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Frequency-Dependent Squeezed Vacuum Source for the Advanced Virgo Gravitational-Wave Detector.
Authors :
Acernese F Agathos M Ain A Albanesi S Alléné C Allocca A Amato A Amra C Andia M Andrade T Andres N Andrés-Carcasona M Andrić T Ansoldi S Antier S Apostolatos T Appavuravther EZ Arène M Arnaud N Assiduo M Melo SAS Astone P Aubin F Babak S Badaracco F Bagnasco S Baird J Baka T Ballardin G Baltus G Banerjee B Barneo P Barone F Barsuglia M Barta D Basti A Bawaj M Bazzan M Beirnaert F Bejger M Benedetto V Berbel M Bernuzzi S Bersanetti D Bertolini A Bhardwaj U Bianchi A Bilicki M Bini S Bischi M Bitossi M Bizouard MA Bobba F Boër M Bogaert G Boileau G Boldrini M Bonavena LD Bondarescu R Bondu F Bonnand R Boschi V Boudart V Bouffanais Y Bozzi A Bradaschia C Braglia M Branchesi M Breschi M Briant T Brillet A Brooks J Bruno G Bucci F Bulashenko O Bulik T Bulten HJ Buscicchio R Buskulic D Buy C Cabras G Cabrita R Cagnoli G Calloni E Canepa M Santoro GC Cannavacciuolo M Capocasa E Carapella G Carbognani F Carpinelli M Carullo G Diaz JC Casentini C Caudill S Cavalieri R Cella G Cerdá-Durán P Cesarini E Chaibi W Chanial P Chassande-Mottin E Chaty S Chessa P Chiadini F Chiarini G Chierici R Chincarini A Chiofalo ML Chiummo A Christensen N Chua S Ciani G Ciecielag P Cieślar M Cifaldi M Ciolfi R Clesse S Cleva F Coccia E Codazzo E Cohadon PF Colombo A Colpi M Conti L Cordero-Carrión I Corezzi S Cortese S Coulon JP Coupechoux JF Croquette M Cudell JR Cuoco E Curyło M Dabadie P Canton TD Dall'Osso S Dálya G D'Angelo B Dangoisse G Danilishin S D'Antonio S Dattilo V Davier M Degallaix J De Laurentis M Deléglise S De Lillo F Dell'Aquila D Del Pozzo W De Matteis F Depasse A De Pietri R De Rosa R De Rossi C De Simone R Di Fiore L Di Giorgio C Di Giovanni F Di Giovanni M Di Girolamo T Diksha D Di Lieto A Di Michele A Ding J Di Pace S Di Palma I Di Renzo F D'Onofrio L Dooney T Dorosh O Drago M Ducoin JG Dupletsa U Durante O D'Urso D Duverne PA Eisenmann M Errico L Estevez D Fabrizi F Faedi F Fafone V Favaro G Fays M Fenyvesi E Ferrante I Fidecaro F Figura P Fiori A Fiori I Fittipaldi R Fiumara V Flaminio R Font JA Frasca S Frasconi F Freise A Freitas O Fronzé GG Gadre B Gamba R Garaventa B Garcia-Bellido J Gargiulo J Garufi F Gasbarra C Gemme G Gennai A Ghosh A Giacoppo L Giri P Gissi F Gkaitatzis S Glotin F Goncharov B Gosselin M Gouaty R Grado A Granata M Granata V Greco G Grignani G Grimaldi A Guerra D Guetta D Guidi GM Gulminelli F Guo Y Gupta P Gutierrez N Haegel L Halim O Hannuksela O Harder T Haris K Harmark T Harms J Haskell B Heidmann A Heitmann H Hello P Hemming G Hennes E Hennig JS Hennig M Hild S Hofman D Holland NA Hui V Iandolo GA Idzkowski B Iess A Iorio G Iosif P Jacqmin T Jacquet PE Janquart J Janssens K Jaraba S Jaranowski P Jasal P Juste V Kalaghatgi C Karathanasis C Katsanevas S Kéfélian F Koekoek G Koley S Kolstein M Kranzhoff SL Królak A Kuijer P Kuroyanagi S Lagabbe P Laghi D Lalleman M Lamberts A La Rana A La Rosa I Lartaux-Vollard A Lazzaro C Leaci P Lemaître A Lenti M Leonova E Lequime M Leroy N Letendre N Lethuillier M Leyde K Linde F London L Longo A Portilla ML Lorenzini M Loriette V Losurdo G Lumaca D Macquet A Magazzù C Maggiore R Magnozzi M Majorana E Man N Mangano V Mantovani M Mapelli M Marchesoni F Pina DM Marion F Marquina A Marsat S Martelli F Martinez M Martinez V Masserot A Mastrodicasa M Mastrogiovanni S Meijer Q Menendez-Vazquez A Mereni L Merzougui M Miani A Michel C Miller A Miller B Milotti E Minenkov Y Mir LM Miravet-Tenés M Mitchell AL Mondal C Montani M Morawski F Morras G Moscatello A Mours B Mow-Lowry CM Msihid E Muciaccia F Mukherjee