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Simulated forecasts for primordial B-mode searches in ground-based experiments

Abstract:

Detecting the imprint of inflationary gravitational waves on the B-mode polarization of the cosmic microwave background (CMB) is one of the main science cases for current and next-generation CMB experiments. In this work we explore some of the challenges that ground-based facilities will have to face in order to carry out this measurement in the presence of galactic foregrounds and correlated atmospheric noise. We present forecasts for stage-3 (S3) and planned stage-4 (S4) experiments based o...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1103/PhysRevD.95.043504

Authors


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
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
More from this funder
Funding agency for:
Alonso, D
Grant:
259505
More from this funder
Funding agency for:
Alonso, D
Grant:
259505
More from this funder
Funding agency for:
Dunkley, J
Grant:
259505
More from this funder
Funding agency for:
Thorne, B
Grant:
Studentship
Publisher:
American Physical Society Publisher's website
Journal:
Physical Review D Journal website
Volume:
95
Issue:
4
Pages:
043504
Publication date:
2017-02-01
DOI:
EISSN:
2470-0029
ISSN:
2470-0010
Source identifiers:
695538
Pubs id:
pubs:695538
UUID:
uuid:6aefcae3-9ce0-4521-b025-1164f2e2d6fd
Local pid:
pubs:695538
Deposit date:
2017-05-17

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