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Revision 2 as of 2022-04-06 13:59:20
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Editor: YoichiAso
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Deletions are marked like this. Additions are marked like this.
Line 9: Line 9:
  * Parametric amplification of the OPO will increase the scattering noise coupling
   * It depends on the green pump power
   * The green pump power should be decided based on the trade-off between the amount of squeezing and anti-squeezing.
   * This trade-off depends on the loss of the interferometer
Line 10: Line 14:
  * Need to preserve the mode-shape after the reflection mirror
  * Need to reduce the beam size on the Faraday isolators
   * Clear aperture is 10mm
   * Beam radius should be below 1.6mm
  * Size and location of the vacuum tubes between the chambers should be taken into consideration
  * We should have in-vac PZT mirrors for alignment

KAGRA Filter Cavity Meeting 2022/4/6

Date/Time: 2022/4/6 13:00 - 14:00

Connection: KAGRA Zoom2 (https://zoom.us/j/6676627462)

Agenda

  • Scattering requirement for FIS (Michael)
    • Parametric amplification of the OPO will increase the scattering noise coupling
      • It depends on the green pump power
      • The green pump power should be decided based on the trade-off between the amount of squeezing and anti-squeezing.
      • This trade-off depends on the loss of the interferometer
  • How to switch FIS and FDS (HuaLi)

    • Need to preserve the mode-shape after the reflection mirror
    • Need to reduce the beam size on the Faraday isolators
      • Clear aperture is 10mm
      • Beam radius should be below 1.6mm
    • Size and location of the vacuum tubes between the chambers should be taken into consideration
    • We should have in-vac PZT mirrors for alignment
  • Status reports
    • Overall design: Matteo
    • Filter Cavity: Marc
    • FIS design: Yuhang
    • Filter Cavity Control: Aritomi, Michael

KAGRA/Upgrades/PostO4Upgrades/FilterCavity/Meetings/20220406 (last edited 2022-04-06 13:59:20 by YoichiAso)