Arm Cavity as Squeezing Filter via Entanglement Swapping
|
|
- Daniela Sanders
- 5 years ago
- Views:
Transcription
1 Arm Cavity as Squeezing Filter via Entanglement Swapping Intra-Cavity Squeezing for White-Light Cavities Yanbei Chen on behalf of Yiqiu Ma, Haixing Miao, Jan Harms, Matt Evans, Roman Schnabel 1
2 p Degenerate vs Non-Degenerate OPA p a1,2 c1,2 degenerate OPA a1,2 b1,2 non-degenerate OPA c1,2 d1,2 c 1 = e +r a 1 c 2 = e r a 2 phase-sensitive amplification S c1 c 1 = e +2r, S c2 c 2 = e 2r, S c1 c 2 = 0. c2 c1 c 1 = a 1 cosh r + b 1 sinh r c 2 = a 2 cosh r b 2 sinh r d 1 = b 1 cosh r + a 1 sinh r d 2 = b 2 cosh r a 2 sinh r phaseinsensitive amplification additional noise S c1 c 1 = S c2 c 2 = cosh 2r, S c1,c 2 = 0 S d1 d 1 = S d2 d 2 = cosh 2r, S d1,d 2 = 0 r 1: c 1 d 1, c 2 d 2 2
3 EPR Entanglement! c2 d2 θ c1 θ d1 can predict c θ = c1cosθ - c2sinθ after subtraction: conditionally squeezed! S c c = 1 cosh 2r, S c /2 c /2 = cosh 2r ~3dB less than single squeezer measuring dθ = d1cosθ + d2sinθ Measurement of entangled beam produces conditional squeezing 3
4 Using EPR c2 d2 θ c1 θ d1 sent to dark-port of main IFO sent to filter cavity then detect frequency-dependent measurement of d [rotate by Φ=-θ, and measure 1st quadrature] means frequency dependent squeezing for c 4
5 Generating EPR a1,2 c1,2 a1,2 degenerate c1,2 OPA b1,2 non-degenerate OPA d1,2 Carrier Carrier +Δ Sub-Carrier signal sidebands c1,2 idler sidebands d1,2 ωgreen = 2 correlations between upper/ lower sideband fields ωgreen = 2+Δ correlations between upper/ lower sideband fields 5
6 Fancy Interpretation A B C D +Δ ωgreen = 2+Δ From squeezer: B & C form EPR pair Detection of sub-carrier: Joint measurement of C & D Conditioning : Classical Operation on B D teleported to B, carrier now squeezed. 6
7 Fancy Interpretation A B C D +Δ ωgreen = 2+Δ From squeezer: B & C form EPR pair Detection of sub-carrier: Joint measurement of C & D Conditioning : Classical Operation on B D teleported to B, carrier now squeezed. 7
8 Fancy Interpretation A B C +Δ D ωgreen = 2+Δ From squeezer: B & C form EPR pair Detection of sub-carrier: Joint measurement of C & D Conditioning : Classical Operation on B D teleported to B, carrier now squeezed. 8
9 Arm as filter cavity ETM resonance any microscopic detuning ITM TITM Carrier: resonance detuning phase of Δ LSR/c Green 2+Δ +Δ SRM TSR RSE for carrier at filter cavity for +Δ +Δ OMC 9
10 Example: Advanced LIGO Pc=800 kw TITM=1.4% TSR=35% farm = 370 Hz any microscopic detuning Sh (f) (Hz -1/2 ) Needs filter cavity with ffilter=51.3hz also detuned by 51.3 Hz detuning phase of Δ LSR/c TITM=1.4% φ= nπ TSR=35% filter cavity for +Δ f (Hz) 10 for LSR=15 meter Δ = 891 khz+10 n MHz n=0,1,2,
11 Noise Spectrum db squeezer Sh (f) (Hz -1/2 ) ideal 1%, 5%,10% loss (each detector) f (Hz) 11 Advanced LIGO ideal 7dB suppression (3dB penalty)
12 Improvement Factor 10 db squeezer 15 db squeezer Amplitude Improvemet lossless 1% 5% 10% Amplitude Improvemet lossless 1% 5% 10% f(hz) f (Hz) loss is the same for both photodetectors 12
13 Details Advanced LIGO Green 2+Δ +Δ y = e i (d 1 cos + d 2 sin ) + p 2 n y +Δ OMC Gain z = e 2i (c 2 Kc 1 ) + p 1 n z + e i p 2K h h SQL Ideal: 3dB less than single squeezer Losses: Filter loss much suppressed; other losses remain Only sub-carrier loss low frequencies 13
14 GEO 600: Detuned SR without RadiationPressure z = e i (c 1 cos + c 2 sin ) + h detuned frequency-dependent quadrature rotation +Δ y = e i (d 1 cos d 2 sin ) detuned oppositely opposite frequency-dependent quadrature rotation Direct subtraction achieves desired squeezing!! 14
15 Intra-Cavity Squeezing Optomechancail Filter for White-Light Cavity can also be realized this way anomalous dispersion Green 2+Δ Question: how to deal with optical instabilities? 15
