Impact of a Locally Measured H-0 on the Interpretation of Cosmic-chronometer Data
Many measurements in cosmology depend on the use of integrated distances or time, but. galaxies evolving passively on a timescale much longer than their age difference allow us to determine the expansion rate H(z) solely as a function of the redshift-time derivative dz/dt. These model-independent &q...
Main Authors: | , , |
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Language: | en |
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IOP PUBLISHING LTD
2017
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Online Access: | http://hdl.handle.net/10150/624388 http://arizona.openrepository.com/arizona/handle/10150/624388 |