Sensitivity Studies for Third-Generation Gravitational Wave Observatories
Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope, a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitat...
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| Veröffentlicht in: | arXiv.org 2010-12 |
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| creator | Hild, S Abernathy, M Acernese, F Amaro-Seoane, P Andersson, N Arun, K Barone, F Barsuglia, M Beker, M Beveridge, N Birindelli, S Bose, S Bosi, L Braccini, S Bradaschia, C Bulik, T Calloni, E Cella, G Chelkowski, S Chincarini, A Colacino, C Cumming, A Danzmann, K De Salvo, R Dent, T De Rosa, R A Di Virgilio Doets, M Fafone, V Falferi, P Flaminio, R Franc, J Frasconi, F Friedrich, D Fulda, P Gair, J Gemme, G Genin, E Gennai, A Giazotto, A Granata, M Grote, H Guidi, G Gurkovsky, A Hammond, G Hannam, M Harms, J Heinert, D Heng, I Hennes, E Huttner, S Jones, G Khalili, F Kokeyama, K Kokkotas, K Krishnan, B Li, T G F Lorenzini, M Lück, H Mandel, I Mantovani, M Martin, I Michel, C Minenkov, Y Morgado, N Mosca, S Müller-Ebhardt, H Nawrodt, R Nelson, J Oshaughnessy, R Ott, C D Palomba, C Parguez, G Passaquieti, R Pinard, L R Poggiani1 Prato, M Puppo, P Rabeling, D Read, J Reid, S Richard, F Rocchi, A Rowan, S Santamaría, L Sassolas, B Schwarz, C Seidel, P Somiya, K Speirits, F Strigin, S Sutton, P Tarabrin, S van den Brand, J M van Veggel van den Broeck, C Vecchio, A Vicere, A Willke, B Yamamoto, K |
| description | Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope, a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this article we describe sensitivity models for the Einstein Telescope and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates. We develop the most accurate sensitivity model, referred to as ET-D, for a third-generation detector so far, including the most relevant fundamental noise contributions. |
| doi_str_mv | 10.48550/arxiv.1012.0908 |
| format | Article |
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The Einstein Telescope, a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this article we describe sensitivity models for the Einstein Telescope and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates. 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A</creatorcontrib><creatorcontrib>Vicere, A</creatorcontrib><creatorcontrib>Willke, B</creatorcontrib><creatorcontrib>Yamamoto, K</creatorcontrib><title>Sensitivity Studies for Third-Generation Gravitational Wave Observatories</title><title>arXiv.org</title><description>Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope, a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this article we describe sensitivity models for the Einstein Telescope and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates. We develop the most accurate sensitivity model, referred to as ET-D, for a third-generation detector so far, including the most relevant fundamental noise contributions.</description><subject>Astronomical models</subject><subject>Astronomy</subject><subject>Frequencies</subject><subject>Gravitation</subject><subject>Gravitational waves</subject><subject>Noise</subject><subject>Observatories</subject><subject>Physics - General Relativity and Quantum Cosmology</subject><subject>Radiation 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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><scope>GOX</scope></search><sort><creationdate>20101204</creationdate><title>Sensitivity Studies for Third-Generation Gravitational Wave Observatories</title><author>Hild, S ; Abernathy, M ; Acernese, F ; Amaro-Seoane, P ; Andersson, N ; Arun, K ; Barone, F ; Barsuglia, M ; Beker, M ; Beveridge, N ; Birindelli, S ; Bose, S ; Bosi, L ; Braccini, S ; Bradaschia, C ; Bulik, T ; Calloni, E ; Cella, G ; Chelkowski, S ; Chincarini, A ; Colacino, C ; Cumming, A ; Danzmann, K ; De Salvo, R ; Dent, T ; De Rosa, R ; A Di Virgilio ; Doets, M ; Fafone, V ; Falferi, P ; Flaminio, R ; Franc, J ; Frasconi, F ; Friedrich, D ; Fulda, P ; Gair, J ; Gemme, G ; Genin, E ; Gennai, A ; Giazotto, A ; Granata, M ; Grote, H ; Guidi, G ; Gurkovsky, A ; Hammond, G ; Hannam, M ; Harms, J ; Heinert, D ; Heng, I ; Hennes, E ; Huttner, S ; Jones, G ; Khalili, F ; Kokeyama, K ; Kokkotas, K ; Krishnan, B ; Li, T G F ; Lorenzini, M ; Lück, H ; Mandel, I ; Mantovani, M ; Martin, I ; Michel, C ; Minenkov, Y ; Morgado, N ; Mosca, S ; Müller-Ebhardt, H ; Nawrodt, R ; Nelson, J ; Oshaughnessy, R ; Ott, C D ; Palomba, C ; Parguez, G ; Passaquieti, R ; Pinard, L ; R Poggiani1 ; Prato, M ; Puppo, P ; Rabeling, D ; Read, J ; Reid, S ; Richard, F ; Rocchi, A ; Rowan, S ; Santamaría, L ; Sassolas, B ; Schwarz, C ; Seidel, P ; Somiya, K ; Speirits, F ; Strigin, S ; Sutton, P ; Tarabrin, S ; van den Brand, J ; M van Veggel ; van den Broeck, C ; Vecchio, A ; Vicere, A ; Willke, B ; Yamamoto, 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K</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</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><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Hild, S</au><au>Abernathy, M</au><au>Acernese, F</au><au>Amaro-Seoane, P</au><au>Andersson, N</au><au>Arun, K</au><au>Barone, F</au><au>Barsuglia, M</au><au>Beker, M</au><au>Beveridge, N</au><au>Birindelli, S</au><au>Bose, S</au><au>Bosi, L</au><au>Braccini, S</au><au>Bradaschia, C</au><au>Bulik, T</au><au>Calloni, E</au><au>Cella, G</au><au>Chelkowski, S</au><au>Chincarini, A</au><au>Colacino, C</au><au>Cumming, A</au><au>Danzmann, K</au><au>De Salvo, R</au><au>Dent, T</au><au>De Rosa, R</au><au>A Di Virgilio</au><au>Doets, M</au><au>Fafone, V</au><au>Falferi, P</au><au>Flaminio, R</au><au>Franc, J</au><au>Frasconi, F</au><au>Friedrich, D</au><au>Fulda, P</au><au>Gair, J</au><au>Gemme, G</au><au>Genin, E</au><au>Gennai, A</au><au>Giazotto, A</au><au>Granata, M</au><au>Grote, H</au><au>Guidi, G</au><au>Gurkovsky, A</au><au>Hammond, G</au><au>Hannam, M</au><au>Harms, J</au><au>Heinert, D</au><au>Heng, I</au><au>Hennes, E</au><au>Huttner, S</au><au>Jones, G</au><au>Khalili, F</au><au>Kokeyama, K</au><au>Kokkotas, K</au><au>Krishnan, B</au><au>Li, T G F</au><au>Lorenzini, M</au><au>Lück, H</au><au>Mandel, I</au><au>Mantovani, M</au><au>Martin, I</au><au>Michel, C</au><au>Minenkov, Y</au><au>Morgado, N</au><au>Mosca, S</au><au>Müller-Ebhardt, H</au><au>Nawrodt, R</au><au>Nelson, J</au><au>Oshaughnessy, R</au><au>Ott, C D</au><au>Palomba, C</au><au>Parguez, G</au><au>Passaquieti, R</au><au>Pinard, L</au><au>R Poggiani1</au><au>Prato, M</au><au>Puppo, P</au><au>Rabeling, D</au><au>Read, J</au><au>Reid, S</au><au>Richard, F</au><au>Rocchi, A</au><au>Rowan, S</au><au>Santamaría, L</au><au>Sassolas, B</au><au>Schwarz, C</au><au>Seidel, P</au><au>Somiya, K</au><au>Speirits, F</au><au>Strigin, S</au><au>Sutton, P</au><au>Tarabrin, S</au><au>van den Brand, J</au><au>M van Veggel</au><au>van den Broeck, C</au><au>Vecchio, A</au><au>Vicere, A</au><au>Willke, B</au><au>Yamamoto, K</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Sensitivity Studies for Third-Generation Gravitational Wave Observatories</atitle><jtitle>arXiv.org</jtitle><date>2010-12-04</date><risdate>2010</risdate><eissn>2331-8422</eissn><abstract>Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope, a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this article we describe sensitivity models for the Einstein Telescope and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates. We develop the most accurate sensitivity model, referred to as ET-D, for a third-generation detector so far, including the most relevant fundamental noise contributions.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1012.0908</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | EISSN: 2331-8422 |
| ispartof | arXiv.org, 2010-12 |
| issn | 2331-8422 |
| language | eng |
| recordid | cdi_arxiv_primary_1012_0908 |
| source | arXiv.org; Free E- Journals |
| subjects | Astronomical models Astronomy Frequencies Gravitation Gravitational waves Noise Observatories Physics - General Relativity and Quantum Cosmology Radiation pressure Sensitivity |
| title | Sensitivity Studies for Third-Generation Gravitational Wave Observatories |
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