LCGT Meeting 12 October, 2010 Norikatsu Mio. Laser Discussion with Mitsubishi – Mitsubishi will offer their laser modules as a laser component and permit.

Slides:



Advertisements
Similar presentations
KIDS INSTITUTE. First Purpose  Bring in the district teachers.  Offer to 20 districts per year.  Launch the KIDS grant.  Train district teachers on.
Advertisements

Vibration Isolation Group R. Takahashi (ICRR)Chief T. Uchiyama (ICRR)Payload design H. Ishizaki (NAOJ)Prototype test R. DeSalvo (Caltech)SAS design A.
Participants: C-1:Cryogenic last-stage suspensions (interferometers) (F.Ricci-G.Frossati) Objectives: -Design new suspension elements for the last stage.
LIGO-G D Comments: Staged implementation of Advanced LIGO Adv LIGO Systems 17 may02 dhs Nifty idea: a way to soften the shock, spread cost, allow.
Application for KAGRA (LCGT) Membership Jun Xu, Jingya Wang, Lihe Zheng, Huili Tang Shanghai Institute of Ceramics, Chinese Academy of Sciences Shanghai.
LCGT Program Advisory Board (June , Kashiwa, Chiba) On behalf of LCGT special working group Masaki Ando (Department of Physics, Kyoto University)
Chapter 6 Product Design & Process Selection-Manufacturing
Laser &Optics of LCGT 2011/10/5(Wed) Norikatsu Mio Photon Science Center University of Tokyo EGO-ICRR Meeting 2011/10/4-5.
BS and Mirrors for the LCGT Norikatsu Mio, PSC Univ. of Tokyo Eiichi Hirose, ICRR Univ. of Tokyo December 13, 2011 CSIRO, Lindfield Australia.
Vibration Isolation R. Takahashi (ICRR), K. Yamamoto (ICRR), T. Uchiyama (ICRR), T. Sekiguchi (ICRR), H. Ishizaki (NAOJ), A. Takamori (ERI), R. DeSalvo.
1 New suspension study for LCGT Erina Nishida Ochanomizu University The Graduate School of Humanities and Sciences The Division of Advanced Sciences/ NAOJ.
SEO report _SAITO 1. Overall schedule of iKAGRA installation/commissioning change to Michelson Interferometer 2. Scheduling of daily works for installation.
Substrate mechanical loss studies Sheila Rowan (Stanford University) for: LIGO Laboratory (Caltech, MIT, LLO, LHO) LSC Partners (University of Glasgow,
Status of LCGT and CLIO Masatake Ohashi (ICRR, The University of TOKYO) and LCGT, CLIO collaborators TAUP2007 Sendai, Japan 2007/9/12.
Intermediate review - ERC – February 9, 2009 – L. Pinard 1 Mirrors Sub-System Overview  Introduction  Scope of the subsystem, main tasks  Job done since.
Test mass dynamics with optical springs proposed experiments at Gingin Chunnong Zhao (University of Western Australia) Thanks to ACIGA members Stefan Danilishin.
LCGT Cryogenics Status Report KEK T.Suzuki.
VIRGO_LCGT Meeting Laser & Mirror 5 November, 2010 Norikatsu Mio.
Current status of Laser development 2nd Korea - Japan Workshop on KAGRA 2012/5/28(Mon)
Ryutaro Takahashi (National Astronomical Observatory of Japan) Vibrtion isolation system for KAGRA The 6th Korea-Japan workshop on KAGRA NAOJ, June,
DFG-NSF Astrophysics Workshop Jun 2007 G Z 1 Optics for Interferometers for Ground-based Detectors David Reitze Physics Department University.
Simulation for KAGRA cryogenic payload: vibration via heat links and thermal noise Univ. Tokyo, D1 Takanori Sekiguchi.
LIGO-G D LIGO R&D1 Advanced LIGO R&D Review The PSL Peter King & Rich Abbott October 8, 2002.
1 K. Yamamoto, R. Takahashi, T. Sekiguchi, T. Uchiyama, H. Ishizaki A, A. Takamori B, R. DeSalvo C, E. Majorana D, LCGT collaboration ICRR, NAO A,ERI B,
LIGO Surf Project Q Of the Thermal Noise Interferometer Adam Bushmaker Mentor: Dr. Eric Black LIGO-G D.
LCGT Technical Review Suspension Point Interferometer for Parasitic Noise Reduction and an Additional IFO S.Miyoki (ICRR, Univ. of TOKYO)
1 Kazuhiro Yamamoto Institute for Cosmic Ray Research The university of Tokyo Current status KAGRA(LCGT) cryogenic payload meeting 8 February 2012.
Laser system for LCGT Norikatsu MIO.
Sapphire for the LCGT project Eiichi Hirose ICRR, University of Tokyo Kyohei Watanabe, Norikatsu Mio PSC, University of Tokyo GT Advanced Technology, Sep.
Low frequency anti-vibration system of LCGT Vibration Isolation Group R. Takahashi (ICRR), K. Yamamoto (ICRR), T. Uchiyama (ICRR), T. Sekiguchi (ICRR),
Aug. 2, 2010 Proposal for Creating New Task Force - To Develop 7-year Scenario for LCGT - Ichiro Nakatani Project Manager, LCGT 1.
Optical Spring Experiments With The Glasgow 10m Prototype Interferometer Matt Edgar.
111 Kazuhiro Yamamoto Institute for Cosmic Ray Research, the University of Tokyo Cryogenic interferometer technologies 19 May 2014 Gravitational Wave Advanced.
KAGRA Domestic Meeting Mirror 17 April, 2013 Norikatsu Mio Eiichi Hirose 1.
7 october 20111T. Schneider Test bench for digital sensor New Philips Digital Light Sensor Outer dimensions 32.6*32.6mm 2 8*8 pixel array Pixel pitch 4*4mm.
LIGO Scientific Collaboration
1 Kazuhiro Yamamoto Institute for Cosmic Ray Research The University of Tokyo KAGRA external review (Cryogenic payload) 18 April 2012.
1 Kazuhiro Yamamoto Institute for Cosmic Ray Research The university of Tokyo LCGT internal review (Cryogenic payload) 30 January 2012.
LCGT Meeting Laser & Mirror 12 December, Laser Ordered fiber amplifiers made by Nufern will be shipped on 16 th December. After the amplifiers arrive.
1 Kazuhiro Yamamoto Institute for Cosmic Ray Research The university of Tokyo LCGT internal review (Cryogenic payload) 30 January 2012.
LIGO-G D Advanced LIGO Systems & Interferometer Sensing & Control (ISC) Peter Fritschel, LIGO MIT PAC 12 Meeting, 27 June 2002.
G R 2004 Plan Update LIGO Systems meeting 22 Jan 04 dhs.
THE NEXT GENERATIONS OF GRAVITATIONAL WAVE DETECTORS (*) Giovanni Losurdo INFN Firenze – Virgo collaboration (*) GROUND BASED, INTERFEROMETRIC.
1 Cascina – October 19, 2011 ASPERA Forum Laurent Pinard Substrates, Polishing, Coatings and Metrology for the 2 nd generation of GW detector Laurent PINARD.
Overview of iLCGT & bLCGT Kazuaki Kuroda LCGT Collaboration F2f meeting 27 September, 2010.
Main Interferometer Subsystem
Mechanical loss measurement for KAGRA sapphire suspension system Takafumi Ushiba Department of Physics, The University of Tokyo The first international.
Cryogenic Payload Modeling: Vibration via Heat Links Takanori Sekiguchi JGW- JGW-G Cryogenic Payload Meeting
Input Mode Matching of LCGT 2012/1/5, Yoichi Aso.
Crystal Growth of Yb:S-FAP [Yb3+:Sr5(PO4)3F] for the Mercury Laser
Chapter 19 Electronic Technology Preview CRCT Preparation.
NSF Annual Review of the LIGO Laboratory
Performance test of KAGRA cryostat at site
Overview of the 20K configuration
New suspension study for LCGT
Performance test of KAGRA cryostat at site
The High Power Light Source for LCGT
Yoichi Aso on behalf of the LCGT ISC Group
Chapter 3—Issue Identification
Ponderomotive Squeezing Quantum Measurement Group
البيئة السياسية للإدارة الدولية
Status in Laser and Mirror group
LIGO Scientific Collaboration
S OPTICAL COMMUNICATIONS AND INSTRUMENTS
New suspension study for LCGT
The Next Generation: Advanced LIGO
KAGRA Domestic Meeting Laser
Development of vibration isolation systems for LCGT VI
Development of vibration isolation systems for LCGT VI
R&D in Glasgow MATERIALS ACTIVITY AIM Silica
Presentation transcript:

LCGT Meeting 12 October, 2010 Norikatsu Mio

Laser Discussion with Mitsubishi – Mitsubishi will offer their laser modules as a laser component and permit us to transfer them to other laser manufactures in order to assemble the laser system. – We will have a meeting on next Friday concerning the price and due date. Fiber laser – Commercial fiber laser: 40W=> 9MYen. – Two lasers will be introduced as a seed laser system. – We will have a meeting on next Thursday concerning the price and due date.

Alternative design Mitsubishi laser modules Fiber laser amplifiers NPRO(200mW) 40 W 80 W 200 W

Mirror Size of the mirrors for main cavities (25cm or 30cm) should be determined. – Design of vibration isolation systems depends on this determination. – If a coating machine is newly developed, there is no significant difference between two sizes. – If LIGO mirrors are used, we consider their dimensions (  25cm x t10cm and 10kg). If we decide to make full use of LIGO’s mirrors for iLICGT, we can save money and time; this fact enables us to develop the elements that are necessary for bLCGT.

Plan A’ For iLCGT, the size of the mirrors is chosen as that of iLIGO’s mirror. BS and ITMs will be newly fabricated from Japanese Silica.

Vibration Isolation iLCGT bLCGT ITMX,ITMY,ETMX,ETMY Type-A IP-GASF ( Fixed) Type-B’ payload Type-A IP-GASF Type-A payload(Cryo) BSStack Type-A payload Type-B IP-GASF Type-A payload PRM,PR2,PR3,SRM,SR2,SR3Stack Type-B’ payload Type-B IP-GASF Type-B’ payload MC2F,MC2E,MMT,PDType-C Type-A payload : 30kg Type-B’ payload : 10kg Type-B payload : 16kg

Sapphire Reply from GT Crystal systems – Current Max size of C-axis mirror:  20cm x t15cm A-Plane mirror:  25cm x t15cm “With time we feel can develop larger C-axis sapphire slabs to achieve your goal of 25cm x 15cm sapphire mirrors with our HEM growth process.” Inquiring – when we can obtain C-axis mirror of  20cm x t15cm? – price and delivery time of max size of C-axis mirror(  20cm x t15cm) and A-Plane mirror (  25cm x t15cm). – No answer.