S Nagar A Napolano V Nardecchia I Narola H Naticchioni L Neilson J Nesseris S Nguyen C Nieradka G Nissanke S Nitoglia E Nocera F Novak J No Siles JFN Oertel M Oganesyan G Oliveri R Orselli M Palomba C Pang PTH Pannarale F Paoletti F Paoli A Paolone A Pappas G Parisi A Pascucci D Pasqualetti A Passaquieti R Passuello D Patricelli B Pedurand R Pegna R Pegoraro M Perego A Pereira A Périgois C Perreca A Perriès S Perry JW Pesios D Petrillo C Phukon KS Piccinni OJ Pichot M Piendibene M Piergiovanni F Pierini L Pierra G Pierro V Pillant G Pillas M Pilo F Pinard L Pinto IM Pinto M Pinto M Piotrzkowski K Placidi A Placidi E Plastino W Poggiani R Polini E Porcelli E Portell J Porter EK Poulton R Pracchia M Pradier T Principe M Prodi GA Prosposito P Puecher A Punturo M Puosi F Puppo P Raaijmakers G Radulesco N Rapagnani P Razzano M Regimbau T Rei L Rettegno P Revenu B Reza A Rezaei AS Ricci F Rinaldi S Robinet F Rocchi A Rolland L Romanelli M Romano R Romero A Ronchini S Rosa L Rosińska D Roy S Rozza D Ruggi P Morales ER Saffarieh P Salafia OS Salconi L Salemi F Sallé M Samajdar A Sanchis-Gual N Sanuy A Sasli A Sassi P Sassolas B Sayah S Schmidt S Seglar-Arroyo M Sentenac D Sequino V Servignat G Setyawati Y Shcheblanov NS Sieniawska M Silenzi L Singh N Singha A Sipala V Soldateschi J Sordini V Sorrentino F Sorrentino N Soulard R Spagnuolo V Spera M Spinicelli P Stachie C Steer DA Steinlechner J Steinlechner S Stergioulas N Stratta G Suchenek M Sur A Suresh J Swinkels BL Syx A Szewczyk P Tacca M Tamanini N Tanasijczuk AJ Martín ENTS Taranto C Tonelli M Torres-Forné A E Melo IT Tournefier E Trapananti A Travasso F Trenado J Tringali MC Troiano L Trovato A Trozzo L Tsang KW Turbang K Turconi M Turski C Ubach H Utina A Valentini M Vallero S van Bakel N van Beuzekom M van Dael M van den Brand JFJ Van Den Broeck C van der Sluys M Van de Walle A van Dongen J van Haevermaet H van Heijningen JV van Ranst Z van Remortel N Vardaro M Vasúth M Vedovato G Verdier P Verkindt D Verma P Vetrano F Viceré A Vinet JY Viret S Virtuoso A Vocca H Walet RC Was M Yadav N Zadrożny A Zelenova T Zendri JP Zhao Y Zerrad M Vahlbruch H Mehmet M Lück H Danzmann K
Source :
Physical review letters [Phys Rev Lett] 2023 Jul 28; Vol. 131 (4), pp. 041403.
Publication Year :
2023
Abstract
In this Letter, we present the design and performance of the frequency-dependent squeezed vacuum source that will be used for the broadband quantum noise reduction of the Advanced Virgo Plus gravitational-wave detector in the upcoming observation run. The frequency-dependent squeezed field is generated by a phase rotation of a frequency-independent squeezed state through a 285 m long, high-finesse, near-detuned optical resonator. With about 8.5 dB of generated squeezing, up to 5.6 dB of quantum noise suppression has been measured at high frequency while close to the filter cavity resonance frequency, the intracavity losses limit this value to about 2 dB. Frequency-dependent squeezing is produced with a rotation frequency stability of about 6 Hz rms, which is maintained over the long term. The achieved results fulfill the frequency dependent squeezed vacuum source requirements for Advanced Virgo Plus. With the current squeezing source, considering also the estimated squeezing degradation induced by the interferometer, we expect a reduction of the quantum shot noise and radiation pressure noise of up to 4.5 dB and 2 dB, respectively.
Details
Language :
English
ISSN :
1079-7114
Volume :
131
Issue :
4
Database :
MEDLINE
Journal :
Physical review letters
Publication Type :
Academic Journal
Accession number :
37566847
Full Text :
https://doi.org/10.1103/PhysRevLett.131.041403