`Nonclassical' States in Quantum Optics: a `Squeezed' Review of the First 75 Years
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Enhancing the Sensitivity of the LIGO Gravitational Wave Detector by Using Squeezed States of Light
, Enhancing the sensitivity of the LIGO gravitational wave detector by using squeezed states of light J. Aasi1, J. Abadie1, B. P. Abbott1, R. Abbott1, T. D. Abbott9 M. R. Abernathy1, C. Adams3, T. Adams36, P. Addesso55, R. X. Adhikari1, C. Affeldt4;11, O. D. Aguiar75, P. Ajith1, B. Allen4;5;11, E. Amador Ceron5, D. Amariutei8, S. B. Anderson1, W. G. Anderson5, K. Arai1, M. C. Araya1, C. Arceneaux29, S. Ast4;11, S. M. Aston3, D. Atkinson7, P. Aufmuth4;11, C. Aulbert4;11, L. Austin1, B. E. Aylott10, S. Babak12, P. T. Baker13, S. Ballmer25, Y. Bao8, J. C. Barayoga1, D. Barker7, B. Barr2, L. Barsotti15, M. A. Barton7, I. Bartos17, R. Bassiri2;6, J. Batch7, J. Bauchrowitz4;11, B. Behnke12, A. S. Bell2, C. Bell2, G. Bergmann4;11, J. M. Berliner7, A. Bertolini4;11, J. Betzwieser3, N. Beveridge2, P. T. Beyersdorf19, T. Bhadbhade6, I. A. Bilenko20, G. Billingsley1, J. Birch3, S. Biscans15, E. Black1, J. K. Blackburn1, L. Blackburn30, D. Blair16, B. Bland7, O. Bock4;11, T. P. Bodiya15, C. Bogan4;11, C. Bond10, R. Bork1, M. Born4;11, S. Bose22, J. Bowers9, P. R. Brady5, V. B. Braginsky20, J. E. Brau24, J. Breyer4;11, D. O. Bridges3, M. Brinkmann4;11, M. Britzger4;11, A. F. Brooks1, D. A. Brown25, D. D. Brown10, K. Buckland1, F. Br¨uckner10, B. C. Buchler34, A. Buonanno27, J. Burguet-Castell49, R. L. Byer6, L. Cadonati28, J. B. Camp30, P. Campsie2, K. Cannon63, J. Cao31, C. D. Capano27, L. Carbone10, S. Caride32, A. D. Castiglia61, S. Caudill5, M. Cavagli`a29, C. Cepeda1, T. Chalermsongsak1, S. -
Wigner Function for SU(1,1)
Wigner function for SU(1,1) U. Seyfarth1, A. B. Klimov2, H. de Guise3, G. Leuchs1,4, and L. L. Sánchez-Soto1,5 1Max-Planck-Institut für die Physik des Lichts, Staudtstraße 2, 91058 Erlangen, Germany 2Departamento de Física, Universidad de Guadalajara, 44420 Guadalajara, Jalisco, Mexico 3Department of Physics, Lakehead University, Thunder Bay, Ontario P7B 5E1, Canada 4Institute for Applied Physics,Russian Academy of Sciences, 630950 Nizhny Novgorod, Russia 5Departamento de Óptica, Facultad de Física, Universidad Complutense, 28040 Madrid, Spain In spite of their potential usefulness, Wigner functions for systems with SU(1,1) symmetry have not been explored thus far. We address this problem from a physically-motivated perspective, with an eye towards applications in modern metrology. Starting from two independent modes, and after getting rid of the irrelevant degrees of freedom, we derive in a consistent way a Wigner distribution for SU(1,1). This distribution appears as the expectation value of the displaced parity operator, which suggests a direct way to experimentally sample it. We show how this formalism works in some relevant examples. Dedication: While this manuscript was under review, we learnt with great sadness of the untimely passing of our colleague and friend Jonathan Dowling. Through his outstanding scientific work, his kind attitude, and his inimitable humor, he leaves behind a rich legacy for all of us. Our work on SU(1,1) came as a result of long conversations during his frequent visits to Erlangen. We dedicate this paper to his memory. 1 Introduction Phase-space methods represent a self-standing alternative to the conventional Hilbert- space formalism of quantum theory. -
Arxiv:2010.08081V3 [Quant-Ph] 9 May 2021 Dipole fields [4]
Time-dependent quantum harmonic oscillator: a continuous route from adiabatic to sudden changes D. Mart´ınez-Tibaduiza∗ Instituto de F´ısica, Universidade Federal Fluminense, Avenida Litor^anea, 24210-346 Niteroi, RJ, Brazil L. Pires Institut de Science et d'Ing´enierieSupramol´eculaires, CNRS, Universit´ede Strasbourg, UMR 7006, F-67000 Strasbourg, France C. Farina Instituto de F´ısica, Universidade Federal do Rio de Janeiro, 21941-972 Rio de Janeiro, RJ, Brazil In this work, we provide an answer to the question: how sudden or adiabatic is a change in the frequency of a quantum harmonic oscillator (HO)? To do this, we investigate the behavior of a HO, initially in its fundamental state, by making a frequency transition that we can control how fast it occurs. The resulting state of the system