𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Evolution of the chameleon scalar field in the early universe

✍ Scribed by Mota, David F.; Schelpe, Camilla A. O.

Book ID
120019293
Publisher
The American Physical Society
Year
2012
Tongue
English
Weight
487 KB
Volume
86
Category
Article
ISSN
1550-7998

No coin nor oath required. For personal study only.

πŸ“œ SIMILAR VOLUMES

Vacuum polarization and scalar field eff
Vacuum polarization and scalar field effects in the early Universe
✍ S. GottlΓΆber; V. MΓΌller πŸ“‚ Article πŸ“… 1986 πŸ› John Wiley and Sons 🌐 English βš– 240 KB πŸ‘ 1 views

Homogeneous isotropic cosmological models driven a t early timcs by a colicrent scalar [ield and the vacuuni polarization arc consitlrretl. Roth effects can lead t o the existence of a finite minimal value of the scale factor and an inflationary stage of expansion. The early as well as the late time