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R&D (Cryogenic)
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SatoshiTanioka - 11:12, Thursday 16 January 2020 (1970)Get code to link to this report
Cooling down test

Since the pressure reached 6.5*10-4 Pa, I turned on the refrigerator.
It seemed working and I left it running.

Comments related to this report
SatoshiTanioka - 20:34, Saturday 18 January 2020 (1974)

After 2.5 days cooling, the cryostat reached the temperature ~60 K.
This value is my guess because the sensor had some problems and it showed higher temperature than actual.

Anyway, the refrigerator worked well though longer cooling time than before.
This is due to some insulators were not installed inside the chamber...
But it can be cooled down at some extent and I gonna do with this configuration.

I turned off the refrigerator around 20:20.

R&D (FilterCavity)
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EleonoraCapocasa - 11:12, Thursday 16 January 2020 (1969)Get code to link to this report
Comment to Replacement of lens for homodyne (Click here to view original report: 1968)

The measurment in the first picure is done when the back reflected light towords the squeezing path is blocked with a sensor card.

R&D (FilterCavity)
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YuhangZhao - 01:22, Thursday 16 January 2020 (1968)Get code to link to this report
Replacement of lens for homodyne

We received the super-polished lens from CVI with 30mm focal length. With this super-polished lens we should have less parasitic interference.

So we compared the back scattering and squeezing level.

As shown in the attached figure, there are some difference at low frequency which is more back scattering(worse) and more squeezing(better). 

Actually the low frequency part, we have already ovserved some uncertainty during different measurment. So it seems the replacement of lens doesn't improve system obviously.

Images attached to this report
1968_20200115172217_bs.png 1968_20200115172223_sqz.png
Comments related to this report
EleonoraCapocasa - 11:12, Thursday 16 January 2020 (1969)

The measurment in the first picure is done when the back reflected light towords the squeezing path is blocked with a sensor card.

R&D (Cryogenic)
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SatoshiTanioka - 20:34, Wednesday 15 January 2020 (1967)Get code to link to this report
Comment to Preparation for cooling down test (Click here to view original report: 1964)

Since the pressure was 1.5*10-5 mbar, I decided to turn on the cryostat on tomorrow morning.
I will leave the scroll and turbo pump running overnight.

R&D (FilterCavity)
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RyutaroTakahashi - 16:16, Wednesday 15 January 2020 (1966)Get code to link to this report
Replacement of DP

I found that the DP (DSP250) back of the TMP was failed with "ALM06" in the south end. Though I tried to restart it some times, it was not rcovered.

I replaced the DP to the other DP (DSP500) from arm front where the TMP is not working now.

R&D (FilterCavity)
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EleonoraCapocasa - 11:03, Wednesday 15 January 2020 (1965)Get code to link to this report
System recovery after holidays

[Yuhang, Eleonora]

Filter cavity lock was recovered easily.

Then we checked green alignment into OPO: we sent BAB and maximized its alignement into OPO by moving the lens in pic 1. We scanned OPO and measure the BAB transmitted TEM00 with and without green pump. The green phase was modulated at 10 Hz. We optimized the alignment of the green beam into OPO by maximizing the BAB transmission. The ratio between BAB transmission with green (pic2) and without green (pic 3) gives the parametric gain which is ~ 25.4 for 50mW of pump. It seems fine. Note that recently we observed a reduced parametric gain but this measurement is in agreemen with the early value (see entry #1131).

We changed OPO temperature from 7.185 to 7.215 kOhm to maximize the non-linear gain, (with the PLL offset without green set to 180 MHz.)

We check the p-pol PLL offset when green is injected into OPO and optimized it by maximizing CC1 error signal. Now the good values for PLL offset are:

  with green without green
PLL offset 180 MHz 325 MHz

We found that p-pol was not well aligned into OPO, and the alignment was very unsatable and difficult to optimize. Eventually we discovered the p-pol laser temperature was 2 degree away from the optimal temperature. So the issue was likely due to mode-hop. We put it back at the nominal value and we confirmed that all the lasers are at the optimal temperature, namely:

  MAIN P-pol CC
temperature 23.105 °C 32.49 °C 38.15 °C

Then we aligned p-pol and CC into OPO. Spectrum is shown in Pic 4 (blue is p-pol, yellow is CC).