16 Summary ETM Squeezer pumped at an offset frequency produces entangled beams Carrier: ITM Arm cavity can be used as squeezing filter. Examples: - Advanced LIGO - GEO 600 Filter for White-Light Cavity SRM Green 2+Δ +Δ +Δ OMC 16
arxiv: v2 [quant-ph] 21 Aug 2017
Broadband sensitivity enhancement of detuned dual-recycled Michelson interferometers with EPR entanglement Daniel D. Brown, 1, Haixing Miao, 1 Chris Collins, 1 Conor Mow-Lowry, 1 Daniel Töyrä, 1 and Andreas
More informationSub khz Squeezing for Gravitational Wave Detection LIGO-G Z
Sub khz Squeezing for Gravitational Wave Detection LIGO-G040416-00-Z Kirk McKenzie, Nicolai Grosse, Warwick Bowen, Stanley Whitcomb, Malcolm Gray, David McClelland and Ping Koy Lam The Center for Gravitational
More informationExperience with Signal- Recycling in GEO600
Experience with Signal- Recycling in GEO600 Stefan Hild, AEI Hannover for the GEO-team Stefan Hild 1 GWADW, Elba, May 2006 Stefan Hild 2 GWADW, Elba, May 2006 Motivation GEO600 is the 1st large scale GW
More informationStable recycling cavities for Advanced LIGO
Stable recycling cavities for Advanced LIGO Guido Mueller LIGO-G070691-00-D with input/material from Hiro Yamamoto, Bill Kells, David Ottaway, Muzammil Arain, Yi Pan, Peter Fritschel, and many others Stable
More informationThe Florida control scheme. Guido Mueller, Tom Delker, David Reitze, D. B. Tanner
The Florida control scheme Guido Mueller, Tom Delker, David Reitze, D. B. Tanner Department of Physics, University of Florida, Gainesville 32611-8440, Florida, USA The most likely conguration for the second
More informationarxiv: v1 [gr-qc] 10 Sep 2007
LIGO P070067 A Z A novel concept for increasing the peak sensitivity of LIGO by detuning the arm cavities arxiv:0709.1488v1 [gr-qc] 10 Sep 2007 1. Introduction S. Hild 1 and A. Freise 2 1 Max-Planck-Institut
More informationInvestigation of Squeezed Light with an Injection Locked Laser
Investigation of Squeezed Light with an Injection Locked Laser Thomas W. Noel REU program, College of William and Mary July 31, 2008 Abstract Quantum physics implies a certain unavoidable amount of noise
More informationAdvanced LIGO optical configuration investigated in 40meter prototype
Advanced LIGO optical configuration investigated in 4meter prototype LSC meeting at LLO Mar. 22, 25 O. Miyakawa, Caltech and the 4m collaboration LIGO- G5195--R LSC meeting at LLO, March 25 1 Caltech 4
More informationIntroduction to laser interferometric gravitational wave telescope
Introduction to laser interferometric gravitational wave telescope KAGRA summer school 013 July 31, 013 Tokyo Inst of Technology Kentaro Somiya Interferometric GW detector Far Galaxy Supernova explosion,
More informationParametric signal amplification
Parametric signal amplification ET meeting @ Birmingham Mar 27, 2017 K.Somiya Observation of high freq GW sources [Kiuchi, 2010] BNS merger with different models D=100Mpc BNS merger appears above the cavity
More informationOptical generation of frequency stable mm-wave radiation using diode laser pumped Nd:YAG lasers
Optical generation of frequency stable mm-wave radiation using diode laser pumped Nd:YAG lasers T. Day and R. A. Marsland New Focus Inc. 340 Pioneer Way Mountain View CA 94041 (415) 961-2108 R. L. Byer
More information5 Advanced Virgo: interferometer configuration
5 Advanced Virgo: interferometer configuration 5.1 Introduction This section describes the optical parameters and configuration of the AdV interferometer. The optical layout and the main parameters of
More informationThis is a brief report of the measurements I have done in these 2 months.
