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Comment:
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Deletions are marked like this. | Additions are marked like this. |
Line 5: | Line 5: |
* Sadakazu Haino(Chair), Chunglee Kim, Kentaro Komori, Yuta Michimura, Matteo Leonardi, Atsushi Nishizawa, RDC chair | * Sadakazu Haino(Chair), Chunglee Kim, Kentaro Komori, Yuta Michimura, Matteo Leonardi, Atsushi Nishizawa, Kentaro Somiya(PRDC chair) |
Line 32: | Line 32: |
* population (parameter estimation) [DA: Hideyuki Tagoshi?] * host galaxy identification (sky localization) [DA: Hideyuki Tagoshi?] |
* population (parameter estimation) [Chunglee Kim] * host galaxy identification (sky localization) [Chunglee Kim] |
Line 36: | Line 36: |
* polulation (parameter estimation) [DA: Hideyuki Tagoshi?] | * polulation (parameter estimation) [Chunglee Kim] |
Line 40: | Line 40: |
* population (parameter estimation) [DA: Hideyuki Tagoshi?] * NS EOS and tidal deformation [Masaru Shibata?] * NS remnant [Masaru Shibata?] * kilonova [Masaru Shibata?] * short gamma-ray burst [Kunihito Ioka?] * stocastic background |
* population (parameter estimation) [Chunglee Kim] * NS EOS and tidal deformation [Masaru Shibata] * NS remnant [Masaru Shibata] * kilonova [Masaru Shibata] * short gamma-ray burst [Kunihito Ioka] |
Line 47: | Line 46: |
* low-mass x-ray binaries [Albert Kong?] | * low-mass x-ray binaries [Albert Kong] |
Line 49: | Line 48: |
* pulsar ellipticity (continuous) [Yousuke Itoh?] * pulsar glitches (burst) [Yousuke Itoh?] * magnetar flare [Yasufumi Kojima?] * stellar oscillation [Hajime Sotani?] |
* pulsar ellipticity (continuous) [Yousuke Itoh] * pulsar glitches and magnetar flare [Yasufumi Kojima] * stellar oscillation [Hajime Sotani] |
Line 54: | Line 52: |
* explosion models [Kei Kotake?] * distinguishing explosion models (parameter estimation) [DA: Kazuhiro Hayama?] |
* explosion models [Kei Kotake] * distinguishing explosion models (parameter estimation) [Kazuhiro Hayama] |
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* test of consistency with GR [Tjonnie G. F. Li?] * generation mechanism [Takahiro Tanaka?] |
* test of consistency with GR [Tjonnie G. F. Li] * generation mechanism [Takahiro Tanaka] |
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* BH no-hair theorem [Hiroyuki Nakano?] | * BH no-hair theorem [Hiroyuki Nakano] |
Line 75: | Line 73: |
* fast radio burst [Kazumi Kashiyama?] | * fast radio burst [Kazumi Kashiyama] |
Line 78: | Line 76: |
* BH echo [Takahiro Tanaka?] | * BH echo [Takahiro Tanaka] |
Future Planning Committee (FPC) working wiki
Overview
FPC is approved under KSC in Dec/2018 with the following initial members:
- Sadakazu Haino(Chair), Chunglee Kim, Kentaro Komori, Yuta Michimura, Matteo Leonardi, Atsushi Nishizawa, Kentaro Somiya(PRDC chair)
- Any comments/questions/requests from anyone are much appreciated and can be sent to the dedicated Mailing List
- ksc-fpc _at_ icrr.u-tokyo.ac.jp
Starting points
LIGO-Virgo white papers
LIGO Instrument science white paper (2017): LIGO-T1700231–v2
LIGO Instrument science white paper (2018): LIGO-T1800133–v3
The LSC-Virgo White Paper on Gravitational Wave Data Analysis and Astrophysics (July 2017 edition): LIGO–T1700214-v4 VIR-0435D-17
The LSC-Virgo White Paper on Gravitational Wave Data Analysis and Astrophysics (Summer 2018 edition): LIGO–T1800058-v2 VIR-0119B-18
Draft of white paper
Link to Overleaf: https://www.overleaf.com/project/5c091fbd8795b4614778100c
Link to Dropbox (backup): https://www.dropbox.com/sh/ry8x2x5wco4xbxx/AAAy782OD9Mhbca7Cov0Ws5Oa?dl=0
White paper plan
- Scientific motivation
- Stellar-mass BBH
- formation scenarios [Kohei Inayoshi]
- population (parameter estimation) [Chunglee Kim]
- host galaxy identification (sky localization) [Chunglee Kim]
- Intermediate-mass BBH
- formation scenarios [Kohei Inayoshi]
- polulation (parameter estimation) [Chunglee Kim]
- intermediate mass-ratio binaries [Norichika Sago?]
