1 Advanced Virgo Monolithic Payloads P.Rapagnani Thermal Noise Workshop 2012_02_24-25.

Slides:



Advertisements
Similar presentations
T1 task- update Mike Plissi. 2 Collaboration Groups actively involved INFN-VIRGO MAT IGR-Glasgow Groups that have expressed interest INFN-AURIGA CNRS-LKB.
Advertisements

LIGO-G D Comments: Staged implementation of Advanced LIGO Adv LIGO Systems 17 may02 dhs Nifty idea: a way to soften the shock, spread cost, allow.
Andrea Paoli AdV 1 st Project Review Cascina, November 3 rd, 2008 IME – infrastructure modifications for environmental noise reduction.
G R LIGO Laboratory1 Advanced LIGO Research and Development David Shoemaker LHO LSC 11 November 2003.
LIGO-G D Suspensions Update: the View from Caltech Phil Willems LIGO/Caltech Livingston LSC Meeting March 17-20, 2003.
April 27th, 2006 Paola Puppo – INFN Roma ILIAS Cryogenic payloads and cooling systems (towards a third generation interferometer) part II: the Vibration.
Payload design methods versus modeling E. Majorana.
Silica Research in Glasgow Gianpietro Cagnoli – IGR - University of Glasgow GEO Collaboration Ginzton Lab, Stanford Caltech.
LCGT seismic Attenuation System DRADF DRAFT DRAFT DRAFT.
rd ILIAS-GW annual general meeting 1 VIRGO Commissioning progress J. Marque (EGO)
Thermally Deformable Mirrors: a new Adaptive Optics scheme for Advanced Gravitational Wave Interferometers Marie Kasprzack Laboratoire de l’Accélérateur.
LIGO-G D Suspensions Design for Advanced LIGO Phil Willems NSF Review, Oct , 2002 MIT.
Development of a CO 2 laser machine for pulling and welding of silica fibres and ribbons D. Crooks for the GEO 600 collaboration Aspen January 2005 LIGO-G Z.
September 8, 2015 THE MONOLITHIC SUSPENSION STATUS FOR THE VIRGO INTERFEROMETER THE MONOLITHIC SUSPENSION STATUS FOR THE VIRGO INTERFEROMETER Helios Vocca.
EMDM Monolithic suspension development Activity plan Piero Rapagnani Detector meeting
GWADW 2010 in Kyoto, May 19, Development for Observation and Reduction of Radiation Pressure Noise T. Mori, S. Ballmer, K. Agatsuma, S. Sakata,
Low noise Fused Silica suspensions: from the GEO600 experience to the 2 nd generation requirements Geppo Cagnoli INFN Sez. Firenze University of Glasgow.
Joshua Smith December 2003 Detector Characterization of Dual-Recycled GEO600 Joshua Smith for the GEO600 team.
Design of Stable Power-Recycling Cavities University of Florida 10/05/2005 Volker Quetschke, Guido Mueller.
Intermediate review - ERC – February 9, 2009 – L. Pinard 1 Mirrors Sub-System Overview  Introduction  Scope of the subsystem, main tasks  Job done since.
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.
Takanori Sekiguchi ALPS Report, Dec. 26th, 2013 Prototype Test of Type-B 1 Takanori Sekiguchi KAGRA F2F MEETING Feb
Status of the Advanced Virgo detector F. Piergiovanni on behalf of The Virgo Collaboration GWPAW, Osaka, 06/17/2015.
SUSPENSION DESIGN FOR ADVANCED LIGO: Update on GEO Activities Norna A Robertson University of Glasgow for the GEO 600 suspension team LSC Meeting, Louisiana,
Conceptual Design for Advanced LIGO Suspensions Norna A Robertson University of Glasgow and Stanford University for the GEO suspension team +contribution.
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.
