Status of Japanese gravitational wave detectors
The Large-scale Cryogenic Gravitational wave Telescope (LCGT) is planned as a future Japanese project for gravitational wave detection. A 3 km interferometer will be built in an underground mine at Kamioka. Cryogenic sapphire mirrors are going to be employed for the test masses. For the demonstratio...
Gespeichert in:
Veröffentlicht in: | Classical and quantum gravity 2009-10, Vol.26 (20), p.204020-204020 (9) |
---|---|
Hauptverfasser: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 204020 (9) |
---|---|
container_issue | 20 |
container_start_page | 204020 |
container_title | Classical and quantum gravity |
container_volume | 26 |
creator | Arai, K Takahashi, R Tatsumi, D Izumi, K Wakabayashi, Y Ishizaki, H Fukushima, M Yamazaki, T Fujimoto, M-K Takamori, A Tsubono, K DeSalvo, R Bertolini, A Márka, S Sannibale, V Uchiyama, T Miyakawa, O Miyoki, S Agatsuma, K Saito, T Ohashi, M Kuroda, K Nakatani, I Telada, S Yamamoto, K Tomaru, T Suzuki, T Haruyama, T Sato, N Yamamoto, A Shintomi, T |
description | The Large-scale Cryogenic Gravitational wave Telescope (LCGT) is planned as a future Japanese project for gravitational wave detection. A 3 km interferometer will be built in an underground mine at Kamioka. Cryogenic sapphire mirrors are going to be employed for the test masses. For the demonstration of LCGT technologies, two prototype interferometers, TAMA300 and CLIO, are being developed. This paper describes the current status of the LCGT project and the two prototype interferometers. |
doi_str_mv | 10.1088/0264-9381/26/20/204020 |
format | Article |
fullrecord | <record><control><sourceid>proquest_pasca</sourceid><recordid>TN_cdi_pascalfrancis_primary_22207884</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>21464916</sourcerecordid><originalsourceid>FETCH-LOGICAL-c494t-bf3dbacac1f02e3126e0cc9956c1a50e06358e184f35633b835ff6f422e89d563</originalsourceid><addsrcrecordid>eNqFkE1LxDAQhoMouK7-BelFPdVmJh-bHmXxkwUP6jlk00Qq3W1Nuor_3pQue1EUBgZmnnnn5SXkFOglUKUKipLnJVNQoCyQpuIU6R6ZAJOQS6Zwn0x20CE5ivGNUgAFOCHFU2_6Tcxanz2YzqxddNlrMB91Gtft2jTZp_lwWeV6Z_s2xGNy4E0T3cm2T8nLzfXz_C5fPN7ez68WueUl7_OlZ9XSWGPBU3QMUDpqbVkKacEI6qhkQjlQ3DMhGVsqJryXniM6VVZpNCUXo24X2veNi71e1dG6pkkW203UM864EqVQiTz_k0TgkpcwSMoRtKGNMTivu1CvTPjSQPWQpB5C0kNIGqVGqsck0-HZ9oOJ1jQ-mLWt4-4aEelMKZ64fOTqttttf9fUXeUTDz_5f7x8A2PCjf8</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>21464916</pqid></control><display><type>article</type><title>Status of Japanese gravitational wave detectors</title><source>IOP Publishing Journals</source><source>Institute of Physics (IOP) Journals - HEAL-Link</source><creator>Arai, K ; Takahashi, R ; Tatsumi, D ; Izumi, K ; Wakabayashi, Y ; Ishizaki, H ; Fukushima, M ; Yamazaki, T ; Fujimoto, M-K ; Takamori, A ; Tsubono, K ; DeSalvo, R ; Bertolini, A ; Márka, S ; Sannibale, V ; Uchiyama, T ; Miyakawa, O ; Miyoki, S ; Agatsuma, K ; Saito, T ; Ohashi, M ; Kuroda, K ; Nakatani, I ; Telada, S ; Yamamoto, K ; Tomaru, T ; Suzuki, T ; Haruyama, T ; Sato, N ; Yamamoto, A ; Shintomi, T</creator><creatorcontrib>Arai, K ; Takahashi, R ; Tatsumi, D ; Izumi, K ; Wakabayashi, Y ; Ishizaki, H ; Fukushima, M ; Yamazaki, T ; Fujimoto, M-K ; Takamori, A ; Tsubono, K ; DeSalvo, R ; Bertolini, A ; Márka, S ; Sannibale, V ; Uchiyama, T ; Miyakawa, O ; Miyoki, S ; Agatsuma, K ; Saito, T ; Ohashi, M ; Kuroda, K ; Nakatani, I ; Telada, S ; Yamamoto, K ; Tomaru, T ; Suzuki, T ; Haruyama, T ; Sato, N ; Yamamoto, A ; Shintomi, T ; the TAMA Collaboration ; the CLIO Collaboration ; The LCGT Collaboration</creatorcontrib><description>The Large-scale Cryogenic Gravitational wave Telescope (LCGT) is planned as a future Japanese project for gravitational wave detection. A 3 km interferometer will be built in an underground mine at Kamioka. Cryogenic sapphire mirrors are going to be employed for the test masses. For the demonstration of LCGT technologies, two prototype interferometers, TAMA300 and CLIO, are being developed. This paper describes the current status of the LCGT project and the two prototype interferometers.