Universe evolution with scalar fields

被引：0
|
作者：
Piccinelli, G [1 ]
机构：
[1] Univ Nacl Autonoma Mexico, ENEP Aragon, Ctr Technol, Mexico City, DF, Mexico
来源：
GALAXY EVOLUTION: THEORY AND OBSERVATIONS | 2003年 / 17卷
关键词：
cosmology; theory;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Cosmological scalar fields with negative pressure and a time-varying, spatially fluctuating energy density -quintessence- have recently obtained wide support from different observations and theoretical considerations. We present here an overview of the cosmological evolution of scalar fields with arbitrary potentials, in the presence of a barotropic fluid, and their influence on the universe expansion.
引用
收藏
页码：30 / 31
页数：2
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