T Akutsu 1, S Telada 2, T Uchiyama 1, S Miyoki 1, K Yamamoto 1, M Ohashi 1, K Kuroda 1, N Kanda 3 and CLIO Collaboration. 1 ICRR, Univ. of Tokyo, 2 AIST,

Slides:



Advertisements
Similar presentations
ET-meeting, 22 th Oct N. KIMURA/KEK The Latest Status of the KAGRA Cryogenics N. KIMURA A, D. CHEN B, T. KUME A, S. KOIKE A, Y. SAKAKIBARA B, T.
Advertisements

Laser Interferometer Gravitational-wave Detectors: Advancing toward a Global Network Stan Whitcomb LIGO/Caltech ICGC, Goa, 18 December 2011 LIGO-G v1.
9 th /July/2013 Amaldi 10 C3 15:24~15:42 N.KIMURA/KEK Progress on the Cryogenic System for the Interferometric Cryogenic Gravitational Wave Telescope,
CLIO Current Status of Japanese Detectors Daisuke Tatsumi National Astronomical Observatory of Japan.
Takanori Sekiguchi Italy-Japan Workshop (19 April, 2013) Inverted Pendulum Control for KAGRA Seismic Attenuation System 1 D2, Institute for Cosmic Ray.
April 27th, 2006 Paola Puppo – INFN Roma ILIAS Cryogenic payloads and cooling systems (towards a third generation interferometer) part II: the Vibration.
Australia-Italy Australia 4, October 2005 LCGT project Kazuaki Kuroda LCGT Collaboration.
Design study for 3rd generation interferometers Work Package 1 Site Identification Jo van den Brand
Rahul Kumar1, T. Takayuki1, K. Yamamoto2, H. Tanaka2,T. Miyamoto2, T
Burst noise investigation for cryogenic GW detector Hiroshima U. NAOJ Daisuke TATSUMI 3rd Symposium ‐ New Development in Astrophysics through.
Vibration Isolation R. Takahashi (ICRR), K. Yamamoto (ICRR), T. Uchiyama (ICRR), T. Sekiguchi (ICRR), H. Ishizaki (NAOJ), A. Takamori (ERI), R. DeSalvo.
11 K. Yamamoto, R. Takahashi, T. Sekiguchi, Y. Sakakibara, C. Tokoku, M. Kamiizumi, U. Iwasaki, T. Uchiyama, S. Miyoki, M. Ohashi, T. Akutsu A, H. Ishizaki.
Cryogenics for LCGT Technical Advisory Committee for LCGT ICRR SUZUKI, Toshikazu High Energy Accelerator Research Organization.
Cryo-payload Kazuhiro Yamamoto Institute for Cosmic Ray Research
Status of LCGT and CLIO Masatake Ohashi (ICRR, The University of TOKYO) and LCGT, CLIO collaborators TAUP2007 Sendai, Japan 2007/9/12.
27/Aug./2015 KAGRA f2f meeting N. KIMURA High Energy Accelerator Research Organization, KEK Progress status of Cryogenic System at KAGRA site.
Test mass dynamics with optical springs proposed experiments at Gingin Chunnong Zhao (University of Western Australia) Thanks to ACIGA members Stefan Danilishin.
Commissioning work on the low temperature interferometer 5/17/2010 GWADW at Kyoto Osamu Miyakawa (ICRR, U-Tokyo) and CLIO collaboration 5/17/2010 GWADW.
Australia-Italy Australia 6, October 2005 LCGT project Kazuaki Kuroda LCGT Collaboration Cryogenics for LCGT.
LCGT Cryogenics Status Report KEK T.Suzuki.
LIGO- G D Status of LIGO Stan Whitcomb ACIGA Workshop 21 April 2004.
LIGO- G D The LIGO Instruments Stan Whitcomb NSB Meeting LIGO Livingston Observatory 4 February 2004.
ICRR Seminar 2009/07/24 Cryogenics in CLIO Masatake Ohashi and the LCGT collaboration.
1 Kazuhiro Yamamoto Institute for Cosmic Ray Research (ICRR) the University of Tokyo ELiTES first collaboration meeting Sanjo conference hall, the University.
Astronomical Telescopes and Instrumentation (August 25, 2002, Hawaii USA) Observation run of TAMA GW detector Masaki Ando Department of Science, University.
Commissioning work on the low temperature interferometer 5/17/2010 GWADW at Kyoto Osamu Miyakawa (ICRR, U-Tokyo) and CLIO collaboration 5/17/2010 GWADW.
[A proposal for ILIAS NEXT: Cryogenics versus vibration] [I3-FP7 call] Abstract The reduction of thermal noise in solids is a basic requirement in many.