</description><identifier>ISSN: 0264-9381</identifier><identifier>EISSN: 1361-6382</identifier><identifier>DOI: 10.1088/0264-9381/26/20/204020</identifier><identifier>CODEN: CQGRDG</identifier><language>eng</language><publisher>Bristol: IOP Publishing</publisher><subject>Exact sciences and technology ; General relativity and gravitation ; Physics</subject><ispartof>Classical and quantum gravity, 2009-10, Vol.26 (20), p.204020-204020 (9)</ispartof><rights>2015 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c494t-bf3dbacac1f02e3126e0cc9956c1a50e06358e184f35633b835ff6f422e89d563</citedby><cites>FETCH-LOGICAL-c494t-bf3dbacac1f02e3126e0cc9956c1a50e06358e184f35633b835ff6f422e89d563</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.1088/0264-9381/26/20/204020/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>309,310,314,776,780,785,786,23909,23910,25118,27901,27902,53805,53885</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=22207884$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Arai, K</creatorcontrib><creatorcontrib>Takahashi, R</creatorcontrib><creatorcontrib>Tatsumi, D</creatorcontrib><creatorcontrib>Izumi, K</creatorcontrib><creatorcontrib>Wakabayashi, Y</creatorcontrib><creatorcontrib>Ishizaki, H</creatorcontrib><creatorcontrib>Fukushima, M</creatorcontrib><creatorcontrib>Yamazaki, T</creatorcontrib><creatorcontrib>Fujimoto, M-K</creatorcontrib><creatorcontrib>Takamori, A</creatorcontrib><creatorcontrib>Tsubono, K</creatorcontrib><creatorcontrib>DeSalvo, R</creatorcontrib><creatorcontrib>Bertolini, A</creatorcontrib><creatorcontrib>Márka, S</creatorcontrib><creatorcontrib>Sannibale, V</creatorcontrib><creatorcontrib>Uchiyama, T</creatorcontrib><creatorcontrib>Miyakawa, O</creatorcontrib><creatorcontrib>Miyoki, S</creatorcontrib><creatorcontrib>Agatsuma, K</creatorcontrib><creatorcontrib>Saito, T</creatorcontrib><creatorcontrib>Ohashi, M</creatorcontrib><creatorcontrib>Kuroda, K</creatorcontrib><creatorcontrib>Nakatani, I</creatorcontrib><creatorcontrib>Telada, S</creatorcontrib><creatorcontrib>Yamamoto, K</creatorcontrib><creatorcontrib>Tomaru, T</creatorcontrib><creatorcontrib>Suzuki, T</creatorcontrib><creatorcontrib>Haruyama, T</creatorcontrib><creatorcontrib>Sato, N</creatorcontrib><creatorcontrib>Yamamoto, A</creatorcontrib><creatorcontrib>Shintomi, T</creatorcontrib><creatorcontrib>the TAMA Collaboration</creatorcontrib><creatorcontrib>the CLIO Collaboration</creatorcontrib><creatorcontrib>The LCGT Collaboration</creatorcontrib><title>Status of Japanese gravitational wave detectors</title><title>Classical and quantum gravity</title><description>The Large-scale Cryogenic Gravitational wave Telescope (LCGT) is planned as a future Japanese project for gravitational wave detection. A 3 km interferometer will be built in an underground mine at Kamioka. Cryogenic sapphire mirrors are going to be employed for the test masses. For the demonstration of LCGT technologies, two prototype interferometers, TAMA300 and CLIO, are being developed. This paper describes the current status of the LCGT project and the two prototype interferometers.