O3 Estimated Sensivitiy for FPMI, PRFPMI and RSE

Document #:

JGW-T1808172-v1

Document type:

T

Submitted by:

Yuta Michimura

Updated by:

Yuta Michimura

Document Created:

20 Apr 2018, 16:41

Contents Revised:

20 Apr 2018, 17:10

DB Info Revised:

20 Apr 2018, 17:10

Abstract:

Estimated sensitivity for O3 in case of different IFO configutations with 10W, including the shot noise coupling with feedforward gain of 100.
IFO configurations considered here are:
- FPMI with tilted PRM (equivalent to 1W input power)
- FPMI with blank PRM
- PRFPMI (R_SRM=0 %)
- RSE with R_SRM=70 %
We also consider four excess noise models:
- No excess
- aLIGO O1 level
- 4x aLIGO O1 level (AdV O2 level)
- 8x aLIGO O1 level

Files in Document:

• O3Sensitivity_FPMI_PRFPMI_RSE.pdf (1.3 MB)
• O3Sensitivity_FPMI_PRFPMI_RSE.ppt (1.4 MB)

Topics:

• Detector:Interferometer Sensing and Control
• Activity:KAGRA

Authors:

• Yutaro Enomoto
• Yuta Michimura

Keywords:

O3 sensitivity FPMI PRFPMI RSE DRFPMI MIF ISC LSC

Related Documents:

• JGW-T1808126: PRFPMI or RSE for Joining O3
• JGW-T1707334: Main Interferometer Configuration for Early Phase of bKAGRA
• JGW-G1707479: Signal Recycling Mirror Reflectivity
• JGW-G1807693: 大型低温重力波望遠鏡 KAGRA の初期観測へむけた主干渉計制御

Referenced by:

• JGW-T1809078: *APPROVED* KAGRA Sensitivity for Observation Scenario Paper 2018
• JGW-G1910807: Report on Simulation Studies on Interferometer Configuration for O3
• JGW-G1910828: Summary of Sensitivity Estimate for O3 in Various Interferometer Configurations
• JGW-G2011541: Discussion on Interferometer Configuration for O4