Observational future of cosmological scalar-tensor theories
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 microw...
主要な著者: | Alonso, D, Bellini, E, Ferreira, P, Zumalacárregui, M |
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フォーマット: | Journal article |
出版事項: |
American Physical Society
2017
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