STREGA-C3 Cryogenic Seismic Isolation Roberto Passaquieti Dipartimento di Fisica “E. Fermi” Università di Pisa INFN sezione di Pisa ILIAS-GW Annual General.

Slides:



Advertisements
Similar presentations
STREGA WP2 - Task C3 Roberto Passaquieti Dipartimento di Fisica E. Fermi Università di Pisa INFN sezione di Pisa ILIAS-GW GENERAL MEETING, Orsay 5 November.
Advertisements

STREGA C1:Cryogenic Last Stage Suspension (10 MIN) Task -C1: thermal conduction investigation of final stage suspension; This part of the suspension system.
Piero Rapagnani I.N.F.N. Sezione di Roma
STREGA C2:Cryogenic suspension system for advanced resonant detectors (5 MIN) Task -C2: development and construction of advanced cryogenic system for resonant.
Io ILIAS - STREGA MEETING
ET- WP2, Thermal noise issues Fulvio Ricci Assergi (L’Aquila) Laboratori Nazionali del Gran Sasso, February, 9th 2008.
Task M2 – Advanced Materials and Techniques for Resonant Detectors Motivation : Reduce thermal noise contribution to the acoustic detector noise budget.
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,
Participants: C-1:Cryogenic last-stage suspensions (interferometers) (F.Ricci-G.Frossati) Objectives: -Design new suspension elements for the last stage.
MICE RF and Coupling Coil Module Outstanding Issues Steve Virostek Lawrence Berkeley National Laboratory MICE Collaboration Meeting October 26, 2004.
Andrea Paoli AdV 1 st Project Review Cascina, November 3 rd, 2008 IME – infrastructure modifications for environmental noise reduction.
April 27th, 2006 Paola Puppo – INFN Roma ILIAS Cryogenic payloads and cooling systems (towards a third generation interferometer) part II: the Vibration.
Seismic attenuation chains concept, design and advancement status Riccardo DeSalvo for the KAGRA Seismic group JGW-G September 10, 20121JGW-G
Rahul Kumar1, T. Takayuki1, K. Yamamoto2, H. Tanaka2,T. Miyamoto2, T
September 8, 2015 THE MONOLITHIC SUSPENSION STATUS FOR THE VIRGO INTERFEROMETER THE MONOLITHIC SUSPENSION STATUS FOR THE VIRGO INTERFEROMETER Helios Vocca.
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
LBNL Test Cryostat Preliminary Design Review Tuning – Field Correction Soren Prestemon, Diego Arbelaez, Heng Pan, Scott Myers, Taekyung Ki.
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.
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.
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.
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,
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.
JRA3 STREGA - Introduction Geppo Cagnoli IGR – University of Glasgow ILIAS-GW Meeting, Orsay, 5 th -6 th Nov 2004.
1 Kazuhiro Yamamoto Institute for Cosmic Ray Research (ICRR) the University of Tokyo ELiTES first collaboration meeting Sanjo conference hall, the University.
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,
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.
External forces from heat links in cryogenic suspensions D1, ICRR, Univ. Tokyo Takanori Sekiguchi GWADW in Hawaii.
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,
Low frequency anti-vibration system of LCGT Vibration Isolation Group R. Takahashi (ICRR), K. Yamamoto (ICRR), T. Uchiyama (ICRR), T. Sekiguchi (ICRR),
Cryogenic Payload Issues
STREGA & ET - 4th ILIAS-GW general meeting 1 STREGA legacy for ET Michele Punturo INFN Perugia.
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.
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.
CERN, 27-Mar EuCARD NCLinac Task /3/2009.
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 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.
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.
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,
Paola Puppo INFN – Rome Thermal Noise Meeting – “Sapienza”-Rome - February 26 th 2008.
VIRGO Superattenuator performance and its evolution in the SAFE Project F. Frasconi – INFN Pisa (ET-WP2 Workshop – Roma – February 27, 2009)
Vibration measurements at KAGRA site
Fulvio Ricci Cascina, November, 24th 2008
Performance test of KAGRA cryostat at site
Last stage SA F7 monitor/control
Michele Punturo WP3 meeting, Cascina 9-July-2004
First clues on ET payload sensing and control
VIRGO–KAGRA Meeting about bottom filter damping
Performance test of KAGRA cryostat at site
LCGT Seismic Attenuation System LCGT-SAS
Radiation shield vibration measurement at KAGRA site
Status of KAGRA Cryogenics II
Vibration measurements at KAGRA site
Control of the KAGRA Cryogenic Vibration Isolation System
External forces from heat links in cryogenic suspensions
Superattenuator for LF and HF interferometers
The Superattenuator upgrades and the SAFE Project
The views of Virgo collaboration groups on upgraded/advanced Virgo
Presentation transcript:

STREGA-C3 Cryogenic Seismic Isolation Roberto Passaquieti Dipartimento di Fisica “E. Fermi” Università di Pisa INFN sezione di Pisa ILIAS-GW Annual General Meeting, Palma de Mallorca October 2005

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October STREGA-C3 Task: Description The aim of C3 task is to realize a full anti-seismic cryogenic suspension system (cryostat+suspension) performing like a Virgo Superattenuator (SA). –Main Actions: to design a cryo-compatible suspension prototype; to install the prototype into a cryogenic environment; to investigate and reduce the extra noise induced by the refrigerator. To achieve such results it is foreseen the merging with the activities of C1 task; especially from the 4th year (1997) of the STREGA project (investigation on sensors and actuators; material properties; noise studies; simulation; etc.).

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October –Design and FEA of a Si test payload intended for a 1:1 scale measurement of the Si mirror Q down to ~ 5K with/without coating. –Investigations on high compliance thermal links at room temperature. –Assembly of a small suspension prototype (SAS) at room temperature. –Contribution to the realization of the EGO cryogenic test facility(CTF). –Design of a full scale cryogenic suspension prototype. C3 Task: Main Activities Ta 2 O 5 coatings, Yamamoto 2003

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October Task C3: 5 Years Implementation Plan Budget: ~18.4 k€

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October Task C3: Month Timetable

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October Si Payload Prototype: Design The designed test payload consists of a Si mirror (350mm diam., 100 mm thick) suspended to a Si marionette by two couples of monolithic silicon ribbons (300 x 30 x 0.8 mm 3 each). Si thermal expansion coefficient shows two zero crossings at  123K and  17K. Displacement fluctuations of mirror driven by thermal expansion are strongly reduced at these low temperature values. Si relatively high thermal conductivity has also positive effects in reducing mirror thermal lensing

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October Si Payload: Design and FEA

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October EGO Cryogenic Test Facility (CTF) The EGO CTF is placed in a building (~ 450 m 2 ) at the mid of the West arm of the Virgo interferometer. The EGO CTF cryostat has an inner 4K chamber able to contain a test payload with one anti-seismic filter stage. It will be suspended over a pit in the ground floor (13.8 x 5.45 x 1.95 m 3 ). CTF W N

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October Status of Works at the EGO-CTF The EGO-CTF infrastructure works are quite advanced: –the pit on the ground is completed; –the cryostat suspension structure is assembled; –the computer room and the laboratories are foreseen to be delivered by the mid of next November.

