Local-oscillator noise coupling in balanced homodyne readout for advanced gravitational wave detectors
The second generation of interferometric gravitational wave detectors are quickly approaching their design sensitivity. For the first time these detectors will become limited by quantum backaction noise. Several backaction evasion techniques have been proposed to further increase the detector sensit...
Gespeichert in:
| Veröffentlicht in: | Physical review. D 2015-10, Vol.92 (7), Article 072009 |
|---|---|
| Hauptverfasser: | , , , , , , , , , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | |
|---|---|
| container_issue | 7 |
| container_start_page | |
| container_title | Physical review. D |
| container_volume | 92 |
| creator | Steinlechner, Sebastian Barr, Bryan W. Bell, Angus S. Danilishin, Stefan L. Gläfke, Andreas Gräf, Christian Hennig, Jan-Simon Houston, E. Alasdair Huttner, Sabina H. Leavey, Sean S. Pascucci, Daniela Sorazu, Borja Spencer, Andrew Strain, Kenneth A. Wright, Jennifer Hild, Stefan |
| description | The second generation of interferometric gravitational wave detectors are quickly approaching their design sensitivity. For the first time these detectors will become limited by quantum backaction noise. Several backaction evasion techniques have been proposed to further increase the detector sensitivity. Since most proposals rely on a flexible readout of the full amplitude- and phase-quadrature space of the output light field, balanced homodyne detection is generally expected to replace the currently used DC readout. Up to now, little investigation has been undertaken into how balanced homodyne detection can be successfully transferred from its ubiquitous application in tabletop quantum optics experiments to large-scale interferometers with suspended optics. Here we derive implementation requirements with respect to local-oscillator noise couplings and highlight potential issues with the example of the Glasgow Sagnac Speed Meter experiment, as well as for a future upgrade to the Advanced LIGO detectors. |
| doi_str_mv | 10.1103/PhysRevD.92.072009 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1793254412</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1793254412</sourcerecordid><originalsourceid>FETCH-LOGICAL-c373t-e014345de8d8f8eee72c1efc70d19676f46efbfbb48c37ad2ff815c870ff95a3</originalsourceid><addsrcrecordid>eNo1kMtOwzAQRS0EEqXwA6y8ZJPiRxLbS1SeUiUQ6t5y7HFrlMbFTor69wSlrGakOfdKcxC6pWRBKeH3H9tj_oTD40KxBRGMEHWGZrSqSMF4Lc9Pu1BKXqKrnL8I4awWYob8KlrTFjHb0Lamjwl3MWTANg77NnQbHDrcmNZ0Fhzexl10xw5wAuPi0GM_8sYdpusmmUPoTR9iZ1r8Yw6AHfRgx9J8jS68aTPcnOYcrZ-f1svXYvX-8rZ8WBWWC94XQGjJy8qBdNJLABDMUvBWEEdVLWpf1uAb3zSlHAPGMe8lrawUxHtVGT5Hd1PtPsXvAXKvdyFbGD_rIA5ZU6E4q8qSshFlE2pTzDmB1_sUdiYdNSX6z6n-d6oV05NT_gsoSW9n</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1793254412</pqid></control><display><type>article</type><title>Local-oscillator noise coupling in balanced homodyne readout for advanced gravitational wave detectors</title><source>American Physical Society Journals</source><creator>Steinlechner, Sebastian ; Barr, Bryan W. ; Bell, Angus S. ; Danilishin, Stefan L. ; Gläfke, Andreas ; Gräf, Christian ; Hennig, Jan-Simon ; Houston, E. Alasdair ; Huttner, Sabina H. ; Leavey, Sean S. ; Pascucci, Daniela ; Sorazu, Borja ; Spencer, Andrew ; Strain, Kenneth A. ; Wright, Jennifer ; Hild, Stefan</creator><creatorcontrib>Steinlechner, Sebastian ; Barr, Bryan W. ; Bell, Angus S. ; Danilishin, Stefan L. ; Gläfke, Andreas ; Gräf, Christian ; Hennig, Jan-Simon ; Houston, E. Alasdair ; Huttner, Sabina H. ; Leavey, Sean S. ; Pascucci, Daniela ; Sorazu, Borja ; Spencer, Andrew ; Strain, Kenneth A. ; Wright, Jennifer ; Hild, Stefan</creatorcontrib><description>The second generation of interferometric gravitational wave detectors are quickly approaching their design sensitivity. For the first time these detectors will become limited by quantum backaction noise. Several backaction evasion techniques have been proposed to further increase the detector sensitivity. Since most proposals rely on a flexible readout of the full amplitude- and phase-quadrature space of the output light field, balanced homodyne detection is generally expected to replace the currently used DC readout. Up to now, little investigation has been undertaken into how balanced homodyne detection can be successfully transferred from its ubiquitous application in tabletop quantum optics experiments to large-scale interferometers with suspended optics. Here we derive implementation requirements with respect to local-oscillator noise couplings and highlight potential issues with the example of the Glasgow Sagnac Speed Meter experiment, as well as for a future upgrade to the Advanced LIGO detectors.