Oganesyan4,5, C Olivetto12, G Pagano6,25, G Pagliaroli4,5, C Palomba14, P T H Pang16, F Pannarale14,55, F Paoletti6, A Paoli12, D Pascucci16, A Pasqualetti12, R Passaquieti6,25, D Passuello6, B Patricelli6,25, A Perego53,54, M Pegoraro28, C Périgois15, A Perreca53,54, S Perriès47, K S Phukon16,73, O J Piccinni14,55, M Pichot33, M Piendibene6,25, F Piergiovanni31,32, V Pierro35,78, G Pillant12, L Pinard50, I M Pinto35,45,78, K Piotrzkowski38, W Plastino74,75, R Poggiani6,25, P Popolizio12, E K Porter10, M Prevedelli84, M Principe35,45,78, G A Prodi53,54, M Punturo18, P Puppo14, G Raaijmakers16,66, N Radulesco33, P Rapagnani14,55, M Razzano6,25, T Regimbau15, L Rei30, P Rettegno63,85, F Ricci14,55, G Riemenschneider63,85, F Robinet11, A Rocchi13, L Rolland15, M Romanelli36, R Romano1,2, D Rosińska39, P Ruggi12, O S Salafia20,21,86, L Salconi12, A Samajdar16, N Sanchis-Gual87, E Santos33, B Sassolas50, O Sauter15, S Sayah50, D Sentenac12, V Sequino30, A Sharma4,5, M Sieniawska29, N Singh39, A Singhal4,14, V Sipala56,57, V Sordini47, F Sorrentino30, M Spera27,28, C Stachie33, D A Steer10, G Stratta32,88, A Sur29, B L Swinkels16, M Tacca16, A J Tanasijczuk38, E N Tapia San Martin16, S Tiwari53,54, M Tonelli6,25, A Torres-Forné89, I Tosta E Melo56,57, F Travasso18,26, M C Tringali39, A Trovato10, K W Tsang16, M Turconi33, M Valentini53,54, N van Bakel16, M van Beuzekom16, J F J van den Brand16,40,69, C Van Den Broeck16,90, L van der Schaaf16, M Vardaro16,73, M Vasúth24, G Vedovato28, D Verkindt15, F Vetrano31,32, A Viceré31,32, J-Y Vinet33, H Vocca17,18, R Walet16, M Was15, A Zadrożny70, T Zelenova12, J-P Zendri28, Henning Vahlbruch91, Moritz Mehmet91, Harald Lück91, Karsten Danzmann91.   

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.

Entities:  

Year:  2019        PMID: 31868444     DOI: 10.1103/PhysRevLett.123.231108

Source DB:  PubMed          Journal:  Phys Rev Lett        ISSN: 0031-9007            Impact factor:   9.161


  3 in total

1.  Quantum fluctuations have been shown to affect macroscopic objects.

Authors:  Valeria Sequino; Mateusz Bawaj
Journal:  Nature       Date:  2020-07       Impact factor: 49.962

Review 2.  The deep space quantum link: prospective fundamental physics experiments using long-baseline quantum optics.

Authors:  Makan Mohageg; Luca Mazzarella; Charis Anastopoulos; Jason Gallicchio; Bei-Lok Hu; Thomas Jennewein; Spencer Johnson; Shih-Yuin Lin; Alexander Ling; Christoph Marquardt; Matthias Meister; Raymond Newell; Albert Roura; Wolfgang P Schleich; Christian Schubert; Dmitry V Strekalov; Giuseppe Vallone; Paolo Villoresi; Lisa Wörner; Nan Yu; Aileen Zhai; Paul Kwiat
Journal:  EPJ Quantum Technol       Date:  2022-10-08       Impact factor: 7.000

3.  Hilbert-Schmidt speed as an efficient figure of merit for quantum estimation of phase encoded into the initial state of open n-qubit systems.

Authors:  Hossein Rangani Jahromi; Rosario Lo Franco
Journal:  Sci Rep       Date:  2021-03-29       Impact factor: 4.379

  3 in total

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