Cosmological tests using the angular size of galaxy clusters
We use measurements of the galaxy-cluster angular size versus redshift to test and compare the standard model ($\Lambda$CDM) and the $R_{\rm h}=ct$ Universe. We show that the latter fits the data with a reduced $\chi^2_{\rm dof}=0.786$ for a Hubble constant $H_{0}= 72.6_{-3.4}^{+3.8}$ km $\rm s^...
| Main Authors: | , , |
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| Other Authors: | |
| Language: | en |
| Published: |
OXFORD UNIV PRESS
2014
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| Online Access: | http://hdl.handle.net/10150/614750 http://arizona.openrepository.com/arizona/handle/10150/614750 |