</description><identifier>ISSN: 1550-7998</identifier><identifier>ISSN: 2470-0010</identifier><identifier>EISSN: 1550-2368</identifier><identifier>EISSN: 2470-0029</identifier><identifier>DOI: 10.1103/PhysRevD.92.072009</identifier><language>eng</language><subject>Balancing ; Cosmology ; Detectors ; Gravitational waves ; Interferometers ; Joining ; Measuring instruments ; Noise</subject><ispartof>Physical review. D, 2015-10, Vol.92 (7), Article 072009</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c373t-e014345de8d8f8eee72c1efc70d19676f46efbfbb48c37ad2ff815c870ff95a3</citedby><cites>FETCH-LOGICAL-c373t-e014345de8d8f8eee72c1efc70d19676f46efbfbb48c37ad2ff815c870ff95a3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,777,781,2863,2864,27905,27906</link.rule.ids></links><search><creatorcontrib>Steinlechner, Sebastian</creatorcontrib><creatorcontrib>Barr, Bryan W.</creatorcontrib><creatorcontrib>Bell, Angus S.</creatorcontrib><creatorcontrib>Danilishin, Stefan L.</creatorcontrib><creatorcontrib>Gläfke, Andreas</creatorcontrib><creatorcontrib>Gräf, Christian</creatorcontrib><creatorcontrib>Hennig, Jan-Simon</creatorcontrib><creatorcontrib>Houston, E. Alasdair</creatorcontrib><creatorcontrib>Huttner, Sabina H.</creatorcontrib><creatorcontrib>Leavey, Sean S.</creatorcontrib><creatorcontrib>Pascucci, Daniela</creatorcontrib><creatorcontrib>Sorazu, Borja</creatorcontrib><creatorcontrib>Spencer, Andrew</creatorcontrib><creatorcontrib>Strain, Kenneth A.</creatorcontrib><creatorcontrib>Wright, Jennifer</creatorcontrib><creatorcontrib>Hild, Stefan</creatorcontrib><title>Local-oscillator noise coupling in balanced homodyne readout for advanced gravitational wave detectors</title><title>Physical review. D</title><description>The second generation of interferometric gravitational wave detectors are quickly approaching their design sensitivity. For the first time these detectors will become limited by quantum backaction noise. Several backaction evasion techniques have been proposed to further increase the detector sensitivity. Since most proposals rely on a flexible readout of the full amplitude- and phase-quadrature space of the output light field, balanced homodyne detection is generally expected to replace the currently used DC readout. Up to now, little investigation has been undertaken into how balanced homodyne detection can be successfully transferred from its ubiquitous application in tabletop quantum optics experiments to large-scale interferometers with suspended optics. Here we derive implementation requirements with respect to local-oscillator noise couplings and highlight potential issues with the example of the Glasgow Sagnac Speed Meter experiment, as well as for a future upgrade to the Advanced LIGO detectors.</description><subject>Balancing</subject><subject>Cosmology</subject><subject>Detectors</subject><subject>Gravitational waves</subject><subject>Interferometers</subject><subject>Joining</subject><subject>Measuring instruments</subject><subject>Noise</subject><issn>1550-7998</issn><issn>2470-0010</issn><issn>1550-2368</issn><issn>2470-0029</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><recordid>eNo1kMtOwzAQRS0EEqXwA6y8ZJPiRxLbS1SeUiUQ6t5y7HFrlMbFTor69wSlrGakOfdKcxC6pWRBKeH3H9tj_oTD40KxBRGMEHWGZrSqSMF4Lc9Pu1BKXqKrnL8I4awWYob8KlrTFjHb0Lamjwl3MWTANg77NnQbHDrcmNZ0Fhzexl10xw5wAuPi0GM_8sYdpusmmUPoTR9iZ1r8Yw6AHfRgx9J8jS68aTPcnOYcrZ-f1svXYvX-8rZ8WBWWC94XQGjJy8qBdNJLABDMUvBWEEdVLWpf1uAb3zSlHAPGMe8lrawUxHtVGT5Hd1PtPsXvAXKvdyFbGD_rIA5ZU6E4q8qSshFlE2pTzDmB1_sUdiYdNSX6z6n-d6oV05NT_gsoSW9n</recordid><startdate>20151020</startdate><enddate>20151020</enddate><creator>Steinlechner, Sebastian</creator><creator>Barr, Bryan W.</creator><creator>Bell, Angus S.</creator><creator>Danilishin, Stefan L.</creator><creator>Gläfke, Andreas</creator><creator>Gräf, Christian</creator><creator>Hennig, Jan-Simon</creator><creator>Houston, E. Alasdair</creator><creator>Huttner, Sabina H.</creator><creator>Leavey, Sean S.</creator><creator>Pascucci, Daniela</creator><creator>Sorazu, Borja</creator><creator>Spencer, Andrew</creator><creator>Strain, Kenneth A.