Task M2 – Working group Auriga-LNL Operation temperature 0.02-300KOperation temperature 0.02-300K Mechanical Attenuation >180dB in the frequency range.

Slides:



Advertisements
Similar presentations
STREGA Start up Meeting IGR - Geppo Cagnoli EGO – Cascina – 12 th May 2004.
Advertisements

STREGA C1:Cryogenic Last Stage Suspension (10 MIN) Task -C1: thermal conduction investigation of final stage suspension; This part of the suspension system.
STREGA C2:Cryogenic suspension system for advanced resonant detectors (5 MIN) Task -C2: development and construction of advanced cryogenic system for resonant.
STREGA M2:Advanced materials and techniques for resonant detectors (5 MIN) Participants: INFN * -Istituto Nazionale di Fisica Nucleare IFN-Istituto di.
ILIAS 5-6/11/2004 WG T2 Task T2 (WG 11) AIM: exact definition (theoretical and experimental) of photo-thermal noise PARTICIPANTS INFN (AURIGA group; also.
Task M2 – Advanced Materials and Techniques for Resonant Detectors Motivation : Reduce thermal noise contribution to the acoustic detector noise budget.
T1 task- update Mike Plissi. 2 Collaboration Groups actively involved INFN-VIRGO MAT IGR-Glasgow Groups that have expressed interest INFN-AURIGA CNRS-LKB.
Participants: C-1:Cryogenic last-stage suspensions (interferometers) (F.Ricci-G.Frossati) Objectives: -Design new suspension elements for the last stage.
T3 considers two aspects of the thermal noise The problem of the interrogation area of the test mass. Small interrogation area means large fluctuations.
WP-M3 Superconducting Materials PArametric COnverter Detector INFN_Genoa Renzo Parodi.
Design and performance of the Dual detector with large area capacitive readout 4 rd ILIAS-GW Meeting, October 8 th – 9 th 2007, Tuebingen Paolo Falferi.
G R LIGO Laboratory1 Advanced LIGO Research and Development David Shoemaker LHO LSC 11 November 2003.
April 27th, 2006 Paola Puppo – INFN Roma ILIAS Cryogenic payloads and cooling systems (towards a third generation interferometer) part II: the Vibration.
4th ILIAS-GW Annual Meeting J.P. Zendri Tuebingen 8-9 October 2007 Materials for Dual: Losses at low Temperature on Si and SiC.
Dual Sphere Detectors by Krishna Venkateswara. Contents  Introduction  Review of noise sources in bar detectors  Spherical detectors  Dual sphere.
LIGO-G W LIGO II Pre-stabilized Laser System Design Requirements and Conceptual Design David Ottaway, Todd Rutherford, Rick Savage, Peter Veitch,
The AMS-02 detector is based on a large acceptance (~0.5 m²sr) and high sensitivity spectrometer composed by a super-conducting magnet (0.8 T), cooled.
Mechanical amplifiers for the DUAL detector: lumped and distributed element design 3 rd ILIAS-GW Meeting, October 26 th – 27 th 2006, London Paolo Falferi.
ILIAS meeting Mallorca 2005 V. Fafone Viviana Fafone INFN - LNF Future plans for resonant detectors
An optomechanical transducer for the AURIGA “bar” gw detector cryogenic optics towards the quantum limit: high finesse cavities, fibers, piezo actuators,
TeV Particle Astrophysics August 2006 Caltech Australian National University Universitat Hannover/AEI LIGO Scientific Collaboration MIT Corbitt, Goda,
September 8, 2015 THE MONOLITHIC SUSPENSION STATUS FOR THE VIRGO INTERFEROMETER THE MONOLITHIC SUSPENSION STATUS FOR THE VIRGO INTERFEROMETER Helios Vocca.
GWADW 2010 in Kyoto, May 19, Development for Observation and Reduction of Radiation Pressure Noise T. Mori, S. Ballmer, K. Agatsuma, S. Sakata,
ILIAS GW Meeting Mallorca - October 23-24, 2005Luca Taffarello Status of the commissioning of the AURIGA detector Luca Taffarello (INFN Sezione di Padova)
Alban REMILLIEUX3 rd ILIAS-GW Annual General Meeting. London, October 26 th -27 th, New coatings on new substrates for low mechanical loss mirrors.
Optical readout for a resonant gw bar. Old setup.
STREGA WP1/M1 mirror substrates GEO LIGO ISA Scientific motivation: Mechanical dissipation from dielectric mirror coatings is predicted to be a significant.
CNRS LKB – Task T1 Current status of the experiment on optomechanical coupling Sensitivity: 5.10  20 m.Hz  1/2   New high-finesse, high-power cavity.
Test mass dynamics with optical springs proposed experiments at Gingin Chunnong Zhao (University of Western Australia) Thanks to ACIGA members Stefan Danilishin.
