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,

Slides:



Advertisements
Similar presentations
1 News in the thermo-mechanical measurement in the Firenze facility Gianpietro Cagnoli a,b), Enrico Campagna a,c), Elisabetta Cesarini a), Matteo Lorenzini.
Advertisements

STREGA Start up Meeting IGR - Geppo Cagnoli EGO – Cascina – 12 th May 2004.
Piero Rapagnani I.N.F.N. Sezione di Roma
Gravitational Wave Astronomy Dr. Giles Hammond Institute for Gravitational Research SUPA, University of Glasgow Universität Jena, August 2010.
Task M2 – Advanced Materials and Techniques for Resonant Detectors Motivation : Reduce thermal noise contribution to the acoustic detector noise budget.
Low temperature dissipative behavior in uncoated fused silica slabs Flavio Travasso Dip. Fisica – Università di Perugia and INFN Perugia Virgo - Perugia.
Aspects of Fused Silica Suspensions in Advanced Detectors Geppo Cagnoli University of Texas at Brownsville and TSC LIGO, Hanford.
Nawrodt 10/07 #1/21 R. Nawrodt, A. Schröter, C. Schwarz, D. Heinert, M. Hudl, W. Vodel, A. Tünnermann, P. Seidel STREGA Meeting Tübingen 10/
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.
Dublin/July'04 1 BLTS interferometers: Big, Low-temperature Transparent Silicon Interferometers Warren Johnson Louisiana State University LIGO-G Z.
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.
Thermal noise in GW detectors How much can an object be at rest on Earth? Geppo Cagnoli INFN - Firenze University of Glasgow ITIS Citta’
Cryogenics for LCGT Technical Advisory Committee for LCGT ICRR SUZUKI, Toshikazu High Energy Accelerator Research Organization.
Interferometric detector for GW: status and perspectives Giovanni Losurdo INFN Firenze-Urbino
Status of LCGT and CLIO Masatake Ohashi (ICRR, The University of TOKYO) and LCGT, CLIO collaborators TAUP2007 Sendai, Japan 2007/9/12.
Alban REMILLIEUX3 rd ILIAS-GW Annual General Meeting. London, October 26 th -27 th, New coatings on new substrates for low mechanical loss mirrors.
1 Kazuhiro Yamamoto Istituto Nazionale di Fisica Nucleare Sezione di Padova Substrate thermoelastic noise and thermo-optic noise at low temperature in.
STREGA WP1/M1 mirror substrates GEO LIGO ISA Scientific motivation: Mechanical dissipation from dielectric mirror coatings is predicted to be a significant.
Design study for ET 3rd generation Gravitational Wave Interferometer Work Package 2 Suspension, Thermal noise and Cryogenics Piero Rapagnani
Australia-Italy Australia 6, October 2005 LCGT project Kazuaki Kuroda LCGT Collaboration Cryogenics for LCGT.
Nawrodt 23/03/2011 Experimental Approaches for the Einstein Telescope Ronny Nawrodt on behalf of the Einstein Telescope Science Team and the ET DS Writing.
R&D activities in Florence Geppo Cagnoli INFN and U. of Glasgow WG2 & WG3 Meeting – 27 th Apr Firenze.
A new facility for thermal conductivity measurements Filippo Martelli Univ. of Urbino and INFN Florence GWADW 2006 – 27/5-02/ – La Biodola.
DFG-NSF Astrophysics Workshop Jun 2007 G Z 1 Optics for Interferometers for Ground-based Detectors David Reitze Physics Department University.
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.
[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.
