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= GW research exchange meeting =
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== 重力波研究交流会とは? ==
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 * [[gw_talks/what_is|重力波研究交流会とは?]]  * [[gw_talks/what_is|What is GW REM? (重力波研究交流会とは?)]]
 * [[#UsefulLinks | Useful Links ]]
 * [[#HowToAnnouncements | How to receive announcements ]]
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<<BR>>
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== Upcoming GW-REMs ==
----
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== 次回の重力波研究交流会 ==
== The past GW REM talks ==
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=== 第78回 2015年8月21日(金) ===

----

 * 場所 東大安東研

 * 時間 13:00-14:00

 * Talk : 井上優貴 (KEK)
  *「宇宙マイクロ波背景放射実験POLARBEARの結果と現状」

 * Seevogh 接続情報
  * Title: JGW monthly seminar
  * Community: Virgo - LSC
  * Password: 案内メールを参照のこと
  * Meeting Access Information:
<<Include(gw_talks/archive_121_130)>>
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== 過去の重力波研究交流会 ==
----
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=== 第77回 2015年7月24日(金) ===
== Archives for the past talks ==
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 * 場所 国立天文台

 * 時間 13:00-15:00

 * 登壇者1:Mark Barton (国立天文台)
  * タイトル: "Suspension Dynamics Modeling for LIGO and KAGRA"[[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=3768|発表ファイル]]
  * 概要: A description of work I did on suspension dynamics modeling at LIGO with particular emphasis on its relation to Sekiguchi-san's adaptation and other things that will be needed for KAGRA.

 * 登壇者2:Manuel Marchio (東大天文D1)
  * タイトル: "Bayesian approach to the locking problem for high-finesse optical cavities"[[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=3863|発表ファイル]]
  * 概要 : To Be Announced

 * Seevogh 接続情報
  *Title:
  *Community: Virgo - LSC
  *Password: 案内メールを参照のこと
  *Meeting Access Information:



=== 第76回 2015年5月8日(金) ===

----

 * 場所 東大宇宙線研

 * 時間 13:00-15:00

 * Talk1: James Quach(物性研究所)「Gravitational Casimir Effect」[[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=3531|発表ファイル]]

 * Talk2: 小野謙次(宇宙線研究所)「New estimation method for mass of an isolated neutron star using gravitational waves」[[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=3535|発表ファイル]]



 * Seevogh 接続情報
  *Title:JGW monthly seminar
  *Community: Virgo - LSC
  *Password: 案内メールを参照のこと
  *Meeting Access Information:


=== 第75回 2015年4月24日(通常より1時間遅いスタートとなります。) ===

----

 * 場所 東工大宗宮研

 * 時間 14:00-16:00

 * Talk1: 矢野和城 (宗宮研M2)
  *「宗宮研でやっている実験レビュー (信号増幅を中心に)」[[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=3511|発表ファイル]]

 * Talk2: 橘優太朗 (河合研M2)
  *「光子で探る活動銀河核(時系列解析を中心に)」[[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ProcessDocumentAdd|発表ファイル]]

 * Seevogh 接続情報
  *Title: JGW monthly seminar
  *Community: Virgo - LSC
  *Password: 案内メールを参照のこと
  *Meeting Access Information:
    *SeeVoghRN Application http://research.seevogh.com/joinSRN?meeting=M9MIMi222iDeDi999iDD99
    *Mobile App : Meeting ID: 727 4165 or Link: http://research.seevogh.com/join?meeting=M9MIMi222iDeDi999iDD99



=== 第74回 2015年2月20日(金) ===
----

 * 場所 東大三尾研

 * 時間 13:00-15:00

 * Talk1: 水谷彬(三尾研M1)
  *「フェムト秒レーザーによるCFRPのレーザー加工」[[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=3332|発表ファイル]]
 * Seevogh 接続情報
  *Title: JGW monthly seminar
  *Community: Virgo - LSC
  *Password: 案内メールを参照のこと
  *Meeting Access Information:
    *SeeVoghRN Application http://research.seevogh.com/joinSRN?meeting=M9MIMi222iD2D29I99DD99
    *WebStart (Java) http://research.seevogh.com/join?meeting=M9MIMi222iD2D29I99DD99
    *Mobile App : Meeting ID: 721 8680 or Link: http://research.seevogh.com/join?meeting=M9MIMi222iD2D29I99DD99