40m Report Kentaro Somiya This is a brief report of the measurements I have done in these 2 months. Mach-Zehnder MZ noise spectrum is measured in various conditions. HEPA filter enhances the noise level
More information레이저의주파수안정화방법및그응용 박상언 ( 한국표준과학연구원, 길이시간센터 )
레이저의주파수안정화방법및그응용 박상언 ( 한국표준과학연구원, 길이시간센터 ) Contents Frequency references Frequency locking methods Basic principle of loop filter Example of lock box circuits Quantifying frequency stability Applications
More informationFilter Cavity Experiment and Frequency Dependent Squeezing. MIT Tomoki Isogai
Filter Cavity Experiment and Frequency Dependent Squeezing MIT Tomoki Isogai Outline What is squeezing? Squeezing so far Why do we need frequency dependent squeezing? Filter Cavity Experiment at MIT Frequency
More informationSqueezed light at 1550 nm with a quantum noise reduction of 12.3 db
Squeezed light at 1550 nm with a quantum noise reduction of 12.3 db Moritz Mehmet, 1,2, Stefan Ast, 1 Tobias Eberle, 1,2 Sebastian Steinlechner, 1 Henning Vahlbruch, 1 and Roman Schnabel 1 1 Max-Planck-Institut
More informationResidual Phase Noise Measurement Extracts DUT Noise from External Noise Sources By David Brandon and John Cavey
Residual Phase Noise easurement xtracts DUT Noise from xternal Noise Sources By David Brandon [david.brandon@analog.com and John Cavey [john.cavey@analog.com Residual phase noise measurement cancels the
More informationOptical Cavity Designs for Interferometric Gravitational Wave Detectors. Pablo Barriga 17 August 2009
Optical Cavity Designs for Interferoetric Gravitational Wave Detectors Pablo Barriga 7 August 9 Assignents.- Assuing a cavity of 4k with an ITM of 934 radius of curvature and an ETM of 45 radius of curvature.
More informationComparison of tuned and detuned Signal-Recycling. Stefan Hild for the GEO-team
Comparison of tuned and detuned Signal-Recycling Stefan Hild for the GEO-team Stefan Hild 1 ILIAS WG1 meeting, Cascina, November 2006 Stefan Hild 2 ILIAS WG1 meeting, Cascina, November 2006 Signal-Recycling
More informationarxiv: v1 [quant-ph] 17 Oct 2011
Squeezed light at 1550 nm with a quantum noise reduction of 12.3 db arxiv:1110.3737v1 [quant-ph] 17 Oct 2011 Moritz Mehmet 1,2, Stefan Ast 1, Tobias Eberle 1, Sebastian Steinlechner 1, Henning Vahlbruch
More informationToward the Advanced LIGO optical configuration investigated in 40meter prototype
Toward the Advanced LIGO optical configuration investigated in 4meter prototype Aspen winter conference Jan. 19, 25 O. Miyakawa, Caltech and the 4m collaboration LIGO- G547--R Aspen winter conference,
More informationThe AEI 10 m Prototype. June Sina Köhlenbeck for the 10m Prototype Team
The AEI 10 m Prototype June 2014 - Sina Köhlenbeck for the 10m Prototype Team The 10m Prototype Seismic attenuation system Suspension Platform Inteferometer SQL Interferometer Suspensions 2 The AEI 10
More informationSqueezing with long (100 m scale) filter cavities
23-28 May 2016, Isola d Elba Squeezing with long (100 m scale) filter cavities Eleonora Capocasa, Matteo Barsuglia, Raffaele Flaminio APC - Université Paris Diderot Why using long filter cavities in enhanced
More informationPossibility of Upgrading KAGRA
The 3 rd KAGRA International Workshop @ Academia Sinica May 22, 2017 Possibility of Upgrading KAGRA Yuta Michimura Department of Physics, University of Tokyo with much help from Kentaro Komori, Yutaro
More informationPlans for DC Readout Experiment at the 40m Lab
Plans for DC Readout Experiment at the 40m Lab Alan Weinstein for the 40m Lab July 19, 2005 Ben Abbott, Rana Adhikari, Dan Busby, Jay Heefner, Keita Kawabe, Osamu Miyakawa, Virginio Sannibale, Mike Smith,
More informationGravitational Wave Detection and Squeezed Light
Gravitational Wave Detection and Squeezed Light David Sliski November 16, 2009 1 Introduction Among the revolutionary predictions of Einstein s theory of general relativity is the existence of gravitational
