We study the axisymmetric, time-dependent hydrodynamics of rotating flows that are under the influence of super-massive black hole gravity and radiation from an accretion disk surrounding the black hole (BH). This work is an extension of the earlier work presented by Proga, in which nonrotating flows were studied. Here, we consider effects of rotation, a position-dependent radiation temperature, density at large radii, and uniform X-ray background radiation. As in the nonrotating case, the rotating flow settles into a configuration with two components, (1) an equatorial inflow and (2) a bipolar inflow/outflow with the outflow leaving the system along the pole. However, with rotation the flow does not always reach a steady state. In addition, rotation reduces the outflow collimation and the outward flux of mass and kinetic energy. Moreover, rotation increases the outward flux of the thermal energy and can lead to fragmentation and time variability of the outflow. We also show that a position-dependent radiation temperature can significantly change the flow solution, In particular, the inflow in the equatorial region can be replaced by a thermally driven outflow. Generally, as has been discussed and shown in the past, we find that self-consistently determined preheating/ cooling from the quasar radiation can significantly reduce the rate at which the central BH is fed with matter. However, our results also emphasize a little-appreciated feature. Namely, quasar radiation drives a nonspherical, multitem-perature, and very dynamic flow. These effects become dominant for luminosities in excess of 0.01 of the Eddington luminosity.
展开▼
机译:用等离子体约束实现重力场的动态控制热核聚变(TLTS)方法,通过热辐射等离子体绝缘的壁反应堆防止中子辐射并节省磁场和等离子体的混合,使用旋转磁场的异步磁惯性约束反应堆(AMITYAR和HFM)为实施该方法,在该反应器中点燃热核反应的方法,爆炸式等离子发生器(VIP)的实施方法,以及具有HFM的特立普安瓿,以实现D + T反应和具有超高温热度的HFM D +3НЕ和1Н+11В的高温反应