LIGO-G020090-00-Z 2) Accomplishment of Japan RSE '98-'01 -- Result of Osamu’s RSE Experiments -- LSC Livingston 2002 Kentaro Somiya University.

Slides:



Advertisements
Similar presentations
Gravitational Wave Astronomy Dr. Giles Hammond Institute for Gravitational Research SUPA, University of Glasgow Universität Jena, August 2010.
Advertisements

Dual Recycling for GEO 600 Andreas Freise, Hartmut Grote Institut für Atom- und Molekülphysik Universität Hannover Max-Planck-Institut für Gravitationsphysik.
Cascina, January 25th, Coupling of the IMC length noise into the recombined ITF output Raffaele Flaminio EGO and CNRS/IN2P3 Summary - Recombined.
Polarization Techniques for Interferometer Control Peter Beyersdorf National Astronomical Observatory of Japan LSC March 2002 Advanced Configurations LIGO-G Z.
Optical simulation – March 04 1 Optical Simulation François BONDU VIRGO Tools Goals Example: tuning of modulation frequency A few questions.
Caltech 40m Current Issues University of Florida Kentaro Somiya.
1 Virgo Commissioning progress and plans ILIAS, Jan 23 rd 2007 Matteo Barsuglia on behalf of the Commissioning Team.
NSF : Nov. 10, LIGO End to End simulation overview  Time domain simulation written in C++  Like MATLAB with Interferometer toolbox  Major physics.
VSR1 summary - post VSR1 Commissioning plans E. Tournefier (LAPP-CNRS) LSC-Virgo meeting Oct 22 nd, 2007.
LIGO-G W Where Did the LSC Signals Come From? Fred Raab 27 June 02.
LIGO- G05XXXX-00-R 40m meeting, May Experimental update from the 40m team 40m TAC meeting May 13, 2005 O. Miyakawa, Caltech and the 40m collaboration.
Koji Arai – LIGO Laboratory / Caltech LIGO-G v1.
Towards dual recycling with the aid of time and frequency domain simulations M. Malec for the GEO 600 team Max-Planck-Institut für Gravitationsphysik Albert-Einstein-Institut.
GWADW 2010 in Kyoto, May 19, Development for Observation and Reduction of Radiation Pressure Noise T. Mori, S. Ballmer, K. Agatsuma, S. Sakata,
RF readout scheme to overcome the SQL Feb. 16 th, 2004 Aspen Meeting Kentaro Somiya LIGO-G Z.
Status of LCGT and CLIO Masatake Ohashi (ICRR, The University of TOKYO) and LCGT, CLIO collaborators TAUP2007 Sendai, Japan 2007/9/12.
Design of Stable Power-Recycling Cavities University of Florida 10/05/2005 Volker Quetschke, Guido Mueller.
The GEO 600 Detector Andreas Freise for the GEO 600 Team Max-Planck-Institute for Gravitational Physics University of Hannover May 20, 2002.
LIGO-G R Aspen Current Status of the 40m Detuned RSE Prototype Seiji Kawamura 2004 Aspen Winter Conference on Gravitational Waves Gravitational.
Stefan Hild October 2007 LSC-Virgo meeting Hannover Interferometers with detuned arm cavaties.
GEO‘s experience with Signal Recycling Harald Lück Perugia,
Amaldi conference, June Lock acquisition scheme for the Advanced LIGO optical configuration Amaldi conference June24, 2005 O. Miyakawa, Caltech.
04. November 2004 A. Freise A. Freise, M. Loupias Collaboration Meeting November 04, 2004 Alignment Status.
GEO600 Detector Status Harald Lück Max-Planck Institut für Gravitationsphysik Institut für Atom- und Molekülphysik, Uni Hannover.
Displacement calibration techniques for the LIGO detectors Evan Goetz (University of Michigan)‏ for the LIGO Scientific Collaboration April 2008 APS meeting.
LIGO- G D The LIGO Instruments Stan Whitcomb NSB Meeting LIGO Livingston Observatory 4 February 2004.
1 Virgo Commissioning progress ILIAS, Nov 13 th 2006 Matteo Barsuglia on behalf of the Commissioning Team.
Advanced Virgo Optical Configuration ILIAS-GW, Tübingen Andreas Freise - Conceptual Design -
LIGO-G Z Guido Mueller University of Florida For the LIGO Scientific Collaboration ESF Exploratory Workshop Perugia, Italy September 21 st –23.
Conversion of the Glasgow 10m Prototype for Detuned Operation Bryan Barr Institute for Gravitational Research University of Glasgow LSC - AIC August 13.
LSC-March  LIGO End to End simulation  Lock acquisition design »How to increase the threshold velocity under realistic condition »Hanford 2k simulation.
RSE Experiment in Japan Feb. 20 th, 2004 Aspen Meeting LIGO-G Z K.Somiya, O.Miyakawa, P.Beyersdorf, and S.Kawamura.
Masaki Ando, Akiteru Takamori, Kimio Tsubono Department of Physics, University of Tokyo Earthquake Research Institute, University of Tokyo 1st International.
Isola d’Elba, Italy 2006GWADW-VESF meeting Diagonalizing sensing matrix of RSE interferometer Shuichi Sato TAMA project National Astronomical Observatory.
Abstract The Hannover Thermal Noise Experiment V. Leonhardt, L. Ribichini, H. Lück and K. Danzmann Max-Planck- Institut für Gravitationsphysik We measure.
AIGO 2K Australia - Italy Workshop th October th October 2005 Pablo Barriga for AIGO group.
Nov 3, 2008 Detection System for AdV 1/8 Detection (DET) Subsystem for AdV  Main tasks and requirements for the subsystem  DC readout  Design for: the.
M. Mantovani, ILIAS Meeting 7 April 2005 Hannover Linear Alignment System for the VIRGO Interferometer M. Mantovani, A. Freise, J. Marque, G. Vajente.
Dual Recycling in GEO 600 H. Grote, A. Freise, M. Malec for the GEO600 team Institut für Atom- und Molekülphysik University of Hannover Max-Planck-Institut.
Institute for Cosmic Ray Research Univ. of Tokyo Development of an RSE Interferometer Using the Third Harmonic Demodulation LIGO-G Z Osamu Miyakawa,
MOTIVATION OF THIS PROJECT Testing the control scheme with a prototype interferometer to demonstrate the control of the tuned RSE for LCGT is necessary.
Concept and Current Status of Japan 4m RSE March Kentaro Somiya LIGO-G Z.
SQL Related Experiments at the ANU Conor Mow-Lowry, G de Vine, K MacKenzie, B Sheard, Dr D Shaddock, Dr B Buchler, Dr M Gray, Dr PK Lam, Prof. David McClelland.
Optical Spring Experiments With The Glasgow 10m Prototype Interferometer Matt Edgar.
LIGO-G Z March 2007, LSC meeting, Osamu Miyakawa 1 Osamu Miyakawa Hiroaki Yamamoto March 21, 2006 LSC meeting Modeling of AdLIGO arm lock acquisition.
1 DC readout for Virgo+? E. Tournefier WG1 meeting, Hannover January 23 rd,2007 DC vs AC readout: technical noises Output mode cleaner for DC readout.
LIGO- G R 40m/AdLIGO, LSC, August Issues in sensing and control of the 40m and Advanced LIGO optical configuration LSC meeting, August.
LIGO-G Z 3) Current Status & Plan for Japan RSE -- Stabilization and Installation of PRC & Detuning -- LSC Livingston 2002 Kentaro Somiya.
ST7 Interferometer LIGO-G Z1 The ST7 Interferometer Andreas Kuhnert Robert Spero Jet Propulsion Laboratory California Institute of Technology.
Active Vibration Isolation using a Suspension Point Interferometer Youichi Aso Dept. Physics, University of Tokyo ASPEN Winter Conference on Gravitational.
ET-ILIAS_GWA joint meeting, Nov Henning Rehbein Detuned signal-recycling interferometer unstableresonance worsesensitivity enhancedsensitivity.
1 Fumiko 2006 Elba Meeting Current status of the 4m RSE.
Yoichi Aso Columbia University, New York, NY, USA University of Tokyo, Tokyo, Japan July 14th th Edoardo Amaldi Conference on Gravitational Waves.
Testing Advanced LIGO length sensing and control scheme at the Caltech 40m interferometer. at the Caltech 40m interferometer. Yoichi Aso*, Rana Adhikari,
Main Interferometer Meeting
Nergis Mavalvala Aspen January 2005
Status report of Polarization RSE
GW related research activities in Hannover UNI/AEI
Design of Stable Power-Recycling Cavities
Heterodyne Readout for Advanced LIGO
Current Status of the 40m Detuned RSE Prototype
Heterodyne Readout for Advanced LIGO
40m Laboratory Upgrade Progress Report
Effect of sideband of sideband on 40m and Advanced LIGO
Advanced LIGO optical configuration investigated in 40meter prototype
A. Heidmann M. Pinard J.-M. Courty P.-F. Cohadon
RF readout scheme to overcome the SQL
Radiation pressure induced dynamics in a suspended Fabry-Perot cavity
Measurement of radiation pressure induced dynamics
Presentation transcript:

LIGO-G Z 2) Accomplishment of Japan RSE '98-'01 -- Result of Osamu’s RSE Experiments -- LSC Livingston 2002 Kentaro Somiya University of Tokyo

Asymmetry ( ~ 3m) 51.75MHz x3 17 . 25MHz Review of Japan RSE rd SB 0 th, 1 st, 2 nd (No 3 rd SB) Suspended by single pendulum. Staying in vacuum chamber. Aligned in parallel (not L). No Power Recycling. No detuning. Only single modulation. Third harmonics demodulation with 60 degree asymmetry. Arm cavity 4m Prototype RSE interferometer RSE cavity 8.75m

Large vacuum chamber Small vacuum chamber 3m Pipe Optical bench Detector bench ←To small chamber FM BS lense FM lense Experimental Setup Compact single pendulum with eddy current damping.

Result : RSE lock! Suspended RSE lock. Typically 10min. lock. Relative TF (Signal Gain) is measured with end mass swept mechanically. Details are written on Osamu's doctor thesis.

Interesting! : SR lock with natural detuning SR is locked on a side robe of error signal (Polarity is changed). Unstable lock produces natural detuning effect. It seems to be averaged for higher frequencies.

Next Step Stabilization Power Recycling Detuning Sweeping?? We built a new RSE experiment in Feb. 2002!!