Slowly rotating dark energy stars

We study isotropic and slowly-rotating stars made of dark energy adopting the extended Chaplygin equation-of-state. compute moment inertia as a function mass stars, both for rotating non-rotating objects. The solution non-diagonal metric component radial coordinate three different star masses is shown well. find that (i) increases with star, (ii) in case objects grows faster, (iii) curve corresponding to rotation lies below one stars.