1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 1 Mirrors Sub-System Overview  Introduction  Scope of the subsystem, main tasks  Substrates.

Slides:



Advertisements
Similar presentations
G v1 1 The reality of Mirrors? GWADW May 15, 2012 GariLynn Billingsley Liyuan Zhang Zygo… CSIRO…
Advertisements

T1 task- update Mike Plissi. 2 Collaboration Groups actively involved INFN-VIRGO MAT IGR-Glasgow Groups that have expressed interest INFN-AURIGA CNRS-LKB.
G R LIGO Laboratory1 Advanced LIGO Research and Development David Shoemaker LHO LSC 11 November 2003.
Progress on Laser Induced Damage Studies of Grazing Incidence Metal Mirrors Mark S. Tillack T. K. Mau Mofreh Zaghloul Laser-IFE Program Workshop May 31-June.
LIGO-G9900XX-00-M LIGO R&D1 Gold Coatings in Advanced LIGO Phil Willems.
Thermal Compensation Review David Ottaway LIGO Laboratory MIT.
Thermally Deformable Mirrors: a new Adaptive Optics scheme for Advanced Gravitational Wave Interferometers Marie Kasprzack Laboratoire de l’Accélérateur.
BS and Mirrors for the LCGT Norikatsu Mio, PSC Univ. of Tokyo Eiichi Hirose, ICRR Univ. of Tokyo December 13, 2011 CSIRO, Lindfield Australia.
Stefan Hild, Andreas Freise, Simon Chelkowski University of Birmingham Roland Schilling, Jerome Degallaix AEI Hannover Maddalena Mantovani EGO, Cascina.
Stefan Hild, Andreas Freise, Simon Chelkowski University of Birmingham Roland Schilling, Jerome Degallaix AEI Hannover Maddalena Mantovani EGO, Cascina.
September 8, 2015 THE MONOLITHIC SUSPENSION STATUS FOR THE VIRGO INTERFEROMETER THE MONOLITHIC SUSPENSION STATUS FOR THE VIRGO INTERFEROMETER Helios Vocca.
1 VAC – Vacuum system modifications Cascina, 03Nov08 A.Pasqualetti for the VAC contributors.
Plans for Advanced Virgo
Alban REMILLIEUX3 rd ILIAS-GW Annual General Meeting. London, October 26 th -27 th, New coatings on new substrates for low mechanical loss mirrors.
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.
Optical Configuration Advanced Virgo Review Andreas Freise for the OSD subsystem.
LIGO-G M May 31-June 2, 2006 Input Optics (IO) Cost and Schedule Breakout Presentation NSF Review of Advanced LIGO Project David Reitze UF.
G M 1 Advanced LIGO Update David Shoemaker LSC/Virgo MIT July 2007.
Advanced VIRGO WG1: Status VIRGO, Cascina Andreas Freise University of Birmingham.
G v5 1 Core Optics Components Technical Status NSF Review of Advanced LIGO Project April 2011 GariLynn Billingsley.
Thermal Compensation in Stable Recycling Cavity 21/03/2006 LSC Meeting 2006 UF LIGO Group Muzammil A. Arain.
LISA October 3, 2005 LISA Laser Interferometer Space Antenna Gravitational Physics Program Technical implications Jo van.
LIGO- G D The LIGO Instruments Stan Whitcomb NSB Meeting LIGO Livingston Observatory 4 February 2004.
Gravitational Wave Detection Using Precision Interferometry Gregory Harry Massachusetts Institute of Technology - On Behalf of the LIGO Science Collaboration.
Université Lyon I NATO/ASI and Euro Summer School September 16-27, 2002 JM.M SMASMA OPTICS IN ASTROPHYSICS Coatings Performances & Limitations Jean-Marie.
DFG-NSF Astrophysics Workshop Jun 2007 G Z 1 Optics for Interferometers for Ground-based Detectors David Reitze Physics Department University.
Advanced Virgo Optical Configuration ILIAS-GW, Tübingen Andreas Freise - Conceptual Design -
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
AIGO 2K Australia - Italy Workshop th October th October 2005 Pablo Barriga for AIGO group.
