1.
Characteristic Surfaces of Dynamic Temporal-space Black Hole with Internal Global Monopole;
含整体单极动态时空黑洞的特征曲面
2.
Black Hole Entropy, Black Hole Information Paradox & Quantum Teleportation in Curved Space-time;
黑洞熵，黑洞信息佯谬及弯曲时空中的量子通讯
3.
Inside a black hole, space and time swap roles.
在黑洞内，空间和时间的角色互换。
4.
Discussion on a Schwarzschild Black Hole with Quintessence;
探讨Quintessence包围的Schwarzschild黑洞时空
5.
Late-time Tail of Dirac Particles Around the Rotating Black Hole;
旋转黑洞时空中Dirac粒子的晚期拖尾
6.
The properties of black holes are inextricably intertwined with those of spacetime.
黑洞的性质与时空的性质纠结缠合，难以釐清。
7.
The center of the black hole is not a point in space but an instant in time.
黑洞的中心不再是空间中的一点，而是时间上的一个瞬间。
8.
Decay of Scalar Fields in a Stationary Axisymmetric EMDA Black Hole Geometry;
稳态轴对称爱因斯坦—麦克斯韦伸缩子黑洞时空中标量场的衰减
9.
Evolution of Perturbations in the Black Hole Spacetime and Quantum Information in the Relativistic Framework;
黑洞时空中微扰的演化与相对论框架下的量子信息
10.
The Energy Distribution of Scalar Particles of a Rectilinearly Accelerating Non-stationary Black Hole with Electric Charges and Magnetic Charges;
带有电荷、磁荷的直线加速黑洞时空背景下标量粒子的能级
11.
The energy distribution of scalar particles in a space-time of general spherically symmetric and evaporating black hole;
一般球对称蒸发黑洞周围时空中标量粒子的能量分布
12.
The Study of Black Hole Based on Space-Time-Matter Theory and Brane World
基于空间—时间—物质理论和膜世界模型的黑洞研究
13.
Witten has shown that a black hole in anti– de Sitter spacetime corresponds to hot radiation in the alternative physics operating on the bounding spacetime.
维顿证明了反德西特时空中的黑洞，所对应的是边界时空中另一种物理的热辐射。
14.
What is happening to space-time around a rotating object that is much more massive than the Earth-a black hole,say-should be more obvious.
那些质量比地球大得多的旋转物体的周围时空中这种效应更为显著，比方说黑洞。
15.
Colliding black holes, collapsing stars, and spinning compact celestial objects such as pulsars create ripples in the fabric of space and time that subtly distort the world around us.
黑洞碰撞、星坍缩以及自旋脉冲星所激起的时空结构波动，微妙的扭曲了我们周围的世界。
16.
It is shown that the entropy of the black hole is proportional to the area of event horizon at any time.
结果表明 ,任一时刻黑洞熵都与黑洞事件视界面积成正比 .
17.
The waves that emanate from the collision of two black holes should be detectable.
两个黑洞相撞时产生的波动可以测到。
18.
black hole( region in outer space from which no matter or radiation can escape)
黑洞（任何物质或辐射均无从逃逸的外太空区域）.