</creator><creator>Wright, Jennifer</creator><creator>Hild, Stefan</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20151020</creationdate><title>Local-oscillator noise coupling in balanced homodyne readout for advanced gravitational wave detectors</title><author>Steinlechner, Sebastian ; Barr, Bryan W. ; Bell, Angus S. ; Danilishin, Stefan L. ; Gläfke, Andreas ; Gräf, Christian ; Hennig, Jan-Simon ; Houston, E. Alasdair ; Huttner, Sabina H. ; Leavey, Sean S. ; Pascucci, Daniela ; Sorazu, Borja ; Spencer, Andrew ; Strain, Kenneth A. ; Wright, Jennifer ; Hild, Stefan</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c373t-e014345de8d8f8eee72c1efc70d19676f46efbfbb48c37ad2ff815c870ff95a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Balancing</topic><topic>Cosmology</topic><topic>Detectors</topic><topic>Gravitational waves</topic><topic>Interferometers</topic><topic>Joining</topic><topic>Measuring instruments</topic><topic>Noise</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Steinlechner, Sebastian</creatorcontrib><creatorcontrib>Barr, Bryan W.</creatorcontrib><creatorcontrib>Bell, Angus S.</creatorcontrib><creatorcontrib>Danilishin, Stefan L.</creatorcontrib><creatorcontrib>Gläfke, Andreas</creatorcontrib><creatorcontrib>Gräf, Christian</creatorcontrib><creatorcontrib>Hennig, Jan-Simon</creatorcontrib><creatorcontrib>Houston, E. Alasdair</creatorcontrib><creatorcontrib>Huttner, Sabina H.</creatorcontrib><creatorcontrib>Leavey, Sean S.</creatorcontrib><creatorcontrib>Pascucci, Daniela</creatorcontrib><creatorcontrib>Sorazu, Borja</creatorcontrib><creatorcontrib>Spencer, Andrew</creatorcontrib><creatorcontrib>Strain, Kenneth A.</creatorcontrib><creatorcontrib>Wright, Jennifer</creatorcontrib><creatorcontrib>Hild, Stefan</creatorcontrib><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Physical review. D</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Steinlechner, Sebastian</au><au>Barr, Bryan W.</au><au>Bell, Angus S.</au><au>Danilishin, Stefan L.</au><au>Gläfke, Andreas</au><au>Gräf, Christian</au><au>Hennig, Jan-Simon</au><au>Houston, E. Alasdair</au><au>Huttner, Sabina H.</au><au>Leavey, Sean S.</au><au>Pascucci, Daniela</au><au>Sorazu, Borja</au><au>Spencer, Andrew</au><au>Strain, Kenneth A.</au><au>Wright, Jennifer</au><au>Hild, Stefan</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Local-oscillator noise coupling in balanced homodyne readout for advanced gravitational wave detectors</atitle><jtitle>Physical review. D</jtitle><date>2015-10-20</date><risdate>2015</risdate><volume>92</volume><issue>7</issue><artnum>072009</artnum><issn>1550-7998</issn><issn>2470-0010</issn><eissn>1550-2368</eissn><eissn>2470-0029</eissn><abstract>The second generation of interferometric gravitational wave detectors are quickly approaching their design sensitivity. For the first time these detectors will become limited by quantum backaction noise. Several backaction evasion techniques have been proposed to further increase the detector sensitivity. Since most proposals rely on a flexible readout of the full amplitude- and phase-quadrature space of the output light field, balanced homodyne detection is generally expected to replace the currently used DC readout. Up to now, little investigation has been undertaken into how balanced homodyne detection can be successfully transferred from its ubiquitous application in tabletop quantum optics experiments to large-scale interferometers with suspended optics. Here we derive implementation requirements with respect to local-oscillator noise couplings and highlight potential issues with the example of the Glasgow Sagnac Speed Meter experiment, as well as for a future upgrade to the Advanced LIGO detectors.</abstract><doi>10.1103/PhysRevD.92.072009</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 1550-7998 |
| ispartof | Physical review. D, 2015-10, Vol.92 (7), Article 072009 |
| issn | 1550-7998 2470-0010 1550-2368 2470-0029 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_1793254412 |
| source | American Physical Society Journals |
| subjects | Balancing Cosmology Detectors Gravitational waves Interferometers Joining Measuring instruments Noise |
| title | Local-oscillator noise coupling in balanced homodyne readout for advanced 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=2025-01-18T21%3A15%3A54IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Local-oscillator%20noise%20coupling%20in%20balanced%20homodyne%20readout%20for%20advanced%20gravitational%20wave%20detectors&rft.jtitle=Physical%20review.%20D&rft.au=Steinlechner,%20Sebastian&rft.date=2015-10-20&rft.volume=92&rft.issue=7&rft.artnum=072009&rft.issn=1550-7998&rft.eissn=1550-2368&rft_id=info:doi/10.1103/PhysRevD.92.072009&rft_dat=%3Cproquest_cross%3E1793254412%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1793254412&rft_id=info:pmid/&rfr_iscdi=true |