More informationElectron Cloud Studies in the Fermilab Main Injector using Microwave Transmission
Electron Cloud Studies in the Fermilab Main Injector using Microwave Transmission J. Charles Thangaraj on behalf of E-cloud team @ Fermilab (B. Zwaska, C. Tan, N. Eddy,..) p ω c ω ω Microwave measurement
More informationControlled dense coding for continuous variables using three-particle entangled states
PHYSICAL REVIEW A 66 032318 2002 Controlled dense coding for continuous variables using three-particle entangled states Jing Zhang Changde Xie and Kunchi Peng* The State Key Laboratory of Quantum Optics
More informationMode mismatch and sideband imbalance in LIGO I PRM
LASER INTERFEROMETER GRAVITATIONAL WAVE OBSERVATORY -LIGO- CALIFORNIA INSTITUTE OF TECHNOLOGY MASSACHUSETTS INSTITUTE OF TECHNOLOGY Technical Note LIGO-T04077-00- E Sep/0/04 Mode mismatch and sideband
More informationQuantum States of Light and Giants
Quantum States of Light and Giants MIT Corbitt, Bodiya, Innerhofer, Ottaway, Smith, Wipf Caltech Bork, Heefner, Sigg, Whitcomb AEI Chen, Ebhardt-Mueller, Rehbein QEM-2, December 2006 Ponderomotive predominance
More informationThe generation and application of squeezed light in gravitational wave detectors and status of the POLIS project
The generation and application of squeezed light in gravitational wave detectors and status of the POLIS project De Laurentis* on behalf of POLIS collaboration *Università degli studi di Napoli 'Federico
More informationAlignment signal extraction of the optically degenerate RSE interferometer using the wave front sensing technique
Alignment signal extraction of the optically degenerate RSE interferometer using the wave front sensing technique Shuichi Sato and Seiji Kawamura TAMA project, National Astronomical Observatory of Japan
More informationInterferometer for LCGT 1st Korea Japan Workshop on Korea University Jan. 13, 2012 Seiji Kawamura (ICRR, Univ. of Tokyo)
Interferometer for LCGT 1st Korea Japan Workshop on LCGT @ Korea University Jan. 13, 2012 Seiji Kawamura (ICRR, Univ. of Tokyo) JGW G1200781 v01 Outline Resonant Sideband Extraction interferometer Length
More informationAdvanced Virgo commissioning challenges. Julia Casanueva on behalf of the Virgo collaboration
Advanced Virgo commissioning challenges Julia Casanueva on behalf of the Virgo collaboration GW detectors network Effect on Earth of the passage of a GW change on the distance between test masses Differential
More informationArm Cavity Finesse for Advanced LIGO
LASER INTERFEROMETER GRAVITATIONAL WAVE OBSERVATORY - LIGO - CALIFORNIA INSTITUTE OF TECHNOLOGY MASSACHUSETTS INSTITUTE OF TECHNOLOGY Technical Note LIGO-T070303-01-D Date: 2007/12/20 Arm Cavity Finesse
More informationThe Core Optics. Input Mirror T ~ 3% T ~ 3% Signal Recycling Photodetector
The Core Optics End Mirror Power Recycling Mirror Input Mirror T ~ 3% T ~ 3% End Mirror T ~ 10 ppm Laser Nd:Yag 6 W 100 W 12 kw 20 m 4000 m Signal Recycling Photodetector Mirror (dark fringe) Fold mirrors
More informationProblems from the 3 rd edition
(2.1-1) Find the energies of the signals: a) sin t, 0 t π b) sin t, 0 t π c) 2 sin t, 0 t π d) sin (t-2π), 2π t 4π Problems from the 3 rd edition Comment on the effect on energy of sign change, time shifting
More informationDevelopment of Optical lever system of the 40 meter interferometer
LASER INTERFEROMETER GRAVITATIONAL WAVE OBSERVATORY -LIGO- CALIFORNIA INSTITUTE OF TECHNOLOGY MASSACHUSETTS INSTITUTE OF TECHNOLOGY Technical Note x/xx/99 LIGO-T99xx- - D Development of Optical lever system
More informationOverview. Tasks: 1.1. Realization of a direct coherent microwave-to-optical link
Overview Optical cavity Microwave cavity Mechanical resonator Tasks: 1.1. Realization of a direct coherent microwave-to-optical link 1.2 Development of large gain-bandwidth product microwave amplifiers
More informationProblem Sheet for Amplitude Modulation
