广义相对论无力电动力学的新公式及其应用

Cong Yu
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引用次数: 1

摘要

我们用一种新的3 + 1语言表述了广义相对论的无力电动力学。在此公式中,当我们适当地定义了电场和磁场时,协变麦克斯韦方程组可以用新的真空本构约束方程转化为传统形式。控制稳定的轴对称无力黑洞磁层的基本方程是用这个公式推导出来的,它以一种更简单的方式重塑了Grad-Shafranov方程。与索恩和麦克唐纳经典的3+1方程组相比,新的3+1方程组既保留了电动力学的双曲结构,又避免了视界处的奇点,更适合于数值应用。这个公式可以很容易地推广到非相对论性极限,并在平坦时空中找到应用。我们研究了它在平时空和弯曲时空的盘风、黑洞磁层和太阳物理中的应用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A New Formulation for General Relativistic Force-Free Electrodynamics and Its Applications
We formulate the general relativistic force-free electrodynamics in a new 3 + 1 language. In this formulation, when we have properly defined electric and magnetic fields, the covariant Maxwell equations could be cast in the traditional form with new vacuum constitutive constraint equations. The fundamental equation governing a stationary, axisymmetric force-free black hole magnetosphere is derived using this formulation which recasts the Grad-Shafranov equation in a simpler way. Compared to the classic 3+1 system of Thorne and MacDonald, the new system of 3+1 equations is more suitable for numerical use for it keeps the hyperbolic structure of the electrodynamics and avoids the singularity at the event horizon. This formulation could be readily extended to non-relativistic limit and find applications in flat spacetime. We investigate its application to disk wind, black hole magnetosphere and solar physics in both flat and curved spacetime.
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