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.
Advanced Virgo Giovanni Losurdo Advanced Virgo Coordinator for the Virgo Collaboration.
AdV Thermal Compensation System Viviana Fafone AdV/aLIGO joint technical meeting, February 4, 2004.
1 PAY Review Meeting 1 18/3/2009 Piero Rapagnani 18/03/2009.
Janyce Franc-Kyoto-GWADW1 Simulation and research for the future ET mirrors Janyce Franc, Nazario Morgado, Raffaele Flaminio Laboratoire des Matériaux.
ACIGA High Optical Power Test Facility
1 Locking in Virgo Matteo Barsuglia ILIAS, Cascina, July 7 th 2004.
17/05/2010A. Rocchi - GWADW Kyoto2 Thermal effects: a brief introduction  In TM, optical power predominantly absorbed by the HR coating and converted.
Advanced Virgo: Optical Simulation and Design Advanced Virgo review Andreas Freise for the OSD Subsystem.
Cascina, Nov. 4 th, 2008 AdV review 1 AdV Injection system E. Genin European Gravitational Observatory.
1 DC readout for Virgo+? E. Tournefier WG1 meeting, Hannover January 23 rd,2007 DC vs AC readout: technical noises Output mode cleaner for DC readout.
Some considerations on radiative cooling V. Fafone, Y. Minenkov, I. Modena, A. Rocchi INFN Roma Tor Vergata.
LIGO Scientific Collaboration
Thermal Compensation System TCS V. Fafone for the TCS Subsystem.
Advanced Advanced Virgo BASELINE DESIGN advanced Giovanni Losurdo – INFN Firenze Advanced Virgo Coordinator for the Virgo Collaboration.
The VIRGO detection system
Coastline Optics, Inc. 906 Via Alondra Camarillo, CA (805)
New MC mirror M.Punturo. New MC mirror? Scattering in the end mirror of the IMC is the first cause of the ISYS upgrade –Poor quality of the substrate.
LIGO-G D Core Optics Components (COC) Polishing Pathfinder Kickoff Advanced LIGO Project GariLynn Billingsley Caltech.
The Proposed Holographic Noise Experiment Rainer Weiss, MIT On behalf of the proposing group Fermi Lab Proposal Review November 3, 2009.
Optical Interference Coatings: from advanced to future GW detectors L. Balzarini, E. Berthélémy, G. Cagnoli, J. Degallaix, V. Dolique, R. Flaminio. D.
1 Cascina – October 19, 2011 ASPERA Forum Laurent Pinard Substrates, Polishing, Coatings and Metrology for the 2 nd generation of GW detector Laurent PINARD.
1 Advanced Virgo Monolithic Payloads P.Rapagnani Thermal Noise Workshop 2012_02_24-25.
Thermal compensation issues: sensing and actuation V. Fafone University of Rome Tor Vergata and INFN ASPERA Technological Forum – EGO October, 2011.
LIGO-G v1 Inside LIGO LIGO1 Betsy Weaver, GariLynn Billingsely and Travis Sadecki 2016 – 02 – 23 at CSIRO, Lindfield.
Material Downselect Rationale and Directions Gregory Harry LIGO/MIT Kavli Institute for Astrophysics and Space Technology On behalf of downselect working.
Characterization of Advanced LIGO Core Optics
A look at interferometer topologies that use reflection gratings
THE COMPANY OPTIKRON, your partner for micro-optics, assemblies and optical coatings was founded in 1992 in the optics and technology region of Jena. We.
The Proposed Holographic Noise Experiment
Laboratoire des Matériaux Avancés - Lyon
Design of Stable Power-Recycling Cavities
LIGO Scientific Collaboration
Flat-Top Beam Profile Cavity Prototype: design and preliminary tests
Heavy IMC end payload requirements
Flat-Top Beam Profile Cavity Prototype
The views of Virgo collaboration groups on upgraded/advanced Virgo
The ET sensitivity curve with ‘conventional‘ techniques
Towards Advanced Virgo Plus
Presentation transcript:

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 1 Mirrors Sub-System Overview  Introduction  Scope of the subsystem, main tasks  Substrates Procurement  Blank Material (fused silica) : material choice, specifications, planning, cost  Polishing : strategy, choice of the company, planning, cost  Coating : planning, cost

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 2 Introduction Mir Sub-system  Procurement and preparation of the AdV test masses and spares Input and End mirrors, Beam Splitter, mirrors for non-degenerate Power and Signal Recycling cavities, Compensation Plates  Mirrors with larger dimensions (thicker) Modification in the coating process  Mirrors with RMS flatness better than 1 nm Polishing and Coating strategy More accurate metrology Description

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 3 Introduction Mir Sub-system Main Tasks  Substrates: Blank materials procurement (fused silica), Choice of the best material (Company), Order preparation  Polishing: Definition of the specifications, Geometry (ROC, monolithic suspension..) Flatness requirements, Definition of the polishing strategy (Corrective Coating) Call for tender for the micropolishing, Order preparation. Control of the different substrates delivered (Defects, roughness, ROC, flatness, bulk absorption, Birefringence) - Characterization report  Coatings: Coating process modification linked to the mirror weight increase (mirror handling tools, new sample-holder (robot) for Corrective Coating) Design optimization, use of the best high index material (thermal noise), annealing  Metrology : Modification of the sample holder on optical metrology benches (Abs./Scat. bench) New ITF bench to measure the wavefront at 0° and 45° of 0.5 nm RMS (TBC) on the AdV test masses

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 4 Introduction Mir Sub-system AdV Mirrors : Reference Solution Geometry and performances Input Mirror IM End Mirror EM Beam Splitter BS Compensation Plate CP Non degenerate Power and Signal recycling Cavities PRM3/SRM3PRM2/SRM2PRM1/SRM1 Number of parts Fused Silica Nature Suprasil 3002Suprasil 312Suprasil 3001Herasil 102 Diameter 350 mm <550 mm (TBC) 280 mm (TBC) 150 mm (TBC) 50 mm (TBC) 50 mm (TBC) Thickness 200 mm 65 mm 100 mm (TBC) 50 mm Roughness Reflective side <1 Å RMS RMS Flatness Reflective side 0.5 nm RMS (TBC)  150 mm 0.5 nm RMS (TBC)  200 mm 3 nm RMS (TBC)  150 mm 3 nm RMS (TBC)  150 mm 3 nm RMS (TBC)  100 mm 3 nm RMS (TBC)  20 mm 3 nm RMS (TBC)  20 mm Transmission Reflective side 0.7 % (TBC) # 10 ppm (TBC) 50 %#100 % # 10 ppm (TBC) # 10 ppm (TBC) TBD

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 5 Detailed revised DRAFT Planning if starting on 01/07/2009 Estimation based on real delay for the manufacturing of the silica and on the real time necessary for the VIRGO + substrates polishing - Mirrors Delivery : beginning of 2012 Mirrors production Plan

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 6 Substrates Fabrication : 1,5 year o Planning for 4 IM-4 EM-2 BS solution (one spare for each mirror) Serial production of the silica blanks. Possibility to produce in parallel but limitation = polishing phase o Heraeus production : first bulk substrate produced after 4 month, then one bulk/2 weeks o Choose the best material for each type of component Compromise between optical/mechanical performances and price Substrates Procurement

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 7 Fused Silica properties comparison

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 8 Substrates Procurement Motivations for Fused silica choice  No real advantages to choose Corning (performances, cost), limitation in size Manufacturer = HERAEUS (like in VIRGO)  For IM, BS : New fused silica (Suprasil 3001/3002) same optical performances Better bulk absorption (0.2 ppm/cm measured): better for thermal lensing Comparable price  For EM : Suprasil 312 Good optical and mechanical properties Cheaper  Non degenerate PR and SR cavities (3 mirrors 5-15 cm) and CP: Herasil 102 : cheap Properties satisfactory for this particular type of mirrors

