40m TAC Update October 2006 The 40m Team 11 April 2019 G060535-00-I.

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Presentation transcript:

40m TAC Update October 2006 The 40m Team 11 April 2019 G060535-00-I

40 meter prototype Objectives: Develop lock acquisition procedure of detuned Resonant Sideband Extraction (RSE) interferometer, as close as possible to AdLIGO optical design Test/Characterize LSC scheme Develop DC readout scheme Characterize noise mechanisms Test QND techniques Develop/Test ASC scheme Extrapolate to AdLIGO via simulation Prototyping will yield crucial information about how to build and run AdvLIGO (and eLIGO). OMC Chamber view from the North side 11 April 2019 G060535-00-I

Work since last update (AugLSC) DC Readout hardware installation Mechanical tuning of the OSEMs Mach Zehnder rework Squeezing work translation stage busted; Go’s drawing a new one 11 April 2019 G060535-00-I

SRM PRM BS Excess Loss 11 April 2019 G060535-00-I

DC readout beamline OMC DC PD Mode matching telescope From SRM 11 April 2019 G060535-00-I

DC Readout I All in-vac hardware installed (~2 weeks open) Tested: OMC Length PZT, DC Photodiodes, OMC length locking (via temporary equip.) Initial alignment is good. OMC locked with decent visibility (~75% w/ no tip/tilt). Transmitted pickoff beam comes out of vacuum. 11 April 2019 G060535-00-I

DC Readout Issues Encapsulated PD electronics vacuum nipple is leaky. Leak rate is ~1 liter/year. Better implementation is on the vent list. Confirmed that MC1/MC3 spots are off in yaw by ~15 mm, same as was measured a year ago. Re-alignment is on the vent list. Pico Fiasco: Using the Squeezer translation stage or the OMC’s MMT Pico motors causes computers to crash and the MOPA to “wink out”. Seems like some kind of immense EMI problem... AR Coatings: Several of the CVI mirrors have none. Beam Dumps: Mostly neglected in the opto-mechanical layout. Black glass retrofit is on the todo list. Various delays due to Piezo Jena. Bottom line: Let’s never ever buy any Piezo Jena stuff again. 11 April 2019 G060535-00-I

40m Long Term Plans From the 40m conceptual design: “The primary goal of the 40 m upgrade is to demonstrate a control scheme for using (RSE)...” Also, from the same doc: “The 40m lab is a facility for the development, testing, implementation, and staging of small improvements to the LIGO interferometers” The 40m prototype should be used to inform the design and reduce the commissioning time in the Enhanced LIGO. Also cannot table the AdvLIGO ISC tasks that are on the 40m plate. 11 April 2019 G060535-00-I

40m Long Term Plans DC Readout (on a Michelson and then a PRFPMI) http://lhocds.ligo-wa.caltech.edu:8000/40m/Long_Term_Plans_@_the_40m DC Readout (on a Michelson and then a PRFPMI) Develop the new AdvLIGO LSC Scheme DC Readout on the DRSE (w/ new LSC config.) Advanced LIGO ASC Scheme 11 April 2019 G060535-00-I

PRFPMI displacement noise (DC v. RF) DC Readout (Phase A) Lock OMC Length Loop (w/ new controls) Lock OMC Alignment Loops (dithering) Characterize in-vac DC PDs (noise, TF) Simple Michelson displacement noise (DC v. RF) PRFPMI displacement noise (DC v. RF) Along the way, DWFs, Oplev filters, new CM servo http://lhocds.ligo-wa.caltech.edu:8000/40m/Long_Term_Plans_@_the_40m 11 April 2019 G060535-00-I

AdvLIGO LSC Re-establish the Full IFO locking Mach-Zender has been reworked to stabilize the RFAM problems New MC servo is in so the frequency noise is better (hopefully) Some characterization ? What exactly ? Adopt the new LSC Scheme (after one is chosen) requires major in-vac overhaul for cavity lengths, finesses, etc. Prototype new style RFPDs (Grote/Sandberg style) Complex Modulation (to replace the Mach-Zehnder) http://lhocds.ligo-wa.caltech.edu:8000/40m/Long_Term_Plans_@_the_40m 11 April 2019 G060535-00-I

AdvLIGO ASC Goes along with the new LSC Scheme This is a hard problem. New WFS circuits (because we don’t have any WFS) This is a hard problem. http://lhocds.ligo-wa.caltech.edu:8000/40m/Long_Term_Plans_@_the_40m 11 April 2019 G060535-00-I

DC Readout (Phase B) Determine a set of measurements to do for this. Laser noise transfer functions, angular noise, scattering. Could also take this opportunity to install AdvLIGO CDS Infrastructure; provides some spares for iLIGO. http://lhocds.ligo-wa.caltech.edu:8000/40m/Long_Term_Plans_@_the_40m 11 April 2019 G060535-00-I

Last Slide ! Check out the Wiki for a schedule goal --- http://lhocds.ligo-wa.caltech.edu:8000/40m/High_Level_Schedule Check out the Wiki for a schedule goal --- What’s missing, what’s extraneous? Need some new grad students to make it all go; send us your hot shot undergraduates. 11 April 2019 G060535-00-I