is shown to be a vacuum squeezed state in two bases related by Bogoliubov transformations. We characterize the time evolution of the squeezing parameter in both bases and discuss its relation with adiabaticity by changing the transition rate from sudden to adiabatic. Finally, we obtain an analytical approximate expression that relates squeezing to the transition rate as well as the initial and final frequencies. Our results shed some light on subtleties and common inaccuracies in the literature related to the interpretation of the adiabatic theorem for this system. I. INTRODUCTION models to the dynamical Casimir effect [32{39] and spin states [40{42], relevant in optical clocks [43]. The main The harmonic oscillator (HO) is undoubtedly one of property of these states is to reduce the value of one of the most important systems in physics since it can be the quadrature variances (the variance of the orthogonal used to model a great variety of physical situations both quadrature is increased accordingly) in relation to coher- in classical and quantum contexts. -
Arxiv:2003.13443V1 [Astro-Ph.IM] 26 Mar 2020 Minimum in the Phase Quadrature, Thus Reducing Shot Broadband Improvement in Sensitivity
Frequency-Dependent Squeezing for Advanced LIGO L. McCuller,1, ∗ C. Whittle,1, y D. Ganapathy,1 K. Komori,1 M. Tse,1 A. Fernandez-Galiana,1 L. Barsotti,1 P. Fritschel,1 M. MacInnis,1 F. Matichard,1 K. Mason,1 N. Mavalvala,1 R. Mittleman,1 Haocun Yu,1 M. E. Zucker,1, 2 and M. Evans1 1LIGO, Massachusetts Institute of Technology, Cambridge, MA 02139, USA 2LIGO, California Institute of Technology, Pasadena, CA 91125, USA (Dated: March 31, 2020) The first detection of gravitational waves by the Laser Interferometer Gravitational-wave Observatory (LIGO) in 2015 launched the era of gravitational wave astronomy. The quest for gravitational wave signals from objects that are fainter or farther away impels technological advances to realize ever more sensitive detectors. Since 2019, one advanced technique, the injection of squeezed states of light is being used to improve the shot noise limit to the sensitivity of the Advanced LIGO detectors, at frequencies above 50 Hz. Below this frequency, quantum back action, in the form of radiation pressure induced motion∼ of the mirrors, degrades the sensitivity. To simultaneously reduce shot noise at high frequencies and quantum radiation pressure noise at low frequencies requires a quantum noise filter cavity with low optical losses to rotate the squeezed quadrature as a function of frequency. We report on the observation of frequency-dependent squeezed quadrature rotation with rotation frequency of 30 Hz, using a 16 m long filter cavity. A novel control scheme is developed for this frequency-dependent squeezed vacuum source, and the results presented here demonstrate that a low-loss filter cavity can achieve the squeezed quadrature rotation necessary for the next planned upgrade to Advanced LIGO, known as \A+." I. -
Classical Models for Quantum Light
Classical Models for Quantum Light Arnold Neumaier Fakult¨atf¨urMathematik Universit¨atWien, Osterreich¨ Lecture given on April 7, 2016 at the Zentrum f¨urOberfl¨achen- und Nanoanalytik Johannes Kepler Universit¨atLinz, Osterreich¨ http://www.mat.univie.ac.at/~neum/papers/physpapers.html#CQlight 1 Abstract In this lecture, a timeline is traced from Huygens' wave optics to the modern concept of light according to quantum electrodynamics. The lecture highlights the closeness of classical concepts and quantum concepts to a surprising extent. For example, it is shown that the modern quantum concept of a qubit was already known in 1852 in fully classical terms. 2 A timeline of light 0: Prehistory I: Waves or particles? (1679{1801) II: Polarization (1809{1852) III: The electromagnetic field (1862{1887) IV: Shadows of new times coming (1887{1892) V: Energies are sometimes quantized (1900{1914) VI: The photon as unitary representation (1926{1946) VII: Quantum electrodynamics (1948{1949) VIII: Coherence and photodetection (1955{1964) IX: Stochastic and nonclassical light (1964-2004) I picked for each period only one particular theme. 3 A timeline of light 0: Prehistory In the beginning God created the heavens and the earth. And God said, "Let there be light", and there was light. (Genesis 1:1.3) It took him only 10 seconds... 10s after the Big Bang: photon epoch begins 2134 BC: oldest solar eclipse recorded in human history (2 Chinese astronomers lost their head for failing to predict it) ca. 1000 BC: It is the glory of God to conceal things, but the kings' pride is to research them. -
