R
R. Flaminio
Researcher at National Institutes of Natural Sciences, Japan
Publications - 540
Citations - 89428
R. Flaminio is an academic researcher from National Institutes of Natural Sciences, Japan. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 103, co-authored 510 publications receiving 71841 citations. Previous affiliations of R. Flaminio include University of Tokyo & University of Savoy.
Papers
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Journal ArticleDOI
Twin mirrors for laser interferometric gravitational-wave detectors.
Benoit Sassolas,Quentin Benoit,R. Flaminio,D. Forest,J. Franc,Massimo Galimberti,Aline Lacoudre,Christophe Michel,J.-L. Montorio,N. Morgado,L. Pinard +10 more
TL;DR: The realization and the characterization of the first twin large low-loss mirrors with transmissions differing by less than 0.01% are described.
Scientific potential of Einstein Telescope
Bangalore Suryanarayana Sathyaprakash,M. R. Abernathy,Fausto Acernese,P. Amaro-Seoane,P. Amaro-Seoane,Nils Andersson,K. Arun,Fabrizio Barone,B. Barr,M. Barsuglia,M. G. Beker,N. Beveridge,S. Birindelli,Suvadeep Bose,L. Bosi,S. Braccini,C. Bradaschia,Tomasz Bulik,Enrico Calloni,G. Cella,E. Chassande-Mottin,Simon Chelkowski,Andrea Chincarini,John A. Clark,E. Coccia,C. N. Colacino,J. Colas,A. Cumming,Liam Cunningham,E. Cuoco,S. L. Danilishin,Karsten Danzmann,R. De Salvo,T. Dent,R. De Rosa,L. Di Fiore,A. Di Virgilio,M. Doets,V. Fafone,Paolo Falferi,R. Flaminio,J. Franc,F. Frasconi,Andreas Freise,D. Friedrich,Paul Fulda,Jonathan R. Gair,G. Gemme,E. Genin,A. Gennai,A. Giazotto,Kostas Glampedakis,C. Gräf,M. Granata,Hartmut Grote,G. M. Guidi,A. Gurkovsky,G. D. Hammond,Mark Hannam,Jan Harms,D. Heinert,Martin Hendry,Ik Siong Heng,Eric Hennes,Stefan Hild,J. H. Hough,Sascha Husa,S. H. Huttner,Gareth Jones,F. Y. Khalili,Keiko Kokeyama,Kostas D. Kokkotas,Badri Krishnan,Tenglin Li,M. Lorenzini,Harald Lück,Ettore Majorana,Ilya Mandel,Ilya Mandel,Vuk Mandic,M. Mantovani,I. W. Martin,C. Michel,Y. Minenkov,N. Morgado,S. Mosca,B. Mours,H. Müller-Ebhardt,P. G. Murray,Ronny Nawrodt,Ronny Nawrodt,John Nelson,Richard O'Shaughnessy,Christian D. Ott,C. Palomba,A. Paoli,G. Parguez,A. Pasqualetti,R. Passaquieti,D. Passuello,L. Pinard,Wolfango Plastino,Rosa Poggiani,P. Popolizio,Mirko Prato,M. Punturo,P. Puppo,D. S. Rabeling,István Rácz,P. Rapagnani,Jocelyn Read,T. Regimbau,H. Rehbein,Stuart Reid,Luciano Rezzolla,F. Ricci,F. Richard,A. Rocchi,Sheila Rowan,A. Rüdiger,Lucía Santamaría,B. Sassolas,Roman Schnabel,C. Schwarz,Paul Seidel,A. M. Sintes,Kentaro Somiya,F. C. Speirits,K. Speirits,K. A. Strain,S. E. Strigin,Patrick J. Sutton,S. P. Tarabrin,A. Thüring,J. F. J. van den Brand,M. van Veggel,C. Van Den Broeck,Alberto Vecchio,John Veitch,F. Vetrano,A. Viceré,Sergey P. Vyatchanin,B. Vyatchanin,Graham Woan,Kazuhiro Yamamoto +144 more
TL;DR: The advanced interferometer network will herald a new era in observational astronomy as mentioned in this paper, and there is a very strong science case to go beyond the advanced detector network and build detectors that operate in a frequency range from 1 Hz to 10 kHz, with sensitivity a factor 10 better in amplitude.
The Virgo interferometric gravitational antenna
Fausto Acernese,P. Amico,M. Alshourbagy,Sofiane Aoudia,Saverio Avino,D. Babusci,G. Ballardin,Regis Barille,Fabrizio Barone,Lisa Barsotti,M. Barsuglia,F. Beauville,M. A. Bizouard,C. Boccara,François Bondu,L. Bosi,C. Bradaschia,S. Braccini,A. Brillet,V. Brisson,L. Brocco,D. Buskulic,Enrico Calloni,E. Campagna,F. Cavalier,R. Cavalieri,G. Cella,E. Chassande-Mottin,Christian Corda,A.-C. Clapson,F. Cleva,J.-P. Coulon,E. Cuoco,V. Dattilo,M. Davier,R. T. DeRosa,L. Difiore,A. Divirgilio,B. Dujardin,Antonio Eleuteri,D. Enard,I. Ferrante,F. Fidecaro,I. Fiori,R. Flaminio,J.-D. Fournier,S. Frasca,F. Frasconi,Andreas Freise,Luca Gammaitoni,A. Gennai,A. Giazotto,G. Giordano,L. Giordano,R. Gouaty,D. Grosjean,G. M. Guidi,S. Hebri,H. Heitmann,Patrice Hello,L. Holloway,S. Kreckelbergh,P. La Penna,V. Loriette,M. Loupias,G. Losurdo,J.-M. Mackowski,Ettore Majorana,C. N. Man,M. Mantovani,Fabio Marchesoni,F. Marion,J. Marque,F. Martelli,A. Masserot,M. Mazzoni,Leopoldo Milano,C. Moins,Julien Moreau,N. Morgado,B. Mours,Archana Pai,C. Palomba,F. Paoletti,Silvio Pardi,A. Pasqualetti,R. Passaquieti,D. Passuello,B. Perniola,F. Piergiovanni,L. Pinard,Rosa Poggiani,M. Punturo,P. Puppo,Ketevan Qipiani,P. Rapagnani,V. Reita,A. Remillieux,F. Ricci,Iolanda Ricciardi,P. Ruggi,Guido Russo,Salvatore Solimeno,A. Spallicci,Ruggero Stanga,R. Taddei,D. Tombolato,M. Tonelli,Alessandra Toncelli,E. Tournefier,F. Travasso,G. Vajente,D. Verkindt,F. Vetrano,A. Viceré,J-Y. Vinet,H. Vocca,M. Yvert,Zhen Zhang +118 more
TL;DR: In this paper, various techniques developed in order to reach its target extreme performance are outlined, and the 3-km-long Virgo gravitational wave antenna, which will be particularly sensitive in the low frequency range (10-100 Hz) is presently in its commissioning phase.
