| 1. | " for their discovery of cosmic microwave background radiation
发现宇宙微波背景辐射 |
| 2. | Tegmark is an expert in analyzing the cosmic microwave background and galaxy clustering
铁马克是分析宇宙微波背景辐射与星系团的专家。 |
| 3. | They had found the cool afterglow of the big bang : the cosmic microwave background radiation
他们发现的是大霹雳冷却后的馀晖：宇宙微波背景辐射。 |
| 4. | They ' ll show up as patterns in the cosmic microwave background ( the fading glow from the big bang from the edge of the universe )
这些信号的表现形式是宇宙微波背景（来自宇宙边缘的大爆炸所产生的余热）中的模式。 |
| 5. | The cosmic microwave background radiation we see today is from the era just before the temperature was low enough to allow neutral hydrogen to form
简单来说，科学家所探测到的宇宙微波背景辐射，是来自刚转为透明前的宇宙。 |
| 6. | This star has a non - zero temperature and there is heat conduction between the star and the surrounding radiation . possible experimental tests are discussed briefly
该星体被放置在一个均匀、各向同性的宇宙微波背景辐射场中，星体与背景辐射场之间存在着热传导。 |
| 7. | We have a snapshot of the universe as it was 400 , 000 years after the big bang ? the cosmic microwave background radiation ? as well as pictures of individual galaxies a billion years later
我们已拥有宇宙在大霹雳40万年后光景的快照：宇宙微波背景辐射，与大霹雳10亿年后星系个体的影像。 |
| 8. | The nobel prize in physics goes to john mather and george smoot " for their discovery of the blackbody form and anisotropy of the cosmic microwave background radiation
2006年的诺贝尔物理学奖授予了美国科学家约翰?马瑟和乔治?斯穆特，以表彰他们发现了宇宙微波背景辐射的黑体形式和各向异性。 |
| 9. | Scientists used wilkinson microwave anisotropy probe wmap to capture the cosmic portrait that reveals the afterglow of the big bang , i . e . the cosmic microwave background radiation
科学家利用威尔金森微波各向异性探测器wilkinson microwave anisotropy probe , wmap ，测量来自不同方向的宇宙微波背景辐射，展示了大爆炸后的馀辉。 |
| 10. | According to cosmological theory , galaxies , galaxy clusters and larger structures evolved from small inhomogeneities in the matter density of the early universe , which are revealed by variations in the temperature of the cosmic microwave background ( cmb )
根据宇宙学的理论，星系、星系团和大尺度结构，都是从早期宇宙中，质量密度的微扰演化而来，这也正是宇宙微波背景（ cmb ）辐射的温度异向性告诉我们的。 |
