| 1. | Another way to think of the problem is in terms of cosmic expansion
思考这个问题的另一个进路，就是宇宙膨胀。 |
| 2. | The inflationary universe theory
宇宙膨胀说 |
| 3. | Inflationary universe theory
宇宙膨胀说 |
| 4. | The primary observation that the universe is expanding emerged between 1910 and 1930
对于宇宙膨胀的首次观测，是在1910 ~ 30年间。 |
| 5. | The basic framework is the standard big bang theory for the expansion of the universe
基本的架构是解释宇宙膨胀的标准大霹雳理论。 |
| 6. | Dark energy is a mysterious repulsive force that opposes gravity , causing the universe to expand
暗能量是一种神秘的与万有引力相反的排斥力，它使宇宙膨胀。 |
| 7. | Through the expansion of the universe , the gas cooled and condensed into the myriad galaxies found today
经宇宙膨胀后，气体冷却并凝缩成无数今日可见的星系。 |
| 8. | Cosmic expansion has got its groove back : once thought to be winding down , it is actually speeding up
宇宙膨胀也因此重获律动：当你认为它应该变慢时，实际上却变快了。 |
| 9. | The negative pressure causes the acceleration of the universe , as observed from the type ia supernova observations
负压强令宇宙膨胀不断加速，就有如从观测ia型超新星所得出的结论一样。 |
| 10. | Cosmic expansion continued to cool the gas , so one might expect that the cosmic gas would still be cold and neutral today
宇宙膨胀持续冷却这些气体，因此我们预期这团宇宙气体在今日仍然应该保持著低温与电中性的状态。 |