Arxiv:2002.04674V1 [Physics.Optics] 11 Feb 2020 in SRS, the Sensitivity and the Imaging Speed Are Fun- Be Reduced by Using a Laser Beam in a Squeezed State
Quantum-Enhanced continuous-wave stimulated Raman spectroscopy R. B. Andrade,1 H. Kerdoncuff,2 K. Berg-Srensen,1 T. Gehring,1 M. Lassen,2 and U. L. Andersen1 1Center for Macroscopic Quantum States bigQ, Department of Physics, Technical University of Denmark, Fysikvej 307, DK-2800 Kgs. Lyngby. 2Danish Fundamental Metrology, Kogle Alle 5, DK-2970, Denmark. Stimulated Raman spectroscopy has become a powerful tool to study the spatiodynamics of molecular bonds with high sensitivity, resolution and speed. However, sensitivity and speed of state- of-the-art stimulated Raman spectroscopy are currently limited by the shot-noise of the light beam probing the Raman process. Here, we demonstrate an enhancement of the sensitivity of continuous- wave stimulated Raman spectroscopy by reducing the quantum noise of the probing light below the shot-noise limit by means of amplitude squeezed states of light. Probing polymer samples with Raman shifts around 2950 cm−1 with squeezed states, we demonstrate a quantum-enhancement of the stimulated Raman signal-to-noise ratio (SNR) of 3:60 dB relative to the shot-noise limited SNR. Our proof-of-concept demonstration of quantum-enhanced Raman spectroscopy paves the way for a new generation of Raman microscopes, where weak Raman transitions can be imaged without the use of markers or an increase in the total optical power. I. INTRODUCTION In this article, we demonstrate the quantum enhance- ment of continuous-wave (cw) SRS using amplitude Optical quantum sensing exploits the unique quantum squeezed light. We demonstrate its functionality and correlations of non-classical light to enhance the detec- superiority by spectroscopically measuring the carbon- tion of physical parameters beyond classical means [1{ hydrogen (C-H) vibrations of polymethylmethacrylate 5]. -
Squeezed Light for Gravitational Wave Astronomy
Squeezed Light for Gravitational Wave Astronomy Von der Fakultät für Mathematik und Physik der Gottfried Wilhelm Leibniz Universität Hannover zur Erlangung des Grades Doktor der Naturwissenschaften – Dr. rer. nat. – genehmigte Dissertation von Dipl.-Phys. Henning Vahlbruch geboren am 29. Juli 1976 in Frankfurt am Main 2008 Referent: Prof. Dr. Roman Schnabel Korreferent: Prof. Dr. Karsten Danzmann Tag der Promotion: 28.11.2008 Abstract During the recent years an international network of interferometric gravitational wave (GW) detectors has been commissioned and searches for various classes of GW- signals are ongoing. Although the observatories are beginning to reach astrophysically interesting sensitivity levels, extensive upgrades are aimed for the next decade bringing us into the era of gravitational wave astronomy. One approach to enhance the detector sensitivity is the injection of squeezed vacuum states of light replacing the vacuum fluctuations entering the detector through its antisymmetric port. In this thesis the unprecedented generation of squeezed vacuum states with a noise power 6.5 dB below vacuum noise within the entire detection bandwidth of ground-based GW-detectors (10 Hz - 10 kHz) was experimentally demonstrated at a wavelength of 1064 nm. For the first time a coherent control scheme was employed for comprehensive phase control of the experimental setup. This scheme is directly applicable to future GW-detector topologies. In addition, parasitic interference in- duced by scattered light was found to be a dominant noise source degrading squeezed states in the audio band. The compatibility of squeezed field injection into a detuned operated dual-recycled Michelson interferometer was demonstrated in a table top experiment. -
Redalyc.Harmonic Oscillator Position Eigenstates Via Application of An
