LIGO-G020091-00-Z 3) Current Status & Plan for Japan RSE -- Stabilization and Installation of PRC & Detuning -- LSC Livingston 2002 Kentaro Somiya.

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Presentation transcript:

LIGO-G Z 3) Current Status & Plan for Japan RSE -- Stabilization and Installation of PRC & Detuning -- LSC Livingston 2002 Kentaro Somiya University of Tokyo

Roles for 3 prototype RSE Caltech 40m : Science Glasgow 10m : Engineering Japan 4m RSE : ?? Development (With Engineering Support) Example : One modulation control, One modulation detuning, WFS for RSE, USB detection, Lock acquisition using polarization, Sweeping, DC readout scheme,,, etc. We can try any new challenges for advanced IFO.

Calendars Future m DRSELIGO II LCGT 40m Infrastructure 10m DRSE BRSE4m DRSE TAMA (w/o RSE) Osamu Seiji (1yr)

We moved to a bigger room, building a new vacuum system.

Comparison with previous 4m RSE 3m thin pipe( 20cm) Small chamber(50cm) Thick pipe( 60cm) Big three chambers in series Asymmetry for THD and SRC for detuning are both less than 3m… This new system allows us various configuration! 1m chamber

Plan 1.Interferometer Stabilization 2.Power Recycling 3.Detuning …etc.

Plan (1) : Interferometer Stabilization 1-1) Suspension Improvement - Decrease Q factor of pitch & yaw, - Negative resistance damping is one way. 1-2)Servo Improvement - Increase DC gain. 1-3)Reduction of the Big Asymmetry - I will explain the reason and a way to do.

Why the asymmetry is to be reduced? 2 nd SB is anti-resonant in RSEC. is set to be 60 deg to eliminate 3 rd SB on dark port. FSR for RSEC is equivalent to the modulation frequency. Carrier becomes anti-resonant as it resonate on the arms. 3 rd SB doesn't come through to the dark port. 2 nd SB becomes anti-resonant as its cosine is negative. asymmetry THD control signal becomes small for high finesse RSEC.

Asymmetry should be small 3 rd SB should be removed There are several ways to meet both conditions. Pre-Michelson Interferometer 3 rd order Anti-modulation LASER Broadband EOM Isolator Resonator x3 Freq. tripler Fixed Michelson with 60 deg asymmetry To IFO Then, Asymmetry can be used to optimize the RSE control. We can use THD at sym. port. THD control for PRC will be improved. RSEC length can be small enough for detuning. Contrast will be improved. LASER noise will be reduced. We will try and choose either.

Plan (2) : Power Recycling Peter B. will explain this at the following talk. FSR of RSE cavity 2 nd SB is anti-resonant in PR cavity. Lock acquisition would be difficult for high finesse PRC.

Plan (3) : Detuning Detune Phase Particular detuning with one modulation using THD control. (RSE cavity should be short. That’s the most inevitable motivation to reduce asymmetry.) We are planning to also try DC offset detuning.

Milestones accomplished Vacuum test (’01 Dec.) : 3.4e-7 torr. Osamu finished his experiment. (’02 Jan.) We moved the room. Three undergrads joined us. (’02 Feb.) Eric Black visited, helping us for 2 weeks. RSE restoration started : With Osamu’s method in new chamber. Broken suspensions are repaired. Each arm cavities lock. Michelson lock. Asymmetry measurement. (’02 Mar.) : error < 0.5mm FPMI lock. Mode matching improvement. This restoration is being done to (1)Educate undergrads, (2)Share Osamu’s knowledge, and (3)Check the Equipments. 8 people in lab!

Schedule April : Restoring completes Polarization experiment starts May : Development of 3 rd order anti-modulation Asymmetry reduction and arm cavity extension June-July : Broadband RSE stabilization August : Power Recycling installation (using polarization) September : PR-RSE stabilization October-December : Detuning installation......