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We study the behavior of dark energy (DE) in the scope of anisotropic Bianchitype V (BV) space-time. First we derive Friedmann-Like Equations, then wecompare the dark energy equation of state (EoS) parameter for viscous andnon-viscous dark energy and make a correspondence between DE and quintessenceand phantom descriptions of non-viscous and viscous dark energy and reconstructthe potential of these two scalar fields. The late time behavior of EoSparameter through a thermodynamical study has also been investigated. Finally,we investigate the conditions under which BV space-time can be mapped into theFRW and how the bulk viscose coefficient may affect dark energy EoS parameterof our $\omega\mbox{BV}$ Model with constraints from 28 Hubble parameter,$H(z)$, measurements at intermediate redshifts $0.07\leq z\leq 2.3$.

Viscous Dark Energy In Bianchi Type V Space-Time