Problem heet for Amplitude Modulation Q1: For the sinusoidaly modulated DB/LC waveform shown in Fig. below. a Find the modulation index. b ketch a line spectrum. c Calculated the ratio of average power
More informationMeasurement of optical response of a detuned resonant sideband extraction gravitational wave detector
PHYSICAL REVIEW D 74, 221 (26) Measurement of optical response of a detuned resonant sideband extraction gravitational wave detector Osamu Miyakawa, Robert Ward, Rana Adhikari, Matthew Evans, Benjamin
More informationModeling of Alignment Sensing and Control for Advanced LIGO
LASER INTERFEROMETER GRAVITATIONAL WAVE OBSERVATORY -LIGO- CALIFORNIA INSTITUTE OF TECHNOLOGY MASSACHUSETTS INSTITUTE OF TECHNOLOGY Technical Note LIGO-T0900511-v4 Modeling of Alignment Sensing and Control
More informationHow to Build a Gravitational Wave Detector. Sean Leavey
How to Build a Gravitational Wave Detector Sean Leavey Supervisors: Dr Stefan Hild and Prof Ken Strain Institute for Gravitational Research, University of Glasgow 6th May 2015 Gravitational Wave Interferometry
More informationExtending the Offset Frequency Range of the D2-135 Offset Phase Lock Servo by Indirect Locking
Extending the Offset Frequency Range of the D2-135 Offset Phase Lock Servo by Indirect Locking Introduction The Vescent Photonics D2-135 Offset Phase Lock Servo is normally used to phase lock a pair of
More informationCavity Field Control - Feedback Performance and Stability Analysis. LLRF Lecture Part3.2 S. Simrock, Z. Geng DESY, Hamburg, Germany
Cavity Field Control - Feedback Performance and Stability Analysis LLRF Lecture Part3.2 S. Simrock, Z. Geng DESY, Hamburg, Germany Motivation Understand how the perturbations and noises influence the feedback
More informationPolarization Sagnac interferometer with a common-path local oscillator for heterodyne detection
1354 J. Opt. Soc. Am. B/Vol. 16, No. 9/September 1999 Beyersdorf et al. Polarization Sagnac interferometer with a common-path local oscillator for heterodyne detection Peter T. Beyersdorf, Martin M. Fejer,
More informationAdvanced Virgo phase cameras
Journal of Physics: Conference Series PAPER OPEN ACCESS Advanced Virgo phase cameras To cite this article: L van der Schaaf et al 2016 J. Phys.: Conf. Ser. 718 072008 View the article online for updates
More informationOur 10m Interferometer Prototype
Our 10m Interferometer Prototype KAGRA f2f, February 14, 2014 Fumiko Kawaoze AEI 10 m Prototype 1 10m Prototype Interferometer Standard Quantum Limit experiment Macroscopic Quantum mechanics Thermal Noise
More informationSupplementary Information:
Supplementary Information: This document contains supplementary text discussing the methods used, figures providing information on the QD sample and level structure (Fig. S), key components of the experimental
More informationLength sensing and control of a Michelson interferometer with power recycling and twin signal recycling cavities
Length sensing and control of a Michelson interferometer with power recycling and twin signal recycling cavities Christian Gräf, André Thüring, Henning Vahlbruch, Karsten Danzmann, and Roman Schnabel Institut
More informationMicroscopic Laser Doppler Vibrometer
Microscopic Laser Doppler Vibrometer System Configuration - 1 PC Controller (APU-Analog processing unit, DPU-Digital processing unit) Optic Head (MEMS Type, XS Type) Function Generator Power Supply Testing
More informationObservation of Three Mode Parametric Interactions in Long Optical Cavities
Observation of Three Mode Parametric Interactions in Long Optical Cavities C. Zhao, L. Ju, Y. Fan, S. Gras. B. J. J. Slagmolen *, H. Miao, P. Barriga D.G. Blair, School of Physics, The University of Western
More informationTesting with Femtosecond Pulses
Testing with Femtosecond Pulses White Paper PN 200-0200-00 Revision 1.3 January 2009 Calmar Laser, Inc www.calmarlaser.com Overview Calmar s femtosecond laser sources are passively mode-locked fiber lasers.
