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| Content Provider | Springer Nature Link |
|---|---|
| Author | Turner, Michael S. |
| Copyright Year | 2003 |
| Abstract | Inflation has been the driving idea in cosmology for two decades and is a pillar of the New Cosmology. The inflationary paradigm has now passed its first round of significant tests, with two of its three basics predictions confirmed at about the 10% level (spatially flat Universe and density perturbations produced from quantum fluctuations with $$| n - 1| \sim {\mathcal{O}}(0.1)$$ ). The Inflationary Paradigm has some of the truth. Over the next decade the precision of these tests, most of which involve measurements of CMB anisotropy and polarization, will improve 30 fold or more(!), testing inflation more sharply and possibly elucidating the underlying cause. Especially important in this regard is detecting the inflation-produced gravitational waves, either directly or through their CMB polarization signature. While inflation has by no means been verified, its successes have raised the bar for competitor theories: Any alternative must feature the two hallmarks of inflation: superluminal expansion and entropy production. |
| Starting Page | 333 |
| Ending Page | 346 |
| Page Count | 14 |
| File Format | |
| ISSN | 14240637 |
| Journal | Annales Henri Poincaré |
| Volume Number | 4 |
| Issue Number | 1 |
| e-ISSN | 14240661 |
| Language | English |
| Publisher | Birkhäuser-Verlag |
| Publisher Date | 2003-01-01 |
| Publisher Place | Basel |
| Access Restriction | One Nation One Subscription (ONOS) |
| Subject Keyword | Mathematical and Computational Physics Dynamical Systems and Ergodic Theory Quantum Physics Mathematical Methods in Physics Relativity and Cosmology Elementary Particles, Quantum Field Theory |
| Content Type | Text |
| Resource Type | Article |
| Subject | Statistical and Nonlinear Physics Nuclear and High Energy Physics Mathematical Physics |
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