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We have developed a system for tapered fiber measurements of optomechanical resonators inside a dilution refrigerator, which is compatible with both on- and off-chip devices. Our apparatus features full three-dimensional control of the…

Mesoscale and Nanoscale Physics · Physics 2015-01-19 A. J. R. MacDonald , G. G. Popowich , B. D. Hauer , P. H. Kim , A. Fredrick , X. Rojas , P. Doolin , J. P. Davis

In this paper, we propose a novel non-contact vibration measurement system that is competent in estimating linear and/or rotational motions of machine parts. The technique combines microwave radar, standard camera, and optical strobe to…

Signal Processing · Electrical Eng. & Systems 2020-06-02 Dibyendu Roy , Arijit Sinharay , Brojeshwar Bhowmick , Raj Rakshit , Tapas Chakravarty , Arpan Pal

We measure molecular vibrations with femtometer precision using time-resolved x-ray absorption spectroscopy. For a demonstration, a Raman process excites the A$_{1g}$ mode in gas-phase SF$_6$ molecules with an amplitude of $\approx50$ fm,…

Integrated optics are used to achieve astronomical interferometry inside robust and compact materials, improving the instruments stability and sensitivity. In order to perform differential phase measurements at the H$\alpha$ line (656.3 nm)…

Virgo is a kilometer-length interferometer for gravitational waves detection located near Pisa. Its first science run, VSR1, occured from May to October 2007. The aims of the calibration are to measure the detector sensitivity and to…

General Relativity and Quantum Cosmology · Physics 2014-11-20 The Virgo collaboration , T. Accadia , F. Acernese , F. Antonucci , S. Aoudia , K. G. Arun , P. Astone , G. Ballardin , F. Barone , M. Barsuglia , Th. S. Bauer , M. G. Beker , A. Belletoile , S. Bigotta , S. Birindelli , M. Bitossi , M. A. Bizouard , M. Blom , C. Boccara , F. Bondu , L. Bonelli , R. Bonnand , L. Bosi , S. Braccini , C. Bradaschia , A. Brillet , V. Brisson , R. Budzynski , T. Bulik , H. J. Bulten , D. Buskulic , C. Buy , G. Cagnoli , E. Calloni , E. Campagna , B. Canuel , F. Carbognani , F. Cavalier , R. Cavalieri , G. Cella , E. Cesarini , E. Chassande-Mottin , A. Chincarini , F. Cleva , E. Coccia , C. N. Colacino , J. Colas , A. Colla , M. Colombini , A. Corsi , J. -P. Coulon , E. Cuoco , S. D'Antonio , A. Dari , V. Dattilo , M. Davier , R. Day , R. De Rosa , M. del Prete , L. Di Fiore , A. Di Lieto , M. Di Paolo Emilio , A. Di Virgilio , A. Dietz , M. Drago , V. Fafone , I. Ferrante , F. Fidecaro , I. Fiori , R. Flaminio , J. -D. Fournier , J. Franc , S. Frasca , F. Frasconi , A. Freise , M. Galimberti , L. Gammaitoni , F. Garufi , G. Gemme , E. Genin , A. Gennai , A. Giazotto , R. Gouaty , M. Granata , C. Greverie , G. M. Guidi , H. Heitmann , P. Hello , S. Hild , D. Huet , P. Jaranowski , I. Kowalska , A. Krolak , N. Leroy , N. Letendre , T. G. F. Li , M. Lorenzini , V. Loriette , G. Losurdo , J. M. Mackowski , E. Majorana , I. Maksimovic , N. Man , M. Mantovani , F. Marchesoni , F. Marion , J. Marque , F. Martelli , A. Masserot , C. Michel , L. Milano , Y. Minenkov , M. Mohan , J. Moreau , N. Morgado , A. Morgia , S. Mosca , V. Moscatelli , B. Mours , I. Neri , F. Nocera , G. Pagliaroli , L. Palladino , C. Palomba , F. Paoletti , S. Pardi , M. Parisi , A. Pasqualetti , R. Passaquieti , D. Passuello , G. Persichetti , M. Pichot , F. Piergiovanni , M. Pietka , L. Pinard , R. Poggiani , M. Prato , G. A. Prodi , M. Punturo , P. Puppo , O. Rabaste , D. S. Rabeling , P. Rapagnani , V. Re , T. Regimbau , F. Ricci , F. Robinet , A. Rocchi , L. Rolland , R. Romano , D. Rosinska , P. Ruggi , B. Sassolas , D. Sentenac , R. Sturani , B. Swinkels , A. Toncelli , M. Tonelli , O. Torre , E. Tournefier , F. Travasso , J. Trummer , G. Vajente , J. F. J. van den Brand , S. van der Putten , M. Vavoulidis , G. Vedovato , D. Verkindt , F. Vetrano , A. Vicere , J. -Y. Vinet , H. Vocca , M. Was , M. Yvert

Beginning in Fall 2018, the VERITAS high energy gamma-ray observatory (Amado, AZ) was upgraded to enable Stellar Intensity Interferometry (SII) observations during bright moon conditions. The system potentially allows VERITAS to spatially…

