An Exact Anisotropic Quark Star Model

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Relativistic model for anisotropic strange stars (2016, methodology): “To this end, we consider that the stellar object is spherically symmetric, static and anisotropic in nature and follows the density profile given by Mak and Harko (2002), which satisfies all the physical conditions.”
A class of relativistic stars with a linear equation of state (2007, background): “Linear equations of state are relevant in the modelling of static spherically symmetric anisotropic quark matter distributions as demonstrated by Mak & Harko (2002) and anisotropic quark stars admitting a conformal symmetry (Mak & Harko 2004).”