Journal article
Detecting the anisotropic astrophysical gravitational wave background in the presence of shot noise through cross-correlations
- Abstract:
- The spatial and temporal discreteness of gravitational wave sources leads to shot noise that may, in some regimes, swamp any attempts at measuring the anisotropy of the gravitational wave background. Cross-correlating a gravitational wave background map with a sufficiently dense galaxy survey can alleviate this issue, and potentially recover some of the underlying properties of the gravitational wave background. We quantify the shot noise level and we explicitly show that cross-correlating the gravitational wave background and a galaxy catalog improves the chances of a first detection of the background anisotropy with a gravitational wave observatory operating in the frequency range (10 Hz, 100 Hz), given sufficient sensitivity.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Preview, Version of record, 244.9KB, Terms of use)
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- Publisher copy:
- 10.1103/PhysRevD.102.023002
Authors
- Publisher:
- American Physical Society
- Journal:
- Physical Review D More from this journal
- Volume:
- 102
- Issue:
- 2
- Article number:
- 23002
- Publication date:
- 2020-07-01
- Acceptance date:
- 2020-06-09
- DOI:
- EISSN:
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1550-2368
- ISSN:
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1550-7998
- Language:
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English
- Keywords:
- Pubs id:
-
1122407
- Local pid:
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pubs:1122407
- 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 publisher's version of the article. The final version is available online from the American Physical Society at: https://doi.org/10.1103/PhysRevD.102.023002
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