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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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Publisher copy:
10.1103/PhysRevD.102.023002

Authors


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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
ORCID:
0000-0002-4598-9719
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
ORCID:
0000-0002-3021-2851


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:
1550-2368
ISSN:
1550-7998


Language:
English
Keywords:
Pubs id:
1122407
Local pid:
pubs:1122407
Deposit date:
2020-08-10

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