Advanced Virgo Status
Jerome Degallaix,T. Accadia,Fausto Acernese,M. Agathos,A. Allocca,P. Astone,G. Ballardin,Fabrizio Barone,M. Barsuglia,A. Basti,Th. S. Bauer,M. Bebronne,M. Bejger,M. G. Beker,M. Bitossi,M. A. Bizouard,M. Blom,François Bondu,L. Bonelli,R. Bonnand,V. Boschi,L. Bosi,B. Bouhou,C. Bradaschia,M. Branchesi,Tristan Briant,A. Brillet,V. Brisson,Tomasz Bulik,H. J. Bulten,D. Buskulic,Christelle Lesvigne-Buy,G. Cagnoli,Enrico Calloni,Benjamin Canuel,F. Carbognani,F. Cavalier,R. Cavalieri,G. Cella,E. Cesarini,E. Chassande-Mottin,Andrea Chincarini,A. Chiummo,F. Cleva,E. Coccia,P.-F. Cohadon,C. N. Colacino,A. Colla,M. Colombini,A. Conte,J.-P. Coulon,E. Cuoco,S. D'Antonio,V. Dattilo,M. Davier,R. Day,R. De Rosa,G. Debreczeni,W. Del Pozzo,L. Di Fiore,A. Di Lieto,A. Di Virgilio,A. Dietz,M. Drago,G. Endroczi,V. Fafone,I. Ferrante,Federico Ferrini,F. Fidecaro,I. Fiori,R. Flaminio,L. A. Forte,J.-D. Fournier,J. Franc,Stefaan Franco,S. Frasca,F. Frasconi,M. Galimberti,Luca Gammaitoni,F. Garufi,M. E. Gáspár,G. Gemme,E. Genin,A. Gennai,A. Giazotto,R. Gouaty,M. Granata,G. M. Guidi,Antoine Heidmann,H. Heitmann,P. Hello,G. Hemming,Piotr Jaranowski,R. J. G. Jonker,M. Kasprzack,Irina Kowalska,A. Królak,N. Leroy,N. Letendre,Tenglin Li,M. Lorenzini,V. Loriette,G. Losurdo,Ettore Majorana,I. Maksimovic,V. Malvezzi,N. Man,M. Mantovani,Fabio Marchesoni,F. Marion,J. Marque,F. Martelli,A. Masserot,J. Meidam,Christine Michel,L. Milano,Y. Minenkov,M. Mohan,N. Morgado,Simona Mosca,B. Mours,L. Naticchioni,Igor Neri,F. Nocera,L. Palladino,C. Palomba,F. Paoletti,R. Paoletti,M. Parisi,A. Pasqualetti,R. Passaquieti,D. Passuello,M. Pichot,F. Piergiovanni,L. Pinard,Rosa Poggiani,G. A. Prodi,M. Punturo,P. Puppo,D. S. Rabeling,István Rácz,P. Rapagnani,V. Re,T. Regimbau,F. Ricci,F. Robinet,A. Rocchi,L. Rolland,Rocco Romano,D. Rosińska,P. Ruggi,E. Saracco,B. Sassolas,D. Sentenac,L. Sperandio,Riccardo Sturani,B. L. Swinkels,M. Tacca,L. Taffarello,A. P. M. ter Braack,Alessandra Toncelli,M. Tonelli,O. Torre,E. Tournefier,F. Travasso,G. Vajente,J. F. J. van den Brand,C. Van Den Broeck,S. Van Der Putten,M. Vasúth,M. Vavoulidis,G. Vedovato,D. Verkindt,F. Vetrano,A. Viceré,J. Y. Vinet,S. Vitale,H. Vocca,R. L. Ward,M. Was,M. Yvert,A. K. Zadrożny,J. P. Zendri +182 more
TL;DR: Advanced Virgo is the successor of the initial Virgo gravitational wave detector as discussed by the authors, which uses the infrastructure of its predecessor but aims to be 10 times more sensitive than the original Virgo detector.
Proceedings ArticleDOI
Realization of low-loss mirrors with sub-nanometer flatness for future gravitational wave detectors
C. Michel,N. Morgado,L. Pinard,Benoit Sassolas,Romain Bonnand,Jerome Degallaix,D. Forest,R. Flaminio,G. Billingsley +8 more
TL;DR: In this paper, a planetary motion completed by masking technique has been studied and the two first configurations based on a single rotation motion combined or not with uniformity masks allow to obtain coating thickness uniformity around 0.2 % rms on 160 mm diameter.