More informationPGx11 series. Transform Limited Broadly Tunable Picosecond OPA APPLICATIONS. Available models
PGx1 PGx3 PGx11 PT2 Transform Limited Broadly Tunable Picosecond OPA optical parametric devices employ advanced design concepts in order to produce broadly tunable picosecond pulses with nearly Fourier-transform
More informationExperimental characterization of frequency-dependent squeezed light
Experimental characterization of frequency-dependent squeezed light Simon Chelkowski, Henning Vahlbruch, Boris Hage, Alexander Franzen, Nico Lastzka, Karsten Danzmann, and Roman Schnabel Institut für Atom-
More informationCharacteristics of absorption and dispersion for rubidium D 2 lines with the modulation transfer spectrum
Characteristics of absorption and dispersion for rubidium D 2 lines with the modulation transfer spectrum Jing Zhang, Dong Wei, Changde Xie, and Kunchi Peng The State Key Laboratory of Quantum Optics and
More informationThe Theta Laser A Low Noise Chirped Pulse Laser. Dimitrios Mandridis
CREOL Affiliates Day 2011 The Theta Laser A Low Noise Chirped Pulse Laser Dimitrios Mandridis dmandrid@creol.ucf.edu April 29, 2011 Objective: Frequency Swept (FM) Mode-locked Laser Develop a frequency
More informationLaboratory Report INFN Milano LASA
Laboratory Report INFN Milano LASA Activities Underway Wire Position Monitor: new generation WPMs mounted on cryomodule and readout connected to control system Piezo Vibration Control: microphonic control
More informationDISPERSION MEASUREMENT FOR ON-CHIP MICRORESONATOR. A Thesis. Submitted to the Faculty. Purdue University. Steven Chen. In Partial Fulfillment of the
i DISPERSION MEASUREMENT FOR ON-CHIP MICRORESONATOR A Thesis Submitted to the Faculty of Purdue University by Steven Chen In Partial Fulfillment of the Requirements for the Degree of Master of Science
More informationi 1 i 2 LOmod 3 RF OUT 4 RF OUT 5 IF 6 IF 7 ENABLE 8 YYWW
Vector Modulator/Mixer Technical Data HPMX-27 Features 5 MHz to 4 GHz Overall Operating Frequency Range 4-4 MHz LOmod range 2.7-5.5 V Operation (3 V, 25 ma) Differential High Impedance i, q Inputs On-Chip
More informationSatellite-based tests of Special and General Relativity
OPTIS Satellite-based tests of Special and General Relativity S. Schiller and the OPTIS Team HYPER Symposium Paris, Nov. 4-6, 2002 The OPTIS team OPTIS Heinrich-Heine- ZARM, Univ. Bremen Universität Düsseldorf
More informationChapter 5 AM Receivers
Chapter 5 AM Receivers Prepared by Prof.V.K.Jain 1 Lecture outcome After studying this lecture, you should be able to: Describe the basic superheterodyne system Choose suitable intermediate frequencies
More informationResults from the Stanford 10 m Sagnac interferometer
INSTITUTE OF PHYSICSPUBLISHING Class. Quantum Grav. 19 (2002) 1585 1589 CLASSICAL ANDQUANTUM GRAVITY PII: S0264-9381(02)30157-6 Results from the Stanford 10 m Sagnac interferometer Peter T Beyersdorf,
More informationStable Recycling Cavities for Advanced LIGO
Stable Recycling Cavities for Advanced LIGO Guido Mueller University of Florida 08/16/2005 Table of Contents Stable vs. unstable recycling cavities Design of stable recycling cavity Design drivers Spot
More informationMethod of Power Recycling in Co-Axial Mach Zender Interferometers for Low Noise Measurements
Method of Power Recycling in Co-Axial Mach Zender Interferometers for Low Noise Measurements arxiv:0904.0288v1 [physics.ins-det] 2 Apr 2009 Abstract We present the first experimental study of a new type
More informationCommissioning of Advanced Virgo
Commissioning of Advanced Virgo VSR1 VSR4 VSR5/6/7? Bas Swinkels, European Gravitational Observatory on behalf of the Virgo Collaboration GWADW Takayama, 26/05/2014 B. Swinkels Adv. Virgo Commissioning
More informationSUPPLEMENTARY INFORMATION DOI: /NPHOTON
Supplementary Methods and Data 1. Apparatus Design The time-of-flight measurement apparatus built in this study is shown in Supplementary Figure 1. An erbium-doped femtosecond fibre oscillator (C-Fiber,
More informationLTP FEE Closed Loop Simulator at ETHZ
LTP FEE Closed Loop Simulator at ETHZ Luigi Ferraioli, Davor Mance, Jan ten Pierick, Jonas Zollinger, Peter Zweifel and Domenico Giardini Departement Erdwissenschaften Institute of Geophysics ETH Zürich
More informationExperimental Test of an Alignment Sensing Scheme for a Gravitational-wave Interferometer
Experimental Test of an Alignment Sensing Scheme for a Gravitational-wave Interferometer Nergis Mavalvala *, Daniel Sigg and David Shoemaker LIGO Project Department of Physics and Center for Space Research,
More informationarxiv:quant-ph/ v1 22 Jul 1999
Continuous Variable Quantum Cryptography T.C.Ralph Department of Physics, Faculty of Science, The Australian National University, ACT 0200 Australia Fax: +61 6 249 0741 Telephone: +61 6 249 4105 E-mail:
More informationHigh-bandwidth squeezed light at 1550 nm from a compact monolithic PPKTP cavity
High-bandwidth squeezed light at 1550 nm from a compact monolithic PPKTP cavity Stefan Ast, 1 Moritz Mehmet, 1,2 and Roman Schnabel 1, 1 Max Planck Institute for Gravitational Physics, Albert Einstein
More informationSingle Conversion LF Upconverter Andy Talbot G4JNT Jan 2009
Single Conversion LF Upconverter Andy Talbot G4JNT Jan 2009 Mark 2 Version Oct 2010, see Appendix, Page 8 This upconverter is designed to directly translate the output from a soundcard from a PC running
More informationsome aspects of Optical Coherence Tomography
some aspects of Optical Coherence Tomography SSOM Lectures, Engelberg 17.3.2009 Ch. Meier 1 / 34 Contents 1. OCT - basic principles (Time Domain Frequency Domain) 2. Performance and limiting factors 3.
