New in-air seismic attenuation system for the next generation gravitational wave detector M.R. Blom, A. Bertolini, E. Hennes, A. Schimmel, H.J. Bulten,

Slides:



Advertisements
Similar presentations
Laser Interferometer Gravitational-wave Detectors: Advancing toward a Global Network Stan Whitcomb LIGO/Caltech ICGC, Goa, 18 December 2011 LIGO-G v1.
Advertisements

Cascina, January 25th, Coupling of the IMC length noise into the recombined ITF output Raffaele Flaminio EGO and CNRS/IN2P3 Summary - Recombined.
LIGO - G R 1 HAM SAS Test Plan at LASTI David Ottaway November 2005 LIGO-G Z.
Andrea Paoli AdV 1 st Project Review Cascina, November 3 rd, 2008 IME – infrastructure modifications for environmental noise reduction.
Takanori Sekiguchi Italy-Japan Workshop (19 April, 2013) Inverted Pendulum Control for KAGRA Seismic Attenuation System 1 D2, Institute for Cosmic Ray.
Seismic attenuation chains concept, design and advancement status Riccardo DeSalvo for the KAGRA Seismic group JGW-G September 10, 20121JGW-G
1 Virgo commissioning status M.Barsuglia LAL Orsay.
LIGO-G W Status of LIGO Installation and Commissioning Frederick J. Raab, LIGO Hanford Observatory.
G M Advanced R&D1 Seismic Isolation Retrofit Plan for the LIGO Livingston Observatory Dennis Coyne 29 Nov 2001.
F. Frasconi I.N.F.N. Pisa for the Virgo Collaboration TAUP2007 Sendai, September 11-15, 2007 VIRGO EXPERIMENT VIRGO: a large interferometer for Gravitational.
VSR1 summary - post VSR1 Commissioning plans E. Tournefier (LAPP-CNRS) LSC-Virgo meeting Oct 22 nd, 2007.
LIGO-G W Commissioning Data on Vibration Isolation & Suspensions Fred Raab 24 October 02.
Overview Ground-based Interferometers Barry Barish Caltech Amaldi-6 20-June-05.
ICRR M2 Takanori Sekiguchi ICRR, NAOJ A, ERI B, Sannio Univ. C, INFN Roma D, NIKHEF E, AEI F Ryutaro Takahashi, Kazuhiro Yamamoto, Takashi Uchiyama, Hideharu.
COMMISSIONING PROGRESS G.LOSURDO – INFN Firenze for the Virgo Collaboration.
Active Seismic Isolation Systems for Enhanced and Advanced LIGO Jeffrey S. Kissel 1 for the LSC 1 Louisiana State University The mechanical system for.
Present Superatttenuator performance vs. AdV & ET Requirements S.Braccini for Virgo Suspension group.
Concepts for Combining Different Sensors for CLIC Final Focus Stabilisation David Urner Armin Reichold.
1 Virgo commissioning since the end of VSR1 E. Tournefier for the commissioning team ILIAS WG1, Cascina March 5 th,2008.
Current Progress of Development of Laser Interferometry for LISA-type Mission in China Hsien-Chi Yeh School of Physics Huazhong University of Science &
LIGO-G W Status of LIGO Installation and Commissioning Frederick J. Raab, LIGO Hanford Observatory.
Some Advanced Virgo Developments Laser Benches suspensions DAQ/Controls B. Mours (with slides from Alain Brillet & Jo Van de Brand) LCGT-Virgo meeting.
22nd March 2005 LIGO-G R Passive attenuation for the LIGO Output mode cleaner; HAM SAS R. DeSalvo, S. Marka, V. Sannibale, A. Takamori, C. Torrie,
Thoughts on short term improvements for Mirror Suspension Control G.Losurdo - P.Ruggi.
Prototype Test of Vibration Isolation System Current Status & Schedule
Takanori Sekiguchi Anual Meeting of Physics Society of Japan Sep. 22nd, 2013) Prototype Test of Vibration Isolation System Current Status & Schedule 1.
Interferometer Control Matt Evans …talk mostly taken from…
ILIAS – WG1 Hierarchical suspension control G.Losurdo INFN Firenze.
Gabriele Vajente ILIAS WG1 meeting - Perugia Couplings of angular noises into dark fringe Diffused light studies.
LIGO- G D Status of LIGO Stan Whitcomb ACIGA Workshop 21 April 2004.
Environmental noise studies at VIRGO Environmental contributions to Virgo readout noise (C-runs) many sources identified through coherency analyses with.
Seismic Attenuation System (SAS) for LCGT Inverted pendulum: 30mHz 3 cascaded GAS filter: 500mHz Test mass suspension: triple pendulum Transfer functions.
Takanori Sekiguchi External Review Control and tuning of suspension 1 T. Sekiguchi KAGRA 4th External Review.