Instrumentation and Methods for Astrophysics · Physics 2019-08-09 Rylee Cardon , Nolan Matthews , A. Udara Abeysekara , David Kieda

A suspension-point interferometer (SPI) is an auxiliary interferometer for active vibration isolation, implemented at the suspension points of the mirrors of an interferometric gravitational wave detector. We constructed a prototype…

General Relativity and Quantum Cosmology · Physics 2009-11-10 Y. Aso , M. Ando , K. Kawabe , S. Otsuka , K. Tsubono

A spherical Fabry-Perot interferometer with adjustable mirror spacing is used to produce interference fringes with frequency separation (c/2L)/N, N=2-15. The conditions for observation of these fringes are derived from the consideration of…

Atomic Physics · Physics 2007-05-23 Katherine Kerner , Simon M. Rochester , Valeriy V. Yashchuk , D. Budker

We report on the measurements of tilt noise performed at the Virgo site with a ring laser gyroscope. The apparatus is a He-Ne laser operating in a square cavity mounted on a vertical plane perpendicular to the north-south arm of the…

Instrumentation and Detectors · Physics 2011-08-17 Jacopo Belfi , Nicolò Beverini , Filippo Bosi , Giorgio Carelli , Angela Di Virgilio , Enrico Maccioni , Fabio Stefani

Resonance modes are intrinsic characteristics of objects when excited at those frequencies. Probing the resonance signatures can reveal useful information about material composition, geometry, presence of defects, and other characteristics…

Applied Physics · Physics 2020-07-02 S. Liao , S. Bakhtiari , T. Elmer , B. Lawrence , E. R. Koehl , N. Gopalsami , A. Raptis

Predictions and measurements of a multimode waveguide interferometer operating in a fibre coupled, ``dual-mode'' regime are reported. With a 1.32 micrometer source, a complete switching cycle of the output beam is produced by a 10.0…

Optics · Physics 2009-11-13 Richard M. Jenkins , Andrew F. Blockley , J. Banerji , Alan R. Davies

We present an absolute distance measurement interferometer based on a two wavelength interferometer and a variable synthetic wavelength technique. The wavelength scanning range was 12 GHz, realized with a phase accuracy of 1.0 m{\lambda} by…

Instrumentation and Detectors · Physics 2014-02-25 Yoshiyuki Kuramoto , Hiroshi Okuda

The possibility of measuring the second order correlation function of the gravitational waves detectors' currents or photonumbers, and the observation of the gravitational signals by using a spectrum analyzer is discussed. The method is…

General Relativity and Quantum Cosmology · Physics 2007-05-23 Y. Ben-Aryeh

We report on the active stabilization of a Michelson interferometer at an arbitrary phase angle with a precision better than one degree at $\lambda = 632.8$ nm, which corresponds to an optical path difference between the two arms of less…

Optics · Physics 2015-06-18 Davide Grassani , Matteo Galli , Daniele Bajoni

In this paper, we report high-precision absolute distance and vibration measurements performed with frequency scanned interferometry. Absolute distance was determined by counting the interference fringes produced while scanning the laser…

Instrumentation and Detectors · Physics 2011-09-13 Hai-Jun Yang , Tianxiang Chen , Keith Riles

A high sensitivity force sensor based on dielectric microspheres in vacuum, optically trapped by a single, upward-propagating laser beam, is described. Off-axis parabolic mirrors are used both to focus the 1064~nm trapping beam and to…

Instrumentation and Detectors · Physics 2020-09-10 Akio Kawasaki , Alexander Fieguth , Nadav Priel , Charles P. Blakemore , Denzal Martin , Giorgio Gratta

Conventional techniques that measure rapid time variations are inefficient or inadequate to discover and observe rapidly pulsating astronomical sources. It is therefore conceivable that there exist some classes of objects pulsating with…

Instrumentation and Methods for Astrophysics · Physics 2015-05-18 Ermanno F Borra

We improve the calculations of the elastic motion induced by the dark matter hits on the surface of the mirror equipped with the interferometer for gravitational waves detection. We focus on the discovery potential of such a dark matter…

High Energy Physics - Phenomenology · Physics 2022-04-20 Chuan-Ren Chen , Chrisna Setyo Nugroho

Gravitational wave detectors such as KAGRA, a 3-km long underground laser interferometer in Japan, require elaborate passive and active seismic isolation of their mirrors. With the aim of detecting passing gravitational waves that create a…

Instrumentation and Detectors · Physics 2025-06-18 Terrence Tsang , Fabián Erasmo Peña Arellano , Takafumi Ushiba , Ryutaro Takahashi , Yoichi Aso , Katherine Dooley

A novel and efficient method for fiber transfer delay measurement is demonstrated. Fiber transfer delay measurement in time domain is converted into the frequency measurement of the modulation signal in frequency domain, accompany with a…

Instrumentation and Detectors · Physics 2016-04-20 J. W. Dong , B. Wang , C. Gao , Y. C. Guo , L. J. Wang
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