| 1. | A historical review of einstein ' s introduction of cosmological constant
爱因斯坦引入宇宙常数的历史评述 |
| 2. | Traditional energy - momentum pseudotensors revisited with a cosmological constant
宇宙常数模型中传统能动量赝张量的修正 |
| 3. | Both the cosmological constant and quintessence fall into the general category of dark energy
不管是宇宙常数还是第五元素，都属于暗能量的?畴。 |
| 4. | In these contexts , the fields work because they are the simplest generalization of einstein ' s cosmological constant
在这样的情况下，由于纯量场是爱因斯坦宇宙常数最简化的归纳，因此它会产生作用。 |
| 5. | String theory , which unites gravity with quantum mechanics , offered the hope of explaining the attenuated cosmological constant
统合重力及量子力学的弦论，似乎能为微小的宇宙常数提供一个合理解释。 |
| 6. | This finding revealed that cosmological constant factor cannot be neglected . it represents a repelling force , which fuels the universe s expansion
这个发现显示宇宙常数不但不可忽略，它还造成一个排斥力，促使宇宙加速膨胀。 |
| 7. | In principle , physicists might like to examine one or a few vacua having the right cosmological constant to see if they offer testable predictions
原则上，物理学家会想挑几个有正确宇宙常数的真空来检验，看看它们是否做得出可试验的预测。 |
| 8. | A first , and perhaps the most convincing candidate for the dark energy , is the cosmological constant , introduced by einstein in 1917 and later rejected by him
黑暗能量其实很可能就是爱恩斯坦在1917年在引力方程中加入，但终被抛弃的宇宙常数。 |
| 9. | At last , we discuss the structure of d - stars in the spacetime with a nonzero cosmological constant . the metric and effective mass formula of d - stars have been educed
本文的第三部分，主要讨论了带有非零宇宙常数时空中d星的结构，导出了它的度规和有效质量公式。 |
| 10. | The leading candidate to explain dark energy ' s effects is vacuum energy , which is mathematically equivalent to the cosmological constant that einstein invented in 1917
要解释暗能量效应的首选，便是真空能量，它与爱因斯坦在1917年所创的宇宙常数，在数学上是等价的。 |
