Noise angular power spectrum of gravitational wave background experiments
We construct a model for the angular power spectrum of the instrumental noise in interferometer networks mapping gravitational wave backgrounds (GWBs) as a function of detector noise properties, network configuration, and scan strategy. We use the model to calculate the noise power spectrum for curr...
| Main Authors: | , , , , |
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| Format: | Journal article |
| Language: | English |
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American Physical Society
2020
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| _version_ | 1826274927210135552 |
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| author | Alonso, D Contaldi, CR Cusin, G Ferreira, PG Renzini, AI |
| author_facet | Alonso, D Contaldi, CR Cusin, G Ferreira, PG Renzini, AI |
| author_sort | Alonso, D |
| collection | OXFORD |
| description | We construct a model for the angular power spectrum of the instrumental noise in interferometer networks mapping gravitational wave backgrounds (GWBs) as a function of detector noise properties, network configuration, and scan strategy. We use the model to calculate the noise power spectrum for current and future ground-based experiments, as well as for planned space missions. We present our results in a language similar to that used in cosmic microwave background and intensity mapping experiments, and connect the formalism with the sensitivity curves that are common lore in GWB analyses. |
| first_indexed | 2024-03-06T22:50:56Z |
| format | Journal article |
| id | oxford-uuid:5ebeaa03-1f26-4b89-998d-78a78c5fcba0 |
| institution | University of Oxford |
| language | English |
| last_indexed | 2024-03-06T22:50:56Z |
| publishDate | 2020 |
| publisher | American Physical Society |
| record_format | dspace |
| spelling | oxford-uuid:5ebeaa03-1f26-4b89-998d-78a78c5fcba02022-03-26T17:42:39ZNoise angular power spectrum of gravitational wave background experimentsJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:5ebeaa03-1f26-4b89-998d-78a78c5fcba0EnglishSymplectic ElementsAmerican Physical Society2020Alonso, DContaldi, CRCusin, GFerreira, PGRenzini, AIWe construct a model for the angular power spectrum of the instrumental noise in interferometer networks mapping gravitational wave backgrounds (GWBs) as a function of detector noise properties, network configuration, and scan strategy. We use the model to calculate the noise power spectrum for current and future ground-based experiments, as well as for planned space missions. We present our results in a language similar to that used in cosmic microwave background and intensity mapping experiments, and connect the formalism with the sensitivity curves that are common lore in GWB analyses. |
| spellingShingle | Alonso, D Contaldi, CR Cusin, G Ferreira, PG Renzini, AI Noise angular power spectrum of gravitational wave background experiments |
| title | Noise angular power spectrum of gravitational wave background experiments |
| title_full | Noise angular power spectrum of gravitational wave background experiments |
| title_fullStr | Noise angular power spectrum of gravitational wave background experiments |
| title_full_unstemmed | Noise angular power spectrum of gravitational wave background experiments |
| title_short | Noise angular power spectrum of gravitational wave background experiments |
| title_sort | noise angular power spectrum of gravitational wave background experiments |
| work_keys_str_mv | AT alonsod noiseangularpowerspectrumofgravitationalwavebackgroundexperiments AT contaldicr noiseangularpowerspectrumofgravitationalwavebackgroundexperiments AT cusing noiseangularpowerspectrumofgravitationalwavebackgroundexperiments AT ferreirapg noiseangularpowerspectrumofgravitationalwavebackgroundexperiments AT renziniai noiseangularpowerspectrumofgravitationalwavebackgroundexperiments |