JGW-T1910359-v1
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ASC simulations for O3 SRM transmission, SRC Gouy phase shift and ITM transmission asymmetry
Document #:
JGW-T1910359-v1
Document type:
T
Submitted by:
Yuta Michimura
Updated by:
Yuta Michimura
Document Created:
20 Jun 2019, 13:10
Contents Revised:
21 Jun 2019, 13:21
Metadata Revised:
21 Jun 2019, 13:21
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JGW-T1910359-v1
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JGW-T1910359-v0
21 Jun 2019, 11:09
Abstract:
Report on the effects of O3 SRM transmission, SRC Gouy phase shift and ITM transmission asymmetry to ASC sensing noise.
Optickle simulation for the following configurations were done:
* Nominal BRSE at the time of Aso 2013 (PRM input power 77.5 W), but with T_PRM = 10.35%
https://journals.aps.org/prd/abstract/10.1103/PhysRevD.88.043007
https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=5744
* Nominal BRSE with updated PRM input power to 65 W (670 W at BS)
https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=7038
* BRSE with T_SRM=30%, PRM input power 1 W (O3 SRM transmission, 10 W at BS)
* BRSE with T_SRM=30%, PRM input power 1 W, SRC one-way Gouy phase 48deg/2 (by changing SR2-SR3 length by +4 cm)
https://klog.icrr.u-tokyo.ac.jp/osl/?r=9246
* BRSE with T_SRM=30%, PRM input power 1 W, SRC one-way Gouy phase 48deg/2, T_ITMX=0.444%, T_ITMY=0.479%
https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=10352
Files in Document:
ASCShotNoiseforO3.pdf
(1.2 MB)
ASCShotNoiseforO3.ppt
(1.5 MB)
Topics:
Activity
:
KAGRA
Detector
:
Interferometer Sensing and Control
:
Alignment Sensing and control
Authors:
Yuta Michimura
Keywords:
O3
optickle
simulation
ASC
ISC
MIF
Related Documents:
JGW-L1605744:
Acceptance for PRM transmission 10.35 %
JGW-T1707038:
Latest estimated sensitivity of KAGRA (v201708) *APPROVED*
JGW-T1910352:
On the effect of arm cavity finesse asymmetry to O3 sensitivity
JGW-G1301664:
WFS信号への要求値
Referenced by:
JGW-G1910807:
Report on Simulation Studies on Interferometer Configuration for O3
Approved for use in external presentations:
Unapproved
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