The linear growth of structure in the Rh = ct universe
We use recently published redshift space distortion measurements of the cosmological growth rate, f sigma(8)(z), to examine whether the linear evolution of perturbations in the R-h = ct cosmology is consistent with the observed development of large-scale structure. We find that these observations fa...
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| Language: | en |
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OXFORD UNIV PRESS
2017
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| Online Access: | http://hdl.handle.net/10150/622916 http://arizona.openrepository.com/arizona/handle/10150/622916 |