Pre-stabilized laser (PSL) for AdV Scope of the system Main tasks Requirements Reference solution and status of the design Plans towards completion Technical.

Slides:



Advertisements
Similar presentations
Status of the Virgo Commissioning G.Losurdo – INFN Firenze/Urbino for the Virgo Collaboration.
Advertisements

September 21, 2005Virgo Status – ESF Workshop1 Status of Virgo B. Mours.
Cascina, January 25th, Coupling of the IMC length noise into the recombined ITF output Raffaele Flaminio EGO and CNRS/IN2P3 Summary - Recombined.
ICSO High Accuracy Laser Telemetry for Kilometric Distance Measurement in Space C.COURDE, H. PHUNG Duy, M. LINTZ, A. BRILLET ARTEMIS, Observatoire.
CNMFrascati 12/01/061 High Power Laser System for Advanced Virgo C.N.Man Design goals Present technology Other activities in the world Virgo+ and Laser.
Lock Acquisition with Auxiliary Lasers Main Question to be answered for the design : What is the goal of auxiliary lasers ? 1. lock independently the arms.
1 Virgo commissioning status M.Barsuglia LAL Orsay.
Optical simulation – March 04 1 Optical Simulation François BONDU VIRGO Tools Goals Example: tuning of modulation frequency A few questions.
LIGO-G W Proposed LHO Commissioning Activities in May 02 Fred Raab 29 Apr 02.
LIGO-G W LIGO II Pre-stabilized Laser System Design Requirements and Conceptual Design David Ottaway, Todd Rutherford, Rick Savage, Peter Veitch,
VSR1 summary - post VSR1 Commissioning plans E. Tournefier (LAPP-CNRS) LSC-Virgo meeting Oct 22 nd, 2007.
Measurement of the laser beam profile at PSL to Mode Cleaner interface for the 40 Meter Prototype Interferometer A table of contents 1. Introduction 1.1.
COMMISSIONING PROGRESS G.LOSURDO – INFN Firenze for the Virgo Collaboration.
Q09/2001 The GEO 600 Laser System LIGO-G Z V. Quetschke°, M. Kirchner°, I.Zawischa*, M. Brendel*, C. Fallnich*, S. Nagano +, B. Willke° +, K.
Current progress of developing Inter-satellite laser interferometry for Space Advanced Gravity Measurements Hsien-Chi Yeh School of Physics Huazhong University.
G D Initial LIGO improvements & Advanced LIGO P Fritschel PAC Meeting LLO, 18 May 2005.
1 Ist Virgo+ review Cascina H. Heitmann Alignment: Virgo+ changes.
Optical Configuration Advanced Virgo Review Andreas Freise for the OSD subsystem.
The GEO 600 Detector Andreas Freise for the GEO 600 Team Max-Planck-Institute for Gravitational Physics University of Hannover May 20, 2002.
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.
Interferometer Control Matt Evans …talk mostly taken from…
1 1.ISC scope and activities 2.Initial Virgo status 3.Design requirements 4.Reference solution and design status 5.Plans toward completion 6.Technical.
Virgo Commissioning update Gabriele Vajente for the Virgo Collaboration LSC/VIRGO Meeting – MIT 2007, July LIGO-G Z.
LIGO-G Advanced LIGO Detector upgrade is planned for »Factor of 10 increase in distance probed (‘reach’) »Factor of 1000 increase in event.
1 Noise sources at high frequency in Virgo E. Tournefier (LAPP-CNRS) ILAS WG1 meeting, Hannover December 12 th,2005 Recycled ITF sensitivities Noise sources.
Current status of Laser development 2nd Korea - Japan Workshop on KAGRA 2012/5/28(Mon)
Environmental noise studies at VIRGO Environmental contributions to Virgo readout noise (C-runs) many sources identified through coherency analyses with.
Status of VIRGO Francesco Fidecaro (after Lisa Barsotti) - University and INFN Pisa – on behalf of the VIRGO collaboration Aspen - January 19 th, 2005.
GEO600 Detector Status Harald Lück Max-Planck Institut für Gravitationsphysik Institut für Atom- und Molekülphysik, Uni Hannover.
Squeezed light and GEO600 Simon Chelkowski LSC Meeting, Hannover.
G Z LIGO R&D1 Input Optics Definition, Function The input optics (IO) conditions light from the pre- stabilized laser (PSL) for injection into.
