G070550-00-I Enhanced LIGO Update Rana Adhikari July ’07 LSC Meeting.

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Presentation transcript:

G I Enhanced LIGO Update Rana Adhikari July ’07 LSC Meeting

G I

U of Minnesota

G I Timeline 1y S5 Coincidence IFOs ready Post-run diag. VENT MAXIMIZE TIME FOR S6 RUN: Several very new subsystems to debug Test different systems H1, L1 ‘Pathfinder phase’ Once teething troubles are debugged, update the other site with what works best ‘Synchronization phase’ Continue leapfrog commissioning w/both instruments completed to reach design sensitivity S6 AdL INSTALL AdL COMMISSION S5 S7 Inst/Comm

G I DC Readout In-vac, DC detectors. No RF demodulation for GW. No more AS_Q. Hardware DC PDs (Rich Abbott) Output Mode Cleaner (Sam W.) Active Beam Stabilization (Bram S.) OMC Suspension (Norna, Janeen, Chris, etc.) Stiff HAM (B. Lantz, ) Diode Testing (Nick Smith, Jamie Rollins) New AdvLIGO controls architecture (CDS) DC Readout Experiments Caltech 40m (Rob Ward) LLO (Rupal Amin, Valera, Sam, Rob)

G I Need serious jitter control to have good noise performance: in- vac, reliable -> ABS Like a iLIGO SOS but smaller and tougher Led by Bram Johannes Jozef ANU Pendulum freqs ~few Hz; passive isolation Large Range ( > 10 mrad & ~1 N/A) Enables dither lock of IFO beam to suspended OMC Dither software tested at 40m Active Beam Stabilization

G I Scattered Light iLIGO baffles were never installed, holes are incompatible (TCS, P-Cal) iLIGO baffles were never installed, holes are incompatible (TCS, P-Cal) Schofield/O’Reilly measurements show coupling from VE ( m/m) Schofield/O’Reilly measurements show coupling from VE ( m/m) Design/Fab/Install new baffles in all potential hot spots (aim for 100x clearance) Design/Fab/Install new baffles in all potential hot spots (aim for 100x clearance)

G IMisc 35 W Laser from LZH/AEI is arriving at CIT soon – integration with iLIGO servos TCS (Tobin Fricke, Phil Willems) – ultra-low noise ISS pre-amp, servo electronics from MIT, ‘Axicons’ for making donut beams. Will have to retire the LHO Quiet Chillers and find room for the new ones. Earthquake Stops – New glass-top stops being developed at MIT to reduce earthquake induced charge buildup. SUS Electronics Noise reduction – bias modules, coil drivers, careful LOS alignment plan MC Loss – absorption measured at LLO by SURF, scatter loss still a problem.

G I Summary So far so good: no large schedule mishaps or technical walls. Enhanced Grad Students (Nick Smith, Rupal Amin, Tobin Fricke,...)