论文标题
限制旋转静态SMBH的未对准环形的簇
Limiting effects in clusters of misaligned toroids orbiting static SMBHs
论文作者
论文摘要
我们考虑绕施瓦茨柴尔德黑洞的未对准的，压力支持的托里的聚集体。引入了领先的功能，调节了中央静态吸引子周围的环形函数分布，使未对准的Tori聚集物将其建模为单个轨道（宏 - ）配置。我们首先分析纯流体动力学完美液体环形的领先函数。后来，该函数将被修改以存在环形磁场。我们研究了对摩托车碰撞出现的限制以及与大量相对倾斜角的未对准Tori的团聚物的不稳定性。我们讨论了双峰高频准周期振荡（HF-QPO）的可能性可能与团聚的内部环形结构有关。该系统的离散几何形状与HF-QPO有关，考虑到与圆环内边缘相关的几个振荡测量模型。我们还研究了托里几何厚度对振荡现象的可能影响。
We consider agglomerates of misaligned, pressure supported tori orbiting a Schwarzschild black hole. A leading function is introduced, regulating the toroids distribution around the central static attractor-it enables to model the misaligned tori aggregate as a single orbiting (macro--)configuration. We first analyze the leading function for purely hydrodynamical perfect fluid toroids. Later, the function is modified for presence of a toroidal magnetic field. We study the constraints on the tori collision emergence and the instability of the agglomerates of misaligned tori with general relative inclination angles. We discuss the possibility that the twin peak high-frequency quasi-periodic oscillations (HF-QPOs) could be related to the agglomerate inner ringed structure. The discrete geometry of the system is related to HF-QPOs considering several oscillation geodesic models associated to the toroids inner edges. We also study possible effect of the tori geometrical thickness on the oscillatory phenomena.