More informationKoji Arai / Stan Whitcomb LIGO Laboratory / Caltech. LIGO-G v1
Koji Arai / Stan Whitcomb LIGO Laboratory / Caltech LIGO-G1401144-v1 General Relativity Gravity = Spacetime curvature Gravitational wave = Wave of spacetime curvature Gravitational waves Generated by motion
More informationSqueezed light and radiation pressure effects in suspended interferometers. Thomas Corbitt
Squeezed light and radiation pressure effects in suspended interferometers Thomas Corbitt MIT Sarah Ackley, Tim Bodiya, Keisuke Goda, David Ottaway, Eugeniy Mihkailov, Daniel Sigg, Nicolas, Smith, Chris
More informationSimulations of Advanced LIGO: Comparisons between Twiddle and E2E
LASER INTERFEROMETER GRAVITATIONAL WAVE OBSERVATORY LIGO CALIFORNIA INSTITUTE OF TECHNOLOGY MASSACHUSETTS INSTITUTE OF TECHNOLOGY Document Type LIGO-T010160-00-R 10/15/01 Simulations of Advanced LIGO:
More informationTiming Noise Measurement of High-Repetition-Rate Optical Pulses
564 Timing Noise Measurement of High-Repetition-Rate Optical Pulses Hidemi Tsuchida National Institute of Advanced Industrial Science and Technology 1-1-1 Umezono, Tsukuba, 305-8568 JAPAN Tel: 81-29-861-5342;
More informationAdvanced Virgo Technical Design Report
Advanced Virgo Technical Design Report VIR xxxa 12 Issue 1 The Virgo Collaboration March 21, 2012 Contents 1 ISC 1 1.1 General description of the sub-system........................ 1 1.2 Input from other
More informationSUPPLEMENTARY INFORMATION
Soliton-Similariton Fibre Laser Bulent Oktem 1, Coşkun Ülgüdür 2 and F. Ömer Ilday 2 SUPPLEMENTARY INFORMATION 1 Graduate Program of Materials Science and Nanotechnology, Bilkent University, 06800, Ankara,
More informationHF Receivers, Part 2
HF Receivers, Part 2 Superhet building blocks: AM, SSB/CW, FM receivers Adam Farson VA7OJ View an excellent tutorial on receivers NSARC HF Operators HF Receivers 2 1 The RF Amplifier (Preamp)! Typical
More informationLength Sensing and Control for AdLIGO
LIGO LASER INTERFEROMETER GRAVITATIONAL WAVE OBSERVATORY LIGO Laboratory / LIGO Scientific Collaboration LIGO T060272 00 I ADVANCED LIGO 06/11/19 Length Sensing and Control for AdLIGO Kentaro Somiya, Osamu
More informationUnderstanding Mixers Terms Defined, and Measuring Performance
Understanding Mixers Terms Defined, and Measuring Performance Mixer Terms Defined Statistical Processing Applied to Mixers Today's stringent demands for precise electronic systems place a heavy burden
More informationshould be easy to arrange in the 40m vacuum envelope. Of course, some of the f 1 sidebands will also go out the asymmetric port of the BS. Because f 1
21 RF sidebands, cavity lengths and control scheme. There will be two pairs of phase-modulated sidebands, placed on the main beam just downstream of the PSL, in air, using two fast- and high-powered Pockels
More informationSupplementary Materials for
advances.sciencemag.org/cgi/content/full/2/4/e1501489/dc1 Supplementary Materials for A broadband chip-scale optical frequency synthesizer at 2.7 10 16 relative uncertainty Shu-Wei Huang, Jinghui Yang,
More informationRF System Models and Longitudinal Beam Dynamics
RF System Models and Longitudinal Beam Dynamics T. Mastoridis 1, P. Baudrenghien 1, J. Molendijk 1, C. Rivetta 2, J.D. Fox 2 1 BE-RF Group, CERN 2 AARD-Feedback and Dynamics Group, SLAC T. Mastoridis LLRF
More informationTechniques for the stabilization of the ALPS-II optical cavities
Techniques for the stabilization of the ALPS-II optical cavities Robin Bähre for the ALPS collaboration 9th PATRAS workshop for Axions, WIMPs and WISPs Schloss Waldthausen, Mainz 2013 Jun 26th Outline
More informationE2E s Physics tools. Biplab Bhawal. Optics Electronics Mechanical Mathematical functions Data generation and output. Ligo doc. no.