=== 第73回 2015年1月23日(金)〜冬のIMC祭り〜 ===
----

 * 場所 Seevogh上

 * 時間 13:00-15:00

 * Talk1:苔山圭以子(Louisiana State Univ.)
  *「aLIGO (LLO) IMC Overview」[[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB//ShowDocument?docid=3258|発表ファイル]]

 * Talk2:中野雅之(宇宙線研)
  *「Installation of KAGRA PSL table」[[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=3256|発表ファイル]]

 * Talk3:斉藤高大(新潟大)
  *「KAGRA IMC suspension report」[[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=3257|発表ファイル]]

 * Seevogh 接続情報
  *Title: JGW monthly seminar
  *Community: Virgo - LSC
  *Password: 案内メールを参照のこと
  *Meeting Access Information:
    *SeeVoghRN Application http://research.seevogh.com/joinSRN?meeting=MsMiMI2l2eDMDv9n9aDt9s
    *WebStart (Java) http://research.seevogh.com/join?meeting=MsMiMI2l2eDMDv9n9aDt9s
    *Mobile App : Meeting ID: 719 6573 or Link: http://research.seevogh.com/join?meeting=MsMiMI2l2eDMDv9n9aDt9s



=== 第72回 2014年12月19日(金) ===
----

 * 場所 東大宇宙線研

 * 時間 13:00-15:00

 * Talk1:土井康平(宇宙線研究所) 発表資料:なし

 * Talk2:和泉究(LIGO ハンフォード)[[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=3117|発表資料]]

 * Seevogh (evo) 接続情報
  *Title: JGW Monthly Seminar
  *Community: Virgo-LSC
  *Password: アナウンスメールを参照して下さい。
  *Meeting Access Information:



=== 第71回 2014年11月21日 ===
----

 * 場所 東京大学安東研

 * 時間 13:00-15:00

 * Talk1: 宇佐見康二(東大先端研)
  *「光-マグノン-マイクロ波-超伝導量子ビットのリンクあるいは量子ピタゴラスイッチ」 [[http://gwdoc.icrr.u-tokyo.ac.jp/DocDB/0030/G1403012/001/2014_11_21_Hongo_n.pdf| 発表資料]]

 * Talk2: 和泉究(LIGO Hanford)
  *「LIGO Hanford での signal recycling cavity 内 mode hop 問題について(仮)」 [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=2995| 発表資料]]

 * Seevogh (evo) 接続情報
  *Title: JGW Monthly Seminar(true)
  *Community: Virgo - LSC
  *Password: アナウンスメールを参照してください。
  *Meeting Access Information:
   *SeeVoghRN Application http://research.seevogh.com/joinSRN?meeting=MMMeMn2D2iDMDu929lD29M
   *WebStart (Java) http://research.seevogh.com/join?meeting=MMMeMn2D2iDMDu929lD29M
   *Mobile App : Meeting ID: 713 3002 or Link: http://research.seevogh.com/join?meeting=MMMeMn2D2iDMDu929lD29M
 * Most of the archives for the earlier years are written in Japanese (it is a history!).
  . {i} [[gw_talks/archive_121_130|121-130th GW-REM talks (2024-)]]
  . {i} [[gw_talks/archive_111_120|111-120th GW-REM talks (2023-2024)]]
  . {i} [[gw_talks/archive_101_110|101-110th GW-REM talks (2019-2022)]]
  . {i} [[gw_talks/archive_91_100|91-100th GW-REM talks (2017-2019)]]
  . {i} [[gw_talks/archive_81_90|81-90th GW-REM talks (2016-2017) ]]
  . {i} [[gw_talks/archive_71_80|71-80th GW-REM talks (2014-2015) ]]
  . {i} [[gw_talks/archive_61_70|61-70th GW-REM talks (2013-2014) ]]
  . {i} [[gw_talks/archive_51_60|51-60th GW-REM talks (2012-2013) ]]
  . {i} [[gw_talks/archive_41_50|41-50th GW-REM talks (2011-2012) ]]
  . {i} [[gw_talks/archive_31_40|31-40th GW-REM talks (2010-2011) ]]
  . {i} [[gw_talks/archive_21_30|21-30th GW-REM talks (2009-2010) ]]
  . {i} [[gw_talks/archive_11_20|11-20th GW-REM talks (2008-2009) ]]
  . {i} [[gw_talks/archive_1_10|1-10th GW-REM talks (2007-2008) ]]
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== これ以前の重力波研究交流会 ==
<<Anchor(UsefulLinks)>>
== Useful links ==
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 * [[JGWDoc/HowTo/UpLoadE| How to upload presentation materials to JGW doc database]]
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    {i} [[gw_talks/archive_61_70|第61回~第70回重力波研究交流会]]  * [[ZoomHowTo | How to use Zoom]]
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    {i} [[gw_talks/archive_51_60|第51回~第60回重力波研究交流会]]  * [[LCGT/Meeting/EVOJ| Use of EVO remote connection system (written in Japanese) ]]
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    {i} [[gw_talks/archive_41_50|第41回~第50回重力波研究交流会]]

