- Abstract:
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The next generation of surveys will greatly improve our knowledge of cosmological gravity. In this paper we focus on how Stage IV photometric redshift surveys, including weak lensing and multiple tracers of the matter distribution and radio experiments combined with measurements of the cosmic microwave background will lead to precision constraints on deviations from General Relativity. We use a broad subclass of Horndeski scalar-tensor theories to forecast the accuracy with which we will be ...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's version
- Files:
-
-
(pdf, 739.5kb)
-
- Publisher copy:
- 10.1103/PhysRevD.95.063502
-
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- Publisher:
- American Physical Society Publisher's website
- Journal:
- Physical Review D Journal website
- Volume:
- 95
- Issue:
- 6
- Pages:
- 063502
- Publication date:
- 2017-03-05
- DOI:
- EISSN:
-
2470-0029
- ISSN:
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2470-0010
- Pubs id:
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pubs:657199
- URN:
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uri:b3738d12-a32b-4a07-ad3b-a0e8604d8865
- UUID:
-
uuid:b3738d12-a32b-4a07-ad3b-a0e8604d8865
- Local pid:
- pubs:657199
- Keywords:
- Copyright holder:
- American Physical Society
- Copyright date:
- 2017
- Notes:
- © 2017 American Physical Society
Journal article
Observational future of cosmological scalar-tensor theories
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