anisotropic quintessence stars

 

we propose a relativistic model for: quintessence stars with the combination of an anisotropic pressure corresponding to normal matter and a quintessence dark energy having a characteristic parameter ω q such that −1<ωq<−13 . we discuss various physical features of the model and show that the model satisfies all the regularity conditions and can provide stable equilibrium configurations. compact objects are of great interest for a long time. theoretical analysis of superdense stars have been done by several authors (rahaman et al. 2012a,b; kalam et al. 2012a,b, 2013; hossein et al. 2012; lobo 2006; bronnikov and fabris 2006; egeland 2007; dymnikova 2002). ruderman (1972).