Takanori Sekiguchi External Review Control and tuning of suspension 1 T. Sekiguchi KAGRA 4th External Review.
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.
Advanced Virgo Optical Configuration ILIAS-GW, Tübingen Andreas Freise - Conceptual Design -
Cold damping of fused silica suspension violin modes V.P.Mitrofanov, K.V.Tokmakov Moscow State University G Z.
1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 1 Mirrors Sub-System Overview  Introduction  Scope of the subsystem, main tasks  Substrates.
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.
Installation Plan of VIS Ryutaro Takahashi (NAOJ) for the 4th external review on 30 June.
AdV Thermal Compensation System Viviana Fafone AdV/aLIGO joint technical meeting, February 4, 2004.
1 LESSONS FROM VIRGO+ May 17th 2010 E. Calloni for the Virgo collaboration.
1 PAY Review Meeting 1 18/3/2009 Piero Rapagnani 18/03/2009.
The VIRGO Suspensions Control System Alberto Gennai The VIRGO Collaboration.
“Detector activities” after the IB upgrade Michele Punturo.
Suspension Thermal Noise Giles Hammond (University of Glasgow) on behalf of the Strawman Red Team GWADW 2012, 18 th May 2012 LIGO-G
MSC winter, short-term schedule Commissioning meeting Cascina 2 Oct 2006.
Paolo La Penna ILIAS N5-WP1 meeting Commissioning Progress Hannover, July 2004 VIRGO commissioning progress report.
1 PAY & OSD Piero Rapagnani 26/02/ Fatal interference with current geometry: deep redesign of the payload needed Positioning another payload close.
Advanced LIGO UK 1 LIGO-G Z Development issues for the UK Advanced LIGO project Caroline Cantley Glasgow University for the UK Advanced LIGO Team.
Monolithic suspensions in Virgo Helios Vocca Dipartimento di Fisica & INFN di Perugia LIGO-G Z.
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.
Advanced Advanced Virgo BASELINE DESIGN advanced Giovanni Losurdo – INFN Firenze Advanced Virgo Coordinator for the Virgo Collaboration.
The VIRGO detection system
Thermal Noise Workshop February 23rd, 2012 Paola Puppo – INFN Roma.
E. Majorana (INFN – Rome) ELiTES 3 rd General Meeting Hongo Campus – Tokyo – 9-10 Feb., 2015 Cryogenic platform with vertical suspension: a practical approach.
Michele Punturo adVirgo and ET thermal noise meeting 1.
Filter #7 control April 18, 2016 –, Cascina Paolo Ruggi.
1 Paola Puppo Last Stage Suspension Mechanics in Virgo+MS Piacciavi, generosa Erculea prole, ornamento e splendor del secol nostro, Ippolito, aggradir.
Paola Puppo INFN – Rome Thermal Noise Meeting – “Sapienza”-Rome - February 26 th 2008.
Assembly of the KAGRA 4-fiber sapphire prototype suspension
Michele Punturo WP3 meeting, Cascina 9-July-2004
First clues on ET payload sensing and control
VIRGO–KAGRA Meeting about bottom filter damping
Outline ideas/status K.A. Strain
LCGT Seismic Attenuation System LCGT-SAS
Evolution of the Virgo detector: The Virgo+ plans
Gingin Advisory Committee Meeting 08 Dec 2009
Superattenuator for LF and HF interferometers
Design of Stable Power-Recycling Cavities
Flat-Top Beam Profile Cavity Prototype: design and preliminary tests
P Fritschel LSC Meeting LLO, 22 March 2005
Characterisation of the aLIGO monolithic suspensions
The views of Virgo collaboration groups on upgraded/advanced Virgo
Presentation transcript:

1 Advanced Virgo Monolithic Payloads P.Rapagnani Thermal Noise Workshop 2012_02_24-25

2 Virgo Payload, until now:

Main new requirements coming from Advanced Virgo Optical Layout The necessity to suspend large (~ 1 m) and heavy baffles close to the mirrors. The necessity to suspend the Compensation Plate (CP) close to the input mirrors, with a significant tilt. The necessity to control the alignment of the CP within 10  rad Installation and pre-alignment of a Pick-off on the Recycling mirror. Moreover, experience with Virgo+MS indicate excess losses in present setup that must be revised.

Filter 7 Marionetta Mirror Reaction Mass Actuatio n Filter 7 Marionetta Mirror Actuation Standard Payload Scheme New Payload Scheme Supporting Cage The new requirements made us think of a new Payload Scheme (with the constraint of keeping Virgo axial symmetric suspension configuration) The new requirements made us think of a new Payload Scheme (with the constraint of keeping Virgo axial symmetric suspension configuration) Actuation Further optical elements

Schematic Thermal Noise: pendulum

the three schemes are equivalent and there is no relevant difference in adopting a double or a double-branched scheme.

Removing the reaction mass: is “a way” to avoid resonances the region between 10 and 20 Hz. makes full lock reallocation to the marionette easier Schematic Thermal Noise: vertical

Red line: residual motion at the level of the actuators when the suspension is in standalone operation. Green line: shows how the disturbance on the actuators support is reduced by controlling F7 pitch with respect to the ground. Blue line: If no F7 pitch control is active, as the interferometer is locked, the recoil on the actuator frame will depend on the applied correction. Cyan line: such a correction recoil is cancelled by means of F7 pitch control. Filter 7 Marionetta Mirror Preliminary Modelling Pitch Control Needed 3 point hierarchy

Test bench design: the AdV BS Filter 7 Marionetta with 8 coils, 2 motors, suitable for monolithic clamps improvement, for FP payloads Marionetta with 8 coils, 2 motors, suitable for monolithic clamps improvement, for FP payloads Side Shafts (Mirror actuators and Baffle Holders) Mirror Cradle Possibility to hold very large baffles Larger room to assemble large optics: vacuum enclosures of the 4 marionette actuators holders (thepots) would disappear and only two shafts will be used Possibility to hold very large baffles Larger room to assemble large optics: vacuum enclosures of the 4 marionette actuators holders (thepots) would disappear and only two shafts will be used Intermediate Vacuum chamber, removing it is very expensive !

10 Essential to the new scheme: Concept Design of a New IVC New IVC Flanges VAC-SAT prj. Design T. Zelenova  1m New Conduct. pipe - The actual pumping system configuration is preserved - Vacuum separation is to be better checked SAT

Main Issues for SAT-BS F7 adapt F7 parts to higher vacuum Requirements (motors, magnets) adapt cablings to tighter space constraints reshuffle enhancement of F7 control system is necessary SAT WE HAVE TO :

Input Mirrors Payloads The F7-Cage will be used also to suspend the CP, according to the design developed in last months. CP frame will be equipped with piezoelectric or electromagnetic actuators. The F7-Cage will allow an effective clamping of the needed cabling. The F7-Cage will be used also to suspend the CP, according to the design developed in last months. CP frame will be equipped with piezoelectric or electromagnetic actuators. The F7-Cage will allow an effective clamping of the needed cabling. Scheme of Compensation Plate holder The new scheme will be used also for the Input Payloads. Filter 7 Marionetta Mirror Pitch Control Compensation Plate Actuators for plate alignment Monolithic Suspension lock

13 Preliminary Design of Input Payloads Cage Compensation Plate The marionette will be similar to that developed for the BS

14 CO 2 Upper cone 1.5 mm rod Lower “anchor” CO 2 Current Monolithic Mirror Suspensions geometry P.Rapagnani - PAY

15 AdV monolithic suspension Mirror suspension ears, machined or silica bonded Upper clamps, on marionette Machining the ears on the mirrors improves reliability: Interaction with MIR to find a possible solution compatible with substrates and coating production.

16 We have found that the Q values, both for pendulum and bulk modes, of the mirrors suspended with fused silica fibers are not high as expected We must improve the technology, finding the simple and affordable solution to the problem (still under investigation). So we shall proceed gradually, trying to implement first the simplest solutions, and increase the complexity as simpler approaches fail. But we have a limited time schedule, so we are working on two parallel lines: Extensive measurement campaign on old payloads and sample items. Study of the most complex solution, to be ready to implement it, if necessary: The Monolithic Marionette Study of the most complex solution, to be ready to implement it, if necessary: The Monolithic Marionette

Paths to Q improvement: Bulk Modes Series of tests to be performed in Rome, on old payloads and test mirrors 17 Bulk Modes: current value 20 times lower than expected, with an erratic behavior (e.g. Q of WI drum mode: ) Bulk Modes: current value 20 times lower than expected, with an erratic behavior (e.g. Q of WI drum mode: ) Possible causes Dissipation in silica bonding of Ears Dissipation between anchor and ear Solution Improve silica bonding, reduce bonded surface Improve silica bonding, change shape of anchors and contact surface Or use spot welding technology as in aLIGO Related Issues Recovery strategy to be redefined Large impact on schedule and costs