1 EIB seismic noise and mitigation I.Fiori, Internal Meeting, 26 August 2009, EGO with E.Genin, F.Frasconi, R.Day, B.Canuel.
LIGO-G D The LIGO-I Gravitational-wave Detectors Stan Whitcomb CaJAGWR Seminar February 16, 2001.
LIGO- G D The LIGO Instruments Stan Whitcomb NSB Meeting LIGO Livingston Observatory 4 February 2004.
SUSPENSIONS Pisa S.Braccini C.Bradaschia R.Cavalieri G.Cella V.Dattilo A.Di Virgilio F.Fidecaro F.Frasconi A.Gennai G.Gennaro A.Giazotto L.Holloway F.Paoletti.
1 Virgo Commissioning progress ILIAS, Nov 13 th 2006 Matteo Barsuglia on behalf of the Commissioning Team.
Minimizing the Resonant Frequency of MGAS Springs for Seismic Attenuation System in Low Frequency Gravitational Waves Interferometers Maddalena Mantovani,
Behavior of an inverted pendulum in the Kamioka mine R. Takahashi (NAOJ), A. Takamori (ERI), E. Majorana (INFN) GWADW 2010 We are investigating behavior.
External forces from heat links in cryogenic suspensions D1, ICRR, Univ. Tokyo Takanori Sekiguchi GWADW in Hawaii.
Abstract The Hannover Thermal Noise Experiment V. Leonhardt, L. Ribichini, H. Lück and K. Danzmann Max-Planck- Institut für Gravitationsphysik We measure.
Noise issues in vibration sensing and isolation for Advanced Virgo Eric Hennes Nikhef.nl GWADW, Hawaii 2012, May 15 Advanced Virgo.
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.
LIGO-G Z The Status of VIRGO E. Tournefier for the Virgo Collaboration GWADW 2004, Aspen From the CITF to VIRGO Commissioning of the Fabry-Perot.
The status of VIRGO Edwige Tournefier (LAPP-Annecy ) for the VIRGO Collaboration HEP2005, 21st- 27th July 2005 The VIRGO experiment and detection of.
The VIRGO Suspensions Control System Alberto Gennai The VIRGO Collaboration.
The control of the Virgo Superattenuator: present and future Giovanni Losurdo - INFN Firenze/Urbino on behalf of the Virgo Collaboration.
Paolo La Penna ILIAS N5-WP1 meeting Commissioning Progress Hannover, July 2004 VIRGO commissioning progress report.
Low frequency anti-vibration system of LCGT Vibration Isolation Group R. Takahashi (ICRR), K. Yamamoto (ICRR), T. Uchiyama (ICRR), T. Sekiguchi (ICRR),
LIGO-G R LIGO R&D1 Improvement of the MGAS Filter Damping Performance Alberto Stochino University of Pisa, Italy SURF Student Mentor: Dr. Riccardo.
The Status of Advanced LIGO: Light at the end of the Tunnels Jeffrey S. Kissel, for the LIGO Scientific Collaboration April APS Meeting, Savannah, GA April.
Caltech, February 12th1 Virgo central interferometer: commissioning and engineering runs Matteo Barsuglia Laboratoire de l’Accelerateur Lineaire, Orsay.
LIGO-G R 1 HAM Passive Seismic Attenuation System (SAS) System Performance, Fabrication, Assembly, Installation Riccardo DeSalvo, Valerio Boschi,
SAT Plans for System R&D Signal Recycling Construction and A&I Short Suspension Upgrade Roberto Passaquieti Università di Pisa and INFN-Pisa AdV Review.
LSC Meeting Baton Rouge, LA, V.Boschi for the HAM-SAS team Ben Abbott, Valerio Boschi, Dennis Coyne, Michael Forte, Jay Heefner, Yu-mei Huang,
Active Vibration Isolation using a Suspension Point Interferometer Youichi Aso Dept. Physics, University of Tokyo ASPEN Winter Conference on Gravitational.
MG 11 - Berlin Virgo status Marie-Anne Bizouard (LAL-Orsay) on behalf of the Virgo Collaboration.
Yoichi Aso Columbia University, New York, NY, USA University of Tokyo, Tokyo, Japan July 14th th Edoardo Amaldi Conference on Gravitational Waves.
Interferometric local sensing for 3G detectors
Type-A SAS Local Control Simulation (Current Status)
Nergis Mavalvala MIT IAU214, August 2002
Control of the KAGRA Cryogenic Vibration Isolation System
Superattenuator for LF and HF interferometers
Commissioning the LIGO detectors
LIGO Detector Commissioning
Status of LIGO Installation and Commissioning
LIGO Detector Commissioning
Improving LIGO’s stability and sensitivity: commissioning examples
HAM SAS Test Plan at LASTI
Presentation transcript:

New in-air seismic attenuation system for the next generation gravitational wave detector M.R. Blom, A. Bertolini, E. Hennes, A. Schimmel, H.J. Bulten, M.G. Beker, F. Mul, M. Doets, J.F.J. van den Brand 13 th TAUP Conference, Asilomar Conference Grounds, Pacific Grove, California, Sep. 2013

Indirect evidence for gravitational waves : Hulse & Taylor’s discovery of first binary pulsar Nobel prize 1993

3 3 kms (1.9 m) gravitational wave detector

4 Virgo, Cascina, Italy GEO600, Hannover, Germany LIGO, Hanford, WA KAGRA, Hida, Japan LIGO, Livingston, LA

5 Direct observation with Michelson interferometers Need to measure length changes of ΔL/L of

6 Direct observation with Michelson interferometers Need to measure length changes of ΔL/L of

Length changes due to gravitational waves - sensitivity 7 Strain = ΔL/L [1/√(Hz)] Frequency [Hz] we measure m over 3km!

8 Initial detector

9 SourceN low N re N high VirgoNS-NS BH-BH 2 x AdvancedNS-NS BH-BH Initial detector

Spanner in the works… 10

11 External Injection Bench LASER bench Vacuum system Interferometer (3 km)

Beam jitter noise from external injection bench 12

Beam jitter noise from external injection bench Modes of legs and optics mounts introduce beam jitter noise 13 Needs to be reduced for AdV

Requirement on EIB motion 14

Commercial “shock damper”: STACIS 15 Frequency (Hz) Acceleration (m/s2)

Commercial “shock damper”: STACIS 16 No commercial product available! Frequency (Hz) Acceleration (m/s2)

Solution? Passive isolation technology 17

A simple pendulum is a 2 nd order low pass filter 18 1/f 2

Longer pendulum = better isolator 19 1/f 2

Long pendulum is impractical 20 ω 0 = 0.1 Hz → L = 24.8 m 1/f 2

Use inverted pendulum 21 1 m Gravity acts as anti-spring:

Horizontal isolation: inverted pendulum 22 Gravity acts as anti-spring: ω 0 = 0.1 Hz → L = 1 m

Vertical isolation: geometric anti-spring filter 23

Vertical isolation: geometric anti-spring filter 24 Tension in blade springs acts as anti-spring

Vertical isolation: geometric anti-spring filter 25 Tension in blade springs acts as anti-spring

External Injection Bench Seismic Attenuation system: EIB-SAS 26 Adapted from the HAM-SAS system

EIB-SAS 27 M. Kraan

EIB-SAS 28 M. Kraan

EIB-SAS 29 M. Kraan

EIB-SAS 30 M. Kraan

EIB-SAS 31 M. Kraan

EIB-SAS 32 M. Kraan

 Comply with seismic attenuation request  Long-term stability and DC control o 1 week o x ref ± 20 µm o θ ref ± 5 µrad  Stable w.r.t. temperature variations of 1 º C  Characterize mechanical modes and acoustic coupling Requirements 33

