Size: 582
Comment:
|
Size: 7197
Comment:
|
Deletions are marked like this. | Additions are marked like this. |
Line 1: | Line 1: |
= ISC Meeting on 2020/06/15 14:00 - 15:00 = Participants: |
= ISC Meeting on 2020/06/15 12:30 - 13:30 = Participants: Haoyu Wang, Eleonora Caposcasa, Hiro Yamamoto, Keiko Kokeyama, Kentaro Somiya, Kiwamu Izumi, Koji Arai, Koji Nagano, Masayuki Nakano, Ryutaro Takahashi, Tomotada Akutsu, Yoichi Aso, Yubo Ma, Yuta Michimura |
Line 4: | Line 4: |
Zoom meeting: https://zoom.us/j/6676627462 | Zoom meeting: https://zoom.us/j/7631499341 Time: https://www.timeanddate.com/worldclock/meetingdetails.html?year=2020&month=6&day=15&hour=3&min=30&sec=0&p1=248&p2=237&p3=4399&p4=137 |
Line 15: | Line 17: |
* New members * Haoyu Wang (University of Shanghai for Science and Technology) [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=11697|JGW-G2011697]] * Yubo Ma (Shanxi Datong University) [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=11696|JGW-G2011696]] |
|
Line 16: | Line 22: |
* [[LCGT/subgroup/ifo/MIF/OptParam|Optical parameters]] | * List of optical parameters [[LCGT/subgroup/ifo/MIF/OptParam|OptParam]] |
Line 18: | Line 24: |
* Interferometer design paper [[https://journals.aps.org/prd/abstract/10.1103/PhysRevD.88.043007|Phys. Rev. D 88, 043007 (2013)]] * Latest KAGRA status paper [[https://arxiv.org/abs/2005.05574|arXiv:2005.05574]] * Summary of measurements related to the interferometer so far [[http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/subgroup/ifo/MIF/Minutes20200309|Minutes20200309]] * O4 schedule [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=9209|JGW-E1809209]] |
|
Line 19: | Line 29: |
* Interferometer issues we have now | * Interferometer issues which require simulation studies * ITMs have different transmission (ITMX: 0.444 % ITMY: 0.479%) [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/ShowDocument?docid=10352|JGW-T1910352]] * ITMs have inhomogeneity [[https://doi.org/10.1103/PhysRevD.100.082005|Phys. Rev. D 100, 082005 (2019)]] * ITMs have inhomogeneous birefringence [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/ShowDocument?docid=10369|JGW-G1910369]], [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/ShowDocument?docid=10388|JGW-G1910388]], [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/ShowDocument?docid=11633|JGW-T2011633]] * So far no success in locking DRFPMI [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=11693|JGW-G2011693]] * WFS not working well [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=11687|JGW-G2011687]] * Laser intensity and frequency noise couplings are too high [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=11662|JGW-T2011662]] * Carrier power recycling gain for PRMI (roughly 3) and PRFPMI (11-12) are too different, which could be due to the Lawrence effect [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/ShowDocument?docid=11633|JGW-T2011633]] |
Line 22: | Line 39: |
* LSC simulations with Optickle originally by Yoichi Aso https://granite.phys.s.u-tokyo.ac.jp/svn/LCGT/trunk/mif/IFOmodel * Used for designing the interferometer, and deriving requirements [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/ShowDocument?docid=913|JGW-T1200913]] * Simulations for O3 by Yutaro Enomoto [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=10341|JGW-T1910341]] * Mach-Zehnder modulator simulations by Kohei Yamamoto [[https://doi.org/10.1088/1361-6382/ab4489|Classical and Quantum Gravity 36, 205009 (2019)]] * ASC simulations with Optickle originally by Yuta Michimura https://granite.phys.s.u-tokyo.ac.jp/svn/LCGT/trunk/mif/ASC-Optickle * Used for designing the interferometer [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/ShowDocument?docid=913|JGW-T1200913]] * Simulations for O3 by Yuta Michimura [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/ShowDocument?docid=10359|JGW-T1910359]] * FINESSE model originally by Kentaro Somiya [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/ShowDocument?docid=2434|JGW-T1402434]] (any updated version?) * Used for OMC design [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=8043|JGW-T1808043]], [[https://link.springer.com/article/10.1007/s10043-015-0028-2|Optical Review 22, 149-152 (2015)]], [[https://iopscience.iop.org/article/10.1088/1742-6596/957/1/012009|J. Phys.: Conf. Ser. 957, 012009 (2018)]] * ITM inhomogeneity effects [[https://doi.org/10.1103/PhysRevD.100.082005|Phys. Rev. D 100, 082005 (2019)]] * Also being used for simulating birefringence effects by Keiko Kokeyama [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/ShowDocument?docid=10461|JGW-G1910461]], [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/ShowDocument?docid=10380|JGW-T1910380]] * Parametric instability by Kiichi Kaihotsu, Kazuhiro Yamamoto * Activities in University of Toyama using COMSOL [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/ShowDocument?docid=10382|JGW-E1910382]] * Thermal lensing by Kentaro Somiya ? * Thermal lensing in cryogenic sapphire mirrors should be small (orders of magnitude smaller than room temperature fused silica) * Thermal lensing in room temperature fused silica BS needs investigation * Rough estimation by Hiroaki Yamamoto shows it is OK-ish, comparing the result with aLIGO * Further investigation necessary (also for future higher power) |
|
Line 24: | Line 59: |
* LSC and ASC simulations with current ITMs and current interferometer setup * Especially LSC simulations not done for PRFPMI and DRMI, and 3f locking * Compare measured LSC and ASC sensing matrices with simulations * Compare measured recycling gain (for carrier and sidebands) with simulations * Compare measured AS mode content with simulations * Compare measured MICH/PRCL/SRCL controls noise coupling with simulations * Compare measured intensity/frequency noise coupling with simulations * Thermal lensing in BS * Measurements necessary to do simulation work * PRC (SRC) length and Gouy phase * Schnupp asymmetry * modulation depth (arm cavity scan) * arm cavity length (arm cavity scan) * arm cavity round-trip loss measurement with birefringence effect correctly taken into account (with PBS at POP/POS and TRX/TRY) [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=11633|JGW-T2011633]] * Power recycling gain for carrier and sidebands * Throughput from IMC output to AS RF, OMC DC, REFL, POP, TRX, TRY * Measurements necessary to compare the result with simulation * frequency/intensity noise coupling, down to ~10 Hz * Measure power recycling gain for sidebands (POP 2f with FPMI locked and PRFPMI locked) * DRFPMI LSC and ASC sensing matrix * LSC https://klog.icrr.u-tokyo.ac.jp/osl/?r=14515 * MICH/PRCL/SRCL to DARM coupling * Measure MICH contrast defect with MICH locked and FPMI locked * OMC cavity scan to scan mode content of AS beam * https://docs.google.com/spreadsheets/d/1w4q8OvX9E6nkYSgshLYLoZH5yvQXHvGmL1agux8ztx0/edit#gid=0 * Type-A, B, Bp actuation efficiency measurements (for actuator noise) |
ISC Meeting on 2020/06/15 12:30 - 13:30
Participants: Haoyu Wang, Eleonora Caposcasa, Hiro Yamamoto, Keiko Kokeyama, Kentaro Somiya, Kiwamu Izumi, Koji Arai, Koji Nagano, Masayuki Nakano, Ryutaro Takahashi, Tomotada Akutsu, Yoichi Aso, Yubo Ma, Yuta Michimura
Zoom meeting: https://zoom.us/j/7631499341
Next meeting
TBD
Minutes
Agenda
- New members
Haoyu Wang (University of Shanghai for Science and Technology) JGW-G2011697
Yubo Ma (Shanxi Datong University) JGW-G2011696
- Useful links to know KAGRA interferometer design and status
List of optical parameters OptParam
MIF Design document JGW-T1200913
Interferometer design paper Phys. Rev. D 88, 043007 (2013)
