论文标题
嵌入的BHS和多极球：静态SMBHS周围的聚集的未对准的厚胶盘
Embedded BHs and multipole globules: Clustered misaligned thick accretion disks around static SMBHs
论文作者
论文摘要
我们研究了绕中央静态施瓦茨柴尔兹黑洞的未对准（倾斜的）托里的群集。为此，我们考虑了一组几何厚，受压，完美的流体托里，分析了纯流体动力学模型。我们研究了Tori碰撞的出现，因此，与固定远处观察者相比，Tori组成的聚集体的稳定性特性。倾斜摩tori的骨料通过引入领先的函数来模仿单个轨道构型，该功能控制着黑洞吸引子周围的圆环分布。最终，根据圆锥形的厚度，可以看到圆锥形的团聚，这是轨道物质的（多极）圆形的，具有不同的环形旋转方向，覆盖了嵌入的中央黑洞。这些系统被证明包括具有与积聚到中央黑洞相关的新兴不稳定性阶段的托里。因此，我们提供了与摩托车能量学有关的数量，例如质量频率，焓 - 流量和通量厚度，具体取决于多层流体的模型参数。因此，该分析对倾斜的托里和未对准磁盘的凝聚的存在和特性施加了约束。一些注释包括在包括原型喷射的骨料上，该原型由与几何厚的托里相关的开放端溶液表示。
We investigate clusters of misaligned (inclined) tori orbiting a central static Schwarzschild black hole. To this purpose we considered a set of geometrically thick, pressure supported, perfect fluid tori analyzing purely hydrodynamic models. We study the tori collision emergence and, consequently, the stability properties of the aggregates composed by tori with different inclination angles relative to a fixed distant observer. The aggregate of tilted tori is modeled as a single orbiting configuration, by introducing a leading function governing the distribution of toroids around the black hole attractor. Eventually the tori agglomerate can be seen, depending on the tori thickness, as a (multipole) gobules of orbiting matter, with different toroidal spin orientations , covering the embedded central black hole. These systems are shown to include tori with emerging instability phase related to accretion onto the central black hole. Therefore we provide an evaluation of quantities related to tori energetics such as the mass-flux, the enthalpy-flux, and the flux thickness depending on the model parameters for polytropic fluids. Consequently this analysis places constraints on the existence and properties of tilted tori and aggregate of misaligned disks. Some notes are included on aggregates including proto-jets, represented by open cusped solutions associated to the geometrically thick tori.
