Task M2 – Advanced Materials and Techniques for Resonant Detectors Motivation : Reduce thermal noise contribution to the acoustic detector noise budget.

Slides:



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

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.
Gravitational Wave Astronomy Dr. Giles Hammond Institute for Gravitational Research SUPA, University of Glasgow Universität Jena, August 2010.
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.
Laser Interferometer Gravitational-wave Detectors: Advancing toward a Global Network Stan Whitcomb LIGO/Caltech ICGC, Goa, 18 December 2011 LIGO-G v1.
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.
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.
Low temperature dissipative behavior in uncoated fused silica slabs Flavio Travasso Dip. Fisica – Università di Perugia and INFN Perugia Virgo - Perugia.
Acoustic properties of a prototype for a hollow spherical gravitational antenna (^) Laboratori Nazionali del Gran Sasso dell’INFN (*) Laboratori Nazionali.
April 27th, 2006 Paola Puppo – INFN Roma ILIAS Cryogenic payloads and cooling systems (towards a third generation interferometer) part II: the Vibration.
Work Package 4: Development of low loss dielectric coatings for advanced detectors Scientific motivation: Mechanical dissipation from dielectric mirror.
4th ILIAS-GW Annual Meeting J.P. Zendri Tuebingen 8-9 October 2007 Materials for Dual: Losses at low Temperature on Si and SiC.
18/6/2007 M.Taborelli, TS-MME Structure fabrication techniques and possibilities M.Taborelli Disk structures Quadrant structures ….most of it inspired.
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,
September 8, 2015 THE MONOLITHIC SUSPENSION STATUS FOR THE VIRGO INTERFEROMETER THE MONOLITHIC SUSPENSION STATUS FOR THE VIRGO INTERFEROMETER Helios Vocca.
Low noise Fused Silica suspensions: from the GEO600 experience to the 2 nd generation requirements Geppo Cagnoli INFN Sez. Firenze University of Glasgow.
ILIAS GW Meeting Mallorca - October 23-24, 2005Luca Taffarello Status of the commissioning of the AURIGA detector Luca Taffarello (INFN Sezione di Padova)
STREGA WP1/M1 mirror substrates GEO LIGO ISA Scientific motivation: Mechanical dissipation from dielectric mirror coatings is predicted to be a significant.
1 Paolo Falferi - ET WG2 meeting - Glasgow, 22/7/2010 Actuator magnetic noise measurement and possible developments Paolo Falferi CNR-FBK Trento and INFN.
Summary and Plans for the WG3 activity H.Lück, M.Punturo.
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.
Ultra-cryogenics for advanced resonant detectors (C2) G.Frossati Kamerlingh Onnes Laboratory Leiden, The Netherlands Second ILIAS-GW Meeting.
LISA October 3, 2005 LISA Laser Interferometer Space Antenna Gravitational Physics Program Technical implications Jo van.
Lisbon, 8 January Research and Development for Gravitational Wave Detectors Raffaele Flaminio CNRS/LMA Lyon.
JRA3 STREGA - Introduction Geppo Cagnoli IGR – University of Glasgow ILIAS-GW Meeting, Orsay, 5 th -6 th Nov 2004.
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.
Flat-Top Beam Profile Cavity Prototype
Silicon as material for 3rd Generation detectors Geppo Cagnoli University of Glasgow INFN Sez. Firenze 2 nd ILIAS-GW Meeting – 25 th Oct. 2005, Palma de.
Task M2 – Working group Auriga-LNL Operation temperature KOperation temperature K Mechanical Attenuation >180dB in the frequency range.
Cold damping of fused silica suspension violin modes V.P.Mitrofanov, K.V.Tokmakov Moscow State University G Z.
R&D on thermal noise in Europe: the STREGA Project Geppo Cagnoli University of Glasgow AMALDI 6 – Okinawa - Japan June
Francesco Cottone INFN & Physics Departments of Perugia, Pisa, Florence (Collaboration Work under VIRGO Project) Thermomechanical properties of silicon.
ILIAS - GWA N5 - Strega JRA3 General Meeting Orsay - November 5th-6th, 2004 M1 Activities.
Virgo-Material “macro” group M.Punturo. VIRGO-MAT2 VIRGO-MAT components Virgo-MAT is composed by three INFN groups –Firenze/Urbino M.Lorenzini, G.Losurdo,
Experimental investigation of dynamic Photothermal Effect
Thermal Noise performance of advanced gravitational wave detector suspensions Alan Cumming, on behalf of the University of Glasgow Suspension Team 5 th.
Thermoelastic dissipation in inhomogeneous media: loss measurements and thermal noise in coated test masses Sheila Rowan, Marty Fejer and LSC Coating collaboration.
Thermal Noise in Thin Silicon Structures
WG3 Report Michele Punturo Harald Lück. WG3 composition Co-Chairmen M.Punturo INFN Perugia, Italy H.Lück MPI für Gravitationsphysik, AEI, Hannover, Germany.
ACIGA High Optical Power Test Facility
TD26CC PLANS FROM CIEMAT Laura Sánchez on behalf Electrical Engineering Group of CIEMAT.
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,
Heinert et al Properties of candidate materials for cryogenic mirrors 1 Properties of candidate materials for cryogenic mirrors D. Heinert,
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.
1 Kazuhiro Yamamoto Institute for Cosmic Ray Research The university of Tokyo LCGT internal review (Cryogenic payload) 30 January 2012.
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.
1 The control of the Virgo mirrors is realized using coil-magnet actuators Can this technique be used in ET, from room to cryogenic temperatures? Is the.
Active Vibration Isolation using a Suspension Point Interferometer Youichi Aso Dept. Physics, University of Tokyo ASPEN Winter Conference on Gravitational.
Department of Physics & Astronomy Institute for Gravitational Research Scottish Universities Physics Alliance Brownian thermal noise associated with attachments.
STREGA WP4 coating development GEO LIGO ISA Scientific motivation: Mechanical dissipation from dielectric mirror coatings is predicted to be a significant.
Material Downselect Rationale and Directions Gregory Harry LIGO/MIT Kavli Institute for Astrophysics and Space Technology On behalf of downselect working.
Michele Punturo WP3 meeting, Cascina 9-July-2004
Studies of some properties of Hydroxide-Catalysis Bonds
Wide Bandwidth Dual Acoustic GW Detectors
MiniGRAIL “Extreme Make-over” Giorgio Frossati
Chapter 1 Morphologic Process Model
Flat-Top Beam Profile Cavity Prototype: design and preliminary tests
Renzo F. Parodi INFN-Genova
Flat-Top Beam Profile Cavity Prototype
The ET sensitivity curve with ‘conventional‘ techniques
R&D in Glasgow MATERIALS ACTIVITY AIM Silica
Presentation transcript:

Task M2 – Advanced Materials and Techniques for Resonant Detectors Motivation : Reduce thermal noise contribution to the acoustic detector noise budget.

Task M2 – General Strategy A) Reduce thermal noise power spectrum 1)Find the materials with the lowest mechanical and/or electrical dissipation and suitable to be cooled down at cryogenic temperatures (Mo,Be,SiC,CuAl,….) 2)Find the assembling and joining procedures that preserve the Q- factor of the material (explosion welding, silica bonding…)

Task M2 – General Strategy B) Reduce the relative contribution of thermal noise (i.e. increase the transducer efficiency  ) Surface treatments, two faces transducer,.. For the capacitive transducer:  is proportional to the Electric bias field For the optical transducer:  is prop. to the laser Power 1/2 time the Finesse  is prop. to the laser Power 1/2 time the Finesse

Task M2 – Advanced Materials and Techniques for Resonant Detectors Main outcomes : - Construction and test of high sensitivity and of low loss capacitive and optical displacement transducers - -Low temperature measurement of the mechanical Q, thermal expansion and heat capacity of several materials (Mo,Be,CuAl,SiC…). -Find joining procedures (electron beam, explosion beam welding, silicate bonding) and surface treatment which preserve high Q-factors. - Low temperature measurement of dielectric losses.

Task M2 – Advanced Materials and Techniques for Resonant Detectors Working GroupFacility used for M2Expertise for M2 INFN ROG MAT Cryogenic facility for testing mechanical and electromechanical resonators Low loss materials, low temperature Q measurements INFN Virgo MAT Clean rooms, Q measurement facilities, mechanical properties measurement facility, hard material milling machine Low loss suspensions, silicate bonding technology, thermal noise, interferometry INFN AURIGA LNL Ultra low temperature test facility for mechanical and optical displacement sensors Cryogenics, interferometry, low loss materials IFN Ultra low temperature test facilityFEM, low loss matching networks for SQUID amplifiers Leiden Ultra low temperature test facilityUltra low temperature technology, low loss electromechanical transducers IGR MAT Q measurements facilities and clean room Low loss suspensions, bonding, thermal noise, interferometry

9.JRA3 First 18 months Implementation Plan Tasks and Deliverables1 st to 6 th month7 th to 12 th month13 th to 18 th month WP 1 - Task M2: Advanced materials and techniques for resonant detectors Tasks: Construction of first CuAl, SiC and Be resonators Construction of first optical and cap. transducers Low T and low frequency, Q measurements on CuAl, SiC and Be Test of a metallic trans. on a resonant sphere Effect of the dieletric coating on the thermal noise Experiments on limiting bias electric fields in the capacitive transducer Upgrade of suspension performance of test facility Surface loss measurements at low temperature after chemical treatment Q of silicate bonding on SiC at low T (as part of improving fab. processes) Deliverables: - CuAl, SiC and Be resonator prototypes - Optical and capacitive transducer prototypes

