首页> 外文期刊>International journal of modern physics, D. Gravitation, astrophysics, cosmology >EXACT RELATIVISTIC MODELS OF THIN DISKS AROUND STATIC BLACK HOLES IN A MAGNETIC FIELD
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EXACT RELATIVISTIC MODELS OF THIN DISKS AROUND STATIC BLACK HOLES IN A MAGNETIC FIELD

机译:磁场中静态黑洞周围薄盘的精确相对论模型

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摘要

The exact superposition of a central static black hole with surrounding thin disk in presence of a magnetic field is investigated. We consider two models of disk, one of infinite extension based on a Kuzmin-Chazy-Curzon metric and other finite based on the first Morgan-Morgan disk. We also analyze a simple model of active galactic nuclei (AGN) consisting of black hole, a Kuzmin-Chazy-Curzon disk and two rods representing jets, in presence of magnetic field. To explain the stability of the disks, we consider the matter of the disk made of two pressureless streams of counter-rotating charged particles (counter-rotating model) moving along electrogeodesic. Using the Rayleigh criterion, we derivate for circular orbits the stability conditions of the particles of the streams. The influence of the magnetic field on the matter properties of the disk and on its stability are also analyzed.
机译:研究了在磁场存在下,中心静态黑洞与周围的薄盘的精确叠加。我们考虑两种磁盘模型,一种是基于Kuzmin-Chazy-Curzon度量的无限扩展,另一种是基于第一个Morgan-Morgan磁盘的有限扩展。我们还分析了一个活动的银河原子核(AGN)的简单模型,该模型由黑洞,一个Kuzmin-Chazy-Curzon磁盘和两个代表射流的杆组成,并且存在磁场。为了解释磁盘的稳定性,我们考虑磁盘的问题,该磁盘由两个沿着电大地运动的反向旋转的带电粒子(反向旋转模型)的无压力流组成。使用瑞利准则,我们推导了圆形轨道流的粒子的稳定性条件。还分析了磁场对磁盘物质特性及其稳定性的影响。

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