Constraining gravitational-wave polarizations with Taiji
Space-based gravitational-wave detectors consist of a triangle of three spacecraft, which makes it possible to detect polarization modes of gravitational waves due to the motion of the detectors in space. In this paper we explore the ability of Taiji to detect the polarization modes in the parametri...
Gespeichert in:
Veröffentlicht in: | Physical review. D 2020-12, Vol.102 (12), Article 124050 |
---|---|
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 | 12 |
container_start_page | |
container_title | Physical review. D |
container_volume | 102 |
creator | Liu, Chang Ruan, Wen-Hong Guo, Zong-Kuan |
description | Space-based gravitational-wave detectors consist of a triangle of three spacecraft, which makes it possible to detect polarization modes of gravitational waves due to the motion of the detectors in space. In this paper we explore the ability of Taiji to detect the polarization modes in the parametrized post-Einsteinian framework. Assuming massive black hole binaries with the total mass of M = 4 × 105 M⊙ at redshift of z = 1 , we find that Taiji can measure the dipole and quadruple emission ( ΔαD/αD and ΔαQ/αQ) with the accuracy of up to ∼ 0.04 % , with the fiducial value of αD = 0.001 , the scalar transverse and longitudinal modes (ΔαB and ΔαL) up to ∼ 0.01 , and the vector modes ( ΔαV) up to ∼ 0.0005 . |
doi_str_mv | 10.1103/PhysRevD.102.124050 |
format | Article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_2481928834</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2481928834</sourcerecordid><originalsourceid>FETCH-LOGICAL-c277t-cf26eec69740a6e99b7b4b1c755d815df3983c5c7d9d16be65b3f2f831d87c003</originalsourceid><addsrcrecordid>eNo9kE1Lw0AYhBdRsNT-Ai8Bz4nvu5vsx1HiJxQUqedls9m0W2pSd9OU-uuNVj3NMAzD8BByiZAhArt-WR3iqxtuMwSaIc2hgBMyobmAFICq03-PcE5mMa5htByUQJwQWXZt7IPxrW-XyTKYwfem911rNuneDC7ZdhsT_OdPFpO971fJwvi1vyBnjdlEN_vVKXm7v1uUj-n8-eGpvJmnlgrRp7ah3DnLlcjBcKdUJaq8QiuKopZY1A1TktnCilrVyCvHi4o1tJEMayksAJuSq-PuNnQfOxd7ve52YbwXNc0lKioly8cWO7Zs6GIMrtHb4N9NOGgE_U1J_1EaA6qPlNgXK5BcZA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2481928834</pqid></control><display><type>article</type><title>Constraining gravitational-wave polarizations with Taiji</title><source>American Physical Society Journals</source><creator>Liu, Chang ; Ruan, Wen-Hong ; Guo, Zong-Kuan</creator><creatorcontrib>Liu, Chang ; Ruan, Wen-Hong ; Guo, Zong-Kuan</creatorcontrib><description>Space-based gravitational-wave detectors consist of a triangle of three spacecraft, which makes it possible to detect polarization modes of gravitational waves due to the motion of the detectors in space. In this paper we explore the ability of Taiji to detect the polarization modes in the parametrized post-Einsteinian framework. Assuming massive black hole binaries with the total mass of M = 4 × 105 M⊙ at redshift of z = 1 , we find that Taiji can measure the dipole and quadruple emission ( ΔαD/αD and ΔαQ/αQ) with the accuracy of up to ∼ 0.04 % , with the fiducial value of αD = 0.001 , the scalar transverse and longitudinal modes (ΔαB and ΔαL) up to ∼ 0.01 , and the vector modes ( ΔαV) up to ∼ 0.0005 .</description><identifier>ISSN: 2470-0010</identifier><identifier>EISSN: 2470-0029</identifier><identifier>DOI: 10.1103/PhysRevD.102.124050</identifier><language>eng</language><publisher>College Park: American Physical Society</publisher><subject>Black holes ; Detectors ; Dipoles ; Gravitation ; Gravitational waves ; Polarization ; Red shift</subject><ispartof>Physical review. D, 2020-12, Vol.102 (12), Article 124050</ispartof><rights>Copyright American Physical Society Dec 15, 2020</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c277t-cf26eec69740a6e99b7b4b1c755d815df3983c5c7d9d16be65b3f2f831d87c003</citedby><cites>FETCH-LOGICAL-c277t-cf26eec69740a6e99b7b4b1c755d815df3983c5c7d9d16be65b3f2f831d87c003</cites><orcidid>0000-0002-3111-5957 ; 0000-0002-0367-3652</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,778,782,2865,2866,27907,27908</link.rule.ids></links><search><creatorcontrib>Liu, Chang</creatorcontrib><creatorcontrib>Ruan, Wen-Hong</creatorcontrib><creatorcontrib>Guo, Zong-Kuan</creatorcontrib><title>Constraining gravitational-wave polarizations with Taiji</title><title>Physical review. D</title><description>Space-based gravitational-wave detectors consist of a triangle of three spacecraft, which makes it possible to detect polarization modes of gravitational waves due to the motion of the detectors in space. In this paper we explore the ability of Taiji to detect the polarization modes in the parametrized post-Einsteinian framework. Assuming massive black hole binaries with the total mass of M = 4 × 105 M⊙ at redshift of z = 1 , we find that Taiji can measure the dipole and quadruple emission ( ΔαD/αD and ΔαQ/αQ) with the accuracy of up to ∼ 0.04 % , with the fiducial value of αD = 0.001 , the scalar transverse and longitudinal modes (ΔαB and ΔαL) up to ∼ 0.01 , and the vector modes ( ΔαV) up to ∼ 0.0005 .