Revista Mexicana de Física ISSN: 0035-001X [email protected] Sociedad Mexicana de Física A.C. México Soto-Eguibar, Francisco; Moya-Cessa, Héctor Manuel Harmonic oscillator position eigenstates via application of an operator on the vacuum Revista Mexicana de Física, vol. 59, núm. 2, julio-diciembre, 2013, pp. 122-127 Sociedad Mexicana de Física A.C. Distrito Federal, México Available in: http://www.redalyc.org/articulo.oa?id=57048159005 How to cite Complete issue Scientific Information System More information about this article Network of Scientific Journals from Latin America, the Caribbean, Spain and Portugal Journal's homepage in redalyc.org Non-profit academic project, developed under the open access initiative EDUCATION Revista Mexicana de F´ısica E 59 (2013) 122–127 JULY–DECEMBER 2013 Harmonic oscillator position eigenstates via application of an operator on the vacuum Francisco Soto-Eguibar and Hector´ Manuel Moya-Cessa Instituto Nacional de Astrof´ısica, Optica´ y Electronica,´ Luis Enrique Erro 1, Santa Mar´ıa Tonantzintla, San Andres´ Cholula, Puebla, 72840 Mexico.´ Received 21 August 2013; accepted 17 October 2013 Harmonic oscillator squeezed states are states of minimum uncertainty, but unlike coherent states, in which the uncertainty in position and momentum are equal, squeezed states have the uncertainty reduced, either in position or in momentum, while still minimizing the uncertainty principle. It seems that this property of squeezed states would allow to obtain the position eigenstates as a limiting case, by doing null the uncertainty in position and infinite in momentum. However, there are two equivalent ways to define squeezed states, that lead to different expressions for the limiting states. -
Fp3 - 4:30 Quantum Mechanical System Symmetry*
Proceedings of 23rd Conference on Decision and Control Las Vegas, NV, December 1984 FP3 - 4:30 QUANTUM MECHANICAL SYSTEM SYMMETRY* + . ++ +++ T. J. Tarn, M. Razewinkel and C. K. Ong + Department of Systems Science and Mathematics, Box 1040, Washington University, St. Louis, Missouri 63130, USA. ++ Stichting Mathematisch Centrum, Kruislaan 413, 1098 S J Amsterdam, The Netherlands. +++M/A-COM Development Corporation, M/A-COM Research Center, 1350 Piccard Drive, Suite 310, Rockville. Maryland 20850, USA. Abstract Cll/i(X, t) ifi at :: H(x,t) , ( 1) The connection of quantum nondemolition observables with the symmetry operators of the Schrodinger where t/J is the wave function of the system and x an equation, is shown. The connection facilitates the appropriate set of dynamical coordinates. construction of quantum nondemolition observables and thus of quantum nondemolition filters for a given Definition 1. The symmetry algebra of the Hamiltonian system. An interpretation of this connection is H of a quantum system is generated by those operators given, and it has been found that the Hamiltonian that commute with H and possess together with H a description under which minimal wave pockets remain common dense invariant domain V. minimal is a special case of our investigation. With the above definition, if [H,X1J:: 0 and [H,X2J = 1. Introduction O, then [H,[X1 ,x 2 JJ:: 0 also on D. Clearly all constants of the motion belong to the symmetry algebra In developing the theory of quantum nondemolition of the Hamiltonian. observables, it has been assumed that the output observable is given. The question of whether or not the given output observable is a quantum nondemolition Denote the Schrodinger operator by filter has been answered in [1,2]. -
Magnon-Squeezing As a Niche of Quantum Magnonics
Magnon-squeezing as a niche of quantum magnonics Akashdeep Kamra,1, 2, a) Wolfgang Belzig,3 and Arne Brataas1 1)Center for Quantum Spintronics, Department of Physics, Norwegian University of Science and Technology, NO-7491 Trondheim, Norway 2)Kavli Institute for Theoretical Physics, University of California Santa Barbara, Santa Barbara, USA 3)Department of Physics, University of Konstanz, D-78457 Konstanz, Germany The spin excitations of ordered magnets - magnons - mediate transport in magnetic insulators. Their bosonic nature makes them qualitatively distinct from electrons. These features include quantum properties tradition- ally realized with photons. In this perspective, we present an intuitive discussion of one such phenomenon. Equilibrium magnon-squeezing manifests unique advantageous with magnons as compared to photons, in- cluding properties such as entanglement. Building upon the recent progress in the fields of spintronics and quantum optics, we