Finally, we measured again squeezing with 50mW green pump. The measured squeezing level is 5.9dB which is consistent with the measurement done before. Besides, the spectrum is as flat as before.

Images attached to this report
1965_20200115025445_baball.jpeg 1965_20200115025502_babg.jpeg 1965_20200115025510_babng.jpeg 1965_20200115115906_polspol.jpeg 1965_20200115165927_squeezing.png
R&D (Cryogenic)
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SatoshiTanioka - 21:59, Tuesday 14 January 2020 (1964)Get code to link to this report
Preparation for cooling down test

I installed the inner shields, forgot to take pictures though...
When the vacuum level gets enough low, I gonna turn on the cryostat.

Comments related to this report
SatoshiTanioka - 20:34, Wednesday 15 January 2020 (1967)

Since the pressure was 1.5*10-5 mbar, I decided to turn on the cryostat on tomorrow morning.
I will leave the scroll and turbo pump running overnight.

R&D (Cryogenic)
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SatoshiTanioka - 17:35, Friday 10 January 2020 (1962)Get code to link to this report
1st vacuum check after the installation of 4K shield

Today, I did vacuum test with the repaired scroll pump and the turbo pump.
Since the chamber had been opend for a long time, the vacuum level was not good though there were no huge leaks.
In addition, one of the vacuum gauge did not work.

I will do another vacuum test, and then do cryogenic test.

KAGRA MIR (Absorption)
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SimonZeidler - 13:59, Friday 10 January 2020 (1961)Get code to link to this report
Setting the FI and adjustment

Pengbo, Simon

Yesterday, we have finally set the FI in place and tried to get the laser beam through it.
We recognized that a proper adjustment stage would be desirable as it decreases the work. However, since we couldn't find a suitable one (or one which isn't used rigth now), we installed the FI-cage on top of two scalable posts and tried or luck with them. In the end, I think we could reach a good position and ca. half of the ligth passes toward the sample chamber (which is as expected since we still don't have the second HWP in front of the second PBS).
Also, in order to have a free space for the ejecting non-used beams, we removed one of the 4 bars of the cage-system for the FI. We think that this is not harming the overall stability of the system since it makes a very sophistictated impression anyway.

Judging from the laser card, the beam shape seems to be fine but we need to investigate it more deeper with the beam-profiler.

After setting the FI, we placed some beam-dumps in those positions were a non-used beam is ejected sideways from the FI. Unfortunately, these beams are under a non-rectangular angle and thus a damping is a bit tricky. We, however, used an elongated post to fix a holder where the angular position can be freely adjusted (see also attached pictures) for the beam that goes also upwards. For the other, we are utilizing a new beam-dump with a large opening so that also the transmitted light from the coated 45 deg mirror can be covered.

Images attached to this report
1961_20200110055652_59.jpg 1961_20200110055702_06.jpg 1961_20200110055711_11.jpg 1961_20200110055717_18.jpg 1961_20200110055722_22.jpg 1961_20200110055727_15.jpg 1961_20200110055731_20.jpg 1961_20200110055736_44.jpg
KAGRA MIR (Absorption)
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SimonZeidler - 22:47, Wednesday 08 January 2020 (1960)Get code to link to this report
Continuation of upgrading the PCI

Pengbo, Simon

Today, the upgrading process was continued by setting everything except the FI in its determined position, according to the draft which is attached to this report.
As for a matter of understanding, this draft is a supposed to be a first trial of the basic working principle which we are aiming for.

By re-activating the laser, I recognized that if the first PBS is set plane in its position as indicated in the draft, only a few percent of power would be P-polarized. Therefore, I rotated the PBS so that the non-used beam would be weakest. With this, I planted a beam-dump on top of the PBS cube (thanks to Thorlabs cage system) to catch that beam. In my opinion, even with this a little bit strange setup, security is maintained. In a next step, the motorized HWP was tested with the laser and confirmed to be working fine.

Addendum: I set also a beam-dump on the second PBS to cover the non-used S-polarization.

Images attached to this report
1960_20200108144821_pciupgrade.png
KAGRA MIR (Absorption)
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PengboLi - 19:14, Tuesday 07 January 2020 (1959)Get code to link to this report
Reset the transation stage

Simon, Pengbo

Today we reset the translation stage make sure it can work properly and then start the upgrade of the laser control part.

