ISC Meeting on 2018/11/5 14:00 - 15:00

Participants:

Zoom meeting: https://zoom.us/j/6676627462

Next meeting

2018/11/19 (Mon) 14:00-15:00 (JST)

https://www.timeanddate.com/worldclock/meetingtime.html?day=19&month=11&year=2018&p1=248&p2=4399&p3=137&iv=0

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Minutes

Agenda

• Main topics for Phase-2 [Michimura]

  • Fix initial alignment scheme for full IFO
    • Enomoto?

    • For XY arm JGW-G1808462

  • Finalize ALS scheme and RF AM generation scheme and finalize lock acquisition scheme
    • Enomoto?
  • ISC modeling, especially ASC modeling, for intermediate IFO configurations
    • Tanioka for ASC?

  • Cabling diagram

    • Almost finalized JGW-D1808394

  • In-vacuum RF PD and RF QPD
    • Izumi will ask LIGO people first. And ask Doi for handling fabrication?
    • Laser welding would be tough (resonant circuit cannot be re-tuned)
    • Use similar design to OMC DC PD preamplifier?
  • Readout DC PDs and OMC

    • In-vac amplifier board made JGW-D1809177

    • Cabling diagram around OMC JGW-G1809012

  • Design output optics on optical tables

    • REFL [Aritomi] (almost done, to be ordered)

    • POP [done for green; ? for IR]
    • POS [done for green; ? for IR]
    • TRX/TRY [K. Nagano for both IR and green]

      • TRX designed and assembled JGW-T1808962

    • AS [??]

    • 20 mm diameter optics post to be ordered by Izumi

• RF modulation system

  • Three-f or f3
    • Agreed to work on both three-f and f3 for redundancy
    • O3 requirement for MZI was calculated (and met?)
      • A/I: The deadline and when to disassemble MZI (remove some of BSs) when the requirement was not met are to be discussed
    • A/I: How to proceed with broadband PDs for f3-f1/f3-f2? Modify our resonant RF PD? (BB PD also necessary for SPOP (and SPOS))
  • Low noise VCO

    • Two Prototype Low Noise VCO for ALSX and Y assembled (JGW-D1808968), and noise of the one of them was measured. Meets the requirement.

    • We need three real ones for ALSX, ALSY and FSS

      • 110MHz for FSS? FSS AOM driver broken. Status?

    • For PLLX and PLLY, Keysight E8663D is used.
      • A/I: Need to develop a code to sweep the frequency.
  • RF source
    • Harmonics Generator will arrive in the beggining of Nov (or end of Nov in worst case)

    • We currently have 6 Agilent N5181B, but we need 7 JGW-T1706762

      • PMC PDH (15MHz)
      • Refcav PDH (51.75MHz)
      • IMC PDH (13.78MHz)
      • seed for Harmonics Generator
        • if Harmonics Generator delayed, we need 2 for f1 and f2, so we will use one for ALSY PDH
      • ALSX PDH (33MHz) (NOTE that 33MHz for ALSX PDH, not 32MHz)
      • ALSY PDH (32MHz)
        • Not necessary until Yarm commissioning starts (mid-Nov?)
      • seed for ALS VCO (~70MHz)
        • for now, we will use Keysight 33612A (Enomoto's own)
        • will be replaced to Keysight 33611A-OCX (ordered)

    • RF amplifier for EOM to be requested to AEL soon. JGW-T180921

• Common mode servo board CMSB wiki JGW-G1808547

  • Summarized, requested to AEL JGW-T1809210

  • We will make 20 boards, and 10 will be assembled as chassis
  • We currently have 5 chassis and used for 1st MZI, IMC, CARM, PLL X, ALS PDHX
  • Needs 4 chassis more soon: 2nd MZI, PLL Y, ALS PDHY, ALS COMM summing node
  • 6 chassis for spare: MZI, IMC, CARM, PLL, PDH, summing node

• OMC status

  • Calculations on DC power and circuit noise -> Somiya & Arai

    • Koji's calculation: DCPDCalculation

  • Electronics status

    • In-vac DC PD amplifier board finalized JGW-D1809177

    • In-air DC QPD amplifier board arrived (without chassis and interfaces)

• ITMY inhomogeneity JGW-T1808715

  • We should check impact on sensitivity and locking as soon as possible
    • For both O3 and full bKAGRA
  • There was a discussion whether we should re-optimize OMC for BRSE or DRSE without homodyne angle optimization.
  • ASC simulation by FINESSE show worse signal when ITMY inhomogeniety is added (a few % degradation in shot noise?)
  • higher order contents, especially odd-order modes are worse
  • But still need to check the Finesse code (alignment loop not closed yet)
• SRM-M with metal parts
  • Characterization results?

