Journal article
Noise angular power spectrum of gravitational wave background experiments
- Abstract:
- 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.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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- Files:
-
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(Preview, Accepted manuscript, 2.0MB, Terms of use)
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- Publisher copy:
- 10.1103/PhysRevD.101.124048
Authors
- Publisher:
- American Physical Society
- Journal:
- Physical Review D More from this journal
- Volume:
- 101
- Issue:
- 12
- Article number:
- 124048
- Publication date:
- 2020-06-22
- Acceptance date:
- 2020-06-04
- DOI:
- EISSN:
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1550-2368
- ISSN:
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1550-7998
- Language:
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English
- Keywords:
- Pubs id:
-
1118771
- Local pid:
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pubs:1118771
- Deposit date:
-
2020-08-10
Terms of use
- Copyright holder:
- American Physical Society
- Copyright date:
- 2020
- Rights statement:
- © 2020 American Physical Society
- Notes:
- This is the accepted manuscript version of the article. The final version is available from American Physical Society at: https://doi.org/10.1103/PhysRevD.101.124048
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