Authors: Farook Rahaman Raju Maulick Anil Kumar Yadav Saibal Ray Ranjan Sharma
Publish Date: 2011/08/30
Volume: 44, Issue: 1, Pages: 107-124
Abstract
We propose a model for an anisotropic dark energy star where we assume that the radial pressure exerted on the system due to the presence of dark energy is proportional to the isotropic perfect fluid matter density We discuss various physical features of our model and show that the model satisfies all the regularity conditions and is stable as well as singularityfree
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