R&D (Cryogenic)
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SatoshiTanioka - 17:36, Tuesday 07 January 2020 (1958)Get code to link to this report
Requirement for ISS

I meaured the laser intensity noise with free-running and estimated the requirement for ISS.
The RIN with free-run laser was the order of 10-6.

Assuming DC lock of HOMs and common mode rejection ratio as 1/10, the requirement for RIN is estimated as 3*10-8.

Therefore, about 100-times stabilization is necessary in order to achieve the requirement.
I will design the intensity stabilization servo which satisfies this requirement.

Images attached to this report
1958_20200107093627_rinfree.png
R&D (FilterCavity)
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NaokiAritomi - 16:59, Tuesday 24 December 2019 (1957)Get code to link to this report
CCFC error signal on 20191224

First I optimized p pol PLL frequency when green power is 50mW and optimal frequency is 150MHz.

Today when filter cavity is locked, a strong 70kHz noise appears in CC1 error signal. This makes it difficult to get clean CCFC error signal.

Anyway I measured CCFC error signal again when CC is locked on resonance (Pic. 1).

I found that when demodulation phase of CCFC changed, CCFC error signal also changed from Pic. 2 to Pic. 3.

Images attached to this report
1957_20191224085954_cc320191224.png 1957_20191224091214_img8163.jpg 1957_20191224091223_img8164.jpg
R&D (FilterCavity)
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EleonoraCapocasa - 06:57, Tuesday 24 December 2019 (1956)Get code to link to this report
Comment to CC3 error signal on 20191223 (Click here to view original report: 1955)

113 Hz is the frequency of the line sent to the rampeauto perturb channel to test LO alignemnt with the technique proposed by Raffaele. I guess we forgot to switch it off last friday. 

I connected remotely and switched it off now. Sorry for the inconvenience!

R&D (FilterCavity)
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NaokiAritomi - 19:22, Monday 23 December 2019 (1955)Get code to link to this report
CCFC error signal on 20191223

First I increased green power from 40mW to 50mW. Carrier and CC resonance frequency is as follows. CC PLL frequency is same as last week.

  AOM frequency (MHz)
carrier 109.035827
CC 109.035977

CCFC error signal when AOM is scanned around CC resonance is shown in Pic. 1 channel 2. It is different from the error signal last week and seems very noisy. I also measured spectrum of CCFC error signal when CC is locked on resonance (Pic. 2). There is a very strong 113Hz peak in CCFC error signal.

Images attached to this report
1955_20191223112527_img8155.jpg 1955_20191223112536_cc320191223.png
Comments related to this report
EleonoraCapocasa - 06:57, Tuesday 24 December 2019 (1956)

113 Hz is the frequency of the line sent to the rampeauto perturb channel to test LO alignemnt with the technique proposed by Raffaele. I guess we forgot to switch it off last friday. 

I connected remotely and switched it off now. Sorry for the inconvenience!

R&D (FilterCavity)
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NaokiAritomi - 18:42, Saturday 21 December 2019 (1954)Get code to link to this report
Trial to get CCFC error signal

[Aritomi, Yuhang, Eleonora]

To make one of CCSB on resonance inside filter cavity, we set CC PLL frequency 6.997043MHz following previous measurement. We also changed 14MHz and 21MHz accordingly in DDS board.

Binary number is as follows.

Frequency (MHz) Binary number
  6.99704303     11 10010101 00011101 11001110
13.99408607   111 00101010 00111011 10011100
20.99112910 1010 10111111 01011001 01101010

Then we split CC1 LO (14MHz) into 50:50 with Z99SC-62-S+ to use it for demodulation of CCFC, but CC1 was unstable due to low SNR. Therefore we amplified CC1 LO by 33dB and attenuated by 20dB before splitting. Since output of DDS board is -6.5dBm, CC1 and CCFC LO is -6.5+33-20-3 = 3.5dBm. Then CC1 locked stably.