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 9 Substrates Procurement Real Fused Silica Cost (IM/EM thickness 20 cm) Solution 4 IM/ 4 EM/ 2 BS/ 6 PR-SR cavities/ 4 CP If thickness 30 cm for IM and EM : extra cost # +30 % CostIM/EM/BS/SR+PR/CPCost - Thickness 30 cm Reference Solution ,00 € 3002 / 312 / 3001 / Herasil ,00 €

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 10 Substrates Polishing : # 2,5 years (for all spares)  Real Time estimation with General Optics production time for the Virgo + mirrors (2007) (6 months for the first substrate, after 1 parts/month) Different from one polisher to the other P olishing starts as soon as first bulk substrate received (nov 2009)  Coating starts as soon as possible Substrates Polishing

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 11  New strategy for the Larger beam splitter (< 55 cm- TBC) Several polishers contacted to check feasibility (in progress)  New geometry of the mirrors (monolithic lateral supports) Check with polishers if feasible (in progress)  Critical point: flatness requirements (# 0.5 nm RMS) Simulations necessary to evaluate the crucial spatial frequency domain Flatness metrology improvement (better accuracy and reproducibility) New bench : stitching interferometry, stable sample holder, measurement also at 45° Substrates Polishing

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 12 Substrates Polishing Two Paths Corrective Coating (LMA) New opportunity Flatness reached with Ion Beam polishing Polisher not able to guarantee the flatness specifications (Best effort) Polisher able to guarantee the flatness specifications Development of a new Robot Reference solution To be tested Cost (?) Future AdV Mirrors upgrades

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 13 Substrates Polishing : Corrective coating Substrate Interferometer Ion source Robot mask Silica target Sputtered atoms Substrate  156 mm VIRGO type Before correction (  120 mm) 3.3 nm R.M.S. / 16 nm P.V. After correction (  120 mm) 0.98 nm R.M.S. /10 nm P.V.

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 14 Substrates Polishing Polishing cost Solution 4 IM/ 4 EM/ 2 BS/ 6 PR-SR cavities / 4 CP Cost estimation obtained for VIRGO+ (2007)  Contact polishing companies : General Optics, CSIRO, SESO (?)  Find the best compromise between the price and the performances k€

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 15 Mirrors Coating : # 2 years Mirrors Coating  Coating start : as soon as 2 IM ready (polished, characterized) Coated at the same time (ITF arm symmetry)  Coatings having the best available optical and mechanical features  Reference path : flatness correction by “Corrective Coating” (IM, EM) 2 CP

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 16  For “Corrective Coating”: new robot in the Virgo large coater (ordered at the same time as the polishing, end 2009) – 300 k€  Study of the robot already started Help from LAPP (P. Mugnier, L. Giacobone) for the technical study of the robot Test on a real large substrate (old VEM ?) Simulation with a corrected wavefront (Nice group) : see if CC improves or not  CC : Quite no impact on the coating planning (limitation : polishing)  Alternative strategy : Advanced polishing company able to reach the 0.5 nm specification by Ion Beam Polishing (final step after a classical polishing). Coating test on this type of substrate Mirrors Coating

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 17 Mirrors Coating Coating cost Cleaning Facility (real) Tooling for cleaning Tooling for coating Handling Tools Robot Ion Assist source (Q improvement) Under vacuum furnace Coating (corrective coating) Total (€) k€

1st Advanced Virgo Review – November 3-4, 2008 – L. Pinard 18 Mirrors Coating Metrology cost : 300 k€ Lots of modifications to control heavier and thicker substrates Metrology mountings (IM/EM/BS) New motorized sample holder for the scattering and transmission measurement (BS) New motorized sample holder coupled with stitching interferometry software for wavefront measurement (0°- 45°)