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An Exact Family of Einstein-Maxwell Wyman-Adler Solution in General Relativity

机译:广义相对论中的一个精确的爱因斯坦-麦克斯韦怀曼-阿德勒解答族

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摘要

This paper presents a family of two-parametric interior solutions of Einstein- Maxwell field equations in general relativity for a static spherically symmetric distribution of a charged perfect fluid with particular choice of charge distribution and the metric component g_(00). This family gives us wide range of parameters, n and K, for which the solutions are regular and acceptable on physical grounds and hence suitable for modeling of charged compact star. The maximum allowable mass and corresponding radius, for this family of solutions with the particular form of charge distribution, is determined to be 2.48M_⊙ and 10.56 km respectively by assuming the stellar "surface" density equal to strange (quark)matter density at zero pressure. It is hoped that our investigation may be of some importance in connection with the study of internal structure of electrically charged strange (quark) star.
机译:本文介绍了广义相对论下带电完美流体的静态球对称分布的Einstein-Maxwell场方程的两参数内部解族,其中电荷选择和度量分量g_(00)有特定选择。这个族为我们提供了广泛的参数n和K,对于这些参数而言,解决方案是常规的并且在物理基础上可以接受,因此适合于对带电紧凑型恒星进行建模。通过假设恒星的“表面”密度等于零的奇异(夸克)物质密度,对于具有特殊电荷分布形式的该系列解决方案,最大允许质量和相应的半径分别确定为2.48M_⊙和10.56 km压力。希望我们的研究对于带电奇(夸克)星内部结构的研究可能具有一定的重要性。

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