Multi-spatial-mode effects in squeezed-light-enhanced interferometric gravitational wave detectors

Proposed near-future upgrades of the current advanced interferometric gravitational wave detectors include the usage of frequency dependent squeezed light to reduce the current sensitivity-limiting quantum noise. We quantify and describe the degradation effects that spatial mode-mismatches between o...

Full description

Saved in:
Bibliographic Details
Published in:arXiv.org 2017-07
Main Authors: Töyrä, Daniel, Brown, Daniel D, McKenna, Davis, Song, Shicong, Wormald, Alex, Harms, Jan, Miao, Haixing, Freise, Andreas
Format: Article
Language:English
Subjects:
Detectors
Gravitational effects
Gravitational waves
Hermite-Gaussian modes
Interferometry
Noise sensitivity
Optical resonators
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by
cites
container_end_page
container_issue
container_start_page
container_title arXiv.org
container_volume
creator Töyrä, Daniel
Brown, Daniel D
McKenna, Davis
Song, Shicong
Wormald, Alex
Harms, Jan
Miao, Haixing
Freise, Andreas
description Proposed near-future upgrades of the current advanced interferometric gravitational wave detectors include the usage of frequency dependent squeezed light to reduce the current sensitivity-limiting quantum noise. We quantify and describe the degradation effects that spatial mode-mismatches between optical resonators have on the squeezed field. These mode-mismatches can to first order be described by scattering of light into second-order Gaussian modes. As a demonstration of principle, we also show that squeezing the second-order Hermite-Gaussian modes \(\mathrm{HG}_{02}\) and \(\mathrm{HG}_{20}\), in addition to the fundamental mode, has the potential to increase the robustness to spatial mode-mismatches. This scheme, however, requires independently optimized squeeze angles for each squeezed spatial mode, which would be challenging to realise in practise.
doi_str_mv 10.48550/arxiv.1704.08237
format article
fullrecord <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2075951264</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2075951264</sourcerecordid><originalsourceid>FETCH-LOGICAL-a524-b77fcf881998eb8f6d40a7a386ccae41c67e2a7578b36c0196821de0df67dc8e3</originalsourceid><addsrcrecordid>eNotzs1KAzEUhuEgCJbaC3A34Do1_8kspfgHFTfdlzPJSZsynalJWsWrd0BX3-KDh5eQO86WymnNHiB_p8uSW6aWzAlpr8hMSMmpU0LckEUpB8aYMFZoLWekez_3NdFygpqgp8cxYIMxoq-lSUNTPs-IPxhon3b7SnHYw-AxTFfFHDGPR6w5-WaX4ZLqZIwD9M0XXLAJWCdlzOWWXEfoCy7-d042z0-b1Stdf7y8rR7XFLRQtLM2-ugcb1uHnYsmKAYWpDPeAyrujUUBVlvXSeMZb40TPCAL0djgHco5uf9jT3mcqkvdHsZznnLKVjCrW82FUfIXD65ZIg</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2075951264</pqid></control><display><type>article</type><title>Multi-spatial-mode effects in squeezed-light-enhanced interferometric gravitational wave detectors</title><source>Publicly Available Content Database (Proquest) (PQ_SDU_P3)</source><creator>Töyrä, Daniel ; Brown, Daniel D ; McKenna, Davis ; Song, Shicong ; Wormald, Alex ; Harms, Jan ; Miao, Haixing ; Freise, Andreas</creator><creatorcontrib>Töyrä, Daniel ; Brown, Daniel D ; McKenna, Davis ; Song, Shicong ; Wormald, Alex ; Harms, Jan ; Miao, Haixing ; Freise, Andreas</creatorcontrib><description>Proposed near-future upgrades of the current advanced interferometric gravitational wave detectors include the usage of frequency dependent squeezed light to reduce the current sensitivity-limiting quantum noise. We quantify and describe the degradation effects that spatial mode-mismatches between optical resonators have on the squeezed field. These mode-mismatches can to first order be described by scattering of light into second-order Gaussian modes. As a demonstration of principle, we also show that squeezing the second-order Hermite-Gaussian modes \(\mathrm{HG}_{02}\) and \(\mathrm{HG}_{20}\), in addition to the fundamental mode, has the potential to increase the robustness to spatial mode-mismatches. This scheme, however, requires independently optimized squeeze angles for each squeezed spatial mode, which would be challenging to realise in practise.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1704.08237</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Detectors ; Gravitational effects ; Gravitational waves ; Hermite-Gaussian modes ; Interferometry ; Noise sensitivity ; Optical resonators</subject><ispartof>arXiv.org, 2017-07</ispartof><rights>2017. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.proquest.com/docview/2075951264?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>780,784,25751,27923,37010,44588</link.rule.ids></links><search><creatorcontrib>Töyrä, Daniel</creatorcontrib><creatorcontrib>Brown, Daniel D</creatorcontrib><creatorcontrib>McKenna, Davis</creatorcontrib><creatorcontrib>Song, Shicong</creatorcontrib><creatorcontrib>Wormald, Alex</creatorcontrib><creatorcontrib>Harms, Jan</creatorcontrib><creatorcontrib>Miao, Haixing</creatorcontrib><creatorcontrib>Freise, Andreas</creatorcontrib><title>Multi-spatial-mode effects in squeezed-light-enhanced interferometric gravitational wave detectors</title><title>arXiv.org</title><description>Proposed near-future upgrades of the current advanced interferometric gravitational wave detectors include the usage of frequency dependent squeezed light to reduce the current sensitivity-limiting quantum noise. We quantify and describe the degradation effects that spatial mode-mismatches between optical resonators have on the squeezed field. These mode-mismatches can to first order be described by scattering of light into second-order Gaussian modes. As a demonstration of principle, we also show that squeezing the second-order Hermite-Gaussian modes \(\mathrm{HG}_{02}\) and \(\mathrm{HG}_{20}\), in addition to the fundamental mode, has the potential to increase the robustness to spatial mode-mismatches. This scheme, however, requires independently optimized squeeze angles for each squeezed spatial mode, which would be challenging to realise in practise.