    {i} [[gw_talks/archive_31_40|第31回~第40回重力波研究交流会]]

    {i} [[gw_talks/archive_21_30|第21回~第30回重力波研究交流会]]

    {i} [[gw_talks/archive_11_20|第11回~第20回重力波研究交流会]]

    {i} [[gw_talks/archive_1_10|第1回~第10回重力波研究交流会]]
 * [[howtouseezuce| How to join KEK community in eZuce]]
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== 暮らしに役立つリンク == <<Anchor(HowToAnnouncements)>>
== How to receive the announcements ==
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 * [[JGWDoc/HowTo/UpLoad | 資料の upload の仕方]]

 * [[LCGT/Meeting/EVOJ| EVO遠隔会議システムの使い方あれこれ]]
 . /!\ One has to subscribe to the mailing list called ''gw_comm'' in order to receive our announcement emails. Please ask one of our organizers for subscription.
 . The organizers can be found in [[gw_talks/what_is|this page]].

SRMface_small.jpg

重力波研究交流会

GW research exchange meeting



Upcoming GW-REMs



The past GW REM talks


back to top page

The 121-130th REM talks


The 127th REM: Dec 10th, 2024


  • Time: 11:00-12:00
  • Speaker: Kazuhiro Agatsuma (EX-Fusion Inc.)
    • Title: "A career path from gazing star to making star"

      • Abstract:
        I show my career path from the field of gravitational waves (GWs) to the field of laser inertial fusion energy (IFE). I have worked on several projects in the GW community for 16 years, for example, TAMA300, CLIO, KAGRA, Ad-Virgo, and Ad-LIGO. The study subjects were broad; seismic attenuation system, pendulum thermal noise, radiation pressure noise, phase camera, and the expansion of the universe. The pandemic caused serious damage in my career, but gave me a chance to challenge another field (IFE). 
        In addition, I show my recent work in EX-Fusion Inc. that is a startup company in Japan. Our goal is to realize a commercial laser fusion reactor. In the future reactor a highly repetitive operation is essential to generate sufficient energy. The fuel targets must be illuminated by the laser spot continuously. However, the target injection system has a limited precision, which causes the target trajectories to fluctuate. The fusion rate can be degraded by a mismatch at the engagement point. We have demonstrated a laser target tracking system to solve this issue. A continuous illumination of targets by 10-Hz operation has been achieved by a controlled mirror. Recently, we have upgraded this system by a new steering mirror, which has a local control system with techniques of GW detectors. 

The 126th REM: Oct. 31st, 2024


  • Time: 11:00-12:00
  • Speaker: Kazuya Kobayashi (ICRR)
    • Title: "Parameter Estimation from Gravitational-wave Data Generated by Compact Binary Coalescences"

      • Abstract:
        Bayesian inference is used to estimate parameters such as masses and spins from gravitational wave data generated by compact binary coalescences.
        This method allows us to calculate the posterior probability distribution of the parameters.
        However, since analytical computation in Bayesian inference is difficult, numerical methods such as MCMC sampling are employed.
        In this talk, I will introduce parameter estimation methods, summarize LIGO-Virgo-KAGRA collaboration results, and present my research on parameter estimation.

The 125th REM: Oct 8th, 2024


  • Time: 14:00-15:00
  • Speaker: Satoru Takano (AEI)
    • Title: "Torsion pendulum detector towards gravity gradient detection"

      • Abstract:
        Torsion pendulum detector is proposed as a ground-based gravitational wave detector focusing on the 0.1 Hz frequency band [1]. The detector, TOBA (TOrsion-Bar Antenna), consists of two perpendicular torsion pendulums and the small stiffness of the torsion pendulum enables the detector to respond to gravitational waves in low frequencies. The target of TOBA is to observe GWs from IMBH binaries with 10 m bars. To demonstrate the measurement principle and establish necessary techniques, our group has developed small prototypes for more than 10 years. Now we are developing a prototype, Phase-III TOBA.
        Phase-III TOBA is a big milestone towards the final detector. One of the key features is the cryogenic technique for reduction of thermal noises. Recently, we have demonstrated the cryogenic torsion pendulum cooled down to 6 K[2] and the monolithic readout system made of silicon[3]. I will introduce our TOBA experiment and talk about recent progress.
        