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October Cryostat Support and Service Structures

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October The EGO-CTF Cryostat The designed cryostat consists of an external vacuum-proof steel cylindrical vessel (2.6m height, 1.4 m diameter). Inside the room temperature vessel there are two nested super-insulated Al chambers which are foreseen to reach their thermal equilibrium respectively at about 80K and 4K. The 4K chamber will host the payload; it has an height of 2m and a diameter of 1.2m. 1.2m 2m

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October The Cryo-Cooler The EGO-CTF cryo-cooling system is initially based on two pulse tube refrigerators (PTR). The Pulse Tube Refrigerator essentially achieves criogenic temperature by expanding high pressure He gas to low pressure (  2Hz). Compression/expansion cycles are source of low frequency excess noise. –The INFN Pisa group (C3) will collaborate with the INFN Roma1 group (C1) that has already achieved experience on the PTR noise reduction. PT410W: Power: 50Hz Stage1: 25K stage2: 4.2K 2.8K Cooling: Liquid Acoust.N: PT410W: Power: 50Hz Stage1: 25K stage2: 4.2K 2.8K Cooling: Liquid Acoust.N: PT60W: Power: 50Hz Stage1: 80K Cool.Thr.: 30K Cooling: Liquid PT60W: Power: 50Hz Stage1: 80K Cool.Thr.: 30K Cooling: Liquid

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October Status of the EGO-CTF Cryostat. Cryomech Pt and compressors, are already purchased. The EGO-CTF infrastructure are being completed The last version of the cryostat design was ready from February –The cryostat has been already built. – Assembly and vacuum leak tests are being performed in the delivering workshop (Cryoanlagenbau) in Germany.

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October The AISI 316L external vessel The 2 AL, super-insulated, inner vessels The EGO-CTF Cryostat

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October The EGO-CTF Cryostat

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October The EGO-CTF Cryostat

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October Cryogenic SA Design: Components SA functional blocks: Filters Blades Magnets for anti-springs Dampers Sensors: LVDT, accelerometers Actuators: coils+magnets Cables Motors Adhesives Need to be tested for cryogenics.

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October Cryogenic SA Design: Materials Suitable materials: 300-series austenitic steels: 304, 304L, 316, 321, 304LN, 316LN OFHC copper and deoxidized copper Al alloys: 6061, 6063, 1100 Titanium, Niobium Invar Kapton, mylar quartz Not recommended (undergo ductile to brittle transition) : martensitic steels carbon steels rubbers, plastics, Teflon Maraging: 18Ni (200) series, already tested at room temperature down to 100K, exhibit ductile fracture

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October Suspension Prototype Assembly A small scale suspension prototype (SAS) is being assembled at the Pisa INFN laboratories. It exhibits less cryogenic incompatible items (no magnets, no glue, no viton) and could be used at 4 K with minor modifications Foreseen Activities: room temperature tests on –blades, –sensors, –actuators.

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October Investigations for a Cryogenic SA List of Investigations: Selection of material for thermal links; measurement of the link stiffness down to cryogenic temperatures; measurement of the link thermal impedance. Quality factor measurement of damping materials at low temperatures. Definition of mechanical and thermal behavior of materials for filter components; test of a full assembled filter at cryogenic temperature. Dimensioning of the electric cables, keeping into account the heat conduction and dissipation. Test of the LVDT sensors and accelerometers at cryogenic temperatures. Qualification of cryogenic motors and traslators. Qualification of the pulse tubes from the point of view of their vibrations; design of a vibration attenuation system.

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October Extra Stiffness Measurement of Soft Thermal Link 1x1x70 cm Aluminum l=60 cm Set of stripes Test Apparatus Prototype: set of brass strips (0.3X0.01X m 3 each) Prototype: set of brass strips (0.3X0.01X m 3 each)

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October Cryogenic SA Prototype: Preliminary Design

Roberto Passaquieti ILIAS-GW Meeting, Palma, 25 October Conclusions - The first year plan was fulfilled:a Si payload prototype was designed and its FEA was performed. - A small scale suspension prototype is being installed at the Pisa INF laboratory. - The EGO CTF is being delivered together with its cryostat. - The work done on the jellifish prototype need to be extended at low temperature. - The design of the cryogenic SA prototype and its cryostat is started. A preliminary design has been delivered (2 nd year deliverable). - Interactions beetwen C1 and C3 tasks have been well clarified and organized.