</description><subject>Detectors</subject><subject>Gravitational effects</subject><subject>Gravitational waves</subject><subject>Hermite-Gaussian modes</subject><subject>Interferometry</subject><subject>Noise sensitivity</subject><subject>Optical resonators</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNotzs1KAzEUhuEgCJbaC3A34Do1_8kspfgHFTfdlzPJSZsynalJWsWrd0BX3-KDh5eQO86WymnNHiB_p8uSW6aWzAlpr8hMSMmpU0LckEUpB8aYMFZoLWekez_3NdFygpqgp8cxYIMxoq-lSUNTPs-IPxhon3b7SnHYw-AxTFfFHDGPR6w5-WaX4ZLqZIwD9M0XXLAJWCdlzOWWXEfoCy7-d042z0-b1Stdf7y8rR7XFLRQtLM2-ugcb1uHnYsmKAYWpDPeAyrujUUBVlvXSeMZb40TPCAL0djgHco5uf9jT3mcqkvdHsZznnLKVjCrW82FUfIXD65ZIg</recordid><startdate>20170706</startdate><enddate>20170706</enddate><creator>Töyrä, Daniel</creator><creator>Brown, Daniel D</creator><creator>McKenna, Davis</creator><creator>Song, Shicong</creator><creator>Wormald, Alex</creator><creator>Harms, Jan</creator><creator>Miao, Haixing</creator><creator>Freise, Andreas</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20170706</creationdate><title>Multi-spatial-mode effects in squeezed-light-enhanced interferometric gravitational wave detectors</title><author>Töyrä, Daniel ; Brown, Daniel D ; McKenna, Davis ; Song, Shicong ; Wormald, Alex ; Harms, Jan ; Miao, Haixing ; Freise, Andreas</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a524-b77fcf881998eb8f6d40a7a386ccae41c67e2a7578b36c0196821de0df67dc8e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Detectors</topic><topic>Gravitational effects</topic><topic>Gravitational waves</topic><topic>Hermite-Gaussian modes</topic><topic>Interferometry</topic><topic>Noise sensitivity</topic><topic>Optical resonators</topic><toplevel>online_resources</toplevel><creatorcontrib>Töyrä, Daniel</creatorcontrib><creatorcontrib>Brown, Daniel D</creatorcontrib><creatorcontrib>McKenna, Davis</creatorcontrib><creatorcontrib>Song, Shicong</creatorcontrib><creatorcontrib>Wormald, Alex</creatorcontrib><creatorcontrib>Harms, Jan</creatorcontrib><creatorcontrib>Miao, Haixing</creatorcontrib><creatorcontrib>Freise, Andreas</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>SciTech Premium Collection (Proquest) (PQ_SDU_P3)</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database (Proquest) (PQ_SDU_P3)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Töyrä, Daniel</au><au>Brown, Daniel D</au><au>McKenna, Davis</au><au>Song, Shicong</au><au>Wormald, Alex</au><au>Harms, Jan</au><au>Miao, Haixing</au><au>Freise, Andreas</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Multi-spatial-mode effects in squeezed-light-enhanced interferometric gravitational wave detectors</atitle><jtitle>arXiv.org</jtitle><date>2017-07-06</date><risdate>2017</risdate><eissn>2331-8422</eissn><abstract>Proposed near-future upgrades of the current advanced interferometric gravitational wave detectors include the usage of frequency dependent squeezed light to reduce the current sensitivity-limiting quantum noise. We quantify and describe the degradation effects that spatial mode-mismatches between optical resonators have on the squeezed field. These mode-mismatches can to first order be described by scattering of light into second-order Gaussian modes. As a demonstration of principle, we also show that squeezing the second-order Hermite-Gaussian modes \(\mathrm{HG}_{02}\) and \(\mathrm{HG}_{20}\), in addition to the fundamental mode, has the potential to increase the robustness to spatial mode-mismatches. This scheme, however, requires independently optimized squeeze angles for each squeezed spatial mode, which would be challenging to realise in practise.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1704.08237</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier EISSN: 2331-8422
ispartof arXiv.org, 2017-07
issn 2331-8422
language eng
recordid cdi_proquest_journals_2075951264
source Publicly Available Content Database (Proquest) (PQ_SDU_P3)
subjects Detectors
Gravitational effects
Gravitational waves
Hermite-Gaussian modes
Interferometry
Noise sensitivity
Optical resonators
title Multi-spatial-mode effects in squeezed-light-enhanced interferometric gravitational wave detectors
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-13T10%3A53%3A25IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Multi-spatial-mode%20effects%20in%20squeezed-light-enhanced%20interferometric%20gravitational%20wave%20detectors&rft.jtitle=arXiv.org&rft.au=T%C3%B6yr%C3%A4,%20Daniel&rft.date=2017-07-06&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.1704.08237&rft_dat=%3Cproquest%3E2075951264%3C/proquest%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-a524-b77fcf881998eb8f6d40a7a386ccae41c67e2a7578b36c0196821de0df67dc8e3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2075951264&rft_id=info:pmid/&rfr_iscdi=true