        [1] M. Ando et al., PRL, 105, 161101 (2011)
        [2] T. Shimoda, Ph.D Thesis, The University of Tokyo (2020)
        [3] S. Takano, Ph.D Thesis, The University of Tokyo (2024)

The 124th REM: September 5th, 2024


  • Time: 11:00-12:00
  • Speaker: Ish Gupta (Penn State)
    • Title: "Expectations and Challenges on the Path to the Next-Generation of Gravitational-Wave Discovery"

      • Abstract:
        The current generation of gravitational-wave detectors have detected close to two hundred binary mergers. These detect ions have imposed constraints on astrophysical populations of binaries, alternate theories of general relativity, cosmological parameters, and the equation of state of the neutron star. Notably, these achievements have been realized despite significant challenges, such as limited localization for most events and the rarity of confidently detected neutron star binaries. Thus, to extract the full potential of gravitational-wave astronomy, bigger and more sensitive detectors are needed. This need will be fulfilled with the Cosmic Explorer and the Einstein Telescope observatories, which are intended to be significantly more sensitive than the current generation. Such observatories will not only increase the number of detections by orders of magnitude, they will also allow for precise estimation of parameters, leading to an era of precision cosmology, refined astrophysical inference and optimized targeted electromagnetic follow-up. In this talk, I will highlight some of these science objectives that will be accomplished by next-generation detectors and address the challenges that must be overcome to realize these objectives, underscoring the importance of concerted efforts in advancing gravitational-wave astronomy.

The 123rd REM: Jul 30th, 2024


  • Time: 15:00-16:00
  • Speaker: Taichi Kawamura (Institut de Physique du Globe de Paris)
    • Title: "Seismic Environment of the Moon"

      • Abstract:
        Abstract: More than 50 years after the first landing on the Moon, lunar exploration has once again become a global trend. In the past decade alone, over eight successful lunar landings have been completed, reflecting a growing scientific interest in the Moon. While lunar science remains a primary focus, the potential to utilize the Moon as a natural laboratory for physics and astrophysics is also being explored. Recently proposed experiments include a lunar-based radio astronomy space telescope and a gravitational wave detector. For such projects to be feasible, it is essential to thoroughly understand the Moon's environment, particularly its seismic activity and associated risks. Observations from the Apollo missions have shown that the Moon remains seismically active, experiencing "moonquakes" almost daily. In this presentation, I will review the seismic data obtained from the Apollo experiments and discuss the Moon's seismic environment. I will conclude by highlighting key considerations for future lunar projects.

The 122nd REM: June 27th, 2024


  • Time: 11:00-12:00
  • Speaker: Prathamesh Joshi (Penn State)
    • Title: "How are gravitational-wave searches for compact binaries performing, and where are they headed?"

      • Abstract:
        During the fourth observing run of the LVK collaboration, we have already seen large improvements in the results produced by the CBC search pipelines in low-latency. We have reached new levels of sensitivity and reliability. In the quest to detect every gravitational wave out there, we are now more ready than ever to participate in the next multimessenger event. In this presentation, I will talk about how the searches work, and some recent search results we have seen in O4. As we start getting high-latency offline results, we will begin to explore gravitational waves from new parameter spaces. We are seeing advancements in searches for precessing binaries, higher order modes of gravitational waves, as well as unmodeled or burst searches. I will discuss how these improvements will play a crucial role in obtaining a better scientific understanding of some of the biggest mysteries of the universe.

The 121th REM: May 30th, 2024


  • Time: 11:00-12:00
  • Speaker: Kenta Tanaka (ICRR)
    • Title: "Introduction to laser interferometric GW telescope and Current status of KAGRA"

      • Abstract:
        Gravitational wave astronomy has made remarkable progress since its first detection in 2015. The Japanese gravitational wave telescope, KAGRA, is currently undergoing an upgrade to participate in the 4th International Joint Observations with LIGO (USA) and Virgo (Europe). In this talk, I will introduce gravitational waves and the telescopes used for their detection, and provide an update on the current status of KAGRA for new students.


Archives for the past talks





How to receive the announcements


  • /!\ One has to subscribe to the mailing list called gw_comm in order to receive our announcement emails. Please ask one of our organizers for subscription.

  • The organizers can be found in this page.

gw_talks (last edited 2024-12-10 16:39:02 by ryosuke.sugimoto)