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Publikováno v:
G. Pordeus da Silva and A. G. Cavalcanti, Brazilian Journal of Physics48, 521 (2018)
In order to clarify the tension between estimates of the Hubble Constant ($H_0$) from local ($z \ll 1$) and global ($z \gg 1$) measurements, Lima and Cunha (LC) proposed a new method to measure $H_0$ in intermediate redshifts ($z \approx 1$), which w
Externí odkaz:
http://arxiv.org/abs/1805.06849
The most recent Hubble constant ($H_0)$ estimates from local methods (z << 1), $H_0=73.8\pm 2.4$ km s$^{-1}$ Mpc$^{-1}$, and the one from high redshifts $H_0=67.3\pm 1.2$ km s$^{-1}$ Mpc$^{-1}$, are discrepant at $2.4 \sigma$ confidence level. Within
Externí odkaz:
http://arxiv.org/abs/1404.4418
Publikováno v:
Brazilian Journal of Physics; Oct2018, Vol. 48 Issue 5, p521-530, 10p