1 Kazuhiro Yamamoto Institute for Cosmic Ray Research (ICRR) the University of Tokyo KAGRA face to face meeting Institute for Cosmic Ray Research, Kashiwa,
Simulation for KAGRA cryogenic payload: vibration via heat links and thermal noise Univ. Tokyo, D1 Takanori Sekiguchi.
1 K. Yamamoto, R. Takahashi, T. Sekiguchi, T. Uchiyama, H. Ishizaki A, A. Takamori B, R. DeSalvo C, E. Majorana D, LCGT collaboration ICRR, NAO A,ERI B,
LCGT Technical Review Suspension Point Interferometer for Parasitic Noise Reduction and an Additional IFO S.Miyoki (ICRR, Univ. of TOKYO)
External forces from heat links in cryogenic suspensions D1, ICRR, Univ. Tokyo Takanori Sekiguchi GWADW in Hawaii.
Status of the Japanese Projects Kazuaki Kuroda TAMA/CLIO/LCGT Collaboration ICRR, University of Tokyo LSC-Virgo Meeting 26 July, 2007 G R.
11 K. Yamamoto and KAGRA collaboration Institute for Cosmic Ray Research the University of Tokyo Current status of KAGRA Cryogenic 16 May 2012 Gravitational-Wave.
1 Kazuhiro Yamamoto Institute for Cosmic Ray Research The university of Tokyo Report from sub-groups Cryogenic Cryogenic payload 4 August 2011.
ACIGA High Optical Power Test Facility
2009/6/25Amaldi 8 in NewYork City1 Thermal-noise-limited underground interferometer CLIO Kazuhiro Agatsuma and CLIO Collaborators Institute for Cosmic.
LCGT f2f meeting/ICRR, 04/Aug./2011 N. KIMURA Status of the Cryogenics Design N. KIMURA A, S. KOIKE B, T. KUME B, T. OHMORI D, Y. SAITO C, Y. SAKAKIBARA.
External forces from heat links in cryogenic suspensions D1, ICRR, Univ. Tokyo Takanori Sekiguchi.
1 Kazuhiro Yamamoto Institute for Cosmic Ray Research The University of Tokyo KAGRA external review (Cryogenic payload) 18 April 2012.
GWADW2011 Elba/Italy, 23/May/2011 N. KIMURA and Y. SAKAKIBARA Present Design of LCGT Cryogenic Payload - Status of Cryogenic Design - N. KIMURA*, Y. SAKAKIBARA**,
1 Kazuhiro Yamamoto Institute for Cosmic Ray Research The university of Tokyo LCGT internal review (Cryogenic payload) 30 January 2012.
1 Kazuhiro Yamamoto Institute for Cosmic Ray Research The university of Tokyo LCGT internal review (Cryogenic payload) 30 January 2012.
Active Vibration Isolation using a Suspension Point Interferometer Youichi Aso Dept. Physics, University of Tokyo ASPEN Winter Conference on Gravitational.
Lessons from CLIO Masatake Ohashi (ICRR, The University of TOKYO) and CLIO collaborators GWADW2012 Hawaii 2012/5/16.
Status of the cryogenic payload system for baseline KAGRA Rahul Kumar 1, K. Craig 2, K. Yamamoto 2, H. Tanaka 2, T. Miyamoto 2,T. Kajita 2, T. Suzuki 1,
Vibration measurements at KAGRA site
Cryogenic development in KAGRA
Performance test of KAGRA cryostat at site
Overview of the 20K configuration
Kazuhiro Yamamoto on behalf of KAGRA collaboration
Performance test of KAGRA cryostat at site
Yuta Michimura Department of Physics, University of Tokyo
Radiation shield vibration measurement at KAGRA site
Is there a future for LIGO underground?
Kazuaki Kuroda On behalf of LCGT Collaboration
Vibration measurements at KAGRA site
External forces from heat links in cryogenic suspensions
Current Status of TAMA300 Shuichi Sato
Yuta Michimura Department of Physics, University of Tokyo
Status of KAGRA Yuta Michimura on behalf of the KAGRA Collaboration
Status of KAGRA Yuta Michimura on behalf of the KAGRA Collaboration
Development of vibration isolation systems for LCGT VII
KAGRA – 3km Cryogenic Laser Interferometer
Development of vibration isolation systems for LCGT VI
Development of vibration isolation systems for LCGT VI
CLIO underground in mine
Yuta Michimura Department of Physics, University of Tokyo
The ET sensitivity curve with ‘conventional‘ techniques
Collaboration Meeting
Presentation transcript:

T Akutsu 1, S Telada 2, T Uchiyama 1, S Miyoki 1, K Yamamoto 1, M Ohashi 1, K Kuroda 1, N Kanda 3 and CLIO Collaboration. 1 ICRR, Univ. of Tokyo, 2 AIST, 3 OCU and CLIO Collaboration Dec th GWDAW, Potsdam, Germany

Dec GWDAW11 Potsdam Germany Contents I.Cryogenic Laser Interferometer Observatory II.First test run III.Influence of cryocooler IV.Summary

Dec GWDAW11 Potsdam Germany 1. Cryogenic Laser Interferometer Observatory (CLIO) Where is CLIO? Tokyo (NAOJ) Kamioka 220km Construction started from 2003 spring.

Dec GWDAW11 Potsdam Germany 1. Cryogenic Laser Interferometer Observatory (CLIO) 1. Reduction of thermal noise limiting sensitivity is targeted using sapphire mirrors and sapphire suspension fibers. 2. Stable operation is expected owing to the low seismic noise of KAMOIKA mine. - Seismic noise at the Kamioka mine is 1/100 lower than that at a city area. - Cooled sapphire mirrors around 20K CLIO operation using cryogenic mirrors was done Apr.2006 ! CLIO is operated at room temperature for noise hunting. Now Motivation of CLIO : Proto-Type for LCGT

Dec GWDAW11 Potsdam Germany 1. Cryogenic Laser Interferometer Observatory (CLIO) Current best sensitivity Observable range (S/N=10) Dec Operation at room temperature Sensitivity Frequency Observable range Calculation by T.Uchiyama and K.Yamamoto

Dec GWDAW11 Potsdam Germany 1. Cryogenic Laser Interferometer Observatory (CLIO) Apparatus of CLIO Compressors Cryostat tank Graphic by S.Miyoki and revised by T.Akutsu cryocooler Inline Perpendicular

Dec GWDAW11 Potsdam Germany Cryocooler 4K cold head Heat link Radiation shield Optical bench for PD Cryostat tank 2. First test run for Data Taking Cryocoolers Vibrations, Acoustic noise - Stable operation is expected owing to the low seismic noise of KAMOIKA mine. Motivation of CLIO In the future, we would like to evaluate the data both, at 20K and at room temperature.

