We have proposed a new model of dark energy star consisting of five zones
namely, solid core of constant energy density, the thin shell between core and
interior, an inhomogeneous interior region with anisotropic pressures, thin
shell and the exterior vacuum region. We have discussed various physical
properties. The model satisfies all the physical requirements. The stability
condition under small linear perturbation has also been discussed.Comment: 11 pages,16 figures, Accepted in European Physical Journal