• RF generation using Mach-Zehnder interferometer [Kohei Yamamoto] JGW-G1707309 JGW-G1807655 JGW-G1808029

  • simulation on imperfections (MZ arm asymmetry, MZ lock, EOM phase difference control etc.)
  • calculate requirements on MZI displacement, EOM modulation phase difference, EOM imbalance
  • Requirements derived from full Optickle simulation and those derived from transfer function between displacement of MZI and sideband power kind of matched after implementing RAM into calculation for the latter. However, we need more investigation on the following issues:
    • Modulation depth for RAM generating EOM changes the requirement.
    • Spectrum shapes of the requirements for mid-fringe do not match. Maybe coming from accuracy of the mid-fringe?
    • Unknown frequency response of the transfer function from the displacement of MZI and sideband power
    • Check if caluculated RF oscillator amplitude noise is relative one or not with simple Optickle model
  • calculations for requirements on delay line lock displacement noise, parallel EOM MZ lock displacement noise, EOM modulation phase difference, EOM imbalance on-going

  • Relative f1 PM and f1 AM also needs to be adjusted (CQG 31, 095003 (2014)). Another EOM for f1 or relative amplitude adjuster between two EOMs?

  • Requirement on carrier power loss?
  • Comment from Stefan Ballmer
    • Similar calculation was done in LIGO in the past. Displacement noise requirement for MZ was tough (~1e-14 m/rtHz).
    • Any in-air interferometer suffer from jitter and frequency noise which cannot be suppressed.

  • Ref: LIGO-T040119

  • MZI implementation starts in May, probably before high power laser installation
  • RF oscillator noise requirements for MZI should also be calculated
• RF generation scheme [Michimura]
  • f1 = 3/8*f2, f3 = 10/8*f2
  • we need 2*f1, 2*f2, f3-f1, f3-f2 as well
  • use harmonics generator (x3, x5, x6, x7, x8, x10, x16 for f2/8 = 5.62698725 MHz (FSR for IMC))

    • Wenzel specsheet JGW-D1808028

      • ordered two units on Apr 21 (takes 14 weeks)

    • It should be x2, x3, x6, x7, x8, x10, x16 (Michimura realized this on June 30)

  • Usage of 6 Agilent N5181B JGW-T1706762

    • Current use: fFSS, fIMC, ISS AOM, f1, fALSX at UToyama, spare at Ando-Lab
    • Possible use in near future: fPMC, fFSS, fIMC, fALSX, fALSY, ALS AOM, ISS AOM, f1, f2, f3
      • buy new RF signal generators for fPMC and fFSS?
    • Final use: fPMC, fFSS, fIMC, fALSX, fALSY, f1/f2/f3 with harmonics generator
      • Use AOM drivers for ALS AOM and ISS AOM
• IMMT1 and IMMT2 transmission [Michimura, Takeda]
  • IMMT2 transmission optics are too much squeezed
• DC QPD holder [Michimura]

  • beam height should be 4inch to use similar mount, with small modification of spacer (instead of 3inch in JGW-D1402607)

    • RF PD, RF QPD boxes are designed for 4inch beam height
  • stages are not needed for ISC DC QPD

  • design new ones; they can be very simple [-> Michimura?]

  • calibration can be done in different ways
  • put strain relief and anchors for cables to protect QPD board
• OMC and OFI [Somiya]
  • look for OFI with larger aperture [Somiya]
  • DC PD and DC QPD [Michimura]
    • DC PD not available. Look for product with similar specs
    • DC QPD available from RS

• In-vacuum RF PD and RF QPD

  • we need them within 1 year, considering OMC REFL and AS RF

• In-vac beam-dumps

  • required spec?
• Actuator noise modeling [Michimura,Miyamoto]

  • Summarized in the paper JGW-P1707051

  • Needs to implement frequency noise, but FSS modeling with ALS is complicated [student!]

  • Discuss mirror vibration from heat link

    • Meeting on July 14 [Yamada, Miyamoto, Ushiba, Michimura]

See this page for other agendas. KAGRA/subgroup/ifo/MIF/Minutes20181105について、ここに記述してください。