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.
1 Paolo Falferi - ET WG2 meeting - Glasgow, 22/7/2010 Actuator magnetic noise measurement and possible developments Paolo Falferi CNR-FBK Trento and INFN.
SUSPENSION DESIGN FOR ADVANCED LIGO: Update on GEO Activities Norna A Robertson University of Glasgow for the GEO 600 suspension team LSC Meeting, Louisiana,
Design study for ET 3rd generation Gravitational Wave Interferometer Work Package 2 Suspension, Thermal noise and Cryogenics Piero Rapagnani
T1 task- update Mike Plissi. 2 Motivation  Thermo-elastic noise is higher than the ‘intrinsic’ noise in crystalline materials  There are several sources.
New materials for DUAL: the LNL activity. Dual detector : Best material parameters Two different materials ‘A’ and ‘B’ with two different Young modulus.
GEO600 Detector Status Harald Lück Max-Planck Institut für Gravitationsphysik Institut für Atom- und Molekülphysik, Uni Hannover.
JRA3 STREGA - Introduction Geppo Cagnoli IGR – University of Glasgow ILIAS-GW Meeting, Orsay, 5 th -6 th Nov 2004.
The AURIGA experiment: updates and prospects BAGGIO Lucio ICRR on behalf of AURIGA collaboration The AURIGA detector re-started data taking in Dec 2003,
SUSPENSION DESIGN FOR ADVANCED LIGO: Update on GEO Activities Norna A Robertson University of Glasgow for the GEO 600 suspension team LSC Meeting, Hanford.
Toward a 3rd generation European Gravitational Wave Observatory Dual R&D: presented by Massimo Cerdonio INFN Section and Department of Physics Padova how.
R&D on thermal noise in Europe: the STREGA Project Geppo Cagnoli University of Glasgow AMALDI 6 – Okinawa - Japan June
ILIAS - GWA N5 - Strega JRA3 General Meeting Orsay - November 5th-6th, 2004 M1 Activities.
Experimental investigation of dynamic Photothermal Effect
1 PAY Review Meeting 1 18/3/2009 Piero Rapagnani 18/03/2009.
1 Kazuhiro Yamamoto Institute for Cosmic Ray Research The university of Tokyo Report from sub-groups Cryogenic Cryogenic payload 4 August 2011.
FNAL efforts on LHC Crab Cavity R&D (Proposals for R&D sub-tasks, resources and schedule) Nikolay Solyak.
Mechanical Mode Damping for Parametric Instability Control
2009/6/25Amaldi 8 in NewYork City1 Thermal-noise-limited underground interferometer CLIO Kazuhiro Agatsuma and CLIO Collaborators Institute for Cosmic.
Monica VarvellaIEEE - GW Workshop Roma, October 21, M.Varvella Virgo LAL Orsay / LIGO CalTech Time-domain model for AdvLIGO Interferometer Gravitational.
LIGO-G Z Silicon as a low thermal noise test mass material S. Rowan, R. Route, M.M. Fejer, R.L. Byer Stanford University P. Sneddon, D. Crooks,
ROG MAT Group: Bassan M., Minenkov Yu., Rocchi A., Simonetti R. – Roma2, INFN Fafone V., Quintieri L. – LNF ILIAS – GW Meeting report May 2004.
Friedrich-Schiller-University Jena Institute of Solid State Physics – Low Temperature Physics Christian Schwarz 15 th September Genoa 1 Investigation.
WP2-WP3 Joint Meeting - Jena - March 1-3, Several different mechanisms contribute to the thermal noise of the mirror: Brownian (BR)(substrate, coating)
The coating thermal noise R&D for the 3rd generation: a multitechnique investigation E. Cesarini 1,2), M.Prato 3), M. Lorenzini 2) 1)Università di Urbino.
E. Majorana (INFN – Rome) ELiTES 3 rd General Meeting Hongo Campus – Tokyo – 9-10 Feb., 2015 Cryogenic platform with vertical suspension: a practical approach.
Lessons from CLIO Masatake Ohashi (ICRR, The University of TOKYO) and CLIO collaborators GWADW2012 Hawaii 2012/5/16.
Friedrich-Schiller-University Jena Institute of Solid State Physics – Low Temperature Physics Christian Schwarz Current status of the bulk.
Fulvio Ricci Cascina, November, 24th 2008
Michele Punturo WP3 meeting, Cascina 9-July-2004
Wide Bandwidth Dual Acoustic GW Detectors
Cryogenic Si-Si Bond Strength Testing
Superattenuator for LF and HF interferometers
Ponderomotive Squeezing Quantum Measurement Group
Advanced LIGO Quantum noise everywhere
Jim Hough for the GEO collaboration
T3 DEVELOPMENT OF SELECTIVE READOUT SCHEMES
A. Heidmann M. Pinard J.-M. Courty P.-F. Cohadon
R&D in Glasgow MATERIALS ACTIVITY AIM Silica
Optical fiber based sensors for low temperature and superconductors
Presentation transcript:

Task M2 – Working group Auriga-LNL Operation temperature KOperation temperature K Mechanical Attenuation >180dB in the frequency range HzMechanical Attenuation >180dB in the frequency range Hz Sub-task: Construction of optical transducer Present state Cryogenic Test facilityCryogenic Test facility Optical readout (now available)Optical readout (now available)

Task M2 – Working group Auriga-LNL Q-Measurements results at 4.2K Mode #1: 908 Hz Mode #2: 1479 Hz Read-out scheme Mode#1 Q=10 6 Mode#2 Q=5.3 x 10 6

Task M2 – Working group Auriga-LNL First 18 months (starting now) Four years Four years 1. 1.Room temperature optical bench S nn <10 -5 Hz Motorized optics mounts for cryogenic alignment 3. 3.Operation at cryogenic temperature 1. 1.Improvement of the mirrors properties: Finesse >10 5, Al 2 O 3 mirrors 2. 2.Achievement of goal sensitivity to gw (S hh ~ Hz -1/2 )

Task M2 – Working group Auriga-LNL Sub-task: Present state k, Q measurements at low T 2. 2.Construction of resonators of CuAl, SiC Be Cryogenic test facility 2. 2.Optical readout for cryogenic Q-measurements First 18 months (starting now) 1. 1.Design and construction of the resonators in the kHz region 2. 2.Modification of the cryogenic suspensions to preserve Q 3. 3.Measurements of Q and k at low T Last time (months 19-24) Conclude low temperature measurements

Task M2 – Working group Auriga-LNL Sub-task: Improving fabrication process Present state First 18 months (staring month 12) Last years (months 13-36) Cryogenic test facility and optical readout for the Q-measurements 1. 1.Assembling transducer and resonators using different joining procedures as silicate bonding 2. 2.Q-measurement after bonding (kHz region) beginning 1. 1.Low temperature Q and k-measurement after bonding 2. 2.Comparison of the results with the single piece machined resonators

Task M2 – Working group Auriga-LNL Other collaborations with the working groups of the task 1. 1.IFN->Limiting bias electric field in the capacitive transducer and effect of dieletric coating on the thermal noise ROG,Leiden->Capacitive transducer All->writing up the final report.