tamago.mtk.nao.ac.jp

TAMA300 interferometer

We started improvements of the detector and developments of observation technique in 1995 using the 300m interferometer gravitational antenna TAMA300. In Mitaka campus of the national astronomical observatory of Japan. The aim of the project is to develop advanced techniques needed for a future km-sized interferometer and catch gravitational waves that may occur within our local group of galaxies. The present sensitivity of TAMA300. To detector development page. Gravitational Wave Project Office /.

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TAMA300 interferometer | tamago.mtk.nao.ac.jp Reviews

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We started improvements of the detector and developments of observation technique in 1995 using the 300m interferometer gravitational antenna TAMA300. In Mitaka campus of the national astronomical observatory of Japan. The aim of the project is to develop advanced techniques needed for a future km-sized interferometer and catch gravitational waves that may occur within our local group of galaxies. The present sensitivity of TAMA300. To detector development page. Gravitational Wave Project Office /.

<META> KEYWORDS

1 about gw

2 people

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4 links

5 kagra lcgt

6 decigo

7 3g r&d

8 internal

9 tama300 interferometer

10 overview of tama300

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TAMA300 interferometer | tamago.mtk.nao.ac.jp Reviews

https://tamago.mtk.nao.ac.jp

We started improvements of the detector and developments of observation technique in 1995 using the 300m interferometer gravitational antenna TAMA300. In Mitaka campus of the national astronomical observatory of Japan. The aim of the project is to develop advanced techniques needed for a future km-sized interferometer and catch gravitational waves that may occur within our local group of galaxies. The present sensitivity of TAMA300. To detector development page. Gravitational Wave Project Office /.

INTERNAL PAGES

tamago.mtk.nao.ac.jp

1

KAGRA Project

http://tamago.mtk.nao.ac.jp/spacetime/lcgt_e.html

KAGRA Project (LCGT Project). Large-scale Cryogenic Gravitational wave Telescope. LCGT) is a project that aims to achieve the first detection of gravitational waves (GW). KAGRA. Is designed to observe several GW events in a year. This Japanese project is hosted by ICRR, University of Tokyo with cooperation of Gravitational Wave Project Office, KEK, and various universities/ institutes in the world. Link to the CLIO project. Link to the KAGRA project. Features of the Telescope. We designed the KAGRA.

2

TAMA Project/Installation Status.

http://tamago.mtk.nao.ac.jp/tama/installation/taskplan.html

Installation and Operation Status. 10m Mode Cleaner (97.4-97.12). Sidebands(15.25MHz) transmittion experiment was successfully finished. Residual excess noise is smaller than 20mW shot noise. One Arm (97.8-98.4). 300m FP cavity was successfully locked. By using a wave front sensing method, the cavity is very stable. Laser and Mode Cleaner (98.1-99.1). 35W output after Mode Cleaner has been realized! Transmittion rate is 54%. Recombine I (98.5-99.1). Laser, MC and FPMI were connected. This is world record.

3

DECIGO

http://tamago.mtk.nao.ac.jp/spacetime/decigo_e.html

Link to the DECIGO project. DECIGO stands for DECi-hertz Interferometer Gravitational wave Observatory. It is a gravitational wave antenna in space operating in the 0.1 - 10 Hz frequency band. We propose DECIGO as the Japanese detector to be built after the ground-based detector LCGT. What is DECIGO Pathfinder? Gravitational Wave Project Office /. Contact: gw-webmaster@ @ @Add following strings : nao.ac.jp.

4

About Gravitational Waves

http://tamago.mtk.nao.ac.jp/spacetime/aboutGW_e.html

What Are Gravitational Waves? On September 14 2015, the LIGO detectors directly observed gravitational waves from the merger of two black holes. This is an enormous achievement, but only the beginning of the entirely new field of gravitational wave astronomy. GWs are generated from an accelerated mass. However, only dense and massive objects can generate GWs with observable amplitudes. Astronomical motions and events are likely to be potential sources of GWs. Some examples of sources are:. GWs can change...

5

Link

http://tamago.mtk.nao.ac.jp/spacetime/links_e.html

Research Institutes in Japan. Institute for Cosmic Ray Research (Gravitational Wave Project Office). Institute for Cosmic Ray Research (GW group). High Energy Accelerator Research Organization (GW group). National Institute of Information and Communications Technology (NICT). Atomic Frequency Standards Project. Interferometer GW detectors overseas. Germany / United Kingdom). Gravitational Wave Project Office /. Contact: gw-webmaster@ @ @Add following strings : nao.ac.jp.

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goede-stiftung.org

Link-Empfehlungen - GÖDE-Stiftung

http://www.goede-stiftung.org/links

Die Provinz Quang Ninh. News & Presse. Allgemeine Artikel zum Thema Gravitation. Messung der Gravitationskonstante G. Alternative Experimente zur Gravitation. Albert-Einstein-Institut für Gravitationsphysik der Max-Planck-Gesellschaft. Institute for Gravitational Research (IGR) – Glasgow, U.K. Zentrum für Gravitationsphysik (Max-Planck-Gesellschaft) – Universität Hannover. CIPA – California Instiute for Physics and Astrophsics. Free Patent searching site. Physical Reference Data (NIST). 8211; Max Rauner.

