We find new stellar models to the field equations for charged anisotropic spheres. We use linear quark equation of state for strange quark matter. We choose a new form of pressure anisotropy as a rational function. In our model, we regain previous isotropic and anisotropic stellar models as specific cases. Isotropic models regained are those found by Komathiraj and Maharaj, Mak and Harko, and Misner and Zapolsky. Anisotropic models regained include the performance by Maharaj, Sunzu and Ray; and Sunzu and Danford. We indicate that our model meets the stability and energy conditions. We also generate stellar masses consistent with observations.

我们为带电各向异性球的场方程找到了新的恒星模型。我们使用线性夸克状态方程来处理奇怪的夸克物质。我们选择一种新形式的压力各向异性作为有理函数。在我们的模型中，我们重新获得了以前的各向同性和各向异性恒星模型作为特定案例。各向同性模型是由Komathiraj和Maharaj，Mak和Harko以及Misner和Zapolsky发现的模型。重新获得的各向异性模型包括Maharaj，Sunzu和Ray的表演；以及Sunzu和Danford。我们表明我们的模型满足稳定性和能量条件。我们还产生与观测结果一致的恒星质量。