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New exact anisotropic static spherically symmetric stellar models satisfying the Eiesland condition

机译:满足EIESLAND条件的新精确各向异性静态球体对称恒星模型

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In a very recent work (Murad, 2018) one of the present authors represents an algorithm for constructing all the static spherically symmetric exact anisotropic solutions of Einstein's field equations of embedding class 1 based on a single generating function. In this work we apply the same algorithm to construct stellar models by generalizing some previous and offering some new forms of the generating function. The resulting equation of state and energy density, radial and tangential pressures, pressure anisotropy for a compact star having mass and radius similar to PSR J1614-2230 have been analyzed and the numerical values are found quite in agreement with the authors' previous works. (C) 2019 Elsevier Inc. All rights reserved.
机译:在最近的工作(Murad,2018)中,本作者中的一个代表了一种基于单一的发电功能构建Einstein的嵌入类别1的Einstein现场方程的所有静态球面对称精确各向异性解的算法。 在这项工作中,我们应用相同的算法来构建恒星模型,通过概括一些先前的和提供一些新的生成功能。 已经分析了所得状态和能量密度,径向和切向压力的方程,具有与PSR J1614-2230类似的具有质量和半径的紧凑型恒星的压力各向异性,并与作者之前的作品一致地发现数值。 (c)2019 Elsevier Inc.保留所有权利。

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