Latest KAGRA status paper arXiv:2005.05574
Summary of measurements related to the interferometer so far Minutes20200309
O4 schedule JGW-E1809209
- Interferometer issues which require simulation studies
ITMs have different transmission (ITMX: 0.444 % ITMY: 0.479%) JGW-T1910352
ITMs have inhomogeneity Phys. Rev. D 100, 082005 (2019)
ITMs have inhomogeneous birefringence JGW-G1910369, JGW-G1910388, JGW-T2011633
So far no success in locking DRFPMI JGW-G2011693
WFS not working well JGW-G2011687
Laser intensity and frequency noise couplings are too high JGW-T2011662
Carrier power recycling gain for PRMI (roughly 3) and PRFPMI (11-12) are too different, which could be due to the Lawrence effect JGW-T2011633
- Status of simulation activities
LSC simulations with Optickle originally by Yoichi Aso https://granite.phys.s.u-tokyo.ac.jp/svn/LCGT/trunk/mif/IFOmodel
Used for designing the interferometer, and deriving requirements JGW-T1200913
Simulations for O3 by Yutaro Enomoto JGW-T1910341
Mach-Zehnder modulator simulations by Kohei Yamamoto Classical and Quantum Gravity 36, 205009 (2019)
ASC simulations with Optickle originally by Yuta Michimura https://granite.phys.s.u-tokyo.ac.jp/svn/LCGT/trunk/mif/ASC-Optickle
Used for designing the interferometer JGW-T1200913
Simulations for O3 by Yuta Michimura JGW-T1910359
FINESSE model originally by Kentaro Somiya JGW-T1402434 (any updated version?)
Used for OMC design JGW-T1808043, Optical Review 22, 149-152 (2015), J. Phys.: Conf. Ser. 957, 012009 (2018)
ITM inhomogeneity effects Phys. Rev. D 100, 082005 (2019)
Also being used for simulating birefringence effects by Keiko Kokeyama JGW-G1910461, JGW-T1910380
- Parametric instability by Kiichi Kaihotsu, Kazuhiro Yamamoto
Activities in University of Toyama using COMSOL JGW-E1910382
- Thermal lensing by Kentaro Somiya ?
- Thermal lensing in cryogenic sapphire mirrors should be small (orders of magnitude smaller than room temperature fused silica)
- Thermal lensing in room temperature fused silica BS needs investigation
- Rough estimation by Hiroaki Yamamoto shows it is OK-ish, comparing the result with aLIGO
- Further investigation necessary (also for future higher power)
- Simulation activities necessary
- LSC and ASC simulations with current ITMs and current interferometer setup
- Especially LSC simulations not done for PRFPMI and DRMI, and 3f locking
- Compare measured LSC and ASC sensing matrices with simulations
- Compare measured recycling gain (for carrier and sidebands) with simulations
- Compare measured AS mode content with simulations
- Compare measured MICH/PRCL/SRCL controls noise coupling with simulations
- Compare measured intensity/frequency noise coupling with simulations
- Thermal lensing in BS
- LSC and ASC simulations with current ITMs and current interferometer setup
- Measurements necessary to do simulation work
- PRC (SRC) length and Gouy phase
- Schnupp asymmetry
- modulation depth (arm cavity scan)
- arm cavity length (arm cavity scan)
arm cavity round-trip loss measurement with birefringence effect correctly taken into account (with PBS at POP/POS and TRX/TRY) JGW-T2011633
- Power recycling gain for carrier and sidebands
- Throughput from IMC output to AS RF, OMC DC, REFL, POP, TRX, TRY
- Measurements necessary to compare the result with simulation
- frequency/intensity noise coupling, down to ~10 Hz
- Measure power recycling gain for sidebands (POP 2f with FPMI locked and PRFPMI locked)
- DRFPMI LSC and ASC sensing matrix
- MICH/PRCL/SRCL to DARM coupling
- Measure MICH contrast defect with MICH locked and FPMI locked
- OMC cavity scan to scan mode content of AS beam
https://docs.google.com/spreadsheets/d/1w4q8OvX9E6nkYSgshLYLoZH5yvQXHvGmL1agux8ztx0/edit#gid=0
- Type-A, B, Bp actuation efficiency measurements (for actuator noise)