| Автор | Norman Cruz |
| Автор | Cristián Martínez |
| Дата выпуска | 2000-08-07 |
| dc.description | We examine Friedmann-Robertson-Walker models in three spacetime dimensions. The matter content of the models is composed of a perfect fluid, with a γ-law equation of state, and a homogeneous scalar field minimally coupled to gravity with a self-interacting potential whose energy density redshifts as a<sup>-2ν</sup>, where a denotes the scale factor. Cosmological solutions are presented for different ranges of values of γ and ν. The potential required to agree with the above redshift for the scalar field energy density is also calculated. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | Cosmological scaling solutions of minimally coupled scalar fields in three dimensions |
| Тип | paper |
| DOI | 10.1088/0264-9381/17/15/302 |
| Electronic ISSN | 1361-6382 |
| Print ISSN | 0264-9381 |
| Журнал | Classical and Quantum Gravity |
| Том | 17 |
| Первая страница | 2867 |
| Последняя страница | 2874 |
| Выпуск | 15 |
