磁星的相对论模型：非微扰分析方法
Relativistic models of magnetars: Nonperturbative analytical approach
摘要：
在本文中，我们专注于建立简单的非微扰分析相对论模型的磁星。考虑到这一目的，我们首先开发了一种方法，用于产生精确的内部解决方案的静态和轴对称的爱因斯坦-麦克斯韦流体动力学方程组与各向异性的理想流体和纯极向磁场。然后，利用显式精确解，我们提出了一个简单的磁星模型，并计算了一些物理上有趣的量，如表面椭圆度和磁化星的总能量。
英文摘要：
In the present paper we focus on building simple nonperturbative analytical relativistic models of magnetars. With this purpose in mind we first develop a method for generating exact interior solutions to the static and axisymmetric Einstein-Maxwell-hydrodynamic equations with anisotropic perfect fluid and with pure poloidal magnetic field. Then using an explicit exact solution we present a simple magnetar model and calculate some physically interesting quantities as the surface elipticity and the total energy of the magnetized star.
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