stationary hole

The stationary vertical structure of a thin disk around a black hole is considered with the anomalous magnetic viscosity~ ( [ 1]).

利用反常粘滞[1]研究了黑洞周围薄吸积盘的静态垂向结构。

The Hawking effect, event horizon and corresponding temperature of a uniformly accelerating, non stationary , charged black hole are given.

给出了匀加速荷电黑洞的 Hawking 效应和事件视界及相应温度.

Taking into account the generalized uncertainty principle ( GUP), we calculate the density of quantum states near the event horizon of a common stationary black hole in pseudo-Riemannian space-time.

在考虑了广义不确定关系原理的基础上，计算了黎曼时空背景中的一般静态黑洞视界附近的量子态密度。

The event horizon of the non-stationary Kerr black hole is rotationallysymrnet-ric, but not spherecally symmetric.

动态Kerr黑洞的事件视界是旋转对称的, 不是球对称的.

Using entropy density of the rectilinearly accelerating non-stationary black hole with electric charges and magnetic charges, we obtain conclusion that the entropy density near the event horizon of non-stationary blank hole in a direction is proportionate to cubic power temperature of event horizon on this direction.

利用带有电荷与磁荷的直线加速动态黑洞的熵密度，得到了任一时刻黑洞视界面附近沿某一方位角的熵密度总是正比于该处视界温度的三次方的结论。

Non thermal radiation of stationary and non stationary spherical symmetry Black Hole with electric charge and magnetic charge are affected by interstellar materials. The average range of particles of non-thermal radiation depends on the maximum energy of the radiation and the energy extent of the radiation.

稳态的动态球对称荷电荷磁黑洞的非热辐射受到星际物质的影响，其非热辐射粒子的平均射程与非热辐射的最大能量和能量范围有关。