I made a first integrated noise budget for PRFPMI with NoiseBudgetter. Plot below is from Mar 9, 2020 14:00 UTC when we reached 0.6 Mpc.
See, also klog #11755 for NB for FPMI.
Shot noise estimated based on measurements done with lower power suggests we are mostly limited by shot noise above 200 Hz.
NoiseBudgetter configuration file lives in
/kagra/Dropbox/Subsystems/MIF/NoiseBudget/PRFPMI/NPconf_20200311_1119.csv
Details
* Suspension thermal noise
- Suspension thermal noise of cryogenic payload at 300 K, based on Somiya-san's calculation (300Knew.nb)
* Mirror thermal noise
- Substrate + thermoelastic + coating thermal noise of sapphire mirror at 300 K, based on Somiya-san's calculation (300Knew.nb)
* Shot noise
- Based on Enomoto-kun's calculation in klog #12772. It was roughly 1.3e-19*sqrt(1+(freq/22 Hz)**2) /rtHz. I simply scaled this with sqrt(1.4/Pin)*sqrt(3.4mW/8mW), where Pin is the IMC output power (2.9 W for this plot). [NEED TO REDO THIS WITH CURRENT OPTICAL GAIN]
- Cavity pole assumed to be 22 Hz, which is the number I heard. [NEED CONFIRMATION]
* OMC DC PD dark noise
- Dark noise of OC DC PD measured at K1:CAL-CS_PROC_DARM_DISPLACEMENT_DQ (there fore you have to calibrate it with 5-stage dewhitening to make it actual DARM displacement spectrum as usual). I'm not sure the details, but DARMsens.xml says it is measured on Feb.11 with 1stage wh.
* Type A noise
- Noise from klog #13474. Sum of all four suspensions.
* Intensity noise
- Based on measurement done by me in klog #13028. K1:PSL-ISS_FIRST_SERVO_PDA_RIN_OUT_DQ is projected to DARM displacement with a gain of 1.1e-12 m and zeros at 100 Hz, 2500 Hz.
* Frequency noise
- K1:LSC-CARM_RESIDUAL_OUT_DQ is projected to DARM with 3e-14. I'm not sure where this 3e-14 is from. DARMsens.xml says "based on 2020 Feb 14" [NEED CONFIRMATION]
- Related: klog #13442
Discussion on shot noise
- Shot noise calculation above is a very rough estimate. We should redo the shot noise measurement.
- Also, theoretical quantum noise with 30 W at BS, 70% loss from SRM is a factor of 2.5 smaller (see attached). This might suggest some very big loss. Please measure the optical loss from BS to OMC DC PD (as was done in klog #11762, with AS RF).
Next:
- Include MICH and PRCL projections
- Let me know if you have your favorite noise projections. Let me know the name of the witness channel, and its coupling transfer function to DARM.