Inverted pendulum & GAS filter modes 34

Actively damp the IP and GAS filter resonances Real-time digital control system  800 kHz 18 bit ADCs  6 displacement sensors (LVDTs)  9 inertial sensors (geophones)  6 voice coil actuator 35

Actively damp low frequency resonances with blended sensor 36

Sensor correction with geophones on the ground 37 x direction y direction (vertical) z direction

Closed loop, long term stability (1 week) RMS deviation of set point is within requirement (5 µrad for tilt d.o.f., 20 µm for translational d.o.f.) 38

Closed loop stability w.r.t. temperature changes (-1°C) 39 As expected, vertical d.o.f. (y) affected strongest: < 3 µm/K Loop gain = ~ 130

Closed loop stability w.r.t. temperature changes (+1°C) 40 As expected, vertical d.o.f. (y) affected strongest: < 3 µm/K EIB-SAS can compensate for ± 3 K

Isolation performance 41

 GAS filter tuned to 300 mHz  60 dB 10 Hz  Above 50 Hz resonances in setup 42 Transfer function GAS filter

Transfer function EIB-SAS 43 Piezo shaker system

Transfer function EIB-SAS 44 Piezo shaker system

Vertical transfer function EIB-SAS < 100 Hz 45

Vertical transfer function EIB-SAS Hz Bounce mode of the springbox on the inverted pendulums

Eddy current damper for bounce 48 Hz 47 Springbox ~ 300 kg, damper 4 kg

Eddy current damper for bounce 48 Hz 48 Springbox ~ 300 kg, damper 4 kg

Vertical TF EIB-SAS > 100 Hz 49

Vertical TF EIB-SAS > 100 Hz 50 Springbox resonances Resonances of GAS filter blades

Vertical TF EIB-SAS > 100 Hz 51 Springbox resonances Resonances of GAS filter blades

Damping the 182 Hz resonance 52

Damping the 182 Hz resonance 53

Horizontal transfer function 54

Horizontal transfer function: 16 Hz mode 55

Horizontal transfer function: 16 Hz mode 56 Damped by control system

Horizontal transfer function: 37 Hz mode 57

Horizontal transfer function: 37 Hz mode 58

Damping 37 Hz mode 59

Damping 37 Hz mode 60 Frequency [Hz]

Horizontal transfer function: 88 Hz “mode” 61 Not a mode of EIB-SAS, but of excitation system

Does EIB-SAS meet the requirement? 62

Displacement spectrum of Virgo 63

EIB-SAS displacement Virgo 64

 New External Injection Bench Seismic Attenuation System for Advanced Virgo meets requirements  Measure EIB-SAS vertical TF with piezo shakers o Attenuate vertical ground motion with 40 dB o Horizontal with 60 dB  Installation in Advanced Virgo Nov Summary 65

66

Extra slides 67

SAS EIB LB SAS  MultiSAS features  Compact design o Inverted pendulums o Geometric antisprings o Consistent with m (rad)/√Hz (6 dof)  UHV compatible Latest activities: Multistage Seismic Attenuation System 68 multiSAS

Transfer function EIB-SAS: 1 st attempt 69 Excite the ground with a shaker bolted to the floor

Transfer function EIB-SAS: 1 st attempt 70 Excite the ground with a shaker bolted to the floor

Transfer function EIB-SAS: 1 st attempt 71 Acoustic coupling: Can we trust the TF measurement?

Improved measurement of vertical TF 72

Acoustic shielding will be improved for Advanced Virgo Commissioning EIB-SAS has shown the prominent role of acoustic noise above 100 Hz The walls between the central hall and the laser lab ( ▬ ) are cleanroom walls → they do not shield from acoustic noise 73 For AdV laser lab walls will be replaced by concrete walls

Interferometer (3 km) Vacuum system Injection system Output gravitational wave signal

Interferometer (3 km) Vacuum system Injection system

Transfer function of inverted pendulum κ

Frequency (Hz) Transfer function κ

Working on the bench: kinematic locking system Works on compressed air

Reproducibility of locked position 79  Locked position is reproducible within 50 µm/µrad  Floating position within 10 µm/µrad