M2.1 - M2.1 - Construction of first CuAl, SiC and Be resonators Working groups Rog, Auriga LNL,Leiden Working groups Rog, Auriga LNL,Leiden Be Hot Isostatic Pressure (ROG,LNL) Mo CuAl (ROG,Leiden) “Pure” resonators Transducer resonators Apr04-Sep04

M2.1 - M2.1 - Construction of first CuAl, SiC and Be resonators Working groups Auriga LNL, IFN Working groups Auriga LNL, IFN C/SiC resonator: status “..The size of the structures that can be manufactured is limited by the scale of the currently available facilities (3mx3mx4m)...” Best geometry under investigation

M2.3 - M2.3 -Low T and low frequency, Q measurements on CuAl, SiC and Be Optical read-out (ready) Working groups Leiden, Auriga LNL, IFN, ROG Working groups Leiden, Auriga LNL, IFN, ROG Apr04-Sep05 the last stage of suspension has to be designed and tested with high Q resonators First results for CuAl resonators: Q 300K =20000, Q LN2 =(3-5)x10 4, Q LHe4 =(5-10)x10 5 For the other materials measurements will be done at LNL: Capacitive read-out (for metal samples)

M2.3 - M2.3 -Low T and low frequency, Q measurements on CuAl, SiC and Be LNL Cryogenic test facility, optical readout

M2.2 -Construction of Optical and Capacitive transducers Optical Transducer: Working groups Auriga Fi,Pd,LNL Construction of the optical transducer is complete Low T Q-factor measurements in the TTF Apr04-Sep04 Only Resonator Assembled

M2.2 -Construction of Optical and Capacitive transducers M2.2 -Construction of Optical and Capacitive transducers Optical Transducer: Next step (Spring 2005) Up-grading

M2.2 -Construction of Optical and Capacitive transducers Capacitive Transducer: Working groups Leiden, Rog Many Capacitive transducer has been constructed Apr04-Sep04 ROG Leiden Rosetta Transducer, CuAl, gap 15  m, freq= 3200 Hz Rosetta Transducer, CuAl, gap 15  m, freq= 3200 Hz Double face transducer, Al5056, freq=920 Hz Double face transducer, Al5056, freq=920 Hz Rosetta Transducer Rosetta Transducer Drum Transducer + Bolt free assembling Drum Transducer + Bolt free assembling MiniGrail Transducer

M2.4 M2.4 Test of a metallic transd. on a resonant sphere Oct04-Dec05 Working groups Leiden, ROG Working groups Leiden, ROG T= 5 K MiniGrail Thermal noise dominated at 5K SQUID output PSD

M2.5 M2.5 Effect of the dielectric coating on the thermal noise Working groups Rog,IFN, Leiden, Auriga LNL Working groups Rog,IFN, Leiden, Auriga LNL Apr05-Dic05 1.Electric losses: measure of the electrical quality factor of a cryogenic LC resonator. The dielectric under investigation fills the capacitor gap. Sensitivity of the existing apparatus (IFN)  = Mechanical losses: measure the quality factor of transducers having dielectric coating. The available facilities are ROG, Leiden, LNL

M2.6 M2.6 - Experiments on limiting bias electric fields in the capacitive transducer Working groups Leiden, IFN, Auriga LNL Working groups Leiden, IFN, Auriga LNL Typical value for operating detectors MV/mTypical value for operating detectors MV/m Best result 25MV/m Leiden-MiniGrail July 2004Best result 25MV/m Leiden-MiniGrail July 2004 Test of surface treatment on small sample (goal 100 MV/m).Test of surface treatment on small sample (goal 100 MV/m). Oct04-Dic05 Experimental set-up (ready) Samples (ready) -Al5056 -Diameter 3 cm -Single point diamond turning (optical quality) -Dielectric coating (if need) still to be done

M2.9 M2.9 - Q of silicate bonding on SiC at low T (as part of improving fabrication processes) Apr05-Dec05 Working groups Auriga LNL, Virgo MAT, IGR MAT Working groups Auriga LNL, Virgo MAT, IGR MAT Assemble the resonators using silicate bonding and then measure the mechanical quality factor Silicate Bonding

Task M2 – Advanced Materials and Techniques for Resonant Detectors Conclusions 1.Almost all the objective of the first 6 months as been obtained. 2.According to the time schedule the second part of the program has begun.