January 12, 2006ILIAS-WG3 Frascati1 Virgo+ & Advanced Virgo B. Mours With material from G. Losurdo, M. Punturo, A. Viceré and others.
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.
LCGT Technical Review Suspension Point Interferometer for Parasitic Noise Reduction and an Additional IFO S.Miyoki (ICRR, Univ. of TOKYO)
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.
STREGA-C3 Cryogenic Seismic Isolation Roberto Passaquieti Dipartimento di Fisica “E. Fermi” Università di Pisa INFN sezione di Pisa ILIAS-GW Annual General.
ILIAS - GWA N5 - Strega JRA3 General Meeting Orsay - November 5th-6th, 2004 M1 Activities.
1 Kazuhiro Yamamoto Max-Planck-Institut fuer Gravitationsphysik (Albert-Einstein-Institut) Institut fuer Gravitationsphysik, Leibniz Universitaet Hannover.
Thermoelastic dissipation in inhomogeneous media: loss measurements and thermal noise in coated test masses Sheila Rowan, Marty Fejer and LSC Coating collaboration.
Janyce Franc-Kyoto-GWADW1 Simulation and research for the future ET mirrors Janyce Franc, Nazario Morgado, Raffaele Flaminio Laboratoire des Matériaux.
Thermal Noise in Thin Silicon Structures
Cryogenic Xylophone Kyoto May Kentaro Somiya Waseda Inst. for Adv. Study Collaboration work with S.Hild, K.Kokeyama, H.Mueller-Ebhardt, R.Nawrodt,
STREGA & ET - 4th ILIAS-GW general meeting 1 STREGA legacy for ET Michele Punturo INFN Perugia.
17/05/2010A. Rocchi - GWADW Kyoto2 Thermal effects: a brief introduction  In TM, optical power predominantly absorbed by the HR coating and converted.
Defining the volumes and functions of the cryogenic suspension Discussion guidance Kashiwa October JGW-G
111 Kazuhiro Yamamoto Institute for Cosmic Ray Research, the University of Tokyo Cryogenic interferometer technologies 19 May 2014 Gravitational Wave Advanced.
Advanced Towards Advanced Virgo Giovanni Losurdo – INFN Firenze Advanced Virgo Coordinator on behalf of the Virgo Collaboration.
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,
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 Kazuhiro Yamamoto Institute for Cosmic Ray Research The university of Tokyo LCGT internal review (Cryogenic payload) 30 January 2012.
E. Majorana (INFN – Rome) ELiTES 3 rd General Meeting Hongo Campus – Tokyo – 9-10 Feb., 2015 Cryogenic platform with vertical suspension: a practical approach.
STREGA WP4 coating development GEO LIGO ISA Scientific motivation: Mechanical dissipation from dielectric mirror coatings is predicted to be a significant.
Fulvio Ricci Cascina, November, 24th 2008
R&D VIRGO-EGO N5-W3 R&D EGO-VIRGO-July 8th, 2004.
Overview of the 20K configuration
Michele Punturo WP3 meeting, Cascina 9-July-2004
First clues on ET payload sensing and control
Pros and cons of cryogenics for Einstein Telescope and Cosmic Explorer
Mirror thermal noises and its implications on the mirror design
External forces from heat links in cryogenic suspensions
Superattenuator for LF and HF interferometers
Flat-Top Beam Profile Cavity Prototype: design and preliminary tests
Thermal effects of the small cryotrap on AdVirgo TM
Flat-Top Beam Profile Cavity Prototype
The views of Virgo collaboration groups on upgraded/advanced Virgo
Fast cooling of interferometer payload
R&D in Glasgow MATERIALS ACTIVITY AIM Silica
Presentation transcript:

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, F. Martelli, F. Piergiovanni, F.Vetrano –Perugia P.Amico, C.Bernardini, L.Gammaitoni, F.Marchesoni, M.Punturo, F.Travasso, H.Vocca –Pisa M. Al-Shourbagy, S.Bigotta, A.Di Lieto, L.Predolin, A.Toncelli, M.Tonelli

VIRGO-MAT3 M1 Activities Advanced materials for mirror substrates –Michelson-Morley ITF in Perugia (next slide) –Mechanical characterization of the VIRGO Mirror substrates in Perugia and in the site ( Vir-Not-Per ) –Measurement of substrates for future ITF CaF2 substrate ( P. Amico et al, Rev.Sci.Instr. 73 (2002), ) Monocrystalline Si substrate “Virgo like”

4 M1:Large substrate measurement facility PZT PHD Vacuum -6 mbar x HV Locking electronics Read-out electronics Pusher

VIRGO-MAT5 M2 Activities Advanced materials and techniques for resonant detectors “Support” role: –Long history in measurement of low losses materials –Several infrastructures to measure thermo-mechanical properties of fibers in Perugia and Firenze, at room temperature and at low temperature (M5 task) Two “clamp free” loss angle measurement facilities One cryostat under completion

VIRGO-MAT6 M4 activities Development of low loss dielectric coatings for advanced detectors Fabry-Perot facility to measure directly thermal noise in thin membranes (see P.Amico report in T1 task) –Coating effect of thin membranes and small mirrors Facility to measure the Q of coated membranes realized under the EGO R&D program and delivered to Lyon

VIRGO-MAT7 M5 activities R&D activities for next generation ITF suspension Realization of mono-crystalline fibers that could improve the suspension thermal noise at room temperature and at low temperature –Best candidate: silicon fibers/ribbons –Exotic cooling technique: anti-stokes fluorescence

VIRGO-MAT8 Micro-Pulling-Down furnace in Pisa

VIRGO-MAT9 Produced mono-crystalline fibers 10/03/04 L  4 cm 12/03/04 L  13 cm 16/03/04 L  13 cm 18/03/04 L  17 cm 22/03/04 L  11 cm 25/03/04 L  21 cm

VIRGO-MAT10 Evaluation of the thermo-elastic contribution 300K 200K 300K 300K 200K 200K Thermoelastic loss angle

VIRGO-MAT11 Particular behavior of Si Crystalline Silicon

VIRGO-MAT12 Magic temperature 100K 117K 100K

VIRGO-MAT13 How to cool locally? It is important to cool locally the flexural point –Cold finger Easy to implement Commercial Liquid N2 is enough Noisy –Anti-stokes fluorescence High difficulties Low (?) efficiency And the noise?

VIRGO-MAT14 Anti-Stokes Cooling To evaluate the temperature distribution along the wire, we must take in account the thermal conduction/dissipation processes Laser T0=300K Si fiber 200  m diameter 700 mm height SiO 2 clamp, 35mm diameter

VIRGO-MAT15 Thermal conduction mechanisms Usual thermo-dynamical sign definition Anti-stokes cooling Laser T0=300K  0 is the temperature where the efficiency goes to zero For ZPLAN we have M.T.Murtagh, J.of Non-Crystalline solids 253 (1999) 50-57

VIRGO-MAT16 Thermal conduction Conduction law qkqk qkqk For each small section we can discretize: IR Radiation

VIRGO-MAT17 Differential Equation The differential equation is, where T=T(t,y) It is a “bordello” then, I adopted a numerical solution

VIRGO-MAT18 Temperature distribution It is not linear and the noise evaluation must take in account it

VIRGO-MAT19 Noise contribution due to optical cooling Fundamentally, the optical cooling can introduce a length noise in the interferometer through the cooling laser power fluctuation coupled with the fiber length The laser power fluctuation causes a wire length fluctuation filtered by –Thermal conduction process –Vertical spring behavior of the suspension wire Laser power fluctuation Optical cooling efficiency Subtracted power fluctuation

VIRGO-MAT20 … noise evaluation 2 The integral length fluctuation is given by: Where T f is the temperature of the (cooled) flexural point, m the mass of the wire, c(T) is the specific heat and the average expansion coefficient is: Taking in account also the filtering effect of the thermal conduction:

VIRGO-MAT21 … noise evaluation 3 Taking into account that the loaded wire acts like a spring: Considering the (minimal) Vertical to Horizontal coupling:

VIRGO-MAT22 M5-Cx: “Classical” cryogenic design Drawing of a cryogenic payload for the EGO-VIRGO cryogenic facility –G.Cella, A.Giazotto, R.Passquieti, M.Punturo, F.Richard