Probing Dark Energy in The scope of Bianchi type I Spacetime
  It is well known that flat FRW metric is a special case of Bianchi type I
spacetime. In this paper, we use 38 Hubble parameter, $H(z)$, measurements at
intermediate redshifts $0.07\leq z\leq 2.36$ and its joint combination with the
latest \textgravedbl joint light curves\textacutedbl (JLA) sample, comprised of
740 type Ia supernovae in the redshift range $z \epsilon [0.01, 1.30]$ to
constrain the parameters of Bianchi type I dark energy model. We also use the
same datasets to constrain flat $\Lambda$CDM Model. In both cases, we
specifically address the expansion rate $H_{0}$ as well as the transition
redshift $z_{t}$ determinations out of these measurements. In both Models we
found that using joint combination of datasets gives rise to lower values for
model parameters. Also to compare the considered cosmologies, we have made
Akaike information criterion (AIC) and Bayes factor ($\Psi$) tests.