</description><subject>Exact sciences and technology</subject><subject>General relativity and gravitation</subject><subject>Physics</subject><issn>0264-9381</issn><issn>1361-6382</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2009</creationdate><recordtype>article</recordtype><recordid>eNqFkE1LxDAQhoMouK7-BelFPdVmJh-bHmXxkwUP6jlk00Qq3W1Nuor_3pQue1EUBgZmnnnn5SXkFOglUKUKipLnJVNQoCyQpuIU6R6ZAJOQS6Zwn0x20CE5ivGNUgAFOCHFU2_6Tcxanz2YzqxddNlrMB91Gtft2jTZp_lwWeV6Z_s2xGNy4E0T3cm2T8nLzfXz_C5fPN7ez68WueUl7_OlZ9XSWGPBU3QMUDpqbVkKacEI6qhkQjlQ3DMhGVsqJryXniM6VVZpNCUXo24X2veNi71e1dG6pkkW203UM864EqVQiTz_k0TgkpcwSMoRtKGNMTivu1CvTPjSQPWQpB5C0kNIGqVGqsck0-HZ9oOJ1jQ-mLWt4-4aEelMKZ64fOTqttttf9fUXeUTDz_5f7x8A2PCjf8</recordid><startdate>20091021</startdate><enddate>20091021</enddate><creator>Arai, K</creator><creator>Takahashi, R</creator><creator>Tatsumi, D</creator><creator>Izumi, K</creator><creator>Wakabayashi, Y</creator><creator>Ishizaki, H</creator><creator>Fukushima, M</creator><creator>Yamazaki, T</creator><creator>Fujimoto, M-K</creator><creator>Takamori, A</creator><creator>Tsubono, K</creator><creator>DeSalvo, R</creator><creator>Bertolini, A</creator><creator>Márka, S</creator><creator>Sannibale, V</creator><creator>Uchiyama, T</creator><creator>Miyakawa, O</creator><creator>Miyoki, S</creator><creator>Agatsuma, K</creator><creator>Saito, T</creator><creator>Ohashi, M</creator><creator>Kuroda, K</creator><creator>Nakatani, I</creator><creator>Telada, S</creator><creator>Yamamoto, K</creator><creator>Tomaru, T</creator><creator>Suzuki, T</creator><creator>Haruyama, T</creator><creator>Sato, N</creator><creator>Yamamoto, A</creator><creator>Shintomi, T</creator><general>IOP Publishing</general><general>Institute of Physics</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>7U5</scope><scope>8FD</scope><scope>L7M</scope></search><sort><creationdate>20091021</creationdate><title>Status of Japanese gravitational wave detectors</title><author>Arai, K ; Takahashi, R ; Tatsumi, D ; Izumi, K ; Wakabayashi, Y ; Ishizaki, H ; Fukushima, M ; Yamazaki, T ; Fujimoto, M-K ; Takamori, A ; Tsubono, K ; DeSalvo, R ; Bertolini, A ; Márka, S ; Sannibale, V ; Uchiyama, T ; Miyakawa, O ; Miyoki, S ; Agatsuma, K ; Saito, T ; Ohashi, M ; Kuroda, K ; Nakatani, I ; Telada, S ; Yamamoto, K ; Tomaru, T ; Suzuki, T ; Haruyama, T ; Sato, N ; Yamamoto, A ; Shintomi, T</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c494t-bf3dbacac1f02e3126e0cc9956c1a50e06358e184f35633b835ff6f422e89d563</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2009</creationdate><topic>Exact sciences and technology</topic><topic>General relativity and gravitation</topic><topic>Physics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Arai, K</creatorcontrib><creatorcontrib>Takahashi, R</creatorcontrib><creatorcontrib>Tatsumi, D</creatorcontrib><creatorcontrib>Izumi, K</creatorcontrib><creatorcontrib>Wakabayashi, Y</creatorcontrib><creatorcontrib>Ishizaki, H</creatorcontrib><creatorcontrib>Fukushima, M</creatorcontrib><creatorcontrib>Yamazaki, T</creatorcontrib><creatorcontrib>Fujimoto, M-K</creatorcontrib><creatorcontrib>Takamori, A</creatorcontrib><creatorcontrib>Tsubono, K</creatorcontrib><creatorcontrib>DeSalvo, R</creatorcontrib><creatorcontrib>Bertolini, A</creatorcontrib><creatorcontrib>Márka, S</creatorcontrib><creatorcontrib>Sannibale, V</creatorcontrib><creatorcontrib>Uchiyama, T</creatorcontrib><creatorcontrib>Miyakawa, O</creatorcontrib><creatorcontrib>Miyoki, S</creatorcontrib><creatorcontrib>Agatsuma, K</creatorcontrib><creatorcontrib>Saito, T</creatorcontrib><creatorcontrib>Ohashi, M</creatorcontrib><creatorcontrib>Kuroda, K</creatorcontrib><creatorcontrib>Nakatani, I</creatorcontrib><creatorcontrib>Telada, S</creatorcontrib><creatorcontrib>Yamamoto, K</creatorcontrib><creatorcontrib>Tomaru, T</creatorcontrib><creatorcontrib>Suzuki, T</creatorcontrib><creatorcontrib>Haruyama, T</creatorcontrib><creatorcontrib>Sato, N</creatorcontrib><creatorcontrib>Yamamoto, A</creatorcontrib><creatorcontrib>Shintomi, T</creatorcontrib><creatorcontrib>the