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| * Can we add a heater back to OMC mirror to control ROC? How should the temperature be sensed and controlled? |
Balanced Homodyne Detection
Requirements
- Displacement noise of OMC/LMC mirrors
- Scatter loss in mirrors
- Cavity design: triangle, quad ring, quad zig-zag (reference the new OMC paper from Koji)
- Laser amplitude / frequency noise including DC offsets in various other lock points and motions to simulate bilinear noise
- Oscillator noise: AM / FM
- Aux length noise: MICH/PRC/ SRC
- Req. on offsets/asymmetries: arm finesse, arm reflectivity, mass imbalance of ETMs
- Phase noise of LO
- Polarization stability requirement for polarization BHD
- Backscatter
Action items
- Design SRC so that
- Suppress 02/20 modes
- Partially transmit 01/10 modes for AS WFS
- Suppress thermally generated modes
- After the above have been satisfied, choose transmission to maximize ponderomotive squeezing
- Budget above noises, but especially investigate polarization stability.
- How is homodyne angle controlled?
- Beam routing
- Where to pick off LO?
- Can we use ETMX transmission for LO? (Koji is crazy)
- A+ BHD noise budget for both baseline double OMC and polarization BHD.
- Can we add a heater back to OMC mirror to control ROC? How should the temperature be sensed and controlled?
Modeling/Noise Budget
Some BHD modeling is done in the OptimalGWextraction repo here.
Polarization BHD
