| タイトル | Homogeneous cosmological models and new inflation |
| 著者（英） | Widrow, Lawrence M.; Turner, Michael S. |
| 著者所属（英） | Chicago Univ.; NASA Headquarters; Fermi National Accelerator Lab. |
| 発行日 | 1986-10-27 |
| 言語 | eng |
| 内容記述 | The promise of the inflationary-universe scenario is to free the present state of the universe from extreme dependence upon initial data. Paradoxically, inflation is usually analyzed in the context of the homogeneous and isotropic Robertson-Walker cosmological models. It is shown that all but a small subset of the homogeneous models undergo inflation. Any initial anisotropy is so strongly damped that if sufficient inflation occurs to solve the flatness and horizon problems, the universe today would still be very isotropic. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 87A21873 |
| 権利 | Copyright |
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