Investigating the effect of precession on searches for neutron-star–black-hole binaries with Advanced LIGO
The first direct detection of neutron-star-blackhole binaries will likely be made with gravitational-wave observatories. Advanced LIGO and Advanced Virgo will be able to observe neutron-star-blackhole mergers at a maximum distance of 900 Mpc. To achieve this sensitivity, gravitational-wave searches...
Gespeichert in:
| Veröffentlicht in: | Physical review. D, Particles, fields, gravitation, and cosmology Particles, fields, gravitation, and cosmology, 2014-01, Vol.89 (2), Article 024010 |
|---|---|
| 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 | 2 |
| container_start_page | |
| container_title | Physical review. D, Particles, fields, gravitation, and cosmology |
| container_volume | 89 |
| creator | Harry, Ian W. Nitz, Alexander H. Brown, Duncan A. Lundgren, Andrew P. Ochsner, Evan Keppel, Drew |
| description | The first direct detection of neutron-star-blackhole binaries will likely be made with gravitational-wave observatories. Advanced LIGO and Advanced Virgo will be able to observe neutron-star-blackhole mergers at a maximum distance of 900 Mpc. To achieve this sensitivity, gravitational-wave searches will rely on using a bank of filter waveforms that accurately model the expected gravitational-wave signal. The emitted signal will depend on the masses of the black hole and the neutron star and also the angular momentum of both components. We identify the regions of parameter space where such systems occur and suggest methods for searching for highly precessing neutron-star-blackhole binaries. |
| doi_str_mv | 10.1103/PhysRevD.89.024010 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1700984220</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1700984220</sourcerecordid><originalsourceid>FETCH-LOGICAL-c280t-30e9cacb7db41961c670d05baf98e0f5217e2a01d16404b0de8abb766a255d13</originalsourceid><addsrcrecordid>eNo1kM1KAzEUhYMoWKsv4CpLN1NvMn-ZZalaC4WKdB-SzE1ndJrUZFrpznfwDX0SK61w4dzFx4HzEXLLYMQYpPcvzT6-4u5hJKoR8AwYnJEBy3NIeFqI89NfVpW4JFcxvgGkvCjLAelmboexb1eqb92K9g1StBZNT72lm4AGY2y9o4eLqIJpMFLrA3W47YN3SexV-Pn61p0y70njO6S6dSq0B-yz7Rs6rnfKGazpfDZdXJMLq7qIN6cckuXT43LynMwX09lkPE8MF9AnKWBllNFlrTNWFcwUJdSQa2UrgWBzzkrkCljNigwyDTUKpXVZFIrnec3SIbk71m6C_9ge1sl1Gw12nXLot1GyEqASGedwQPkRNcHHGNDKTWjXKuwlA_lnVv6blaKSR7PpL6xRcG4</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1700984220</pqid></control><display><type>article</type><title>Investigating the effect of precession on searches for neutron-star–black-hole binaries with Advanced LIGO</title><source>American Physical Society Journals</source><creator>Harry, Ian W. ; Nitz, Alexander H. ; Brown, Duncan A. ; Lundgren, Andrew P. ; Ochsner, Evan ; Keppel, Drew</creator><creatorcontrib>Harry, Ian W. ; Nitz, Alexander H. ; Brown, Duncan A. ; Lundgren, Andrew P. ; Ochsner, Evan ; Keppel, Drew</creatorcontrib><description>The first direct detection of neutron-star-blackhole binaries will likely be made with gravitational-wave observatories. Advanced LIGO and Advanced Virgo will be able to observe neutron-star-blackhole mergers at a maximum distance of 900 Mpc. To achieve this sensitivity, gravitational-wave searches will rely on using a bank of filter waveforms that accurately model the expected gravitational-wave signal. The emitted signal will depend on the masses of the black hole and the neutron star and also the angular momentum of both components. We identify the regions of parameter space where such systems occur and suggest methods for searching for highly precessing neutron-star-blackhole binaries.</description><identifier>ISSN: 1550-7998</identifier><identifier>EISSN: 1550-2368</identifier><identifier>DOI: 10.1103/PhysRevD.89.024010</identifier><language>eng</language><subject>Angular momentum ; Banks ; Black holes (astronomy) ; Cosmology ; Emittance ; Gravitation ; Mathematical models ; Precession ; Searching ; Waveforms</subject><ispartof>Physical review. D, Particles, fields, gravitation, and cosmology, 2014-01, Vol.89 (2), Article 024010</ispartof><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c280t-30e9cacb7db41961c670d05baf98e0f5217e2a01d16404b0de8abb766a255d13</citedby><cites>FETCH-LOGICAL-c280t-30e9cacb7db41961c670d05baf98e0f5217e2a01d16404b0de8abb766a255d13</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,2876,2877,27924,27925</link.rule.ids></links><search><creatorcontrib>Harry, Ian W.</creatorcontrib><creatorcontrib>Nitz, Alexander H.</creatorcontrib><creatorcontrib>Brown, Duncan A.</creatorcontrib><creatorcontrib>Lundgren, Andrew P.</creatorcontrib><creatorcontrib>Ochsner, Evan</creatorcontrib><creatorcontrib>Keppel, Drew</creatorcontrib><title>Investigating the effect of precession on searches for neutron-star–black-hole binaries with Advanced LIGO</title><title>Physical review. D, Particles, fields, gravitation, and cosmology</title><description>The first direct detection of neutron-star-blackhole binaries will likely be made with gravitational-wave observatories. Advanced LIGO and Advanced Virgo will be able to observe neutron-star-blackhole mergers at a maximum distance of 900 Mpc. To achieve this sensitivity, gravitational-wave searches will rely on using a bank of filter waveforms that accurately model the expected gravitational-wave signal. The emitted signal will depend on the masses of the black hole and the neutron star and also the angular momentum of both components. We identify the regions of parameter space where such systems occur and suggest methods for searching for highly precessing neutron-star-blackhole binaries.