E2E s Physics tools Ligo doc. no. G020044-00-E Date: Mar 18, 2002 E2E school, LLO Biplab Bhawal LIGO, Caltech Tools: Optics Electronics Mechanical Mathematical functions Data generation and output 1 Optics
More informationCavity Optics for Frequency-Dependent Light Squeezing
Cavity Optics for Frequency-Dependent Light Squeezing Natalie Macdonald St. Johns University (Dated: August 1, 2017) Abstract. In gravitational wave detection, frequency-dependent squeezed light sources
More information200-GHz 8-µs LFM Optical Waveform Generation for High- Resolution Coherent Imaging
Th7 Holman, K.W. 200-GHz 8-µs LFM Optical Waveform Generation for High- Resolution Coherent Imaging Kevin W. Holman MIT Lincoln Laboratory 244 Wood Street, Lexington, MA 02420 USA kholman@ll.mit.edu Abstract:
More informationIntegrated disruptive components for 2µm fibre Lasers ISLA. 2 µm Sub-Picosecond Fiber Lasers
Integrated disruptive components for 2µm fibre Lasers ISLA 2 µm Sub-Picosecond Fiber Lasers Advantages: 2 - microns wavelength offers eye-safety potentially higher pulse energy and average power in single
More informationUsing the Soft Rock 5 as a Microwave IF Spectrum Analyzer
Using the Soft Rock 5 as a IF Spectrum Analyzer By Al Ward W5LUA February 4, 2006 WWW..ORG 1 Soft Rock 5 Designed by Tony Parks KB9YIG 2 Board Approach Top board has the LNAs, Comparators and QSD Bottom
More informationExperimental Demonstration of a Gravitational Wave Detector Configuration Below the Shot Noise Limit
Experimental Demonstration of a Gravitational Wave Detector Configuration Below the Shot Noise Limit Kirk McKenzie 20 June 2002 Supervisors Prof. David McClelland Dr Daniel Shaddock Dr Ping Koy Lam Dr
More informationAlessio Rocchi, INFN Tor Vergata
Topics in Astroparticle and Underground Physics Torino 7-11 September 2015 Alessio Rocchi, INFN Tor Vergata On behalf of the TCS working group AdVirgo optical layout The best optics that current technology
More informationsmall signal linear gain G s is: More realistically, oscillation occurs at frequencies where the G 2 Oscillation frequency is controlled by
VOLTAGE CONTROLLED OSCILLATORS (VCOs) VCOs are RF oscillators whose actual output frequency can be controlled by the voltage present at a control (tuning) port. Barkhausen Criterion: Systems breaks into
More informationReview of 40m upgrade goals ffl The primary goal of the 40 m upgrade is to demonstrate a scheme for using resonant sideband extraction (RSE), in eithe
40m Upgrade Plans ffl Review of 40m upgrade goals ffl 40m infrastructure upgrade ffl RSE configuration - design considerations ffl IFO optical configuration ffl RSE control scheme ffl people, money, schedule
More informationarxiv:quant-ph/ v1 20 Nov 2006
Squeezed light for bandwidth limited atom optics experiments at the Rubidium D1 line arxiv:quant-ph/0611204v1 20 Nov 2006 G. Hétet, O. Glöckl, K. A. Pilypas, C.C. Harb, B.C. Buchler, H.-A. Bachor, P.K.
More informationNarrow- and wideband channels
RADIO SYSTEMS ETIN15 Lecture no: 3 Narrow- and wideband channels Ove Edfors, Department of Electrical and Information technology Ove.Edfors@eit.lth.se 2012-03-19 Ove Edfors - ETIN15 1 Contents Short review
More informationTheoretical Approach. Why do we need ultra short technology?? INTRODUCTION:
Theoretical Approach Why do we need ultra short technology?? INTRODUCTION: Generating ultrashort laser pulses that last a few femtoseconds is a highly active area of research that is finding applications
More informationEXAMINATION FOR THE DEGREE OF B.E. Semester 1 June COMMUNICATIONS IV (ELEC ENG 4035)
EXAMINATION FOR THE DEGREE OF B.E. Semester 1 June 2007 101902 COMMUNICATIONS IV (ELEC ENG 4035) Official Reading Time: Writing Time: Total Duration: 10 mins 120 mins 130 mins Instructions: This is a closed
More informationECEN689: Special Topics in Optical Interconnects Circuits and Systems Spring 2016
ECEN689: Special Topics in Optical Interconnects Circuits and Systems Spring 016 Lecture 7: Transmitter Analysis Sam Palermo Analog & Mixed-Signal Center Texas A&M University Optical Modulation Techniques
More information