18 The Bulk Modes will be measured in Rome in our Vacuum Test Chamber. We shall measure both the old monolithic payloads and the test mirror, with standard bonded ears, used during Virgo+MS development. The Bulk Modes will be measured in Rome in our Vacuum Test Chamber. We shall measure both the old monolithic payloads and the test mirror, with standard bonded ears, used during Virgo+MS development. Virgo+MS Test Mirror Rome Test Vacuum Chamber Excitation will be provided by the standard coils on the Reaction Mass. As a readout we shall use a small interferometer developed by the Naples Group Excitation will be provided by the standard coils on the Reaction Mass. As a readout we shall use a small interferometer developed by the Naples Group

19 We shall be able to test the bulk modes of a mirror both suspended to the marionette, and simply supported on two knife edge bars. In this way we should be able to measure the coupling of the bulk modes with the violin modes of the fibers, and we hope to identify the sources of excess losses at high frequency.

Paths to Q improvement: Pendulum Modes Series of tests to be performed in Perugia and Rome, on old payloads and test mirrors 20 Pendulum modes: diagnostic measurements: Q of violin modes current value 30 – 100 times lower than expected Pendulum modes: diagnostic measurements: Q of violin modes current value 30 – 100 times lower than expected Possible causes Upper Clamp: Motion of clamp box on the marionetta Friction of silica part inside the clamp box Motion of silica part inside the clamp box Lower Clamp: Friction of anchors on ears Solution Improve clamp box blocking Improve the contact between surfaces Increase the size of the silica part...or use a monolithic marionette... Improve silica bonding, change shape of anchors and contact surface...or use spot welding technology as in aLIGO Related Issues More complex payload, additional DOF to control Recovery strategy to be redefined Large impact on schedule and costs

21 We shell test the upper and lower clamp dissipations on a sigle fiber in the Perugia facility, and we shall also measure the violin modes of the old monolithic payloads in Rome. Set up to measure violin modes on a single fiber We hope to be able to optimize the clamp box, avoiding the complication of a monolithic marionette: However, just in case, we are studying possible solutions also in that direction... Indeed, in a test performed in 2010 on a free fiber clamped with the standard clamp box, we have found:  ≈ , close to the nominal value. A 1.5 mm fused silica bar has been welded to the upper block and clamped in the “monolithic suspension” way. The free loaded bar dissipation has been measured from about 20 Hz to 1200 Hz.  = No excess losses appear in the upper clamp system

Input Mirrors Payloads: Monolithic Marionette The simplest approach to a monolithic marionette is to interpose a third mass of fused silica between the standard marionette and the mirror. The standard marionette will keep its functions and hardware: balancing motors and magnets, while the monolithic marionette would have only the ears for the anchors of the fibers and, eventually, some magnets for control and mode damping. The monolithic marionette will be suspended with standard steel wires. The simplest approach to a monolithic marionette is to interpose a third mass of fused silica between the standard marionette and the mirror. The standard marionette will keep its functions and hardware: balancing motors and magnets, while the monolithic marionette would have only the ears for the anchors of the fibers and, eventually, some magnets for control and mode damping. The monolithic marionette will be suspended with standard steel wires. Filter 7 Standard Marionette Mirror Pitch Control Compensation Plate Actuators for Alignment Monolithic Suspension Steel Suspension Monolithic Marionette Currently we are starting the study of this configuration: Optimization of wire lenghts and masses for a cylindric fused silica marionette, in two possible configurations: with the axis parallel to the axis of the mirror, or orthogonal to it. Currently we are starting the study of this configuration: Optimization of wire lenghts and masses for a cylindric fused silica marionette, in two possible configurations: with the axis parallel to the axis of the mirror, or orthogonal to it.

23 In any case, we shall make a diagnostic of dissipations (violin modes and bulk modes) of all payloads, before their integration into Advanced Virgo. For this, we are building a test vacuum chamber to be integrated in the 1500 W Clean Room. In any case, we shall make a diagnostic of dissipations (violin modes and bulk modes) of all payloads, before their integration into Advanced Virgo. For this, we are building a test vacuum chamber to be integrated in the 1500 W Clean Room.

24 END

25 Spare Slides

26 Upper clamp measurements A 1.5 mm fused silica bar has been welded to the upper block and clamped in the “monolithic suspension” way. The free loaded bar dissipation has been measured from about 20 Hz to 1200 Hz. No excess losses appear in the upper clamp system  =