</description><subject>Angular momentum</subject><subject>Banks</subject><subject>Black holes (astronomy)</subject><subject>Cosmology</subject><subject>Emittance</subject><subject>Gravitation</subject><subject>Mathematical models</subject><subject>Precession</subject><subject>Searching</subject><subject>Waveforms</subject><issn>1550-7998</issn><issn>1550-2368</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2014</creationdate><recordtype>article</recordtype><recordid>eNo1kM1KAzEUhYMoWKsv4CpLN1NvMn-ZZalaC4WKdB-SzE1ndJrUZFrpznfwDX0SK61w4dzFx4HzEXLLYMQYpPcvzT6-4u5hJKoR8AwYnJEBy3NIeFqI89NfVpW4JFcxvgGkvCjLAelmboexb1eqb92K9g1StBZNT72lm4AGY2y9o4eLqIJpMFLrA3W47YN3SexV-Pn61p0y70njO6S6dSq0B-yz7Rs6rnfKGazpfDZdXJMLq7qIN6cckuXT43LynMwX09lkPE8MF9AnKWBllNFlrTNWFcwUJdSQa2UrgWBzzkrkCljNigwyDTUKpXVZFIrnec3SIbk71m6C_9ge1sl1Gw12nXLot1GyEqASGedwQPkRNcHHGNDKTWjXKuwlA_lnVv6blaKSR7PpL6xRcG4</recordid><startdate>20140113</startdate><enddate>20140113</enddate><creator>Harry, Ian W.</creator><creator>Nitz, Alexander H.</creator><creator>Brown, Duncan A.</creator><creator>Lundgren, Andrew P.</creator><creator>Ochsner, Evan</creator><creator>Keppel, Drew</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20140113</creationdate><title>Investigating the effect of precession on searches for neutron-star–black-hole binaries with Advanced LIGO</title><author>Harry, Ian W. ; Nitz, Alexander H. ; Brown, Duncan A. ; Lundgren, Andrew P. ; Ochsner, Evan ; Keppel, Drew</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c280t-30e9cacb7db41961c670d05baf98e0f5217e2a01d16404b0de8abb766a255d13</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2014</creationdate><topic>Angular momentum</topic><topic>Banks</topic><topic>Black holes (astronomy)</topic><topic>Cosmology</topic><topic>Emittance</topic><topic>Gravitation</topic><topic>Mathematical models</topic><topic>Precession</topic><topic>Searching</topic><topic>Waveforms</topic><toplevel>online_resources</toplevel><creatorcontrib>Harry, Ian W.</creatorcontrib><creatorcontrib>Nitz, Alexander H.</creatorcontrib><creatorcontrib>Brown, Duncan A.</creatorcontrib><creatorcontrib>Lundgren, Andrew P.</creatorcontrib><creatorcontrib>Ochsner, Evan</creatorcontrib><creatorcontrib>Keppel, Drew</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, Particles, fields, gravitation, and cosmology</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Harry, Ian W.</au><au>Nitz, Alexander H.</au><au>Brown, Duncan A.</au><au>Lundgren, Andrew P.</au><au>Ochsner, Evan</au><au>Keppel, Drew</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Investigating the effect of precession on searches for neutron-star–black-hole binaries with Advanced LIGO</atitle><jtitle>Physical review. D, Particles, fields, gravitation, and cosmology</jtitle><date>2014-01-13</date><risdate>2014</risdate><volume>89</volume><issue>2</issue><artnum>024010</artnum><issn>1550-7998</issn><eissn>1550-2368</eissn><abstract>The first direct detection of neutron-star-blackhole binaries will likely be made with gravitational-wave observatories. Advanced LIGO and Advanced Virgo will be able to observe neutron-star-blackhole mergers at a maximum distance of 900 Mpc. To achieve this sensitivity, gravitational-wave searches will rely on using a bank of filter waveforms that accurately model the expected gravitational-wave signal. The emitted signal will depend on the masses of the black hole and the neutron star and also the angular momentum of both components. We identify the regions of parameter space where such systems occur and suggest methods for searching for highly precessing neutron-star-blackhole binaries.</abstract><doi>10.1103/PhysRevD.89.024010</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 1550-7998 |
| ispartof | Physical review. D, Particles, fields, gravitation, and cosmology, 2014-01, Vol.89 (2), Article 024010 |
| issn | 1550-7998 1550-2368 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_1700984220 |
| source | American Physical Society Journals |
| subjects | Angular momentum Banks Black holes (astronomy) Cosmology Emittance Gravitation Mathematical models Precession Searching Waveforms |
| title | Investigating the effect of precession on searches for neutron-star–black-hole binaries with Advanced LIGO |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-06T09%3A16%3A02IST&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=Investigating%20the%20effect%20of%20precession%20on%20searches%20for%20neutron-star%E2%80%93black-hole%20binaries%20with%20Advanced%20LIGO&rft.jtitle=Physical%20review.%20D,%20Particles,%20fields,%20gravitation,%20and%20cosmology&rft.au=Harry,%20Ian%20W.&rft.date=2014-01-13&rft.volume=89&rft.issue=2&rft.artnum=024010&rft.issn=1550-7998&rft.eissn=1550-2368&rft_id=info:doi/10.1103/PhysRevD.89.024010&rft_dat=%3Cproquest_cross%3E1700984220%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=1700984220&rft_id=info:pmid/&rfr_iscdi=true |