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Is it possible to acquire lock with radiation pressure?

Time domain simulation for a FP cavity with AdLIGO parameters on E2E. Osamu Miyakawa, Hiroaki Yamamoto Caltech 8/14/2006 LSC meeting at LSU. Is it possible to acquire lock with radiation pressure? Is it possible to control alignment with radiation pressure? Optical spring in ASC?

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Is it possible to acquire lock with radiation pressure?

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  1. Time domain simulation fora FP cavity with AdLIGO parameters on E2E Osamu Miyakawa, Hiroaki Yamamoto Caltech 8/14/2006 LSC meeting at LSU • Is it possible to acquire lock with radiation pressure? • Is it possible to control alignment with radiation pressure? • Optical spring in ASC? • Do we need test mass actuator for ASC? both ETM and ITM? • Is the actuator dynamic range enough? • Noise performance?

  2. What implemented • AdLIGO Quad suspension (Mark’s model 03/31/2006) • Local damping (6 DOFs of M0) • Seismic motion and optical table motion on X,Y, tY and tZ (length, side, pitch and yaw) • 3995m FP single cavity with AdLIGO parameters • ROC = 2076m for both ITM, ETM test mass • Full laser power inside cavity = 0.73MW • Radiation pressure force on length and alignment • Shot noise and radiation pressure noise • Length control for M3 through M1, M2, M3 • M3 alignment control through M2 using WFS • Electronic noise of WFS PD Main Ref. Top mass (M0) Upper Intermidiate mass (M1) Penultimate mass (M2) Test mass(M3) Z X Y

  3. Quad Suspension ETM Quad Suspension ETM Seismic motion Seismic motion Main mass Actuator Ref. mass FP summation cavity Feedback filters Laser PDs Optics Local Damping Rdiation pressure Rdiation pressure E2E

  4. Main Ref. Damped DOFs (OSEM DOFs) 6(6) M0 0(3) M1 0(3) M2 0(0) M3 Local damping Example M0: pitch Zero @ 0Hz Pole @ 10,10Hz

  5. Local damping: impulse response Example M0: pitch E2E simulation Measured data

  6. Quad suspension withradiation pressure (length) • LSC only, no ASC • Only TEM00; misalignment not break lock • Test masses are pushed by radiation pressure. • ETM test mass is pushed back by LSC keeping distance between test masses. • Position shift ~10 wave length • Angle shift ~10mrad ITM ETM LSC LSC Radiation pressure LSC 1.2e-5 m 8e-6 rad

  7. Lock acquisition with radiation pressure Locked No lock Locked • 60nm/sec :enough slow to acquire lock for LSC by Matt Evans • Radiation pressure and alignment incleded • Full power : 0.7MW • Lock can be acquired with less than few kW • Is it possible such low power? Offset lock used at 40m? ->Optical spring • Needs Monte Carlo simulation

  8. Alignment instability with no ASC Lost lock • After lock acquisition, input power increased with no ASC. • Pitch motion due to Radiation pressure breaks lock with 10%(70kW) of full power if there is no ASC

  9. ITM ETM LSC ASC ASC LSC ASC ASC Radiation pressure LSC 1.3e-5 m Test mass alignment control through M2with radiation pressure • Control M3 through M2 • f 3 filter • Boost at 2Hz • 10Hz control band width

  10. Two modes of optical instability Differential : stable -> spring Common : unstable -> no spring

  11. Opt-mechanical (suspension) TF Optical spring Optical spring • TF from M2 actuator to WFS error signal, simulated in time domain. • Low frequency gain and peak are suppressed. • Needs compensating gain for full power • Optical spring in differential mode at 4.5Hz for pitch and 4.1Hz for yaw. • Control BW must be higher than optical spring frequency.

  12. Open loop TF of ASC • 10Hzcontrol band width • Gain in low frequency is suppressed a lot by radiation pressure

  13. Noise performance • Residual RMS: <10-9 rad (depends on servo) of 10-9rad requirement • Actuation torque(force): 3x10-5 Nm (1x10-4 N) on M2 OSEM (max 20mN)

  14. Noise performance in spectra • Spectrum depends on seismic noise model. • Length to pitch coupling is not ignorable, but can be avoided using unbalance of OSEM. • High frequency is limited by shotnoise at 10-14 rad/rHz with 100mW input(25mW for each quadrant).

  15. Electronic noise with low power WFS ON 10% of full power M2 OSEM Dynamic range Start increasing power Locked with 1kW • Full power: 0.7MW with electronic noise of 10-6rad/V, 100mVmax, 10nV/rHz • 10-14rad/rHz (same level as shotnoise), force: 3x10-4Np-p (maximum:20mN) • Low power: 1kW for lock acquisition, 7x10-4rad/V, 100mVmax, 10nV/rHz • 7x10-12rad/rHz, force: 20mNp-p(maximum:20mN) -> OSEM saturation

  16. Electronic noise with low power M2 OSEM Dynamic range Electronic Noise Enhancement • Feedback Penultimate mass(M2) and test mass(M3) for both ITM and ETM? • Low/High gain WFS? • Variable transimpedance of factor sqrt(700)? • Same level as shotnoise of low power case • Pole around 30Hz?

  17. 2-pole at 30Hz WFS ON 10% of full power M2 OSEM Dynamic range Start increasing power Locked with 1kW • Seems stable

  18. Conclusion • Is it possible to acquire lock with radiation pressure? • Yes, with less than few kW • Is it possible to control alignment with radiation pressure? • Yes, with 10Hz control band-width • Optical spring in ASC? • Yes, 4-5Hz • Do we need test mass actuator for ASC? both ETM and ITM? • No for full power, penultimate mass actuator enough, but might be necessary for low power • Is the actuator dynamic range enough? • Yes for full power: 1mN of 20mN, but No for low power: 20mN of 20mN -> low-pass filter around 30Hz • Noise performance? • < 10-9 rad

  19. Next step • Unbalance on OSEM • Miss-centering • Another g-factor • Monte-Carlo lock acquisition test • Lock acquisition for full DRFPMI case • simulation time : real time = 10 : 1 for single FP cavity = 200 : 1 for DRFPMI with LSC only = 400000 : 1 for DRFPMI with ASC ->needs summation DRMI for alignment

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