TAMA Collaboration</creatorcontrib><creatorcontrib>the CLIO Collaboration</creatorcontrib><creatorcontrib>The LCGT Collaboration</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Classical and quantum gravity</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Arai, K</au><au>Takahashi, R</au><au>Tatsumi, D</au><au>Izumi, K</au><au>Wakabayashi, Y</au><au>Ishizaki, H</au><au>Fukushima, M</au><au>Yamazaki, T</au><au>Fujimoto, M-K</au><au>Takamori, A</au><au>Tsubono, K</au><au>DeSalvo, R</au><au>Bertolini, A</au><au>Márka, S</au><au>Sannibale, V</au><au>Uchiyama, T</au><au>Miyakawa, O</au><au>Miyoki, S</au><au>Agatsuma, K</au><au>Saito, T</au><au>Ohashi, M</au><au>Kuroda, K</au><au>Nakatani, I</au><au>Telada, S</au><au>Yamamoto, K</au><au>Tomaru, T</au><au>Suzuki, T</au><au>Haruyama, T</au><au>Sato, N</au><au>Yamamoto, A</au><au>Shintomi, T</au><aucorp>the TAMA Collaboration</aucorp><aucorp>the CLIO Collaboration</aucorp><aucorp>The LCGT Collaboration</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Status of Japanese gravitational wave detectors</atitle><jtitle>Classical and quantum gravity</jtitle><date>2009-10-21</date><risdate>2009</risdate><volume>26</volume><issue>20</issue><spage>204020</spage><epage>204020 (9)</epage><pages>204020-204020 (9)</pages><issn>0264-9381</issn><eissn>1361-6382</eissn><coden>CQGRDG</coden><abstract>The Large-scale Cryogenic Gravitational wave Telescope (LCGT) is planned as a future Japanese project for gravitational wave detection. A 3 km interferometer will be built in an underground mine at Kamioka. Cryogenic sapphire mirrors are going to be employed for the test masses. For the demonstration of LCGT technologies, two prototype interferometers, TAMA300 and CLIO, are being developed. This paper describes the current status of the LCGT project and the two prototype interferometers.</abstract><cop>Bristol</cop><pub>IOP Publishing</pub><doi>10.1088/0264-9381/26/20/204020</doi></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0264-9381 |
ispartof | Classical and quantum gravity, 2009-10, Vol.26 (20), p.204020-204020 (9) |
issn | 0264-9381 1361-6382 |
language | eng |
recordid | cdi_pascalfrancis_primary_22207884 |
source | IOP Publishing Journals; Institute of Physics (IOP) Journals - HEAL-Link |
subjects | Exact sciences and technology General relativity and gravitation Physics |
title | Status of Japanese gravitational wave detectors |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-30T17%3A26%3A31IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_pasca&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Status%20of%20Japanese%20gravitational%20wave%20detectors&rft.jtitle=Classical%20and%20quantum%20gravity&rft.au=Arai,%20K&rft.aucorp=the%20TAMA%20Collaboration&rft.date=2009-10-21&rft.volume=26&rft.issue=20&rft.spage=204020&rft.epage=204020%20(9)&rft.pages=204020-204020%20(9)&rft.issn=0264-9381&rft.eissn=1361-6382&rft.coden=CQGRDG&rft_id=info:doi/10.1088/0264-9381/26/20/204020&rft_dat=%3Cproquest_pasca%3E21464916%3C/proquest_pasca%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=21464916&rft_id=info:pmid/&rfr_iscdi=true |