Dec GWDAW11 Potsdam Germany Cryocooler 4K cold head Heat link Radiation shield Optical bench for PD Cryostat tank 2. First test run for Data Taking Cryocoolers (ultra low vibration type) Vibrations, Acoustic noise Sound level meter in the PD room Cryocooler switch on! How does a cryocooler have influence on the feed back signal ? A PD is near a cryostat tank

Dec GWDAW11 Potsdam Germany 2. First test run for Data Taking Calculation by T.Uchiyama and K.Yamamoto Observable range (S/N=10) Data taken on Nov was used in this work First Data Taking Sensitivity at data taking 49kpc at best sensitivity Nov hours Nov hours  Without alignment control  Consecutive lock BOLFUR suspension wires No heat link Room temperature Configuration at the present

Dec GWDAW11 Potsdam Germany Fluctuation of sensitivity Apparently, it seems that acoustic noise does not influence the data so much. Influence on noise level 3. Contamination of cryocooler Histogram of fluctuation

Dec GWDAW11 Potsdam Germany 3. Contamination of cryocooler In order to search the effect of burst-like noise, we used a slope filter (P.R.D ). Time of analyzed data No remarkable difference between on and off of the refrigerator. Influence on burst-like noise Switch off 39 min. Switch on 15 min. Evaluation of hrss : A&A (2002)

Dec GWDAW11 Potsdam Germany 3. Contamination of cryocooler Nov Observable Range1.4Msol-1.4Msol (S/N=10) Do cryocoolers really have any influences for the data? Cryocooler on car unlock

Dec GWDAW11 Potsdam Germany 3. Contamination of cryocooler Histogram for observable distance PDs and its beam guiding optics will be installed in a vacuum tank in January 2007! Acoustic influence would be much reduced. mean std Switch off 34.22kpc 2.27 Switch on 32.38kpc 2.48 Do cryocooler really have any influence for the data? Cryocoolers have an affect on the data.

Dec GWDAW11 Potsdam Germany Summary  CLIO Demonstration of the cryogenic operation was done Apr Present operation is at room temperature for noise hunting.  Data Taking First test run was implemented on Nov  Contamination of cryocooler - No remarkable influence as for burst noise. - A little influence for floor level by observable range. - More complete countermeasures for acoustic noise will be prepared. Next schedule Next data taking is planned on Jan after some acoustic countermeasures.

Dec GWDAW11 Potsdam Germany Appendix Seismic noise level at Kamioka site and Mitaka site 1/100 -1/1000

Dec GWDAW11 Potsdam Germany Appendix -Difference between the seismic noise on the surface and in the ground of the isolated area is distinguishing above 1 Hz. - Stable operation without alignment control is demonstrated for ?? hours. (Normally, GWDs on the ground without alignment control is impossible.)

Dec GWDAW11 Potsdam Germany 1 st Targeted Displacement Noise Thermal Noises limit the sensitivity around 100Hz, and they will be reduced after cooling. Laser power : 200mW for one arm Mirror Mass : 1.8 kg

Dec GWDAW11 Potsdam Germany Low Vibration Refrigerator - outlook -

Dec GWDAW11 Potsdam Germany Ultra-Low Vibration Refrigerator - vibration reduction performance - Vibration of the 4K vibration reduction stage in time. Vibration on the 300K stage in the Cryostat in the KAMIOKA mine X-axisY-axisZ-axis The values show mainly the operation frequency vibration.

Dec GWDAW11 Potsdam Germany Cryostat - outlook -

Dec GWDAW11 Potsdam Germany Appendix mean std off 2.88e e-20 on 2.93e e off 7.58e e-20 on 8.19e e off 9.92e e-20 on 1.05e e off 1.54e e-20 on 1.53e e-20

Dec GWDAW11 Potsdam Germany 1. Cryogenic Laser Interferometer Observatory (CLIO) The sounds caused by cryocoolers is loud although its system has low vibration. Sound level meter in the PD room Acceleration meter under a cryostat tank Cryocooler switch on! Cryocooler switch on! How does it have influence for the data quality ? average root-mean-square (average root-mean-square )

Dec GWDAW11 Potsdam Germany Appendix Observable range