lisa6.gsfc.nasa.gov

AstroGravS: Ground-Based Detectors

http://lisa6.gsfc.nasa.gov/docs/ground_based_det.html

Mock LISA Data Challenge. Proposal Info and Deadlines. LIGO Scientific Collaboration (LSC). LIGO LSC Source Groups. Mock LISA Data Challenge. Proposal Info and Deadlines. Images and Movies Links. Is a service of the Astrophysics Science Division (ASD). Download Adobe Acrobat to read PDF files. Other plugins and helper applications. Privacy Policy and Important Notices.

ligo.org

LSC Partners

http://www.ligo.org/partners.php

Partner Experiments and Collaborations. The GEO600 Experiment &#47 Collaboration. The Virgo Collaboration &#47 European Gravitational Observatory (EGO) consortium. The Australian Consortium for Interferometric Gravitational Astronomy (ACIGA). KAGRA - The Kamioka Gravitational Wave Telescope. The KAGRA project aims to construct and operate a single 3km baseline cryogenic interferometer underground in Japan at the Kamioka mine. The aim is to minimize gravitational gradient and thermal noise through und...

lisa-science.org

About the LISC — Welcome to the LISC web portal LISC - LISA International Science Community

http://www.lisa-science.org/about-the-lisc

Only in current section. The LISC portal webteam. LISA Brownbag and GW Notes. The LISC is an informal network of researchers maintained by the LISA International Science Team (which coordinates the development of the space-based gravitational wave detector LISA) for the purpose of exchanging information with the wider science community. And in the US. The development of LISA is coordinated by the LISA International Science Team (LIST). List of LISC members. By offering a repository of helpful resources.

aigo.org.au

AIGO- a gravitational wave telescope for the southern hemisphere

http://www.aigo.org.au/index.php

The Quest to discover Einstein's Waves. Listen to some Gravitational Waves. Gravitational Wave Observatories - how they work. The need for a Southern Hemisphere Detector. Stage 1 - Current Research Facility. Stage 2 - Long baseline Detector. Contribution to international Science. Education - Research Programme. The Gravity Discovery Centre. China GW Working Group. CSIRO Center for Precision Optics. Login - Relativity Outreach. Login - Education Enrichment. International Workshop: 27-29 September 2012.

auriga.lnl.infn.it

AURIGA: useful links

http://www.auriga.lnl.infn.it/auriga/links.html

A list of useful links. Gravitational wave detector community:. Resonant bar detectors: ALLEGRO. Resonant spherical detectors: MiniGRAIL. Wideband acoustic detector: DUAL. The resonant detectors international network: IGEC. The Gravitational Wave International Committee: GWIC. Http:/ www.batse.msfc.nasa.gov/. NASA site on GRB. Http:/ www.phys.lsu.edu/mog/. Http:/ vizier.u-strasbg.fr/. Library of published astronomical catalogues and data tables. Http:/ relativity.livingreviews.org/.

astrogravs.gsfc.nasa.gov

AstroGravS: Ground-Based Detectors

https://astrogravs.gsfc.nasa.gov/docs/ground_based_det.html

Mock LISA Data Challenge. Proposal Info and Deadlines. LIGO Scientific Collaboration (LSC). LIGO LSC Source Groups. Mock LISA Data Challenge. Proposal Info and Deadlines. Images and Movies Links. Is a service of the Astrophysics Science Division (ASD). Download Adobe Acrobat to read PDF files. Other plugins and helper applications. Privacy Policy and Important Notices.

gwpo.mtk.nao.ac.jp

Gravitational Wave Project Office

http://gwpo.mtk.nao.ac.jp/en

May 16, 2016. The Special Breakthrough Prize for Fundamental physics awarded for the Detection of Gravitational Waves. February 12, 2016. On the direct detection of the gravitational waves by LIGO. January 19, 2016. Professor. Raffaele Flaminio, was interviewed by NAOJPRC. March 1, 2017. The Gravitational Wave Project Office of NAOJ has an open position for an assistant professor. February 17, 2017. Two members of the project office are among the recipients of the 2016 Gruber Cosmology Prize. July 1, 2016.

astrogravs.nasa.gov

AstroGravS: Ground-Based Detectors

http://astrogravs.nasa.gov/docs/ground_based_det.html

Mock LISA Data Challenge. Proposal Info and Deadlines. LIGO Scientific Collaboration (LSC). LIGO LSC Source Groups. Mock LISA Data Challenge. Proposal Info and Deadlines. Images and Movies Links. Is a service of the Astrophysics Science Division (ASD). Download Adobe Acrobat to read PDF files. Other plugins and helper applications. Privacy Policy and Important Notices.

vselenata.blogspot.com

Вселената: Септември 2007

http://vselenata.blogspot.com/2007_09_01_archive.html

Събота, септември 29, 2007. Най-странните неща във Вселената: гравитационни вълни. В продължение на 10 седмици ще ви запозная малко по-подробно с всяко едно от явленията и обектите, включени в анкетата на space.com. Можете да гласувате за вашите фаворити тук. Тази събота е денят на гравитационните вълни. Общата теория на относителността. Но какво може да причинява тези гравитационни вълни? Двойка звезди, звезда и планета.), експлозия на свръхнова. Стига да не е напълно симетрична), сливане на черни дупки.

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TAMA300 interferometer

We started improvements of the detector and developments of observation technique in 1995 using the 300m interferometer gravitational antenna TAMA300. In Mitaka campus of the national astronomical observatory of Japan. The aim of the project is to develop advanced techniques needed for a future km-sized interferometer and catch gravitational waves that may occur within our local group of galaxies. The present sensitivity of TAMA300. To detector development page. Gravitational Wave Project Office /.

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