</description><subject>Black holes</subject><subject>Detectors</subject><subject>Dipoles</subject><subject>Gravitation</subject><subject>Gravitational waves</subject><subject>Polarization</subject><subject>Red shift</subject><issn>2470-0010</issn><issn>2470-0029</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNo9kE1Lw0AYhBdRsNT-Ai8Bz4nvu5vsx1HiJxQUqedls9m0W2pSd9OU-uuNVj3NMAzD8BByiZAhArt-WR3iqxtuMwSaIc2hgBMyobmAFICq03-PcE5mMa5htByUQJwQWXZt7IPxrW-XyTKYwfem911rNuneDC7ZdhsT_OdPFpO971fJwvi1vyBnjdlEN_vVKXm7v1uUj-n8-eGpvJmnlgrRp7ah3DnLlcjBcKdUJaq8QiuKopZY1A1TktnCilrVyCvHi4o1tJEMayksAJuSq-PuNnQfOxd7ve52YbwXNc0lKioly8cWO7Zs6GIMrtHb4N9NOGgE_U1J_1EaA6qPlNgXK5BcZA</recordid><startdate>20201222</startdate><enddate>20201222</enddate><creator>Liu, Chang</creator><creator>Ruan, Wen-Hong</creator><creator>Guo, Zong-Kuan</creator><general>American Physical Society</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-3111-5957</orcidid><orcidid>https://orcid.org/0000-0002-0367-3652</orcidid></search><sort><creationdate>20201222</creationdate><title>Constraining gravitational-wave polarizations with Taiji</title><author>Liu, Chang ; Ruan, Wen-Hong ; Guo, Zong-Kuan</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c277t-cf26eec69740a6e99b7b4b1c755d815df3983c5c7d9d16be65b3f2f831d87c003</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Black holes</topic><topic>Detectors</topic><topic>Dipoles</topic><topic>Gravitation</topic><topic>Gravitational waves</topic><topic>Polarization</topic><topic>Red shift</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Liu, Chang</creatorcontrib><creatorcontrib>Ruan, Wen-Hong</creatorcontrib><creatorcontrib>Guo, Zong-Kuan</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>Liu, Chang</au><au>Ruan, Wen-Hong</au><au>Guo, Zong-Kuan</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Constraining gravitational-wave polarizations with Taiji</atitle><jtitle>Physical review. D</jtitle><date>2020-12-22</date><risdate>2020</risdate><volume>102</volume><issue>12</issue><artnum>124050</artnum><issn>2470-0010</issn><eissn>2470-0029</eissn><abstract>Space-based gravitational-wave detectors consist of a triangle of three spacecraft, which makes it possible to detect polarization modes of gravitational waves due to the motion of the detectors in space. In this paper we explore the ability of Taiji to detect the polarization modes in the parametrized post-Einsteinian framework. Assuming massive black hole binaries with the total mass of M = 4 × 105 M⊙ at redshift of z = 1 , we find that Taiji can measure the dipole and quadruple emission ( ΔαD/αD and ΔαQ/αQ) with the accuracy of up to ∼ 0.04 % , with the fiducial value of αD = 0.001 , the scalar transverse and longitudinal modes (ΔαB and ΔαL) up to ∼ 0.01 , and the vector modes ( ΔαV) up to ∼ 0.0005 .</abstract><cop>College Park</cop><pub>American Physical Society</pub><doi>10.1103/PhysRevD.102.124050</doi><orcidid>https://orcid.org/0000-0002-3111-5957</orcidid><orcidid>https://orcid.org/0000-0002-0367-3652</orcidid></addata></record> |
fulltext | fulltext |
identifier | ISSN: 2470-0010 |
ispartof | Physical review. D, 2020-12, Vol.102 (12), Article 124050 |
issn | 2470-0010 2470-0029 |
language | eng |
recordid | cdi_proquest_journals_2481928834 |
source | American Physical Society Journals |
subjects | Black holes Detectors Dipoles Gravitation Gravitational waves Polarization Red shift |
title | Constraining gravitational-wave polarizations with Taiji |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-17T00%3A54%3A47IST&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=Constraining%20gravitational-wave%20polarizations%20with%20Taiji&rft.jtitle=Physical%20review.%20D&rft.au=Liu,%20Chang&rft.date=2020-12-22&rft.volume=102&rft.issue=12&rft.artnum=124050&rft.issn=2470-0010&rft.eissn=2470-0029&rft_id=info:doi/10.1103/PhysRevD.102.124050&rft_dat=%3Cproquest_cross%3E2481928834%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=2481928834&rft_id=info:pmid/&rfr_iscdi=true |