- BNS and BHNS
- binary evolution [Chunglee Kim]
- population (parameter estimation) [Chunglee Kim]
- NS EOS and tidal deformation [Masaru Shibata]
- NS remnant [Masaru Shibata]
- kilonova [Masaru Shibata]
- short gamma-ray burst [Kunihito Ioka]
- Accereting binaries
- low-mass x-ray binaries [Albert Kong]
- Isolated NS
- pulsar ellipticity (continuous) [Yousuke Itoh]
- pulsar glitches and magnetar flare [Yasufumi Kojima]
- stellar oscillation [Hajime Sotani]
- Supernova
- explosion models [Kei Kotake]
- distinguishing explosion models (parameter estimation) [Kazuhiro Hayama]
- polarization [Kazuhiro Hayama]
- Cosmic string
- burst signal [Sachiko Kuroyanagi]
- stochastic background [Sachiko Kuroyanagi]
- parameter estimation [Kipp Cannon?]
- Stochastic background
- inflation models [Jun'ichi Yokoyama?]
- phase transition [Shinya Kanemura?]
- astrophysical background [??]
- spectral shape (parameter estimation) [Sachiko Kuroyanagi]
- Test of gravity
- test of consistency with GR [Tjonnie G. F. Li]
- generation mechanism [Takahiro Tanaka]
- propagation effect [Atsushi Nishizawa]
- polarization [Hiroki Takeda]
- BH no-hair theorem [Hiroyuki Nakano]
- Cosmology
- Hubble constant measurement [Atsushi Nishizawa]
- Multimessenger
- fast radio burst [Kazumi Kashiyama]
- long gamma-ray burst [Ryo Yamazaki?]
- Others
- BH echo [Takahiro Tanaka]
- Stellar-mass BBH
- Survey of the current technologies (price and readiness)
- High power laser (how much power? stability?) [Haino?]
- Parametric instabilty vs power, mitigation schemes [Michimura? KYamamoto?]
- Squeezing (squeezing level, losses) [Matteo, Eleonora]
- Filter cavity (losses) [Matteo, Eleonora]
- Mirror (mass, coating, absorption) [Hirose?]
- Suspending larger mirror [Okutomi?]
- Suspension design for suspension thermal noise reduction (upper stage masses, sapphire blades, ribbon design) [Tomaru?]
- Improving heat conductivity of sapphire fibers [Tomaru?]
- Extreme RSE (high SRM reflectivity possible?) [Michimura?]
- Technological noises at low frequencies [Michimura?]
- Newtonian noise cancellation [Nishizawa?]
- QND, quantum locking [KNagano]
- Technologies to accerelate commissioning work (e.g. machine learning for auto alignment)
- Technologies to improve stability
- Technologies to improve duty cycle
- Technologies to reduce calibration error
- Status of the current facility
- TUN
- FCL
- VAC
- CRY [Tomaru]
- VIS [Takahashi, Aso]
- MIR [Hirose]
- LAS [Mio]
- IOO [Kokeyama, Somiya]
- AOS [Akutsu]
- ...
- Limits of the current facility
- Mirror size in cryostat [KYamamoto?]
- Filter cavity length [Matteo, Eleonora]
- Computing resources [Chunglee?]
- Trade-off studies
- Time scale of plans: near-term(more realistic) and longer-term(some dreams)
- Back up plans
R&Ds to be done : input to the PRDC
- Budget estimate
- Project execution plan
Schedule for the white paper
- Work in progress draft to be presented @ KIW in Feb 2019 : Feedbacks from Virgo
- First draft to be circulated @ April 2019 F2F
- Final version to be put for approval @ Aug 2019 F2F