1 Virgo Commissioning progress ILIAS, Nov 13 th 2006 Matteo Barsuglia on behalf of the Commissioning Team.
1 1.Status a.Design requirements: almost complete. b.Preliminary design: on-going 2.WBS a.Tasks and subtasks b.Manpower, responsibility issues 3.Interfaces.
Paolo La Penna Injection optics for Advanced VirgoLSC/VIRGO joint meeting, Cascina, 25/05/ Advanced VIRGO Input optics LIGO-G Z.
1 1.Definition 2.Deliverables 3.Status of preliminary design 4.Risks 5.Tasks to be done 6.Decisions to be taken 7.Required simulations 8.Planning ISC workshop:
Status of the Advanced LIGO PSL development LSC Virgo meeting, Caltech, March 2008 LIGO G Z Benno Willke for the PSL team.
1 Intensity Stabilization in Advanced LIGO David Ottaway (Jamie Rollins Viewgraphs) Massachusetts Institute of Technology March, 2004 LSC Livingston Meeting.
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.
Status of the Advanced LIGO PSL development LSC meeting, Baton Rouge March 2007 G Z Benno Willke for the PSL team.
LIGO-G Z The Status of VIRGO E. Tournefier for the Virgo Collaboration GWADW 2004, Aspen From the CITF to VIRGO Commissioning of the Fabry-Perot.
Laser system for LCGT Norikatsu MIO.
The status of VIRGO Edwige Tournefier (LAPP-Annecy ) for the VIRGO Collaboration HEP2005, 21st- 27th July 2005 The VIRGO experiment and detection of.
1 Virgo Commissioning Status WG1 meeting Potsdam, 21 st July 2006.
Stefan Hild 111th WG1 meeting, Hannover, January 2007 DC-Readout for GEO Stefan Hild for the GEO-team.
Paolo La Penna ILIAS N5-WP1 meeting Commissioning Progress Hannover, July 2004 VIRGO commissioning progress report.
Status of Virgo GWDAW12 Status of Virgo GWDAW Dec Leone B. Bosi INFN and University of Perugia (Italy) On behalf of the Virgo Collaboration.
1 Locking in Virgo Matteo Barsuglia ILIAS, Cascina, July 7 th 2004.
Status of Virgo a short update Michele Punturo. A bit of History July 29 – August –C6 run Duty cycle: Locking 89%, Science Mode 86% September.
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.
Caltech, February 12th1 Virgo central interferometer: commissioning and engineering runs Matteo Barsuglia Laboratoire de l’Accelerateur Lineaire, Orsay.
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.
Monica VarvellaIEEE - GW Workshop Roma, October 21, M.Varvella Virgo LAL Orsay / LIGO CalTech Time-domain model for AdvLIGO Interferometer Gravitational.
1 Frequency Noise in Virgo by Matt Evans. 2 The Actors  Noise Sources  Input Mode Cleaner length noise  Sensing noise on IMC lock  Frequency Servo.
Advanced Advanced Virgo BASELINE DESIGN advanced Giovanni Losurdo – INFN Firenze Advanced Virgo Coordinator for the Virgo Collaboration.
The VIRGO detection system
The Proposed Holographic Noise Experiment Rainer Weiss, MIT On behalf of the proposing group Fermi Lab Proposal Review November 3, 2009.
High power fibered optical components for gravitational waves detector Matthieu Gosselin, PhD Student at EGO ELiTES : 3 rd general meeting February 10.
Automation of the Lock Acquisition of the 3 km Arm Virgo Interferometer F. Carbognani for The Virgo Collaboration ICALEPCS - Geneva 14 October, 2005.
NSF Annual Review of the LIGO Laboratory
Advanced Virgo INJ: Faraday isolator, Electro-optical modulator, high power beam dump and Input mode-cleaner E. Genin for AdV INJ team European Gravitational.
bKAGRA PSL Design Study
Daniel Sigg, Commissioning Meeting, 11/11/16
The Proposed Holographic Noise Experiment
Commissioning Progress and Plans
Update on the Advanced LIGO PSL Program
Homodyne readout of an interferometer with Signal Recycling
Virgo – Injection SYStem
Frequency Noise in Virgo
Squeezed Light Techniques for Gravitational Wave Detection
Presentation transcript:

Pre-stabilized laser (PSL) for AdV Scope of the system Main tasks Requirements Reference solution and status of the design Plans towards completion Technical issues Conclusion 1AdV 1st review 3-4/11/08 Catherine Nary MAN C.N.Man

Scope of the PSL system AdV 1st review 3-4/11/08 2C.N.Man High power lasers system of 200W, pre-stabilized in frequency and power stabilized  noise level required at entrance of IMC IMC PSL system

Main tasks AdV 1st review 3-4/11/083 The high power laser(s) the injection locking optics and electronics. The frequency pre-stabilization loop the fast electronics utilized in that loop A triangular pre-mode-cleaner (PMC) the control electronics. The power stabilization of the laser the control loop and vacuum photodiode The positioning of the optical elements on the laser bench Matching and steering optics modulators (EOM) and Faraday isolators (FI) Monitoring photodiodes C.N.Man

Requirements C.N.ManAdV 1st review 3-4/11/084 RequirementValueFreq. range Power 200 W Frequency noise linear spectral density * f > 10 Hz Power noise RIN (−170 dB/ √ Hz) ** 10 Hz< f <10 kHz Beam jitter *** Beam geometry High order modes content <5% * to be refined by Interf Sensing Control (ISC) system ** assume contrast of 0.01% and arm finesse of 900, to be refined *** need 1 nrd/ √ Hz & assume IMC filtering factor of 1000 NB: Virgo+ will also help refining the specs as it will serve too as testbed for some technological choices

Baseline design AdV 1st review 3-4/11/085C.N.Man 1-2W 20W 50W 200W

Rigid reference cavity LF itf lock Control Strategies AdV 1st review 3-4/11/086 HP slave 200W Inj L2 MP slave 20W Inj L1 Master 1-2W RIN L Suspended IMC Freq pre-stab C.N.Man Pre-mode cleaner pmc lockIMC lock 3kms baseline cavity Power stab

Plan towards completion 7AdV 1st review 3-4/11/08C.N.Man 1/ Refine stabilizations requirements: a few outputs from other systems asap: ISC  if DC detection is confirmed, simplify pmc design & power stabilization alignments performances predictions give residual beam jitter required locking precision gives residual RIN in LF and in detection range OSD  asymmetry (freq stab), contrast (power stab), … a trade-off to find 2/ Order HP stage for tests in lab: noise spectrum, beam quality and jitter, … 3/ Pre-mode-cleaner realization (depends on HP beam quality and amplitude noise) 4/ Power stabilization (check of real performances in LF range going on) 5/ Frequency stabilization (after IMC completion)

Tasks towards completion C.N.ManAdV 1st review 3-4/11/088 topicsrequirementsprocurementsR&D realization Tests/commission.

Technical issues C.N.ManAdV 1st review 3-4/11/089 Can we skip the 20W medium power stage ? Injection locking  noise of the master inside locking range could be done during the development of injection lock loop Option of using 200W fiber amplifier : 200W class, to be tested in 2009, much cheaper than SSL tests & controls to be done Option of using fiber to transport HP beam to Injection bench under study Combination of the 2 options in an all-fibered PSL can make the PSL schematic evolve certainly in a simpler way

Conclusion C.N.ManAdV 1st review 3-4/11/0810 The baseline solution of this SubSystem shows no surprise From Virgo+ to AdV, the main change is the replacement of 50W HP stage by 200W stage. Virgo+ is an intermediate step for testing some improvements that would help refine the requirements AdV PSL is a simple extrapolation of Virgo & Virgo+ If necessary some performances can be improved Still some requirements need to be refined by other SS This SS is not on the critical path and can evolve even during the commissioning phase.