outline challenges and opportunities in this emerging field of quantum magnonics. The spin excitations of ordered magnets, broadly called We find it convenient to introduce the equilibrium \magnons", carry spin information1{8 and offer a viable magnon-squeezing physics first and later place it in the path towards low-dissipation, unconventional comput- context of the more mature and widely known nonequi- ing paradigms. Their bosonic nature enables realizing librium squeezing phenomenon28,29,31,32. Magnons in a and exploiting phenomena not admitted by electrons9{15. ferromagnet admit single-mode squeezing mediated by The field of \magnonics" has made rapid progress to- the relatively weak spin-nonconserving interactions16,17, wards fundamental physics as well as potential applica- thereby providing an apt start of the discussion. -
Squeeze Operators in Classical Scenarios
Squeeze operators in classical scenarios Jorge A. Anaya-Contreras1, Arturo Z´u˜niga-Segundo1, Francisco Soto-Eguibar2, V´ıctor Arriz´on2, H´ector M. Moya-Cessa2 1Departamento de F´ısica, Escuela Superior de F´ısica y Matem´aticas, IPN Edificio 9 Unidad Profesional ‘Adolfo L´opez Mateos’, 07738 M´exico D.F., Mexico 2Instituto Nacional de Astrof´ısica Optica´ y Electr´onica Calle Luis Enrique Erro No. 1, Sta. Ma. Tonantzintla, Pue. CP 72840, Mexico Abstract We analyse the paraxial field propagation in the realm of classical optics, showing that it can be written as the action of the fractional Fourier transform, followed by the squeeze operator applied to the initial field. Secondly, we show that a wavelet transform may be viewed as the application of a displacement and squeeze operator onto the mother wavelet function. PACS numbers: arXiv:1901.05491v1 [physics.optics] 16 Jan 2019 1 I. INTRODUCTION In the late seventies, squeezed states were introduced [1, 2]. On the one hand, Yuen [3] defined them squeezing the vacuum and then displacing the resulting state. On the other hand, Caves [4] defined them by displacing the vacuum and then squeezing the produced coherent state. Squeezed states have been shown to produce ringing revivals (a fingerprint that a squeezed state is used) in the interaction between light and matter [5]. Applications of quantum techniques in classical optics have been the subject of many studies during the last years [6, 7]. Along the same line, one of the goals of this article is to show, that in a mathematical sense, the squeeze operator could have been introduced in the description of free light propagation, i.e. -
An Atomic Source of Quantum Light
University of Calgary PRISM: University of Calgary's Digital Repository Graduate Studies The Vault: Electronic Theses and Dissertations 2012-10-25 An Atomic Source of Quantum Light MacRae, Andrew MacRae, A. (2012). An Atomic Source of Quantum Light (Unpublished doctoral thesis). University of Calgary, Calgary, AB. doi:10.11575/PRISM/24840 http://hdl.handle.net/11023/310 doctoral thesis University of Calgary graduate students retain copyright ownership and moral rights for their thesis. You may use this material in any way that is permitted by the Copyright Act or through licensing that has been assigned to the document. For uses that are not allowable under copyright legislation or licensing, you are required to seek permission. Downloaded from PRISM: https://prism.ucalgary.ca UNIVERSITY OF CALGARY An Atomic Source of Quantum Light by Andrew John MacRae A THESIS SUBMITTED TO THE FACULTY OF GRADUATE STUDIES IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY DEPARTMENT OF PHYSICS AND ASTRONOMY INSTITUTE FOR QUANTUM INFORMATION SCIENCE CALGARY, ALBERTA October, 2012 �c Andrew John MacRae 2012 Abstract This thesis presents the experimental demonstration of an atomic source of narrowband nonclassical states of light. Employing four-wave mixing in hot atomic Rubidium vapour, the optical states produced are naturally compatible with atomic transitions and may be thus employed in atom-based quantum communication protocols. We first demonstrate the production of two-mode intensity-squeezed light and ana lyze the correlations between the two produced modes. Using homodyne detection in each mode, we verify the production of two-mode quadrature-squeezed light, achieving a reduction in quadrature variance of 3 dB below the standard quantum limit.