We set CC PLL 7MHz as usual and scanned AOM around one of CC resonance while other CC sideband was off resonance. CCFC error signal was shown in Pic. 1 (Channel 1: IR transmission, Channel 2: CCFC error signal). It seems like usual PDH signal. Then we set CC PLL 6.99704303MHz and found CC resonance at 109.03598MHz while carrier is 109.03584MHz which means carrier is detuned by 109.03598-109.03584 = 140Hz. CCFC error signal was shown in Pic. 2. The error signal was just a dip and didn't change by demodulation phase.

Images attached to this report
1954_20191221104219_img8150.jpg 1954_20191221104227_img8149.jpg
R&D (FilterCavity)
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EleonoraCapocasa - 11:22, Wednesday 18 December 2019 (1953)Get code to link to this report
Filter cavity remote lock and servo gain adjustment

On Monday, I found that the cavity remote locking was not working properly. Matteo told me that somehow the treshold for lock acquisition was changed last week.

I put it back to the original value of -0.5 V and now it seems to work quite good.

I also found the the transmission was not stable despite the dithering was engaged. The situation improveed after I increased the gain. (Pic 1) 

Current values:

INPUT ATTENUATION: 2.9

GAIN: 5.7

Images attached to this report
1953_20191218032144_gain1.jpeg 1953_20191218032209_gain2.jpeg
R&D (FilterCavity)
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NaokiAritomi - 08:50, Wednesday 18 December 2019 (1952)Get code to link to this report
LO power reduction for LO back scattering

[Aritomi, Yuhang, Eleonora]

First we measured shot noise spectrum with sensor card in squeezing path to see LO back scattering. Then we reduced LO power from 1.86mW to 0.158mW by putting ND filter after IRMC. Pic. 1 shows shot noise with different LO power. Shot noise reduced by 10.5dB and 13Hz peak from LO back scattering reduced by 21dB as expected.

Then we measured shot noise with filter cavity. At the beginning we saw low frequency bump in shot noise spectrum, but after some alignment of homodyne, the low frequency bump somehow reduced a lot. Pic. 2 shows shot noise with filter cavity.

Images attached to this report
1952_20191218005026_sensorcard20191217.png 1952_20191218005041_shotfc20191217.png
R&D (FilterCavity)
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NaokiAritomi - 08:08, Wednesday 18 December 2019 (1951)Get code to link to this report
FDS at 60Hz

[Aritomi, Yuhang, Eleonora]

CC2 demodulation phase
sqz: 80 deg, asqz: 130 deg
 

sqz_dB = 11.5;                    % produced SQZ

L_rt = 100e-6;                    % FC losses

L_inj = 0.20;                     % Injection losses

L_ro = 0.11;                      % Readout losses

A0 = 0.1;                         % Squeezed field/filter cavity mode mismatch losses

C0 = 0.1;                         % Squeezed field/local oscillator mode mismatch losses

ERR_L =   5e-12;                  % Lock accuracy [m]

ERR_csi = 80e-3;                  % Phase noise[rad]

phi_Hom = [0/180*pi, pi/2*90/90];      % Homodyne angle [rad] (you can input a vector of values)

det =  [100 60];                       % detuning frequency [Hz]

Images attached to this report
1951_20191218000835_fds6020191217.png 1951_20191220023702_degradation20191217.png
R&D (Cryogenic)
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SatoshiTanioka - 17:24, Tuesday 17 December 2019 (1950)Get code to link to this report
4K shield installation

[Sato-san, Tanioka]

We installed a 4K shield which was modified by Namai-san and Ueda-san.
The procedures are as following.

  1. Attached the cables on the shield as heat anchors
    At this moment, we found that the cable which was used for thermometer was disconnected. This was solved by bypassing the cable. But the displayed temperature seemed not correct. Calibration is needed.
  2. Installed insulator on the shield.
  3. Made holes on the insulators in order to pass through the beam.
  4. Put the shield on the optical breadboard.
  5. Check the cabling and the status of insulators.
  6. Then clamped to the table.

[note]

  • We found that we forgot to install the insulator under the optical table...
    I hope that the impact will be small enough.
  • I forgot to prepare appropriate screws and washers.
    The ones installed temporary should be replaced.

[next step]

  • Replace screws.
  • Calibrate thermometer.
  • Vacuum test
  • Cooling test
Images attached to this report
1950_20191217090701_20191217shield.jpg